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1

Determination of correction factors for alpha activity measurements in the environment (conditions of high dust loading)  

Within the framework of a French national monitoring program to survey the man-made radioactivity in the environment, several power plants and research facilities on the territory use environmental air monitors for unwanted releases of radioactive aerosols. High sensitivity and lack of false alarms are all important for environmental air monitors. The project aims to conduct investigations to improve operation of environmental air monitors, particularly under conditions where a lot of non-radioactive dust may be deposited on the filters (conditions of high dust loading). The dust may increase the frequency with which filters must be changed and can lead to an underestimation of the real activity. This underestimation is due to deteriorated alpha energy resolution and response specificity t...

2

Development of a computer model for calculation of radioactive materials into the atmosphere after an accident  

Secondary atmospheric contamination with radioactive dust and chemical species deposited on the ground and resuspended by wind occur very widely. This process is particularly pronounced in case of extensive contamination of soil and under extreme weather conditions, for example, during dust storms. The mechanism of wind dust generation consists in the following. At low wind speed U=2-3 m/s, which is most common in midlatitude, small radioactive dust particles (diameter of hundredth of a micron to 10-20 microns) are lifted from soil surface due to turbulent vortexes. Under the gravitational force the particles of 1-2 micron diameter practically do not settle. Larger dust particles cannot remain in the air for a long time: they are lifted by turbulent vortexes and settle, their motion in the wind flow is jump-wise and the interaction of particles with the flow is called saltation /I/. Saltation is the main mechanism of dust generation up to the wind velocity at which wind erosion starts. The size of dust particles can be as large as 100 pm. When dropping they can be ricocheting from ground or pass the impulse to other particles which begin rolling over and jumping up. The process of dust transport by wind can be compared to a chain reaction. At the velocity of 10 m/s large particles of about 500 pm stop skipping and roll over only, while particles of more than 1 mm remain stationary. Thus, the fine fraction is blown out from the polydispersed soil particles. The intensity of wind resuspension of radioactive dust from the ground is characterized either by a resuspension factor or a resuspension rate.

3

Applications of high-speed dust injection to magnetic fusion  

It is now an established fact that a significant amount of dust is produced in magnetic fusion devices due to plasma-wall interactions. Dust inventory must be controlled, in particular for the next-generation steady-state fusion machines like ITER, as it can pose significant safety hazards and degrade performance. Safety concerns are due to tritium retention, dust radioactivity, toxicity, and flammability. Performance concerns include high-Z impurities carried by dust to the fusion core that can reduce plasma temperature and may even induce sudden termination of the plasma. We have recognized that dust transport, dust-plasma interactions in magnetic fusion devices can be effectively studied experimentally by injection of dust with known properties into fusion plasmas. Other applications of injected dust include diagnosis of fusion plasmas and edge localized mode (ELM)'s pacing. In diagnostic applications, dust can be regarded as a source of transient neutrals before complete ionization. ELM's pacing is a promising scheme to prevent disruptions and type I ELM's that can cause catastrophic damage to fusion machines. Different implementation schemes are available depending on applications of dust injection. One of the simplest dust injection schemes is through gravitational acceleration of dust in vacuum. Experiments at Los Alamos and Princeton will be described, both of which use piezoelectric shakers to deliver dust to plasma. In Princeton experiments, spherical particles (40 micron) have been dropped in a systematic and reproducible manner using a computer-controlled piezoelectric bending actuator operating at an acoustic (0,2) resonance. The circular actuator was constructed with a 2.5 mm diameter central hole. At resonance ({approx} 2 kHz) an applied sinusoidal voltage has been used to control the flux of particles exiting the hole. A simple screw throttle located {approx}1mm above the hole has been used to set the magnitude of the flux achieved for a given voltage. Particle fluxes ranging from a few tens of particle per second up to thousands of particles per second have been achieved using this simple device. To achieve higher dust injection speed, another key consideration is how to accelerate dust at controlled amount. In addition to gravity, other possible acceleration mechanisms include electrostatic, electromagnetic, gas-dragged, plasma-dragged, and laser-ablation-based acceleration. Features and limitations of the different acceleration methods will be discussed. We will also describe laboratory experiments on dust acceleration.

4

Allergies, asthma, and dust  

Allergic rhinitis - dust ... make allergies or asthma worse are called triggers. Dust is a common trigger. When your asthma, or allergies, becomes worse due to dust you are said to have a dust allergy. ...

5

Model of particle resuspension in turbulent flows  

The graphite dust generated in an HTR/PBMR during normal reactor operation is deposited inside the primary system and becomes radioactive due to sorption of fission products. A significant amount of radioactive dust may be resuspended and released to the environment in case of LOCA. Therefore accurate particle resuspension models are required for HTR/PBMR safety analyses. Thermal-hydraulic safety analyses of HTR/PBMR type reactors are typically performed using computer codes such as FLOWNEX, MELCOR, or SPECTRA. None of these codes currently includes a well-tested mechanistic resuspension model. The resuspension model based on the Vainshtein model has been developed and implemented into the SPECTRA thermal-hydraulic system code. The resuspension model formulation has been extended in such w...

6

Estimates of the occupational exposure to tenorm in the phosphoric acid production plant in Iran.  

Phosphate rock is used world wide for manufacturing phosphoric acid and several chemical fertilisers. It is known that the phosphate rock contains various concentrations of uranium, thorium, radium and their daughters. The subject of this study is the evaluation of the radiation exposure to workers in the phosphoric acid production plant due to technologically enhanced naturally occurring radioactive materials that can result from the presence of naturally occurring radioactive materials in phosphate ores used in the manufacturing of phosphoric acid. Radiation exposure due to direct gamma radiation, dust inhalation and radon gas has been investigated and external and internal doses of exposed workers have been calculated. Natural radioactivity due to (40)K, (226)Ra and (232)Th have been measured in phosphate rock, phosphogypsum, chemical fertilisers and other samples by gamma spectrometry system with a high-purity germanium. The average concentrations of (226)Ra and (40)K observed in the phosphate rock are 760 and 80 Bq kg(-1), respectively. Annual effective dose from external radiation had a mean value of ?0.673 mSv y(-1). Dust sampling revealed greatest values in the storage area. The annual average effective dose from inhalation of long-lived airborne was 0.113 mSv y(-1). Radon gas concentrations in the processing plant and storage area were found to be of the same value as the background. In this study the estimated annual effective doses to workers were below 1 mSv y(-1). PMID:22361352

7

Basic radiological studies contamination control experiments  

This report describes the results of experiments relating to contamination control performed in support of the Environmental Restoration Programs Retrieval Project. During the years 1950 to 1970 waste contaminated with plutonium and other transuranic radionuclides was disposed of in shallow land-filled pits and trenches at the Idaho National Engineering Laboratory. Due to potential for migration of radionuclides to an existing aquifer the feasibility of retrieving and repackaging the waste for placement in a final repository is being examined as part of a retrieval project. Contamination control experiments were conducted to determine expected respirable and nonrespirable plutonium contaminated dust fractions and the effectiveness of various dust suppression techniques. Three soil types were tested to determine respirable fractions: Rocky Flats Plant generic soil, Radioactive Waste Management Complex generic soil, and a 1:1 blend of the two soil types. Overall, the average respirable fraction of airborne dust was 5.4% by weight. Three contamination control techniques were studied: soil fixative sprays, misting agents, and dust suppression agents. All of the tested agents proved to be effective in reducing dust in the air. Details of product performance and recommended usage are discussed.

8

Fission product plateout and liftoff in the MHTGR primary system: A review  

A review is presented of the technical basis for predicting radioactivity release resulting from depressurization of an MHTGR primary system. Consideration is restricted to so called dry events with no involvement of the steam system. The various types of deposition mechanisms effective for iodine, cesium, strontium, and silver are discussed in terms of their chemical characteristics and the nature of the materials in the primary system. Emphasis is given to iodine behavior, including means for estimating the quantity available for release, the types of plateout locations in the primary system, and the effect of dust on distribution and release. The behavior of fission products cesium, strontium, and silver in such accidents is presented qualitatively. A major part of the review deals with expected dust levels, types, and transport. Available information on the level and nature of dust in the HTGR primary system is reviewed. A summary is presented of dust deposition and liftoff mechanisms. It was concluded that recent approaches to dust liftoff modeling, based on turbulent burst concepts for removal from surfaces, probably offer advantages over the current shear ratio approach. This study concludes that iodine releases from dry depressurization events are likely to be extremely low, on the order of millicuries, due to a predictably low degree of chemical desorption, a low degree of dust liftoff, and a low involvement of iodine with dust. It was also concluded that deposition mechanisms controlling the distribution of fission product material in the primary system, and hence also controlling the degree of liftoff, depend strongly on the chemical nature of the individual elements. Therefore contrary to the current practice, both plateout and liftoff models should reflect those unique chemical and physical properties. 56 refs., 16 figs., 23 tabs.

9

The fragmentation of porous dust in cometary comae due to the internal gas pressure  

In-situ observations of the Dust Flux Monitor Instrument on Stardust showed the variations of dust flux and size distribution One of the possible interpretations of the date is the occurrence of dust fragmentations Moreover high spatial resolution observations show variations of dust light scattering properties in cometary comae which also imply dust fragmentations The dust fragmentation has also been considered as one of the proposed mechanisms to produce an extended source of gas in comae The existence of extended sources has been confirmed by both in-situ and remote observations We investigate the possibility of dust fragmentation due to the gas pressure that built up inside the porous dust For this we carry out model calculations to simulate the heating of a mixture of ice and dust The model takes into account the gas leaking through porous dust material and the heat transfer within porous dust Discussion is given on whether dust fragmentation due to the gas pressure is plausible or not

10

ASSESSMENT OF RADIONUCLIDE RELEASE FROM CONTAMINATED CONCRETE AT THE YANKEE NUCLEAR POWER STATION.  

Yankee Atomic Energy Company (YAEC) is considering allowing portions of existing structures at the Yankee Nuclear Power Station (YNPS) to remain on site at the time of license termination. Accordingly, release of residual radioactive contaminants (i.e., H-3, C-14, Co-60, Ni-63, Sr-90, and Cs-137) from remaining subsurface concrete structures (Darman, 2004) and dose due to that release must be evaluated. Analyses were performed using DUST-MS to assess the rate of release for each radionuclide from the concrete, based upon an assumed concentration of 1 pCi/g and a concrete density of 2.5 g/cm{sup 3}. Using the same assumptions that were applied to the soil DCGL calculation (and where appropriate, the same input parameters), RESRAD was used to calculate the dose from water pathways. Values for selected RESRAD input parameters were chosen to match the release rate calculated by DUST-MS. The results indicated that Cs-137 yielded the highest dose.

11

Reduction of airborne radioactive dust by means of a charged water spray  

An electrostatic precipitator based on charged water spray technology has been used in an underground uranium mine to control long-lived radioactive dust and short-lived aerosol concentration in a mine gallery where dust from a rock breaking/ore transportation operation was discharged. Two main sampling stations were established: one upstream of the dust precipitator and one downstream. In addition, dust samplers were placed at different locations between the dust discharge and the end of the mine gallery. Long-lived radioactive dust was measured using cascade impactors and nylon cyclone dust samplers, and measurement of the radioactivity on the samples was carried out by conventional methods. Radon and thoron progeny were estimated using standard techniques. Experiments were conducted under a variety of airflow conditions. A maximum radioactive dust reduction of about 40% (approximately 20% caused by gravitational settling) at a ventilation rate of 0.61 m{sup 3}/sec was obtained as a result of the combined action of water scrubbing and electrostatic precipitation by the charged water spray electrostatic precipitator. This represents the optimum efficiency attained within the range of ventilation rates investigated. The dust reduction efficiency of the charged water spray decreased with increasing ventilation rate, i.e., decreasing air residence time, and hence, reduced dust cloud/charged water droplets mixing time.

12

Anomalous dust temperature in dusty plasma experiments  

Dust heating in dusty plasmas due to thermal electric field fluctuations and dust acoustic waves is examined. It is shown that dust particles acquire large random motion in fluctuating electric fields (within dust cloud) of background plasma causing dust electrostatic pressure Formula Not Shown [K. Avinash, Phys. Plasmas 13 (2006) 012109] and corresponding large temperature Formula Not Shown . Due to quadratic dependence on Formula Not Shown and high dust charge ( Formula Not Shown ), Formula Not Shown is much bigger than the dust kinetic temperature Formula Not Shown and is in the range of 10â??????300 eV for typical experimental numbers. Using global energy constraints dust heating due to dust acoustic waves is examined. It is shown that dust acoustic waves are potentially capable of he...

13

Plasma Emission Modifications and Instabilities Induced by the Presence of Growing Dust Particles  

Formation of dust particles in a plasma can strongly change its properties due to electron attachment on dust surface. An easy way to detect dust formation is to analyze modifications of the plasma emission. In this paper, changes in the plasma emission are related to the growth of dust particles. W...

14

Purification of the off-gases of the process of radioactive waste vitrification in induction melter  

Moscow SIA RADON has developed the method of vitrifying both radioactive ashes, arising from radioactive waste incineration, and liquid radioactive waste in induction melter. In the experimental plant the characteristics of off-gases were determined and various constructions of filters and filtering materials for dust trapping were tested. On the base of test results the plant for liquid radioactive waste vitrification has been constructed on the base of induction melter {sup c}old crucible{sup ,} equipped with modern effective dust and gas purification system, consisting of filtration unit, absorption unit and unit for nitrogen oxide catalytic reduction. (author). 3 refs., 9 tabs., 3 figs.

15

User's manual for RESRAD-BUILD version 3.  

The RESRAD-BUILD computer code is a pathway analysis model designed to evaluate the potential radiological dose incurred by an individual who works or lives in a building contaminated with radioactive material. The transport of radioactive material within the building from one compartment to another is calculated with an indoor air quality model. The air quality model considers the transport of radioactive dust particulates and radon progeny due to air exchange, deposition and resuspension, and radioactive decay and ingrowth. A single run of the RESRAD-BUILD code can model a building with up to three compartments, four source geometries (point, line, area, and volume), 10 distinct source locations, and 10 receptor locations. The volume source can be composed of up to five layers of different materials, with each layer being homogeneous and isotropic. A shielding material can be specified between each source-receptor pair for external gamma dose calculations. The user can select shielding material from eight different material types. Seven exposure pathways are considered in the RESRAD-BUILD code: (1) external exposure directly from the source, (2) external exposure to materials deposited on the floor, (3) external exposure due to air submersion, (4) inhalation of airborne radioactive particulates, (5) inhalation of aerosol indoor radon progeny and tritiated water vapor, (6) inadvertent ingestion of radioactive material directly from the source, and (7) ingestion of materials deposited on the surfaces of the building compartments. Various exposure scenarios may be modeled with the RESRAD-BUILD code. These include, but are not limited to, office worker, renovation worker, decontamination worker, building visitor, and residency scenarios. Both deterministic and probabilistic dose analyses can be performed with RESRAD-BUILD, and the results can be shown in both text and graphic reports.

16

Paleoclimatology: Speleothems : Feature Articles  

Jun 28, 2005 ... Loess deposits, composed of fine wind-blown dust produced by the grinding ... by measuring how much uranium, a radioactive element, has decayed. ... “In southeast Brazil, for example, winter rain comes from the nearby ...

17

Solitary waves and vortices in plasmas with nanoparticles  

Dust ion-acoustic (DIA) solitons in complex plasmas are considered, and acoustic-gravitational vortices with nanoscale dust particles and dust vortices at altitudes of the ionosphere are studied. "Weakly-dissipative" DIA compressive and rarefactive solitons propagating with decreasing velocity are shown to exist. Vortex motions in the ionosphere are demonstrated to be closely connected with dynamics of the dust nanoscale particles. Redistribution of nanoscale dust particles in the ionosphere is possible due to vortical motions.

18

Model of particle resuspension in turbulent flows  

The graphite dust generated in an HTR/PBMR during normal reactor operation is deposited inside the primary system and becomes radioactive due to sorption of fission products. A significant amount of radioactive dust may be resuspended and released to the environment in case of LOCA. Therefore accurate particle resuspension models are required for HTR/PBMR safety analyses. Thermal-hydraulic safety analyses of HTR/PBMR type reactors are typically performed using computer codes such as FLOWNEX, MELCOR, or SPECTRA. None of these codes currently includes a well-tested mechanistic resuspension model. The resuspension model based on the Vainshtein model has been developed and implemented into the SPECTRA thermal-hydraulic system code. The resuspension model formulation has been extended in such way that other formulations, for example the Rock'n Roll model, may easily be defined and used within the general model framework. Several test calculations were performed, including comparisons of the numerical SPECTRA results with the analytical solutions obtained by means of MathCAD. Furthermore, comparisons with the experimental results of the Reeks and Hall, and STORM experiments were made. It was concluded that the model gives satisfactory results for a number of tests.

19

Radiocesium contamination at a steel plant in Ireland.  

Radioactive sources have been inadvertently incorporated into consignments of scrap metal in various locations throughout the world. In 1990, a 3.7 GBq 137 Cs source, due for transfer from a Scottish industrial establishment to one in England, was mistakenly included in a scrap consignment destined for Irish Steel, a metal recycling plant in County Cork in the Republic of Ireland. Unaware of the presence of the source, Irish Steel smelted this consignment in the usual manner. This involved separation of some non-ferrous materials which were then exported, in pellet form, To Pasminco Europe (now Britannia Zinc Ltd.) in Avonmouth, U.K. The presence of 137 Cs contamination in these pellets was detected by the U.K. company in the course of a routine radiation survey. Irish Steel carried out extensive decontamination of its plant, placing the contaminated dust in secure storage. The company has equipped itself with radiation detection devices which monitor incoming scrap. Outgoing products and furnace dust are also monitored on a routine basis. While this incident was of negligible radiological significance as far as personnel were concerned, the financial cost to Irish Steel have been substantial. It highlights the need for surveillance, by national competent authorities, of the movement of radioactive sources from production through use to final disposal. PMID:8617600

20

Stabilization of the Shear Instability in a Dust Layer of a Protoplanetary Disk and Possible Formation of Planetesimals due to Gravitational Fragmentation of the Dust Layer  

We show that the planetesimal formation due to the gravitational fragmentation of a dust layer in a protoplanetary disk is possible. The dust density distribution in the dust layer would approach the constant Richardson number distribution due to the dust stirring by the shear instability and dust settling. We perform the analysis of the shear instability of dust layer in a protoplanetary disk with the constant Richardson number density distribution. Our study revealed that this distribution is stable against the shear instability even if the dust density at the midplane reaches the critical density of the gravitational instability, and the planetesimal formation through the gravitational fragmentation of the dust layer can occur even for the dust to gas surface density ratio with the solar composition.

 
 
 
 
21

Respirable quartz hazard associated with coal mine roof bolter dust  

Pneumoconiosis has been reported to be increasing among underground coal miners in the Southern Appalachian Region. The National Institute for Occupational Safety and Health conducted a study to examine the particle size distribution and quartz content of dust generated by the installation of roof bolts in mines. Forty-six bulk samples of roof bolting machine pre-cleaner cyclone dump dust and collector box dust were collected from 26 underground coal mines. Real-time and integrated airborne respirable dust concentrations were measured on 3 mining sections in 2 mines. The real-time airborne dust concentrations profiles were examined to identify any concentration changes that might be associated with pre-cleaner cyclone dust discharge events. The study showed that bolter dust is a potential inhalation hazard due to the fraction of dust less than 10 {mu}m in size, and the quartz content of the dust. The pre-cleaner cyclone dust was significantly larger than the collector box dust, indicating that the pre-cleaner functioned properly in removing the larger dust size fraction from the airstream. However, the pre-cleaner dust still contained a substantial amount of respirable dust. It was concluded that in order to maintain the effectiveness of a roof bolter dust collector, periodic removal of dust is required. Appropriate work procedures and equipment are necessary to minimize exposure during this cleaning task. 13 refs., 3 tabs., 2 figs.

22

On the usability of frequency distributions and source attribution of Cs-137 detections encountered in the IMS radio-nuclide network for radionuclide event screening and climate change monitoring  

Under the provisions of the Comprehensive Nuclear-Test-Ban Treaty (CTBT), airborne radioactivity is measured by means of high purity Germanium gamma ray detectors deployed in a global monitoring network. Almost 60 of the scheduled 80 stations have been put in provisional operations by the end of 2008. Each station daily sends the 24 hour samples' spectroscopic data to the Vienna based Provisional Technical Secretariat (PTS) of the CTBT Organization (CTBTO) for review for treaty-relevant nuclides. Cs-137 is one of these relevant isotopes. Its typical minimum detectable concentration is in the order of a few Bq/m3. However, this isotope is also known to occur in atmospheric trace concentrations, due to known non CTBT relevant processes and sources related to, for example, the re-suspension of cesium from historic nuclear tests and/or the Chernobyl reactor disaster, temporarily enhanced by bio-mass burning (Wotawa et al. 2006). Properly attributed cesium detections can be used as a proxy to detect Aeolian dust events (Igarashi et al, 2001) that potentially carry cesium from all aforementioned sources but are also known to play an important role for the radiative forcing in the atmosphere (shadow effect), at the surface (albedo) and the carbon dioxide cycle when interacting with oceanic phytoplankton (Mikami and Shi, 2005). In this context this paper provides a systematic attribution of recent Cs-137 detections in the PTS monitoring network in order to Characterize those stations which are regularly affected by Cs-137 Provide input for procedures that distinguish CTBT relevant detection from other sources (event screening) Explore on the capability of certain stations to use their Cs-137 detections as a proxy to detect aeolian dust events and to flag the belonging filters to be relevant for further investigations in this field (-> EGU-2009 Session CL16/AS4.6/GM10.1: Aeolian dust: initiator, player, and recorder of environmental change). References Igarashi, Y., M. Aoyama, K. Hirose,M. Takashi and S. Yabuki, 2001: Is It Possible to Use 90Sr and 137Cs As Tracers for the Aeolian Dust Transport? Water, Air, & Soil Pollution 130, 349-354. Mikami, M. and G. Shi, 2005: Preliminary summary of aeolian dust experiment on climate impact -Japan-Sino joint project ADEC. Geophysical Research Abstracts, 7, 05985 Wotawa, G., L.-E. De Geer, A. Becker, R.D'Amours, M. Jean, R. Servranck and K. Ungar, 2006: Inter- and intra-continental transport of radioactive cesium released by boreal forest fires, Geophys. Res. Lett. 33, L12806, doi: 10.1029/2006GL026206 Disclaimer The views expressed in this publication are those of the author and do not necessarily reflect the views of the CTBTO Preparatory Commission.

23

Reducing aluminum dust explosion hazards: case study of dust inerting in an aluminum buffing operation.  

Metal powders or dusts can represent significant dust explosion hazards in industry, due to their relatively low ignition energy and high explosivity. The hazard is well known in industries that produce or use aluminum powders, but is sometimes not recognized by facilities that produce aluminum dust as a byproduct of bulk aluminum processing. As demonstrated by the 2003 dust explosion at aluminum wheel manufacturer Hayes Lemmerz, facilities that process bulk metals are at risk due to dust generated during machining and finishing operations [U.S. Chemical Safety and Hazard Investigation Board, Investigation Report, Aluminum Dust Explosion Hayes Lemmerz International, Inc., Huntington, Indiana, Report No. 2004-01-I-IN, September 2005]. Previous studies have shown that aluminum dust explosions are more difficult to suppress with flame retardants or inerting agents than dust explosions fueled by other materials such as coal [A.G. Dastidar, P.R. Amyotte, J. Going, K. Chatrathi, Flammability limits of dust-minimum inerting concentrations, Proc. Saf. Progr., 18-1 (1999) 56-63]. In this paper, an inerting method is discussed to reduce the dust explosion hazard of residue created in an aluminum buffing operation as the residue is generated. This technique reduces the dust explosion hazard throughout the buffing process and within the dust collector systems making the process inherently safer. Dust explosion testing results are presented for process dusts produced during trials with varying amounts of flame retardant additives. PMID:18423857

24

Thermophoresis and dust devils on the planet Mars  

In the Martian atmosphere dust is abundant and is continuously replenished by the entrainment of materials and sediments from the surface of the planet. The sediment concentrations are particularly high and noticeable in whirlwinds, also known as dust devils. Assuming the thermophoresis force as the main driver of dust particles lifting from the surface, the dust process of the Martian atmosphere and its naturally formed dust devils are investigated for the northern polar region of the planet. Our simulated convective boundary layer shows that it may be unlikely that visible dust devils are formed only due to thermophoresis effects and some other lifting mechanisms are required.

25

Magneto-thermal condensation modes including the effects of charged dust particles  

We study thermal instability in a magnetized and partially ionized plasma with charged dust particles. Our linear analysis shows that the growth rate of the unstable modes in the presence of dust particles strongly depends on the ratio of the cooling rate and the modified dust-cyclotron frequency. If the cooling rate is less than the modified dust-cyclotron frequency, then growth rate of the condensation modes does not modify due to the existence of the charged dust particles. But when the cooling rate is greater than (or comparable to) the modified dust-cyclotron frequency, the growth rate of unstable modes increases because of the dust particles. Also, wavenumber of the perturbations corresponding to the maximum growth rate shifts to the smaller values (larger wavelengths) as the cooling rate becomes larger than the modified dust-cyclotron frequency. We show that growth rate of the condensation modes increases with the electrical charge of the dust particles.

26

Detection of Interstellar Dust with STEREO/WAVES at 1 AU  

Most in situ measurements of cosmic dust have been carried out with dedicated dust instruments. However, dust particles can also be detected with radio and plasma wave instruments. The high velocity impact of a dust particle generates a small crater on the spacecraft, and the dust particle and the crater material are vaporised and partly ionised. The resulting electric charge can be detected with plasma instruments designed to measure electric waves. Since 2007 the STEREO/WAVES instrument has recorded a large number of events due to dust impacts. Here we will concentrate on the study of those impacts produced by dust grains originating from the local interstellar cloud. We present these fluxes during five years of the STEREO mission. Based on model calculations, we determine the direction of arrival of interstellar dust. We find that the interstellar dust direction of arrival is ˜260?, in agreement with previous studies.

27

Dusty plasmas: synthesis, structure and dynamics of a dust cloud in a plasma  

Plasmas are energetic media that can give birth to dust particles due to the presence of reactive gases or plasma-surface interactions. Industrial plasmas are often concerned by these dust particles that can be either unwanted or useful for the process. For fusion plasmas, production of dust particl...

28

Evaluation of occupational exposure to naturally occurring radioactive materials in the Iranian ceramics industry.  

Zircon contains small amounts of uranium, thorium and radium in its crystalline structure. The ceramic industry is one of the major consumers of zirconium compounds that are used as an ingredient at ?10-20 % by weight in glaze. In this study, seven different ceramic factories have been investigated regarding the presence of radioactive elements with focus on natural radioactivity. The overall objective of this investigation is to provide information regarding the radiation exposure to workers in the ceramic industry due to naturally occurring radioactive materials. This objective is met by collecting existing radiological data specific to glaze production and generating new data from sampling activities. The sampling effort involves the whole process of glaze production. External exposures are monitored using a portable gamma-ray spectrometer and environmental thermoluminescence dosimeters, by placing them for 6 months in some workplaces. Internal routes of exposure (mainly inhalation) are studied using air sampling, and gross alpha and beta counting. Measurement of radon gas and its progeny is performed by continuous radon gas monitors that use pulse ionisation chambers. Natural radioactivity due to the presence of ²³?U, ²³²Th and ??K in zirconium compounds, glazes and other samples is measured by a gamma-ray spectrometry system with a high-purity germanium detector. The average concentrations of ²³?U and ²³²Th observed in the zirconium compounds are >3300 and >550 Bq kg?¹, respectively. The specific activities of other samples are much lower than in zirconium compounds. The annual effective dose from external radiation had a mean value of ?0.13 mSv y?¹. Dust sampling revealed the greatest values in the process at the powdering site and hand weighing places. In these plants, the annual average effective dose from inhalation of long-lived airborne radionuclides was 0.226 mSv. ²²²Rn gas concentrations in the glaze production plant and storage warehouse were found to range from 10 to 213 Bq m?³. In this study, the estimated annual effective doses to exposed workers were <1 mSv y?¹. PMID:21148590

29

DUSTMS-D: DISPOSAL UNIT SOURCE TERM - MULTIPLE SPECIES - DISTRIBUTED FAILURE DATA INPUT GUIDE.  

Performance assessment of a low-level waste (LLW) disposal facility begins with an estimation of the rate at which radionuclides migrate out of the facility (i.e., the source term). The focus of this work is to develop a methodology for calculating the source term. In general, the source term is influenced by the radionuclide inventory, the wasteforms and containers used to dispose of the inventory, and the physical processes that lead to release from the facility (fluid flow, container degradation, wasteform leaching, and radionuclide transport). Many of these physical processes are influenced by the design of the disposal facility (e.g., how the engineered barriers control infiltration of water). The complexity of the problem and the absence of appropriate data prevent development of an entirely mechanistic representation of radionuclide release from a disposal facility. Typically, a number of assumptions, based on knowledge of the disposal system, are used to simplify the problem. This has been done and the resulting models have been incorporated into the computer code DUST-MS (Disposal Unit Source Term-Multiple Species). The DUST-MS computer code is designed to model water flow, container degradation, release of contaminants from the wasteform to the contacting solution and transport through the subsurface media. Water flow through the facility over time is modeled using tabular input. Container degradation models include three types of failure rates: (a) instantaneous (all containers in a control volume fail at once), (b) uniformly distributed failures (containers fail at a linear rate between a specified starting and ending time), and (c) gaussian failure rates (containers fail at a rate determined by a mean failure time, standard deviation and gaussian distribution). Wasteform release models include four release mechanisms: (a) rinse with partitioning (inventory is released instantly upon container failure subject to equilibrium partitioning (sorption) with the waste form), (b) diffusion release.(release from either a cylindrical, spherical, or rectangular wasteform), (c) dissolution release (uniform release over time due to dissolution of the wasteform surface), and (d) solubility limited release. The predicated wasteform releases are corrected for radioactive decay and ingrowth. A unique set of container failure and wasteform release parameters can be specified for each control volume with a container. Contaminant transport is modeled through a finite-difference solution of the advective transport equation with sources (wasteform release and ingrowth) and radioactive decay. Although DUST-MS simulates one-dimensional transport, it can be used to simulate migration down to an aquifer and then transport in the aquifer by running the code twice. A special subroutine allows the flux into the aquifer from the first simulation to be input as the flux at the upstream boundary in the aquifer. This document presents the models used to calculate release from a disposal facility, verification of the model, and instructions on the use of the DUST-MS code. In addition to DUST-MS, a preprocessor, DUSTINMS, which helps the code user create input decks for DUST-MS and a post-processor, GRAFMS, which takes selected output files and plots them on the computer terminal have been written. Use of these codes is also described. In using DUST-MS, as with all computer models, the validity of the predictions relies heavily on the validity of the input parameters. Often, the largest uncertainties arise from uncertainty in the input parameters. Therefore, it is crucial to document and support the use of these parameters. The DUST-MS code, because of its flexibility and ability to compute release rates quickly, is extremely useful for screening to determine the radionuclide released at the highest rate, parameter sensitivity analysis and, with proper choice of the input parameters, provide upper bounds to release rates.

30

Public exposure to hazards associated with natural radioactivity in open-pit mining in Ghana  

The results of studies carried out on public exposure contribution from naturally occurring radioactive materials (NORMS) in two open-pit mines in the Western and Ashanti regions of Ghana are reported. The studies were carried out under International Atomic Energy Agency-supported Technical Co-operation Project GHA/9/005. Measurements were made on samples of water, soil, ore, mine tailings and air using gamma spectrometry. Solid-state nuclear track detectors were used for radon concentration measurements. Survey was also carried out to determine the ambient gamma dose rate in the vicinity of the mines and surrounding areas. The effective doses due to external gamma irradiation, ingestion of water and inhalation of radon and ore dusts were calculated for the two mines. The average annual ef...

31

The possibility of radioactive dust collection in fusion reactor by use of thermophoretic force  

A large amount of radioactive dusts are generated in fusion reactors as a result of sputtering and/or plasma disruption, and they adhere and deposit in the vacuum vessel. The condition in the vessel is in high vacuum of 10{sup -4} Torr order as well as strong electromagnetic field. Once the vacuum condition is destroyed to collect the dusts, the vacuum pumping of the huge vessel requires at least several days or a week. Therefore, it is necessary for an economical operation to collect the dusts without destroying the vacuum. In this research, a dust collecting system that makes use of thermophoresis phenomenon known as a rarefaction effect of gas is proposed and its experimental verification is performed to examine its possibility. The system is very simple, namely, temperature gradient is made by setting a low temperature plate close to another high temperature wall on which the dusts are deposited and the dusts are recovered onto the low temperature plate by the thermophoresis phenomenon. It has been found that, in principle, it is possible to collect the radioactive dusts by weakening adhesive force which acts on the dusts and raising temperature gradient enough. (author)

32

Coupling Mars' Dust and Water Cycles: Effects on Dust Lifting Vigor, Spatial Extent and Seasonality  

The dust cycle is an important component of Mars' current climate system. Airborne dust affects the radiative balance of the atmosphere, thus greatly influencing the thermal and dynamical state of the atmosphere. Dust raising events on Mars occur at spatial scales ranging from meters to planet-wide. Although the occurrence and season of large regional and global dust storms are highly variable from one year to the next, there are many features of the dust cycle that occur year after year. Generally, a low-level dust haze is maintained during northern spring and summer, while elevated levels of atmospheric dust occur during northern autumn and winter. During years without global-scale dust storms, two peaks in total dust loading were observed by MGS/TES: one peak occurred before northern winter solstice at Ls 200-240, and one peak occurred after northern winter solstice at L(sub s) 305-340. These maxima in dust loading are thought to be associated with transient eddy activity in the northern hemisphere, which has been observed to maximize pre- and post-solstice. Interactive dust cycle studies with Mars General Circulation Models (MGCMs) have included the lifting, transport, and sedimentation of radiatively active dust. Although the predicted global dust loadings from these simulations capture some aspects of the observed dust cycle, there are marked differences between the simulated and observed dust cycles. Most notably, the maximum dust loading is robustly predicted by models to occur near northern winter solstice and is due to dust lifting associated with down slope flows on the flanks of the Hellas basin. Thus far, models have had difficulty simulating the observed pre- and post- solstice peaks in dust loading. Interactive dust cycle studies typically have not included the formation of water ice clouds or their radiative effects. Water ice clouds can influence the dust cycle by scavenging dust from atmosphere and by interacting with solar and infrared radiation, thereby modifying the thermal structure of the atmosphere and its circulation. Results presented in other papers at this workshop show that including the radiative effects of water ice clouds greatly influence the water cycle and the vigor of weather systems in both the northern and southern hemispheres. Our goal is to investigate the effects of fully coupling the dust and water cycles on the dust cycle. We show that including water ice clouds and their radiative effects greatly affect the magnitude, spatial extent and seasonality of dust lifting and the season of maximum atmospheric dust loading.

33

Assessment of the radiological impact of oil refining industry  

The field of radiation protection and corresponding national and international regulations has evolved to ensure safety in the use of radioactive materials. Oil and gas production processing operations have been known to cause naturally occurring radioactive materials (NORMs) to accumulate at elevated concentrations as by-product waste streams. A comprehensive radiological study on the oil refining industry in Egypt was carried out to assess the radiological impact of this industry on the workers. Scales, sludge, water and crude oil samples were collected at each stage of the refining process. The activity concentration of {sup 226}Ra, {sup 232}Th and {sup 40}K were determined using high-resolution gamma spectrometry. The average activity concentrations of the determined isotopes are lower than the IAEA exempt activity levels for NORM isotopes. Different exposure scenarios were studied. The average annual effective dose for workers due to direct exposure to gamma radiation and dust inhalation found to be 0.6 muSv and 3.2 mSv, respectively. Based on the ALARA principle, the results indicate that special care must be taken during cleaning operations in order to reduce the personnel's exposure due to maintenance as well as to avoid contamination of the environment.

34

Active dust control and mitigation technology for lunar and Martian exploration  

Mars is covered with a layer of dust that has been homogenized by global dust storms. Dust, levitated by these storms as well as by the frequent dust devils, is the dominant weather phenomenon on Mars. NASA's Mars exploration rovers have shown that atmospheric dust falling on solar panels can decrease their efficiency to the point of rendering the rover unusable. Dust covering the surface of the moon is expected to be electrostatically charged due to the solar wind, cosmic rays, and the solar radiation itself through the photoelectric effect. Electrostatically charged dust has a large tendency to adhere to surfaces. The Apollo missions to the moon showed that lunar dust adhesion can hinder manned and unmanned exploration activities. In this paper, we report on our efforts to develop an ele...

35

Geometry optimisation of a gravity dust-catcher using computational fluid dynamics simulation  

A gravity dust-catcher is a high tonnage device that is widely used to separate a mixture of dusts from blast furnace (BF) top gas flow. Dusts include limestone, iron ore and coke/coal. The flow pattern within the dust-catcher is complex due to the turbulent vortices formed within, consequently making it hard to accurately predict dust-catcher performance. Using data from an on-site dust-catcher, CFD simulations are conducted on a range of geometry modifications to produce an optimised dust-catcher design specification. The effect on particle separation efficiency during a typical blast furnace (BF) operational cycle is analysed. An attempt is made to develop and optimise a more efficient gravity dust-catcher using CFD simulation results at distinct stages of the design process. It is conc...

36

Influence of section intake dust levels as an exposure assessment parameter in Dust Exposure Level Index (DELI) model  

This paper summarises the intake dust levels measured in selected South African underground coal mining sections over the past five years and its use as a parameter in assessing worker exposure to dust through a newly developed model called the Dust Exposure Level Index (DELI). Based on the measured data of the South African coal mines, the average section intake dust level was 0.78 mg/m{sup 3}. Approximately 60 per cent of the samples collected for the study have exceeded the 0.5 mg/m{sup 3}. The intake dust level measured at a longwall face was much higher than in the CM headings. The measured section intake dust levels furnish the South African coal mining industry with the latest depiction of the level of face area dust contamination due to the intake air. Further, this paper demonstrates the use of intake dust level as a parameter in estimating exposure levels of workers, as it clearly plays as a corner stone in effective control of exposure to face area respirable dust. It must be borne in mind that intake dust is a base level to the mine worker exposed to dust without carrying out any additional work in the section. If the intake air is seriously contaminated by airborne respirable dust; then the exposure of the workforce in the section will constantly be elevated by that background dust level. 20 refs., 4 figs., 1 tab.

37

Dust-Particle Transport in Tokamak Edge Plasmas  

Dust particulates in the size range of 10nm-100{micro}m are found in all fusion devices. Such dust can be generated during tokamak operation due to strong plasma/material-surface interactions. Some recent experiments and theoretical estimates indicate that dust particles can provide an important source of impurities in the tokamak plasma. Moreover, dust can be a serious threat to the safety of next-step fusion devices. In this paper, recent experimental observations on dust in fusion devices are reviewed. A physical model for dust transport simulation, and a newly developed code DUSTT, are discussed. The DUSTT code incorporates both dust dynamics due to comprehensive dust-plasma interactions as well as the effects of dust heating, charging, and evaporation. The code tracks test dust particles in realistic plasma backgrounds as provided by edge-plasma transport codes. Results are presented for dust transport in current and next-step tokamaks. The effect of dust on divertor plasma profiles and core plasma contamination is examined.

38

Status of Activities on Rehabilitation Of Radioactively Contaminated Facilities and the Site of Russian Research Center ''Kurchatov Institute''  

This paper describes the program, the status, and the course of activities on rehabilitation of radioactively contaminated facilities and the territory of temporary radioactive waste (radwaste) disposal at the Russian Research Center ''Kurchatov Institute'' (RRC KI) in Moscow as performed in 2001-2002. The accumulation of significant amounts of radwaste at RRC KI territory is shown to be the inevitable result of Institute's activity performed in the days of former USSR nuclear weapons project and multiple initial nuclear power projects (performed from 1950's to early 1970's). A characterization of RRC KI temporary radwaste disposal site is given. Described is the system of radiation control and monitoring as implemented on this site. A potential hazard of adverse impacts on the environment and population of the nearby housing area is noted, which is due to possible spread of the radioactive plume by subsoil waters. A description of the concept and project of the RRC KI temporary radwaste disposal site is presented. Specific nature of the activities planned and performed stems from the nearness of housing area. This paper describes main stages of the planned activities for rehabilitation, their expected terms and sources of funding, as well as current status of the project advancement. Outlined are the problems faced in the performance and planning of works. The latter include: diagnostics of the concrete-grouted repositories, dust-suppression technologies, packaging of the fragmented ILW and HLW, soil clean-up, radioactive plume spread prevention, broad radiation monitoring of the work zone and environment in the performance of rehabilitation works. Noted is the intention of RRC KI to establish cooperation with foreign, first of all, the U.S. partners for the solution of problems mentioned above.

39

Assessment of the amount of lung tumors induced by radon and radon-daughter-products in the Netherlands. Schatting van het aantal longtumoren veroorzaakt door radon en radon-dochterprodukten in Nederland  

Radon is a radioactive noble gas. After the decay of radon, the daughter products become attached to dust particles. The inhaled dust particles can induce lung tumours by the alpha radiation they emit. In this article an assessment is given for the amount of deaths caused by radon induced lung tumors in the Netherlands and the dispersion as result of the uncertainties of the risk factors. (R.B.). 22 refs.; 2 figs.; 1 tab.

40

Theory of dust and dust-void structures  

A dust void appears as a dust-free region where the plasma ionization rate (comparatively higher than that in a dust region due to strong plasma dissipation on dust particles) supports an outward ion flow exerting an outward ion drag force on the dust particles. The sharp dust-void boundary presents a new type of discontinuities in a dusty plasma where the dust density can change rapidly while the ion and electron densities as well as the dust charge are continuous. The observed boundaries are often stationary, with the established balance of forces acting on dust particles. Here, we investigate the dust void structures in the case when the ion diffusion on the neutral gas atoms plays an important role. We demonstrate that this dissipative process not only allows the existence of the dust voids (i. e., the absence of dust grains in the void region) but can create new types of discontinuities inside the dust structure. The results are obtained for a one-dimensional model, with planar geometry that is symmetric about the center of the void, by numerical investigation of the stationary force balance equations for the void structure. In the considered model, we numerically investigate the non-linear balance equations and obtain new results. Namely, we show that if the ion diffusion on neutral gas atoms is taken into account, the dust density has no discontinuity (according to the dairy conditions used) at the surface of the dust boundary; nevertheless, the ion diffusion process still creates sharp dust boundaries with complete absence of dust in the void region. It appears that not the dust density but the derivatives of various plasma parameters have discontinuities at the dust boundary. Note that in the presence of the ion diffusion the condition that the dust density is zero at the void boundary is automatically fulfilled when the boundary conditions are satisfied. We therefore loose the previous important condition that the dust density jump at the boundary is positive which was a crucial for the selection of those surfaces that can describe the dust voids from other non-physical surfaces satisfying the boundary conditions. Thus in order to construct the theory of dust voids in this case we also have to revise the main concepts and procedures of the theoretical study of the dust void formation. (Author)

 
 
 
 
41

Simulating Mars' Dust Cycle with a Mars General Circulation Model: Effects of Water Ice Cloud Formation on Dust Lifting Strength and Seasonality  

The dust cycle is critically important for the current climate of Mars. The radiative effects of dust impact the thermal and dynamical state of the atmosphere [1,2,3]. Although dust is present in the Martian atmosphere throughout the year, the level of dustiness varies with season. The atmosphere is generally the dustiest during northern fall and winter and the least dusty during northern spring and summer [4]. Dust particles are lifted into the atmosphere by dust storms that range in size from meters to thousands of kilometers across [5]. Regional storm activity is enhanced before northern winter solstice (Ls200 degrees - 240 degrees), and after northern solstice (Ls305 degrees - 340 degrees ), which produces elevated atmospheric dust loadings during these periods [5,6,7]. These pre- and post- solstice increases in dust loading are thought to be associated with transient eddy activity in the northern hemisphere with cross-equatorial transport of dust leading to enhanced dust lifting in the southern hemisphere [6]. Interactive dust cycle studies with Mars General Circulation Models (MGCMs) have included the lifting, transport, and sedimentation of radiatively active dust. Although the predicted global dust loadings from these simulations capture some aspects of the observed dust cycle, there are marked differences between the simulated and observed dust cycles [8,9,10]. Most notably, the maximum dust loading is robustly predicted by models to occur near northern winter solstice and is due to dust lifting associated with down slope flows on the flanks of the Hellas basin. Thus far, models have had difficulty simulating the observed pre- and post- solstice peaks in dust loading.

42

Spitzer spectroscopy of carbon stars in the Small Magellanic Cloud  

ABSTRACT We present Spitzer Space Telescope spectroscopic observations of 14 carbon-rich asymptotic giant branch (AGB) stars in the Small Magellanic Cloud (SMC). SiC dust is seen in most of the carbon-rich stars but it is weak compared to Large Magellanic Cloud (LMC) stars. The SiC feature is strong only for stars with significant dust excess, opposite to what is observed for Galactic stars. We argue that in the SMC, SiC forms at lower temperature than graphite dust, whereas in the Galaxy SiC and graphite condensate at more comparable temperatures. Dust input into the interstellar medium by AGB stars consists mostly of carbonaceous dust, with little SiC or silicate dust. Only the two coolest stars show a 30-mm band due to MgS dust. We suggest that this is due to the fact that, in the SMC, ...

43

Use of SEVIRI images and derived products in a WMO Sand and dust Storm Warning System  

The Visible/IR images of SEVIRI (Spinning Enhanced Visible and Infrared Imager), on board Meteosat Second Generation (MSG) satellites, are used to monitor dust events. Satellite-based detection of dust is a difficult problem due in part to the observing-system limitations. The main difficulty is that the dust can be confused with water/ice clouds. SEVIRI is not as optimal for the viewing of dust as SEAWIFS or MODIS, due to the fact that both of them count with additional short-wavelength channels. However, the SEVIRI 15-minute loop images can detect small dust plumes as well as subtle changes from one image to the next. A description of how the AEMET, former INM, is developing the environment to support MSG satellite imagery to the WMO/GEO Sand and Dust Storm Warning System (SDS WS) for Europe, Africa and Middle East Regional Centre will be briefly presented, together with some on-going operational developments to best monitor dust events.

44

A dust storm over the Ukraine and Belarus territory contaminated by radionuclides after the Chernobyl accident  

A meteorological situation is under consideration during a dust storm observed on September 5â??????7, 1992 over the Ukraine and Belarus territory contaminated by radionuclide products after the Chernobyl accident. The highest average wind speed in Chernobyl and Pripyat was 10â??????12 m/s, wind gusts reached 20 m/s. It was found that the radioactive aerosol concentration in the zone of alienation of the Chernobyl NPP increased by one or two orders of magnitude. The transfer of radioactive dust particles to the Vilnius outskirts is recorded.

45

Electrostatic dust detector  

An apparatus for detecting dust in a variety of environments which can include radioactive and other hostile environments both in a vacuum and in a pressurized system. The apparatus consists of a grid coupled to a selected bias voltage. The signal generated when dust impacts and shorts out the grid is electrically filtered, and then analyzed by a signal analyzer which is then sent to a counter. For fine grids a correlation can be developed to relate the number of counts observed to the amount of dust which impacts the grid.

46

The effect of media area on the dust holding capacity of deep pleat HEPA filters  

The high potential cost of storage, treatment and disposal of radioactive wastes places a premium on the longevity of installed HEPA filters in situations in radioactive processing facilities where dust capacity is a life determining factor. Previous work investigated the dust holding capacity v pressure drop characteristics of different designs of HEPA filter and also the effect of using graded density papers. This paper records an investigation of the effect of media area variation on the dust holding capacity of the {open_quotes}deep-pleat{close_quotes} design of HEPA filter. As in the previously reported work two test dusts (carbon black and sub micron sodium chloride) in the range (0.15 - 0.4{mu}m) were used. Media area adjustment was effected by varying the number of separators within the range 60 - 90. Results with the coarser dust allowed an optimum media area to be identified. Media areas greater or smaller than this optimum retained less dust than the optimum for the same terminal pressure drop. Conversely with the finer sodium chloride aerosol the dust holding capacity continued to increase up to the maximum area investigated. 7 refs., 4 figs.

47

The Structure of the Dust Layer over the Taklimakan Deser during the Dust Storm in April 2002 as Observed Using a Depolarization Lidar  

In April 2002, a severe dust storm occurred in the Taklimakan Desert. A large amount of the dust was lifted up by the dust storm and gradually removed in the following few days. The whole event of the dust storm was observed by the Mie-scattering depolarization lidar at Aksu, Xinjiang, China (40.62°N, 80.83°E, 1028 m above mean sea level). This paper describes the dust event and the removal process that was observed by the lidar. During the dust storm (April 13-16), a dense dust layer developed from the ground up to 5.5 km. The backscattering ratio was 20 or more, and the depolarization ratio was 15-25%. Due to the absorption of the laser beam by the heavy dust, a normal lidar observation was impossible for several hours. In this study, we estimated the backscattering ratio at the lowest height during the dust storm by solving the lidar equation directly. After the dust storm (April 17-20), a clear diurnal variation of the top of the dust layer was found by the lidar. An investigation of the lidar signals at different heights shows that there were two types of the removal process of the dust. The lidar signals at lower heights (less than the 2 km) gradually decreased during the post-dust storm period. This result indicates that the gravitational settling of the relatively large sized dust (coarse particles with a diameter of 10 ?m or more) occurs near the ground. On the other hand, lidar signals at 2-4 km had a clear diurnal variation with spike-like peaks from evening to midnight. These peaks suggest that the advection of the relatively small sized dust picked up in other location is due to the local circulation that occurs in the Tianshan Mountains and Tarim Basin.   

48

Study of the Sensitivity of Optical Properties of Mineral Dust to the Direct Aerosol Radiative Perturbation Using a Global Aerosol Transport Model  

The sensitivity of optical properties of mineral dust aerosol to its direct radiative effect was investigated using four dust optical datasets (ADEC-1, ADEC-2, OPAC-MD and Dust-Like) with a global aerosol transport model. The annual and global mean direct aerosol radiative perturbation (DARP) by dust at the top of the atmosphere (TOA) can be positive or negative (-0.52 to +0.11 W m -2) depending on the absorptive property of dust aerosol dataset. The annual and global mean DARP at the surface is negative for all the dust optical datasets (-1.25 to -0.27 W m -2). If dust is strongly absorptive, DARP at the TOA over oceans at high latitude (> 40°) is positive due to the vertical configuration of dust and clouds. The longwave heating at the surface is strong and can exceed the shortwave cooling over desert regions if the absorption of dust is weak. Over a surface with high dust loading, the annual mean shortwave (longwave) DARP can reach -28 W m -2 (+16 W m -2). The global mean DARP values both at the TOA and surface are almost proportional to the imaginary part of the refractive index of dust. Seasonal variations of global mean DARP at the TOA significantly depend on the optical properties of dust.   

49

The Effects of Snow Cover and Soil Moisture on Asian Dust: I. A Numerical Sensitivity Study  

Semi-arid regions of East Asian dust source areas are frequently covered by snow. We conducted a sensitivity study of East Asian dust storms to investigate the effects of snow cover and soil moisture with a global aerosol model (MASINGAR). The simulated dust concentration greatly underestimated the dust event in late March 2007 relative to the observed PM10 concentration. When the effect of soil moisture is not taken into consideration, the simulated total dust emission amount is almost doubled, and the simulated dust concentration is comparable or overestimated with regard to the PM10 observations. The result of the sensitivity study suggests that the underestimation of the dust event is due to excessive soil moisture, which suppresses the dust emission. In contrast, the simulated dust concentration of the control experiment is in agreement with the observed PM10 concentration in May, suggesting that the effects of snow cover and soil moisture on the dust event in May were very small. To improve our ability to forecast Asian dust events in March, the treatment of the hydrological cycles of snow in the land surface model and the soil moisture dependence of dust emission flux should be regarded as the key factors.   

50

Dust Studies in DIII-D Tokamak  

Studies of submicron dust using Mie scattering from Nd:YAG lasers and video data of micron to sub-millimeter sized dust on DIII-D tokamak have provided the first data of dust sources and transport during tokamak discharges. During normal operation on DIII-D dust observation rates are low, a few events per discharge or less. The net carbon content of the dust corresponds to a carbon atom density a few orders of magnitude below the core impurity density. Statistical analysis of Mie data collected over months of operation reveal correlation of increased dust rate with increased heating power and impulsive wall loading due to edge localized modes (ELMs) and disruptions. Generation of significant amounts of dust by disruptions is confirmed by the camera data. However, dust production by disruptions alone is insufficient to account for estimated in-vessel dust inventory in DIII-D. After an extended entry vent, thousands of dust particles are observed by cameras in the first 2-3 plasma discharges. Individual particles moving at velocities up to {approx}300 m/s, breakup of larger particles into pieces, and collisions of particles with walls are observed. After {approx}70 discharges, dust levels are reduced to a few events per discharge. In order to calibrate diagnostics and benchmark modeling, milligram amounts of micron-sized carbon dust have been injected into DIII-D discharges, leading to the core carbon density increase by a factor of 2-3. Following injection, dust trajectories in the divertor are mostly in the toroidal direction, consistent with the ion drag force. Dust from the injection is observed in the outboard midplane by a fast framing camera. The observed trajectories and velocities of the dust particles are in qualitative agreement with modeling by the 3D DustT code.

51

The electrostatic environments of Mars and the Moon  

The electrical activity present in the environment near the surfaces of Mars and the moon has very different origins and presents a challenge to manned and robotic planetary exploration missions. Mars is covered with a layer of dust that has been redistributed throughout the entire planet by global dust storms. Dust, levitated by these storms as well as by the frequent dust devils, is expected to be electrostatically charged due to the multiple grain collisions in the dust-laden atmosphere. Dust covering the surface of the moon is expected to be electrostatically charged due to the solar wind, cosmic rays, and the solar radiation itself through the photoelectric effect. Electrostatically charged dust has a large tendency to adhere to surfaces. NASA's Mars exploration rovers have shown that atmospheric dust falling on solar panels can decrease their efficiency to the point of rendering the rover unusable. And as the Apollo missions to the moon showed, lunar dust adhesion can hinder manned and unmanned lunar exploration activities. Taking advantage of the electrical activity on both planetary system bodies, dust removal technologies are now being developed that use electrostatic and dielectrophoretic forces to produce controlled dust motion. This paper presents a short review of the theoretical and semiempirical models that have been developed for the lunar and Martian electrical environments.

52

Calculation guide mining. Calculation guide for the determination of radiation exposure due to environmental radioactivity resulting from mining  

The present ''Calculation Guide Mining'' serves to determine mining-caused radiation exposure of members of the public and of workers. It is applicable for the use, decommissioning, remediation, and reuse of mining plants and installations as well as for the use, remediation, and reuse of land contaminated as a result of mining plants and installations. The ''Calculation Guide Mining'' describes procedures and parameters to determine effective dose indoors, at underground workplaces, and outdoors, as well as for consumption of breast milk and locally produced foodstuff. The following exposure pathways are considered: external exposure due to gamma-radiation from the soil, exposure due to inhalation of dust, exposure due to inhalation of radon and its short-lived decay products, exposure from ingestion of breast milk and locally produced foodstuff (drinking water, fish, milk and milk products, meat and meat products, leafy vegetables, other vegetable products), and exposure due to direct soil ingestion. In order to account for the natural level of environmental radioactivity involved in measurements, the ''Calculation Guide Mining'' includes levels of natural background for all relevant environmental media. (orig.)

53

Spinning Dust Emission from Wobbling Grains: Important Physical Effects and Implications  

We review major progress on the modeling of electric dipole emission from rapidly spinning tiny dust grains, including polycyclic aromatic hydrocarbons (PAHs). We begin by summarizing the original model of spinning dust proposed by Draine and Lazarian and recent theoretical results improving the Draine and Lazarian model. The review is focused on important physical effects that were disregarded in earlier studies for the sake of simplicity and recently accounted for by us, including grain wobbling due to internal relaxation, impulsive excitation by single-ion collisions, the triaxiality of grain shape, charge fluctuations, and the turbulent nature of astrophysical environments. Implications of the spinning dust emission for constraining physical properties of tiny dust grains and environment conditions are discussed. We discuss the alignment of tiny dust grains and possibility of polarized spinning dust emission. Suggestions for constraining the alignment of tiny grains and polarization of spinning dust emiss...

54

Detection of Interstellar Dust with STEREO/WAVES at 1 AU  

Most in situ measurements of cosmic dust have been carried out with dedicated dust instruments. However, dust particles can also be detected with radio and plasma wave instruments. The high velocity impact of a dust particle generates a small crater on the spacecraft, and the dust particle and the crater material are vaporised and partly ionised. The resulting electric charge can be detected with plasma instruments designed to measure electric waves. Since 2007 the STEREO/WAVES instrument has recorded a large number of events due to dust impacts. Here we will concentrate on the study of those impacts produced by dust grains originating from the local interstellar cloud. We present these fluxes during five years of the STEREO mission. Based on model calculations, we determine the direction ...

55

Diffuse UV Background: GALEX Results  

A bright UV GALEX image in the direction of a dense high galactic latitude interstellar dust cloud is examined to test (and to reject) the idea that a bright extragalactic UV background radiation field exists. A GALEX "Deep Imaging Survey" image of a second high latitude region (a region almost totally free of dust) shows a similar bright background, which, clearly, cannot be due to starlight scattered from interstellar dust. I speculate that the background is due to dark matter particles interacting with interstellar gas/dust nucleons.

56

Density currents as a desert dust mobilization mechanism  

The formation and propagation of density currents are well studied processes in fluid dynamics with many applications to other science fields. In the atmosphere, density currents are usually meso-?/? mechanisms and are often associated with storm downdrafts. These storms are responsible for the formation of severe dust episodes (haboobs) over desert areas. In the present study, the formation of a convective cool pool and the associated dust mobilization is examined for a representative event over the western part of Sahara desert. The physical processes involved in the mobilization of dust are described in the framework of the integrated atmospheric-air quality RAMS/ICLAMS model. Dust is effectively produced due to the development of near surface vortices and increased turbulence mixing along the frontal line. Increased dust emissions and recirculation of the elevated particles inside the density current head result in the formation of a moving "dust wall". Transport of the uplifted dust in higher layers - outside of the density current - occurs mainly in three ways: (1) uplifting of preexisting dust over the frontal line with the aid of the strong updraft (2) entrainment at the upper part of the density current head due to turbulent mixing (3) vertical mixing after the dilution of the system. The role of the produced dust in the associated convective cloud system was found to be limited. Proper representation of convective processes and dust fluxes requires the use of high resolution (cloud resolving) model configuration and online parameterization of dust production. Haboob-type of dust storms are effective dust sources and should be treated accordingly in dust modeling applications.

57

DETECTION OF LOSSES IN PRODUCTION OF THE VALUABLE ELEMENT RHENIUM. AN EXAMPLE FOR THE APPLICATION OF RADIOISOTOPES IN METALLURGY  

The production of Re from Pb--Zn flue dust is investigated during individual processing steps using the radioactive isotopes Re/sup 186/ and Re/sup 188/. The steps investigated includei leaching of filter oxides, thickening by evaporation, removal of Cd by cementation, precipitation of Re as sulfide, and roasting of sulfide to determine metal losses during production. (Rev. Metal Lit. 18: No. 9)

58

Soil fixative study progress report aerial application test:  

A soil fixative has been developed (a simple wheat flour paste mixture) and tested in the laboratory that appears suitable for the temporary fixation of radioactive dusts in case of an accidental spill. A limited field test was made and the feasibility of aircraft delivery examined. A videotape was made of the operations. 3 figs.

59

Monthly results of measurements. January 1996; Tableaux mensuels des mesures. Janvier 1996  

This report of the OPRI (Office of Protection against Ionizing Radiations) exposes the principal results concerning the routine monitoring of environmental radioactivity in France: atmospheric dusts, rainwater, surface water, underground water, sewage water, drinking water, food chain (milk, vegetables, fishes), sea water around nuclear sites and other sites. The activities of various radioisotopes are presented in tables.

60

Dust Model Intercomparison Between ADAM and CFORS/Dust For Asian Dust Case in 2007 (March 28 - April 3)  

As one of research activities of the Joint Research on Dust and Sand Storms (DSS) among China, Korea and Japan, intercomparison between two operational dust forecasting models (ADAM and CFORS/Dust) has been conducted using the selected DSS case which occurred in 2007. The results of simulations by both models were compared with various observations such as surface PM10, Aerosol Optical Thickness, and dust extinction coefficient. In general, both models produced similar results and the predicted values matched well with the observations, despite differences in emission treatment, the adoption of data assimilation technique, and meteorological inputs. However, a large difference (up to 4 times) in modeled surface PM10 concentrations between the models was observed at sites located in source or near-source regions. For the selected case, the dust emission amount calculated by ADAM was larger than that by CFORS/Dust. The vertical structure of dust layer from the models was different due to the characteristics of meteorological inputs used for each model. This study suggests that the construction of more accurate dust source allocation scheme, comprehensive dust emission treatment, improved meteorological inputs and the development of dust data assimilation technique with various dust observations are required for building a more accurate early-warning system of DSS in East Asia.   

 
 
 
 
61

Hot-surface ignition temperatures of dust layers  

Minimum dust layer ignition temperatures on a hot surface were determined for several dusts, using a test procedure recommended by the National Academy of Sciences. The dusts included coal, three oil shales, lycopodium spores, corn starch, grain and brass powder. For a few of the dusts the effects of particle size and layer thickness on the minimum ignition temperatures were examined. Test results were repeatable and reliable for the fuels, the lycopodium and the brass powder. The minimum hot-surface ignition temperatures of 12.7-mm thick layers of these dusts ranged from 160 degrees C for brass to 290 degrees C for 20-gal ton{sup -}{sup 1} oil shale. Flaming combustion was observed only with the brass powder. The minimum ignition temperatures decreased with thicker layers and with smaller particle sizes. Some difficulties were encountered with the corn starch and grain dusts. During heating, the starch charred and expanded; the grain dust swelled and distorted. The test was found acceptable for the purpose of determining the minimum layer ignition temperature of a variety of dusts. To prevent fire hazards due to smoldering of flaming dust layers the temperatures of surfaces on which combustible dusts accumulate should be lower than the minimum hot-surface ignition temperatures of the dusts. 9 figs., 6 tabs.

62

Desert dust deposition reduces snow cover in Colorado Mountains  

Dust deposition on the mountains of southwest Colorado may have reduced springtime snow cover by 1–2 months per year compared to low-dust conditions, a new study finds. When dust is deposited on snow surface, it increases absorption of solar radiation, accelerating snowmelt. Increasing land disturbances, beginning since the early settlers arrived in the western United States during the mid-1800s, have kicked large quantities of dust into the atmosphere; this dust gets deposited on the snow-covered mountains of Colorado. Skiles et al. used 6 years of observations, between 2005 and 2010, to understand how soil dust loading has affected snow cover on the San Juan Mountains of southwest Colorado during the springtime snow-melting season. The authors found that dust loading, which varied by an order of magnitude over the study period, was not necessarily related to the number of seasonal dust events. The increased dust load reduced snow cover by 25–51 days during spring, with the magnitude of impact being directly related to the amount of dust loading. The authors further suggest that the thinning of snow cover due to dust is greater than that expected from the projected 2°C–4°C increase in regional temperature.

63

Building-related symptoms and inflammatory potency of dust from office buildings.  

The aim was to investigate the association between building-related symptoms (BRS) in office buildings and the inflammatory potency of dust (PD). Furthermore, the association between dust potency and various building characteristics was investigated. Occupants of 22 office buildings received a retrospective questionnaire about BRS (2301 respondents). Dust was collected from groups of offices and building characteristics were recorded. The potency of a dust sample to induce interleukin-8 (IL-8) secretion from the lung epithelial cell line A549 was measured as the slope of the initial linear part of the concentration-response curve. Symptoms of the central nervous system (CNS) were associated with the potency of surface dust (OR = 1.4). This association may be due to an association between an index of CNS symptoms and dust potency in offices of 1-6 occupants (OR = 1.5). No single symptoms correlated with the potency of surface dust. The PD was not related to single building factors. The inflammatory PD may be used as an integrated proxy measure of biologically active compounds in dust, reflecting health relevant properties of the dust. PRACTICAL IMPLICATIONS: The potency of surface dust may be used as a crude measurement of the chemical and biological exposures present in the building, and being associated with the development of central nervous system symptoms. However, additional research is needed to establish the predictive value of the potency of surface dust. PMID:18045270

64

Hazardous Waste Treatment Facility and skid-mounted treatment systems at Los Alamos  

To centralize treatment, storage, and areas for hazardous wastes, Los Alamos National Laboratory has designed a 1115 m2 hazardous waste treatment facility. The facility will house a treatment room for each of four kinds of wastes: nonradioactive characteristic wastes, nonradioactive listed wastes, radioactive characteristic wastes, and radioactive listed wastes. The facility will be used for repacking labpacks; bulking small organic waste volumes; processing scintillation vials; treating reactives such as lithium hydride and pyrophoric uranium; treating contaminated solids such as barium sand; treating plating wastes and other solutions with heavy metals and oxidizing organics: Separate treatment rooms will allow workers to avoid mixing waste types and prevent cross-contamination. The ventilation air from the treatment areas may contain hazardous or radioactive dust. Gas may also leak from process equipment. The gas treatment process includes separating solids and gases and neutralization or adsorption of the hazardous gases. The ventilation air from each room will first be filtered before being scrubbed in a common gas caustic scrubber on an outside pad. There are two levels of exhaust in each treatment room, one for heavy gases and another for light gases. Several features help mitigate or eliminate hazards due to spills and releases: each treatment room is sealed and under slight negative pressure; each room has its own HEPA filtration; to avoid mixing of incompatible wastes and reagents, portable individual spill-containment trays are used for skids, to limit the danger of spills, the waste is directly transferred from outside storage to the treatment room; to mitigate the consequences of a gas release in the room, mobile hoods are connected to the exhaust-air treatment system; the floor, walls, ceilings, fixtures, ducts, and piping are made of acid-resistant material or are coated.

65

Survey monitoring of environmental radioactivity in Busan area  

At Regional Radioactivity Monitoring Station in Busan have been measured periodically in 2002 gross beta activities in the airborne dust, fallout, precipitation and tap water and gamma exposure rates. Gamma nuclides in airborne dust, fallout and precipitation have also been monitored at the station. As a part of environmental radiation/radioactivity distribution survey around Pusan foodstuffs, dust, drinking water (total 24ea) samples were taken from sampling sites which were selected by KINS. We analysis gamma nuclide for all. No significant changes from the previous survey have been found in both beta activities and gamma exposure rates. As the results of analyzing an gamma nuclide concentration in environmental samples in Pusan are fee of radiological contaminants.

66

Use of natural radionuclides to determine the time range of the accidental melting of an orphan radioactive source in a steel recycling plant  

In the rare event that an orphan radioactive source is melted in an Electric Arc Furnace steel recycling plant, the radionuclides present are partitioned in the different products, by-products and waste. As a consequence of an unforeseen melting of a radiocesium source, cesium radioisotopes can be found in the dust, together with many natural radionuclides from the decay of radon and thoron, which are present in the atmosphere, picked up from the off-gas evacuation system and associated with the dust of the air filtration system (''baghouse''). In this work we verified that the activity concentration of ^2^1^2Pb in this dust is essentially constant in a specific factory so that it is possible to use it to date back to the time of the accidental melting of the orphan radioactive source. The...

67

Revisiting the radiative impact of dust on Mars using the LMD Global Climate Model  

Airborne dust is the main driver of Martian atmospheric temperature, and accurately accounting for its radiative effect in Global Climate Models (GCMs) is essential. This requires the modeling of the dust distribution and radiative properties, and when trying to simulate the true climate variability, the use of the observed dust column opacity to guide the model. A recurrent problem has been the inability of Mars GCMs to predict realistic temperatures while using both the observed dust radiative properties and column opacity. One would have to drive the model with a tuned opacity to reach an agreement with the observations, thereby losing its self-consistency. In this paper, we show that using the most recently derived dust radiative properties in the LMD (Laboratoire de Météorologie Dynamique) GCM solves this problem, which was mainly due to the underestimation of the dust single scattering albedo in the solar domain. However, an overall warm temperature bias remains above the 1 hPa pressure level. We therefore refine the model by implementing a “semi-interactive” dust transport scheme which is coupled to the radiative transfer calculations. This scheme allows a better representation of the dust layer depth in the model and thereby removes the remaining warm bias. The LMD/GCM is now able to predict accurate temperatures without any tuning of the dust opacity used to guide the model. Remaining discrepancies are discussed, and seem to be primarily due to the neglect of the radiative effect of water-ice clouds, and secondarily to persisting uncertainties in the dust spatial distribution.

68

Biological hazard issues from potential releases of tritiated dust from ITER  

Tritiated dust will be generated during the operation of ITER. Several dedicated studies, involving in vitro and in vivo experiments on metal tritide and carbon tritide dust, have raised some concerns about the protection guidelines for workers exposed to tritiated dust, because they are based on the radiotoxicity of tritium in form of tritium gas (HT), tritiated water (HTO) or organically bound tritium (OBT). While the behaviour of HT, HTO and OBT in the human body is well understood, the same is not fully true for tritiated dust, because of the size distributions of the particles and the variety of base materials. The in vivo and in vitro studies on tritiated dust have shown the dependence of the tritium clearance and retention in the human body on the physico-chemical parameters (mainly the particle size and density). Some recent studies on JET dust relative to graphite and CFC dust have dealt with physico-chemical characterisation and with in vitro tritium dissolution studies. Some uncertainties still remain and further testing is necessary (in vitro and in vivo), restricting if possible the investigation to relevant parameters. In the working areas of ITER the radioactive dust concentration in air will be kept at a very low level. However, in the event of an accident, the atmosphere inside the buildings, including operative areas as well, might get contaminated with small amounts of tritiated dust and hence inhalation risks cannot be excluded. The present paper summarizes the results from previous investigations on the subject which are relevant in deriving sound dose conversion factors for tritiated dust. At the same time, it proposes a dose conversion factor for dust which is conservative in order to envelope all ITER relevant materials.

69

Direct observations of the atmospheric processing of Asian mineral dust  

The accumulation of secondary acids and ammonium on individual mineral dust particles during ACE-Asia has been measured with an online single-particle mass spectrometer, the ATOFMS. Changes in the amounts of sulphate, nitrate, and chloride mixed with dust particles correlate with air masses from different source regions. The uptake of secondary acids depended on the individual dust particle mineralogy; high amounts of nitrate accumulated on calcium-rich dust while high amounts of sulphate accumulated on aluminosilicate-rich dust. Oxidation of S(IV) to S(VI) by iron in the aluminosilicate dust is a possible explanation for this enrichment of sulphate, which has important consequences for the fertilization of remote oceans by soluble iron. This study shows the segregation of sulphate from nitrate and chloride in individual aged dust particles for the first time. A transport and aging timeline provides an explanation for the observed segregation. Our data suggests that sulphate became mixed with the dust first. This implies that the transport pathway is more important than the reaction kinetics in determining which species accumulate on mineral dust. Early in the study, dust particles in volcanically influenced air masses were mixed predominately with sulphate. Dust mixed with chloride then dominated over sulphate and nitrate when a major dust front reached the R. V. Ronald Brown. We hypothesize that the rapid increase in chloride on dust was due to mixing with HCl(g) released from acidified sea salt particles induced by heterogeneous reaction with volcanic SO2(g), prior to the arrival of the dust front. The amount of ammonium mixed with dust correlated strongly with the total amount of secondary acid reaction products in the dust. Submicron dust and ammonium sulphate were internally mixed, contrary to frequent reports that they exist as external mixtures. The size distribution of the mixing state of dust with these secondary species validates previous mechanisms of the atmospheric processing of dust and generally agrees with simulated aerosol chemistry from the STEM-2K3 model. This series of novel results has important implications for improving the treatment of dust in global chemistry models and highlights a number of key processes that merit further investigation through laboratory and field studies.

70

Survey monitoring of environmental radioactivity in Jeju area  

The project is carried out to monitor the change of environmental radioactivity in Jeju, and to provide a systematic data for radiation monitoring and counter measurement at a radiological emergency situation. Also the survey of natural environmental radioactivities in the samples was conducted to make the reliable data base for evaluation of internal exposure and environmental contamination of radiation. This report contains the data of gamma exposure rates and radioactivities of airborne dust, fallout, precipitation and tap water which were analyzed periodically by Jeju Regional Monitoring Station in 2000. Also it contains the data of natural radioactivity levels of food stuff such as agricultural and marine products, including drinking waters. There was no significant difference in environmental radioactivities between 1999 and 2000.

71

Effect of Simulant Type on the Absorptance and Emittance of Dusted Thermal Control Surfaces in a Simulated Lunar Environment  

During the Apollo program the effects of lunar dust on thermal control surfaces was found to be more significant than anticipated, with several systems overheating due to deposition of dust on them. In an effort to reduce risk to future missions, a series of tests has been initiated to characterize the effects of dust on these surfaces, and then to develop technologies to mitigate that risk. Given the variations in albedo across the lunar surface, one variable that may be important is the darkness of the lunar dust, and this study was undertaken to address that concern. Three thermal control surfaces, AZ-93 white paint and AgFEP and AlFEP second surface mirrors were dusted with three different lunar dust simulants in a simulated lunar environment, and their solar absorptivity and thermal emissivity values determined experimentally. The three simulants included JSC 1AF, a darker mare simulant, NU-LHT-1D, a light highlands simulant, and 1:1 mixture of the two. The response of AZ-93 was found to be slightly more pronounced than that of AgFEP. The increased with fractional dust coverage in both types of samples by a factor of 1.7 to 3.3, depending on the type of thermal control surface and the type of dust. The of the AZ-93 decreased by about 10 percent when fully covered by dust, while that of AgFEP increased by about 10 percent. It was found that alpha/epsilon varied by more than a factor of two depending on the thermal control surface and the darkness of the dust. Given that the darkest simulant used in this study may be significantly lighter than the darkest dust that could be encountered on the lunar surface, it becomes apparent that the performance degradation of thermal control surfaces due to dust on the moon will be strongly dependent on the and of the dust in the specific locality.

72

Physical setting and natural sources of exposure to carcinogenic trace elements and radionuclides in Lahontan Valley, Nevada  

In Lahontan Valley, Nevada, arsenic, cobalt, tungsten, uranium, radon, and polonium-210 are carcinogens that occur naturally in sediments and groundwater. Arsenic and cobalt are principally derived from erosion of volcanic rocks in the local mountains and tungsten and uranium are derived from erosion of granitic rocks in headwater reaches of the Carson River. Radon and ^2^1^0Po originate from radioactive decay of uranium in the sediments. Arsenic, aluminum, cobalt, iron, and manganese concentrations in household dust suggest it is derived from the local soils. Excess zinc and chromium in the dust are probably derived from the vacuum cleaner used to collect the dust, or household sources such as the furnace. Some samples have more than 5 times more cobalt in the dust than in the local soil,...

73

Report of radioactivity survey research in fiscal year 1997  

In National Institute of Radiological Sciences, a survey was made on radioactivities in the environment due to the substances released from nuclear installations and radioactive fall-out brought out by nuclear explosion tests since 1959. As the marked progress of non-military utilization of nuclear energy the national concern on environmental radioactivity has been increasing in Japan and thus it has become more and more important to make a survey research of radioactivities, which might affect the environment and human health. In these situations, the institute attempted to make the following six surveys in the fiscal year of 1997; `a survey on radioactive levels in environment, foods and human bodies`, `survey on the radioactive level in the regions around nuclear installations`, `works in radioactive data center`, `fundamental survey on the evaluation of the results from radioactivity survey`, `workshop for technical experts of environmental radioactivity monitoring` and `survey research on the measurement and countermeasures for emergency exposure`. (J.P.N.)

74

Black hole formation from collapsing dust fluid in a background of dark energy  

The gravitational collapse of a spherically symmetric star, made of a dust fluid, ?DM, in a background of dark energy, p=w? (wblack holes are never formed. When both of them are present, black holes can be formed, due to the condensation of the dust fluid. Initially the dust fluid may not play an important role, but, as time increases, it will dominate the collapse and finally lead to formation of black holes. This result remains true even when the interaction between the dust fluid and dark energy does not vanish. When wblack hole.

75

Validation of a Lagrangian dust transport model with data from the Fennec/LADUNEX field campaign  

Mineral dust aerosol is a key player in the Earth system. Strong winds over the world's major deserts mobilise and subsequently lift mineral dust high into the atmosphere. Due to the harshness and inaccessibility of desert regions, the exact processes of mobilisation and lifting, and layer formation are still unclear. One major unknown in the dust cycle is the dust source or emission strength. Despite better quantification being key for global models, the assessment of impacts on clouds, radiation and biogeochemical cycles, estimates in the literature from global and regional models span a wide range. Here, we validate the state-of-the-art Lagrangian particle dispersion model FLEXPART, which has been made capable of simulating dust mobilisation and settling, with airborne and ground-based mineral aerosol and turbulence measurements from the Fennec/LADUNEX field campaign, which was carried out over the western Sahara during June 2011. For a selected case study we compare in-situ and remote-sensing data from an aircraft and the CALIOP LIDAR observations with FLEXPART dust transport simulations. The reliability of ECMWF analysis data in the vicinity of a convectively-generated dust plume is assessed using a set of model simulations, in which dust emissions are prescribed manually from SEVIRI satellite images. Dust emission associated with deep moist convection has been recently identified as a key problem. Overall, this research underlines the potential of jointly using measurements and observations from many data sources with models to better understand dust emission processes in the Sahara desert, and to limit model uncertainty.

76

Cost efficient alternative to stone dust for suppressing coal dust explosions  

Stone dust has long been used as an incombustible material spread over the walls and floor of coal mines to act as a heat shield and to arrest a propagating coal dust explosion. Recent research has shown that legislative requirements for incombustible material in the practice of stone dusting to suppress potential coal dust explosions have been too low. Recent changes to the Queensland Coal Mining Safety and Health Regulations have increased these levels to reflect results of this research. The use of rock phosphate as an alternative to stone dust is investigated here, as it is readily available by virtue of the fact that the fertilizer industry currently imports it from worldwide sources. The recent development of the Phosphate Hill deposit near Mt Isa by QMC also makes the use of this material attractive. Various forms of rock phosphate were tested against stone dust with regard to their ability to inert coal dust explosions. In all cases the rock phosphate showed no appreciable advantage in inerting ability. The cost of using such an alternative would appear to be 50% greater. Ammonium phosphate, which is a processed form of rock phosphate, did show a significant advantage in inerting level, when compared to stone dust, with only one third of the amount of inert material required for full inerting of a coal dust explosion. This material however is not suitable for general stone dusting due to its increased solubility in water. It could be used in bag barriers which are protected from moisture.

77

Contribution of shield movement to airborne dust levels in longwall faces  

Dust control in high-production longwalls requires attention to operating practices and ventilation schemes. Several studies have shown that the shearer is the major source of dust on a longwall face. Support movement has not been regarded as a major source of dust in US longwalls. Yet, under certain conditions, 31% of the shearer operator`s dust exposure can be due to support movement. Several methods have been developed for the control of shield-generated dust. But the need for better methods is apparent. In this paper, the amount of airborne, respirable dust generated per shield move is estimated from specially designed experiments on longwall faces. Ten experiments were conducted on five longwall faces in four mines. Each experiment involved one face visit and lasted three to six hours. The contribution of shield movement to the airborne, respirable dust concentration immediately downwind of the shield move varied between 0.12 and 1.75 mg/m{sup 3} in the five longwall faces. The mass of airborne, respirable dust generated by shield movement was found to vary between 39 and 386 mg per shield move. The results from this study reveal that control of dust from longwall shields requires a combination of approaches involving alternative operating practices, reducing shield dust generation rate, increasing face air flow and decreasing personnel exposure. 14 refs., 5 figs., 2 tabs.

78

Dust-Tolerant Intelligent Electrical Connection System  

Faults in wiring systems are a serious concern for the aerospace and aeronautic (commercial, military, and civilian) industries. Circuit failures and vehicle accidents have occurred and have been attributed to faulty wiring created by open and/or short circuits. Often, such circuit failures occur due to vibration during vehicle launch or operation. Therefore, developing non-intrusive fault-tolerant techniques is necessary to detect circuit faults and automatically route signals through alternate recovery paths while the vehicle or lunar surface systems equipment is in operation. Electrical connector concepts combining dust mitigation strategies and cable diagnostic technologies have significant application for lunar and Martian surface systems, as well as for dusty terrestrial applications. The dust-tolerant intelligent electrical connection system has several novel concepts and unique features. It combines intelligent cable diagnostics (health monitoring) and automatic circuit routing capabilities into a dust-tolerant electrical umbilical. It retrofits a clamshell protective dust cover to an existing connector for reduced gravity operation, and features a universal connector housing with three styles of dust protection: inverted cap, rotating cap, and clamshell. It uses a self-healing membrane as a dust barrier for electrical connectors where required, while also combining lotus leaf technology for applications where a dust-resistant coating providing low surface tension is needed to mitigate Van der Waals forces, thereby disallowing dust particle adhesion to connector surfaces. It also permits using a ruggedized iris mechanism with an embedded electrodynamic dust shield as a dust barrier for electrical connectors where required.

79

Two-fluid Instability of Dust and Gas in the Dust Layer of a Protoplanetary Disk  

Instabilities of the dust layer in a protoplanetary disk are investigated. It is known that the streaming instability develops and dust density concentration occurs in a situation where the initial dust density is uniform. This work considers the effect of initial dust density gradient vertical to the midplane. Dust and gas are treated as different fluids. Pressure of dust fluid is assumed to be zero. The gas friction time is assumed to be constant. Axisymmetric two-dimensional numerical simulation was performed using the spectral method. We found that an instability develops with a growth rate on the order of the Keplerian angular velocity even if the gas friction time multiplied by the Keplerian angular velocity is as small as 0.001. This instability is powered by two sources: (1) the vertical shear of the azimuthal velocity, and (2) the relative motion of dust and gas coupled with the dust density fluctuation due to advection. This instability diffuses dust by turbulent advection and the maximum dust densi...

80

Characterisation of Manganese Furnace Dust and Zinc Balance in Production of Manganese Alloys  

Manganese furnace dust is made up of volatiles and raw materials fines collected from the off-gas during smelting of manganese alloys. Currently, manganese furnace dust is accumulated in large settling ponds. Major factors preventing recycling of the manganese furnace dust to the ferroalloy furnaces are handling, due to its tar content, and accumulation of zinc in the furnaces, which can cause irregularities in their operation. This paper presents characteristics of manganese furnace dust generated in ferromanganese and silicomanganese production at Tasmanian Electrometallurgical Company and analyses zinc balances in light of furnace dust recycling. If manganese furnace dust is recycled to the ferroalloy furnaces via the sinter plant, the overall zinc input will increase by 51-143 % depending on charging materials.   

 
 
 
 
81

Herschel photometric observations of the nearby low metallicity irregular galaxy NGC 6822  

We present the first Herschel PACS and SPIRE images of the low-metallicity galaxy NGC6822 observed from 70 to 500 mu and clearly resolve the HII regions with PACS and SPIRE. We find that the ratio 250/500 is dependent on the 24 mu surface brightness in NGC6822, which would locally link the heating processes of the coldest phases of dust in the ISM to the star formation activity. We model the SEDs of some regions HII regions and less active regions across the galaxy and find that the SEDs of HII regions show warmer ranges of dust temperatures. We derive very high dust masses when graphite is used in our model to describe carbon dust. Using amorphous carbon, instead, requires less dust mass to account for submm emission due to its lower emissivity properties. This indicates that SED models including Herschel constraints may require different dust properties than commonly used.

82

Charge Variation Effects on Low-Frequency Electrostatic Waves in Dusty Plasmas  

A general formula for the dispersion characteristics of electrostatic waves in dusty plasmas in the presence of charge fluctuation of dust particles is derived based on the linear response theory. The formula is applicable to arbitrary plasma models and waves. Charging equation due to plasma current on the dust surface is employed to describe the charge fluctuation effect. In particular, temperature fluctuation associated with the space charge fluctuation is taken into account in the charging equation and is found to make an important contribution to the damping or growth of the wave. Stability of low frequency waves where the electron response can be treated as static is discussed in detail. It is shown that the dust charge fluctuation contributes to damping when the dust is negatively charged, but to growth when the dust is positively charged. Results are applied to ion waves with positive dust charge.   

83

Impurity Seeding with Dust Injection in Tokamak Edge Plasmas  

Abstract Impurity seeding of tokamak edge plasmas in the form of dust is modeled using the recently coupled DUSTT/UEDGE code. The effects on edge plasma performance due to lithium and carbon dust continuously injected at different poloidal locations in NSTX and ITER are modeled. Modeling demonstrates that dust injection into the edge plasma with rates of the order of several 10 mg s-1 for NSTX and 1 g s-1 for ITER can significantly increase radiation power losses leading to substantial reduction of the divertor heat load. The impact of different rates of dust injection on plasma operation and stability is discussed. The simulated edge plasma performance with injected dust is compared with the case of injection of an equivalent amount of dust material in the form of atomic vapor. It is show...

84

Characterization of stockpiled phosphogypsum in Brazil and evaluation of its environmental impact  

Phosphogypsum, a waste by-product derived from the wet process production of phosphoric acid, represents a serious problem facing the phosphate industry in Brazil. This by-product (mainly calcium sulphate dihydrate) precipitates during the reaction of sulphuric acid with phosphate rock and is stored at a rate of about 2,500 ton per day on several stacks in Cubat, Brazil. Contents of natural radionuclides from thorium and uranium series were measured in Brazilian phosphogypsum samples from stacks, using high-resolution gamma spectrometry. As a complementary study, trace and microelements (Ba, Co, Cr, Fe, Hf, Sb, Sc, Ta, Th, U, and rare earths Ce, Eu, La, Lu, Nd, Sm, Tb and Yb) were also determined by instrumental neutron activation analysis (INAA). This phosphogypsum stacks present a potential threat to the surrounding environment and to the individual occupationally exposed. The most critical pathway between phosphogypsum and the public is through water contamination. The aquatic environment near the disposal area was assessed by measuring natural radionuclides activity in groundwater, river water and sediment samples. As for the individual occupationally exposed, the pathways considered were internal exposure due to inhalation of radon emanated from phosphogypsum stacks and inhalation of dust particulates, and external gamma and beta exposures due to immersion in the radioactive plume. The results obtained in this study show that radionuclides, although present in relatively high concentrations in phosphogypsum, do not imply in significant doses for individuals occupationally exposed and for the general public. (author)

85

A simple model for the evolution of the dust population in protoplanetary disks  

Context. The global size and spatial distribution of dust is an important ingredient in the structure and evolution of protoplanetary disks and in the formation of larger bodies, such as planetesimals. Aims: We aim to derive simple equations that explain the global evolution of the dust surface density profile and the upper limit of the grain size distribution and which can readily be used for further modeling or for interpreting of observational data. Methods: We have developed a simple model that follows the upper end of the dust size distribution and the evolution of the dust surface density profile. This model is calibrated with state-of-the-art simulations of dust evolution, which treat dust growth, fragmentation, and transport in viscously evolving gas disks. Results: We find very good agreement between the full dust-evolution code and the toy model presented in this paper. We derive analytical profiles that describe the dust-to-gas ratios and the dust surface density profiles well in protoplanetary disks, as well as the radial flux by solid material "rain out", which is crucial for triggering any gravity assisted formation of planetesimals. We show that fragmentation is the dominating effect in the inner regions of the disk leading to a dust surface density exponent of -1.5, while the outer regions at later times can become drift-dominated, yielding a dust surface density exponent of -0.75. Our results show that radial drift is not efficient in fragmenting dust grains. This supports the theory that small dust grains are resupplied by fragmentation due to the turbulent state of the disk.

86

Releases of radioactivity from uranium mills and effluent treatment costs. [Stabilization of uranium mill tailings  

Airborne releases of radioactive materials from uranium milling to the environment consist of ore dust, yellowcake dust, tailings dust, and radon gas while the mill is active. After a mill has ceased operations, tailings may be stabilized to minimize or prevent airborne releases of radioactive particulates. However, radon gas will continue to be released in amounts inversely proportional to the degree of stabilization treatment (and expense). Liquid waste disposal is by evaporation and natural seepage to the ground beneath the tailings impoundment area. The release of radioactive materials (and potential radiation exposures) determines the majority of costs associated with minimizing the environmental impact of uranium milling. Radwaste treatments to reduce estimated radiation doses to individuals to 3 to 5% of those received with current milling practices are equivalent to $0.66 per pounds of U/sub 3/O/sub 8/ and 0.032 mill per kWhr of electricity. This cost would cover a high efficiency reverse jet bag filter and high energy venturi scrubbers for dusts, neutralization of liquids, and an asphalt-lined tailings basin with a clay core dam to reduce seepage. In addition, this increased cost would cover stabilization of tailings, after mill closure, with a 1-in. asphalt membrane topped by 2 ft of earth and 0.5 ft of crushed rock to provide protection against future leaching and wind erosion. The cost of reducing the radiological hazards associated with uranium milling to this degree would contribute about 0.4% to the current total cost of nuclear power.

87

Observed 20th Century Desert Dust Variability: Impact on Climate and Biogeochemistry  

Desert dust perturbs climate by directly and indirectly interacting with incoming solar and outgoing long wave radiation, thereby changing precipitation and temperature, in addition to modifying ocean and land biogeochemistry. While we know that desert dust is sensitive to perturbations in climate and human land use, previous studies have been unable to determine whether humans were increasing or decreasing desert dust in the global average. Here we present observational estimates of desert dust based on paleodata proxies showing a doubling of desert dust during the 20th century over much, but not all the globe. Large uncertainties remain in estimates of desert dust variability over 20th century due to limited data. Using these observational estimates of desert dust change in combination with ocean, atmosphere and land models, we calculate the net radiative effect of these observed changes (top of atmosphere) over the 20th century to be -0.14 {+-} 0.11 W/m{sup 2} (1990-1999 vs. 1905-1914). The estimated radiative change due to dust is especially strong between the heavily loaded 1980-1989 and the less heavily loaded 1955-1964 time periods (-0.57 {+-} 0.46 W/m{sup 2}), which model simulations suggest may have reduced the rate of temperature increase between these time periods by 0.11 C. Model simulations also indicate strong regional shifts in precipitation and temperature from desert dust changes, causing 6 ppm (12 PgC) reduction in model carbon uptake by the terrestrial biosphere over the 20th century. Desert dust carries iron, an important micronutrient for ocean biogeochemistry that can modulate ocean carbon storage; here we show that dust deposition trends increase ocean productivity by an estimated 6% over the 20th century, drawing down an additional 4 ppm (8 PgC) of carbon dioxide into the oceans. Thus, perturbations to desert dust over the 20th century inferred from observations are potentially important for climate and biogeochemistry, and our understanding of these changes and their impacts should continue to be refined.

88

Effects of particle shape, hematite content and semi-external mixing with carbonaceous components on the optical properties of accumulation mode mineral dust  

The radiative forcing estimation of the polluted mineral dust is limited due to lack of morphological analysis, mixing state with the carbonaceous components and the hematite content in the pure dust. The accumulation mode mineral dust has been found to mix with anthropogenically produced black carbon, organic carbon and brown carbon during long range transport. The above features of the polluted dust are not well accounted in the optical models and lead the uncertainty in the numerical estimation of their radiative impact. The Semi-external mixing being a prominent mixing of dust and carbonaceous components has not been studied in details so for compared to core-shell, internal and external mixing studies. In present study, we consider the pure mineral dust composed of non-metallic components (such as Quartz, Feldspar, Mica and Calcite) and metalic component like hematite (Fe2O3). The hematite percentage in the pure mineral dust governs its absorbance. Based on this hematite variation, the hematite fraction in pure mineral dust has been constrained between 0-8%. The morphological and mineralogical characterization of the polluted dust led to consider the three sphere, two sphere and two spheroid model shapes for polluted dust particle system. The pollution gives rise to various light absorbing aerosol components like black carbon, brown carbon and organic carbon (comprising of HUmic-Like Substances, HULIS) in the atmosphere. The entire above discussed model shapes have been considered for the mineral dust getting polluted with (1) organic carbon (especially HULIS component) (2) Brown carbon and (3) black carbon by making a semi-external mixture with pure mineral dust. The optical properties (like Single Scattering Albedo, SSA; Asymmetry parameter, g and Extinction efficiency, Qext) of above model shapes for the polluted dust have been computed using Discrete Dipole Approximation, DDA code. For above model shapes, the SSA was found to vary depending on hematite content (0-8%) and model shape composition. For the two sphere BC-mineral dust cluster, hematite was found to be dominating absorber compared to that of black carbon as the RBC/Rdust decreases. (i.e. with increase of dust sphere size compared to black carbon sphere in the composite 2-sphere cluster). SSA was found to be very sensitivity for the hematite content when both of the spheres (i.e. mineral dust and BC) are nearly of same size. The two spheroid system composed of organic carbon and dust with 0% hematite (OCD'-0) showed the maximum deviation of SSA (i.e.~5%) compared to the two sphere system of same composition and hematite content (OCD-0 ). Increase in hematite from 0 to 8% caused maximum SSA deviation of ~20% for two sphere organic carbon-dust system (OCD) while the same has been observed to be ~18% for two spheroid organic carbon-dust system (OCD'). SSA was found to be more sensitive to hematite content than that of particle shape. Compared to SSA, Asymmetry parameter, g was found to be more sensitive towards particle shape. For three-sphere model shapes with 0% hematite composed of black carbon-dust-dust (BCDD-0), brown carbon-dust-dust (BrCDD-0 ) and organic carbon-dust-dust (OCDD-0), the deviation of SSA and g relative to conjugate black carbon (BC), brown carbon (BrC) and organic carbon (OC) spheres are ~68% and ~31%, ~83% and ~31% and ~70% and ~33%, respectively. Thus modeled polluted dust optics will provide a better basis for radiative forcing estimation and many sensitivity studies.

89

Effect of liquid radioactive waste discharge on water recipient in the vicinity of Jaslovske Bohunice  

Studies of radioactivity in the water recipient in the vicinity of the nuclear power plant Jaslovske Bohunice showed an increase of radioactivity in the river Dudvah beyond the outlet of the sewer. Since 1978 the radioactivity in the water has been found to decrease. The recorded values represent only fractions of percentages of the permissible volumetric activity of radionuclides. Radioactivity is practically constant along the whole length of the river Dudvah beyond the outlet of the sewer. Increased radioactivity has been observed only in Siladice, due to the high level of /sup 40/K in the waste waters discharged from a food processing factory. The increased radioactivity of the river Dudvah does not affect the radioactivity level in the river Vah where a dilution of more than 1:100 occurs. Drinking waters are not affected by radioactive contamination.

90

Change of the Asian dust source region deduced from the relationship between anthropogenic radionuclides in surface soil and precipitation in Mongolia  

The Asian dust source region may be expanding primarily as a result of recent climate change, especially during the 2000s. This change was investigated by examining anthropogenic radionuclides contained in surface soil samples from Mongolia. Surface soil was globally labeled by radioactive fallout from nuclear testing during the late 1950s and early 1960s. There are no current direct sources for anthropogenic radionuclides in the air, so the radionuclides in the atmosphere are mainly carried by dust from wind-blown surface soil, that is, aeolian dust. Asian dust carries 90Sr, 137Cs, and other anthropogenic radionuclides; the heaviest deposition occurs in spring and has been recorded in Japan since the early 1990s. The composition of anthropogenic radionuclides in atmospheric depositions would be affected by a change in the dust source. Previous studies of atmospheric depositions at long-term monitoring sites (e.g. in Tsukuba, Japan) have detected changes in the 137Cs/90Sr ratio and in the specific activity of the radionuclides. These changes in the composition of observed atmospheric depositions should be a reflection for a change in the climatic conditions of the dust source region. To investigate this dust source change, a field survey for radionuclides (90Sr and 137Cs) in surface soil samples was conducted in September 2007 in the eastern and southern regions of Mongolia, where dust storms have occurred more frequently since 2000. It was found that specific activities of both radionuclides as well as the 137Cs/90Sr ratio in the surface soil correlated well with annual average precipitation in the Mongolian desert-steppe zone. The higher specific activities and the higher 137Cs/90Sr ratio were found in the grassland region with the greater precipitation. This finding suggests that the increased specific activities and the activity ratio detected in the atmospheric depositions in Japan during years of the frequent Asian dust transport event since 2000 should be a sign of grassland degradation.

91

Mineral Dust in Polar Ice Cores as a Paleoclimatic Proxy  

Ice cores from polar regions provide a unique archive for paleo climate since a variety of proxies can be obtained from the same sample. One of these are mineral dust particles eroded from arid areas which have been entrained into the atmosphere, transported over large distances and deposited on the ice caps. Those dust particles are stored in an extremely clean environment. Due to the thickness of the polar ice sheets and an extremely low snow accumulation rate the longest record obtained from Antarctica up to now spans more than 800 000 years (Lambert, 2008), records in Greenland reach up to 120 000 years B.P. (NGRIP- community-members, 2004). On the other hand very high resolution records of seasonal cycles can be obtained up to the last glacial period, which allows studies ranging from annual to glacial-interglacial variability. Dust concentration changes in ice cores mirror changing conditions in the source and during the atmospheric transport of the dust. Measurements of concentration and size at the same time offer the possibility to distinguish between influences by transport and by the source of the dust. The dust provenance can be obtained by comparison of the chemical composition of the ice core dust with that in the potential source areas. An overview of the dust records from Antarctic and Greenland ice cores is presented with emphasis on dust concentration variability on different timescales and studies of provenance and transport changes.

92

Secondary charging effects due to icy dust particle impacts on rocket payloads  

We report measurements of dust currents obtained with a small probe and a larger probe during the flight of the ECOMA-4 rocket through the summer polar mesosphere. The payload included two small dust probes behind a larger dust probe located centrally at the front. For certain phases of the payload rotation, the current registered by one of the small dust probes was up to 2 times the current measured with the larger probe, even though the effective collection area of the larger probe was 4 times that of the small one. We analyze the phase dependence of the currents and their difference with a model based on the assumption that the small probe was hit by charged dust fragments produced in collisions of mesospheric dust with the payload body. Our results confirm earlier findings that secondary charge production in the collision of a noctilucent cloud/Polar Summer Mesospheric Echo (NLC/PMSE) dust particle with the payload body must be several orders of magnitude larger than might be expected from laboratory studies of collisions of pure ice particles with a variety of clean surfaces. An important consequence is that for some payload configurations, one should not assume that the current measured with a detector used to study mesospheric dust is simply proportional to the number density of ambient dust particles. The higher secondary charge production may be due to the NLC/PMSE particles containing multiple meteoric smoke particles.

93

A Study of LYNDS 1251 Dark Cloud : II. Infrared Properties  

We have studied the star forming activities and dust properties of Lynds 1251, a dark cloud located at relatively high galactic latitude. Eleven IRAS point sources identified toward Lynds 1251 are discussed. Estimate of stellar masses, and far-infrared lumnosities of the young stars associated with two prominent IRAS point sources imply that these are T-Tauri stars with masses smaller than 0.3 Mo. The low dust temperature of 27 K and low ratio of FIR emission to hydrogen column density are probably due to the lack of internal heating sources. Presumably two low mass young stars do not have enough energy to heat up the dust and gas associated. The dust heating is dominated by the interstellar heating source, and the weaker interstellar radiation field can explain the exceptionally low dust temperatures found in Lynds 1251. The estimated dust mass of Lynds 1251 is just about 1Mo, or about 1/1000 of gas mass, which implies that there must be a substantial amount of colder dust. The infrared flux at 100 micromis is matching well with 13CO peak temperature, while the 12CO integrated intensity is matching with the boundary of dust emission. Overall, the dust properties of Lynds 1251 is similar to those of normal dark clouds even though it does have star forming activities.

94

Concentration of atmospheric particulates during a dust storm period in central Taiwan, Taichung.  

In this study we monitored concentrations of particles in central Taiwan using PS-1 (GPS1 PUF Sampler) and Model 310 Universal Air Sampler (UAS) from 02/23/2001 to 03/12/2001 at two sampling sites. During this period, an Asian dust storm moved across central Taiwan from 3/3 to 3/6. The total ambient air particle concentrations during the dust storm period were than compared with previous data from this region. In general, the average total suspended particulate (TSP) concentration order was during dust storm period > after dust storm period > non-dust storm period at both HKITT (traffic) and THUC (rural) sampling sites. The ratio of PM2.5/PM10 was 60% before and after the dust storm period. However, this ratio was decreased to less than 50% during the dust storm. This demonstrates that the coarse particulate concentrations (PM2.5-10) increased during the dust storm period. In contrast the increase of ambient air particles concentrations after the Taiwan Chi-Chi Earthquake were mainly due to fine particles (PM2.5). And, the increased of ambient air particles concentrations after dust storm period were mainly coarse particle (PM2.5-10) concentrations in central Taiwan. PMID:11883755

95

Genesis and evolution of dust in galaxies in the early Universe I. Modeling dust evolution in starburst galaxies  

We have developed a numerical galactic chemical evolution model. The model is constructed such that the effect of a wide range of parameters can be investigated. It takes into account results from stellar evolution models, a differentiation between diverse types of core collapse SNe and the contribution of AGB stars in the mass range 3-8 Msun. We consider the lifetime-dependent yield injection into the ISM by all sources as well as dust destruction due to SN shocks in the ISM. We ascertain the temporal progression of the dust mass, the dust-to-gas and dust-to-metal mass ratios as well as other physical properties of a galaxy and study their dependence on the mass of the galaxy, the IMF, dust production efficiencies and dust destruction in the ISM. The amount of dust and the physical properties of a galaxy strongly depend on the initial gas mass available. Overall, while the total amount of dust produced increases with galaxy mass, the detailed outcome depends on the SN dust production efficiency, the IMF and ...

96

A survey of radioactive levels of agricultural products in Saitama prefecture  

Past atmospheric nuclear testing which have been conducted frequently, have caused environmental pollution due to the diffusion of radioactive substances into the atmosphere and from the radioactive fallout. The environmental pollution from nuclear testing into the atmosphere has resulted in the radioactive contamination in agricultural products and has continued for a long time. The radioactive contamination of agricultural products occurs through air, water and soil which were contaminated by radioactive fallout. In this paper, for the purpose of analyzing the extent of the radioactive contamination levels in the agricultural products of Saitama Prefecture, spinach, green soybeans, dried shiitake and welsh onion, were selected among products, as the amount of the harvest is abundant in all of Japan. Radioactivity concentration was investigated by gamma-ray spectrometry and radiochemical analysis. The radioactivity concentrations of artificial radioactive nuclides, cesium-137 ({sup 137}Cs) and strontium-90 ({sup 90}Sr), were detected in the range which is considered to be the result of radioactive fallout. Moreover, in order to examine the effect on radioactivity concentrations in agricultural products by culinary processing, the raw agricultural products were boiled, and their radioactivity concentrations were compared with the raw produce. The radioactivity concentrations in the boiled were lower than those in the raw produce. (author)

97

Survey monitoring of environmental radioactivity in Daegu area  

The objectives of the project are to monitor an abnormal radiation level in Taegu and Kyungpook region, and to enhance our ability to prepare for the radiological emergency situation by establishing the radioactivity monitoring system in Taegu and Kyungpook region. Gross beta activities were measured and gamma radionuclides were analysed for the environmental samples of air-borned dust. precipitation. fallout and drinking water collected in Taegu radioactivity monitoring center. and gamma exposure rates were also measured. To establish the basic data base on the environmental radioactivity, gamma radionuclide analyses were carried out for the samples of soil, drinking water, grain, vegetable, milk, and fish which were obtained from 31 different areas, and the spatial gamma exposure rates from 61 different points were also measured in Taegu and Kyungpook region. In conclusion, it didn't appear any evidence for newly pollution of artificial radioactivity in Taegu and Kyungpook region.

98

A Tour of the MODIS Land Products - ARSET: Air Quality - NASA  

... Volatile organic compounds (VOCs); Nitrogen dioxide (NO2); Sulfur dioxide ( SO2); Particulate matter ... Biomass burning - Forest, grassland, savannah, crops; Dust due to desertification; Volcanoes (SO2). 15 ... Columnar Integrated Loading ...

99

ExMC 4.22: Limited capability to diagnose and treat  

Chronic lifetime risks – Expected to be a result of prolonged exposures to ... and the potential for acute and chronic manifestations of radiation exposure in ..... and treat pulmonary or systemic disease due to non-terrestrial dust exposure ...

100

The Deep Space Network Progress Report 42-39 March and April ...  

Apr 15, 1977 ... A Preliminary Analysis of Viking S-X Doppler Data and. Comparison to ..... degraded due to possible dust clouds in the southern hemi- ..... Bad thermal switch on klystron ...... Fig. 6. PVB and PVS Incrementing data format ...

 
 
 
 
101

Using thermal infrared (TIR) data to characterize dust sources, dust fall and the linkage to climate in the Middle East  

Prior to mineral dust deposition affecting albedo, aerosols can have direct and indirect effects on local to regional scale climate by changing both the shortwave and longwave radiative forcing. In addition, mineral dust causes health hazards, such as respiratory-related illnesses and deaths, loss of agricultural soil, and safety hazards to aviation and motorists due to reduced visibility. Previous work utilized satellite and ground-based TIR data to describe the direct longwave radiative effect of the Saharan Air Layer (SAL) over the Atlantic Ocean originating from dust storms in the Western Sahara. TIR emission spectroscopy was used to identify the spectral absorption features of that dust. The current research focuses on Kuwait and utilizes a comprehensive set of spatial, analytical and geological tools to characterize dust emissions and its radiative effects. Surface mineral composition maps for the Kuwait region were created using ASTER images and GIS datasets in order to identify the possible sources of wind-blown dust. Backward trajectory analysis using the Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) model suggests the dust source areas were located in Iraq, Syria, Jordan and Saudi Arabia. Samples collected from two dust storms (May and July 2010) were analyzed for their mineral composition and to validate the dust source areas identified by the modeling and remote sensing analysis. These air fall dust samples were collected in glass containers on a 13 meter high rooftop in the suburb of Rumaithiya in Kuwait. Additional samples will be collected to expand the analysis and their chemical compositions will be characterized by a combination of laboratory X-ray fluorescence (XRF), Scanning Electron Microscopy (SEM) and TIR emission spectroscopy. The overarching objective of this ongoing research is to both characterize the effects of mineral dust on climate as well as establish a predictive tool that can identify dust storm sources and potentially aid in establishing a more accurate prediction and warning system in the Middle East region.

102

DIAMOND: an impact sensor for the characterization of Martian dust tori .  

Dust is supposed to be present in several orbits around Mars. The sources of these hypothetical dust belts are expected to be the two Martian satellites Phobos and Deimos, due to their continuous hypervelocity bombardment by interplanetary micro-meteoroids. Due to the low escape speeds from the surfaces of the two tiny moons and high ejecta yields, it is expected that a great amount of dust is ejected in areocentric orbit, forming tenuous tori around the orbits of the moons. Time of permanence of dust in the tori depends on grains mass and shape. Different models have been proposed in order to describe the process of generation and stabilization of dust in the tori but several uncertainties do exist about numerical density and size distribution of dust grains. In situ measurements are thus needed, in order to shed light on the extraction, escape and trap processes of particles in the tori. The instrument DIAMOND (Direct In-situ Analyser and Monitor of Orbiting Natural Dust) has been designed for the detection and characterization of dust in the hypothetical tori of Mars. It has been accepted by the Russian space agency as part of the payload of the Russian Phobos-Soil mission to be launched in 2011. The project is now under evaluation by ASI.

103

Quantification of impurities in the radioactive europium Quadra met with Hp Ge detector; Cuantificacion de impurezas de europio en el radiofarmaco Quadramet mediante detector de Ge Hp  

The reason of this study is due to the detection of radioactivity in the waste more than one year after its administration, due to impurities of europium generated during the production process itself Sm I53 neutron activation.

104

Dust Filtration by Planet-induced Gap Edges: Implications for Transitional Disks  

By carrying out two-dimensional two-fluid global simulations, we have studied the response of dust to gap formation by a single planet in the gaseous component of a protoplanetary disk—the so-called dust filtration mechanism. We have found that a gap opened by a giant planet at 20 AU in an ? = 0.01, \\dot{M}=10^{-8}\\,M_{\\odot }\\,yr^{-1} disk can effectively stop dust particles larger than 0.1 mm drifting inward, leaving a submillimeter (submm) dust cavity/hole. However, smaller particles are difficult to filter by a gap induced by a several M J planet due to (1) dust diffusion and (2) a high gas accretion velocity at the gap edge. Based on these simulations, an analytic model is derived to understand what size particles can be filtered by the planet-induced gap edge. We show that a dimensionless parameter Ts /?, which is the ratio between the dimensionless dust stopping time and the disk viscosity parameter, is important for the dust filtration process. Finally, with our updated understanding of dust filtration, we have computed Monte Carlo radiative transfer models with variable dust size distributions to generate the spectral energy distributions of disks with gaps. By comparing with transitional disk observations (e.g., GM Aur), we have found that dust filtration alone has difficulties depleting small particles sufficiently to explain the near-IR deficit of moderate \\dot{M} transitional disks, except under some extreme circumstances. The scenario of gap opening by multiple planets studied previously suffers the same difficulty. One possible solution is to invoke both dust filtration and dust growth in the inner disk. In this scenario, a planet-induced gap filters large dust particles in the disk, and the remaining small dust particles passing to the inner disk can grow efficiently without replenishment from fragmentation of large grains. Predictions for ALMA have also been made based on all these scenarios. We conclude that dust filtration with planet(s) in the disk is a promising mechanism to explain submm observations of transitional disks but it may need to be combined with other processes (e.g., dust growth) to explain the near-IR deficit of some systems.

105

Occupational radiation exposures of artisans mining columbite-tantalite in the eastern Democratic Republic of Congo  

Artisans in Masisi and other parts of the North Kivu province in the eastern Democratic Republic of Congo (DRC) mine columbite-tantalite mineral ores (also called 'coltan') for the tantalum content. The potential occupational radiation exposures in the course of this operation, due to the presence of naturally occurring radioactive material (NORM), have been investigated in this screening survey. Activity concentrations of the naturally occurring radionuclides in samples of coltan were measured using gamma-ray spectrometry. The average values in Bq g{sup -1} are 10.75 {+-} 5.11 for {sup 238}U, 7.06 {+-} 3.39 for {sup 226}Ra, 1.75 {+-} 0.85 for {sup 232}Th, and 1.63 {+-} 0.52 for {sup 40}K. Based on these values and the working scenarios involved in artisanal coltan mining, the occupational doses that may accrue from a variety of exposure pathways were determined by model calculations. The results, assuming conservative dust load and dilution factors, indicate that grinding and sieving coltan can give rise to high occupational doses, up to 18 mSv per annum on average.

106

Occupational radiation exposures of artisans mining columbite-tantalite in the eastern Democratic Republic of Congo.  

Artisans in Masisi and other parts of the North Kivu province in the eastern Democratic Republic of Congo (DRC) mine columbite-tantalite mineral ores (also called 'coltan') for the tantalum content. The potential occupational radiation exposures in the course of this operation, due to the presence of naturally occurring radioactive material (NORM), have been investigated in this screening survey. Activity concentrations of the naturally occurring radionuclides in samples of coltan were measured using gamma-ray spectrometry. The average values in Bq g(-1) are 10.75 +/- 5.11 for (238)U, 7.06 +/- 3.39 for (226)Ra, 1.75 +/- 0.85 for (232)Th, and 1.63 +/- 0.52 for (40)K. Based on these values and the working scenarios involved in artisanal coltan mining, the occupational doses that may accrue from a variety of exposure pathways were determined by model calculations. The results, assuming conservative dust load and dilution factors, indicate that grinding and sieving coltan can give rise to high occupational doses, up to 18 mSv per annum on average. PMID:17664663

107

Radiological characterisation of an industrial waste dump at a fertilizer plant in Tarragona (Spain)  

The solid waste coming from the fertilizer factory belonging to the Ercros Company in the town of Flix (Tarragona-Spain) is stocked in an industrial dump located close to the town. Measurements of natural radionuclide activity, principally from the U-238 chain, were done from mud samples taken from various depth points and areas within the dump. Specific activity of the various components of the chain reaches values in the range of 2000 to 4500 Bq/kg. There were some values outside this range, chiefly in the case of Th-230, which reached values of 13000 Bq/kg. The total radioactive inventory in the dump if long-period radioisotopes are considered, can be estimated to be approximately 9000 GBq. Determination of equivalent environmental dose using thermoluminescent dosemeters reached values less than 1.8 mSv/year, if permanence was supposed. Radiological testing of atmospheric dust collected at the site did not show significant values. Average radon concentrations of 30 Bq/m{sup 3}, were measured, slightly higher than 10 Bq/m{sup 3}, a value that was considered as a reference value for the area. Values for the increase of the effective dose due to external or internal exposure caused by the waste at the dump are lower than 1 mSv/year. (authors)

108

Public exposure to hazards associated with natural radioactivity in open-pit mining in Ghana.  

The results of studies carried out on public exposure contribution from naturally occurring radioactive materials (NORMS) in two open-pit mines in the Western and Ashanti regions of Ghana are reported. The studies were carried out under International Atomic Energy Agency-supported Technical Co-operation Project GHA/9/005. Measurements were made on samples of water, soil, ore, mine tailings and air using gamma spectrometry. Solid-state nuclear track detectors were used for radon concentration measurements. Survey was also carried out to determine the ambient gamma dose rate in the vicinity of the mines and surrounding areas. The effective doses due to external gamma irradiation, ingestion of water and inhalation of radon and ore dusts were calculated for the two mines. The average annual effective dose was found to be 0.30 +/- 0.06 mSv. The result was found to be within the levels published by other countries. The study provides a useful information and data for establishing a comprehensive framework to investigate other mines and develop guidelines for monitoring and control of NORMS in the mining industry and the environment as a whole in Ghana. PMID:19767601

109

Environmental radioactivity survey in Andong area  

To protect the our country from the environmental radioactivity pollution by the nuclear weapon experiments, atomic power plants and other nuclear matters etc, It is important to watching and inspect the environmental radiation/radioactivity on the airborne dust, rice, chinese cabbage, pollack, hair-tail, anchovy, tap water, soils and others. Measuring samples is airborne dust, precipitation, fall-out and tap water. Gamma exposure rates of Andong monitoring post measured every day through 1997 year, and 63 points of north Kyung Pook area measured one time through a year. Collect and handling samples is rice, chinese cabbage, tap water of 5 regions and milk of 3 regions and 3 kinds of fishes(Alaska pollack, Hair-tail, Anchovy), and 30 points soils in north Kyung Pook areas.

110

Relevance of aerosol size spectrum analysis as support to qualitative source apportionment studies.  

This work presents a diagnostic methodology in support to source apportionment studies to identify remote and local pollution sources. It is based on the temporal analysis of both PM size distributions and PM size fraction correlation along with natural radioactivity measurements as index of Planetary Boundary Layer dynamic. A correlation drop is indicative of changing aerosol sources. When this observation is coupled with decreasing level of natural radioactivity and increasing aerosol concentration, be it coarse or fine, it is indicative of the inflow of remote polluted air masses. The methodology defines in which size range operates the contribution of remote pollution sources. It was applied to two PM10 pollution episodes: the first involved the advection of coarse PM, the second entailed the inflow of two air masses, one transporting coarse dust and the other fine PM. Dust models and backward trajectories analysis confirmed such results, indicating the air mass provenience. PMID:22766004

111

Test plan for glove box testing with the real-time transuranic dust monitor  

This test plan describes the objectives, instrumentation, and testing procedures used to prove the feasibility of a real-time transuranic dust monitor (RTDM). The RTDM is under development at the Idaho National Engineering Laboratory (INEL) as a Waste Characterization Technology funded by the Buried Waste Integrated Demonstration Project. The instrument is an in situ monitor that uses optical techniques to establish particle size, particle number density, and mass and species of heavy metal contamination. US Department of Energy orders mandate the assessment of radiological exposure and contamination spread during the remediation of radioactive waste. Of particular concern is heavy metal contamination of dust, both radioactive and nonradioactive. Small particles of metal, particularly the radioactive species, tend to become electrically charged and consequently attach themselves to dust particles. This airborne activated dust is a primary means of contamination transport during remediation activities, and therefore, must be continuously monitored to protect personnel involved in the operations and to control the spread of contamination. If real-time monitoring is not available there is increased likelihood of generating unacceptably high levels of contamination and being forced to shut down costly retrieval operations to decontaminate. A series of experiments are described to determine the optimal experimental design, operational parameters, and levels of detection for the RTDM. Initial screening will be performed using monodisperse particle standards to set parameters and calibrate the instrument. Additional testing will be performed using INEL soil samples spiked with a surrogate, cerium oxide, to prove the design before transporting the apparatus to the Test Reactor Area for testing with plutonium-contaminated dusts.

112

Synoptic and remote sensing analysis of dust events in southwestern Iran  

Southwest regions of Iran, due to dry environmental and climatic conditions, have been identified as one of the five major regions in the world. In recent years, large parts of Iran have been affected by suspended particles from the dust storms. The studied area is located in foothills of the Zagros Mountain Range just north of Persian Gulf in southwest of Iran. Dust and other meteorological data were prepared in 3-hour intervals from 12 synoptic weather stations. For tracking dust storms, satellite images of MODIS were used. Atmospheric conditions during the occurrence of dust storms were determined using NCEP reanalysis data. According to the statistical calculations, most storms occurred in the spring and summer. The lowest number of dust events occurred in the fall and winter particula...

113

Dust collectors chop costs  

The use of dust collectors in pharmaceutical manufacturing is described as a means of fulfilling the FDA requirements concerning airborne dusts (due to weighing, granulating, drying, milling, blending, compressing, and packaging medicinal materials). Key areas in design are: (1) method of dust entry; (2) bag attachment; and (3) cleaning system design. These factors are discussed as well as energy conservation techniques. Of a total exhaust volume of 100,000 cfm, the system described is able to recirculate nearly 75,000 cfm, representing 1.6 million BTU or $5.25/hr. The two types of dust capture are described which result in a slight negative air pressure in each room. Efficiency of dust removal is 99.9%. (MJJ)

114

The ecology of dust: local- to global-scale perspectives  

Emission and redistribution of dust due to wind erosion in drylands drives major biogeochemical dynamics and provides important aeolian environmental connectivity at scales from individual plants up to the global scale. Yet, perhaps because most relevant research on aeolian processes has been presented in a geosciences rather than ecological context, most ecological studies do not explicitly consider dust-driven processes. To bridge this disciplinary gap, we provide a general overview of the ecological importance of dust, examine complex interactions between wind erosion and ecosystem dynamics from the plant-interspace scale to regional and global scales, and highlight specific examples of how disturbance affects these interactions and their consequences. Changes in climate and intensification of land use will both likely lead to increased dust production. To address these challenges, environmental scientists, land managers and policy makers need to more explicitly consider dust in resource management decisions.

115

Electrostatic precipitator with new energization system  

The collecting efficiency of a conventional electrostatic precipitator (EP) decreases when dust resistivity becomes high due to the 'back corona phenomenon'. A new type of EP suppresses back corona thus providing better efficiency even when dust resistivity is high. The principle of the new EP is basically to provide a high pulse peak voltage onto the discharge electrodes of the precharging section to maximise dust charge. The pulse voltage is supplied from a directly coupled pulse generator. Four EPs incorporating the pulse precharger, which have demonstrated enhanced collecting efficiency for high resistivity dust, have already been installed. A large capacity directly coupled pulse generator has also been connected to a whole field of conventional EPs and better collecting efficiency was attained for high resistivity dust.

116

Stability of dust lattice modes in the presence of charged dust grain polarization in plasmas  

We discuss the effect of the attractive force associated with overlapping Debye spheres on the dispersion properties of the longitudinal and transverse dust lattice waves in strongly coupled dust crystals. The dust grain attraction is shown to contribute to a destabilization of the longitudinal dust lattice oscillations. The (optic-like) transverse mode dispersion law is shown to change, due to the Debye sphere dressing effect, from the known inverse-dispersive ('backward wave') form into a normal dispersive law (i.e. the group velocity changes sign). The stability of one-dimensionless bi-layers, consisting of (alternating) negatively and positively charged dust particles, is also discussed. The range of parameter values (mainly in terms of the lattice parameter {kappa}) where the above predictions are valid, are presented.

117

IRAC Observations of M81  

IRAC images of M81 show three distinct morphological constituents: a smooth distribution of evolved stars with bulge, disk, and spiral arm components; a clumpy distribution of dust emission tracing the spiral arms; and a pointlike nuclear source. The bulge stellar colors are consistent with M-type giants, and the disk colors are consistent with a slightly younger population. The dust emission generally follows the blue and ultraviolet emission, but there are large areas that have dust emission without ultraviolet and smaller areas with ultraviolet but little dust emission. The former are presumably caused by extinction, and the latter may be due to cavities in the gas and dust created by supernova explosions. The nucleus appears fainter at 8 um than expected from ground-based 10 um observations made four years ago.

118

Numerical Modeling of the Coagulation and Porosity Evolution of Dust Aggregates  

Porosity evolution of dust aggregates is crucial in understanding dust evolution in protoplanetary disks. In this study, we present useful tools to study the coagulation and porosity evolution of dust aggregates. First, we present a new numerical method for simulating dust coagulation and porosity evolution as an extension of the conventional Smoluchowski equation. This method follows the evolution of the mean porosity for each aggregate mass simultaneously with the evolution of the mass distribution function. This method reproduces the results of previous Monte Carlo simulations with much less computational expense. Second, we propose a new collision model for porous dust aggregates on the basis of our N-body experiments on aggregate collisions. We first obtain empirical data on porosity changes between the classical limits of ballistic cluster-cluster and particle-cluster aggregation. Using the data, we construct a recipe for the porosity change due to general hit-and-stick collisions as well as formulae fo...

119

Asthma and the indoor environment: assessment of the health implications of high indoor air humidity  

Asthma and rhinitis are common chronic airway diseases often caused by exposure to allergens. Two important indoor allergens are house dust mites and spores from fungi. Fungal growth in house is caused either faulty insulation or indoor humidity. Below 45% relative humidity at 20-22/sup 0/C almost no house dust mites are able to survive, but at higher humidities the number of mites increases rapidly up to several thousand mites per gram house dust. Humid indoor conditions also favor the growth of fungi indoors. About 60% of all cases of newly diagnosed house dust mite asthma are due to a heavy exposure to house dust mites caused by high indoor humidities. Preventive measures are reduction of the indoor generated water vapor and higher ventilation rates. The size of the latter should not be fixed, but be adapted to keep indoor humidities so low that the growth of allergens is not favored.

120

Building-related symptoms and inflammatory potency of dust from office buildings  

Abstract The aim was to investigate the association between building-related symptoms (BRS) in office buildings and the inflammatory potency of dust (PD). Furthermore, the association between dust potency and various building characteristics was investigated. Occupants of 22 office buildings received a retrospective questionnaire about BRS (2301 respondents). Dust was collected from groups of offices and building characteristics were recorded. The potency of a dust sample to induce interleukin-8 (IL-8) secretion from the lung epithelial cell line A549 was measured as the slope of the initial linear part of the concentration-response curve. Symptoms of the central nervous system (CNS) were associated with the potency of surface dust (OR = 1.4). This association may be due to an association ...

 
 
 
 
121

STUDY OF THE RADIOACTIVITY IN AIR IN THE LOWER REGIONS OF THE ATMOSPHERE IN MEXICO CITY  

The radioactivity of the lowest layers of the atmosphere is studied by filter collection of the air-carried dust. Data are presented for Mexico City during the year 1959. From the autoradiography of the filters, the size distribution of the spots left by the active particles on the photographic plate is obtained. The slopes of the decay curves of some of the samples are also given. (auth)

122

Radiological survey and assessment of associated activity concentration of the naturally occurring radioactive materials (NORM) in the Migori artisanal gold mining belt of southern Nyanza, Kenya  

A radiological survey and assessment was carried out at selected sites (Osiri, Mikei, Masara and Macalder) in the Migori gold mines of southern Nyanza, Kenya to determine the levels of exposure of the artisanal miners to the naturally occurring radioactive materials (NORM) and dust. The activity concentrations of 40K and the decay products of 232Th and 226Ra were obtained using an innovative method in single channel NaI(Tl) gamma-ray spectrometry. The counts for both the sample and the reference material in a specific window for a particular radionuclide were compared to arrive at the activity concentration of the radionuclide in the sample. Measurement of dust loading at various crushing sites was carried out by trapping the dust particles on a 0.45 mu m cellulose acetate filter paper (47...

123

Radio-phobia, fantasies and realities; Radiophobie, fantasmes et realites  

After having criticized the attitude of the media after the discovery of a higher than normal radioactivity level on a beach of Camargue, which was in fact due to a natural phenomenon and had no health consequences, the author discusses the fear associated with radioactive radiations. He recalls the critical levels expressed in Sievert, the different levels associated either with natural or artificial radioactivity. He notices that radiation is generally feared whatever its radioactive level is. He outlines that the number of natural cancers is already relatively high. He finally proposes the use of the DARI as a unit (DARI stands for annual dose due to internal radiation)

124

Asian dust event observed in Seoul, Korea, during 29-31 May 2008: analysis of transport and vertical distribution of dust particles from lidar and surface measurements.  

In this study, we investigate the transport of dust particles, its vertical distribution, and the associated meteorological conditions during an Asian dust event that was observed in Seoul, Korea on May 29-31, 2008. This study analyzes data from ground-based and space-borne 2-wavelength polarization lidars, particulate mass concentrations, and synoptic weather data. Surface meteorological station observations of dust phenomena, dust transport model, and weather maps consistently show that the dust particles were transported from the source regions (Inner Mongolia, Man-Ju, and Ordos areas) to Korea via the northeastern part of China. Network observations of the PM(10) concentrations in Korea revealed that a majority of the heavy dust particles traveled across South Korea from the northwest to the southeast direction with a horizontal scale of 250-300km and a traveling speed of approximately 40kmh(-1). This extraordinary dust event, in terms of its intensity and timing during the year, occurred due to the blockage of an unusually intensified low-pressure system in the northeastern part of China as well as high-pressure system centered over the Sea of Okhotsk and the Kuril Islands. The low values of the particle depolarization ratio (delta(532)) (Lidar measurements in Seoul (delta(532) approximately 0.136+/-0.027). The value of delta(532) during the 2nd multilayered dust episode ranged between 0.081 and 0.120 for near-surface dust layers, and between 0.076 and 0.114 for elevated dust layers. The CALIPSO measurements of beta(532), delta(532), and CR also revealed the presence of dense dust aerosols along the transport route. PMID:20060573

125

Dust storms and their horizontal dust loading in the Sistan region, Iran  

The Sistan region in southeast Iran is considered as one of the most active dust source regions in South west Asia. The strong "Levar" winds in summer favor the uplift of large quantities of dust from the Hamoun basin, which is located in the northern part of Sistan. After a dry period at the end of the 1999s, and due to land-use change and desiccation of the Hamoun lakes, the frequency and severity of dust storms have been significantly increased. Within this framework, this study analyses the aerosol characteristics, dust loading and air quality over the Sistan region. The dust loading was measured using dust traps up to four and eight meters height (with a one meter distance between the traps) at two locations near the Hamoun basin during the period August 2009 to July 2010. The results show large quantities of transported dust that strongly dependent on the duration of the dust events, and secondarily, on the wind speed and distance from the source region. The grain size distribution of the dusts reveals that the coarser calibers are found at the station nearer to Hamoun, while the large differences in the grain-size distribution found between the two stations indicate significant spatio-temporal variation in dust characteristics. Furthermore, to assess the air quality, Particulate Matter (PM10) concentrations were measured over Zabol city during September 2010 to July 2011, and the Air Quality Index (AQI) was obtained. Daily PM10 levels during intense dust storms rise up to 2000 ?g m-3, even reaching to 3094 ?g m-3, while the monthly mean PM10 variation shows extreme values (>500 ?g m-3) for the period June to October. Analysis of the AQI shows that 61% of the days are associated with a high health risk, while 30.1% are even identified as hazardous.

126

A thermodynamic and mechanical model for formation of the Solar System via 3-dimensional collapse of the dusty pre-solar nebula  

The fundamental and shared rotational characteristics of the Solar System (nearly circular, co-planar orbits and mostly upright axial spins of the planets) record conditions of origin, yet are not explained by prevailing 2-dimensional disk models. Current planetary spin and orbital rotational energies (R.E.) each nearly equal and linearly depend on gravitational self-potential of formation (Ug), revealing mechanical energy conservation. We derive -?Ug??.R.E. and stability criteria from thermodynamic principles, and parlay these relationships into a detailed model of simultaneous accretion of the protoSun and planets from the dust-bearing 3-d pre-solar nebula (PSN). Gravitational heating is insignificant because Ug is negative, the 2nd law of thermodynamics must be fulfilled, and ideal gas conditions pertain to the rarified PSN until the objects were nearly fully formed. Combined conservation of angular momentum and mechanical energy during 3-dimensional collapse of spheroidal dust shells in a contracting nebula provides ?R.E.?R.E. for the central body, whereas for formation of orbiting bodies, ?R.E.?R.E.f(1-If/Ii), where I is the moment of inertia. Orbital data for the inner planets follow 0.04×R.E.f?-Ug which confirms conservation of angular momentum. Significant loss of spin, attributed to viscous dissipation during differential rotation, masks the initial spin of the un-ignited protoSun predicted by R.E.=-Ug. Heat production occurs after nearly final sizes are reached via mechanisms such as shear during differential rotation and radioactivity. We focus on the dilute stage, showing that the PSN was compositionally graded due to light molecules diffusing preferentially, providing the observed planetary chemistry, and set limits on PSN mass, density, and temperature. From measured planetary masses and orbital characteristics, accounting for dissipation of spin, we deduce mechanisms and the sequence of converting a 3-d dusty cloud to the present 2-d Solar System, and infer the evolution of dust and gas densities. Duration of events is obtained from the time-dependent virial theorem. As the PSN slowly contracted, collapse of pre-solar dust in spheroidal shells simultaneously formed rocky protoplanets embedded in a dusty debris disk, creating their nearly circular co-planar orbits and upright axial spins with the same sense as orbital rotation, which were then enhanced via subsequent local contraction of nearby nebulae. Because rocky kernels at great distance out-competed the pull of the co-accreting star, gas giants formed in the outer reaches within ˜3 Ma as PSN contraction hastened. This pattern repeated to form satellite systems. The PSN imploded, once constricted to within Jupiter's orbit. Afterwards, disk debris slowly spiraled toward the protoSun, cratering and heating intercepted surfaces. Our conservative 3-d model, which allows for different behaviors of gas and dust, explains key Solar System characteristics (spin, orbits, gas giants and their compositions) and second-order features (dwarf planets, comet mineralogy, satellite system sizes).

127

Comparing modeled and observed changes in mineral dust transport and deposition to Antarctica between the Last Glacial Maximum and current climates  

Mineral dust aerosols represent an active component of the Earth's climate system, by interacting with radiation directly, and by modifying clouds and biogeochemistry. Mineral dust from polar ice cores over the last million years can be used as paleoclimate proxy, and provide unique information about climate variability, as changes in dust deposition at the core sites can be due to changes in sources, transport and/or deposition locally. Here we present results from a study based on climate model simulations using the Community Climate System Model. The focus of this work is to analyze simulated differences in the dust concentration, size distribution and sources in current climate conditions and during the Last Glacial Maximum at specific ice core locations in Antarctica, and compare with available paleodata. Model results suggest that South America is the most important source for dust deposited in Antarctica in current climate, but Australia is also a major contributor and there is spatial variability in the relative importance of the major dust sources. During the Last Glacial Maximum the dominant source in the model was South America, because of the increased activity of glaciogenic dust sources in Southern Patagonia-Tierra del Fuego and the Southernmost Pampas regions, as well as an increase in transport efficiency southward. Dust emitted from the Southern Hemisphere dust source areas usually follow zonal patterns, but southward flow towards Antarctica is located in specific areas characterized by southward displacement of air masses. Observations and model results consistently suggest a spatially variable shift in dust particle sizes. This is due to a combination of relatively reduced en route wet removal favouring a generalized shift towards smaller particles, and on the other hand to an enhanced relative contribution of dry coarse particle deposition in the Last Glacial Maximum.

128

Air quality impacts analysis for area G. Final report  

The impact of fugitive radioactive emissions from the disposal site, Area G, was evaluated in support of site characterization for the Performance Assessment and for the Radioactive Air Emissions Management (RAEM) program. Fugitive emissions of tritiated water and contaminated windblown dust were considered. Data from an extensive field measurement program were used to estimate annual emissions of tritiated water. Fugitive dust models were used to calculate estimates of the annual emissions of windblown dust. These estimates were combined with data on contamination levels in surface soils to develop annual emission rates for specific radionuclides: tritium, uranium-238, cesium-137, plutonium-238, plutonium-239,240, and strontium-90. The CAP-88 atmospheric transport model was used to predict areas potentially affected by long-term dust deposition and atmospheric concentrations. The annual emission rate of tritiated water was estimated from the field data to be 14.0 Ci/yr. The emission rate of soil-borne radionuclides from open areas and from soils handling operations totaled less than 1x10{sup -4} Ci/yr. The CAP-88 results were used to develop effective dose equivalents (EDEs) for receptor locations downwind of Area G. All EDEs were several orders of magnitude below the national standard of 10 mrem/yr. Fugitive air emissions from Area G were found not to pose a health threat to persons living or working downwind of the facility.

129

Results of the radiological survey at the former Chapman Valve Manufacturing Company, Indian Orchard, Massachusetts (CIO001)  

Radiological survey was conducted at Building 23 (Department No. 40) at the former Chapman Valve Manufacturing Company, Indian Orchard, Massachusetts. The survey was performed in August 1991. The purpose of the survey was to determine whether the property was contaminated with radioactive residues, principally {sup 238}U, as a result of work done for the Atomic Energy Commission (AEC) during the 1940s. The survey included a gamma scan, a beta-gamma scan, and measurement of alpha activity; measurement of direct and removable alpha and beta-gamma levels; and the collection of soil, dust, debris, and smear samples for radionuclide analyses. Survey emphasis was on interior floors, walls, and overhead beams. Radionuclide analysis of soil, dust, and debris, and analysis of smear samples indicate that residual {sup 238}U attributable to former AEC-supported operations is present at this site. Elevated levels of radioactivity were particularly evident on the floors and walls in the western part of the central area of the building (grid blocks Al through A6). Concentrations of {sup 238}U in dust samples collected from overhead beams exceeded DOE guidelines in grid blocks Al through A14 and remained elevated in grid blocks A15 through A19. Dust on a movable overhead crane in grid block A23 was well above the guideline, probably because the crane had at some time been located further west. Some contamination was evident in grid blocks B1 through B5, but clutter and debris in this area prevented a thorough survey.

130

Methodology for radiological safety assessment in a Brazilian Norm/tenorm installation  

Handling, storage or any other operations involving materials containing elevated levels of natural radionuclides always causes some excess exposure to the worker and to the environment. C.N.E.N. is the regulatory authority to assess the magnitude of the potential environmental and occupational exposure. In the last year year the draft of the standard to establish safety and radiological protection requirements to ensure an adequate control level of the exposure of workers and environmental in the T.E.N.O.R.M. industries was published. The extent of exposure varies considerably in different operations, depending on the concentration of the radioactive material, chemical and physical processing, occupation times, dusting conditions etc... Exposure cannot, therefore, be assessed solely on basis of material activity concentrations. In order to determine the different ways by which the radionuclides can contaminate the environment, wastes and streams, a mass balance at the entire installation has been performed and main ways of workers exposition were characterized. During the last years the Brazilian Regulatory Body has been performing the characterization, monitoring and inspection of this kind of installation, and a methodology of work was implemented, including mass balance, radiological survey, area dust control, personal dust monitoring and internal contamination evaluation. This paper presents the methodology, including the description of a mass balance, typical results for the radiological survey, dust measurement (area and personal) and internal contamination in a typical N.O.R.M./T.E.N.O.R.M. installation. It is described, in detail, the dust monitoring related to excreta collection; the results for the radionuclide concentration in dust. The internal contamination evaluation will be reported in terms of radioactive contamination of the workers. (author)

131

Health-hazard evaluation report MHETA 85-226-1839, Freshlabs, Inc. , Warren, Michigan  

In response to a request from workers at the Freshlabs vitamin manufacturing facility located in Warren, Michigan, a study was made of dust exposures, with specific attention to asbestos in ceiling insulation. Over half of all workers (about 70) reported watery itchy eyes, sneezing, or runny stuff noses. Symptoms of skin rashes, cough, chest tightness, and shortness of breath were also reported throughout the facility. Dust concentrations were highest in the composition area, where all workers experienced irritation of eyes, nose, and throat, and a few developed occupational asthma confirmed by company physicians. Workers were exposed to several vitamin products which were irritating to eyes and nasal and respiratory mucosa because of acidity. Some workers became hypersensitive to dusts due to protein and polysaccharide contents. Most samples showed total and respirable dust measurements well below Occupational Safety and Health Administration permissible exposure limits for nuisance dusts. However, these are not common nuisance dust components. The authors suggest that the limits provide little protection for average workers exposed to such dusts. Asbestos sampling revealed potential hazard from falling insulation. Recommendations pertaining to local exhaust hoods, amended work practices, use of personal dust respirators, avoidance of skin contact, and proper ceiling insulation are offered.

132

Discovery of Potassium Chloride in the Sintering Dust by Chemical and Physical Characterization  

Sintering plant dust arrested by electrostatic precipitator (ESP dust) in an integrated iron and steel company is perceived as a precious secondary material to steelmaking process, due to the presence of important elements to the industry such as, Fe and C with an attractive concentration. However, some hazardous elements such as, K, Na, Zn, Pb, seriously destroying normal working of the blast furnace, are enriched meanwhile. Therefore, it becomes very important to know how to separate these elements from Fe and C before reusing the dust. The aim of this work is to carry out a chemical, physical, structural and morphological characterization of the sintering dust. The dust was subjected to granulometry analysis, chemical analysis, scanning electron microscopy (SEM), energy dispersive X-ray spectroscopy via SEM (EDS), X-ray mapping analysis via SEM and X-ray diffraction. With the help of these analysis ways and some comparison made between characterization of the dust before and after water leaching, an encouraging conclusion was drawn: KCl was identified in the sintering dust with a content percentage up to 30%. Considering serious lack of potassium fertilizer in China, it is necessary to recover KCl from the sintering dust. In addition, endanger of K to the steelmaking process is restricted at the same time.   

133

Upgrading a lime kiln chain section to reduce dust loading and improve thermal efficiency  

In order to meet a 50 per cent increase in pulp production, Daishowa Marubeni International Limited purchased additional quick lime for its Peace River Pulp Division to supplement the mill's lime requirements. However, the thermal efficiency of the kiln was poor because of excessive dust recycle in the kiln. This problem was addressed by replacing the inefficient, high maintenance kiln chain system with a high efficiency system. The result was a significant decrease in natural gas consumption by the kiln, thereby allowing for sustainable kiln production at high rates and reducing quick lime purchases. This article presented details of the lime kiln, kiln feed, kiln dust handling, kiln fuel and product lime. Kiln issues such as dust loading and heat transfer efficiency were also addressed. Lime kiln upgrades included a vacuum dust handling system upgrade and a chain section upgrade. The results of kiln upgrades were presented with particular reference to the effect on dust loading, kiln production, kiln thermal efficiency, ring formation and chain maintenance. It was concluded that the maximum capacity of the kiln was increased due to the upgrade in the dust handling system. However, the upgrade failed to address dust loading with in the kiln. The chain system upgrade reduced dust loading considerably and enabled sustained kiln operation at higher production rates. 1 ref., 14 figs.

134

Dust Filtration by Planet-Induced Gap Edges: Implications for Transitional Disks  

By carrying out two-dimensional two-fluid global simulations, we have studied the response of dust to gap formation by a single planet in the gaseous component of a protoplanetary disk - the so-called "dust filtration" mechanism. We have found that a gap opened by a giant planet at 20 AU in a \\alpha=0.01, \\dot{M}=10^{-8} Msun/yr disk can effectively stop dust particles larger than 0.1 mm drifting inwards, leaving a sub-millimeter dust cavity/hole. However, smaller particles are difficult to filter by a planet-induced gap due to 1) dust diffusion, and 2) a high gas accretion velocity at the gap edge. An analytic model is also derived to understand what size particles can be filtered by the gap edge. Finally, with our updated understanding of dust filtration, we have computed Monte-Carlo radiative transfer models with variable dust size distributions to generate the spectral energy distributions (SEDs) of disks with gaps. By comparing with transitional disk observations (e.g. GM Aur), we have found that dust fi...

135

Mineral Dust Transport to the North Atlantic and the North Pacific Oceans: Temporal Variability and the Link to Climate  

The North Atlantic and the North Pacific are heavily impacted by dust transport from North Africa and Asia respectively. The University of Miami, often in cooperation with other groups, has operated networks of aerosol sampling stations in these ocean regions for many years. In this presentation we present an overview of dust concentration data from these networks focusing on the temporal and geographical variability. Our objective is a better understanding of this variability in terms of source and transport processes. We place emphasis on two stations where we have a long record of aerosol measurements: Barbados, West Indies, (13.17N, 59.43W) and Midway (28.22N,177.35W) in the central North Pacific. The Barbados record is continuous from 1965 to present and Midway from 1981 to 2001. Dust concentrations show considerable variation over decadal and shorter time-scales. Prospero and Lamb [2003] recently showed that Barbados dust concentrations varied over a large range in a coherent way that is closely linked to rainfall (or the meteorology associated with rainfall) in the Soudano-Sahel region of North Africa. The dust record from Midway also shows large excursions especially over 1999 to 2001 reflecting intensified dust activity in Asia. During this period, large areas of China were impacted by drought. Thus both the Barbados and Midway data suggest that dust emissions increase sharply with the onset of drought. The question arises about the cause of increased dust emissions and transport. Is it simply due to drought conditions or does it reflect the combined effects of drought and human impacts? We suggest that poor land-use practices do not appear to be a major factor in these two examples. In the case of the North African dust sources, satellite images show that the major dust sources are located in exceedingly remote environments. In the case of Chinese dust sources, much literature has attributed increased dust to vastly increased agriculture and grazing in marginal lands. Yet statistics show that the frequency of dust storms has decreased markedly over the past several decades. Furthermore, there was relatively little change in dust concentrations at Midway through the late 1980s and into the 1990's when China was undergoing rapid development. In contrast North Africa has experienced a great increase in dust storm activity during the last 30 years and a concomitant decrease in visibility due to increased dust in the air. Dust sources are extremely sensitive to environmental conditions. Satellite images show that many prominent dust source regions are, in effect, composed of a series of "point" sources - that is, most of the dust is emitted from a relatively small area. This suggests that in order to better constrain the global dust budget, we need to have a much better understanding of the factors that affect the rate of emissions on scales reflecting the existence of these dust "hot spots".

136

Investigation of direct radiative effects of aerosols in dust storm season over East Asia with an online coupled regional climate-chemistry-aerosol model  

A new online coupled regional climate-chemistry-aerosol model (RIEMS-Chemaero) has been developed and applied to investigate direct radiative effects of dust aerosol and mixed aerosols over East Asia in March 2010, when an extremely intense dust storm on 19-22 March swept across almost the entire east China including the Pearl River Delta of south China, where little dust storm was observed before. The model results are evaluated against ground observation of PM10 concentration, aerosol optical depth (AOD) from both AERONET measurement and satellite retrieval (MODIS). The comparison demonstrates a good ability of RIEMS-Chemaero in reproducing major features of aerosol spatial distribution and temporal variation, as well as dust evolution during the dust storm period. However, the model tends to generally underpredict AOD at AERONET sites, with larger biases at urban sites than that at rural sites. Dust aerosols exerted a significant impact on radiation energy budget during the dust storm period, with the 4-day mean values of shortwave and longwave radiative forcings at the surface up to -90 W m-2 and +40 W m-2, respectively, over the Gobi desert. The monthly mean net dust radiative forcings at the surface ranged from -9 to -24 W m-2 over the dust source regions, and from -6 to -21 W m-2 over wide downwind areas including the middle and lower reaches of the Yellow River and the Yangtze River and the Yellow Sea. The net dust radiative forcing at TOA varied from near zero to +6.0 W m-2 in large areas of the continent. The monthly mean values of the net direct radiative forcings due to dust, non-dust aerosols and all aerosols (dust + sea salt + anthropogenic aerosols) averaged over the whole domain are estimated to be -3.9 W m-2, -5.6 W m-2 and -9.3 W m-2, respectively, at the surface, and to be +0.9 W m-2, -3.0 W m-2 and -2.0 W m-2, respectively, at TOA, indicating a light dust warming effect and an overall aerosol cooling effect in the springtime over East Asia. In east China, the net radiative forcings due to dust, non-dust aerosols and all aerosols at the surface are enhanced to -8.4 W m-2, -10.2 W m-2 and -18.0 W m-2, respectively, due to both the frequent dust influence and the intensive anthropogenic emissions in this region. The dust forcing accounts for about 42% of the total aerosol forcing at the surface in the domain, implying a potentially important role of mineral dust in radiation budget and regional climate. The semi-direct effect of dust aerosol tends to reduce cloud cover throughout the domain and it is partly responsible for the direct radiative forcings because of the feedbacks among aerosol, radiation, cloud and dynamics.

137

Contribution of Saharan dust on radionuclide aerosol activity levels in Europe? The 21-22 February 2004 case study  

In February 2004, a spectacular dust event was observed in the south of France. Associated with huge particulate matter deposition, unusual {sup 137}Cs concentrations were found in samples. Using the transport model CHIMERE-DUST, we first show that these dust aerosols came from North Africa. More precisely, the question is whether this sudden increase of measured {sup 137}Cs concentrations was due to a huge amount of dust over a large region (with an usual radionuclide content) or due to an import of more concentrated air masses over a limited area. This question is connected to the open debate about the contribution of {sup 137}Cs concentrations in Europe from 'Gerboise' sites, where former French nuclear tests in the 1960's were performed. With the model in scenario mode, this study attempts to track down {sup 137}Cs concentrations recorded in the south of France. To quantify the origin and percentage of dust originating from North Africa to the south of France, three simulations are performed: (1) with the complete dust emissions inventory of Africa, (2) with only emissions in the eastern Maghreb, and (3) only considering the Gerboise sites. It is showed that the majority (80%) of the dust was coming from eastern Maghreb, but only 0.7% of the African emissions were from Gerboise, leading to 1-5% of the concentrations recorded in the south of France for the day of the peak. (authors)

138

Effects of density gradient and dust concentration on ion acoustic solitons in multicomponent plasmas  

The ion acoustic solitons have been investigated in an inhomogeneous two-temperature electron plasma in the presence of immobile dust particles. The modified Korteweg-de Vries equation with an additional term due to density gradients is deduced by employing reductive perturbation technique. It is noticed that the amplitude of the soliton is increased with the decrease in the positively charged dust concentration, while the soliton amplitude is increased with the increase in negatively charged dust concentration in such inhomogeneous plasmas. The equilibrium density profile is taken exponential type and density gradient effects on soliton formation are also studied. The numerical results are shown for illustration.

139

A study of the properties of a local dust storm with Mars Express OMEGA and PFS data  

We present observations of a local dust storm performed by the OMEGA and PFS instruments aboard Mars Express. OMEGA observations are used to retrieve the dust single-scattering albedo in the spectral range 0.4-4.0 mm. The single-scattering albedo shows fairly constant values between 0.6 and 2.6 mm, and a sharp decrease at wavelengths shorter than 0.6 mm, in agreement with previous studies. It presents a small absorption feature due to ferric oxide at 0.9 mm, and a strong absorption feature due to hydrated minerals between 2.7 and 3.6 mm. We use a statistical method, the Independent Component Analysis, to determine that the dust spectral signature is decoupled from the surface albedo, proving that the retrieval of the single-scattering albedo is reliable, and we map the dust optical thickne...

140

Survey monitoring of environmental radioactivity in Chuncheon area  

Gross beta radioactivities in airborne dust, fallout, precipitation and tap water, and gamma exposure rates have been monitored periodically in 2000 at Chunchon Regional Radioactivity Monitoring Station. The concentrations of radioactive nuclide of {sup 7}Be and {sup 137}Cs on airborne dust, and {sup 7}Be, {sup 40}K and {sup 137}Cs on fallout, precipitation have been analyzed monthly. The {sup 7}Be, {sup 40}K, {sup 137}Cs and {sup 226}Ra etc. concentrations in the 23 foodstuffs(potato, sweet potato, bean sprout, onion, pumpkin, spinach, welsh onion, radish leaves, red pepper, garlic, lettuce, apple, persimmon, orange, pear, grape, mackerel, Alaska pollack, hairtail, squid oyster, baby clam, mussed) and 5 tap water sampled in Youngsoe area of Kangwon-do have also been measured. No significant changes from the previous years have been found in gross beta radioactivities in environmental samples and gamma exposure rates. The concentrations of {sup 7}Be, {sup 40}K, and {sup 137}Cs nuclide in the foodstuffs sampled in Youngseo area are less(or slightly higher in some cases) than the MDA value, except {sup 40}K nuclide. The concentrations of {sup 137}Cs and {sup 226}Ra nuclide in tap water are less(or is slightly higher in one sample) than the MDA value.

 
 
 
 
141

Survey monitoring of environmental radioactivity in Chuncheon area  

Gross beta radioactivities in airborne dust, fallout, precipitation and tap water, and gamma exposure rates have been monitored periodically in 2001 at Chunchon Regional Radioactivity Monitoring Station. The concentrations of radioactive nuclide of {sup 7}Be and {sup 137}Cs on airborne dust, and {sup 7}Be, {sup 40}K and {sup 137}Cs on fallout, precipitation have been analyzed monthly. The {sup 7}Be, {sup 40}K, {sup 137}Cs and {sup 226}Ra etc. concentrations in the 23 foodstuffs(potato, sweet potato, bean sprout, onion, pumpkin, spinach, welsh onion, radish leaves, red pepper, garlic, lettuce, apple, persimmon, orange, pear, grape, mackerel, Alaska pollack, hairtail, squid oyster, baby clam, mussel) and 5 tap water sampled in Youngseo area of Kangwon-do have also been measured. No significant changes from the previous years have been found in gross beta radioactivities in environmental samples and gamma exposure rates. The concentrations of {sup 7}Be, {sup 40}K, and {sup 137}Cs nuclide in the foodstuffs sampled in Youngseo area are less(or slightly higher in some cases) than the MDA values, except {sup 40}K nuclide. All the concentrations of {sup 137}Cs and {sup 226}Ra nuclides in the water are less than the MDA values.

142

Biochemical studies on the toxicity of hematite dust. [Guinea pigs  

Biochemical alterations in guinea pig lungs caused by hematite dust were followed at 150 days after intratracheal administration of the dust. In vivo dust exposure caused a significant increase in mitochondrial protein content and cytochrome c oxidase activity whereas diaphorase activity remained unaltered. Mitochondria from the exposed animals were apparently in a swollen state and their contraction profile upon the addition of ATP reflected permeability changes. However, in vitro dust caused no significant alterations. Significant increases in glycogen content along with an insignificant decrease in glycogen phosphorylase activity were also observed in hematite-treated guinea pig lungs. Decrease in drug-metabolizing enzymes such as aniline hydroxylase and tyrosine aminotransferase activities were also evident in the post mitochondrial fraction of the siderotic lungs. (/sup 3/H)Leucine-incorporation studies showed increased protein synthesis in the postmitochondrial fraction. Increase in protein synthesis in mitochondria was only marginal whereas in whole homogenate it decreased considerably. Experiments employing dust tagged with radioactive iron indicated the rapid mobilization of iron from lung and its distribution to various organs. The presence of iron-binding protein was confirmed by employing Sephadex gel-filtration techniques.

143

Mixing of Asian mineral dust with anthropogenic pollutants over East Asia: a model case study of a super-duststorm in March 2010  

Mixing of Asian mineral dust with anthropogenic pollutants allows pollutants (e.g. sulfate and nitrate) to be transported over longer distances (e.g. to the northern Pacific, even to North America) along with dust particles. This mixing therefore affects the atmospheric and oceanic environment at local, regional and even continental scales. In this study, we used a three-dimensional regional chemical transport model (Nested Air Quality Predicting Modeling System, NAQPMS) to examine the degree of mixing between Asian mineral dust and anthropogenic pollutants in a super-duststorm event during 19-22 March 2010. Influences of the mixing processes on regional atmospheric environmental and oceanic biogeochemical cycles were also investigated. A comparison with measurements showed that the model reproduced well the trajectory of long-range dust transport, the vertical dust profile, and the chemical evolution of dust particles. We found that along-path mixing processes during the long-range transport of Asian dust led to increasingly polluted particles. As a result, ~60% of the sulfate and 70-95% of the nitrate in the downwind regions was derived from active mixing processes of minerals with pollutants sourced from the North China Plain and enhanced by transport over South China. This mixing had a significant impact on the regional-scale atmospheric composition and oceanic biogeochemical cycle. Surface HNO3, SO2 and O3 were decreased by up to 90%, 40% and 30%, respectively, due to the heterogeneous reactions on dust particles. Fe solubility rose from ~0.5% in the Gobi region to ~3-5% in the northwestern Pacific, resulting from oxidization of SO2 on dust particles. Total Fe(II) deposition in the ocean region of East Asia reached 327 tons during the 4-day dust event, and created a calculated primary productivity of ~520 mgC m-2 d-1 in the Kuril Islands, which can support almost 100% of the observed mean marine primary productivity in spring in this region (526 mgC m-2 d-1).

144

Response of East Mediterranean surface water to Saharan dust: On-board microcosm experiment and field observations  

An on-board microcosm experiment was performed during the CYCLOPS May 2002 cruise to track the biogeochemical response of Eastern Mediterranean surface seawater to a gradient addition of fresh and pre-leached Saharan dust, mimicking the potential fertilization effect as opposed to the impact of adding particles alone. Response parameters examined were P-turnover time, bacterial production and abundance, chlorophyll a, other phytopigments, abundance of different pico and nanophytoplankton groups, primary production rates, abundance of heterotrophic nanoflagellates and ciliates. The addition of fresh Saharan dust (range: 0.2 4.9mgl) and the subsequent nutrient release triggered an increase in phytopigments and primary production, while no response was detected for pre-leached dust particles. Most responses were linearly related to the amount of fresh dust added. Synechococcus and prymnesiophytes increased in abundance along with cellular pigment content while Prochlorococcus disappeared, heterotrophic bacteria increased production rates, and ciliates showed a small increase in cell density. A less clear response was recorded by in situ measurements following a Saharan dust storm during a cruise in the Levantine Basin in May 2001. The calculated amount of nutrients and dust particles delivered by such an event to a 15-m thick mixed surface layer is low (˜0.3nmolPl, ˜9nmolNl and 0.06mgdustl), falling close to the lowest dust addition in our microcosm experiment. Even so, an enhancement of phosphate turnover time, a sharp decline of Prochlorococcus abundance, and slight increases in chlorophyll a and bacterial activity were observed in response to the dust storm. Considering the linear effect of fresh dust concentrations on the bacterial activity, primary production and pigment concentration (total and per cell), and the likely stimulation of grazing, it is not surprising that changes due to moderate strength dust storms are mostly close to detection limit of either field or remote sensing measurements.

145

Heating of dust in the broad-line regions of active galaxies and quasars  

In this paper we discuss the relevant energy sources which heat (and, in many cases, destroy) the dust grains in the emission-line clouds (ELCs) which give rise to the broad-line emission seen in active extragalactic objects. We compare the heating rates from the external radiation field, trapped line radiation, and the diffuse bound-free continua. We find that in hot clouds (T/sub e/ = 1.5 x 10/sup 4/ K) Ly..cap alpha.. dominates the dust heating rate, while in cooler clouds (T/sub e/ = 1.0 x 10/sup 4/ K) the external radiation field dominates. In all cases, the dust residing in the broad-line clouds is quite hot (T>500 K). These results are discussed in light of the observed infrared properties of active galaxies and quasars, and the following conclusions are reached: (1) If the infrared emission of Seyfert 1 galaxies is primarily thermal in origin, then the redder near-IR colors distinguishing the Seyfert 1 galaxies from the Seyfert 2 galaxies may be understood in terms of the broad-line regions (BLR) concentrating hot dust within the inner parsec of the of the nucleus. (2) Substantial near-infrared dust emission may originate in the neutral regions of the ELCs with only minor accompanying reddening of the hydrogen Balmer lines, since dust confined to the neutral zone reddens only lines emitted from the back side of the cloud. (3) If the broad-line regions of the quasars are characterized by hotter temperatures than Seyfert 1 galaxies, dust may not be able to exist in this region, thereby explaining the apparent lack of thermal dust emission in quasars. (4) Because of the cooling times of the ELCs, near-IR variability due to changes in the dust temperature is dominated by light travel considerations. (5) The present calculations suggest that the dust-to-gas mass ratio in the BLRs of Seyfert 1 galaxies is substantially smaller than the value of 0.01 typically found in our Galaxy.

146

Solar Wind Plasma and UV effects on Surfaces in Space  

Dust plasma interactions on airless bodies in space affect both the exposed surfaces and the plasma flow around them. For example, charging, evaporation, and sputtering can shape the spatial and size distributions of small dust particles, and simultaneously alter the composition and energy distribution of the solar wind flow. Recent Ulysses observations of the temporal variability of the flux and direction of the interstellar dust flow show that the dynamics of submicron sized interplanetary and interstellar dust is determined by their charge and interactions with the large-scale structure of the heliospheric magnetic fields. Future observations by the Solar Probe Plus mission near the Sun are expected to identify pick-up ions from the evaporation and sputtering of dust and the effects of mass-loading on the solar wind. Charging of surfaces, combined with near-surface electric fields can lead to the mobilization and transport of small charged dust particles on all airless bodies in the solar system. Halley's comet showed large brightness fluctuations on very short time-scales at distances well beyond 8 AU. Surface charging due to intermittent high-speed solar wind streams have been suggested to be responsible for lofting small grains, increasing the effective surface area of the dormant nucleus. Images taken of the surface of asteroid Eros indicated the accumulation of fine dust in craters, possibly due to electrostatic dust transport. Remote sensing and in situ observations indicating dust transport on the Moon date back to the Apollo era and remain highly controversial. This presentation, motivated by existing observations, will describe a series of small-scale laboratory experiments and supporting theory to investigate dust charging, the properties of photoelectron sheaths, and the emergence of intense electric fields near boundaries of lit and dark surfaces, and regions shielded and exposed to the solar wind plasma flow. The Moon is the nearest place where dusty plasma effects could be investigated the easiest. The presentation will conclude with a summary of the science, measurement and instrument requirements for a Lunar Dust Transport Package (LDTP) to be placed on the lunar surface. LDTP will measure the time-dependent characteristics of the plasma sheath, and observe both the high-speed impacts of interplanetary and interstellar dust, and the putative fluxes of low-speed, highly charged lunar dust particles. LDTP will bring closure to decades-long open issues about dusty plasma effects on the lunar surface, and all other airless bodies in our solar system.

147

Saharan dust event impacts on cloud formation and radiation over Western Europe  

We investigated the impact of mineral dust particles on clouds, radiation and atmospheric state during a strong Saharan dust event over Europe in May 2008, applying a comprehensive online-coupled regional model framework that explicitly treats particle microphysics and chemical composition. Sophisticated parameterizations for aerosol activation and ice nucleation, together with two-moment cloud microphysics are used to calculate the interaction of the different particles with clouds depending on their physical and chemical properties. The impact of dust on cloud droplet number concentration was found to be low, with just a slight increase in cloud droplet number concentration for both uncoated and coated dust. For temperatures lower than the level of homogeneous freezing, no significant impact of dust on the number and mass concentration of ice crystals was found, though the concentration of frozen dust particles reached up to 100 l-1 during the ice nucleation events. Mineral dust particles were found to have the largest impact on clouds in a temperature range between freezing level and the level of homogeneous freezing, where they determined the number concentration of ice crystals due to efficient heterogeneous freezing of the dust particles and modified the glaciation of mixed phase clouds. Our simulations show that during the dust events, ice crystals concentrations were increased twofold in this temperature range (compared to if dust interactions are neglected). This had a significant impact on the cloud optical properties, causing a reduction in the incoming short-wave radiation at the surface up to -75 W m-2. Including the direct interaction of dust with radiation caused an additional reduction in the incoming short-wave radiation by 40 to 80 W m-2, and the incoming long-wave radiation at the surface was increased significantly in the order of +10 W m-2. The strong radiative forcings associated with dust caused a reduction in surface temperature in the order of -0.2 to -0.5 K for most parts of France, Germany, and Italy during the dust event. The maximum difference in surface temperature was found in the East of France, the Benelux, and Western Germany with up to -1 K. This magnitude of temperature change was sufficient to explain a systematic bias in numerical weather forecasts during the period of the dust event.

148

Impacts of dust deposition on dissolved trace metal concentrations (Mn, Al and Fe) during a mesocosm experiment  

The deposition of atmospheric dust is the primary process supplying trace elements abundant in crustal rocks (e.g. Al, Mn and Fe) to the surface ocean. Upon deposition, the residence time in surface waters for each of these elements differs according to their chemical speciation and biological utilization. Presently however their behavior after atmospheric deposition is poorly constrained, principally because of the difficulty in following natural dust events in-situ. In the present work we examined the temporal changes in the biogeochemistry of crustal metals (in particular Al, Mn and Fe) after an artificial dust deposition event. The experiment was contained inside trace metal clean mesocosms (0-12.5 m depths) deployed in the surface waters of the Northwestern Mediterranean, close to the coast of Corsica in the frame of the DUNE project (a DUst experiment in a low Nutrient low chlorophyll Ecosystem). Two consecutive artificial dust deposition events, each mimicking a wet deposition of 10 g m-2 of dust, were performed during the course of this DUNE-2 experiment. The changes in dissolved manganese (dMn), iron (dFe) and aluminium (dAl) concentrations were followed immediately and over the following week and their inventories and loss or dissolution rates were determined. The evolution of the inventories after the two consecutive additions of dust showed distinct behaviors for dMn, dAl and dFe. Even though the mixing conditions differed from one seeding to the other, dMn and dAl showed clear increases directly after both seedings due to dissolution processes. Three days after the dust additions, dAl concentrations decreased as a consequence of scavenging on sinking particles. dAl appeared to be highly affected by the concentrations of biogenic particles, with an order of magnitude difference in its loss rates related to the increase of biomass after the addition of dust. For dFe concentrations, the first dust addition decreased the concentrations through scavenging of the dust particles, whereas the second seeding induced dissolution of Fe from the dust particles. This difference, which might be related to a change in Fe-binding ligand concentration in the mesocosms, highlights the complex processes that control the solubility of Fe. Based on the inventories at the mesocosm scale, the estimations of solubility of metals from dust particles in seawater were 1% for Al and 40% for Mn which were in good agreement with laboratory based estimates. Overall, the trace metal dataset presented here makes a significant contribution to enhancing our knowledge on the processes influencing trace metals release from Saharan dust and the subsequent processes of bio-uptake and scavenging in a low nutrient low chlorophyll area.

149

Estimation of Direct Radiative Forcing of Asian Dust Aerosols with Sun/Sky Radiometer and Lidar Measurements at Gosan, Korea  

In this study the aerosol direct radiative forcing (ADRF) of Asian dust is evaluated by model simulation at Gosan, Jeju using the data from a sun/sky radiometer, a Micro-Pulse Lidar (MPL), and column radiometer measurements of solar downwelling irradiance in April, 2001. We suggest a method of determining aerosol parameters for the radiative transfer model from the Aerosol Robotic Network (AERONET) data set. Since the AERONET measurements provide the refractive indices at only four wavelengths, and the aerosol parameters can be calculated at these wavelengths with a Mie code, we use a linear regression method for extending these measurements to the full wavelength spectrum of the radiative transfer model. The aerosol forcing by the Asian dust aerosols is estimated and compared to the aerosol forcing of non-dust aerosols. On the Asian dust event day, April 13, the daily average ADRF was estimated as -58.1 W/m² at the surface and -25.7 W/m² at the top of the atmosphere (TOA). On April 15, a nondust day slightly influenced by anthropogenic aerosols, the ADRF was -29.0 W/m² at the surface and -11.6 W/m² at the TOA. Although the Asian dust aerosols show larger forcing, its forcing efficiency (forcing per unit optical thickness) is smaller than that of non-dust aerosols; ²41.0 W/m²/?670 at the TOA and -94.9 W/m²/?670 at the surface on the dust day for dust aerosols, as opposed to -50.0 W/m²/?670 at the TOA and -129.3 W/m²/?670 at the surface on the non-dust day for non-dust aerosols. We believe that this is due to the larger single scattering albedo of dust aerosols, which causes smaller absorption, and the larger asymmetry factor which causes more forward scattering or less reflection, compared to anthropogenic aerosols. The model results were validated with the surface irradiance measurement data and the comparison showed a good agreement. The radiative transfer calculation underestimates the solar irradiance of 2?3% on average. The aerosol profiles measured by lidar are used to estimate the influence of the vertical distribution of Asian dust aerosols on the ADRF. Using the vertical aerosol profiles, we found an instantaneous short wave radiative heating larger than 2 K/day. We believe the enhanced heating rate by the aerosol layers contributes to the increase in static stability within the dust layer. This fact is verified by the temperature profile measured by the sonde, and may explain the longevity and consequently long-range transport of Asian dust.   

150

Reduction potential of traffic measures to the fine dust and NO{sub 2} load; Minderungspotenzial verkehrlicher Massnahmen auf die Feinstaub- und NO{sub 2}-Belastung  

Significant reduction potentials with respect to fine dust and NO{sub 2} emissions are expected in case of traffic measures. Taking into account the contribution of the local road traffic to the pollutant load it is clear that only small reductions can be reached by realistic traffic measures. Since fine dust emissions are even lower than NO{sub 2} emissions the potential savings due to specific traffic measures are marginal. Several examples are discussed to show these relations.

151

An attempt to make an inventory of dust emissions in France; Tentative d`inventaire des emissions de poussieres en France  

The various dust emissions due to combustion and industrial processes, have been quantified; data and diagrams are presented for France from 1960 to 1995: the emission contributions from the residential and commercial sectors, industrial sector, power plants and road transportation are detailed and their evolutions are compared; emission charts are also presented, according to fuel type and dust granulometry. The importance of road transportation emissions is pointed out

152

Overview of radiation safety in the tin by-product (amang) industry of South East Asia.  

Processing of by-product heavy minerals (amang) from tin mining involves potential exposure to external and internal sources of radioactivity. The radioactivity arises through the presence of thorium and uranium series radionuclides in the various minerals. Monazite is the most radioactive mineral, containing 3% to 7% thorium by weight, while ilmenite is generally the least radioactive mineral containing typically less than 0.05% thorium. External exposure occurs when workers are in close proximity to accumulations or stockpiles of the radioactive minerals, whereas internal exposure occurs when workers are involved in dusty processes. This paper summarizes the nature of the amang industry in South East Asia and presents the results of preliminary measurements of external radiation and airborne radioactivity in twelve Malaysian and Thai plants. Although constrained by a paucity of exposure data, it is concluded that radiation doses to some amang plant workers may approach or exceed international standards and that appropriate control measures are required as a matter of priority, Radiation doses may approach or exceed 100 mSv in situations where workers are exposed to excessive levels of ambient dust and no protective measures are used. Observations and recommendations are made relating to monitoring and surveillance, instruction and training, and engineering and administrative protection measures. PMID:8690608

153

L-Moments and fuzzy cluster analysis of dust storm frequencies in Iran  

In this study, we use the L-moments and fuzzy-clustering techniques to analyze dust storm frequencies in Iran. A homogeneity test based on H statistics is first carried out using the dust-storm-frequency time series at 122 weather stations. The test shows that dust storms over the study area as a whole do not have the same probabilistic behavior. To identify homogeneous regions within the study area, a fuzzy c-means algorithm based on the L-moments of the dust-storm-frequency time series is employed. By use of the cluster validation index, partition coefficient and partition entropy, four clusters are identified, i.e., the first Zagros east cluster (Cluster 1A) and the second Zagros east cluster (Cluster 1B), related respectively to the Dashte Kevir and Dashte-Lout dust source regions, the Zagros west cluster (Cluster 2) and the Iran northwest cluster (Cluster 3). Based on the goodness-of-fit test, ZDist, the best regional distribution models for Clusters 1A, 1B, 2 and 3 are found to be Pearson III, generalized normal, generalized Pareto and generalized normal distributions, respectively. The different types of the distributions suggest that the dust storms in the different cluster regions are due to different generation mechanisms and are associated with different dust sources. The regional growth curves are then constructed using the regional distribution models. The sharp slope of the growth curve for Cluster 2 and 3 suggests that the dust storms in the northwestern and western parts of Iran are mainly due to dust transport from the Sahara, Rub al Khali and Arabian deserts.

154

Pebble Bed Reactor Dust Production Model  

The operation of pebble bed reactors, including fuel circulation, can generate graphite dust, which in turn could be a concern for internal components; and to the near field in the remote event of a break in the coolant circuits. The design of the reactor system must, therefore, take the dust into account and the operation must include contingencies for dust removal and for mitigation of potential releases. Such planning requires a proper assessment of the dust inventory. This paper presents a predictive model of dust generation in an operating pebble bed with recirculating fuel. In this preliminary work the production model is based on the use of the assumption of proportionality between the dust production and the normal force and distance traveled. The model developed in this work uses the slip distances and the inter-pebble forces computed by the authors’ PEBBLES. The code, based on the discrete element method, simulates the relevant static and kinetic friction interactions between the pebbles as well as the recirculation of the pebbles through the reactor vessel. The interaction between pebbles and walls of the reactor vat is treated using the same approach. The amount of dust produced is proportional to the wear coefficient for adhesive wear (taken from literature) and to the slip volume, the product of the contact area and the slip distance. The paper will compare the predicted volume with the measured production rates. The simulation tallies the dust production based on the location of creation. Two peak production zones from intra pebble forces are predicted within the bed. The first zone is located near the pebble inlet chute due to the speed of the dropping pebbles. The second peak zone occurs lower in the reactor with increased pebble contact force due to the weight of supported pebbles. This paper presents the first use of a Discrete Element Method simulation of pebble bed dust production.

155

Climate affected by dust aerosol over arid region of Makkah, Saudi Arabia  

Aerosols play an important role in the global climate balance, and therefore they could be important in climate change. Natural variations of aerosols, especially due to dust storm are recognized as a significant climate forcing, that is, a factor that alters the Earth's radiation balance and thus tends to cause a global temperature change. Aerosol optical depth, ?(?) is the most comprehensive variable to characterize aerosol due to atmospheric pollution. The aerosol optical properties in Makkah observed during dust period (March-May) from 2006 to 2009 had been presented in this study. Aerosol optical depths at all wavelengths showed a sharp increase during major dust outbreak in spring when compared with the average for the season. For example at Makkah, aerosol optical depths increase from the spring average value of 0.43+/-0.02 at 550 nm to values >0.70 during major dust event days in 2006. These tend to increasingly of temperature during this period as results of absorbing aerosol effect. In this paper, we used AOD data from Terra MODIS to evaluate the trend of dust aerosol events in Makkah throughout 4 years dataset with supported data of subtype of aerosol and air temperature from CALIPSO and MERRA respectively. The higher values of AOD are corresponding to the low visibility due to presents of high concentration of dust.

156

Biological hazard issues from potential releases of tritiated dust from ITER  

Tritiated dust will be generated during the operation of ITER. Several dedicated studies, having performed in-vitro and in-vivo experiments on metal tritide and carbon tritide dust, raised some concerns about the protection guidelines for workers exposed to tritiated dust, if based on the radiotoxicity of tritium in form of tritium gas (HT), tritiated water (HTO) or organically bound tritium (OBT). While the behaviour of HT, HTO and OBT in the human body is well understood, the same is not fully true for tritiated dust, considering the different size distributions and the variety of base materials (through density and morphology), just to cite the most important ones. Inhaled HTO is translocated to blood completely and instantaneously, and then distributes uniformly throughout the body without changing its chemical form. About 1% of the inhaled HT is dissolved in body fluids and tissues and out of this fraction about 1% is then converted to HTO and the rest exhaled. The in-vivo and in-vitro studies on tritiated dust have shown the dependence of the tritium clearance and retention in the human body from their physico-chemical parameters. The most important ones are: - The dust particles size, influencing the dust deposition pattern and the self absorption fraction of beta rays which in turn affects the dose delivered to lungs; - The particle density influencing the tritium dissolution fraction and the self absorption fraction of betas particles; - The dust particle specific surface area influencing the tritium dissolution fraction. Therefore, it is important to develop credible and sound biokinetic models and from there dose conversion factors for tritiated dust for materials considered in ITER. From studies carried out so far, it is evident that absorption to lung differs from other tritium forms. Tritiated dust ranges from absorption type S (slow) to type M (moderate) according to the ICRP classification, whereas HTO and HT are classified as F (fast). Some recent studies on JET dust relative to graphite and CFC dust have dealt with physico-chemical characterization and with in vitro tritium dissolution studies. Some uncertainties still remain and further testing is necessary. In the working areas of ITER the radioactive dust concentration in air will be kept at a very low level. However in an incidental sequence, the atmosphere inside the buildings, including operative areas as well, might get contaminated with small amounts of tritiated dust and hence inhalation risks cannot be excluded. The present paper summarizes the results from previous investigations on the subject which can build the basis for deriving sound dose conversion factors for tritiated dust aimed for internal dosimetry. At the same time, it proposes further studies and experiments in order to have a complete understanding of the biological hazards of tritiated dust for ITER relevant materials. (orig.)

157

Radiological impact of phosphogypsum discharged into the Venice lagoon: 222Rn  

For about 20 years, between the 60 's and the 80 's of the last century, in the Passo a Campalto area (Lagoon of Venice - Italy) about 400,000 m3 of phosphogypsum (PG) were deposited at the border of the lagoon and next to urban areas without any environmental control. These materials are a by-product formed during the wet processing of phosphate rocks by sulphuric acid and have a significant environmental impact due to their abundance and their chemical-physical and radiochemical characteristics. The PG contains both chemical elements, which are considered dangerous for the ecosystems and natural radionuclides whose concentrations are much higher if compared to those typical for the Earth's crust. These discarded materials caused for many years the dispersion of radionuclides in the environment due to the tidal erosion, the re-suspension of radioactive inhalable dusts, the uncontrolled radon exhalation and the bioaccumulation of some radionuclides in the lagoon environment. After a decision of the appointed authorities, the Venice Water Authority (Ministry of Infrastructure and Transport), planned a permanent safety control of the site resulting in the complete isolation of the entire volume of contaminated materials from the environmental system. The entire project was specific for the particular features of the site and it required the improvement of analytical, sampling and measurement techniques in order to verify the effectiveness of the safety action. The radon assessment, in particular the check of the effectiveness of the inhibition of radon exhalation, is part of a more complex study, covering many other aspects of the management of a permanent disposal; they will be the object of further notes. The ultimate results of this study prove the efficacy of the intervention: radon concentrations in air and exhalation values from the restored area, measured during surveys, have been proved to be well in agreement with those of non contaminated soils.

158

Hinkley Point C inquiry report  

The evidence of several expert witnesses to the Hinkley Point C inquiry is reported. Topics such as the safe disposal of radioactive nuclear waste without dangers to the environment, possible mutations in micro-organisms due to radiation and the need for a waste repository for radioactive materials were addressed. (UK).

159

Change of the Asian dust source region deduced from the composition of anthropogenic radionuclides in surface soil in Mongolia  

Recent climate change, especially during the 2000s, may be the primary reason for the expansion of the Asian dust source region. The change in the dust source region was investigated by examining anthropogenic radionuclides contained in surface soil samples from Mongolia. Surface soil was globally labeled by radioactive fallout from nuclear testing during the late 1950s and early 1960s, but there are no current direct sources for anthropogenic radionuclides in the air (before the Fukushima nuclear power plant accident in 2011). Radionuclides in the atmosphere are therefore carried mainly by wind-blown dust from surface soil, that is, aeolian dust. Asian dust carries traces of 90Sr, 137Cs, and other anthropogenic radionuclides; the heaviest deposition occurs in spring and has been recorded in Japan since the early 1990s. The composition of anthropogenic radionuclides in atmospheric depositions would be affected by a change in the dust source. Previous studies of atmospheric deposition at long-term monitoring sites (e.g. in Tsukuba, Japan) have detected changes in the 137Cs/90Sr ratio and in the specific activity of the radionuclides. These changes in the composition of observed atmospheric depositions are supposed to reflect changes in the climatic conditions of the dust source region. To investigate this dust source change, we conducted a field survey of radionuclides (90Sr and 137Cs) in surface soil samples in September 2007 in the eastern and southern regions of Mongolia, where dust storms have occurred more frequently since 2000. The specific activities of both radionuclides as well as the 137Cs/90Sr ratio in the surface soil were well correlated with annual average precipitation in the Mongolian desert-steppe zone. Higher specific activities and a higher 137Cs/90Sr ratio were found in grassland regions that experienced greater precipitation. These findings suggest that the increased specific activities and the activity ratio detected in atmospheric depositions in Japan during years with frequent Asian dust transport events in the 2000s are a sign of grassland degradation.

160

Transformation of Graphitic and Amorphous Carbon Dust to Complex Organic Molecules in a Massive Carbon Cycle in Protostellar Nebulae  

More than 95% of silicate minerals and other oxides found in meteorites were melted, or vaporized and recondensed in the Solar Nebula prior to their incorporation into meteorite parent bodies. Gravitational accretion energy and heating via radioactive decay further transformed oxide minerals accreted into planetesimals. In such an oxygen-rich environment the carbonaceous dust that fell into the nebula as an intimate mixture with oxide grains should have been almost completely converted to CO. While some pre-collapse, molecular-cloud carbonaceous dust does survive, much in the same manner as do pre-solar oxide grains, such materials constitute only a few percent of meteoritic carbon and are clearly distinguished by elevated D/H, N-15/N-16, C-13/C-12 ratios or noble gas patterns. Carbonaceous Dust in Meteorites: We argue that nearly all of the carbon in meteorites was synthesized in the Solar Nebula from CO and that this CO was generated by the reaction of carbonaceous dust with solid oxides, water or OH. It is probable that some fraction of carbonaceous dust that is newly synthesized in the Solar Nebula is also converted back into CO by additional thermal processing. CO processing might occur on grains in the outer nebula through irradiation of CO-containing ice coatings or in the inner nebula via Fischer-Tropsch type (FTT) reactions on grain surfaces. Large-scale transport of both gaseous reaction products and dust from the inner nebula out to regions where comets formed would spread newly formed carbonaceous materials throughout the solar nebula. Formation of Organic Carbon: Carbon dust in the ISM might easily be described as inorganic graphite or amorphous carbon, with relatively low structural abundances of H, N, O and S . Products of FTT reactions or organics produced via irradiation of icy grains contain abundant aromatic and aliphatic hydrocarbons. aldehydes, keytones, acids, amines and amides.. The net result of the massive nebular carbon cycle is to convert relatively inert carbonaceous dust from the ISM into the vital organic precursors to life such as amino acids and sugars intimately mixed with dust and ice in primitive planetesimals. Since the number of carbon atoms entering the Solar Nebula as dust exceeds the number of atoms entering the nebula as oxide grains. the formation of large quantities of complex organic molecules may represent the largest single chemical cycle in the nebula.

 
 
 
 
161

Electromagnetic mixed waste processing system for asbestos decontamination  

DOE sites contain a broad spectrum of asbestos materials (cloth, pipe lagging, sprayed insulation and other substances) which are contaminated with a combination of hazardous and radioactive wastes due to its use during the development of the U.S. nuclear weapons complex. These wastes consist of cutting oils, lubricants, solvents, PCB`s, heavy metals and radioactive contaminants. The radioactive contaminants are the activation, decay and fission products of DOE operations. The asbestos must be converted by removing and separating the hazardous and radioactive materials to prevent the formation of mixed wastes and to allow for both sanitary disposal and effective decontamination. Currently, no technology exists that can meet these sanitary and other objectives.

162

Electromagnetic mixed waste processing system for asbestos decontamination  

DOE sites contain a broad spectrum of asbestos materials (cloth, pipe lagging, sprayed insulation and other substances) which are contaminated with a combination of hazardous and radioactive wastes due to its use during the development of the U.S. nuclear weapons complex. These wastes consist of cutting oils, lubricants, solvents, PCB`s, heavy metals and radioactive contaminants. The radioactive contaminants are the activation, decay and fission products of DOE operations. The asbestos must be converted by removing and separating the hazardous and radioactive materials to prevent the formation of mixed wastes and to allow for both sanitary disposal and effective decontamination. Currently, no technology exists that can meet these sanitary and other objectives.

163

Wind tunnel tests of biodegradable fugitive dust suppressants being considered to reduce soil erosion by wind at radioactive waste construction sites  

Wind tunnel tests were performed of three fugitive dust control agents derived from potato and sugar beet products. These materials are being considered for use as dust suppressants to reduce the potential for transport of radioactive materials by wind from radioactive waste construction and remediation sites. Soil and dust control agent type, solution concentrations, application quantities, aging (or drying) conditions, surface disturbance, and wind and saltating sand eolian erosive stresses were selected and controlled to simulate application and exposure of excavated soil surfaces in the field. A description of the tests, results, conclusions, and recommendations are presented in this report. The results of this study indicate that all three dust control agents can protect exposed soil surfaces from extreme eolian stresses. It is also clear that the interaction and performance of each agent with various soil types may differ dramatically. Thus, soils similar to that received from ML should be best protected by high concentration ({approximately}2.5%) solutions of potato starch at low water application levels ({approximately}1 to 2 L/m{sup 2}). Because the effectiveness of PS on this soil type is degraded after a moderate amount of simulated rainfall, other options or additives should be considered if surfaces are to be protected for long intervals or during periods of intermittent rainfall and hot, windy conditions. On the other hand, XDCA should be considered when excavating sandy soils. It should be noted, however, that because the Hanford soil test results are based on a small number of tests, it would be prudent to perform additional tests prior to selecting a fugitive dust control agent for use at the Hanford Site. While fermented potato waste was not the best fixative used on either soil, it did perform reasonably well on both soil types (better than XDCA on Idaho soil and better than PS on Hanford soil).

164

Controlled particle removal from surfaces by electrodynamic methods for terrestrial, lunar, and Martian environmental conditions  

An Electrodynamic Dust Shield to remove already deposited micron-size particles from surfaces and to prevent the accumulation of such particles on surfaces has been developed. In addition to terrestrial application, our NASA laboratory is adapting this technology for the dusty and harsh environments of the Moon and Mars. The Apollo missions to the moon showed that lunar dust can hamper astronaut surface activities due to its ability to cling to most surfaces. NASA's Mars exploration landers and rovers have also shown that the problem is equally hard if not harder on Mars. In this paper, we show that an appropriate design can prevent the electrostatic breakdown at the low Martian atmospheric pressures. We are also able to show that uncharged dust can be lifted and removed from surfaces under simulated Martian environmental conditions. This technology has many potential benefits for removing dust from visors, viewports and many other surfaces as well as from solar arrays. We have also been able to develop a version of the electrodynamic dust shield working under hard vacuum conditions. This version should work well on the moon. We present data on the design and optimization of both types of dust shields as well substantial data on the clearing factors for transparent dust shields designed to protect solar panels for Martian exploration.

165

Quantifying non-star formation associated 8um dust emission in NGC 628  

Combining Ha and IRAC images of the nearby spiral galaxy NGC 628, we find that between 30-43% of its 8um dust emission is not related to recent star formation. Contributions from dust heated by young stars are separated by identifying HII regions in the Ha map and using these areas as a mask to determine the 8um dust emission that must be due to heating by older stars. Corrections are made for sub-detection-threshold HII regions, photons escaping from HII regions and for young stars not directly associated to HII regions (i.e. 10-100 Myr old stars). A simple model confirms this amount of 8um emission can be expected given dust and PAH absorption cross-sections, a realistic star-formation history, and the observed optical extinction values. A Fourier power spectrum analysis indicates that the 8um dust emission is more diffuse than the Ha emission (and similar to observed HI), supporting our analysis that much of the 8um-emitting dust is heated by older stars. The 8um dust-to-Ha emission ratio declines with gal...

166

Impact of vegetation and soil moisture seasonal dynamics on dust emissions over the Sahel  

To address the challenging issue of estimating mineral dust emissions from the semi-arid Sahel, a modeling approach is developed by combining two specific models: one dedicated to the simulation of the seasonal herbaceous layer in the Sahel (STEP) and the other to the estimation of dust emissions (MB). The area of interest is the Sahelian belt (12°N-20°N, 20°W-35°E) and the simulations were performed at a 0.25° spatial resolution over a 4-year period (2004-2007). The rainfall forcing is provided by a TRMM (Tropical Rainfall Measuring Mission) satellite-derived product; the other meteorological data are ECMWF products. An empirical parameterization is used to estimate the surface roughness and its temporal dynamics according to the characteristics of the simulated vegetation in terms of surface cover and height. Where no vegetation grows, the surface properties are considered as constant in time and are derived from the POLDER-1 satellite measurements. Simulations are constrained step by step by comparisons with observations. Simulated annual dust fluxes emitted from the whole area range from approximately 100 Mt to 400 Mt depending on the year, in good agreement with previous works dealing with Saharan dust emissions. For the fringe where herbaceous vegetation can affect dust emissions, the annual dust emission fluxes range between 0.5 Mt and 20 Mt depending on the year. Inhibition of dust emissions due to the seasonal dynamics of vegetation and surface soil moisture over this fringe varies between 20% and 35%.

167

Dust and the type II-Plateau supernova 2004dj  

We present mid-infrared (MIR) spectroscopy of a Type II-plateau supernova, SN 2004dj, obtained with the Spitzer Space Telescope, spanning 106--1393 d after explosion. MIR photometry plus optical/near-IR observations are also reported. An early-time MIR excess is attributed to emission from non-silicate dust formed within a cool dense shell (CDS). Most of the CDS dust condensed between 50 d and 165 d, reaching a mass of 0.3 x 10^{-5} Msun. Throughout the observations much of the longer wavelength (>10 microns) part of the continuum is explained as an IR echo from interstellar dust. The MIR excess strengthened at later times. We show that this was due to thermal emission from warm, non-silicate dust formed in the ejecta. Using optical/near-IR line-profiles and the MIR continua, we show that the dust was distributed as a disk whose radius appeared to be slowly shrinking. The disk radius may correspond to a grain destruction zone caused by a reverse shock which also heated the dust. The dust-disk lay nearly face-...

168

Synthetic monitoring of Asian dust from space, ground and/or simulations  

It is well known that the heavy soil dust has been transported from the China continent to Japan on westerly winds, especially in spring. It is also known that the increasing emissions of anthropogenic aerosols associated with continuing economic growth in Asia has caused serious air pollution over the wide range of East Asia. Accordingly the dust particles involve anthropogenic aerosols as well as soil dust. Thus aerosols in Asia are very complex due to mixing of small anthropogenic particles and large dust particles, which are called Asian dust. The satellite observation is an effective tool for global monitoring of the Asian dust. A new algorithm for detection of Asian dust from space is proposed based on the multispectral satellite (Terra/Aqua/MODIS) data. The derived space-based results are validated with the ground-based measurements and/or model simulations. The sun/sky photometry has been undertaken at NASA/AERONET stations at Higashi-Osaka in Japan, where the suspended particulate matter (SPM) sampling and NIES/LIDAR network equipment have been simultaneously working. In order to validate the satellite results with these surface-level data, an aerosol transportation model is available. In other word, the space-based and/or surface-based measurements are examined with the model simulations, and vice-versa.

169

Origins of Solar System Dust Beyond Jupiter  

The measurements of cosmic interplanetary dust by the instruments on board the Pioneer 10 and 11 spacecraft contain the dynamical signature of dust generated by Edgeworth-Kuiper Belt objects, as well as short period Oort Cloud comets and short period Jupiter family comets. While the dust concentration detected between Jupiter and Saturn is mainly due to the cometary components, the dust outside Saturn's orbit is dominated by grains originating from the Edgeworth-Kuiper Belt. In order to sustain a dust concentration that accounts for the Pioneer measurements, short period external Jupiter family comets, on orbits similar to comet 29P/Schwassmann-Wachmann-1, have to produce $8\\times 10^4:{\\rm g}:{\\rm s}^{-1}$ of dust grains with sizes between 0.01 and $6:{\\rm mm}$. A sustained production rate of $3\\times 10^5:{\\rm g}:{\\rm s}^{-1}$ has to be provided by short period Oort cloud comets on 1P/Halley-like orbits. The comets can not, however, account for the dust flux measured outside Saturn's orbit. The measurements...

170

INTERNATIONAL UNION OF OPERATING ENGINEERS NATIONAL HAZMAT PROGRAM - PORTER-CABLE CIRCULAR SAW OENHP: 2001-04, VERSION A  

Florida International University's (FIU) Hemispheric Center for Environmental Technology (HCET) evaluated five saws for their effectiveness in cutting specially prepared fiberglass-reinforced plywood crates. These crates were built as surrogates for crates that presently hold radioactively contaminated glove boxes at the Department of Energy's (DOE) Los Alamos facility. The Porter-Cable circular saw was assessed on August 15-16, 2001 (Porter-Cable No.1 and Porter-Cable No.2, respectively). During the FIU test of efficacy, a team from the Operating Engineers National Hazmat Program (OENHP) evaluated the occupational safety and health issues associated with this technology. The Porter-Cable saw is a straightforward machine for cutting wood of varying thickness. The blade is fully guarded with a fixed upper and a lower retractable guard. The lower guard retracts as the blade engages the work piece. The unit is operated with an on/off guarded trigger switch and is supported with a handgrip mounted near the front of the saw. The saw is equipped with a directional nozzle, which aims sawdust away from the operator and the line of cut. An optional vacuum system, attached to the directional nozzle, is used to remove and collect dust. During the demonstration of Porter-Cable No.1, personal noise sampling indicated that one worker was under and one was at the Occupational Safety and Health Administration's (OSHA) Action Level of 85 decibels (dBA) with time-weighted averages (TWA's) of 82.7 and 84.6 dBA, respectively. During the demonstration of Porter-Cable No.2, however, both workers did exceed the Action Level with TWA's of 89.7 and 90.0 dBA. These data are not entirely representative as they were gathered during a simulation and not at the actual worksite. Additional sampling should be conducted on-site, but the workers should wear hearing protection until it is determined that it is no longer necessary. The total nuisance dust sample for Porter-Cable No.1 was 3.53 milligrams per cubic meter (mg/m{sup 3}), which is lower than the OSHA Permissible Exposure Limit (PEL) of 15 mg/m{sup 3} and the American Conference of Governmental Industrial Hygienists' (ACGIH) Threshold Limit Value (TLV) of 10 mg/m{sup 3}. Porter-Cable No.2's nuisance dust results yielded a value of 22.05 mg/m{sup 3}, which is over the PEL and TLV. The fiber analysis for the first demonstration yielded 12.9 fibers per cubic centimeter (f/cc), which is much higher than the PEL of 1 f/cc. Galson Laboratories considered the fiber analysis for the second demonstration void due to the overloading of dust on the filter. Kickback, the sudden reaction to a pinched blade, is possible with this saw and could cause the saw to lift up and out of the work piece and toward the operator. Proper work position and firm control of the saw minimizes the potential for a sprain or strain. Care needs to be exercised to support the work piece properly and to not force the tool.

171

Reconstructing dust input to the Subarctic North Pacific - Past and Present  

The Subarctic North Pacific constitutes one of the high-nutrient-low chlorophyll (HNLC) regions of the modern ocean, where the biological pump is relatively inefficient at transferring carbon from the atmosphere to the deep sea. Iron limitation is traditionally suggested as the main controlling factor of biological production/the HNLC status of the Subarctic North Pacific, with iron thought to be primarily delivered by atmospheric dust transport from the East Asian desert areas. However, our understanding of the links between dust, biological production and climate is hampered by the lack of reliable dust flux records in the Subarctic North Pacific as well as longstanding discrepancies among specific techniques that have been used in previous research to reconstruct biological productivity. The lack of reliable dust flux reconstructions from North Pacific sediments is due a variety of reasons, among them sparsity of sediment cores, uncertain age control of the sediments as well as the impact of sediment input other than dust, such as hemipelagic and volcanic material as well as ice-rafted debris. Here, we map and compare spatial patterns of two proxies of eolian dust fluxes (230Thxs-normalized 232Th and 4He fluxes) as well as REE elements (e.g., La/Yb and Th/Sc ratios to deconvolve eolian and volcanic input to the sediments) from 37 multicore core-top sediments across the Subarctic North Pacific, obtained during the INOPEX cruise in 2009. We will present spatial patterns of these tracers to test their validity as proxies of mineral dust and to deconvolve dust and volcanic input to the sediments. The spatial patterns of the reconstructed dust fluxes will be compared to results of published reconstructions of modern dust trajectories to test the validity of these methods to capture modern dust flux patterns to the Subarctic North Pacific. The results from this study will be used for future research focusing on dust flux and productivity changes during the abrupt climate change sequence of the last deglaciation: the sequence from the cold and dusty Heinrich Stadial 1, through the dust-poor Bølling-Allerød warm period and a return to the near-glacial conditions of the Younger Dryas stadial. Ultimately, our results will allows us test the traditional hypothesis of eolian iron input primarily controlling the biological productivity in the Subarctic North Pacific and to evaluate how the Subarctic North Pacific's ecosystem responds to and mediates climate change.

172

Aging of mineral dust during transport from the Sahara into the Cape Verde area - results from airborne measurements during SAMUM  

The Saharan Mineral Dust Experiment (SAMUM) was conducted to better understand the properties of fresh and aged mineral dust. Within SAMUM, two field missions were performed: SAMUM-1 (summer 2006, Morocco) focused on the chemical, microphysical, optical and radiative properties of fresh dust aerosol in the vertical column over the Sahara, while SAMUM-2 (winter 2008, Cape Verde) concentrated on the properties of aged dust and the mixing of mineral dust with biomass burning aerosol. During both field experiments, the DLR Falcon research aircraft was equipped with an extensive set of aerosol instruments for size, volatility, and absorption measurements, impactor sampling for chemical analyses and with a nadir-looking High Spectral Resolution Lidar (HSRL). In the Cape Verde area, we found a complex stratification with dust covering the altitude range below 2 km and tropical biomass burning layers aloft. We show that the aerosol type of individual aerosol layers can be classified based on depolarization and lidar ratios and, in addition, on in situ measured Ångström exponents of absorption åap. The dust layers had a geometrical depth of 1.3 ± 0.4 km and showed a median åap of 3.95. The median effective diameter Deff was 2.5 ?m and the dust layers over Cape Verde yielded clear signals of aging: large particles were depleted due to gravitational settling and the accumulation mode diameter was shifted towards larger sizes as a result of coagulation. The tropical biomass layers had a depth of 2.0 ± 1.1 km and were characterized by a median åap of 1.34. They always contained a certain amount of large dust particles and showed a median Deff of 1.1 ?m and a fine mode Deff,fine of 0.33. The dust and biomass burning layers had a median aerosol optical depth (AOD) of 0.23 and 0.09, respectively. The median contributions of the dust and biomass burning layers to the AOD of the total atmospheric column below 10 km were 75 and 37%, respectively. We present the properties of aerosol layers in the Cape Verde region and compare the properties of aged dust with those of fresh dust observed close the Sahara. Changes in the size distribution during transport will be discussed and the impact of the changed size distribution on the radiation budget will be evaluated.

173

Emission, distribution, and transport of mineral dust in the Southern Hemisphere, and the dust deposition in Antarctica during present-day and the Last Glacial Maximum  

Mineral dust is an important component of the atmospheric aerosols in the Earth's climate system, but there are relatively few in-depth investigations of the emission, transport, distribution, and deposition of dust aerosols in the Southern Hemisphere (SH). These physical processes are crucial in climate studies, such as in the understanding of the 10--100 times higher dust concentrations in the Antarctic ice cores during the Last Glacial Maximum (LGM) compared with present-day, but are poorly understood. This dissertation conducts an in-depth investigation into the above areas, and addresses the following questions: (1) What are the characteristics of dust emission, distribution, atmospheric burden and deposition in the SH? (2) What are the contributions from the various continental sources? (3) Are there typical meteorological conditions associated with the transport of dust to the high-latitude SH? (4) What are the plausible causes for the observed high dust concentrations in Antarctic ice cores during the LGM? The methodology consists of three principal steps, using a combination of the Geophysical Fluid Dynamics Laboratory (GFDL) General Circulation Model (GCM) models, a trajectory model (HYSPLIT), and in situ and satellite observations. First, we investigate the dust cycle in the SH and quantify the contributions of the major sources by tagging dust based on its origin, using the GFDL GCM ("AM2.1n"). Second, the transport of the South American Patagonian dust to Antarctica is diagnosed by analyzing the GFDL model results together with results from the trajectory model simulations and using satellite observations. Third, sensitivity experiments are performed using AM2.1n to determine the sensitivity of the source characteristics, circulation, and precipitation on the dust deposition in Antarctic ice cores during the LGM. The results show that South America, Australia, and Northern Hemisphere are the main sources of the dust atmospheric burden in the SH, with Northern Hemisphere's contributing up to ˜40% over Antarctica. In the case of dust deposition, South America and Australia combine to contribute more than 85% in Antarctica. In the Antarctica, each source dominates half of a hemisphere along 120°E--60°W: the Pacific half is dominated by the Australian dust while the other half is dominated by the South American Patagonian dust. Trajectory analysis indicates that only 13--20% of air masses from Patagonia reach Antarctica, with ¼ of the air masses getting to West Antarctica in 4--5 days and the other ¾ reaching East Antarctica within 7 days. The transport to East Antarctica is driven by the low pressure systems moving eastward in the subpolar low-pressure zone, while southward transport to West Antarctica typically happens when a high pressure system over the Atlantic Ocean blocks depression in the Drake Passage. These two mechanisms are consistent with available satellite observations. For the LGM climate, the model simulations show that the expansion of source areas and changes in the Antarctic ice accumulation rates together can account for most of the observed increase of dust concentrations in the Vostok, Dome C and Taylor Dome cores, but there is an overestimate of the LGM-to-present ratio in the case of the Byrd core. The source expansion due to the lowering of sea level yields a factor of 2--3 higher contribution than that due to the reduction of continental vegetation. The changes in other climate parameters (e.g., SH precipitation change) are estimated to be relatively less important within the context of this sensitivity study, while the model-simulated LGM surface winds yield a 20--30% reduction rather than an increase in dust deposition in Antarctica. The outcomes of the research provide a fundamental understanding of the emission and distribution of dust in the SH and of the causes for the significant enhancement of the dust deposition in the Antarctic ice cores during the LGM.

174

Silicosis and bronchial cancer resulting from work in uranium mines  

After a man had worked underground in the uranium mines in Aue from his 41st to his 47th year of life, silicosis appeared when he was 57 and a bronchial carcinoma at the age of 66. The silicosis due to quartz dust and the bronchial carcinoma caused by ionizing radiation were recognized as occupational diseases in which compensation is due.

175

Volcanic loading: The dust veil index  

Dust ejected into the high atmosphere during explosive volcanic eruptions has been considered as a possible cause for climatic change. Dust veils created by volcanic eruptions can reduce the amount of light reaching the Earth`s surface and can cause reductions in surface temperatures. These climatic effects can be seen for several years following some eruptions and the magnitude and duration of the effects depend largely on the density or amount of tephra (i.e. dust) ejected, the latitude of injection, and atmospheric circulation patterns. Lamb (1970) formulated the Dust Veil Index (DVI) in an attempt to quantify the impact on the Earth`s energy balance of changes in atmospheric composition due to explosive volcanic eruptions. The DVI is a numerical index that quantifies the impact on the Earth`s energy balance of changes in atmospheric composition due to explosive volcanic eruptions. The DVI is a numerical index that quantifies the impact of a particular volcanic eruptions release of dust and aerosols over the years following the event. The DVI for any volcanic eruptions are available and have been used in estimating Lamb`s dust veil indices.

176

Thermo-Oxidation of Tokamak Carbon Dust  

The oxidation of dust and flakes collected from the DIII-D tokamak, and various commercial dust specimens, has been measured at 350 ºC and 2.0 kPa O2 pressure. Following an initial small mass loss, most of the commercial dust specimens showed very little effect due to O2 exposure. Similarly, dust collected from underneath DIII-D tiles, which is thought to comprise largely Grafoil™ particulates, also showed little susceptibility to oxidation at this temperature. However, oxidation of the dust collected from tile surfaces has led to ~ 18% mass loss after 8 hours; thereafter, little change in mass was observed. This suggests that the surface dust includes some components of different composition and/or structure – possibly fragments of codeposited layers. The oxidation of codeposit flakes scraped form DIII-D upper divertor tiles showed an initial 25% loss in mass due to heating in vacuum, and the gradual loss of 30-38% mass during the subsequent 24 hours exposure to O2. This behavior is significantly different from that observed for the oxidation of thinner DIII-D codeposit specimens which were still adhered to tile surfaces, and this is thought to be related to the low deuterium content (D/C ~ 0.03 – 0.04) of the flakes.

177

Episodic Post-Shock Dust Formation in the Colliding Winds of Eta Carinae  

Eta Carinae shows broad peaks in near-infrared (IR) JHKL photometry, roughly correlated with times of periastron passage in the eccentric binary system. After correcting for secular changes attributed to reduced extinction from the thinning Homunculus Nebula, these peaks have IR spectral energy distributions (SEDs) consistent with emission from hot dust at 1400-1700 K. The excess SEDs are clearly inconsistent, however, with the excess being entirely due to free-free wind or photospheric emission. One must conclude, therefore, that the broad near-IR peaks associated with Eta Carinae's 5.5 yr variability are due to thermal emission from hot dust. I propose that this transient hot dust results from episodic formation of grains within compressed post-shock zones of the colliding winds, analogous to the episodic dust formation in Wolf-Rayet binary systems like WR140 or the post-shock dust formation seen in some supernovae like SN2006jc. This dust formation in Eta Carinae seems to occur preferentially near and afte...

178

Numerical simulations of Asian dust storms using a coupled climate-aerosol microphysical model  

We have developed a three-dimensional coupled microphysical/climate model based on the National Center for Atmospheric Research Community Atmospheres Model and the University of Colorado/NASA Community Aerosol and Radiation Model for Atmospheres. We have used the model to investigate the sources, removal processes, transport, and optical properties of Asian dust aerosol and its impact on downwind regions. The model simulations are conducted primarily during the time frame of the Aerosol Characterization Experiment-Asia field experiment (March-May 2001) since considerable in situ data are available at that time. Our dust source function follows Ginoux et al. (2001). We modified the dust source function by using the friction velocity instead of the 10-m wind based on wind erosion theory, by adding a size-dependent threshold friction velocity following Marticorena and Bergametti (1995) and by adding a soil moisture correction. A Weibull distribution is implemented to estimate the subgrid-scale wind speed variability. We use eight size bins for mineral dust ranging from 0.1 to 10 ?m radius. Generally, the model reproduced the aerosol optical depth retrieved by the ground-based Aerosol Robotic Network (AERONET) Sun photometers at six study sites ranging in location from near the Asian dust sources to the Eastern Pacific region. By constraining the dust complex refractive index from AERONET retrievals near the dust source, we also find the single-scattering albedo to be consistent with AERONET retrievals. However, large regional variations are observed due to local pollution. The timing of dust events is comparable to the National Institute for Environmental Studies (NIES) lidar data in Beijing and Nagasaki. However, the simulated dust aerosols are at higher altitudes than those observed by the NIES lidar.

179

Long-range transport of Saharan dust over northwestern Europe during EUCAARI 2008 campaign: Evolution of dust optical properties by scavenging  

The evolution of dust optical properties is illustrated in this paper through a case of long-range transport of Saharan dust over northwestern Europe during the European Integrated Project on Aerosol-Cloud-Climate and Air Quality Interactions (EUCAARI) experimental campaign in 2008. This spread of dust over northwestern Europe is investigated by combining satellite, airborne, ground-based observations and the non-hydrostatic meso-scale model Meso-NH. The total dust amount emitted during the study period is estimated to 185 Tg. The analysis of the removal processes reveals that only 12.5 Tg is lost by dry deposition, and that wet deposition is the main process of dust removal (73 Tg). The observed aerosol optical thickness ranged from 0.1 to 0.5 at the wavelength of 440 nm, with a maximum value close to 1 is found over the Netherlands (51.97°N, 4.93°E). Over that site, the main dust layer is located between 2.5 and 5.2 km above sea level (asl), moreover dust was also present at 0.9 km asl. The nephelometer measurements on board the ATR-42 aircraft revealed a strong wavelength dependence of the scattering coefficient over the Netherlands. The Angström exponent is greater than 0.5, whereas usually it approaches zero in presence of Saharan dust. This is due to high precipitation scavenging efficiency for the coarse mode, particularly below 4 km. Our results confirm that atmospheric conditions govern the life cycle of dust microphysical phenomena, providing conditions for transformation processes during transport, and removal of particles from the atmosphere.

180

Detailed cloud resolving model simulations of the impacts of Saharan air layer dust on tropical deep convection - Part 1: Dust acts as ice nuclei  

Observational studies suggest that the Saharan Air Layer (SAL), an elevated layer (850-500 hPa) of Saharan air and mineral dust, has strong impacts on the microphysical as well as dynamical properties of tropical deep convective cloud systems along its track. In this case study, numerical simulations using a two-dimensional Detailed Cloud Resolving Model (DCRM) were carried out to investigate the dust-cloud interactions in the tropical deep convection, focusing on the dust role as Ice Nuclei (IN). The simulations showed that mineral dust considerably enhanced heterogeneous nucleation and freezing at temperatures warmer than -40 °C, resulting in more ice hydrometeors number concentration and reduced precipitating size of ice particles. Because of the lower in the saturation over ice as well as more droplet freezing, total latent heating increased, and consequently the updraft velocity was stronger. On the other hand, the increased ice deposition consumed more water vapor at middle troposphere, which induces a competition for water vapor between heterogeneous and homogeneous freezing and nucleation. As a result, dust suppressed the homogeneous droplet freezing and nucleation due to the heterogeneous droplet freezing and the weakened transport of water vapor at lower stratosphere, respectively. These effects led to decreased number concentration of ice cloud particles in the upper troposphere, and consequently lowered the cloud top height during the stratus precipitating stage. Acting as IN, mineral dust also influenced precipitation in deep convection. It initiated earlier the collection because dust-related heterogeneous nucleation and freezing at middle troposphere occur earlier than homogeneous nucleation at higher altitudes. Nevertheless, the convective precipitation was suppressed by reduced collection of large graupel particles and insufficient fallout related to decreased sizes of precipitating ice hydrometeors. On the contrary, dust increased the precipitation in stratiform precipitation through deposition growth. Overall, the comprehensive effects of mineral dust suppressed the precipitation by up to 22%.

 
 
 
 
181

Two evolutional paths of an axisymmetric gravitational instability in the dust layer of a protoplanetary disk  

Nonlinear numerical simulations are performed to investigate the density evolution in the dust layer of a protoplanetary disk due to the gravitational instability and dust settling toward the midplane. We assume the region where the radial pressure gradient at equilibrium is negligible so that the shear-induced instability is avoided, and also restrict to an axisymmetric perturbation as a first step of nonlinear numerical simulations of the gravitational instability. We find that there are two different evolutional paths of the gravitational instability depending on the nondimensional gas friction time, which is defined as the product of the gas friction time and the Keplerian angular velocity. If the nondimensional gas friction time is equal to 0.01, the gravitational instability grows faster than dust settling. On the other hand, if the nondimensional gas friction time is equal to 0.1, dust aggregates settle sufficiently before the gravitational instability grows. In the latter case, an approximate analytic...

182

Environmental relevant heavy metals in dust particles and ground dust of a garbage compost plant with integrated incinerator  

During August and November 1984 dust particles and ground dust were collected in a communal garbage compost plant. The samples were analysed for the elements zinc, copper, manganese, chromium, nickel, cadmium, lead and mercury by means of atomic absorption spectrometry. In further investigations the lead intoxication of the employees of this plant should be pointed out. For the assessment of the concentration values of the dust as well as of the heavy metals the MAK-, TRK- and BAT-rules have been used for comparison. The results show that there exists certain dust and heavy metal capacities in this garbage compost plant which are below the above cited standards but nevertheless should be taken into account due to the health of the employees. (orig./PW).

183

Ion-acoustic solitons in dusty plasma  

The dynamics of dust ion-acoustic solitons is analyzed in a wide range of dusty plasma parameters. The cases of both a positive dust grain charge arising due to the photoelectric effect caused by intense electromagnetic radiation and a negative grain charge established in the absence of electromagnetic radiation are considered. The ranges of plasma parameters and Mach numbers in which ?conservative? (nondissipative) solitons can exist are determined. It is shown that, in dusty plasma with negatively charged dust grains, both compression and rarefaction solitons can propagate, whereas in plasma with positively charged dust grains, only compression solitons can exist. The evolution of soliton-like compression and rarefaction perturbations is studied by numerically solving the hydrodynamic eq...

184

Solar flare track densities in interplanetary dust particles The determination of an asteroidal versus cometary source of the zodiacal dust cloud  

The possibility is explored whether an IDP (interplanetary dust particle) is cometary or asteroidal from measurements of the solar flare track density within its constituent mineral grains. Dust particles that are larger than 1 micron, when injected into the Solar System from comets and asteroids, will spiral into the sun due to the Poynting-Robertson effect. During the process of spiraling in, such dust particles accumulate solar flare tracks. The accumulated track density for a given dust grain is a function of the duration of its space exposure and its distance from the sun. Using a computer model, it was determined that the expected track density distributions from grains produced by comets are very different from those produced by asteroids. Individual asteroids produce populations of particles that arrive at 1 AU with scaled track density distributions containing spikes, while comets supply particles with a flatter and wider distribution of track densities. 36 references.

185

Interstellar Grains  

Our current understanding of interstellar dust is summarized at an introductory level. Submicron-sized interstellar dust grains absorb and scatter light, and reradiate the absorbed energy in the infrared. The grain population spans a range of sizes, from molecules containing only tens of atoms, to particles containing 10^{10} atoms. Most of the grain mass appears to be due to two types of solid, in approximately equal amounts: amorphous silicate mineral, and carbonaceous material. Approximately 2/3 of the interstellar carbon in diffuse clouds is in solid form. Interstellar grains are important for many reasons: they obscure our view (in a wavelength-dependent manner); the infrared emission from dust provides a valuable probe of dense regions; and because dust grains play a central role in interstellar chemistry, gas dynamics, and heating and cooling of interstellar gas.

186

Polarisation properties of comet NEAT C/2001 Q4  

Comets exhibit high (up to 25 %) amount of optical polarization when they are observed through ground based or space telescopes. These polarizations are caused due to the scattering of cometary dust. The observed linear polarisation of comets is generally a function of the wavelength of incident light (?), the scattering angle (?), the geometrical shape and size of the particle and the composition of dust particles in terms of the complex values of the refractive index. The scattering properties of cometary dust will help to know the nature of cometary dust. In the present work, the observed linear polarization data of Comet NEAT are studied through simulations using Ballistic Particle-Cluster Aggregate (BPCA) and Ballistic Cluster-Cluster Aggregate (BCCA). Using Superposition T-matrix cod...

187

Comparing modeled and observed changes in mineral dust transport and deposition to Antarctica between the Last Glacial Maximum and current climates  

Mineral dust aerosols represent an active component of the Earth?s climate system, by interacting with radiation directly, and by modifying clouds and biogeochemistry. Mineral dust from polar ice cores over the last million years can be used as paleoclimate proxy, and provide unique information about climate variability, as changes in dust deposition at the core sites can be due to changes in sources, transport and/or deposition locally. Here we present results from a study based on climate model simulations using the Community Climate System Model. The focus of this work is to analyze simulated differences in the dust concentration, size distribution and sources in current climate conditions and during the Last Glacial Maximum at specific ice core locations in Antarctica, and compare with...

188

The Keck Aperture Masking Experiment: Dust Enshrouded Red Giants  

While the importance of dusty asymptotic giant branch (AGB) stars to galactic chemical enrichment is widely recognised, a sophisticated understanding of the dust formation and wind-driving mechanisms has proven elusive due in part to the difficulty in spatially-resolving the dust formation regions themselves. We have observed twenty dust-enshrouded AGB stars as part of the Keck Aperture Masking Experiment, resolving all of them in multiple near-infrared bands between 1.5 microns and 3.1 microns. We find 45% of the targets to show measurable elongations that, when correcting for the greater distances of the targets, would correspond to significantly asymmetric dust shells on par with the well-known cases of IRC+10216 or CIT6. Using radiative transfer models, we find the sublimation temperature of 1130 +- 90 K and 1170 +- 60 K for silicates and amorphous carbon respectively, both somewhat lower than expected from laboratory measurements and vastly below temperatures inferred from the inner edge of YSO disks. Th...

189

Propagation of the three-dimensional dust acoustic solitons in magnetized quantum plasmas with dust polarity effect  

The quantum hydrodynamical model is employed to investigate the nonlinear properties of the quantum dust acoustic waves in a magnetized dusty plasma composed of inertialess electrons, ions, and mobile positive/negative charged dust particles. For this purpose, a quantum Zakharov-Kuznetsov equation is derived and the basic features of the electrostatic excitations are investigated by applying the direct method. It is found that positive and negative bell-shaped solitary pulses become explosive pulses depending mainly upon the angles of propagation and dust polarity. Furthermore, the effects due to nondimensional quantum parameter and the external magnetic field are examined on the width of the quantum dust acoustic solitary pulses. The relevance of the present results to semiconductor quantum wells is mentioned.

190

Regional modelling of Saharan dust and biomass-burning smoke  

Abstract The direct radiative forcing and dynamic atmospheric response due to Saharan dust and biomass-burning aerosol particles are presented for a case study during the SAMUM-2 field campaign in January and February 2008. The regional model system COSMO-MUSCAT is used. It allows online interaction of the computed dust and smoke load with the solar and terrestrial radiation and with the model dynamics. Model results of upward solar irradiances are evaluated against airborne radiation measurements in the Cape Verde region. The comparison shows a good agreement for the case of dust and smoke mixture. Dust and smoke particles influence the atmospheric dynamics by changing the radiative heating rates. The related pressure perturbations modify local and synoptic scale air-flow patterns. In the...

191

Collective analysis of pharmaceutical dust explosion testing data  

Abstract Dust explosions in the process industries have recently been highlighted due to a number of high profile incidents. These explosions can be very powerful and destructive, and the lack of awareness of the hazards is often cited as a root cause in incident investigations. Although specific test data about some widely handled dusts have been compiled in some references, the availability for most materials handled in the pharmaceutical industry is less common. Pharmaceutical powders are chemically rich for combustion, but quantities available for testing are often limited. This work summarizes some of the historical dust explosion data from samples tested at Abbott. Observations of this data provide insight into the explosion behavior of pharmaceutical dusts, provide a basis for equip...

192

Reading the climate record of the martian polar layered deposits  

The martian polar regions have layered deposits of ice and dust. The stratigraphy of these deposits is exposed within scarps and trough walls and is thought to have formed due to climate variations in the past. Insolation has varied significantly over time and caused dramatic changes in climate, but it has remained unclear whether insolation variations could be linked to the stratigraphic record. We present a model of layer formation based on physical processes that expresses polar deposition rates of ice and dust in terms of insolation. In this model, layer formation is controlled by the insolation record, and dust-rich layers form by two mechanisms: (1) increased summer sublimation during high obliquity, and (2) variations in the polar deposition of dust modulated by obliquity variations...

193

Dead Zones and the Diversity of Exoplanetary Systems  

Planetary migration provides a theoretical basis for the observed diversity of exoplanetary systems. We demonstrate that dust settling - an inescapable feature of disk evolution - gives even more rapid type I migration by up to a factor of about 2 than occurs in disks with fully mixed dust. On the other hand, type II migration becomes slower by a factor of 2 due to dust settling. This even more problematic type I migration can be resolved by the presence of a dead zone; the inner, high density region of a disk which features a low level of turbulence. We show that enhanced dust settling in the dead zone leaves a dusty wall at its outer edge. Back-heating of the dead zone by this wall produces a positive radial gradient for the disk temperature, which acts as a barrier for type I migration.

194

Outgassing of icy bodies in the solar system - I. The sublimation of hexagonal water ice through dust layers  

Our knowledge about the physical processes determining the activity of comets were mainly influenced by several extremely successful space missions, the predictions of theoretical models and the results of laboratory experiments. However, novel computer models should not be treated in isolation but should be based on experimental results. Therefore, a new experimental setup was constructed to investigate the temperature dependent sublimation properties of hexagonal water ice and the gas diffusion through a dry dust layer covering the ice surface. We show that this experimental setup is capable to reproduce known gas production rates of pure hexagonal water ice. The reduction of the gas production rate due to an additional dust layer on top of the ice surface was measured and compared with the results of another experimental setup in which the gas diffusion through dust layers at room temperature was investigated. We found that the relative permeability of the dust layer is inversely proportional to its thickn...

195

Rapid microbial stabilization of unconsolidated sediment against wind erosion and dust generation  

Purpose Mineral dust pollution is a concern for human health due to the reaction of mineral particles in the organism and their role as pathogen carriers. Human activity generates unconsolidated sediments that become a dust source. This study investigates the effect of microbial growth on dust stabilization through aggregation in order to help alleviate this problem. Materials and methods Four representative potential dust sources (volcanic ash, carbonate, mine waste, and diatomaceous earth) and three organic nutrients (humic acids, glucose?+?peptone and yeast extract) were selected. We used the indigenous microbial communities in the mineral samples, rain and tap water. All experiments were carried out in Petri dishes, in moist conditions. The experiments were illuminated artificially for...

196

Tomography of the Heliosphere: Ulysses Dust Measurements  

We report on the modeling of the motion of interstellar dust particles through the heliosphere and compare these calculations with the Ulysses observations. While the flux and direction of interstellar dust particles are expected to be constant, the Ulysses measurements show that both area function of time. The observed variability has been suggested to be related to the configuration of the magnetic fields in the heliosphere. Since the observed dust particles travel for about 20 years from interstellar space to the inner solar system, they experience electromagnetic perturbations due the heliospheric magnetic fields through almost two complete solar cycles. Matching the modeled and measured dust fluxes is an excellent indicator of the validity of our models of the history and large-scale structure of magnetic fields in the heliosphere.

197

Soil Properties Database of Spanish Soils. Volumen XI.- Castilla-Leon (b) : Palencia, Valladolid and Avila.  

The soil vulnerability determines the sensitivity of the soil after an accidental radioactive contamination due to Cs-137 and Sr-90. The Departamento de Impacto Ambiental de la Energia of CIEMAT is carrying out an assessment of the radiological vulnerabil...

198

5  

Monte Carlo codes with similar capabilities have ..... are used to simulate the delayed energy deposits due to radioactive decays in the instrument. .... the actual discrete nuclear levels and the well-know selection rules for transitions between ...

199

Determination of heavy metals in indoor dust from Istanbul, Turkey: Estimation of the health risk.  

Levels of eight potentially toxic heavy metals in indoor dust from homes and offices in Istanbul were investigated. The concentrations of heavy metals in indoor dust from homes+office ranged from 62 to 1800?gg(-1) for Cu, 3-200?gg(-1) for Pb, 0.4-20?gg(-1) for Cd, 210-2800?gg(-1) for Zn, 2.8-460?gg(-1) for Cr, 8-1300?gg(-1) for Mn, 2.4-25?gg(-1) for Co, 120-2600?gg(-1) for Ni. Results of the study were comparable to other studies conducted on indoor dust and street dust from a variety of cities globally. Considering only ingestion + inhalation, the carcinogenic risk level of Cr for adults and children (3.7×10(-5) and 2.7×10(-5)) in Istanbul was in the range of EPA's safe limits (1×10(-6) and 1×10(-4)), indicating that cancer risk of Cr due to exposure to indoor dust in Istanbul can be acceptable. According to calculated Hazard Quotient (HQ), for non-cancer effects, the ingestion of indoor dust appears to be the major route of exposure to the indoor dust that results in a higher risk for heavy metals, followed by dermal contact and inhalation pathways. However, compared to ingestion and dermal contact exposure, exposure through inhalation is almost negligible. Hazard Index (HI) values for all studied elements were lower than safe limit of 1 and this result suggested that none of the population groups would likely to experience potential health risk due to exposure to heavy metals from indoor dust in the study area. PMID:23073482

200

Influence of dust storms on the aerosol optical properties over the Indo-Gangetic basin  

Dust storms are considered natural hazards, which affect day-to-day life for a short time from a few hours to a few days. They are common in India especially in the western Rajasthan Province, which is covered by the Thar Desert. In this paper, we present the effects of the dust events on the aerosol parameters retrieved over Kanpur (located in heart of the Indo-Gangetic basin) from ground-based Aerosol Robotic Network (AERONET) measurements. The aerosol parameters show strong seasonal variability in this region, with least spectral dependence of aerosol optical depth (AOD) during the premonsoon season, characterized by dust loading. The aerosol optical properties over the Indo-Gangetic basin are controlled by the diurnal and seasonal cycles of urban pollutants, but the dust storms are so significant that the local cycle is completely overshadowed. A rise in AOD by more than 50% and corresponding decrease in angstrom parameter by 70-90% have been observed after each dust event. The diurnal variations of AOD during the dust events have been found to be controlled by the onset of the dust storms. The changes in the single scattering albedo (SSA) and real n(?) and imaginary k(?) parts of the refractive index indicate that the 27 May 2002 event influences the optical state to be absorbing, whereas for the other four events the aerosols are found to be dominantly scattering in nature. SSA has been found to increase sharply at higher wavelengths (? > 440 nm) during the dust events, whereas n(?) and k(?) increase 2-3 times more at ? = 440 nm compared to those at higher wavelengths. The contrasting change in the spectral variations of the optical properties is due to the difference in the nature of the aerosols loading during the events. Aerosol volume concentration at coarse mode is found to increase three times after the dust events, whereas no significant change has been observed in the volume concentration at fine mode. Concentration of the particulate matters less than 10 ?m (PM10) is also found to increase by ~150 ?g m-3 after each dust event except on the 27 May 2002 event, when heavy rainfall after the dust storm washed out the suspended particulate matters from the atmosphere, and the ground level PM10 concentration was not influenced by the advected dust particles on that day. Aerosol index values in successive Total Ozone Mapping Spectrometer (TOMS) images over the region support the characterization of the aerosols in this region in terms of their optical properties, which are being transported over the Indo-Gangetic basin from the western Thar Desert and the Gulf regions depending upon the size of the particles, shown by the air mass trajectories.

 
 
 
 
201

Actively accumulating dust changes phosphorus abundance and fractionation in soils and tree foliage in a super-humid, high leaching environment, West Coast, New Zealand  

Pedogenesis in humid climates, as found in chronosequence studies, ultimately leads to nutrient depletion and enhanced formation of secondary, less plant-available forms of nutrients with progressing time. Deposition of mineral dust has been shown to be an important process to mitigate such depletion in soils and ecosystems (e.g. Hawaii, Amazon Basin). However, the magnitude of its effect has hardly been quantified and little is known about the accession pathways. This study exploits a unique geomorphic setting of a Holocene sequence of sand dune ridges. This sequence combines an active dust flux gradient along the dunes downwind of a braided riverbed and, distal from the dust source, a chronosequence across the dunes (170-6500 y). Pedogenesis is very rapid with Spodosols developing after 1000 y under a thick organic root mat. Comparison of soil and ecosystem phosphorus (P) across the chronosequence and along the dust gradient on the 6500 y dune allows us to quantify the capacity of active dust deposition to alter the P pool and to determine the biogeochemical pathways by which P fluxes are assimilated under super-humid, high leaching conditions. Across both gradients, we quantified the P concentrations in tree foliage and the P fractions in the upper 50 cm of the soils (total P, organic P, apatite P, occluded P, non-occluded P), including solution 31P NMR spectroscopy of organic P in selected profiles. Soil P across the chronosequence follows the P evolution model of Walker and Syers (1976) - a 75% decline of total P within 6500 y due to strong leaching losses of apatite P (82% loss) coinciding with an increase in secondary P forms. Along the dust gradient, increasing eolian deposition towards the river from ~1000 m distance is associated with a decline of apatite P and an increase of organic P. Foliar P mirrors the total P and apatite P decline of the soils across the chronosequence with a steep decrease after 1000 y. Along the dust gradient, foliar P correlates with deposition rates and organic P. This positive correlation of dust deposition rates and organically bound P, and the concomitant negative correlation with apatite P, requires biological transformation of the mineral P in the dust prior to the dust being incorporated into the soil. We suggest a rapid assimilation of dust-derived mineral P by plants within the organic root mat and a conversion into organic P as part of the living biomass, finally returned to the soil with the dead biomass. We will also present results from 31P NMR spectroscopy to qualitatively discriminate between organic P in soils formed under high dust flux and organic P in soils derived only from in situ dune sand parent material.

202

Planck early results. XVII. Origin of the submillimetre excess dust emission in the Magellanic Clouds  

The integrated spectral energy distributions (SED) of the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) appear significantly flatter than expected from dust models based on their far-infrared and radio emission. The still unexplained origin of this millimetre excess is investigated here using the Planck data. The integrated SED of the two galaxies before subtraction of the foreground (Milky Way) and background (CMB fluctuations) emission are in good agreement with previous determinations, confirming the presence of the millimetre excess. In the context of this preliminary analysis we do not propose a full multi-component fitting of the data, but instead subtract contributions unrelated to the galaxies and to dust emission. The background CMB contribution is subtracted using an internal linear combination (ILC) method performed locally around the galaxies. The foreground emission from the Milky Way is subtracted as a Galactic Hi template, and the dust emissivity is derived in a region surrounding the two galaxies and dominated by Milky Way emission. After subtraction, the remaining emission of both galaxies correlates closely with the atomic and molecular gas emission of the LMC and SMC. The millimetre excess in the LMC can be explained by CMB fluctuations, but a significant excess is still present in the SMC SED. The Planck and IRAS-IRIS data at 100 ?m are combined to produce thermal dust temperature and optical depth maps of the two galaxies. The LMC temperature map shows the presence of a warm inner arm already found with the Spitzer data, but which also shows the existence of a previously unidentified cold outer arm. Several cold regions are found along this arm, some of which are associated with known molecular clouds. The dust optical depth maps are used to constrain the thermal dust emissivity power-law index (?). The average spectral index is found to be consistent with ? = 1.5 and ? = 1.2 below 500?m for the LMC and SMC respectively, significantly flatter than the values observed in the Milky Way. Also, there is evidence in the SMC of a further flattening of the SED in the sub-mm, unlike for the LMC where the SED remains consistent with ? = 1.5. The spatial distribution of the millimetre dustexcess in the SMC follows the gas and thermal dust distribution. Different models are explored in order to fit the dust emission in the SMC. It is concluded that the millimetre excess is unlikely to be caused by very cold dust emission and that it could be due to a combination of spinning dust emission and thermal dust emission by more amorphous dust grains than those present in our Galaxy. © ESO, 2011.

203

Uptake of HNO3 to Deliquescent Sea-Salt and Mineral Dust Aerosol Particles  

Uptake of HNO3 to aerosol particles is an important removal pathway of nitrogen oxides in the troposphere. Uptake of HNO3 to deliquescent sea-salt aerosol particles was studied in an aerosol flow reactor. Submicron sea-salt particles were used to avoid diffusion limitation in the gas-phase at atmospheric pressure. To overcome the sensitivity problems associated with low amount of reactants processed in such low aerosol masses, we used the short-lived radioactive tracer 13N to label the trace gas molecules at very low concentration. Uptake of HNO3 to deliquescent sea-salt particles was studied under a wide range of HNO3 concentration. Between 1 and 60 ppbv, the uptake coefficient was constant at 0.5+/-0.2 within the first few seconds, whereas at higher concentrations of about 600ppbv, the uptake coefficient rapidly dropped to 0.1 after about 1 second. This drop was due to complete release of chloride as HCl. The equilibrium conditions for these experiments were explored using the North American Aerosol Inorganics (AIM) model, which accounts for the activities of the concentrated solution of the deliquescent aerosol. It is concluded that the rates of uptake at low concentration were limited by the mass accommodation coefficient as both the diffusion in the liquid phase or the rate of release of HCl were not rate limiting. Using an identical approach, we started to investigate the uptake of HNO3 to mineral dust aerosol particles in a similar flow reactor, and first results will be presented. References Ammann, M, Using 13N as tracer in heterogeneous atmospheric chemistry experiments, Radiochim. Acta., 89, 831-838, 2001 Guimbaud, C., F., Arens, L., Gutzwiller, H.W, Gäggeler, and M. Ammann, Uptake of HNO3 to Deliquescent Sea-Salt Aerosol Particles, Atmos. Chem. Phys. Discuss., 2, 739-763, 2002

204

Disposal of coal combustion residues in terrestrial systems: contamination and risk management.  

The world's ever-growing energy demand will lead to the installation of new coal-fired power plants. At least part of the coal combustion residue (CCR) generated in the coming years will be disposed of, adding to the large number of CCR disposal sites generated in the past and reinforcing the need for sound assessment and management of associated risks. Physical and chemical composition of CCR varies considerably depending on the quality of the feed coal, the combustion technology, fraction considered, and the method of disposal. Related risk pathways include (i) aerial routes, i.e., dust resuspension (Cr(VI)), emanation of radioactivity (Rn associated with U and Th series), and Hg volatilization threatening animal and human health; (ii) phytoaccumulation (B, Se, Mo, As) and plant toxicity (B) with subsequent effects on animals (e.g., Mo-induced hypocuprosis, As and Se toxicity) and humans (e.g., selenosis; food chain); and (iii) effluent discharge and percolation to groundwater and rivers (suspended solids, unfavorable pH, high Se, B, Hg, and As(III) concentrations). Recent and projected changes of CCR composition due to emerging clean coal technologies require close monitoring as the concentration of volatile elements such as Hg and Se, solubility (Hg, Cd, Cu) and volatilization (Hg, NH(3)) of some pollutants are likely to increase because of higher retention in certain fractions of CCRs and concurrent changes in pH (e.g., by mineral carbonation) and NH(3) content. These changes require additional research efforts to explore the implications for CCR quality, use, and management of risk associated with disposal sites. PMID:20400572

205

Clementine Observations of the Zodiacal Light and the Dust Content of the Inner Solar System  

Using the Moon to occult the Sun, the Clementine spacecraft used its navigation cameras to map the inner zodiacal light at optical wavelengths over elongations of 3 approx. less than epsilon approx. less than 30 deg from the Sun. This surface brightness map is then used to infer the spatial distribution of interplanetary dust over heliocentric distances of about 10 solar radii to the orbit of Venus. The averaged ecliptic surface brightness of the zodiacal light falls off as Z(epsilon) is a member of epsilon(sup -2.45 +/- 0.05), which suggests that the dust cross-sectional density nominally falls off as sigma(r) is a member of r(sup - 1.45 +/- 0.05). The interplanetary dust also has an albedo of alpha approx. = 0.1 that is uncertain by a factor of approx. 2. Asymmetries of approx. 10% are seen in directions east-west and north-south of the Sun, and these may be due the giant planets' secular gravitational perturbations. We apply a simple model that attributes the zodiacal light as due to three dust populations having distinct inclination distributions, namely, dust from asteroids and Jupiter-family comets (JFCs) having characteristic inclinations of i approx. 7 deg, dust from Halley-type comets having i approx. 33 deg, and an isotropic cloud of dust from Oort Cloud comets. The best-fitting scenario indicates that asteroids + JFCs are the source of about 45% of the optical dust cross section seen in the ecliptic at 1 AU but that at least 89% of the dust cross section enclosed by a 1-AU-radius sphere is of a cometary origin. Each population's radial density variations can also deviate somewhat from the nominal sigma(r) is a member of r(sup -1.45). When these results are extrapolated out to the asteroid belt, we find an upper limit on the mass of the light-reflecting asteroidal dust that is equivalent to a 12-km asteroid, and a similar extrapolation of the isotropic dust cloud out to Oort Cloud distances yields a mass equivalent to a 30-km comet, although the latter mass is uncertain by orders of magnitude.

206

Report of radioactivity survey research in fiscal year 1998  

In National Institute of Radiological Sciences, a survey was made on radioactivities in the environment due to the substances released from nuclear installations and radioactive fall-out brought out by nuclear explosion tests since 1959. As the marked progress of non-military utilization of nuclear energy the national concern on environmental radioactivity has been increasing in Japan and thus it has become more and more important to make a survey research of radioactivities, which might affect the environment and human health. In these situations, the institute attempted to make the following six surveys in the fiscal year of 1998; 'a survey on radioactive levels in environment, foods and human bodies', 'survey on the radioactive level in the regions around nuclear installations', 'works in radioactive data center', 'fundamental survey on the evaluation of the results from radioactivity survey', 'workshop for technical experts of environmental radioactivity monitoring' and 'survey research on the measurement and countermeasures for emergency exposure'. (J.P.N.)

207

Effects of operating conditions on dust cake behavior in filters with high surface-to-volume ratios  

Generally, new filter elements with large S/V ratios typically have inlet passages with a small cross sectional area to reach a large filter surface area internal to the filter element. To prevent plugging of the inlet passages, or to prevent the filter passage inlet velocity from becoming dangerously high causing cake disturbance, the high S/V filter can only accommodate a very thin cake. The conventional backpulse cleaning technique may not be able to dislodge this thin cake. The multi-tier design using ceramic candles can tolerate a thick dust cake. The conventional back-pulse cleaning technique could then be used to remove the dust cake. However, due to the proximity of the neighboring tiers, the large-volume flow of the back-pulse mixing with a huge quantity of dislodged dust cake could potentially perturb the local flow distribution from its initially well-mixed uniform flow and dust concentration. As soon as one spot or patch of dust cake forms on the neighboring candle surface due to this redistributed nonuniform flow and dust concentration, patching dust redeposition will occur on the neighboring tiers, leading eventually to ash bridging. This is because the rigid ceramic candle, unlike the fabric filter, does not flex during back-pulse cleaning; therefore, it cannot tolerate the uneven flow distribution. The back-pulse flow universally seeks the least resistance path, resulting in an uneven or patchy cleaning. Ash bridging is known to cause ceramic candle breakage due to the pulse ratchet problem. To understand the back-pulse cleaning problem caused by the use of high S/V rigid filter elements or the implementation of a multi-tier design, a bench-scale, two-dimensional (2-D) cold flow filter test facility is being constructed, and is scheduled for shakedown and testing in July 1993.

208

Characterizing adult human nasal airway dimensions  

Respiratory tract models used in calculating radiation dose from exposure to inhaled radioactive aerosols have only recently focused attention on the importance of the nasal airways (NAs). Because the NAs are the first tissues of the respiratory tract available for aerosol deposition in normally nose-breathing people, any deposition of aerosol in this anatomical structure will reduce the amounts available to be deposited in the remainder of the respiratory tract. Thus, uncertainties in estimating the deposition fractions in the NAs will propagate throughout the remainder of the respiratory tract, creating errors in the calculated dose estimates. Additionally, there is evidence that the NAs are also at risk for induction of cancer from exposure to certain occupational aerosols such as wood dust, leather dust, chromium, and nickel. The purpose of this investigation was to conduct an anatomical study to assess the variabilities in NA dimensions.

209

Survey monitoring of environmental radioactivity in Busan area  

At Pusan Regional Monitoring Station in Busan have been measured periodically in 2000 gross beta activities in the airborne dust, fallout, precipitation and tap water and gamma exposure rates. Gamma nuclides in airborne dust, fallout and precipitation have also been monitored at the station. As a part of environmental radiation/radioactivity distribution survey around Pusan, vegetables, fishes, shellfish, drinking water (total 23ea) samples were taken from sampling sites which were selected by KlNS. We analysis gamma nuclide for all. No significant changes from the previous survey have been found in both beta activities and gamma exposure rates. As the results of analyzing an gamma nuclide concentration in environmental samples in Pusan are fee of radiological contaminants.

210

Thermal conductivity measurements of porous dust aggregates: I. Technique, model and first results  

We present a novel, non-invasive technique for measuring the thermal conductivity of fragile and sensitive materials. In the context of planet formation research, the investigation of the thermal conductivity of porous dust aggregates provide important knowledge about the influence of heating processes, like internal heating by radioactive decay of short-lived nuclei, e.g. 26Al, on the evolution and growth of planetesimals. The determination of the thermal conductivity was performed by a combination of laboratory experiments and numerical simulations. An IR camera measured the temperature distribution of the sample surface heated by a well-characterized laser beam. The thermal conductivity as free parameter in the model calculations, exactly emulating the experiment, was varied until the experimental and numerical temperature distributions showed best agreement. Thus, we determined for three types of porous dust samples, consisting of spherical, micron-sized SiO2 particles, with volume filling factors in the ...

211

Study on occurrence possibility of dust explosion, hydrogen explosion and decay heat for safety of a process of manufacturing for DUPIC fuel  

DUPIC process is a dry powder processing technology to manufacture CANDU fuel from spent PWR fuel through powder fabrication processes. The DUPIC process consist of the slitting of the spent PWR fuel rods, OREOX processing to produce the powder feedstock, the milling of the produced powder, the granulation of the milled powder, an the mixing of the granulated powder with pressing lubricants, the pelletizing and sintering, and the welding of the fuel rod by laser welding technique. All these processes should be conducted by remote means in a hot-cell environment(M6 hot-cell). Since this process contains powder handling of highly radioactive spent fuel and reduction process with hydrogen, prevention of dust explosion, hydrogen explosion and safe control on decay heat of the fuel is very important. Therefore, this study estimated an occurrence possibility of dust explosion, hydrogen explosion and decay heat for safety of a process of manufacturing for DUPIC fuel. 9 refs., 12 figs., 29 tabs. (Author)

212

Test plan for the field evaluation and demonstration of the Contamination Control Unit  

This report describes test details of a full demonstration of the Contamination Control Unit (CCU). The CCU is a mobile trailer capable of employing the use of soil fixatives, dust suppression agents, misting, and vacuum systems. These systems can perform a large number of contamination control functions to support the Office of Waste Technology Development (OTD) Buried Waste Integrated Demonstration (BWID) projects, transuranic (TRU) waste retrieval operations, and emergency response for hazardous and radioactive materials incidents. The demonstration will include both performance testing at the North Holmes Laboratory Facility (NHLF) and field testing in conjunction with the Remote Excavation System Demonstration at the Cold Test Pit. The NHLF will test operational parameters using water only, and the field demonstration at the Cold Test Pit involves full scale operation of vacuum, fixant, misting, and dust suppression systems. Test objectives, detailed experimental procedures, and data quality objectives necessary to perform the field demonstration are included in this test plan.

213

Demonstration experience with an abrasive blasting technique for decontaminating concrete pads  

A demonstration was performed for decontaminating a radioactivity contaminated concrete pad with a portable abrasive blasting system. The system utilizes a rotating blast wheel that scours the concrete surface with metal abrasive. The metal abrasive, pulverized concrete dust, and contaminants rebound into a separator chamber. The reusable metal abrasive is recycled, and the pulverized media are removed to an integral dust collection system. The exhaust is HEPA filtered to minimize release of airborne contaminants. However, the technique had limited success in reducing contamination around the cracks and seams in the concrete where the higher activity levels of contamination were detected during the radiological survey before the cleanup. The technique can be successful and cost-effective in decontaminating large areas of low contamination; however, careful characterization and planning are necessary. 3 refs., 3 figs., 1 tabs.

214

Indoor air quality and allergy. Airborne dust and its effect of health; Shitsunai kukishitsu to seitai allergy. Fuyu funjin to seitai eikyo  

This paper describes the effect of airborne dust on health. Among fiber dusts in usual houses, cotton-derived dust occupies 71%, paper-derived 11%, chemical fiber-derived 10%, hair-derived 5%, and others occupy the rest. Cotton, silk and hair can be allergens which are antigens causing allergy. Cigarette smoke composes of various gaseous substances, and by-flow smoke from the ignition part is hazardous. The dust generation by smoking provides ten times of standard concentration in a Japanese 6 rush-mat room per one cigarette. Asbestos can be a carcinogen due to their accumulation. They do not have an allowable standard for absolute safety, and they should be removed by manual method under an obligation. This paper also describes the effect of ticks and mold particles as allergen dusts on health, and the measures for them. Pollens and their measures are described. Air cleaners are usually used for removing airborne dusts in the houses with high air-tightness. Nearly 100% of particles with a diameter more than several {mu}m can be collected with a fan filter-type air cleaner. However, the collecting performance is decreased to 70 to 80% for submicron particles such as cigarette smoke. An ion-type air cleaner can not be so promising. 24 refs., 5 figs., 5 tabs.

215

Cooling of Dense Gas by H2O Line Emission and an Assessment of its Effects in Chondrule-Forming Shocks  

We consider gas at densities appropriate to protoplanetary disks and calculate its ability to cool due to line radiation emitted by H2O molecules within the gas. Our work follows that of Neufeld & Kaufman (1993; ApJ, 418, 263), expanding on their work in several key aspects, including use of a much expanded line database, an improved escape probability formulism, and the inclusion of dust grains, which can absorb line photons. Although the escape probabilities formally depend on a complicated combination of optical depth in the lines and in the dust grains, we show that the cooling rate including dust is well approximated by the dust-free cooling rate multiplied by a simple function of the dust optical depth. We apply the resultant cooling rate of a dust-gas mixture to the case of a solar nebula shock pertinent to the formation of chondrules, millimeter-sized melt droplets found in meteorites. Our aim is to assess whether line cooling can be neglected in chondrule-forming shocks or if it must be included....

216

Comet Halley: An optical continuum study  

From an analysis of narrowband CCD images of Comet Halley from 1986 January, March, and April, certain dust structures which are redder than the remainder of the dust coma have become apparent. Mie calculations suggest that this reddening is due to an enhancement of particles with sizes comparable to the observing wavelengths. Although the mass range derived from the calculations presented here is somewhat uncertain as a result of the limitations of Mie theory, these values are in the expected range derived from the calculations presented here is somewhat uncertain as a result of particle sizes which would be both sensitive to radiation pressure and significantly reddened with respect to the solar spectrum at the observing wavelengths. Thus, the red envelopes are plausibly the result of size sorting by solar radiation pressure. The red jets observed on 1986 January 10, March 1 and March 9 can then be explained by the enhanced dust flux at the jet sources, and the subsequent trapping of a relative excess of intermediate mass (i.e. red) particles into the jets which are visible in the continuum images. Analysis of narrowband photometry of the optical continuum of Comet Halley reveals no correlation between the color of the dust and heliocentric distance, phase angle, strength of the continuum or gas-to-dust ratio. The photometric data are thus consistent with a post-ejection sorting mechanism. Chemical inhomogeneities of the nucleus are therefore not necessary to explain the observed structure in the color of the dust in Comet Halley.

217

Effect of spectral-dependent surface albedo on Saharan dust direct radiative forcing  

Direct radiative forcing (DRF) due to mineral dust has quite large uncertainty. Surface albedo is one of the most important factors affecting dust radiative forcing and climate. Here we investigate the effect of spectral-dependent surface albedo on dust DRF over the Saharan desert region using MODIS surface albedo data and a size-resolved global aerosol model. In one simulation, surface albedo in 7 wavebands from MODIS-retrieved data is interpolated to the corresponding 4 solar wavebands of the radiation transfer model (case 1). In another simulation, surface albedo for visible wavebands is applied to all 4 solar spectral-bands (case 2), which was previously used by many global model simulations. Our results show that the annual averaged DRF for all sky over the Saharan dust is -2.4 W m-2 and -5.6 W m-2 at TOA, and -9.9 W m-2 and -12.9 W m-2 at surface for cases 1 and 2, respectively. Such a large difference highlights the importance of using accurate spectral-dependent surface albedo, and implies that previous studies employing only visible-band surface albedo might have significantly overestimated the dust cooling effect over the Saharan dust.

218

French children's exposure to metals via ingestion of indoor dust, outdoor playground dust and soil: contamination data.  

In addition to dietary exposure, children are exposed to metals via ingestion of soils and indoor dust, contaminated by natural or anthropogenic outdoor and indoor sources. The objective of this nationwide study was to assess metal contamination of soils and dust which young French children are exposed to. A sample of 484 children (6 months to 6 years) was constituted in order to obtain representative results for young French children. In each home indoor settled dust was sampled by a wipe in up to five rooms. Outdoor playgrounds were sampled with a soil sample ring (n=315) or with a wipe in case of hard surfaces (n=53). As, Cd, Cr, Cu, Mn, Pb, Sb, Sr, and V were measured because of their potential health concern due to soil and dust ingestion. The samples were digested with hydrochloric acid, and afterwards aqua regia in order to determine both leachable and total metal concentrations and loadings by mass spectrometry with a quadrupole ICP-MS. In indoor settled dust most (total) loadings were below the Limit of Quantification (LOQ), except for Pb and Sr, whose median loadings were respectively 9 and 10 ?g/m². The 95th percentile of loadings were 2 ?g/m² for As, calculated on >LOQ measurements, differed among metals. To a lesser extent, they were also affected by type of matrix, with (except for Cd) a greater leachability of dust (especially indoor) compared to soils. PMID:22613504

219

Early Formation of Dust in the Ejecta of Type Ib SN 2006jc and Temperature and Mass of the Dust  

SN 2006jc is a peculiar supernova (SN), in which the formation of dust has been confirmed at an early epoch of ~50 days after the explosion. We investigate the possibility of such an earlier formation of dust grains in the expanding ejecta of SN 2006jc, applying the Type Ib SN model that is developed to reproduce the observed light curve. We find that the rapid decrease of the gas temperature in SN 2006jc enables the condensation of C grains in the C-rich layer at 40--60 days after the explosion, which is followed by the condensation of silicate and oxide grains until ~200 days. The average radius of each grain species is confined to be less than 0.01 micron due to the low gas density at the condensation time. The calculated total dust mass reaches to ~1.5 Msun, of which C dust shares 0.7 Msun. On the other hand, based on the calculated dust temperature, we show that the dust species and mass evaluated to reproduce the spectral energy distribution observed by AKARI and MAGNUM at day 200 are different from tho...

220

Leaching of metals from copper smelter flue dust (Mufulira, Zambian Copperbelt)  

Highlights: > The leaching behaviour of Cu smelter flue dust is pH-dependent. > Maximum concentrations of metals were released at pH 3-4.5. > Primary chalcanthite was dissolved and secondary Cu sulphates were formed. > Potential risk of contamination of dust-polluted acidic soils near the smelter. - Abstract: The leaching behaviour of electrostatic precipitator dust from the Mufulira Cu smelter (Copperbelt, Zambia) was studied using a 48-h pH-static leaching experiment (CEN/TS 14997). The release of metals (Cd, Co, Cu, Ni, Pb and Zn) and changes in mineralogical composition using X-ray diffraction and PHREEQC-2 modelling were investigated in the pH range of 3-7. The highest concentrations of metals were released at pH 3-4.5, which encompasses the natural pH of the dust suspension ({approx}4.3). About 40% of the total Cu was leached at pH 3, yielding 107 g/kg. Chalcanthite (CuSO{sub 4}.5H{sub 2}O), magnetite (Fe{sub 3}O{sub 4}) and delafossite (CuFeO{sub 2}) represented the principal phases of the studied dust. In contact with water, chalcanthite was dissolved and hydrated Cu sulphates precipitated at pH 4-7. Gypsum (CaSO{sub 4}.2H{sub 2}O) and secondary Fe or Al phases were observed in the leached residues. Serious environmental impact due to leaching may occur in dust-contaminated soil systems in the vicinity of the smelting plants.

 
 
 
 
221

Wide-Area Mapping of 155 Micron Continuum Emission from the Orion Molecular Cloud Complex  

We present the results of a wide-area mapping of the far-infrared continuum emission toward the Orion complex by using a Japanese balloon-borne telescope. The 155-um continuum emission was detected over a region of 1.5 deg^2 around the KL nebula with 3' resolution similar to that of the IRAS 100-um map. Assuming a single-temperature model of the thermal equilibrium dust, maps of the temperature and the optical depth were derived from the 155 um intensity and the IRAS 100 um intensity. The derived dust temperature is 5 - 15 K lower and the derived dust optical thickness were derived from the 155-um intensity and the IRAS 100-um intensity. The derived dust temperature is 5 - 15 K lower and the derived dust optical depth is 5 - 300 times larger than those derived from the IRAS 60 and 100-um intensities due to the significant contribution of the statistically heated very small grains to the IRAS 60-um intensity. The optical-thickness distribution shows a filamentary dust ridge that has a 1.5 degrees extent in the...

222

Dust Expansion Speed of Comet 103P/Hartley 2  

The Deep Impact eXtended Investigation (DIXI) redirected the Deep Impact Flyby (DI) spacecraft to fly past Comet 103P/Hartley 2 on November 4th, 2010. During the approach and departure, the DI spacecraft continuously monitored Hartley 2 with its imaging instruments. We measured the broadband visible lightcurves of the comet through various aperture diameters from 3 to 40 pixels. The coma dominates the total brightness of the comet measured in all aperture sizes, and the changes in the dust production rate due to the rotation of the nucleus causes lightcurve variations. The propagation of the coma dust particles causes variations in the timing of lightcurve extrema determined at consecutively larger annulus apertures. In order to measure the expansion speed of coma particles, we measured the timing variations of these lightcurve extrema during 20 days bracketing the closest encounter. Our analysis shows that the apparent expansion speed of dust particles in the inner coma is between 20 and 100 m/s. However, the apparent expansion speed may not represent the actual expansion speed, and is affected by several factors, including radiation pressure, multiple speed components, and possibly other factors such as outgassing from the nucleus and sublimation of icy particles. We also found spatial and temporal variations of the apparent expansion speed, evidently related to the periodic variations in dust production rate. We constructed numerical models to reproduce the observed dust expansion speed measurements, and to help us understand how the dust particles propagate away from the nucleus in the inner coma of Hartley 2.

223

Chaotic dust orbits at Uranus may explain hemispherical color asymmetries on its regular satellites  

When [1] noticed that Uranus' four largest moons had leading-trailing hemispherical color asymmetries, they conjectured that infalling dust from yet-to-be discovered, retrograde irregular satellites might be responsible. Eight such retrograde moons have since been found, and the recent detection of Phoebe's ring at Saturn [6] suggests that large dust rings generated by irregular satellites might be common around the giant planets. We therefore investigate whether infalling dust in the Uranian system might explain the color dichotomies among its regular satellites. In particular, we aim to understand why dust seems to have been distributed among them all rather than concentrated almost exclusively on the outermost moon, Oberon, as in the Saturnian case of Iapetus. When studying the orbits of evolving dust grains, we find that Uranus' unique, extreme obliquity ( 98°) results in chaotic, large-amplitude variations in orbital eccentricity and inclination due to the wide misalignment between perturbations from the planet's oblateness and tidal perturbations from the Sun. These rapid orbital variations allow dust to access all the regular satellites simultaneously (rather than in sequence fromoutermost inward). This can explain the fact that all four moons exhibit leading-trailing hemispherical color asymmetries.

224

Lidar ratio of Saharan dust over Cape Verde Islands: Assessment and error calculation  

Lidar ratios Sp of Saharan dust were determined at the Cape Verde Islands in the framework of the second phase of the Saharan Mineral Dust Experiment to investigate possible changes during the first few days of transport from the source regions. Lidar ratios were retrieved from vertical profiles of particle extinction coefficients and backscatter coefficients measured simultaneously at 355 and 532 nm with the two Raman lidar systems MULIS and POLIS of the Meteorological Institute of the Ludwig-Maximilians-Universität. As previous studies are lacking, one of the main foci of this paper is the elaboration of an extensive error analysis of the Sp retrieval. Only the determination of systematic errors, resulting from the uncertainties of the input parameters of the retrieval, and statistical errors of Sp due to signal noise allows one to compare measurements at different sites and to gain insight into the changes of the dust lidar ratio with time. Suitable conditions for the assessment of Sp and the error analysis were met during a strong Saharan dust outbreak from 28 to 30 January 2008, where particle extinction coefficients of the dust layer as high as 0.2-0.4 km-1 in the UV and visible spectral region were observed. We found an average lidar ratio of dust over Cape Verde Islands of 63 ± 6 sr at 355 and 532 nm.

225

Past dust and GAS/FUME exposure and COPD in Chinese: the Guangzhou Biobank Cohort Study.  

The impact of occupational dust and gas/fume exposure on chronic obstructive pulmonary disease (COPD) in developing countries has not been quantified. We examined the relationship between past dust and fume exposure and prevalence of COPD and respiratory symptoms in a cross-sectional analysis of a large Chinese population sample. Participants in the Guangzhou Biobank Cohort Study (n = 8216; 27.3% men, mean age 61.9 ± 6.8 years) had spirometry and a structured interview including exposures, symptoms, and lifestyle. Self-reported intensity and duration of dust and gas/fume exposure was used to derive cumulative exposure. COPD was diagnosed from spirometry using lower limit of normal based on prediction equations. COPD was associated with high exposure to dust or gas/fume (exposed: 87/1206 v non-exposed: 191/3853; adjusted odds ratio: 1.41; 95% confidence interval (CI) 1.06, 1.87) with no evidence of effect modification by smoking. Respiratory symptoms were associated with exposures to dust and gas/fume, with adjusted odds ratios for chronic cough/phlegm of 1.57 (1.13, 2.17) and 1.39 (1.20, 1.60) for dyspnoea. The overall population attributable fraction for COPD due to occupational exposure was 10.4% (95% CI -0.9%, 19.5%). Occupational dust and gas/fume exposure is associated with an increased prevalence of COPD in this Chinese sample, independent of smoking. The population attributable fraction in Chinese is similar to that in Western populations. PMID:22795505

226

Short-lived and long-lived dust devil tracks in the coastal desert of southern Peru  

In the coastal desert of southern Peru, sequential high-resolution satellite images document the presence of short-lived and long-lived dust devil tracks. Dust devil tracks in the study region remain visible for less than 6 months in one area and for more than 4 years in another area. Short-lived tracks are generally darker than the surrounding ground surface. The brightness of long-lived tracks is often equal to that of their surroundings; they become visible due to a brighter edge along their margins. Different modes of formation related to ground surface properties are suggested to explain the differences in persistence and appearance. Dark, short-lived dust devil tracks are ascribed to the removal of silt-sized material from largely sand-sized surface materials. Long-lived tracks with bright margins are ascribed to coarser surface materials and the fallout of sand-sized particles along the track edges. Locating suitable areas on Earth for the study of dust devil tracks and distinguishing between different types of dust devil tracks is expected to further promote terrestrial analogue studies for Martian dust devil streaks.

227

Quantifying dust and the ultraviolet radiation-density in the local universe  

A sample of local galaxies for which far infrared and uv fluxes are available is used to estimate the characteristic dust extinction in galaxies and to test whether standard dust properties are plausible. Assuming galaxies can be characterized by a single dust optical depth (certainly not valid for galaxies with a dominant starburst component), the infrared excess and ultraviolet colours of local galaxies are found to be consistent with normal Milky Way dust, with a mean value for E(B-V) of 0.16. A significant fraction of the dust heating is due to older, lower mass stars, and this fraction increases towards earlier galaxy types. Analysis of F_fir/F_uv versus uv colour diagrams for starburst galaxies in terms of a simple screen dust model does not support a Calzetti (1999) rather than a Milky Way extinction law, though the absence of the expected strong 2200 A feature in several galaxies with IUE spectra does show that more detailed radiative transfer models are needed, probably with non-spherical geometry. A...

228

Aeolian removal of dust from radiator surfaces on Mars  

Simulated radiator surfaces made of arc-textured copper and niobium-one percent-zirconium, and ion beam textured graphite and carbon-carbon composite were fabricated and their integrated spectral emittance characterized from 300 to 3000 K. A thin layer of aluminum oxide, basalt, or iron (III) oxide dust was then deposited on them, and they were subjected to low pressure winds in the Martian Surface Wind Tunnel. It has been found that dust deposited on simulated radiator surfaces may or may not seriously lower their integrated spectral emittance, depending upon the characteristics of the dust. With Al{sub 2}O{sub 3} there is no appreciable degradation of emittance on a dusted sample, with basaltic dust there is a 10-20 percent degradation, and with Fe{sub 2}O{sub 3} a 20-40 percent degradation. It was also found that very high winds on dusted highly textured surfaces can result in their abrasion. Degradation in emittance due to abrasion was found to vary with radiator material. Arc-textured copper and Nb-1%Zr was found to be more susceptible to emittance degradation than graphite or carbon-carbon composite. The most abrasion occurred at low angles, peaking at the 22.5{degrees} test samples.

229

Coke breeze-less sintering of BOF dust and its capability of dezicing  

In order to promote recycling of basic oxygen furnace (BOF) dust, sintering of the dust without coke breeze (fuel) has been researched by pot test method and the possibility of dezincing during the sintering has been evaluated. Typical BOF dust, containing about 20% of metallic iron (M.Fe), is agglomerated without fuel and dezinced by about 50% during sintering. The agglomeration is caused by heat generation due to oxidation of the metallic iron. The dezincing takes place by the reaction: ZnO + M.Fe {yields} Zn(gas) + FeO at elevated temperature. Secondary dust emitted during sintering mainly consisted of ZnO containing 40 to 50% of zinc. The ratio of dezincing is improved by blast furnace (BF) dust addition and updraft sintering method. The carbon in BF dust produces metallic iron and CO gas from 'FeO' melt, then they accelerate ZnO reduction. The up-drafting makes a melt pool in the lower layer, where the melt remains longer at high temperature, resulting in increase in the ratio of dezincing. (author)

230

Ion-acoustic solitons in dusty plasma  

The dynamics of dust ion-acoustic solitons is analyzed in a wide range of dusty plasma parameters. The cases of both a positive dust grain charge arising due to the photoelectric effect caused by intense electromagnetic radiation and a negative grain charge established in the absence of electromagnetic radiation are considered. The ranges of plasma parameters and Mach numbers in which "conservative" (nondissipative) solitons can exist are determined. It is shown that, in dusty plasma with negatively charged dust grains, both compression and rarefaction solitons can propagate, whereas in plasma with positively charged dust grains, only compression solitons can exist. The evolution of soliton-like compression and rarefaction perturbations is studied by numerically solving the hydrodynamic equations for ions and dust grains, as well as the equation for dust grain charging. The main dissipation mechanisms, such as grain charging, ion absorption by dust grains, momentum exchange between ions and dust grains, and ion-neutral collisions are taken into account. It is shown that the amplitudes of soliton-like compression and rarefaction perturbations decrease in the course of their evolution and their velocities (the Mach numbers) decrease monotonically in time. At any instant of time, the shape of an evolving soliton-like perturbation coincides with the shape of a conservative soliton corresponding to the current value of the Mach number. It is shown that, after the interaction between any types of soliton-like perturbations, their velocities and shapes are restored (with a certain phase shift) to those of the corresponding perturbations propagating without interaction; i.e., they are in fact weakly dissipative solitons.

231

Microphysical and optical properties of dust and tropical biomass burning aerosol layers in the Cape Verde region - an overview of the airborne in situ and lidar measurements during SAMUM-2  

In the framework of the Saharan Mineral Dust Experiment (SAMUM) airborne High Spectral Resolution Lidar and in situ measurements of the particle size, aerosol mixing state and absorption coefficient were conducted. Here, the properties of mineral dust and tropical biomass burning layers in the Cape Verde region in January/February 2008 are investigated and compared with the properties of fresh dust observed in May/June 2006 close the Sahara. In the Cape Verde area, we found a complex stratification with dust layers covering the altitude range below 2 km and biomass burning layers aloft. The aerosol type of the individual layers was classified based on depolarization and lidar ratios and, in addition, on in situ measured Ångström exponents of absorption åap. The dust layers had a depth of 1.3 ± 0.4 km and showed a median åap of 3.95. The median effective diameter Deff was 2.5 ?m and the dust layers over Cape Verde yielded clear signals of aging: large particles were depleted due to gravitational settling and the accumulation mode diameter was shifted towards larger sizes as a result of coagulation. The tropical biomass layers had a depth of 2.0 ± 1.1 km and were characterized by a median åap of 1.34. They always contained a certain amount of large dust particles and showed a median Deff of 1.1 ?m and a fine mode Deff, fine of 0.33. The dust and biomass burning layers had a median aerosol optical depth (AOD) of 0.23 and 0.09, respectively. The median contributions to the AOD of the total atmospheric column below 10 km were 75 and 37%, respectively.

232

Microphysical and optical properties of dust and tropical biomass burning aerosol layers in the Cape Verde region-an overview of the airborne in situ and lidar measurements during SAMUM-2  

In the framework of the Saharan Mineral Dust Experiment (SAMUM) airborne High Spectral Resolution Lidar and in situ measurements of the particle size, aerosol mixing state and absorption coefficient were conducted. Here, the properties of mineral dust and tropical biomass burning layers in the Cape Verde region in January/February 2008 are investigated and compared with the properties of fresh dust observed in May/June 2006 close the Sahara. In the Cape Verde area, we found a complex stratification with dust layers covering the altitude range below 2 km and biomass burning layers aloft. The aerosol type of the individual layers was classified based on depolarization and lidar ratios and, in addition, on in situ measured Aangstroem exponents of absorption aa{sub ap}. The dust layers had a depth of 1.3 +- 0.4 km and showed a median aa{sub ap} of 3.95. The median effective diameter D{sub eff} was 2.5 mum and the dust layers over Cape Verde yielded clear signals of aging: large particles were depleted due to gravitational settling and the accumulation mode diameter was shifted towards larger sizes as a result of coagulation. The tropical biomass layers had a depth of 2.0 +- 1.1 km and were characterized by a median aa{sub ap} of 1.34. They always contained a certain amount of large dust particles and showed a median D{sub eff} of 1.1 mum and a fine mode D{sub eff,fine} of 0.33. The dust and biomass burning layers had a median aerosol optical depth (AOD) of 0.23 and 0.09, respectively. The median contributions to the AOD of the total atmospheric column below 10 km were 75 and 37%, respectively

233

Evaluation of the approach to respirable quartz exposure control in U.S. coal mines.  

Occupational exposure to high levels of respirable quartz can result in respiratory and other diseases in humans. The Mine Safety and Health Adminstration (MSHA) regulates exposure to respirable quartz in coal mines indirectly through reductions in the respirable coal mine dust exposure limit based on the content of quartz in the airborne respirable dust. This reduction is implemented when the quartz content of airborne respirable dust exceeds 5% by weight. The intent of this dust standard reduction is to restrict miners' exposure to respirable quartz to a time-weighted average concentration of 100 ?g/m(3). The effectiveness of this indirect approach to control quartz exposure was evaluated by analyzing respirable dust samples collected by MSHA inspectors from 1995 through 2008. The performance of the current regulatory approach was found to be lacking due to the use of a variable property-quartz content in airborne dust-to establish a standard for subsequent exposures. In one situation, 11.7% (4370/37,346) of samples that were below the applicable respirable coal mine dust exposure limit exceeded 100 ?g/m(3) quartz. In a second situation, 4.4% (895/20,560) of samples with 5% or less quartz content in the airborne respirable dust exceeded 100 ?g/m(3) quartz. In these two situations, the samples exceeding 100 ?g/m(3) quartz were not subject to any potential compliance action. Therefore, the current respirable quartz exposure control approach does not reliably maintain miner exposure below 100 ?g/m(3) quartz. A separate and specific respirable quartz exposure standard may improve control of coal miners' occupational exposure to respirable quartz. PMID:22181563

234

Rocket Effect For Fragments And Meteoroids Of The Split Comet 73P/Schwassmann-Wachmann 3  

The fragments and debris from the split comet 73P/Schwassmann-Wachmann 3 were observed with the Spitzer and Hubble Space Telescopes, revealing the distribution of fragments on sizes from the major nuclei (km) down to dust (10 microns). The dust particles form a tail in the antisolar direction due to radiation pressure. The large fragments and meteoroids form a trail arranged along the projected orbit. Intermediate-sized fragments detected by HST move with the dust in the tailward direction. We interpret the dynamics by combining radiation pressure and reflex momentum loss due to outgassing (rocket effect). The HST fragments must be very icy, while the meteoroids must be very dry. We discuss the relationship between the observed fragments and the cometary nuclei and the nature of cometary material.

235

Vehicle non-exhaust emissions from the tyre-road interface - effect of stud properties, traction sanding and resuspension  

In Northern cities respirable street dust emission levels (PM10) are especially high during spring. The spring time dust has been observed to cause health effects as well as discomfort among citizens. Major sources of the dust are the abrasion products from the pavement and traction sand aggregates that are formed due to the motion of the tyre. We studied the formation of respirable abrasion particles in the tyre-road interface due to tyre studs and traction sanding by a mobile laboratory vehicle Sniffer. The measurements were preformed on a test track, where the influence of varying stud weight and stud number per tyre on PM10 emissions was studied. Studded tyres resulted in higher emission levels than studless tyres especially with speeds 50 km h-1 and higher; however, by using light wei...

236

The Effect of Line of Sight Temperature Variation and Noise on Dust Continuum Observations  

We investigate the effect of line of sight temperature variations and noise on two commonly used methods to determine dust properties from dust continuum observations of dense cores. One method employs a direct fit to a modified blackbody SED; the other involves a comparison of flux ratios to an analytical prediction. Fitting fluxes near the SED peak produces inaccurate temperature and dust spectral index estimates due to the line of sight temperature (and density) variations. Longer wavelength fluxes in the Rayleigh-Jeans part of the spectrum (>~ 600 micron for typical cores) may more accurately recover the spectral index, but both methods are very sensitive to noise. The temperature estimate approaches the density weighted temperature, or "column temperature," of the source as short wavelength fluxes are excluded. An inverse temperature - spectral index correlation naturally results from SED fitting, due to the inaccurate isothermal assumption, as well as noise uncertainties. We show that above some "thresh...

237

Episodic post-shock dust formation in the colliding winds of Eta Carinae  

ABSTRACT Eta Carinae shows broad peaks in near-infrared (IR) JHKL photometry, roughly correlated with times of periastron passage in the eccentric binary system. After correcting for secular changes attributed to reduced extinction from the thinning Homunculus nebula, these peaks have IR spectral energy distributions (SEDs) consistent with emission from hot dust at 1400-1700 K. The excess SEDs are clearly inconsistent, however, with the excess being entirely due to free-free wind or photospheric emission. One must conclude, therefore, that the broad near-IR peaks associated with Eta Carinae's 5.5 yr variability are due to thermal emission from hot dust. I propose that this transient hot dust results from episodic formation of grains within compressed post-shock zones of the colliding winds...

238

Radioactivity survey data in Japan. Pt. 2. Dietary materials  

This is a report on radioactivity in Japan issued by National Institute of Radiological Sciences, Chiba on September, 1998. This data relates to some environmental materials such as rain and dry fallout, airborne dust, service water, freshwater, soil, sea water and sea sediments and some dietary materials such as rice, milk, vegetables, tea, fish, shellfish, and seaweeds, which were collected from Oct. 1995 to Mar. 1996. In the survey data, followings are contained: 1) Collection and pretreatment of samples, 2) Preparation of samples for analysis, 3) Separation of Strontium 90 and Cesium 137, 4) Determination of stable Strontium, Calcium, and Potassium, 5) Counting, 6) Results, and 7) Contents of Figure. (J.P.N.)

239

Radioactivity survey data in Japan. Pt. 2. Dietary materials  

This is a report on radioactivity in Japan issued by National Institute of Radiological Sciences, Chiba on August, 1998. This data relates to some environmental materials such as rain and dry fallout, airborne dust, service water, freshwater, soil, sea water and sea sediments and some dietary materials such as rice, milk, vegetables, tea, fish, shellfish, and seaweeds, which were collected from April to September, 1995. In the survey data, followings are contained: 1) Collection and pretreatment of samples, 2) Preparation of samples for analysis, 3) Separation of Strontium 90 and Cesium 137, 4) Determination of stable Strontium, Calcium, and Potassium, 5) Counting, 6) Results, and 7) Contents of Figure. (J.P.N.)

240

Results of the radiological survey at Diebold Safe Company, 1550 Grand Boulevard, Hamilton, Ohio (HO001)  

At the request of the US Department of Energy (DOE), a group from Oak Ridge National Laboratory conducted investigative radiological surveys at Diebold Safe Company, 1550 Grand Boulevard, Hamilton, Ohio in 1988 and 1989. The purpose of the surveys was to determine whether the property was contaminated with radioactive residues, principally {sup 238}U. The surveys included gamma scans; direct and transferable measurements of alpha, beta, and gamma radiation levels; and dust, debris, air, and soil sampling for radionuclide analyses. 6 refs., 6 figs., 5 tabs.

 
 
 
 
241

Insitu Cleanable Alternative HEPA Filter Media  

Two types of filter media, sintered nickel metal and ceramic monolith membrane, are being investigated as in situ regenerable/cleanable high efficiency particulate air (HEPA) filters. Particle retention testing was conducted on the filters at the Oak Ridge Filter Test Facility to ensure HEPA efficiency, greater than 99.97 percent. During simulant testing, The filters were challenged using non-radioactive simulated high-level waste materials and atmospheric dust; materials that cause filter pluggage in the field. After plugging the filters they were cleaned in situ using an aqueous solution. This innovative approach of the in situ regenerative filtration system may be a significant improvement upon the shortfalls of conventional disposable HEPA filters.

242

Air filter. [For radioactive dust in air  

An air filter consists of an upright cylinder of corrugated or pleated filter fabric, joined at its upper end to a tubular right-angled elbow. The open end of the elbow includes an internal lip seal, so the elbow can be slid onto a horizontal spigot in an air filter unit. The filter can be cleaned by subjecting the fabric to a reverse pressure pulse from a nozzle. The construction facilitates removal of the filter into a plastic bag secured round a frame behind a door, when the unit is used to filter radioactive dust from air. (author).

243

Assessing inhalation exposure from airborne soil contaminants  

A method of estimation of inhalation exposure to airborne soil contaminants is presented. this method is derived from studies of airborne soil particles with radioactive tags. The concentration of contaminants in air (g/m{sup 3}) can be derived from the product of M, the suspended respirable dust mass concentration (g/m{sup 3}), S, the concentration of contaminant in the soil (g/g), and E{sub f}, an enhancement factor. Typical measurement methods and values of M, and E{sub f} are given along with highlights of experiences with this method.

244

Implications of the broad Al-26 1809 keV line observed by GRIS  

The astrophysical implications of the large width of the 1809 keV gamma ray line from the decay of radioactive Al-26, recently observed with the gamma ray imaging spectrometer (GRIS), are discussed. While there may be no apparent single mechanism that can explain the observed broadening, high speed dust grains, extremely hot superbubbles and a large, low density gaseous halo were identified in the Galactic center region as the possible origins. The implications of these observations on the hot gas content in the interstellar medium are discussed.

245

Monitoring airborne alpha-emitter contamination  

Facilities that may produce airborne alpha emitter contamination require a continuous air monitoring (CAM) system. However, these traditional CAMs have difficulty in environments with large quantities of non-radioactive particulates such as dust and salt. Los Alamos has developed an airborne plutonium sensor (APS) for the REBOUND experiment at the Nevada Test Site which detects alpha contamination directly in the air, and so is less vulnerable to the problems associated with counting activity on a filter. In addition, radon compensation is built into the detector by the use of two measurement chambers.

246

ISOCELL{trademark} proof-of-concept for retrieval of wastes and contaminated soil  

ISOCELL{sup TM} cryogenic technology is designed to immobilize buried hazardous, radioactive, and mixed waste and contaminated soil by creating a block of frozen waste and soil that can be safely retrieved, stored, transported, and treated with a minimum of dust or aerosol production. A ``proof-of-concept`` test of the ISOCELL process was conducted in clean soil by RKK, Ltd., for the Idaho National Engineering Laboratory (INEL). Results indicate ISOCELL technology successfully froze moist soil into a solid block capable of being lifted and retrieved. Test conditions were compared to characteristics of possible buried waste sites in the INEL.

247

ISOCELL trademark proof-of-concept for retrieval of wastes and contaminated soil  

ISOCELL{sup TM} cryogenic technology is designed to immobilize buried hazardous, radioactive, and mixed waste and contaminated soil by creating a block of frozen waste and soil that can be safely retrieved, stored, transported, and treated with a minimum of dust or aerosol production. A proof-of-concept'' test of the ISOCELL process was conducted in clean soil by RKK, Ltd., for the Idaho National Engineering Laboratory (INEL). Results indicate ISOCELL technology successfully froze moist soil into a solid block capable of being lifted and retrieved. Test conditions were compared to characteristics of possible buried waste sites in the INEL.

248

Radioactivity in the environment  

Natural and man-made radioactivities in the environment have been extensively researched in the second half of this century. Recently, increased attention has been given to (1) radioactive waste willfully placed in the environment by discharges from nuclear reprocessing plants or by dumping at sea, and (2) radioactive materials lost due to accidents in terrestrial (civilian power) or marine (submarine propulsion) reactors. Increasing field measurements, and disclosures of dumping and accidents in the former Soviet Union, are adding greatly to the knowledge of environmental radioactivity. New, more powerful computers are having a double impact. They make possible Geographical Information Systems for geo-referencing and correlating multi-variable datasets. Furthermore, supercomputers enable global atmospheric, oceanographic and terrestrial circulation and transport models, which include physical, chemical and biological processes. We will review exemplary work on the sources, transport, disposition and impact of anthropogenic environmental radioactivity. Such work both provides new knowledge of environmental processes and furnishes the basis for deciding on potential remediation actions.

249

FINAL DISPOSAL OF RADIOACTIVE WASTE IN GERMANY: PLAN APPROVAL PROCESS OF KONRAD MINE AND ACCEPTANCE REQUIREMENTS  

Currently no final repository for any type of radioactive waste is operated in Germany. Preliminary Final Storage Acceptance Requirements for radioactive waste packages were published in 1995. Up to now these are the basis for treatment of radioactive waste in Germany. After licensing of the final repository these preliminary waste acceptance requirements are completed with licensing conditions. Some of these conditions affect the preliminary waste acceptance requirements, e. g. behavior of chemo-toxic substances in case of accidents in the final repository or the allowed maximum concentration of fissile material. The presented examples of radioactive waste conditioning campaigns demonstrate that no difficulties are expected in management, characterization and quality assurance of radioactive wastes due to the licensing conditions.

250

Transport of mineral dust to Nepal Climate Observatory - Pyramid (5079 m a.s.l., South Himalayas)  

Desert dust is one of the greatest sources of natural aerosol in atmosphere, representing about 37% of the total (natural and anthropogenic) emission of atmospheric primary aerosols. Mineral dust can impact climate through many complex processes, i.e. by scattering and absorbing solar and infrared radiation and by affecting the variability of cloud aerosol optical properties. Moreover, mineral dust can also affect the concentrations of other climate-altering species (e.g. surface ozone) in troposphere. South Asia is a region frequently affected by major dust transport from Africa and Asia. In particular, these "dust clouds" can reach the Himalayas also mixed with the heavy anthropogenic pollution present within the so-called Asian Brown Cloud. With the purpose to define the frequency of long-range mineral dust transport towards the Himalayan range and to evaluate their influence on the atmospheric aerosol background level, in this work we analyse the first 2-year (from March 2006 to February 2008) of coarse (Dp > 1 micron) aerosol number concentration observed at the WMO - GAW station "Nepal Climate Observatory - Pyramid" (NCO-P, 5079 m a.s.l., Nepal). This measurement station, part of UNEP-ABC and EV-K2-CNR SHARE projects, is not far from the Everest Base Camp and the observation here conducted can be considered representative for the South-Eastern slope of the Himalayan range. During the investigated period we detect more than 80 days/year as possibly affected by mineral dust transport. As deduced by the NCO-P measurements, these events significantly influenced the seasonal variation of coarse aerosol number concentration as well as the number and volumetric aerosol size distribution over South Himalayas. Due to the combination of the large-scale westerly circulation and the higher frequency of dust out-breaks, the majority of the identified events occurred during the pre-monsoon season. Although of lesser intensity and frequency, a significant amount of dust transports were also observed during the winter season, while during summer major monsoon mineral dust transport occurred mainly during monsoon break episodes. The analysis of the 3D back-trajectories ending at the NCO-P and calculated by the LAGRANTO model, permitted to identify the possible source areas for the mineral dust: the Thar Desert, the arid areas in the Indo-Gangetic plains, the Tibetan Plateau as well as the Arabian peninsula and the North Africa.

251

Variation of aerosol characteristics in the detail scale of time and space  

In this work, we intend to demonstrate the spatial and temporal variation of atmospheric aerosols around AERONET/Osaka site. Osaka is the second big city in Japan and a typical Asian urban area. It is well known that the aerosol distribution in Asia is complicated due to the increasing emissions of anthropogenic aerosols in association with economic growth and in addition behavior of natural dusts significantly varies with the seasons. Therefore local spatially and temporally resolved measurements of atmospheric particles in Asian urban city are meaningful. We equip various ground measurement devices of atmosphere in the campus of Kinki University (KU). The data supplied by the Cimel instrument are analyzed with a standard AERONET (Aerosol Robotics Network) processing system. It provides us with Aerosol optical thickness (AOT), the Ångström exponent and so on. We set up a PM sampler and a standard instrument of NIES/LIDAR network attached to our AERONET site. The PM sampler provides particle information about the concentrations of PM2.5, PM10 and OBC separately. In addition to the simultaneous measurements, we make observation of the air quality at several locations in the neighbour-hood using portable sun-photometers (Solar-Light Company Microtops-2). The simultaneous measurements of aerosols and numerical model simulations indicate that the spatial and temporal factors influence the characterization of atmospheric particles especially in dust event. Then we observe the air quality at such several locations within a few 10 km area from KU, as Izumi and Nara, in ordinal days and dust days. Izumi site locates near industrial area and Nara is in the east of KU beyond the mountain-Ikoma. It is found from the simultaneous measurements at these three sites that AOT at Izumi in ordinal days is the highest and Nara's lowest. It indicates that the Ikoma-mountains block off the polluted air from the west. However in dust days, AOT at Nara is as large as that at Higashi-Osaka. We guess dust aerosols are transported over the mountains because dust aerosols exist higher than usual. In order to investigate change of aerosol properties before and after dust event, we analyze particulate matter with scanning electron microscope (SEM) coupled with energy dispersive X-ray analyzer (EDX). It is found from the scaling of particle size and ratio of major and minor axis for PM2.5 sampling on 21 March, 2010 when dust event occurred that at the peak of dust event nonspherical particles with large particle size are dominant. A componential analysis also presents temporal variation of aerosol properties. Sulfur is major component before dust comes but Si becomes major component with dust event.

252

Experimental Investigation of In Situ Cleanable or Regenerative Filters for High Level Radioactive Waste Tanks  

The Westinghouse Savannah River Company, located at the Savannah River Site (SRS) in Aiken, South Carolina, is currently testing two types of filter media for application as in situ regenerable/cleanable filters on high-level radioactive liquid waste tanks. Each of the 1.3 million-gallon tanks is equipped with an exhaust ventilation system to provide tank ventilation and to maintain the tank contents at approximately 1-in. water gauge vacuum to prevent the release of radioactive material to the environment. These systems are equipped with conventional, disposable, glass-fiber, High Efficiency Particulate Air (HEPA) filters that require frequent removal, replacement, and disposal. The need for routine replacements is often caused by accelerated filter loading due to the moist operating environment, which structurally weakens the filter media. This is not only costly, but subjects site personnel to radiation exposure and possible contamination. The types of filter media tested, as part of a National Energy Technology Laboratory procurement, were sintered metal and monolith ceramic. The media were subjected to a hostile environment to simulate conditions that challenge the tank ventilation systems. The environment promoted rapid filter plugging to maximize the number of filter loading/cleaning cycles that would occur in a specified period of time. The filters were challenged using non-radioactive, simulated high level waste materials and atmospheric dust, as these materials are most responsible for filter pluggage in the field. The filters were cleaned/regenerated in situ using an aqueous solution of dilute (10% volume) nitric acid. The study found that both filter media were insensitive to high humidity or moisture conditions and were easily cleaned in situ. The filters regenerated to approximately clean filter status even after numerous plugging and cleaning cycles. The filters were leak tested using poly alpha olefin aerosol at the beginning, middle, and end of the test campaign. Both the sintered metal and ceramic filters passed the challenge test with the efficiency of a conventional HEPA filter each time. The sintered metal and ceramic filters not only can be cleaned in situ but also hold great potential as a long life alternative to conventional HEPA filters. The Defense Nuclear Facility Safety Board Technical Report, entitled HEPA Filters Used in the Department of Energy's Hazardous Facilities, found that conventional glass fiber HEPA filters are structurally weak and easily damaged by water or fire. The structurally stronger sintered metal and ceramic filter media would reduce the potential of a catastrophic HEPA filter failure due to filter media breakthrough in the process ventilation system. An in situ regenerable system may also be applicable to recovery of nuclear materials, such as plutonium, collected on glove box exhaust HEPA filters. This innovative approach of the in situ regenerable filtration system may be a significant improvement upon the shortfalls of conventional disposable HEPA filters.

253

Satellite Observations from SEVIRI of Saharan dust over West Africa, within the context of the Fennec project  

During the summer months, the atmosphere over the western half of the Sahara carries some of the highest dust loadings on the planet. This situation develops when intense solar heating over the dry desert creates a deep and hot low pressure system (the Saharan Heat Low, SHL), which allows a strong vertical mixing of dust. The Fennec* consortium project aims to address the deficiency in observations from the sparsely populated western Sahara through the use of field campaign measurements made in June 2011, incorporating observations from ground instruments, aircraft, and from satellite instruments such as SEVIRI, in combination with climate modelling. Fennec aims to study the poorly understood behaviour of the SHL, and the processes which take place within it. Due to their high temporal resolution, observations from SEVIRI can offer new insights into the timing of activation of specific dust sources, and the processes governing their behaviour. Here we employ a multi-year, high time-resolution record of dust detection and aerosol optical depth (AOD) derived from SEVIRI using an algorithm developed at Imperial College to both identify areas of high dust loading and diagnose diurnal patterns in their activation. We will present results from the SEVIRI record alongside results from other satellite instruments such as MODIS, and place these findings in the context of the initial ground-based and in-situ observations available from the Fennec field campaign. We will also identify surface features which can contaminate the dust detection retrieval, due to their emissivities in the 8.7 micron channel. New techniques can be used to filter out these features, based on the difference between the brightness temperatures at 10.8 and 8.7 microns. Using surface visibility measurements and AERONET data, we will evaluate the consequences of this on the dust detection and AOD record. * Fennec is a consortium project which includes groups from the universities of Oxford, Imperial College London, Leeds, Reading, and Sussex, as well as the UK Met Office and collaborators in France, Germany, Algeria, and Mauritania.

254

The HETDEX Pilot Survey. II. The Evolution of the Ly? Escape Fraction from the Ultraviolet Slope and Luminosity Function of 1.9 < z < 3.8 LAEs  

We study the escape of Ly? photons from Ly? emitting galaxies (LAEs) and the overall galaxy population using a sample of 99 LAEs at 1.9 ultraviolet (UV) luminosities and UV slopes, and estimate E(B - V) under the assumption of a constant intrinsic UV slope for LAEs. These quantities are used to estimate dust-corrected star formation rates (SFRs). Comparison between the observed Ly? luminosity and that predicted by the dust-corrected SFR yields the Ly? escape fraction. We also measure the Ly? luminosity function and luminosity density (?Ly?) at 2 (3-6) × 1042 erg s-1 (0.25-0.5 L*), have a mean langE(B - V)rang = 0.13 ± 0.01, implying an attenuation of ~70% in the UV. They show a median UV uncorrected SFR = 11 M sun yr-1, dust-corrected SFR = 34 M sun yr-1, and Ly? equivalent widths (EWs) which are consistent with normal stellar populations. We measure a median Ly? escape fraction of 29%, with a large scatter and values ranging from a few percent to 100%. The Ly? escape fraction in LAEs correlates with E(B - V) in a way that is expected if Ly? photons suffer from similar amounts of dust extinction as UV continuum photons. This result implies that a strong enhancement of the Ly? EW with dust, due to a clumpy multi-phase interstellar medium (ISM), is not a common process in LAEs at these redshifts. It also suggests that while in other galaxies Ly? can be preferentially quenched by dust due to its scattering nature, this is not the case in LAEs. We find no evolution in the average dust content and Ly? escape fraction of LAEs from z ~ 4 to 2. We see hints of a drop in the number density of LAEs from z ~ 4 to 2 in the redshift distribution and the Ly? luminosity function, although larger samples are required to confirm this. The mean Ly? escape fraction of the overall galaxy population decreases significantly from z ~ 6 to z ~ 2, in agreement with recent results. Our results point toward a scenario in which star-forming galaxies build up significant amounts of dust in their ISM between z ~ 6 and 2, reducing their Ly? escape fraction, with LAE selection preferentially detecting galaxies which have the highest escape fractions given their dust content. The fact that a large escape of Ly? photons is reached by z ~ 6 implies that better constraints on this quantity at higher redshifts might detect re-ionization in a way that is uncoupled from the effects of dust.

255

Design of remote handling equipment for the ITER NBI  

The ITER machine has three Neutral Beam Injectors (NBIs) placed tangential to the plasma at a minimum radius of 6.25 m. During operation, neutrons produced by the D-T reactions will irradiate the NBI structure and it will become radioactive. Radiation levels will be such that all subsequent maintenance of the NBIs must be carried out remotely. The presence of tritium and possibly radioactive dust requires that precautions be taken during maintenance to prevent the escape of these contaminants beyond the prescribed boundaries. The scope of this task is both the development of remote maintenance procedures and the design of the remote handling equipment to handle the NBIs. This report describes the design of remote handling tools for the ion source and its filaments, transfer cask, maintenance time, manufacturing schedule and cost estimation. (author)

256

Development of portable flow calibrator  

In the nuclear facilities, air sniffer system is often utilized to evaluate atmospheric concentration of radioactivity in the working environment. The system collects airborne dust on the filter during some sampling period. In this method, total air flow during the sampling period is an important parameter to evaluate the radioactivity concentration correctly. Therefore, calibration for the flow meter of air sniffer system must be done periodically according to Japan Industry Standards (JIS). As we have had to available device to calibrate the flow meter in the working area, we had to remove the flow meters from the installed place and carry them to another place where calibration can be made. This work required a great deal of labor. Now we have developed a portable flow calibrator for air sniffer system which enables us to make in-site calibration of the flow meter in the working area more easily. This report describes the outline of portable flow calibrator and it`s experimental results. (author).

257

Broad-band optical polarimetric studies towards the Galactic young star cluster Berkeley 59  

We present multiwavelength optical linear polarimetric observations of 69 stars towards the young open cluster Berkeley 59. The observations reveal the presence of three dust layers located at distances of ˜300, ˜500 and ˜700 pc. The dust layers produce a total polarization PV˜ 5.5 per cent. The mean values of polarization and polarization angles due to the dust layers are found to increase systematically with distance. We show that polarimetry in combination with the (U-B)-(B-V) colour-colour diagram yields a better identification of cluster members. The polarization measurements suggest that the polarization due the intracluster medium is ˜2.2 per cent. An anomalous reddening law exists for the cluster region, indicating a relatively larger grain size than that in the diffuse interstellar medium. The spatial variation of polarization and colour excess E(B-V) are found to increase with radial distance from the cluster centre, whereas ?V and ?max are found to decrease with increasing radial distance from the cluster centre. About 40 per cent of cluster members show the signatures of either intrinsic polarization or rotation in their polarization angles. There is an indication that the starlight of the cluster members might have been depolarized because of non-uniform alignment of dust grains in the foreground dust layers and in the intracluster medium.

258

The Central Region of NGC4696: Manifestation of the Physics of Mergers?  

Massive, dominant ellipticals with attendant emission-line gas, dust and hot, heavy X-ray emitting coronae lie at the very centers of galaxy clusters. The physics of these complex, high pressure regions remains controversial: Are cooling flows responsible? Do mergers dominate, with massive accretion events triggering an array of phenomena? Is the AGN crucial? A major impetus to understanding the physics of these regions will come with Chandra. NGC4696 in the Centaurus galaxy cluster is archetypal. WFPC2 images have shown a dramatic bifurcation between gas and dust. The nucleus itself is seen to be a compact triple, with two blue components straddling a third red one. We propose to obtain STIS long- slit spectra { omannumeral1} along a line-emission filament and { omannumeral2} along a dust filament: are we witnessing physical separation of gas and dust, as in comet ion/dust tails, due to late stage merger physics; or are very high velocities, due to powerful AGN influences, shifting emission lines out of filters? Is the HAlpha+NII filament a shock, responsible for the known off-center X-ray peak? { omannumeral3} A third spectrum will be across the compact 0.26'' triple nucleus: is it a multiple nucleus confirming the merger scenario; or a disk around a black-hole, allowing mass determination; or the first double optical synchrotron jet; or a gravitational lens? A wealth of vital physical and kinematical data will result from these carefully selected spectra.

259

Investigation of techniques to improve continuous air monitors under conditions of high dust loading in environmental setting. 1998 annual progress report  

'Improvement in understanding of the deposition of ambient dust particles on ECAM (Environmental Continuous Air Monitor) filters, reduction of the alpha-particle interference of radon progeny and other radioactive aerosols in different particle size ranges on filters, and development of ECAM''s with increased sensitivity under dusty outdoor conditions. As of May 1, 1998 (1/2 year into the project) the research-prototype 30-cm pulsed ionization chamber (PIC) is assembled and operational with an alpha particle energy resolution of better than 45 keV for 5-MeV alpha particles. Measurements of spectral resolution for alpha particles from radon decay products have been made as a function of filter type and dust loading conditions. So far, a study of ten filter types has found that the best combination of resolution and throughput is obtained with 3.0 \\265m Millipore fluoropore and 1.0 \\265m Corning FNMB filters. Experiments with gypsum and Portland cement dust in the size range 1 to 20 \\265m indicate significant degradation in alpha particle resolution for dust loading above about 0.5 mg cm{sup -2}. Study of metalized films for possible use as a PIC window indicate a minimum broadening of 5-MeV alpha particle peaks from 43 (no film) to 301 keV (with film) for AVR film type B8 (0.20 mg cm{sup -2} polycarbonate). A modified ECAM sampling head, equipped with an optical microscopy system feeding data to a high resolution video data capture and logging instrument, was constructed. This system will enable time-lapse study of dust build-up on ECAM filters and formation of dendrite structures that can reduce alpha-particle resolution.'

260

Supercritical Carbon Dioxide Ligands for Extracting Actinide Metal Ions from Porous Solids  

Numerous types of actinide-bearing waste materials are found throughout the DOE complex. Most of these wastes consist of large volumes of non-hazardous materials contaminated with relatively small quantities of actinide elements. Separation of these wastes into their inert and radioactive components would dramatically reduce the costs of stabilization and disposal. For example, the DOE is responsible for decontaminating concrete within 7000 surplus contaminated buildings. The best technology now available for removing surface contamination from concrete involves removing the surface layer by grit blasting, which produces a large volume of blasting residue containing a small amount of radioactive material. Disposal of this residue is expensive because of its large volume and fine particulate nature. Considerable cost savings would result from separation of the radioactive constituents and stabilization of the concrete dust. Similarly, gas diffusion plants for uranium enrichment contain valuable high-purity nickel in the form of diffusion barriers. Decontamination is complicated by the extremely fine pores in these barriers, which are not readily accessible by most cleaning techniques. A cost-effective method for the removal of radioactive contaminants would release this valuable material for salvage.

 
 
 
 
261

NASA & IPY - Search Results for Educators - Images & Video  

Layered Ice Deposits Near North Pole of Mars: 09.20.07 -- This false-color ... they may be due to variations in dust composition within the layered deposits. ... Island off Greenland: 06.03.07 -- Long connected to Greenland's coast by ice, ... Draining from the East Antarctic Ice Sheet is a river of ice nearly 800 kilometers long.

262

Ridley Island: a progress report. [Canada  

This paper describes the design and construction of the Ridley Island coal export terminal in Canada, which is due for completion at the end of 1983. The handling facilities are described and the layout of the terminal is outlined. Measures have been taken to control coal dusts from the railhead, the dock, and the conveying system.

263

Duct penetration. Stutzendurchfuehrung  

A compensating ring is provided between a shoulder of the duct and the supporting surface of the RDB lid, whose height and thermal coefficient of expansion are selected so that the change of length of the dust and lid material due to thermal expansion in the area if the shoulder is compensated for to the section giving a force locking connection.

264

Can a dust dominated universe have accelerated expansion?  

Recently, there has been suggestions that the apparent accelerated expansion of the universe is due not to a cosmological constant, but rather to inhomogeneities in the distribution of matter. In this work, we investigate the behavior of the dust dominated inhomogeneous Lemaitre-Tolman-Bondi universe models, and show that they do not permit accelerated cosmic expansion.

265

A Model of Oxygen Isotopic Fractionation in the Proto-Solar Nebula due to Nebular Lightning  

In order to explain the fractionation of oxygen isotopes along a slope=1 line we have developed a model of the oxygen isotopic evolution of dust in the solar nebula due to nebular lightning. The model produces both average an statistical results.

266

Trace element content of chondritic cosmic dust: Volatile enrichments, thermal alterations, and the possibility of contamination  

Trace element abundances in 51 chondritic Interplanetary Dust Particles (IDP's) were measured by Synchrotron X-Ray Fluorescence (SXRF). The data allow us to determine an average composition of chondritic IDP's and to examine the questions of volatile loss during the heating pulse experienced on atmospheric entry and possible element addition due to contamination during atmospheric entry, stratospheric residence, and curation.

267

Age-sex incidence in symptomatic allergies: an excess of females in the child-bearing years.  

Eight-hundred and one patients amongst 1912 referred for skin testing because of suspected allergies were found suffering from asthma due to the house-dust mite or from grass pollenosis. They were analysed in terms of sex, age of referral and age of onset of symptoms. Amongst children referred below...

268

Prevalence and risk factors for obstructive respiratory conditions among textile industry workers in Zimbabwe, 2006  

Introduction: Workers in the cotton processing industries risk developing obstructive respiratory conditions due to prolonged exposure to cotton dust. We noted a tenfold increase in asthma among workers in a Textile Manufacturing Company. We determined the prevalence of respiratory obstructive condi...

269

On the spectrum of relativistic Schrödinger equation in finite differences  

We develop a method for constructing asymptotic solutions of finite-difference equations and implement it to a relativistic Schroedinger equation which describes motion of a selfgravitating spherically symmetric dust shell. Exact mass spectrum of black hole formed due to the collapse of the shell is determined from the analysis of asymptotic solutions of the equation.

270

Does radioactive contamination affect the shell morphology of the pond snail Lymnaea stagnalis in the exclusion zone of the Chernobyl NPP (Ukraine)?  

A distinct external shell abnormality, coarse seam, was found in a high percentage of the pond snail Lymnaea stagnalis (L.) collected near Chernobyl Nuclear Power Plant (NPP), Ukraine. The negative cytogenetical and hematological effects of long-term irradiation on pond snails in the Chernobyl Exclusion Zone have been repeatedly reported; consequently, it has been assumed that radioactivity may also affect shell morphology. However, due to the absence of this shell abnormality in pond snails collected from two radioactive sites in Russia, it can be concluded that the appearance of abnormal shells in snail population near Chernobyl NPP cannot directly be explained by the radioactive contamination.

271

Comparison of international back-end solutions for low and intermediate level wastes  

In spite of the fact that the use of radioactivity in different applications demands maximum attention due to its potential risks, a unique assessment of the matter is impossible to reach. When compared to other hazardous waste categories or even domestic waste, the amount of radioactive waste generated is not significant. The objective of this work is to analyze the variation associated to the amount of radioactive waste storage in many places. The results showed that this amount is increasing, a fact coherent to the growth in the last years of both the nuclear energy applications and the share of nuclear energy in the global market. (author)

272

SELF SINTERING OF RADIOACTIVE WASTES  

A method is described for disposal of radioactive liquid waste materials. The wastes are mixed with clays and fluxes to form a ceramic slip and disposed in a thermally insulated container in a layer. The temperature of the layer rises due to conversion of the energy of radioactivity to heat boillng off the liquid to fomn a dry mass. The dry mass is then covered with thermal insulation, and the mass is self-sintered into a leach-resistant ceramic cake by further conversion of the energy of radioactivity to heat.

273

Workshop on measurement quality assurance for ionizing radiation: Proceedings  

This workshop was held to review the status of secondary level calibration accreditation programs, review related measurement accreditation programs, document lessons learned, and to present changes in programs due to new national priorities involving radioactivity measurements. Contents include: fundamentals of measurement quality assurance (MQA), standards for MQA programs; perspectives and policies; complete MQA programs; future MQA programs; QA/QC programs--radioactivity; QA/QC programs--dosimetry; laboratory procedures for QA/QC; in-house control of reference dosimetry laboratories; in-house controls of radioactivity laboratories; and poster session. Selected papers are indexed separately for inclusion in the Energy Science and Technology Database.

274

Monitoring of radioactivity in drinking water; Control de la radiactividad en las aguas de consumo humano  

Radioactivity is a physical phenomenon whose presence in water is monitored due to its potential capability to induce deleterious effects on human health. In this article the effects that can be caused by radioactivity as well as the way in which regulations establish how to perform a monitorization of water that enables us to ascertain that the radiological quality of water is in agreement with the accepted standard of quality of life are analyzed. Finally the means available to know the content of radioactivity in water together with some clues on how to remove it from water are described. (Author) 5 refs.

275

Process for improving the security of storage and transport of fuel dust and fuel dust treated by the process. Verfahren zur Verbesserung der Lager- und Transportsicherheit von Brennstoffstaub und nach dem Verfahren behandelter Brennstoffstaub  

In a process for improving the security of storage and transport of fuel dust, the fuel dust is mixed with a safe dust in such quantities that after mixing the grains of fuel dust are largely surrounded by grains of the safe dust. The fuel dust is mixed with an inert safe dust to improve the protective effect.

276

Cosmology of the Solar System  

The early solar system accreted from ice crystals, which encapsulated the refractory elements. Ice was needed to bind the smallest particles, so accretion only occurred in the outer solar system. Solar wind gusts expelled dust in the inner solar system to where it became accreted into the giant planets. Thus, the original solar system comprised four giant planets, accreted from ice and dust. Their initial accretion was rapid, forming rocky iron cores from the refractory elements. But due to their great orbital radii, the entire process required more than 50 million years, so the bulk of the process was cold. Studies of young Sun-like stars show that hydrogen gas is expelled from the nebula before the accretion had hardly begun. As a result these are all solid bodies and not gas giants. The recognition that Jupiter is solid was masked by a high energy impact which occurred 6,000 years BP. The hot gases still streaming from the impact crater heat the atmosphere, forming the GRS, while the planet remains frozen. The temperature excesses, thought to be primordial, are an important factor in the gas giant assumption. Scientists have come close to recognizing the true nature of these bodies in recent years, due to the study of clathrates beneath the our oceans. These strong, low density structures of water molecules form naturally at low temperature and high pressure, exactly the conditions in the large bodies of the outer solar system. Their properties are responsible for the low average density of the giant planets. Clathrates encapsulate foreign molecules, such as methane. One expert has proposed that clathrates are the most abundant form of matter in the outer solar system - the Galilean moons, Pluto, Charon and the KBOs. However, until now, no one has suggested that the giant planets themselves are so composed, moreover that these bodies alone comprised the original solar system. The terrestrial planets result from later, high energy impacts on the giant planets. Fortunately, the birth of a new terrestrial planet, Venus, occurred within proto-history and the entire process is documented in ancient writings. It formed as a result of the impact on Jupiter cited above, expelling a plasma cloud several times the mass of Venus and thousands of times the volume of Jupiter. Most escaped Jupiter and entered an eccentric planetary orbit, while contracting to a star-like proto-Venus, with a temperature above 10,000K. Its perihelion, close to the ancient interior orbit of Mars, and its aphelion, at the orbit of Jupiter, gave it a period of some five years. But its great orbital energy was rapidly reduced, due to repeated interactions with Mars and the Sun at perihelion. The tidal force of the Sun and its magnetic field combined to heat the ionized, fluid body, slowing its orbital velocity. Each pass reheated it, further reducing its aphelion and increasing the frequency of interactions. Its repeated heating caused the out-gassing of most lighter elements to space by Jeans escape. Thus the loss of orbital energy resulted in the increasing of its average density from 1.3 gm/cm3, the density of Jupiter, to over 5.5 g/cm3, the density of Venus. This is how all terrestrial planets were formed. This catastrophic birth ensures the concentration of iron in the core, the rising of hot radioactive elements Th, Ur, K, and the less dense materials to the surface. Although the volatiles, H2, C, N, O2, which comprised the vast majority of the rebounded cloud, were initially lost, they remained in the inner solar system, to be captured later by the proto-planet as it cooled or by extant planets, thereby rapidly providing the elements necessary for life.

277

Helium isotopic abundance variation in nature  

The isotopic abundance of helium in nature has been reviewed. This atomic weight value is based on the value of helium in the atmosphere, which is invariant around the world and up to a distance of 100,000 feet. Helium does vary in natural gas, volcanic rocks and gases, ocean floor sediments, waters of various types and in radioactive minerals and ores due to {alpha} particle decay of radioactive nuclides.

278

Radioactivity measurement in the granites of North Karnataka, India and its radiological implications  

The natural radioactivities due to uranium, thorium and potassium in granite samples contribute to the radiation dose received by human beings significantly. It is essential to evaluate the activity levels of these nuclides for the assessment of natural radiation dose. The natural radioactivity levels of some granite samples collected from different quarries of North Karnataka, India are estimated using high-resolution gamma ray spectrometry technique and the results are reported in this paper.

279

Impact Produced and Mobilized Dust in the Martian Atmosphere  

The objective of this work is to study possible mechanisms of new dust production and existing dust entrainment after impacts of meteoroids onto Mars and to assess the possible relationship to dust clouds. We use detailed numerical simulations based on the SOVA multi-dimensional multi-material hydrocode [1]. In the first run of simulations, partially described in [2], only the dust ejected from the crater was taken into account. In the process of ejection soil density decreases near the cavity boundary. At the moment when the density falls below some critical value the solid material is replaced by a set of discrete particles (dust, boulders) of equivalent mass [3]. The distribution of particles by sizes was taken according experimental data obtained in the course of large-scale TNT and nuclear explosions on the Earth's ground [4]. The radius of impactor was varied from 1 to 100 m. The lowest value corresponds to high strength meteoroids passing through the rarefied Martian atmosphere without substantial fragmentation and deceleration. The impact velocity was taken to be 11 and 20 km/s. In all the variants the mass of the dust ejected from the forming craters was about 10 M, where M is the impactor mass. It was suggested [5] that the dust may be mobilized even if the impactor does not reach the ground surface. To check this idea the code was modified to take into account blast produced impulsive winds blowing the preexisting dust from the surface by mechanism similarly to that of the stationary winds [6]. Turbulent viscosity and diffusion were taken into acount. Some portions of dust are deposited on the surface due to gravity. The particles striking the surface increase a flux of the suspended dust. The saltation thresholds were taken according [7-8]. For a 1 m radius stony asteroid releasing its energy (0.15 kt TNT) at an altitude of about 100 m above the surface after first two seconds the mass of the dust in the air was 3.5 M, and after 15 s it decreased to 2.8 M. For a disrupted meteoroid releasing 3/4 of its energy in a long cylindrical channel with the diameter of 17 m the dust is removed at a distance of 700 m from the impact point. At 20 s after the impact the lifted mass is about 0.1 M. In both cases the size of the columnar shaped dust cloud exceeded 1 km. The risen mass in the air is larger than that in a typical dust devil [8-9]. Addition mechanisms such as thermal layer effect due to radiation, explosion of the upper soil layer under decompression, interaction between the ballistic wave and the surface [5,10], interactions between the natural convective and impact generated plumes, impact induced and natural winds and others may produce vortices and increase the amount of mass in the impact produced clouds. The work was supported by NASA Grant NRA 98-OSS-08 JURISS. References:[1] Shuvalov V.V. 1999. Shock Waves 9(6), 391-390[2] Nemtchinov I.V., et al., 1999 5th Int. Conf. on Mars, abstract #6081[3] Teterev A.V. 1999. J. Impact Engn. 23, 921-927[4] Adushkin V.V. and Spivak A.A. 1992. Geomechanics of large scale explosions. Nedra, Moscow, 320 p (in Russian)[5] Rybakov V.A., et al., 1997. JGR 102(E4), 9211-9220.[6] Greeley R. and Iversen J.D. 1985. Wind as a geological process. Cambridge Univ. Press, New York, 330p.[7] Greeley r., et al., 1980. GRL, 7, 121-124[8] Greeley R, et al., 1992. Mars (Eds. Kieffer H.H. et al.) Univ. Arizona Press, Tucson and London, 770-788 [9] Thomas P. and Gierasch P. 1985. Science, 230, 175-177[10] Kosarev I.B. et al. 2000. Meteoritics and Planetary Sci., 3115, Supplement, A91-A92

280

African dust outbreaks over the Mediterranean Basin during 2001-2011: PM10 concentrations, phenomenology and trends, and its relation with synoptic and mesoscale meteorology  

The occurrence of African dust outbreaks over the whole Mediterranean Basin has been identified on an 11-yr period (2001-2011). In order to evaluate the impact of such mineral dust outbreaks on ambient concentrations of particulate matter, PM10 data from regional and suburban background sites across the Mediterranean area were compiled. After identifying the daily influence of African dust, a methodology for estimating natural dust contributions on daily PM10 concentrations was applied. Our results reveal that African dust outbreaks occur with much higher frequency in southern areas of the Mediterranean, from 30 to 37% of the annual days, whereas they take place less than 20% of the annual days in northern sites. The central Mediterranean emerges as a transitional area, with slightly higher frequency of dust episodes in its lower extreme when compared to equivalent areas in western and eastern sides of the Basin. A decreasing south to north gradient of African dust contribution to PM10 is patent across the Mediterranean. Our study demonstrates that this gradient may be mainly explained by the latitudinal position. A longitudinal increasing trend of African dust contribution to PM10 is also observed from 25° E eastwards, and is due to the annual occurrence of intense dust episodes. Thus, the slightly higher frequency of African dust episodes over the lower part of Central Mediterranean is compensated by its moderately lower intensity. Concerning seasonality patterns and intensity characteristics, a clear summer prevalence is observed in the western part, with low occurrence of severe episodes (daily dust averages over 100 ?g m-3 in PM10); no seasonal trend is detected in the central region, with moderate-intensity episodes; and significantly higher contributions are common in autumn-spring in the eastern side, with yearly occurrence of various severe episodes. Overall, African dust emerges as the largest PM10 source in regional background southern areas of the Mediterranean (35-50% of PM10), with seasonal peak contributions to PM10 up to 80% of the total mass. The multi-year study of African dust episodes and their contributions to PM10 concentrations allowed us to identify a consistent decreasing trend in the period 2006/2007 to 2011 in 4 of the 17 studied regions, all of them located in the NW of the Mediterranean. The observed trend is almost parallel to the NAO (North Atlantic Oscillation) index for the summer period, progressively more negative since 2006 onwards. As a consequence, a sharp change in the atmospheric circulation over the last 5 yr (a similar negative NAO period occurred in the 1950 decade) have affected the number of African dust episodes and their mean contribution to PM10 in the NW part of the Mediterranean. The investigation of summer temperatures at 850 hPa suggest that warm air accomplishing African dust air masses moved anomalously through the central Mediterranean in the 2007-2008 period, whereas it was displaced atypically to the NW African coast and the Canary Islands in the 2009-2011 period.

 
 
 
 
281

Experiments and Simulations of Particle Flows in a Magnetized Dust Torus  

Abstract An overview is given of the confinement and dynamical phenomena observed in experiments and simulations of magnetized dust tori. Due to the presence of gravity, a strongly inhomogeneous velocity field is found along the circumference of the torus. The simulations show that the dust flow, which is unsheared and nearly incompressible, exhibits a distinct shell structure, which can be understood by rapid frictional cooling and strong Coulomb coupling. At lower frictional damping, the symmetry of the flow can be spontaneously broken, leading to a region of strong velocity shear and excitation of Kelvin-Helmholtz instabilities. New experimental evidence of counterflows is found ( 2012 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

282

Global climatic effects of atmospheric dust from an asteroid or comet impact on Earth  

Impacts of comets and small (ca. 10 km) asteroids with Earth-frequent events over geologic time-would generate atmospheric dust in amounts orders of magnitude greater than historically large volcanic explosions. Three-dimensional atmospheric model simulations show that climatic effects of such impacts would include drastic cooling of land surfaces due to interception of sunlight by high-altitude dust. Unlike earlier one-dimensional calculations, the three-dimensional results indicate that large areas of the planet would escape freezing. They also suggest catastrophic changes in the hydrological cycle

283

CCD observations of gas and dust in NGC 4696 - Implications for cooling flows?  

The nearby radio elliptical galaxy NGC 4696 is a prominent candidate for interpretation as a galaxy that serves as host to a cooling flow. While the optical emission lines of 'cooling-flow galaxies' have been interpreted as indications of thermally unstable condensations, both continuum and narrow-band direct CCD images indicate that the dust properties are essentially normal; this favors interpretation in terms of external infall. Due consideration of the thermal interaction between infalling material and hot gas leads to an acknowledgement of the consistency between an observed dust lane energetic output that is balanced by an X-ray gas energy input via electron-heat conduction.

284

H/sub 2/ fluorescence and the diffuse galactic light in the vacuum ultraviolet  

Fluorescence by molecular H/sub 2/ within the Lyman and Werner bands, as well as to continuum levels of the X/sup 1/S/sub g/ /sup +/ state, occurs at wavelengths l< or =0.18 mm. This emission is shown to be of intensity comparable to that scattered by dust over the same wavelength range in diffuse clouds. The implied increase in dust albedo in the vacuum ultraviolet (VUV) is likely due to this effect. Thus the small particles responsible for VUV extinction are of conventional chemical composition, i.e., absorbing oxides, silicates, or carbons.

285

Health Hazard Evaluation Report HETA 84-050-1595, PPG Industries, Mt. Zion, Illinois  

Environmental and breathing zone samples were analyzed for adipic-acid and total and respirable dust at PPG Industries, Mount Zion, Illinois, January and September, 1984. The evaluation was requested to investigate employee exposure to Lucor and wood flour, used during the off/bearing of flat glass. The author concludes that a health hazard due to exposure to Lucor does not exist at the facility. It could not be determined if a health hazard from exposure to wood dusts existed in the past, since the use of wood flour had been discontinued. Recommendations include using a heavy duty industrial vacuum cleaner during cleanup operations and practicing good housekeeping.

286

IRAS maps of galactic emission and the zodiacal bands  

We present maps of the IRAS large-scale 100 {mu}m emission, after subtraction of a physical model for the zodiacal emission. There is a good detailed agreement with maps of the H I column density, assuming a normal gas-to-dust ratio, but several areas of very low dust column density can be identified. These may be of considerable importance for observations in the UXV band. Towards the Galactic Centre the 100 {mu} m emissivity per hydrogen atom increases, due to the increased intensity of starlight, and towards the anticentre it declines as we look out into the outer part of the galactic disc.(Author).

287

Wind-driven particle mobility on Mars: Insights from Mars Exploration Rover observations at \\  

The ripple field known as 'El Dorado' was a unique stop on Spirit's traverse where dust-raising, active mafic sand ripples and larger inactive coarse-grained ripples interact, illuminating several long-standing issues of Martian dust mobility, sand mobility, and the origin of transverse aeolian ridges. Strong regional wind events endured by Spirit caused perceptible migration of ripple crests in deposits SSE of El Dorado, erasure of tracks in sandy areas, and changes to dust mantling the site. Localized thermal vortices swept across El Dorado, leaving paths of reduced dust but without perceptibly damaging nearly cohesionless sandy ripple crests. From orbit, winds responsible for frequently raising clay-sized dust into the atmosphere do not seem to significantly affect dunes composed of (more easily entrained) sand-sized particles, a long-standing paradox. This disparity between dust mobilization and sand mobilization on Mars is due largely to two factors: (1) dust occurs on the surface as fragile, low-density, sand-sized aggregates that are easily entrained and disrupted, compared with clay-sized air fall particles; and (2) induration of regolith is pervasive. Light-toned bed forms investigated at Gusev are coarse-grained ripples, an interpretation we propose for many of the smallest linear, light-toned bed forms of uncertain origin seen in high-resolution orbital images across Mars. On Earth, wind can organize bimodal or poorly sorted loose sediment into coarse-grained ripples. Coarse-grained ripples could be relatively common on Mars because development of durable, well-sorted sediments analogous to terrestrial aeolian quartz sand deposits is restricted by the lack of free quartz and limited hydraulic sediment processing. Copyright 2008 by the American Geophysical Union.

288

Long-range Transport of Asian Dust Storms: A Satellite/Surface Perspective on Societal and Scientific Influence  

Among the many components contributing to air pollution, airborne mineral dust plays an important role due to its biogeochemical impact on the ecosystem and its radiative forcing effect on the weather/climate system. As much as one-third to half of the global dust emissions, estimated about 800 Tg, are introduced annually into Earth's atmosphere from various deserts in China. Asian dust storm outbreaks are believed to have persisted for hundreds and thousands years over the vast territory of north and northwest China, but not until recent decades that many studies reveal the compelling evidence in recognizing the importance of these eolian dust particles for forming Chinese Loess Plateau and for biogeochemical cycling in the North Pacific Ocean to as far as in the Greenland ice-sheets through long-range transport. The Asian dust and air pollution aerosols can be detected by its colored appearance on current Earth observing satellites and its evolution monitored by satellite and surface network. In this paper, we will demonstrate the capability of a new satellite algorithm, called Deep Blue, to retrieve aerosol properties, particularly but not limited to, over bright-reflecting surfaces such as urban areas and deserts. Recently, many field campaigns were designed and executed to study the compelling variability in spatial and temporal scale of both pollution-derived and naturally occurring aerosols, which often exist in high concentrations over eastern Asia and along the rim of the western Pacific. We will provide an overview of the outbreak of Asian dust storms, near source/sink and their evolution along transport pathway, from space and surface observations. The climatic effects and societal impacts of the Asian dusts will be addressed in depth. (to be presented in the International Workshop on Semi-Arid Land Surface-

289

A Nano-Dust Analyzer on the Moon  

Lunar microcrater analysis [Gruen et al., Icarus, 62, 244-272, 1985] showed that there is an excess of nanometer-sized craters over those expected from interplanetary grains. This excess has been interpreted as due to high-speed ejecta particles from bigger meteoroid impacts onto the lunar surface. Recently, the STEREO WAVES instruments recorded a large number of intense electric field signals, which were interpreted as impacts from nanometer sized particles striking the spacecraft with velocities of about the solar wind speed [Meyer-Vernet, N. et al., Solar Physics, 256, 463, 2009]. This high flux and strong spatial and/or temporal variations of nanometer sized dust grains appears to be uncorrelated with the solar wind properties. A new highly sensitive Nano Dust Analyzer is being developed within NASA's Heliophysics Program to confirm the existence of the so-called nano-dust particles, characterize their impact parameters, and measure their chemical composition. Such an instrument is placed on the moon can at the same time test the hypothesis of an enhanced high-speed ejecta flux near the lunar surface. The instrument is based on the Cassini Dust Analyzer, CDA [Srama, R. et al., SSR, 114, 465, 2004] and the LDEX instrument that is currently being developed to be flown on the LADEE mission to the Moon. By applying technologies implemented in solar wind instruments and coronagraphs the highly sensitive dust analyzer will be able to be pointed towards the solar direction. The measurements will enable us to identify the source of the dust by comparing their elemental composition with that of larger micrometeoroid particles of cometary and asteroid origin or with that of lunar regolith particles. In addition the flux direction of these different particle types will be significantly different: while high speed ejecta particles will arrive from shallow angles with respect to the lunar surface heliospheric nano-dust particles will arrive mostly from the solar hemisphere.

290

Dust extinction of the stellar continua in starburst galaxies: The ultraviolet and optical extinction law  

We analyze the International Ultraviolet Explorer (IUE) UV and the optical spectra of 39 starburst and blue compact galaxies in order to study the average properties of dust extinction in extended regions of galaxies. The optical spectra have been obtained using an aperture which matches that of IUE, so comparable regions within each galaxy are sampled. The data from the 39 galaxies are compared with five models for the geometrical distribution of dust, adopting as extinction laws both the Milky Way and the Large Magellanic Cloud laws. The commonly used uniform dust screen is included among the models. We find that none of the five models is in satisfactory agreement with the data. In order to understand the discrepancy between the data and the models, we have derived an extinction law directly from the data in the UV and optical wavelength range. The resulting curve is characterized by an overall slope which is more gray than the Milky Way extinction law's slope, and by the absence of the 2175 A dust feature. Remarkably, the difference in optical depth between the Balmer emission lines H(sub alpha) and H(sub beta) is about a factor of 2 larger than the difference in the optical depth between the continuum underlying the two Balmer lines. We interpret this discrepancy as a consequence of the fact that the hot ionizing stars are associated with dustier regions than the cold stellar population is. The absence of the 2175 A dust feature can be due either to the effects of the scattering and clumpiness of the dust or to a chemical composition different from that of the Milky Way dust grains. Disentangling the two interpretations is not easy because of the complexity of the spatial distribution of the emitting regions. The extinction law of the UV and optical spectral continua of extended regions can be applied to the spectra of medium- and high-redshift galaxies, where extended regions of a galaxy are, by necessity, sampled.

291

Dust exposure and the risk of cancer in cement industry workers in Korea.  

BACKGROUND: Cement is used widely in the construction industry, though it contains hazardous chemicals such as hexavalent chromium. Several epidemiological studies have examined the association between cement dust exposure and cancer, but these associations have proved inconclusive. In the present study, we examined the association between dust exposure and cancer in cement industry workers in Korea. METHODS: Our cohort consisted of 1,324 men who worked at two Portland cement manufacturing factories between 1997 and 2005. We calculated cumulative dust exposures, then categorized workers into high and low dust exposure groups. Cancer cases were identified between 1997 and 2005 by linking with the national cancer registry. Standardized incidence ratios (SIRs) were calculated for all workers and the high and low dust exposure groups, respectively. RESULTS: The SIR for overall cancers in all workers was increased (1.35, 95% CI: 1.01-1.78). The SIR for stomach cancer in the high dust exposure group was increased (2.18, 95% CI: 1.19-3.65), but there was no increased stomach cancer risk in the low dust exposure group. The SIR for rectal cancer in all workers was increased (3.05, 95% CI: 1.32-6.02). Rectal cancer risk was similar in the high and low exposure groups. CONCLUSIONS: Our findings suggest a potential association between exposure in the cement industry and an increased risk of stomach and rectal cancers. However, due to the small number of cases, this association should be further investigated in a study with a longer follow-up period and adjustment for confounders. Am. J. Ind. Med. © 2012 Wiley Periodicals, Inc. PMID:23109188

292

Dust Accumulation and Solar Panel Array Performance on the Mars Exploration Rover (MER) Project  

One of the most fundamental design considerations for any space vehicle is its power supply system. Many options exist, including batteries, fuel cells, nuclear reactors, radioisotopic thermal generators (RTGs), and solar panel arrays. Solar arrays have many advantages over other types of power generation. They are lightweight and relatively inexpensive, allowing more mass and funding to be allocated for other important devices, such as scientific instruments. For Mars applications, solar power is an excellent option, especially for long missions. One might think that dust storms would be a problem; however, while dust blocks some solar energy, it also scatters it, making it diffuse rather than beamed. Solar cells are still able to capture this diffuse energy and convert it into substantial electrical power. For these reasons, solar power was chosen to be used on the 1997 Mars Pathfinder mission. The success of this mission set a precedent, as NASA engineers have selected solar power as the energy system of choice for all future Mars missions, including the Mars Exploration Rover (MER) Project. Solar sells have their drawbacks, however. They are difficult to manufacture and are relatively fragile. In addition, solar cells are highly sensitive to different parts of the solar spectrum, and finding the correct balance is crucial to the success of space missions. Another drawback is that the power generated is not a constant with respect to time, but rather changes with the relative angle to the sun. On Mars, dust accumulation also becomes a factor. Over time, dust settles out of the atmosphere and onto solar panels. This dust blocks and shifts the frequency of the incoming light, degrading solar cell performance. My goal is to analyze solar panel telemetry data from the two MERs (Spirit and Opportunity) in an effort to accurately model the effect of dust accumulation on solar panels. This is no easy process due to the large number of factors involved. Changing solar flux (the amount of solar energy reaching the planet), solar spectrum, solar angle, rover tilt, and optical depth (the opacity of the atmosphere due to dust) were the most significant. Microsoft Excel and Visual Basic are used for data analysis. The results of this work will be used to improve the dust accumulation and atmosphere effects model that was first created after the Mars Pathfinder mission. This model will be utilized and applied when considering the design of solar panel array systems on future Mars projects. Based on this data, and depending upon the tenure and application of the mission, designers may also elect to employ special tools to abate dust accumulation, or decide that the expected level of accumulation is acceptable.

293

ICP-MS nebulizer performance for analysis of SRS high salt simulated radioactive waste tank solutions ({number_sign}3053)  

High Level Radioactive Waste Tanks at the Savannah River Site are high in salt content. The cross-flow nebulizer provided the most stable signal for all salt matrices with the smallest signal loss/suppression due to this matrix. The DIN exhibited a serious lack of tolerance for TDS; possibly due to physical de-tuning of the nebulizer efficiency.

294

Radioactivity of household water  

The guide presents the safety requirements to limit the radiation exposure due to the radioactive nuclides in household water. The requirements does not apply during extraordinary circumstances, as during fallout due to an accident at a nuclear power station. (2 refs., 1 tab.).

295

Metastatic follicular carcinoma of the thyroid presenting with thyrotoxic induced impaired control of diabetes mellitus.  

We report a patient with pulmonary and bony metastases due to follicular carcinoma of the thyroid, occurring 12 years after the initial diagnosis. This was brought to light by worsening diabetic control due to thyrotoxicosis from functioning malignant thyroid tissue. Following radio-active iodine th...

296

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297

Radon exposure experiments on rats and mice  

Experimental animals were exposed to about 0.01 Ci radon/ml of chamber air. The concentration of radon was measured by a double screen ionization chamber. The concentration of dust free daughters in the chamber is decreased by radioactive decay, attachment to dust particles and deposition to the chamber wall. To express the rate of decrease, the attachment constant k/sub p/ and the deposition constant k/sub w/ were introduced in addition to the radioactive decay constant. The values of k/sub p/ and k/sub w/ were experimentally obtained by using a semiconductor detector installed on the chamber wall. The diffusion constant of daughter atoms estimated from the deposition constant k/sub w/ was in good agreement with those obtained by other methods. The absorbed lung doses to rats and mice were 8.0 and 18.9 rads, respectively, when radon was introduced into the test chamber at a level of 0.01 Ci/ml. The retention efficiency of the lung was approximately 2% for rats and mice. (auth)

298

Jupiter's Rings: Sharpest View  

The New Horizons spacecraft took the best images of Jupiter's charcoal-black rings as it approached and then looked back at Jupiter. The top image was taken on approach, showing three well-defined lanes of gravel- to boulder-sized material composing the bulk of the rings, as well as lesser amounts of material between the rings. New Horizons snapped the lower image after it had passed Jupiter on February 28, 2007, and looked back in a direction toward the sun. The image is sharply focused, though it appears fuzzy due to the cloud of dust-sized particles enveloping the rings. The dust is brightly illuminated in the same way the dust on a dirty windshield lights up when you drive toward a 'low' sun. The narrow rings are confined in their orbits by small 'shepherding' moons.

299

Chondrule Formation and Protoplanetary Disk Heating by Current Sheets in Non-Ideal Magnetohydrodynamic Turbulence  

We study magnetic field steepening due to ambipolar diffusion (Brandenburg & Zweibel 1994) in protoplanetary disk environments and draw the following conclusions. Current sheets are generated in magnetically active regions of the disk where the ionization fraction is high enough for the magnetorotational instability to operate. In late stages of solar nebula evolution, the surface density is expected to have lowered and dust grains to have gravitationally settled to the midplane. If the local dust-to-gas mass ratio near the midplane is increased above cosmic abundances by factors > 10^3, current sheets reach high enough temperatures to melt millimeter-sized dust grains, and hence may provide the mechanism to form meteoritic chondrules. In addition, these current sheets possibly explain the near-infrared excesses observed in spectral energy distributions (SEDs) of young stellar objects. Direct imaging of protoplanetary disks via a nulling interferometer or, in the future, a multi-band, adaptive optics coro...

300

Origin of Molecular Outflow Determined from Thermal Dust Polarization  

The observational expectation of polarization measurements of thermal dust radiation is investigated to find information on molecular outflows based on magnetohydrodynamical (MHD) and radiation transfer simulations. There are two major proposed models for the driving of molecular outflows: (1) molecular gas is accelerated by a magnetic pressure gradient or magnetocentrifugal wind mechanism before the magnetic field and molecular gas are decoupled, (2) the linear momentum of a highly collimated jet is transferred to the ambient molecular gas. In order to distinguish between these two models, it is crucial to observe the configuration of the magnetic field. An observation of a toroidal magnetic field is strong evidence that the first of the models is appropriate. In this paper, we calculated the polarization distribution of thermal dust radiation due to the alignment of dust grains along the magnetic field using molecular outflow data calculated by two-dimensional axisymmetric MHD simulations. An asymmetric dis...

 
 
 
 
301

Distribution of Chemical Elements in Attic Dust as Reflection of Their Geogenic and Anthropogenic Sources in the Vicinity of the Copper Mine and Flotation Plant  

The main aim of this article was to assess the atmospheric pollution with heavy metals due to copper mining Bu?im near Radovi?, the Republic of Macedonia. The open pit and mine waste and flotation tailings are continually exposed to open air, which leads to winds carrying the fine particles into the atmosphere. Samples of attic dust were examined as historical archives of mine emissions, with the aim of elucidating the pathways of pollution. Dust was collected from the attics of 29 houses, built between 1920 and 1970. Nineteen elements (Ag, Al, As, Ba, Ca, Cd, Co, Cr, Cu, Li, Fe, K, Mg, Mn, Na, Ni, Pb, Sr, and Zn) were analyzed by atomic emission spectrometry with inductively coupled plasma. The obtained values of the investigated elements in attic dust samples were statistically processed...

302

Acupuncture as method of treatment and arresting progress of dust-induced bronchitis  

Acupuncture is an effective therapy for treatment of dust-induced bronchitis. It can be used independently or in combination with medicaments. Fifty men were divided into two groups of 20 and 30. One group was treated by acupuncture alone, the other with combined therapy. Acupuncture produced excellent results; combined treatment, good and satisfactory results. Since acupuncture reduced the possibility of complications, allergic reactions and side effects due to medication, it is an excellent means of preventing progress of dust-induced bronchitis. Patients experience 9 months remission of symptoms after treatment with acupuncture while medical therapy alone only relieves them for 1 to 1 1/2 months. Patients with chronic dust-induced bronchitis should receive a second course of acupuncture in 6 to 8 months to prevent recurrence of symptoms and progress of disease. Because of insufficient study of lasting effects of acupuncture, final conclusions about its effectiveness cannot be made, however, current evidence indicates it is a highly useful therapy. 6 references.

303

A preliminary study on gram-negative bacteria (GNB) and their endotoxins in a gin house in India.  

The presence of byssinosis, an occupational disease found among cotton mill workers, has been well documented in different parts of the world. The disease develops due to exposure to environmental cotton dust. Evidence suggests that the causative agent for the disease is gram-negative bacteria (GNB) and their endotoxins present on the cotton fibers. An investigation was carried out in a gin house in western India. Environmental dust samples were collected by vertical elutriator (VE). Airborne dust concentrations were very high in the working environment: 2.11 mg/m3 in ginning and 0.95 mg/m3 in the press department (p Enterobacter agglomerans were the dominant bacterial flora. Results indicate that gin workers are occupationally exposed to airborne GNB and endotoxins, and require masks. PMID:17133691

304

Mode-coupling of low-frequency electromagnetic waves in dusty plasmas with temperature anisotropy  

This paper studies the effects of the presence of dust particles with variable charge, in fully ionized, homogeneous, magnetized plasma of electrons and ions, with the electrons and ions described by bi-Maxwellian distributions in the equilibrium. The dispersion relation and the absorption rate are obtained for low frequency waves, with frequencies much lower than the ion cyclotron frequency. Two branches are obtained, identified as the whistler branch and the branch of circularly polarized waves, featuring damping due to the Landau damping process and to the collisional charging of the dust particles. The effects of the anisotropy of temperature on the damping rate of low frequency waves, and on the mode coupling which was demonstrated to occur in the isotropic situation, are numerically investigated. The results obtained show that in the anisotropic case the point of mode coupling is displaced to different values of dust density, and that a new point of mode coupling may appear from the effect of the temperature anisotropy.

305

Minimum ignition energy for micro and nano flash powders  

Abstract The minimum ignition energy (MIE) of dust clouds is required to assess the electrostatic ignition risk. Recently, the growing number of accidents shows that fire and explosions occurring in fireworks industry are due to electrostatic discharge (ESD). The objective of the this paper is to discuss the various practical concerns during the handling of flash powders of various compositions containing potassium nitrate, sulfur, and aluminum in fireworks. These powders form dust clouds and cause fires and explosions because the MIEs of these dust clouds are very low. This study is carried out with powders of various sizes ranging from micron and nanometer. The measurements are done by using a 1.2-L Hartmann apparatus. The experimental results show that the MIEs for flash powders are in ...

306

A Survey and Analysis of Spitzer Infrared Spectrograph Spectra of T Tauri Stars in Taurus  

We present mid-infrared spectra of T Tauri stars in the Taurus star-forming region obtained with the Spitzer Infrared Spectrograph (IRS). For the first time, the 5-36 micron spectra of a large sample of T Tauri stars belonging to the same star-forming region is studied, revealing details of the mid-infrared excess due to dust in circumstellar disks. We analyze common features and differences in the mid-IR spectra based on disk structure, dust grain properties, and the presence of companions. Our analysis encompasses spectral energy distributions from the optical to the far-infrared, a morphological sequence based on the IRS spectra, and spectral indices in IRS wave bands representative of continuum emission. By comparing the observed spectra to a grid of accretion disk models, we infer some basic disk properties for our sample of T Tauri stars, and find additional evidence for dust settling.

307

Linear and nonlinear dynamics of current-driven waves in dusty plasmas  

The linear and nonlinear dynamics of a recently proposed plasma mode of dusty plasma is studied using kappa distribution for electrons. This electrostatic wave can propagate in the plasma due to the sheared flow of electrons and ions parallel to the external magnetic field in the presence of stationary dust. The coupling of this wave with the usual drift wave and ion acoustic wave is investigated. D'Angelo's mode is also modified in the presence of superthermal electrons. In the nonlinear regime, the wave can give rise to dipolar vortex structures if the shear in flow is weaker and tripolar vortices if the flow has steeper gradient. The results have been applied to Saturn's magnetosphere corresponding to negatively charged dust grains. But the theoretical model is applicable for positively charged dust as well. This work will be useful for future observations and studies of dusty environments of planets and comets.

308

Recent developments in coal mining technology and their impact on miners' health  

Advances in technology have significantly reduced the long-term health risks associated with underground coal mining. While the potential risks include exposure to hazardous substances and noise, the reduction of respirable dust in the workplace has been emphasized here because of the greater probability of exposure and the well-documented consequences. Since enactment of the Mine Health and Safety Act of 1969, great strides have been made in reducing worker exposure to respirable dust. As production rates continue to increase, particularly in longwall sections, continued advances in dust control technology will be required. These advances will be needed to meet existing, and perhaps even more stringent future, exposure limits. Mechanization has resulted in a significant reduction in exposure to hazards while increasing productivity. Use of remotely controlled equipment is also increasing rapidly, and efforts are underway to develop completely automated mining systems. These automated systems may further reduce the risk of health impairment due to the underground working environment. 80 refs.

309

Recent developments in coal mining technology and their impact on miners' health.  

Advances in technology have significantly reduced the long-term health risks associated with underground coal mining. While the potential risks include exposure to hazardous substances and noise, the reduction of respirable dust in the workplace has been emphasized here because of the greater probability of exposure and the well-documented consequences. Since enactment of the Mine Health and Safety Act of 1969, great strides have been made in reducing worker exposure to respirable dust. As production rates continue to increase, particularly in longwall sections, continued advances in dust control technology will be required. These advances will be needed to meet existing, and perhaps even more stringent future, exposure limits. Mechanization has resulted in a significant reduction in exposure to hazards while increasing productivity. Use of remotely controlled equipment is also increasing rapidly, and efforts are underway to develop completely automated mining systems. These automated systems may further reduce the risk of health impairment due to the underground working environment. PMID:8456343

310

Determination of parameters used to prevent ignition of stored materials and to protect against explosions in food industries  

There are always risks associated with silos when the stored material has been characterized as prone to self-ignition or explosion. Further research focused on the characterization of agricultural materials stored in silos is needed due to the lack of data found in the literature. The aim of this study was to determine the ignitability and explosive parameters of several agricultural products commonly stored in silos in order to assess the risk of ignition and dust explosion. Minimum Ignition Temperature, with dust forming a cloud and deposited in a layer, Lower Explosive Limit, Minimum Ignition Energy, Maximum Explosion Pressure and Maximum Explosion Pressure Rise were determined for seven agricultural materials: icing sugar, maize, wheat and barley grain dust, alfalfa, bread-making whea...

311

Silica exposure to excavation workers during the excavation of a low level radiological waste pit and tritium disposal shafts  

This study evaluated the task-length average (TLA) respirable dust and respirable silica airborne concentrations to which construction workers excavating volcanic tuff at Los Alamos National Laboratory (LANL) were exposed. These workers were excavating a low level radiological waste disposal pit of final dimensions 720 feet long, 132 feet wide and 60 feet deep. The objectives of this study were as follows: (1) evaluate exposures; (2) determine if the type of machinery used affects the respirable dust concentration in the breathing zone of the worker; (3) evaluate the efficacy of wetting the pit to reduce the respirable dust exposure; and (4) determine if exposure increases with increasing depth of pit due to the walls of the pit blocking the cross wind ventilation.

312

Towards a physical model of dust tori in Active Galactic Nuclei - Radiative transfer calculations for a hydrostatic torus model  

We explore physically self-consistent models of dusty molecular tori in Active Galactic Nuclei (AGN) with the goal of interpreting VLTI observations and fitting high resolution mid-IR spectral energy distributions (SEDs). The input dust distribution is analytically calculated by assuming hydrostatic equilibrium between pressure forces - due to the turbulent motion of the gas clouds - and gravitational and centrifugal forces as a result of the contribution of the nuclear stellar distribution and the central black hole. For a fully three-dimensional treatment of the radiative transfer problem through the tori we employ the Monte Carlo code MC3D. We find that in homogeneous dust distributions the observed mid-infrared emission is dominated by the inner funnel of the torus, even when observing along the equatorial plane. Therefore, the stratification of the distribution of dust grains - both in terms of size and composition - cannot be neglected. In the current study we only include the effect of different sublim...

313

Dust Spectroscopy and the Nature of Grains  

Ground-based, air-borne and space-based, infrared spectra of a wide variety of objects have revealed prominent absorption and emission features due to large molecules and small dust grains. Analysis of this data reveals a highly diverse interstellar and circumstellar grain inventory, including both amorphous materials and highly crystalline compounds (silicates and carbon). This diversity points towards a wide range of physical and chemical birthsites as well as a complex processing of these grains in the interstellar medium. In this talk, I will review the dust inventory contrasting and comparing both the interstellar and circumstellar reservoirs. The focus will be on the processes that play a role in the lifecycle of dust in the interstellar medium.

314

Surface physical properties and its effects on the wetting behaviors of respirable coal mine dust  

In the present research work, coal dust physical properties as well as its wetting behaviors were analyzed systemically. The influences of different surfactants on coal dust's wetting behaviors were also investigated and compared with deionized water. Research results show that the finer the coal particle sizes, the more complex the coal particle micro structures are, which may cause the poor wetting abilities. Among the three different coal dust samples, the wetting performance is poor for the coal with higher volatile content due to the easier release of volatile matter and the easier formation of gas film around the particle. The fractal dimension and contact angles are presenting perfect correlations. With the increase of the fractal dimension, the contact angle would increase correspo...

315

Environment and respiratory system diseases  

It is generally acknowledged that there are causal connections between lung cancer and the influence of asbestos fibers, chromates, nickel dust, coke oven gases, and tobacco smoke; furthermore, between a long-term effect of oak and beech wood dusts and the adenocarcinoma of the nasal cavities. Benign and malignant changes of the pleura caused by asbestos as well are recognized as occupational diseases in the FRG as are lung fibroses due to anorganic and organic dusts. The most important exogeno-allergic alveolites are the farmer lung, the bird raiser lung, and the humidifier lung that is mainly found in printing plants. The most frequent occupational asthma is the flour dust asthma. Its causes, i.e. baking material such as amylase, hemicellulase, and soya bean meal, are often not recognized. Allergic, chemoirritant or toxically caused obstructive bronchial diseases also develop due to isocyanates inhaled in the production of synthetics and lacquers and due to aliphatic amines frequently used as solvents. There are no proven, generally acknowledged findings on the relation between air pollution in our broader environment and diseases of the respiration organs yet. Contradictory results of individual epidemiologic analyses are discussed.

316

The effects of the Tidal Force on Shear Instabilities in the Dust Layer of the Solar Nebula  

The linear analysis of the instability due to vertical shear in the dust layer of the solar nebula is performed. The following assumptions are adopted throughout this paper: (1) The self-gravity of the dust layer is neglected. (2) One fluid model is adopted, where the dust aggregates have the same velocity with the gas due to strong coupling by the drag force. (3) The gas is incompressible. The calculations with both the Coriolis and the tidal forces show that the tidal force has a stabilizing effect. The tidal force causes the radial shear in the disk. This radial shear changes the wave number of the mode which is at first unstable, and the mode is eventually stabilized. Thus the behavior of the mode is divided into two stages: (1) the first growth of the unstable mode which is similar to the results without the tidal force, and (2) the subsequent stabilization due to an increase of the wave number by the radial shear. If the midplane dust/gas density ratio is smaller than 2, the stabilization occurs before ...

317

On Forcing the Winter Polar Warmings in the Martian Middle Atmosphere during Dust Storms  

Using a Martian general circulation model, we investigated the changes in the meridional circulation during planet-encircling dust storms on Mars that produce strong temperature vertical inversions in the middle atmosphere over winter polar regions. It is shown that vigorous poleward and downward transport, and, consequently, the adiabatic heating are caused by dissipating thermal tides, planetary and resolved small-scale gravity waves and eddies in almost equal degree. The increase of tidal forcing is mainly due to a stronger excitation in the summer hemisphere. Contribution of the stationary planetary wave (SPW) with the zonal wavenumber s = 1 increases during dust storms due to intensified generation in the lower atmosphere as well as due to more favorable vertical propagation. SPW (s = 2) varies less with the dust load, dissipates lower, and contributes to the warming only below ? 0.1 mb. Transient planetary wave (s = 1, period ? 5 sols) with a barotropic/baroclinic vertical structure provides up to 1/3 of the forcing by SPW (s = 1). For the first time, we demonstrated a significance of small-scale gravity waves and eddies in maintaining the meridional circulation in Martian middle atmosphere, at least in high winter latitudes during dust storms.   

318

Understanding A New Class of Mid-IR Transients  

There is a new class of stellar transients whose progenitors are completely obscured (probably) extreme AGB stars, where the dust in the surviving wind appears to reform after the transient and again cloak the system. Whether these are true supernovae or a new class of stellar eruption is unclear, so the key question is whether or not the star survived. However, their present day emission appears to be due to optically thick dust (shock) heated by the ejecta from the transient, so we must understand the evolution of this emission and the dust optical depths before we can determine the survival of the stars. We propose a combination of Spitzer, Hubble and Chandra observations to characterize 6 of the new transients and a comparison sample of 5 supernovae with late time emission due to shocks and 3 luminous variable outbursts with late time emission due to a surviving star surrounded by ejected matter. The SST data will characterize the shock luminosity and its rate of decay, both exploring the physics of dusty shocks and setting limits on the flux from any surviving star. The near-IR HST data will tightly constrain the optical depth of the dust and potentially allow us to see through it to any surviving star. If the emission is from a dusty shock, there must be X-ray emission, and the amount of soft X-ray absorption will determine the the absorbing column densities.

319

The PIERNIK MHD code - a multi-fluid, non-ideal extension of the relaxing-TVD scheme (II)  

We present a new multi-fluid, grid-based magnetohydrodynamics (MHD) code PIERNIK, which is based on the Relaxing Total Variation Diminishing (RTVD) scheme (Jin & Xin 1995). The original scheme (see Trac & Pen 2003 and Pen et al. 2003) has been extended by an addition of dynamically independent, but interacting fluids: dust and a diffusive cosmic ray (CR) gas, described within the fluid approximation, with an option to add other fluids in an easy way. The code has been equipped with shearing-box boundary conditions, a selfgravity module, an Ohmic resistivity module, as well as other facilities which are useful in astrophysical fluid-dynamical simulations. The code is parallelized by means of an MPI library. In this paper we introduce a multifluid extension of the RTVD scheme and present a test case of dust migration in a two-fluid disk composed of gas and dust. We demonstrate that due to the difference in azimuthal velocities of gas and dust and the drag force acting on both components, dust drifts towards maxima of the gas pressure distribution.

320

PIERNIK mhd code - a multi-fluid, non-ideal extension of the relaxing-TVD scheme (II)  

We present a new multi-fluid, grid MHD code PIERNIK, which is based on the Relaxing TVD scheme (Jin and Xin, 1995). The original scheme (see Trac & Pen (2003) and Pen et al. (2003)) has been extended by an addition of dynamically independent, but interacting fluids: dust and a diffusive cosmic ray gas, described within the fluid approximation, with an option to add other fluids in an easy way. The code has been equipped with shearing-box boundary conditions, and a selfgravity module, Ohmic resistivity module, as well as other facilities which are useful in astrophysical fluid-dynamical simulations. The code is parallelized by means of the MPI library. In this paper we introduce the multifluid extension of Relaxing TVD scheme and present a test case of dust migration in a two-fluid disk composed of gas and dust. We demonstrate that due to the difference in azimuthal velocities of gas and dust and the drag force acting on both components dust drifts towards maxima of gas pressure distribution.

 
 
 
 
321

SPH simulations of grain growth in protoplanetary disks  

Aims: In order to understand the first stages of planet formation, when tiny grains aggregate to form planetesimals, one needs to simultaneously model grain growth, vertical settling and radial migration of dust in protoplanetary disks. In this study, we implement an analytical prescription for grain growth into a 3D two-phase hydrodynamics code to understand its effects on the dust distribution in disks. Methods: Following the analytic derivation of Stepinski & Valageas (1997), which assumes that grains stick perfectly upon collision, we implement a convenient and fast method of following grain growth in our 3D, two-phase (gas+dust) SPH code. We then follow the evolution of the size and spatial distribution of a dust population in a classical T Tauri star disk. Results: We find that the grains go through various stages of growth due to the complex interplay between gas drag, dust dynamics, and growth. Grains initially grow rapidly as they settle to the mid-plane, then experience a fast radial migration w...

322

Dynamics of the Optical Properties of Fine/Coarse Mode Aerosol Mixtures in Diverse Environments  

Several regions of the earth exhibit seasonal mixtures of fine and coarse mode aerosol types, which are challenging to characterize from satellite remote sensing. Over land the coarse mode aerosols originate primarily from arid regions, which generate airborne soil dust, and the primary fine mode sources are urban/industrial emissions of gases and particulates and also biomass burning. The recently developed AERONET Version 2 retrieval algorithm produces more accurate retrievals of particle size distribution when non-spherical particles (such as dust) are present and also more accurate spectral single scattering albedo due to improved specification of the earth surface bidirectional reflectance. We show comparison of AERONET Version 1 and 2 retrievals that exhibit differences and suggest significantly improved single scattering albedo in Version 2. AERONET almucantar retrievals from several years are analyzed for the urban sites of Beijing, China and Kanpur, India (in the Ganges floodplain) where seasonal coarse mode dust particles mix with fine mode pollution aerosol, predominately in the spring. Additionally we compare multi-year data from Ilorin, Nigeria where desert dust from the Sahara and Sahel mix with fine mode biomass-burning aerosols. We also analyze data from two sites in the United Arab Emirates where dust mixes with urban/industrial pollution largely from petroleum industry emissions. The data are analyzed as a function of the aerosol optical depth fine mode fraction and also by Angstrom exponent, with comparisons made between sites.

323

Desulfurization Ability of Metallurgical Dusts from Blast Furnace Ironmaking Process  

The sulfur capacity of metallurgical dusts from blast furnace ironmaking processes was measured in the temperature range from 298 to 923 K. The experimental results show that the sulfur capacity of metallurgical dusts is considerably increased with the increase of temperature from 298 to 923 K. The desulfurization ability of metallurgical dusts is mainly depend on its content of oxides of ZnO, PbO, CaO and MnO when the temperature is lower than 623 K, but when the temperature is higher than 623 K the contributions of iron oxides become dominant. Carbon content, due to its absorption effect, has a positive effect on the desulfurization ability of metallurgical dusts below 623 K. If the temperature increased to higher than 623 K the absorption effect of carbon disappears and the role of desulfurization reaction between H2S and the metal oxide such as ZnO, PbO, Fe2O3, CaO and MnO as well as the H2S diffusion in intraparticle of metallurgical dusts seems more important.   

324

A Laboratory Study of the Charging/Discharging Mechanisms of a Dust Particle Exposed to an Electron Beam  

The interaction of micron sized particles or "dust particles" with different space and planetary environments has become an important area of research. One particular area of interest is how dust particles interact with plasmas. Studies have shown that charged dust particles immersed in plasmas can alter plasma characteristics, while ions and electrons in plasmas can affect a particle's potential and thereby, its interaction with other particles. The basis for understanding these phenomena is the charging mechanisms of the dust particle, specifically, how the particle's charge and characteristics are affected when exposed to ions and electrons. At NASA Marshall Space Flight Center, a laboratory experiment has been developed to study the interaction of dust particles with electrons. Using a unique laboratory technique known as electrodynamic suspension, a single charged particle is suspended in a modified quadrupole trap. Once suspended, the particle is then exposed to an electron beam to study the charging/discharging mechanisms due to collisions of energetic electrons. The change in the particle's charge, approximations of the charging/discharging currents, and the charging/discharging yield are calculated.

325

ATCA and Spitzer Observations of the Binary Protostellar Systems CG30 and BHR71  

We present interferometric observations with resolution of ~3 arcsecs of the isolated, low-mass protostellar double cores CG30 and BHR71 in the N2$H+(1-0) line and at 3mm dust continuum, using the Australian Telescope Compact Array (ATCA). The results are complemented by infrared data from the Spitzer Space Telescope. In CG30, the 3mm dust continuum images resolve two compact sources with a separation of ~21.7 arcsecs (~8700 AU). In BHR71, strong dust continuum emission is detected at the position of the mid-infrared source IRS1, while only weak emission is detected from the secondary mid-infrared source IRS2. Assuming optically thin 3mm dust continuum emission, we derive hydrogen gas masses of 0.05--2.1 $M_\\odot$ for the four sub-cores. N2H+(1-0) line emission is detected in both CG30 and BHR71, and is spatially associated with the thermal dust continuum emission. We derive the velocity fields and find symmetric velocity gradients in both sources. Assuming that these gradients are due to core rotation, we es...

326

Impact of Asian dust and continental pollutants on cloud chemistry observed in northern Taiwan during the experimental period of ABC/EAREX 2005  

Observations of particulate matter (PM), vertical cloud and aerosol structure and cloud water chemistry in northern Taiwan were conducted during the ABC/EAREX 2005 period. Five Asian continental outflow regimes reaching Taiwan were identified. One was coupled with a dust storm observed not only at Gosan, Korea, but also over Taiwan, suggesting the scope of its regional impact. The arrival of the dust event was determined by lidar, cloud water, and surface PM measurements. When continental outflow events correspond to the presence of significant dust concentrations, air quality can be drastically worsened due to high levels of PM. PM10 (PM with aerodynamic diameters dust case. Cloud water may have become acidified by pollution from industrial and urban regions along the coast of eastern China. Nevertheless, abundant Ca2+ contributed to the neutralization of acidic cloud water during the dust stage. The much higher aerosol and chemical loading injected into these clouds caused an enrichment effect in the cloud water, which can double the cloud loading of total ions, when Ca2+ increases by approximately 7 times.

327

Searching for Saturn's Dust Swarm: Limits on the size distribution of Irregular Satellites from km to micron sizes  

We describe a search for dust created in collisions between the Saturnian irregular satellites using archival \\emph{Spitzer} MIPS observations. Although we detected a degree scale Saturn-centric excess that might be attributed to an irregular satellite dust cloud, we attribute it to the far-field wings of the PSF due to nearby Saturn. The Spitzer PSF is poorly characterised at such radial distances, and we expect PSF characterisation to be the main issue for future observations that aim to detect such dust. The observations place an upper limit on the level of dust in the outer reaches of the Saturnian system, and constrain how the size distribution extrapolates from the smallest known (few km) size irregulars down to micron-size dust. Because the size distribution is indicative of the strength properties of irregulars, we show how our derived upper limit implies irregular satellite strengths more akin to comets than asteroids. This conclusion is consistent with their presumed capture from the outer regions o...

328

Determination of heavy metals in indoor dust from Istanbul, Turkey: Estimation of the health risk  

Levels of eight potentially toxic heavy metals in indoor dust from homes and offices in Istanbul were investigated. The concentrations of heavy metals in indoor dust from homes+office ranged from 62 to 1800@mgg^-^1 for Cu, 3-200@mgg^-^1 for Pb, 0.4-20@mgg^-^1 for Cd, 210-2800@mgg^-^1 for Zn, 2.8-460@mgg^-^1 for Cr, 8-1300@mgg^-^1 for Mn, 2.4-25@mgg^-^1 for Co, 120-2600@mgg^-^1 for Ni. Results of the study were comparable to other studies conducted on indoor dust and street dust from a variety of cities globally. Considering only ingestion + inhalation, the carcinogenic risk level of Cr for adults and children (3.7x10^-^5 and 2.7x10^-^5) in Istanbul was in the range of EPA's safe limits (1x10^-^6 and 1x10^-^4), indicating that cancer risk of Cr due to exposure to indoor dust in Istanbul can...

329

Incineration of irradiated graphite fuel elements in a fluidized bed. Verbrennung von bestrahlten Graphitbrennelementen in der Wirbelschicht  

The reprocessing of irradiated fuel elements from a high-temperature reactor requires the separation of the fuel from the graphite matrix. This can be achieved by burning the graphite in a fluid-bed furnace. This process step was experimentally investigated using cold and hot spherical fuel elements. To this end, a fluidized bed combustion facility was set up in a hot cell with a fluidized bed reactor of 95 mm diameter and 1 m length. The maximum combustion rate was 1 kg graphite/h at a combustion temperature of 900 to 950deg C. Fine dust separation from the flue gas and above all recycling the dust to the fluidized reactor posed the greatest experimental problems. The best results for dust recycling were obtained by using an injector nozzle. BISO-coated UO{sub 2} fuel kernels disintegrate into U{sub 3}O{sub 8} dust during combustion. This leads to heavy-metal losses of up to 40% per combustion batch in a clean combustion unit due to the deposition of dust. The amount of heavy metal recovered increases by repeating the combustion process. An equilibrium in heavy-metal output was not achieved in hot tests. (orig.).

330

Industrial hygiene characterization of automotive wood model shops  

A suspicion of an excess cancer risk in automotive model shops prompted the Industrywide Studies Branch, NIOSH, to conduct a proportionate mortality study and an industrial hygiene characterization of operations in these shops. The mortality study showed a statistically significant excess proportion of deaths due to colon cancer and leukemia (for woodshops only). The materials used in the model shops include various natural woods, laminated woods, plastics, resins, varnishes, putties and paints. Personal breathing zone samples were collected for total and respirable dust, amines, various hydrocarbons (including styrene, and toluene), formaldehyde, and nitrosamines. Particle size distribution studies were conducted on the wood dust and bulk airborne samples of dusts were subjected to various mutagenicity test systems. Work practices, ventilation and general housekeeping were checked. Total wood dust samples ranged from 0.03 to 25 mg/m3 with an average around 1.0 mg/m3. The percent respirable dust ranged from 19 to 38% as measured with Andersen impactors. Solvent exposure samples ranged from non-detectable to about 10% of the OSHA Permissible Exposure Levels. Relevant recommendations for improvement of contaminant control were made.

331

Distribution of dust in the rat lung following administration by inhalation and by single intratracheal instillation  

A comparison was made of the distribution of dust in the rat lung following its administration by inhalation and by a single intratracheal instillation. Due to the wide variety of instillation techniques, an average method was adopted based on the results from a survey of 15 laboratories in Europe and the USA. Novel techniques were developed to quantify the distribution of dust within the lung both microscopically and macroscopically. The distribution of dust obtained by instillation was shown to be much less homogeneous than that obtained by inhalation and penetration to the periphery was minimal. The effects of (a) changing the volume of suspension, (b) changing the concentration of the suspension, and (c) introducing air into the syringe were investigated. Although the use of air in the syringe was beneficial, none of the other modifications effected any improvement in the distribution. The difference in distribution following inhalation and instillation leads to the conclusion that the latter may be of use in establishing the nature and comparative response of the lung to different dusts, but not for establishing an absolute dose-response relationship. It is recommended that no more than 1 mg of fibrous or 5 mg of nonfibrous dust be given in a single instillation to adult rats.

332

Regional modelling of Saharan dust and biomass-burning smoke. Part 2: Direct radiative forcing and atmospheric dynamic response  

The direct radiative forcing and dynamic atmospheric response due to Saharan dust and biomass-burning aerosol particles are presented for a case study during the SAMUM-2 field campaign in January and February 2008. The regional model system COSMO-MUSCAT is used. It allows online interaction of the computed dust and smoke load with the solar and terrestrial radiation and with the model dynamics. Model results of upward solar irradiances are evaluated against airborne radiation measurements in the Cape Verde region. The comparison shows a good agreement for the case of dust and smoke mixture. Dust and smoke particles influence the atmospheric dynamics by changing the radiative heating rates. The related pressure perturbations modify local and synoptic scale air-flow patterns. In the radiative feedback simulations, the Hadley circulation is enhanced and convergence zones occur along the Guinea coast. Thus, the smoke particles spread more than 5 deg further north and the equatorward transport is reduced. Within the convergence zones, Saharan dust and biomass-burning material are more effectively advected towards the Cape Verdes. Given the model uncertainties, the agreement between the modelled and observed aerosol distribution is locally improved when aerosol-radiation interaction is considered

333

The Structure of Pre-transitional Protoplanetary Disks I: Radiative Transfer Modeling of the Disk+Cavity in the PDS 70 system  

Through detailed radiative transfer modeling, we present a disk+cavity model to simultaneously explain both the SED and Subaru H-band polarized light imaging for the pre-transitional protoplanetary disk PDS 70. Particularly, we are able to match not only the radial dependence, but also the absolute scale, of the surface brightness of the scattered light. Our disk model has a cavity 65 AU in radius, which is heavily depleted of sub-micron-sized dust grains, and a small residual inner disk which produces a weak but still optically thick NIR excess in the SED. To explain the contrast of the cavity edge in the Subaru image, a factor of ~1000 depletion for the sub-micron-sized dust inside the cavity is required. The total dust mass of the disk may be on the order of 1e-4 M_sun, only weakly constrained due to the lack of long wavelength observations and the uncertainties in the dust model. The scale height of the sub-micron-sized dust is ~6 AU at the cavity edge, and the cavity wall is optically thick in the vertic...

334

The dust emission law in the wind erosion process on soil surface  

The dust emission models to date cannot describe the relation between the transport rate of different sized grains and their grain size composition in soil surface, so Aeolian grain transport on a soil-like bed composed of fine sand and silt powder was measured in a wind tunnel. Six types of soil-like beds with different silt fractions have been tested in this experiment. The mass flux profiles of silt dust and sand grains are much different due to their different motion modes. Analysis of the vertical distribution of the powder and sand grains reveals that for a given soil bed, the ratio of the horizontal dust flux to the horizontal sand flux is directly proportional to their mass ratio in the bed. The dust flux is closely linked to the sand flux by the bombardment mechanism. For a given wind velocity and grain size of the bed, the slopes of the vertical mass flux profiles of sand grains larger than 100 ?m are nearly equal in a log-linear plot and the ratio between the fraction of transport rate of each size group to the whole transport rate and the mass fraction of each size group in the bed is a constant only dependent on grain size. With this law, the transport rate of dust and different sized grains can be related with the grain size composition in the soil surface.

335

Aircraft-based observations and high-resolution simulations of a dust storm in Iceland  

The first aircraft-based observations of an Icelandic dust storm are presented. Themeasurementswere carried out over the ocean near Iceland's south coast in February 2007. This dust event occurred in conjunction with an easterly barrier jet of more than 30 m/s. The aircraft measurements show high particlemass mixing ratios in an area of low wind speeds in the wake of Iceland near the coast, decreasing abruptly towards the jet. Simulations from the Weather Research and Forecasting Model coupled with Chemistry (WRF/Chem) indicate that the measured high mass mixing ratios and observed low visibility inside the wake are due to dust transported from Icelandic sand fields towards the ocean. This is confirmed by meteorological station data. Primary dust sources are glacial outwash terrains located near the ?yrdalsj ¨okull glacier. Sea salt aerosols produced by the impact of strong winds on the ocean surface started to dominate as the aircraft flew away from Iceland into the jet. The present results support recent studies which suggest that Icelandic deserts should be considered as important dust sources in global and regional climate models.

336

Aircraft-based observations and high-resolution simulations of an Icelandic dust storm  

The first aircraft-based observations of an Icelandic dust storm are presented. The measurements were carried out over the ocean near Iceland's south coast in February 2007. This dust event occurred in conjunction with an easterly barrier jet of more than 30 m s-1. The aircraft measurements show high particle mass mixing ratios in an area of low wind speeds in the wake of Iceland near the coast, decreasing abruptly towards the jet. Simulations from the Weather Research and Forecasting Model coupled with Chemistry (WRF/Chem) indicate that the measured high mass mixing ratios and observed low visibility inside the wake are due to dust transported from Icelandic sand fields towards the ocean. This is confirmed by meteorological station data. Primary dust sources are glacial outwash terrains located near the Mýrdalsjökull glacier. Sea salt aerosols produced by the impact of strong winds on the ocean surface started to dominate as the aircraft flew away from Iceland into the jet. The present results support recent studies which suggest that Icelandic deserts should be considered as important dust sources in global and regional climate models.

337

Country specific comparison for profile of chlorinated, brominated and phosphate organic contaminants in indoor dust. Case study for Eastern Romania, 2010.  

We have evaluated the levels and specific profiles of several organohalogenated contaminants, including organochlorine pesticides (OCPs), polychlorinated biphenyls (PCBs), and flame retardants (FRs), such as polybrominated diphenyl ethers (PBDEs), hexabromocyclododecanes (HBCDs), novel brominated FRs (NBFRs), and organophosphate FRs (OPFRs), in 47 indoor dust samples collected in 2010 from urban locations from Iasi, Eastern Romania. The dominant contaminants found in the samples were OPFRs (median sum OPFRs 7890ng/g). Surprisingly, OCPs were also measured at high levels (median 1300ng/g). Except for BDE 209 (median 275ng/g), PBDEs were present in dust samples at relatively low levels (median sum PBDEs 8ng/g). PCBs were also measured at low levels (median sum PCBs 35ng/g), while NBFRs were only occasionally detected, showing a low usage in goods present on the Romanian market. The results of the present study evidence the existence of a multitude of chemical formulations in indoor dust. FRs are usually associated to human exposure via ingestion of dust, but other chemicals, such as OCPs, are not commonly reported in such matrix. Although OCPs were found at comparable levels with OPFRs in Romanian dust, OCPs possess a higher risk to human health due to their considerably lower reference dose (RfD) values. Indeed, the OCP exposure calculated for various intake scenarios was only 2-fold lower than the corresponding RfD. Therefore, the inclusion of OCPs as target chemicals in the indoor environment becomes important for countries where elevated levels in other environmental compartments have been previously shown. PMID:22929296

338

The Solar-System-Scale Disk Around AB Aurigae  

The young star AB Aurigae is surrounded by a complex combination of gas-rich and dust dominated structures. The inner disk which has not been studied previously at sufficient resolution and imaging dynamic range seems to contain very little gas inside a radius of least 130 astronomical units (AU) from the star. Using adaptive-optics coronagraphy and polarimetry we have imaged the dust in an annulus between 43 and 302 AU from the star, a region never seen before. An azimuthal gap in an annulus of dust at a radius of 102 AU, along with a clearing at closer radii inside this annulus, suggests the formation of at least one small body at an orbital distance of about 100 AU. This structure seems consistent with crude models of mean motion resonances, or accumulation of material at two of the Lagrange points relative to the putative object and the star. We also report a low significance detection of a point source in this outer annulus of dust. This source may be an overdensity in the disk due to dust accreting onto...

339

Lunar Dust Environment and Plasma Package for Lunar Lander - Denition Study  

Dust, the charged lunar surface, and the ambient plasma form a closely coupled system. The lunar surface is permanently under the in turn may lead to mobilization and transport of charged dust particles. Furthermore, the environment can become even more complex in the presence of local crustal magnetic anomalies or due to sunlight/shadow transitions. A detail understanding of these phenomena and their dependence on external in uences is a key point for future robotic/human lunar exploration and requires an appropriately tuned instrumentation for in situ measurements. We present preliminary results from the concept and design phase A study of the Lunar Dust Environment and Plasma Package (L-DEPP), which has been proposed as one of model instrument payloads for the planned Lunar Lander mission of the European Space Agency. Focus is held on scientic objectives and return of the mission with respect to environmental and mission technology constraints and requirements. L-DEPP is proposed to consist of the following instruments: ELDA - Electrostatic lunar dust analyser, LP - Langmuir probe, RADIO - Broadband radio receiver and electric eld antennae, LEIA - Lunar electron and ion analyser, and MAG - Flux-gate magnetometer. In addition to the dust and plasma measurements the RADIO experiment will provide a site survey testing for future radio astronomy observations.

340

Lunar Dust Environment and Plasma Package for Lunar Lander - Definition Study  

Dust, the charged lunar surface, and the ambient plasma form a closely coupled system. The lunar surface is permanently under the influence of charging effects such as UV radiation or energetic solar wind and magnetospheric particles. The surface charging effects result in strong local electric fields which in turn may lead to mobilization and transport of charged dust particles. Furthermore, the environment can become even more complex in the presence of local crustal magnetic anomalies or due to sunlight/shadow transitions. A detail understanding of these phenomena and their dependence on external influences is a key point for future robotic/human lunar exploration and requires an appropriately tuned instrumentation for in situ measurements. Here we present preliminary results from the concept and design phase A study of the Lunar Dust Environment and Plasma Package (L-DEPP), which has been proposed as one of model instrument payloads for the planned Lunar Lander mission of the European Space Agency. Focus is held on scientific objectives and return of the mission with respect to environmental and mission technology constraints and requirements. L-DEPP is proposed to consist of the following instruments: ELDA - Electrostatic lunar dust analyser, LP - Langmuir probe, RADIO - Broadband radio receiver & electric field antennae, LEIA - Lunar electron and ion analyser, and MAG - Flux-gate magnetometer. In addition to the dust and plasma measurements the RADIO experiment will provide a site survey testing for future radio astronomy observations.

 
 
 
 
341

A dozen type II-P supernovae seen with the eyes of Spitzer  

Core-collapse supernovae (CC SNe), especially those of type II-plateau (II-P), are thought to be important contributors to cosmic dust production. The most obvious indicator of the presence of newly-formed and/or pre-existing dust is the time-dependent mid-infrared (MIR) excess coming from the environment of SNe. Our goal was to collect publicly available, previously unpublished measurements on type II-P (or peculiar IIP) SNe from the Spitzer database. The temporal changes of the observed fluxes may be indicative of the underlying supernova, while spectral energy distribution (SED) fitting to the fluxes in different IRAC channels may reveal the physical parameters of the mid-IR radiation, presumably due to warm dust. IRS spectra were extracted and calibrated with SPICE, while photometric SEDs were assembled using IRAF and MOPEX. Calculated SEDs from observed fluxes were fit with simple dust models to get basic information on the dust presumed as the source of MIR radiation. We found twelve SNe satisfying the ...

342

Deposition of atmospheric (137)Cs in Japan associated with the Asian dust event of March 2002.  

Considerable deposition of (137)Cs was observed in the northwestern coastal area of Japan in March 2002. Since there were no nuclear explosions or serious nuclear accidents in the early 2000s, transport of previously contaminated dust appears to be the only plausible explanation for this event. In March 2002, there was a massive sandstorm on the East Asian continent, and the dust raised by the storm was transported across the sea to Japan. This dust originated in Mongolia and northeastern China, in an area distant from the Chinese nuclear test site at Lop Nor or any other known possible sources of (137)Cs. Our radioactivity measurements showed (137)Cs enrichment in the surface layer of grassland soils in the area of the sandstorm, which we attributed to accumulation as a result of past nuclear testing. We suggest that the grassland is a potential source of (137)Cs-bearing soil particles. Since the late 1990s, this area has experienced drought conditions, resulting in a considerable reduction of vegetation cover. We attribute the prodigious release of (137)Cs-bearing soil particles into the atmosphere during the sandstorm and the subsequent deposition of (137)Cs in Japan to this change. PMID:17604085

343

Evaluation of dust-related health hazards associated with air coring at G-Tunnel, Nevada Test Site  

The Yucca Mountain Project was established to evaluate the potential for storing high-level radioactive wastes in geologic formations. Hydrologists recommended that drilling or coring in support of characterization tests be performed dry. Dry drilling, or air coring, presents a concern about health protection for the drilling personnel. The rock generally has a high silica content, and natural zeolites are abundant. Some zeolites are fibrous, leading to concerns that inhalation may result in asbestos-like lung diseases. An industrial hygiene study (IH) was conducted as part of an air coring technical feasibility test. The IH study found the potential for exposures to airborne silica and nuisance dusts to be within regulatory requirements and determined the commercial dust control equipment monitored to be effective when used in conjunction with a good area ventilation system and sound IH practices. Fibrous zeolites were not detected. Recommendations for the Yucca Mountain studies are (1) dust collection and control equipment equivalent or superior to that monitored must be used for any dry drilling activity and must be used with good general dilution ventilation and local exhaust ventilation provided on major emission sources; (2) good industrial hygiene work practices must be implemented, including monitoring any area where zeolitic fibers are suspect; and (3) a study should be conducted to determine the biological effects of the fibrous zeolite, mordenite. 25 refs., 17 figs., 14 tabs.

344

On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes  

The dust probe DUSTY, first launched during the summer of 1994 (flights ECT-02 and ECT-07) from Andoeya Rocket Range, northern Norway, was the first probe to unambiguously detect heavy charged mesospheric aerosols, from hereon referred to as dust. In ECT-02 the probe detected negatively charged dust particles in the height interval of 83 to 88.5 km. In this flight, the lower grid in the detector (Grid 2) measures both positive and negative currents in various regions, and we find that the relationship between the current measurements of Grid 2 and the bottom plate can only be explained by influence from secondary charge production on Grid 2. In ECT-07, which had a large coning, positive currents reaching the top grid of the probe were interpreted as due to the impact of positively charged dust particles. We have now reanalyzed the data from ECT-07 and arrived at the conclusion that the measured positive currents to this grid must have been mainly due to secondary charging effects from the impacting dust particles. The grid consists of a set of parallel wires crossed with an identical set of wires on top of it, and we find that if the observed currents were created from the direct impact of charged dust particles, then they should be very weakly modulated at four times the rocket spin rate {omega}{sub R}. Observations show, however, that the observed currents are strongly modulated at 2{omega}{sub R}. We cannot reproduce the observed large modulations of the impact currents in the dust layer if the currents are due only to the transfer of the charges on the impacted dust particles. Based on the results of recent ice cluster impact secondary charging experiments by Tomsic (2003), which found that a small fraction of the ice clusters, when impacting with nearly grazing incidence, carried away one negative charge - 1e, we have arrived at the conclusion that similar, but significantly more effective, charging effects must be predominantly responsible for the positive currents measured by the top grid in ECT-07 and their large rotational modulation at 2{omega}{sub R}. (orig.)

345

Casting Light and Shadows on a Saharan Dust Storm  

On March 2, 2003, near-surface winds carried a large amount of Saharan dust aloft and transported the material westward over the Atlantic Ocean. These observations from the Multi-angle Imaging SpectroRadiometer (MISR) aboard NASA's Terra satellite depict an area near the Cape Verde Islands (situated about 700 kilometers off of Africa's western coast) and provide images of the dust plume along with measurements of its height and motion. Tracking the three-dimensional extent and motion of air masses containing dust or other types of aerosols provides data that can be used to verify and improve computer simulations of particulate transport over large distances, with application to enhancing our understanding of the effects of such particles on meteorology, ocean biological productivity, and human health.MISR images the Earth by measuring the spatial patterns of reflected sunlight. In the upper panel of the still image pair, the observations are displayed as a natural-color snapshot from MISR's vertical-viewing (nadir) camera. High-altitude cirrus clouds cast shadows on the underlying ocean and dust layer, which are visible in shades of blue and tan, respectively. In the lower panel, heights derived from automated stereoscopic processing of MISR's multi-angle imagery show the cirrus clouds (yellow areas) to be situated about 12 kilometers above sea level. The distinctive spatial patterns of these clouds provide the necessary contrast to enable automated feature matching between images acquired at different view angles. For most of the dust layer, which is spatially much more homogeneous, the stereoscopic approach was unable to retrieve elevation data. However, the edges of shadows cast by the cirrus clouds onto the dust (indicated by blue and cyan pixels) provide sufficient spatial contrast for a retrieval of the dust layer's height, and indicate that the top of layer is only about 2.5 kilometers above sea level.Motion of the dust and clouds is directly observable with the assistance of the multi-angle 'fly-over' animation (Below). The frames of the animation consist of data acquired by the 70-degree, 60-degree, 46-degree and 26-degree forward-viewing cameras in sequence, followed by the images from the nadir camera and each of the four backward-viewing cameras, ending with 70-degree backward image. Much of the south-to-north shift in the position of the clouds is due to geometric parallax between the nine view angles (rather than true motion), whereas the west-to-east motion is due to actual motion of the clouds over the seven minutes during which all nine cameras observed the scene. MISR's automated data processing retrieved a primarily westerly (eastward) motion of these clouds with speeds of 30-40 meters per second. Note that there is much less geometric parallax for the cloud shadows owing to the relatively low altitude of the dust layer upon which the shadows are cast (the amount of parallax is proportional to elevation and a feature at the surface would have no geometric parallax at all); however, the westerly motion of the shadows matches the actual motion of the clouds. The automated processing was not able to resolve a velocity for the dust plume, but by manually tracking dust features within the plume images that comprise the animation sequence we can derive an easterly (westward) speed of about 16 meters per second. These analyses and visualizations of the MISR data demonstrate that not only are the cirrus clouds and dust separated significantly in elevation, but they exist in completely different wind regimes, with the clouds moving toward the east and the dust moving toward the west. [figure removed for brevity, see original site] (Click on image above for high resolution version)The Multi-angle Imaging SpectroRadiometer observes the daylit Earth continuously and every 9 days views the entire globe between 82 degrees north and 82 degrees south latitude. These data products were generated from a portion of the imagery acquired during Terra orbit 17040.

346

Is it necessary to raise awareness about technologically enhanced naturally occurring radioactive materials?  

Since radiation risks are usually considered to be related to nuclear energy, the majority of research on radiation protection has focused on artificial radionuclides in radioactive wastes, spent nuclear fuel or global fallout caused by A-bomb tests and nuclear power plant failures. Far less attention has been paid to the radiation risk caused by exposure to ionizing radiation originating from natural radioactivity enhanced due to human activity, despite the fact that technologically enhanced naturally occurring radioactive materials are common in many branches of the non-nuclear industry. They differ significantly from "classical" nuclear materials and usually look like other industrial waste. The derived radiation risk is usually associated with risk caused by other pollutants and can not be controlled by applying rules designed for pure radioactive waste. Existing data have pointed out a strong need to take into account the non-nuclear industry where materials containing enhanced natural radioactivity occur as a special case of radiation risk and enclose them in the frame of the formal control. But up to now there are no reasonable and clear regulations in this matter. As a result, the non-nuclear industries of concern are not aware of problems connected with natural radioactivity or they would expect negative consequences in the case of implementing radiation protection measures. The modification of widely comprehended environmental legislation with requirements taken from radiation protection seems to be the first step to solve this problem and raise awareness about enhanced natural radioactivity for all stakeholders of concern. PMID:19809704

347

Radioactive contamination in imported foods; Apr. 1988 similar to Mar. 1990  

On April 26, 1986, explosion occurred in Chernobyl nuclear power station in USSR, and radioactivity contamination was brought about in almost all countries in the world. In European countries, crops were contaminated directly with radioactive fallout to high concentration. Also in Japan, after one week the radioactivity higher than usual was detected in environment, and also in vegetables, milk, tea leaves and others. Thereafter, in order to cope with the import of contaminated foods, inspection and watch system was strengthened by deciding the interim limit of radioactive concentration. However the cases of exceeding the interim limit were often reported. In order to remove the harmful foods due to radioactive contamination and to meet the fear of consumers, the authors measured the radioactive concentration in foods distributed in Tokyo and investigated the actual state of contamination. The samples were 920 imported foods. The experimental method, the preparation of samples, the method of analysis and the results are reported. The samples in which the radioactive concentration exceeding 50 Bq/kg was detected were 25 cases. The food having the high frequency of detection was flavors. (K.I.).

348

Ten years of research on the cycle of some radionuclides in the marine environment  

Several radionuclides (/sup 90/Sr, /sup 137/Cs, /sup 144/Ce, /sup 155/ Eu, /sup 147/Pm, /sup 54/Mn, and /sup 226/Ra) were determined in plankton and seawater samples: their content is in relation to the radioactive fallout intensity. Particular attention was paid to /sup 90/Sr the presence of which in the plankton may be correlated with the Acantharia frequency. Such a radionuclide was determined in many marine substrata also. The same radionuclides were found in the coastal marine sediments of the Ligurian and North Adriatic Seas. The radioactivity due to their presence in the various layers was correlated with the radioactive fallout and suggested to us an hypothesis on the accumulation rate of marine sediments in the coastal zones. In 1968 the radioecological study of Taranto Gulf was begun. The value of the radioactivity measurements in such a zone has a practical importance as in future a reprocessing plant of the nuclear iuel will start to operate at Rotondella, with a consequent release of radioactive wastes in the Jonian Sea. A fresh water environment was also considered, the Lago Santo Parmense. The radioactivity measured in the various substrata (sediment, water, vegetables) is by far higher than the one of the marine environment. In particular the /sup 137/Cs contribution to the sediment radioactivity is remarkable. (auth)

349

Works of chemists researching radioactivity involved in two accidents this fall; Houshano wo kenkyu suru kagakusha no kataraki. Honshu no 2 jiken ni saishite  

Two accidents happened in September 1999 (meteorite dropping accident and JCO criticality accident) are linked to each other at a common point concerning radioactivity, and chemists specialized in radioactivity have been executing active researches. In this paper, a focus of discussion is put on the measurement of radioactivity induced by neutrons due to cosmic rays or criticality. Researches executed actively by the chemists during several weeks for calculating neutron fluxes around the spot of the criticality accident and estimating the meteorite matrix on the basis of nuclear reaction in outer space under absolute time restriction of radioactive half life. In the meteorite dropping falling accident, a stone fell through the roof of the second floor of a private house in Kobe, and this stone was proved to be a meteorite on the basis of a non-destructive {gamma} ray spectrum measurement carried out by the Low Level Radioactivity Experiment Facility of Science Department of Kanazawa University. Detections of Mg-28 with a radioactive half life of 21 hours and Ni-57 with a radioactive half life of 1.45 days were succeeded for the first time in the world owing to an extremely short time from finding information on the internet till carrying out the measurements. (NEDO)

350

Purification of nuclear power plant decontamination solutions by preparative scale reactive adsorption  

During alkaline, oxidative decontamination of nuclear power plant equipment a radioactive solution is produced. Owing to the storing difficulties of radioactive solutions it is necessary to develop a method for the in situ treatment of radioactive, alkaline, oxidative decontamination solutions, and for the concentration of radioactive components. Reactive adsorption seems to be promising for this purpose. In reactive adsorption the radioactive nuclides are sorbed at 95{sup o}C by an activated carbon. Under the circumstances the reduction of Mn(VII) to Mn(VI) becomes significant on the surface of the activated carbon, and MnO{sub 2} precipitation occurs in the pores of the adsorbent. Due to the adsorption- ion exchange properties of MnO{sub 2} it can uptake the radioactive isotopes. Simultaneously the new precipitating MnO{sub 2} layers cover the surface saturated with radioactive isotopes hereby preventing their desorption, and provide fresh adsorption, ion exchange layer. Under inactive conditions the kinetics of MnO{sub 2} precipitation was studied in a stirred batch reactor and the sorption of silver was investigated in a chromatographic column. The purification of nuclear power plant decontamination solutions was also carried out. (Author).

351

Radioactive wastes management development in Chile  

A Facility for immobilizing and conditioning of radioactive wastes generated in Chile, has recently started in operation. It is a Radioactive Wastes Treatment Plant, RWTP, whose owner is Comision Chilena de Energia Nuclear, CCHEN. A Storgement Building of Conditioned Wastes accomplishes the facility for medium and low level activity wastes. The Project has been carried with participation of chilean professionals at CCHEN and Technical Assistance of International Atomic Energy Agency, IAEA. Processes developed are volume reduction by compaction; immobilization by cementation and conditioning. Equipment has been selected to process radioactive wastes into a 200 liters drum, in which wastes are definitively conditioned, avoiding exposition and contamination risks. The Plant has capacity to treat low and medium activity radioactive wastes produced in Chile due to Reactor Experimental No. 1 operation, and annex Laboratories in Nuclear Research Centers, as also those produced by users of nuclear techniques in Industries, Hospitals, Research Centers and Universities, in the whole country. With the infrastructure developed in Chile, a centralization of Radioactive Wastes Management activities is achieved. A data base system helps to control and register radioactive wastes arising in Chile. Generation of radioactive wastes in Chile, has found solution for the present production and that of near future.

352

Dispersal of radioactivity by wildlife from contaminated sites in a forested landscape  

Oak Ridge National Laboratory (ORNL) is located within the Valley and Ridge Physiographic Province of eastern Tennessee (USA). Wildlife populations have access to some radioactively contaminated sites at ORNL. Contaminated animals or animal nests within the Laboratory's boundaries have been found to contain {sup 90}Sr or {sup 137}Cs on the order of 10{sup -2}-10{sup 4} Bqg{sup -1} and trace amounts of other radionuclides (including transuranic elements). Animals that are capable of flight and animals with behavior patterns or developmental life stages involving contact with sediments in radioactive ponds, like benthic invertebrates, present the greatest potential for dispersal of radioactivity. The emigration of frogs and turtles from waste ponds also presents a potential for dispersal of radioactivity but over distances < 5 km. Mud-dauber wasps (Hymenoptera) and swallows (Hirundinidae) may transport radioactive mud for nest building, but also over relatively short distances (0.2-1 km). Movement by small mammals is limited by several factors, including physical barriers and smaller home ranges. Larger animals, like white-tailed deer (Odocoileus virginianus), are potential vectors of radioactivity due to their greater body size, longer life expectancy, and larger home range. Larger animals contain greater amounts of total radioactivity than smaller animals, but tissue concentrations of {sup 137}Cs generally decline with body size.

353

Radioecological impact of Saharan dusts fallout. Case study of a major event on the 21. of february 2004 in south part of France; Impact radioecologique des retombees de poussieres sahariennes. Episode majeur du 21/02/2004 dans le sud de la France  

Lithometeors, Sirocco or more commonly 'red mud' are all in fact related to a single phenomenon which affects France every year: the wind transport and deposit of desert particles from the Sahara. On the 21. of February 2004, the southern part of France is swept by a weather event of wind transport of Saharan particles. The recordings of atmospheric dust contamination and the deposit of dust, which results from it, make an episode of exceptional width. In a few hours, the thickness of the deposit exceeds 1 mm (up to 4 mm in Corsica) with a maximum density of surface charge of 50 g.m{sup -2} (50 tons per km{sup 2}). The loads of the PM{sub 10} type particles in the air, recorded by associations of monitoring of the quality of the air, indicate concentrations multiplied to the maximum by 10 and an influence on the ground of the plume ranging between 300 000 and 350 000 km{sup 2}. To the end, 2 million tons are deposited on a portion of the territory located at the south of a line from Nantes to Besancon. This event also had a significant radio-ecological impact, leading to significant {sup 137}Cs, {sup (239+240)}Pu, {sup 241}Am, activity levels of 38 Bq. kg{sup -1} sec, 1 Bq. kg{sup -1} sec and 0,46 Bq. kg{sup -1} sec, respectively. Quality of air monitoring organisations recorded 10-fold increases in the concentration of charged PM{sub 10} {sup 2}type particles within the cloud; ground coverage stretched over a 300 000 km{sup 2} surface area. Across this whole area, the artificial radioactivity deposits are estimated to 37.10{sup 10} Bq. In term of flow of deposit, this episode represents, with him only, i.e. in a few hours, a {sup 137}Cs deposition equivalent to that recorded on average in a cumulated time of one year. Data from this study show that these weather-climatic episodes generate today, environmental samples which on average, present the highest levels and flux of artificial radioactivities, more than those in the sediments of the Rhone river deposited by flood events, for example. Changes in artificial radionuclide activity levels in the atmospheric area close to ground level are routinely attributed to resuspension of formerly deposited aerosols. In the particular case of the Saharan dust deposits, apart from the resuspension mechanisms that caused the Saharan soil particles to be taken up, other mechanisms may have intervened during transports up until deposit on French soil. Such mechanisms, which have already been identified for other atmospheric compounds or pollutants, give a lead in attempting to understand the enhanced relative or absolute radioactivity of the mineral particles. Two hypotheses have been put forward to explain this enhanced radioactivity: either a process rather like a 'horizontal leaching' of compounds or pollutants present in the atmosphere during transport, or the early fall of the heavier and thus less radioactive mineral particles, giving rise to a relative increase in specific activity. One cannot overlook the contribution these sporadic phenomena make to atmospheric deposits on an annual basis. Further studies are needed to evaluate the weight of these phenomena on a multi-annual scale in the reduction of activity levels in the atmospheric compartment by dry or wet process and at short time scale the deposition of radioactivity with dust from remote regions. Taking into account current metrological performance devices at the IRSN (Institute for Radiological Protection and Nuclear Safety), regular monitoring of these events allow opportunity to follow the changes of plutonium isotopes in the atmosphere. (authors)

354

The radioactivity measurements in soils and fertilizers using gamma spectrometry technique  

Because of their mineral content, soils are naturally radioactive and one of the sources of radioactivity other than those of natural origin is mainly due to the extensive use of fertilizers. The main aim of this paper is to evaluate the fluxes of natural radionuclides in local production of phosphate fertilizers to determine the content of radioactivity in several commercial fertilizers produced in Algeria and to estimate their radiological impact in a cultivated soil even for the long-term exposure due to their application.For these purposes, virgin and fertilized soils were collected from outlying Setif region in Algeria and from phosphate fertilizers used in this area.Gamma spectrometry was exploited to determine activity concentration due to naturally occurring 226Ra, 232Th and 40K in...

355

75 FR 73995 - Lowering Miners' Exposure to Respirable Coal Mine Dust, Including Continuous Personal Dust Monitors  

...1219-AB64 Lowering Miners' Exposure to Respirable Coal Mine Dust, Including Continuous...addressing Lowering Miners' Exposure to Respirable Coal Mine Dust, Including Continuous...dust and lower miners' exposure to respirable coal mine dust. DATES:...

356

NASA GISS: Science Briefs: Desert Dust, Dust Storms and Climate  

Airborne dust particles, or dust aerosols, alter the climate by intercepting sunlight ... Earth from the sun's radiation, dust aerosols have the same effect as a rain cloud. ... While solar radiation is reduced beneath the dust cloud, the absorption of ...

357

42 CFR 84.1145 - Silica dust test; non-powered single-use dust respirators; minimum requirements.  

...Public Health 1 2010-10-01 2010-10-01 false Silica dust test; non-powered single-use dust respirators; minimum...Efficiency Respirators and Combination Gas Masks § 84.1145 Silica dust test; non-powered single-use dust respirators;...

358

Vertical distribution of the Saharan Air Layer from 5 years of CALIPSO observations  

The Saharan Air Layer (SAL) forms as dry and hot air moves across the Sahara desert. SAL, containing substantial amounts of mineral dust, is a dominant feature that influences the large scale environment from West Africa to eastern tropical America, inhibiting tropical cyclogenesis and Atlantic hurricane formation. Furthermore, SAL dust aerosols have a strong impact on the energy budget through the so-called direct and indirect effects. The SAL has been studied with dedicated campaigns at the two sides of the Atlantic or using space observations due to lack of systematic in situ measurements away from the continents. However the campaigns are restricted in time, while satellite observations of thermodynamic variables are affected by the presence of dust. Moreover, satellite measurements of aerosols, particularly in the visible, mostly provide column integrated properties like the optical depth, without information about the vertical distribution. On the other hand, new generation infrared sounders now bring reliable information on the dust layer mean altitude, but their new established results need further validation. However, the two-wavelength lidar CALIOP, launched on board CALIPSO in April 2006, permits an accurate determination of the aerosol vertical distribution, on a global scale. Thanks to depolarisation at 532 nm, CALIOP is able to discriminate between dust and other types of aerosols, which generally do not depolarize light. Here, the L2 5 km aerosol layer product (version 3.01) is used to calculate the vertical distribution of the dust aerosols above the Atlantic during the last 5 years (June 2006 - May 2011) with a horizontal resolution of 1 degree for the four seasons. More specifically, two classes of aerosols are used from the L2 product: dust and polluted dust, in order to take into account the change of dust aerosols optical properties with transport. Results show the latitudinal displacement of the SAL between winter [-5, 15]°N and summer [10, 30]°N. Concerning the vertical distribution, the SAL during winter is between the surface and 3 km near Africa, while its top level drops to 2 km near South America. In summer, SAL is found in the range 1-5 km near Africa, while above the Caribbean Sea its southern part reaches the surface and its top drops to 4 km. During the seasonal cycle from winter to summer, the northern low part of SAL appears decoupled from the ocean surface, indicating the influence of the trade winds on the shape of the SAL. This is further examined by using the ECMWF ERA-Interim wind data for the same period.

359

About contaminant element composition of roadside dust samples from Budapest and Seoul, including Pt and Pd  

Roadside dust was sampled in Seoul megacity /Korea as well as in Budapest and some other places in Hungary, digested with reverse aqua regia in presence of bromine, and analyzed for 29 chemical elements with ICP-OES and ICP-MS methods. In addition to rather traditionally investigated elements, like Pb-Cd-Cr-Ni-As-Sb, newly emerging Pt and Pd from abrasion of automotive catalysts were included in the study. For the analysis of Pd, separation by precipitation with dithizone had to be applied. Principal component analysis was used as a tool to estimate the contribution of various sources. Geogenic element contents were used to estimate geogenic backgrounds und inputs from soils erosion. Seoul is an East Asian densely populated megacity, not far from the seaside, and surrounded by granite rocks. To the contrary, Budapest is a European continental city surrounded mainly by plains formed in the tertiary. Background concentrations were estimated from median concentrations in soils over alluvial deposits from the East of Austria, as well as from Poland. Background concentrations for Seoul were estimated from Shiheung farmland soil, a town close to the megacity. As a result, traffic related contaminations were highly effected by traffic related activities, like stop and go. Pt and Pb levels in roadside dusts from Budapest citiy were in the range of 2-133 ?g/kg (av. 62,9 ?g/kg), and 88 - 2838 mg/kg (av. 662 mg/kg) respectively. The highest Pt and Pb levels in roadside dust were found at major roads with high traffic volumes. Due to the geo-accumulation index, in all roadside soils sampled in Hungary, Cu-Pb-Zn were enriched, and Cd-Mo and occasionally Ba from Budapest in addition, but As-Co-Cr-Hg-Ni-Tl-V were not. In roadside dusts from Seoul, heavy contaminations of As-Cd-Cu-Mo-Pb-Zn were found, but no significant increase of Co-Cr-Ni-V. The pollution index, which refers to the permissible levels of As-Cd-Cu-Hg-Pb-Sb-Tl-V, indicates heavy pollution for roadside dusts from both cities, and moderate pollution for roadside dusts from the rest of Hungary. Pt and Pd concentrations were strongly intercorrelated, but not with the pollution index. In dusts from Budapest, Pt and Pd were strongly correlated with each other, and moderately just with Sn and Bi. In Seoul dusts, Pt was strong positively correlated with Ba-Cu-Fe-Ir-Mo-Pd-Sb, and slightly with Cr-Fe-Mo-Ni, but negatively with Ca-Cd-Hg-Pb. Pd in Seoul dusts, however, was positively correlated just with Pt and Ir, but negatively with K-Li-Na-Pb-Sr.

360

Activation of the major constituents of tissue and air by a fast neutron radiation therapy beam  

The production of /sup 11/C, /sup 13/N, /sup 15/O from C, N, O, and of /sup 39/Cl and /sup 41/Ar from Ar by a p(66)Be(49) clinical neutron therapy beam has been measured. The results of these measurements were used to estimate the production of other radionuclides, then to estimate airborne radioactivity in a typical neutron therapy room and radioactivity induced in body tissues during treatment. Only under special circumstances would airborne radioactivity necessitate a waiting period before entering a typical treatment room. The additional dose to a treatment volume due to decay products from radioactivity induced within that volume would amount to a few thousandths of the given dose and the additional body dose outside the treated volume would be a few millionths of the given dose.

 
 
 
 
361

Radiological characterization of targets from the ISOLDE facility at CERN  

The European Laboratory for Particle Physics (CERN, Geneva) has been operating accelerators for high-energy physics both on Swiss and French territory for 50 years. Due to the interaction of the particle beams with matter, part of the accelerator structure and its surroundings become radioactive. Once at the end of their operational lifetime, these materials are defined as waste. The elimination of radioactive waste towards the final repositories in France and Switzerland requires the determination of the radionuclide inventory. The radioactive nuclides generated in accelerators are different from those identified in reactors. With very few exceptions there are no fission products and alpha emitters. One of the requirements for acceptance of an item of waste in a repository is an estimate of the residual long-lived radioactive nuclides with their specific activity. The list should be exhaustive and include also those nuclides which are difficult to be experimentally detected. Different methods for the evaluat...

362

An experimental study regarding the determination of seasonal heat transfer coefficient in KURT by convection conditions  

In high-level radioactive waste repositories, heat is generated by the radioactive decay of the waste. This can affect the safety of the repository because the surrounding environment can be changed by heat transferred through the rock. Therefore, in order to ensure the safety of the repository, the temperature change of the atmosphere in the repository due to the heat generated by high-level radioactive wastes needs to be predicted and an appropriate heat reduction system is required. Through the construction of the KAERI Underground Research Tunnel (KURT) by Korea Atomic Energy Research Institute (KAERI), variable experiments about radioactive wastes disposal are in progress and the data on the properties of the surrounding rock in KURT had already been secured. As the internal heater se...

363

The strategy of APO-Hazardous Waste Management Agency in forming the model of public acceptance of Croatian Waste Management Facility  

Some of basic elements related to public participation in hazardous and radioactive waste management in Croatia are underlined in the paper. Most of them are created or led by the APO-Hazardous Waste Management Agency. Present efforts in improvement of public participation in the field of hazardous and radioactive waste management are important in particular due to negligible role of public in environmentally related issues during former Yugoslav political system. For this reason it is possible to understand the public fearing to be deceived or neglected again. Special attention is paid to the current APO editions related to public information and education in the field of hazardous and radioactive waste management. It is important because only the well-informed public can present an active and respectful factor in hazardous and radioactive waste management process.

364

Radiological Terrorism - Chemcases.com  

Radiological TerrorismWhile attacks by terrorists have not involved the use of non-fissionable, radioactive materials, they have nevertheless increased concerns over the possibility of individuals or groups acquiring these materials. Radiological materials have the potential to be used as weapons as either radiological dispersal devices (RDD) or radiation emission devices (RED). An RDD is a device that disperses radioactive material into the environment. By contrast, an RED employs a stationary radioactive source to expose victims to high levels of radiation. These devices are often referred to as Âweapons of mass disruption in contrast to fission devices, which are known as a Âweapons of mass destruction due to their massive impact on the targets. No successful radiological attack has occurred to date, although intelligence data reveals that Al Qaeda has expressed an interest in acquiring radioactive materials, and RDDs planted by Chechen rebels were disarmed in 1995 and 1998.

365

[Assessment of modern radioecological situation at nuclear explosion "Chagan" (Balapan Site, Semipalatinsk Nuclear Test Site, Kazakhstan)].  

Results on estimation of modern radioecological situation at nuclear explosion "Chagan" based on large-scale cartographic studies (1:25000) of a test area (4 km2) are presented. Maximum gamma-irradiation doses were observed at bulk of ground surrounded a crater and at radioactive fall-outs extended to the North-East and to the SouthWest from the crater. Based on data on artificial radionuclide specific activity most part of soil samples were attributed to radioactive wastes according to IAEA (1996) and OSPORB (1999). Natural decrease of soil radioactivity up to safety level due to 60Co, 137Cs, 90Sr, 152Eu, 154Eu radioactive decay and 241Am accumulation-decay will not take place within the next 60 years at the studied area. PMID:19004330

366

Automatic control by natural gamma radiation emitted by coal; Control Automatico mediante Radiometria Gamma Natural de la Cenizas de los Carbones  

Due to the characteristics of its coal and orebody, Monsacro shaft was chosen to host the test. The ash percentage of the different coal seams was carried out by two different methods: Traditional analysis in laboratory. Analysis by means of natural gamma radiation emitted by coal. The following conclusions were obtained after the test: Neither during the mounting nor during the test, a problem was encountered in the working of the radioactive methods. The absolute error between the two methods was minimum. The radioactive analysis is total (this means that the whole coal is analysed) and it is carried out in short period of time. The traditional one is just partial, and could take a few hours to accomplish it. The radioactive one is done in the wagon or in the belt conveyor directly, meanwhile the traditional one needs sample takers permanently. The investment cost of the radioactivity method is amortized within two years. (Author)

367

Generation of atomic hydrogen in the air under action of beta decay of radioactive elements  

Physical and chemical properties of the atmospheric components change under action of radioactive emissions, and, as a result, anomalous gas-aerosol and ionized areas are occurred and can be registered by remote optical and radiometric methods. One of the effects, in the view of passive detection of radioactive pollution is the dissociation of water vapor (H2O) and formation of anomalous fields with the high contents of hydrogen (H) and hydroxyl (OH), which spontaneous radiation in the microwave range can be used for identification of radioactivity in emissions. The process of electron multiplication due to degradation of energy of ?-electrons, generated at decay of a radioactive isotope 85Kr in the emission stack is described in this paper. The estimation of atomic hydrogen concentration in cross-section of the stack on various distances from an emission source is carried out depending on its height and activity.

368

Anthropocene changes in desert area: Sensitivity to climate model predictions  

Changes in desert area due to humans have important implications from a local, regional to global level. Here we focus on the latter in order to better understand estimated changes in desert dust aerosols and the associated iron deposition into oceans. Using 17 model simulations from the World Climate Research Programme's Coupled Model Intercomparison Project phase 3 multi-model dataset and the BIOME4 equilibrium vegetation model we estimate changes in desert dust source areas due to climate change and carbon dioxide fertilization. If we assume no carbon dioxide fertilization, the mean of the model predictions is that desert areas expand from the 1880s to the 2080s, due to increased aridity. If we allow for carbon dioxide fertilization, the desert areas become smaller. Thus better understanding carbon dioxide fertilization is important for predicting desert response to climate. There is substantial spread in the model simulation predictions for regional and global averages.

369

Interstellar dust  

Dust is a key component of the Universe, especially regarding galaxies evolution, playing an essential role for both the physics and chemistry of the interstellar medium. In this paper, we give a brief review of interstellar dust. We describe the main dust observables and how it allows us to constrain dust properties. We discuss the dust lifecycle and the dust evolution in the ISM. We also present a physical dust model, DustEM.

370

Vehicle non-exhaust emissions from the tyre-road interface - effect of stud properties, traction sanding and resuspension  

In Northern cities respirable street dust emission levels (PM10) are especially high during spring. The spring time dust has been observed to cause health effects as well as discomfort among citizens. Major sources of the dust are the abrasion products from the pavement and traction sand aggregates that are formed due to the motion of the tyre. We studied the formation of respirable abrasion particles in the tyre-road interface due to tyre studs and traction sanding by a mobile laboratory vehicle Sniffer. The measurements were preformed on a test track, where the influence of varying stud weight and stud number per tyre on PM10 emissions was studied. Studded tyres resulted in higher emission levels than studless tyres especially with speeds 50 km h-1 and higher; however, by using light weight studs, which approximately halves the weight of studs, or by reducing the number of studs per tyre to half, the emission levels decreased by approximately half. Additionally measurements were done with and without traction sand coverage on the pavement of a public road. After traction sanding the emission levels were not affected by tyre type but by formation and suspension of traction sand related dust from the road surface. The emissions after traction sanding decreased as a function of time as passing vehicles’ motion shifted the sand grains away from the areas with most tyre-road contact.

371

High levels of antimony in dust from e-waste recycling in southeastern China.  

Environmental contamination due to uncontrolled e-waste recycling is an emerging global issue. Antimony (Sb) is a toxic element used in semiconductor components and flame retardants for circuit board within electronic equipment. When e-waste is recycled, Sb is released and contaminates the surrounding environment; however, few studies have characterized the extent of this problem. In this study, we investigated Sb and arsenic (As) distributions in indoor dust from 13 e-waste recycling villages in Guiyu, Guangdong Province, southeastern China. Results revealed significantly elevated concentrations of Sb (6.1-232 mg/kg) in dust within all villages, which were 3.9-147 times higher than those from the non e-waste sites, indicating e-waste recycling was an important source of Sb pollution. On the contrary, As concentrations (5.4-17.7 mg/kg) in e-waste dusts were similar to reference values from the control sites. Therefore, dusts emitted from e-waste recycling may be characterized by high Sb/As ratios, which may help identify the contamination due to the e-waste recycling activities. PMID:21907394

372

Molecular Gas, Dust and Star Formation in the Barred Spiral NGC 5383  

We present multi-wavelength (interferometer and single-dish CO J=1-0, Halpha, broadband optical and near-infrared) observations of the classic barred spiral NGC 5383. We compare the observed central gas and dust morphology to the predictions of recent hydrodynamic simulations. In the nuclear region, our observations reveal three peaks lying along a S-shaped gas and dust distribution. In contrast, the model predicts a circumnuclear ring, not the observed S-shaped distribution; moreover, the predicted surface density contrast between the central gas accumulation and the bar dust lanes is an order of magnitude larger than observed. The discrepancies are not due to unexplored model parameter space or a nuclear bar but are probably due to the vigorous (7 solar masses per year) star formation activity in the center. As is common in similar bars, the star formation rate in the bar between the bar ends and the central region is low (~0.5 solar masses per yr), despite the high gas column density in the bar dust lanes;...

373

Far-ultraviolet Observation of the Aquila Rift with FIMS/SPEAR  

We present the results of far ultraviolet (FUV) observations of the broad region around the Aquila Rift including the Galactic plane. As compared with various wavelength data sets, dust scattering is found to be the major origin of the diffuse FUV continuum in this region. The FUV intensity clearly correlates with the dust extinction level for E(B - V) 0.2 due to heavy dust extinction combined with the effect of nonuniform interstellar radiation fields. The FUV intensity also correlates well with H? intensity, implying that at least some fraction of the observed H? emission could be the dust-scattered light of H? photons originating elsewhere in the Galaxy. Most of the Aquila Rift region is seen devoid of diffuse FUV continuum due to heavy extinction while strong emission is observed in the surrounding regions. Molecular hydrogen fluorescent emission lines are clearly seen in the spectrum of "Aquila-Serpens," while "Aquila-East" does not show any apparent line features. CO emission intensity is also found to be higher in the "Aquila-Serpens" region than in the "Aquila-East" region. In this regard, we note that regions of star formation have been found in "Aquila-Serpens" but not in "Aquila-East."

374

Models Support Energy-Saving Microwave Technologies  

During the Apollo Program, astronauts on the Moon encountered a small menace that created big problems: lunar dust. Similar to how tiny bits of Styrofoam behave on Earth adhering to anything they touch lunar dust sticks to spacesuits, spacecraft, tools, and equipment, and is extremely difficult to remove. The clingy nature of the substance is partly due to its electrostatic charge but is also due to its physical characteristics: The sharp, irregularly shaped grains have edges like burrs and feel like abrasive talcum powder to the touch. Not only a nuisance, Moon dust is also a potential health and safety risk. Because it is often laden with ultraviolet radiation and high iron content, it can be detrimental if it gets into the eyes or lungs. In fact, some of the particles are so small that the human body does not even detect them in order to expel them. On the Apollo missions, equipment covered with the dark-colored Moon dust suffered from the absorption of sunlight and tended to overheat. NASA has investigated tools and techniques to manage the sticky stuff, including magnets, vacuums, and shields. In 2009, Kennedy Space Center collaborated with a small business to investigate a method to harden the Moon's surface in a sense, to pave the surface so astronauts and robots could land, drive, and work without disrupting and scattering the material.

375

Constraining the Origin of Impact Craters on Al Foils from the Stardust Interstellar Dust Collector  

Preliminary examination (PE) of the aerogel tiles and Al foils from the Stardust Interstellar Dust Collector has revealed multiple impact features. Some are most likely due to primary impacts of interstellar dust (ISD) grains, and others are associated with secondary impacts of spacecraft debris, and possibly primary impacts of interplanetary dust particles (IDPs) [1, 2]. The current focus of the PE effort is on constraining the origin of the individual impact features so that definitive results from the first direct laboratory analysis of contemporary ISD can be reported. Because crater morphology depends on impacting particle shape and composition, in addition to the angle and direction of impact, unique particle trajectories are not easily determined. However, elemental analysis of the crater residues can distinguish real cosmic dust from the spacecraft debris, due to the low cosmic abundance of many of the elements in the spacecraft materials. We present here results from the elemental analysis of 24 craters and discuss the possible origins of 4 that are identified as candidate ISD impacts

376

EPA FABRIC FILTRATION STUDIES: 6. INFLUENCE OF DUST PROPERTIES ON PARTICLE PENETRATION  

The report examines the importance of dust properties in determining dust penetration through a fabric filter. The major property considered is the size distribution of the dust, which is an important dust property for dust penetration. Most other important variables of dust pene...

377

Decontamination works by entering cells in hot laboratories  

The decontamination of radioactive substances in the post-irradiation testing facilities is the indispensable, important works for maintaining the performance of testing equipment related to the works in cells. The inside of cells and various testing equipments are contaminated at high level by the cutting and destructive testing of irradiated fuel and material samples. Consequently, the restriction of the accumulation of contamination in cells is endeavored, and the decontamination works by entering cells once every year have been carried out prior to the maintenance and checkup of the equipments in cells, shielding doors, in-cell monitors, ventilation facilities and so on. At present, for the labor saving in works, the shortening of period, the reduction of materials, the reduction of radioactive wastes, the improvement of safety in works and so on, the chemical decontamination using the material for removing coating is carried out in addition to usual wiping method. In this report, the decontamination works for concrete cells are described. The outline of test cells, the nuclides contaminating hot cells, the particle size of radioactive dusts, the procedure of decontamination works, protective clothes and the protectors for breathing, the decontaminating material for removing coating, the amount of waste generation and so on are reported. (K.I.).

378

Monitoring of scrap and finished products for radioactive components; Ueberwachung von Schrott und Fertigprodukten auf radioaktive Bestandteile  

Radioactive components can get through carelessness or intentionally with scrap deliveries to steelworks in the melting units, where they would deposit in the melt (and thus in the finished products) as well as in the slag, refractory lining and waste gas dust. Monitoring measuring systems capable of sounding an early alarm in case of radioactive contamination of the scrap, are required to prevent an endangerement of the personnel and a negative effect on the utilization of the material steel. Measuring systems with large-area scintillators feature a high detection sensitivity, without essentially changing the supply routes of scrap-processing plants. Such monitoring facilities can be installed for incoming and outgoing inspection at scrap traders and scrap users, but also at territorial limits to prevent the import of radioactive scrap and finished products. (orig.) [Deutsch] Durch Fahrlaessigkeit oder Vorsatz koennen mit den Schrottlieferungen an die Stahlwerke radioaktive Bestandteile in die Schmelzaggregate gelangen, die sich in der Schmelze (und damit in den Fertigprodukten), der Schlacke, der Feuerfestauskleidung sowie im Abgasstaub ablagern wuerden. Um eine Gefaehrdung des Personals zu verhindern und eine Beeintraechtigung des Gebrauchs des Werkstoffs Stahl zu vermeiden, sind ueberwachende Messsysteme erforderlich, die fruehzeitig im Fall einer radioaktiven Verunreinigung des Schrotts Alarm geben. Messsysteme mit grossflaechigen Szintillatoren verfuegen ueber eine hohe Nachweiswahrscheinlichkeit, ohne die Versorgungswege der schrottverarbeitenden Betriebe wesentlich zu veraendern. Derartige Monitoreinrichtungen koennen zur Eingangs- und Ausgangskontrolle bei Schrotthaendlern und Schrottverbrauchern, aber auch an den Territorialgrenzen zur Verhinderung des Imports von radioaktiven Schrotten und Fertigprodukten installiert werden. (orig.)

379

Unique radiation protection design for processing high grade uranium ores at the McClean Lake mill  

Rich uranium deposits in northern Saskatchewan are coming into production and will last for the next few decades. The combination of high ore grades and more stringent radiation protection regulations require complex mill design features far different then those for conventional uranium mills. The Mc Clean Lake mill, which has operated since June 1999 with production rates of approximately 6 million lbs of U{sub 3}O{sub 8} annually, is currently being expanded to receive uranium ore slurry with nominal feed grades up to about 20% U{sub 3}O{sub 8} and production rate of up to 12 million lbs annually. The mill design ensures that workers are separated from radioactive ore being processed through the use of slurry handling and processing systems that are totally enclosed and has several state-of-the-art shielding and ventilation features that protect workers against external gamma radiation and airborne radioactive materials (radon progeny and radioactive dusts). This paper discusses the unique design of the Cogema Mc Clean Lake mill, with some key radiation protection results and comparisons to conventional uranium mills. (authors)

380

Relationship between leukemia incidence and residing and/or working near the Pilgrim 1 nuclear power plant in Plymouth, Massachusetts  

To determine whether a strong association between leukemia incidence between 1978 and 1986 and potential for exposure to radiation emitted from the Pilgrim 1 nuclear power plant in Plymouth, Massachusetts was a spurious finding resulting from either (1) failure to account for temporal variation in the level of radioactivity released from the plant or (2) inattention to certain potentially confounding factors, additional age/sex-matched case-control analyses controlled for the effects of socioeconomic status (SES), work history, and cigarette smoking were performed with data collected in the Southeastern Massachusetts Health Investigation -- a study of leukemia among residents aged 13 and older of 22 southeastern Massachusetts towns. None of the additional analyses, including incorporation of emissions data into the exposure-assessment scheme and crude attempts to control for (1) medical-radiation exposure, (2) potential for exposure to pesticides sprayed on cranberry bogs, or (3) workplace exposure to radiation, chemical solvents, dust, or fumes, altered the finding of a statistically significant dose-response relationship between leukemia incidence and potential for exposure to radioactive emissions. The trend in the association over time was not entirely consistent, however, with the hypothesis that unusually large amounts of radioactivity reportedly released from the plant during the mid-1970s were responsible for the observed effects. Recommendations were made for further study of the Plymouth-area population for studies of this problem elsewhere.

 
 
 
 
381

Volume reduction by the incineration of the combustible radioactive solid samples from radioisotope usage at the utilization facility. Estimation of the distribution of low energy {beta}-emitter using the imaging plate  

We want to establish a system of volume reduction by the incineration of the combustible radioactive solid wastes from radioisotope usage at the utilization facility. We have been performing experiments using an experimental incineration system to examine the distribution of radionuclides during incineration and to collect basic data. To reproduce the realistic conditions of incineration of low-level radioactive wastes in an experimental system, we adopted new incineration methods in this study. Low level radioactive samples (LLRS) were set up in a mesh container of stainless steel and incinerated at high temperature (over 800 degC) generated by two sets of high calorie gas burners. Low energy {beta}-emitters {sup 35}S, {sup 45}Ca, {sup 33}P, and a high energy {beta}-emitter {sup 32}P were used for the experiment. Their translocation percentages in