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Volumn 102, Issue A7, 1997, Pages 14661-14676

A fast solar wind model with anisotropic proton temperature

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Indexed keywords


EID: 37148999069     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/97JA01040     Document Type: Article
Times cited : (84)

References (11)
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    • Cuperman, S.1    Detman, T.2    Dryer, M.3
  • 4
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    • Dere, K. P., Explosive events, magnetic reconnection, and coronal heating, Adv. Space Res., 14(4), 13, 1994.
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    • Dere, K.P.1
  • 6
    • 37149050259 scopus 로고    scopus 로고
    • Hot proton temperatures in the inner corona and their effect on flow properties in the solar wind
    • Esser, R., S. R. Habbal, W. A. Coles, and J. V. Hollweg, Hot proton temperatures in the inner corona and their effect on flow properties in the solar wind, J. Geophys. Res., 102, 7063, 1997.
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  • 8
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  • 9
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    • The damping of interplanetary Alfvénic fluctuations and the heating of the solar wind
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    • Tu, C.-Y.1
  • 10
    • 0041948670 scopus 로고
    • The radial evolution of the IMF fluctuations: A comparison with theoretical models
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    • Villante, U.1    Vellante, M.2
  • 11
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    • The temperature structure, mass and energy flow in the corona and inner solar wind
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    • Withbroe, G.L.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.