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Volumn 26, Issue 11, 2000, Pages 743-749

An axisymmetric magnetohydrodynamic model for the interaction of the solar wind with the local interstellar medium

Author keywords

Heliopause; Heliosphere; Hydrogen atoms; Interstellar magnetic field; Interstellar medium; Shock waves; Solar system; Solar wind

Indexed keywords


EID: 0034346009     PISSN: 10637737     EISSN: None     Source Type: Journal    
DOI: 10.1134/1.1323281     Document Type: Article
Times cited : (43)

References (29)
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  • 13
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    • Preprint No. 585, IPM RAN Institute for Problems of Mechanics, Russian Academy of Sciences
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    • Preprint No. 584, IPM RAN Institute for Problems of Mechanics, Russian Academy of Sciences
    • A. V. Myasnikov and E. V. Barsky, Preprint No. 584, IPM RAN (Institute for Problems of Mechanics, Russian Academy of Sciences, 1997).
    • (1997)
    • Myasnikov, A.V.1    Barsky, E.V.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.