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Sample records for chislennoe modelirovanie dissipativnykh

  1. Simulation of << Hot >> particles formation during the accident at the Chernobyl NPP.; Modelirovanie obrazovaniya << goryachikh >> chastits vo vremya avarii na ChAEhS.

    Energy Technology Data Exchange (ETDEWEB)

    Kashparov, V A; Ivanov, Yu A; Prister, B S; Zvarich, S I; Protsak, V P; Khomutinin, Yu V; Polyakov, V D; Gudkov, A N; Kurepin, A D; Pazukhin, Eh M [Yinstitut Syil` s` kogospodars` koyi Radyiologyiyi, Kyiv (Ukraine); [Moskovskij Inzhenerno-Fizicheskij Inst., Moscow (Russian Federation)

    1994-12-31

    Dispersal composition of fuel << hot >> particles formed after oxidation of real Chernobyl nuclear fuel in the air for 3-21 hours at 673-1173 K was obtained. Mechanism of ruthenium particles formation during the accident (with dispersion of nuclear fuel) as a result of ruthenium oxidation, its sublimation, condensation and restoration on materials, presented by the elements of iron group was modelled. Dynamics of relative release of fission products, as well as of transuranium and transplutonium elements from real and modeled << hot >> particles at their high temperature incineration (1273-2273 K) in the inert media was measured.

  2. Modelling of the Woods-Saxon eikonal function for nuclear elastic scattering; Modelirovanie ehjkonal`noj funktsii uprugogo rasseyaniya v pole potentsiala Vudsa-Saksona

    Energy Technology Data Exchange (ETDEWEB)

    Luk` yanov, V K; Permyakov, V P; Chubov, Yu V

    1999-12-31

    The eikonal phase is needed for the analytical calculations for the nuclear scattering in the high energy approximation (E>>U, kR>>1). In this paper we obtain its model expression for scattering on Woods-Saxon potential which with a good accuracy reproduces its behaviour in complex plane which is found numerically. In the case one evaluates explicitly the scattering amplitude using saddle-point method makes the physics more understandable. The numerical amplitudes and cross sections of nucleus-nucleus scattering are compared with exact calculations. (author) 9 refs., 7 figs. Submitted to Izvestiya Akademii Nauk. Rossijskaya Akademiya Nauk. Seriya Fizicheskaya

  3. Modelirovanie rasprostranenija izlučenija v BIKS s učetom anizotropii rassejanjia dlja optimizacii raspoloženjia istočnikov i prijomnikov izlučenija.

    Czech Academy of Sciences Publication Activity Database

    Isaev, M.R.; Oganesyan, V.V.; Húsek, Dušan; Snášel, V.

    2017-01-01

    Roč. 67, č. 4 (2017), s. 546-553 ISSN 0044-4677 Institutional support: RVO:67985807 Keywords : brain -computer interface * Monte-Carlo simulation * near-infrared spectroscopy * focuses of hemodynamic activity Subject RIV: IN - Informatics, Computer Science OBOR OECD: Computer sciences, information science, bioinformathics (hardware development to be 2.2, social aspect to be 5.8) Impact factor: 0.236, year: 2016 https://elibrary.ru/item.asp?id=29766803

  4. Anisotropic Migration in Slab Lattices; Migration Anisotrope dans les Reseaux a Plaques; Anizotropicheskaya migratsiya v reshetkakh iz plastin; Migracion Anisotropica en Reticulados de Placas

    Energy Technology Data Exchange (ETDEWEB)

    Honeck, H. C.; Quiquemelle, B. C. [Brookhaven National Laboratory, Upton, NY (United States)

    1965-08-15

    }{sub n} dara los coeficientes de difusion. En el Brookhaven National Laboratory se estan haciendo experimentos con placas alternadas de aluminio y polietileno. Los autores han seleccionado las siguientes secciones eficaces en un solo grupo: aluminio, {Sigma}a = 0, 01228 cm{sup -1}, {Sigma}s = 0, 08428 cm{sup -1}, {mu} = 0; polietileno, {Sigma}a - 0, 01947 cm-1, {Sigma}s = 2,593 cm{sup -1}, {mu} = 0,25. (author) [Russian] Odnoj iz samyh novyh oblastej primenenija jeksperimentov s impul'snymi nejtronami javljaetsja izmerenie kojefficienta diffuzii teplovyh nejtronov v razlichnyh napravlenijah v geterogennoj srede. Opisyvaetsja teoreticheskij metod, razrabotannyj s celyo predskazanija takih kojefficientov diffuzii, i predstavljajutsja nekotorye rezul'taty jeksperimentov, provodimyh v nastojashhee vremja v Brukhejvene. Interpretacija jetih jeksperimentov v znachitel'noj stepeni uproshhaetsja, esli jeksperimental'naja sborka javljaetsja bol'shoj. V jetom sluchae mozhno prenebregat' diffuzionnym ohlazhdeniem, spektry schitat' maksvellovskimi i rassmatrivat' edinstvennuju gruppu energii. Pri takom uproshhenii mozhno chislenno reshit' uravnenie perekosa dlja sluchaja plastinchatoj geometrii. My podstavljaem reshenie modeli Empty-Set (x, y, z, {Omega}, t) = exp (iB{sub 1}X + iB{sub 2}y - {lambda}t) Empty-Set (x, {Omega}) v uravnenie perenosa i reshaem Empty-Set (x, {Omega}) putem sochetanija metodov fil'trov dlja vyravnivanija dannyh i integral'noj teorii perenosa. Osnovnye preimushhestva jetogo metoda po sravneniju s sushhestvujushhimi sostojat v tom, chto legko vkljuchajutsja pogloshhenie i anijeotropiches- koe rassejanie i jachejka mozhet sostojat' iz mnogih podoblastej. Hotja sdelana popytka najti B{sub 1} i B{sub 2} s dannym sobstvennym znacheniem {lambda}, udobnee vmesto iB{sub l} postavit' kj i vmesto i V{sub 2} - k{sub 2} i opredelit' k{sub 2} s dannym k{sub 1} i {lambda} takom sluchae {lambda} mozhno vyrazit' v vide stelennogo rjada K{sup 2}{sub 1} i K{sup 2}{sub 2

  5. Stability of a Magnetically Confined 20-KeV Steady-State Plasma; Stabilite d'un Plasma Stationnaire de 20 KeV Confine par un Champ Magnetique; Ustojchivost' 20 KehV-statsionarnoj plazmy, uderzhivaemoj magnitnym polem; Estabilidad en Regimen Estacionario de un Plasma de 20 KeV Confinado Magneticamente

    Energy Technology Data Exchange (ETDEWEB)

    Futch, Jr., A. H.; Damm, C. C.; Foote, J. H.; Freis, R.; Gordon, F. J.; Hunt, A. L.; Killeen, J.; Moses, K. G.; Post, R. F.; Steinhaus, J. F. [Lawrence Radiation Laboratory, Livermore, CA (United States)

    1966-04-15

    ''Alisa'' (Livermor) issledovalas' ustojchivost' 20-kilovol'tovoj stacionarnoj vodorodnoj plazmy pri razlichnyh konfiguracijah uderzhivajushhih magnitnyh polej. Dlja sozdanija plazmy ispol'zovalsja metod inzhekcii nejtral'nyh chastic v lovushku. V magnitnom pole prostoj probochnoj konfiguracii nabljudalis' kolebanija nizkoj chastoty, i plotnost' zahvachennyh chastic byla ogranichennoj. Jeti fakty ob{sup j}asnjajutsja dejstviem mehanizma nizkochastotnoj drejfovoj neustojchivosti. Teoreticheskoe izuchenie jetoj neustojchivosti provodilos' s uchetom jeffektov, svjazannyh s konechnym razmerom ionnyh orbit, s jelektricheskim polem nulevogo priblizhenija i s neravnymi znachenijami ionnyh i jelektronnyh plotnostej. V nastojashhem issledovanii kak jelektricheskoe, tak i magnitnoe pole mogut byt' proizvol'nymi funkcijami prostranstvennoj koordinaty g. Poskol'ku poluchit' analiticheskoe reshenie dlja poluchennyh differencial'nyh uravnenij voobshhe nevozmozhno, to osnovnye uravnenija byli resheny chislenno metodom konechnyh raznostej. Rezul'taty soglasujutsja s analiticheskimi reshenijami, poluchennymi dlja chastnogo sluchaja jelektricheskogo polja ne nulevogo priblizhenija i uspeshno ob{sup j}asnjajut variacii plotnosti i drejfa, nabljudavshiesja jeksperimental'no v uslovijah slabogo jelektricheskogo polja. Poskol'ku dannoe teoreticheskoe issledovanie polagaet, chto magnitnoe pole dolzhno javljat'sja proizvol'noj funkciej g, mozhno poluchit' reshenija dlja polej s pervonachal'no otricatel'nym gradientom, kotoryj potom stanovitsja polozhitel'nym po mere uvelichenija koordinaty g. Rezul'taty jetih raschetov sravnivajutsja s jeksperimental'nymi nabljudenijami stabilizacii, poluchennymi pri dobavlenii k prostomu probkovomu polju giperbolicheskih polej. Jeksperimental'no pokazano, chto dobavlenie kak dodekapol'nyh, tak i oktupol'nyh polej jeffektivno podavljaet poteri ionov, vyzvannyh drejfovoj neustojchivost'ju. Ostavshiesja ionnye poteri voznikajut iskljuchitel'no za schet ih

  6. Theoretical Studies of Electron Injection and E-Layer Build-Up in Astron; Etudes Theoriques sur l'Injection d'Electrons et la Formation de la Couche E dans l'Astron; Teoreticheskie izucheniya ehlektronnoj inzhektsii i narashchivaniya sloya-E v ustanovke ''Astron''; Estudios Teoricos de Electrones y Formacion de la Capa E en la Instalacion Astron

    Energy Technology Data Exchange (ETDEWEB)

    Killeen, J.; Neil, V. K.; Heckrotte, W. [Lawrence Radiation Laboratory, Livermore, CA (United States)

    1966-04-15

    inversion del campo. (author) [Russian] Zahvat vysoko intensivnyh puchkov reljativistskih jelektronov, inzhektiruemyh v ustanovku Astron, mozhet chastichno osushhestvljat'sja za schet kogerentnyh jelektromagnitnyh sil. Osevoe jelektrostaticheskoe razmytie azimutal'no inzhektiruemogo puchka mozhet byt' predotvrashheno ili podavleno blagodarja sootvetstvujushhej konstrukcii vneshnej passivnoj shemy. Pod dejstviem sobstvennyh sil chasticy rasprostranjajutsja v fazovom prostranstve z-Pz, i chast' puchka zahvatyvaetsja za schet poter' drugoj chasti. V dopolnenie k jetomu jeffektu dlja dostatochno vysokih tokov v puchke svjaz' reljativistskogo puchka s passivnoj shemoj mozhet privesti k znachitel'noj potere osevogo momenta iz-za dissipacii jEhnergii. Teoreticheski byla izuchena odnomernaja model' real'noj geometrii Astrona. Funkcii Grina dlja sobstvennyh jelektricheskih i magnitnyh polej byli rasschitany analiticheskim sposobom i vvedeny v uravnenie Vlasova, kotoroe opredeljaet osevoe dvizhenie jelektronov. Rezul'taty raschetov pozvoljajut provesti nekotorye kachestvennye sravnenija s jeksperimental'nymi rezul'tatami, poluchennymi v jeksperimente na Astrone. Kak i predpolagalos', zahvachennye jelektrony obrazujut cilindricheskij sloj dostatochnoj intensivnosti, tak chto sobstvennoe magnitnoe pole sravnimo s prilozhennym polem. Matematicheskaja model' dlja narastanija jelektronnogo sloja i sobstvennogo polja javljaetsja zavisimym ot vremeni uravneniem Vlasova sovmestno s uravnenijami Maksvella. Sistema javljaetsja aksial'no-simmetrichnoj, i predpolagaetsja polnaja nejtralizacija. Komponenty polja Vg i B z mozhno vyvesti na osnovanii funkcii potoka {psi}(r, z, t). Kanonicheskij uglovoj moment javljaetsja konstantoj dvizhenija, i pojetomu my mozhem rassmatrivat' funkciju jelektronnogo raspredelenija f{sub e} (r, z, R{sub g}, R{sub g}). Differencial'nye uravnenija dlja f{sub e} i {psi} reshajutsja chislenno s ispol'zovaniem metodov konechnyh raznostej. Fazovoe prostranstvo soderzhit