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Current loop coalescence studied by 3-D electromagnetic particle codeSolar flare plasma data from the Yohkoh satellite is analyzed. The interactions of current loops were observed in the active regions on the Sun. This observation pointed out the importance of the idea that the solar flare is generated by the coalescence of current loops. The three dimensional electromagnetic particle simulations are to help in understanding the global interaction between two current loops including the evolution of the twist of loops due to instabilities. Associated rapid dynamics of current loop coalescence such as reconnection, shock waves and associated kinetic processes such as energy transfer, acceleration of particles, and electromagnetic emissions are to be studied by the code to complement analytical theories and magnetohydrodynamic simulations of the current loop coalescence. The simulation results show the strong interactions between two current loops, beam and whistler instabilities, and associated parallel and perpendicular particle heating.
Document ID
19940018187
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Nishikawa, Ken-Ichi
(Iowa Univ. Iowa City, IA, United States)
Sakai, Jun-Ichi
(Toyama Univ. Japan)
Koide, Shinji
(Toyama Univ. Japan)
Buneman, O.
(Stanford Univ. CA., United States)
Neubert, T.
(Michigan Univ. Ann Arbor., United States)
Date Acquired
September 6, 2013
Publication Date
May 1, 1993
Publication Information
Publication: ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion
Subject Category
Solar Physics
Accession Number
94N22660
Funding Number(s)
CONTRACT_GRANT: NSF ATM-91-21116
CONTRACT_GRANT: NAGW-2350
CONTRACT_GRANT: ASR-ME-03640247
CONTRACT_GRANT: NSF ATM-91-06639
CONTRACT_GRANT: NAS8-38772
Distribution Limits
Public
Copyright
Other
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