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Volumn 439, Issue 3, 2005, Pages 1171-1181

Kinetic vs. multi-fluid models of H atoms in the heliospheric interface: A comparison

Author keywords

Interplanetary medium; ISM: atoms; Sun: solar wind

Indexed keywords

ASTROPHYSICS; FLUIDICS; KINETIC THEORY; WIND EFFECTS;

EID: 24944458991     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20052821     Document Type: Article
Times cited : (76)

References (64)
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    • Fahr, H.J.1
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    • Izmodenov, V. V. 2003, Proc. of the Interstellar enviroment of the heliosphere, COSPAR Colloquium in Honour of Stanislaw Grzedzielski, ed. D. Breitschwerdt, & G. Haerendel, MPE Report, 285, 113
    • (2003) MPE Report , vol.285 , pp. 113
    • Izmodenov, V.V.1
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    • Myasnikov, A. V., Belov, N. A., & Zhekov, S. A. 1997, Preprint 582 of Institute for Problems in Mechanics RAS
    • Myasnikov, A. V., Belov, N. A., & Zhekov, S. A. 1997, Preprint 582 of Institute for Problems in Mechanics RAS
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    • Witte, M. 2004, A&A, 426, 835
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    • Witte, M.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.