Matches in SemOpenAlex for { <https://semopenalex.org/work/W3104267550> ?p ?o ?g. }
- W3104267550 endingPage "1077" @default.
- W3104267550 startingPage "1063" @default.
- W3104267550 abstract "We have developed a three-dimensional numerical model and applied it to simulate plasma flows in semi-detached binary systems whose accretor possesses a strong intrinsic magnetic field. The model is based on the assumption that the plasma dynamics are determined by the slow mean flow, which forms a backdrop for the rapid propagation of MHD waves. The equations describing the slow motion of matter were obtained by averaging over rapidly propagating pulsations. The numerical model includes the diffusion of magnetic field by current dissipation in turbulent vortices, magnetic buoyancy, and wave MHD turbulence. A modified three-dimensional, parallel, numerical code was used to simulate the flow structure in close binary systems with various accretor magnetic fields, from 105 to 108 G. The conditions for the formation of the accretion disk and the criteria distinguishing the two types of flow corresponding to intermediate polars and polars are discussed." @default.
- W3104267550 created "2020-11-23" @default.
- W3104267550 creator A5065846440 @default.
- W3104267550 creator A5078669921 @default.
- W3104267550 date "2010-12-01" @default.
- W3104267550 modified "2023-10-18" @default.
- W3104267550 title "Formation of accretion disks in close-binary systems with magnetic fields" @default.
- W3104267550 cites W1611149296 @default.
- W3104267550 cites W2013997547 @default.
- W3104267550 cites W2018346330 @default.
- W3104267550 cites W2018978491 @default.
- W3104267550 cites W2023148293 @default.
- W3104267550 cites W2026700540 @default.
- W3104267550 cites W2044230743 @default.
- W3104267550 cites W2047170888 @default.
- W3104267550 cites W2053318695 @default.
- W3104267550 cites W2055706704 @default.
- W3104267550 cites W2064397845 @default.
- W3104267550 cites W2085024994 @default.
- W3104267550 cites W2097332955 @default.
- W3104267550 cites W2789977770 @default.
- W3104267550 cites W3099555891 @default.
- W3104267550 cites W3124871405 @default.
- W3104267550 cites W3214785470 @default.
- W3104267550 cites W4206521167 @default.
- W3104267550 cites W4250995714 @default.
- W3104267550 cites W4301644607 @default.
- W3104267550 doi "https://doi.org/10.1134/s1063772910120012" @default.
- W3104267550 hasPublicationYear "2010" @default.
- W3104267550 type Work @default.
- W3104267550 sameAs 3104267550 @default.
- W3104267550 citedByCount "18" @default.
- W3104267550 countsByYear W31042675502012 @default.
- W3104267550 countsByYear W31042675502013 @default.
- W3104267550 countsByYear W31042675502015 @default.
- W3104267550 countsByYear W31042675502016 @default.
- W3104267550 countsByYear W31042675502017 @default.
- W3104267550 countsByYear W31042675502018 @default.
- W3104267550 countsByYear W31042675502019 @default.
- W3104267550 countsByYear W31042675502020 @default.
- W3104267550 countsByYear W31042675502021 @default.
- W3104267550 crossrefType "journal-article" @default.
- W3104267550 hasAuthorship W3104267550A5065846440 @default.
- W3104267550 hasAuthorship W3104267550A5078669921 @default.
- W3104267550 hasBestOaLocation W31042675502 @default.
- W3104267550 hasConcept C115260700 @default.
- W3104267550 hasConcept C121332964 @default.
- W3104267550 hasConcept C135402231 @default.
- W3104267550 hasConcept C140820882 @default.
- W3104267550 hasConcept C196558001 @default.
- W3104267550 hasConcept C25621703 @default.
- W3104267550 hasConcept C2776401274 @default.
- W3104267550 hasConcept C30475298 @default.
- W3104267550 hasConcept C31532427 @default.
- W3104267550 hasConcept C33923547 @default.
- W3104267550 hasConcept C38349280 @default.
- W3104267550 hasConcept C44870925 @default.
- W3104267550 hasConcept C48372109 @default.
- W3104267550 hasConcept C538625479 @default.
- W3104267550 hasConcept C57879066 @default.
- W3104267550 hasConcept C62520636 @default.
- W3104267550 hasConcept C74650414 @default.
- W3104267550 hasConcept C82706917 @default.
- W3104267550 hasConcept C94375191 @default.
- W3104267550 hasConcept C97355855 @default.
- W3104267550 hasConceptScore W3104267550C115260700 @default.
- W3104267550 hasConceptScore W3104267550C121332964 @default.
- W3104267550 hasConceptScore W3104267550C135402231 @default.
- W3104267550 hasConceptScore W3104267550C140820882 @default.
- W3104267550 hasConceptScore W3104267550C196558001 @default.
- W3104267550 hasConceptScore W3104267550C25621703 @default.
- W3104267550 hasConceptScore W3104267550C2776401274 @default.
- W3104267550 hasConceptScore W3104267550C30475298 @default.
- W3104267550 hasConceptScore W3104267550C31532427 @default.
- W3104267550 hasConceptScore W3104267550C33923547 @default.
- W3104267550 hasConceptScore W3104267550C38349280 @default.
- W3104267550 hasConceptScore W3104267550C44870925 @default.
- W3104267550 hasConceptScore W3104267550C48372109 @default.
- W3104267550 hasConceptScore W3104267550C538625479 @default.
- W3104267550 hasConceptScore W3104267550C57879066 @default.
- W3104267550 hasConceptScore W3104267550C62520636 @default.
- W3104267550 hasConceptScore W3104267550C74650414 @default.
- W3104267550 hasConceptScore W3104267550C82706917 @default.
- W3104267550 hasConceptScore W3104267550C94375191 @default.
- W3104267550 hasConceptScore W3104267550C97355855 @default.
- W3104267550 hasIssue "12" @default.
- W3104267550 hasLocation W31042675501 @default.
- W3104267550 hasLocation W31042675502 @default.
- W3104267550 hasLocation W31042675503 @default.
- W3104267550 hasOpenAccess W3104267550 @default.
- W3104267550 hasPrimaryLocation W31042675501 @default.
- W3104267550 hasRelatedWork W1984668662 @default.
- W3104267550 hasRelatedWork W2017899146 @default.
- W3104267550 hasRelatedWork W2050942819 @default.
- W3104267550 hasRelatedWork W2160615342 @default.
- W3104267550 hasRelatedWork W2963621444 @default.
- W3104267550 hasRelatedWork W3104267550 @default.
- W3104267550 hasRelatedWork W3145073591 @default.