The roles of direct input of energy from the solar wind and unloading of stored magnetotail energy in driving magnetospheric substorms

Space Science Reviews

Volumn 46, Issue 1-2, 1988, Pages 93-111

  Rostoker, G ^a   Akasofu, S I ^b   Baumjohann, W ^c   Kamide, Y ^d,e   McPherron, R L ^f  

^a UNIVERSITY OF ALBERTA   (Canada)

^b UNIVERSITY OF ALASKA FAIRBANKS   (United States)

^c UNIVERSITY OF MÜNSTER   (Germany)

^d KYOTO SANGYO UNIVERSITY   (Japan)

^e NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 34250092806     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/BF00173876     Document Type: Article

References (33)

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9. A comprehensive model current system for high-latitude magnetic activity - I. The steady state system
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11. Dependence of substorm occurrence probability on the interplanetary magnetic field and on the size of the auroral oval
12. The expansive phase of magnetospheric substorms: 1. Development of the auroral electrojets and auroral arc configuration during a substorm
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19. Response of dayside net downward field-aligned current to changes in the interplanetary magnetic field and to substorm perturbations
20. Equatorial current sheet in the magnetosphere