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Volumn 57, Issue 2, 2005, Pages 131-137

On the validity of Akasofu's e parameter and of the Vasyliunas et al. general formula for the rate of solar wind-magnetosphere energy input

Author keywords

coupling function; IMF clock angle; Substorm; varepsilon parameter; Vasyliunas et al. general formula

Indexed keywords

SOLAR WIND;

EID: 21844465703     PISSN: 13438832     EISSN: 18805981     Source Type: Journal    
DOI: 10.1186/BF03352557     Document Type: Article
Times cited : (5)

References (13)
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  • 2
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  • 4
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    • Statistical analyses in the study of solar wind-magnetosphere coupling
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    • Baker, D. N., Statistical analyses in the study of solar wind-magnetosphere coupling, in Solar Wind-Magnetosphere Coupling, edited by Y. Kamide and J. A. Slavin, pp.17-38, Terrapub/Reidel, Tokyo, 1986.
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    • Baker, D.N.1
  • 5
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    • Influence of the east-west component of the interplanetary magnetic field on the intensity of the auroral electrojet
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  • 7
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    • Magnetospheric energy budget and the epsilon parameter
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    • Koskinen, H.E.J.1    Tanskanen, E.I.2
  • 8
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    • Statistical study of the dependence of geomagnetic activity on solar wind parameters, in Quantitative Modeling of Magneto-spheric Processes
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    • Maezawa, K., Statistical study of the dependence of geomagnetic activity on solar wind parameters, in Quantitative Modeling of Magneto-spheric Processes, Geophys. Monogr. Ser., vol. 21, edited by W. P. Olson, pp.436-447, AGU, Washington, D.C., 1979.
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  • 9
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  • 10
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    • Empirical formula to relate the auroral electrojet intensity with interplanetary parameters
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.