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Volumn 17, Issue 3, 1996, Pages 61-64

The global solar magnetic field as a "controller" for the origin and acceleration model of solar wind streams

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EID: 0042877726     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00499-5     Document Type: Article
Times cited : (3)

References (10)
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  • 3
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  • 4
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    • Yu.V. Pisanko, 3-D subalfvenic transonic solar wind on the flow formation region: results of numerical MHD simulations, in: Solar Terrestrial Energy Program, ed. D.N. Baker, V.O. Papitashvili, M.J. Teaguc, COSPAR Colloquia Series v.5, Pergamon Press 1994, p.791
    • (1994) COSPAR Colloquia Series , vol.5 , pp. 791
    • Pisanko, Yu.V.1
  • 5
    • 0006812976 scopus 로고
    • Observations of the solar wind near the Sun from microwave IPS phenomena
    • Solar Wind Seven, ed. E. Marsch, R. Schwenn, Pergamon Press
    • M. Tokumara, H. Mori, T. Tanaka, T. Kondo, H. Takaba and Y. Koyama, Observations of the solar wind near the Sun from microwave IPS phenomena, in: Solar Wind Seven, ed. E. Marsch, R. Schwenn, COSPAR Colloquia Series v.3, Pergamon Press 1992, p.289
    • (1992) COSPAR Colloquia Series , vol.3 , pp. 289
    • Tokumara, M.1    Mori, H.2    Tanaka, T.3    Kondo, T.4    Takaba, H.5    Koyama, Y.6
  • 6
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    • (1992) COSPAR Colloquia Series , vol.3 , pp. 319
    • Woo, R.1    Armstrong, J.W.2
  • 7
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    • Radio astronomical observations connected with the solar wind problem
    • "Mir", Moscow
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    • Wyndham, J.D.1
  • 8
    • 0042360545 scopus 로고
    • About the radial character of the coronal rays
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  • 9
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    • R. Schwenn, K.H. Muhlhauser, E. Marsch and H. Rosenbauer, Two states of the solar wind at the time of solar activity minimum. 2. Radial gradients of plasma parameters in fast and slow streams, in: Solar Wind Four, ed. H. Rosenbauer, Report No MPAE-W-100-81-31, Max-Planck-Institute fur Acronomie, Katlenburg-Lindau and Max-Planck-Institute fur extraterrestrische Physik, Garching, Germany 1981, p. 126
    • (1981) Solar Wind Four , pp. 126
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  • 10
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    • Comparison of solar wind velocity measurements with a theoretical acceleration model
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.