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Energy dissipation in substormsThe energy dissipated by substorms manifested in several ways is discussed: the Joule dissipation in the ionosphere; the energization of the ring current by the injection of plasma sheet particles; auroral election and ion acceleration; plasmoid ejection; and plasma sheet ion heating during the recovery phase. For each of these energy dissipation mechanisms, a 'rule of thumb' formula is given, and a typical dissipation rate and total energy expenditure is estimated. The total energy dissipated as Joule heat (approximately) 2 x 10(exp 15) is found about twice the ring current injection term, and may be even larger if small scale effects are included. The energy expended in auroral electron precipitation, on the other hand, is smaller than the Joule heating by a factor of five. The energy expended in refilling and heating the plasma sheets is estimated to be approximately 5 x 10(exp 14)J, while the energy lost due to plasmoid ejection is between (approximately) (10 exp 13)(exp 14)J.
Document ID
19950011849
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Weiss, Loretta A.
(Rice Univ. Houston, TX, United States)
Reiff, P. H.
(Rice Univ. Houston, TX, United States)
Moses, J. J.
(Rice Univ. Houston, TX, United States)
Heelis, R. A.
(Texas Univ. Dallas, TX., United States)
Moore, B. D.
(Rice Univ. Houston, TX, United States)
Date Acquired
August 16, 2013
Publication Date
June 1, 1992
Publication Information
Publication: ESA, Substorms 1
Subject Category
Geophysics
Accession Number
95N18264
Funding Number(s)
CONTRACT_GRANT: NAG5-305
CONTRACT_GRANT: NAGW-1655
CONTRACT_GRANT: NAG5-775
CONTRACT_GRANT: NSF ATM-90-22662
Distribution Limits
Public
Copyright
Other
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