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Volumn 102, Issue A6, 1997, Pages 11263-11272

Latitudinal solar wind velocity variations from polar coronal holes: A self-consistent MHD model

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[No Author keywords available]

Indexed keywords


EID: 37149025688     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/96JA02873     Document Type: Article
Times cited : (17)

References (11)
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  • 2
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  • 3
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  • 4
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    • The large angle spectroscopic coronagraph (LASCO) experiment on SOHO. Instrument description and early results
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  • 5
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    • Towards a consistent treatment of thermally conductive magnetohydrodynamic flows in helmet-streamer coronal structures
    • Cupermann, S., T. R. Detman, C. Bruma, and M. Dryer, Towards a consistent treatment of thermally conductive magnetohydrodynamic flows in helmet-streamer coronal structures, Astron. Astrophys., , 265, 785, 1992
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  • 6
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    • The magnetohydrodynamic equilibrium of coronal helmet streamers
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    • Cupermann, S.1    Bruma, C.2    Dryer, M.3    Semel, M.4
  • 7
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  • 8
    • 0006382955 scopus 로고
    • Coronal heating and plasma parameters at 1 AU
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  • 10
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    • Solar wind mass and momentum flux variations at 0.3 AU
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.