Plasma jet and shock formation during current loop coalescence in solar flares

Solar Physics ◽  
1989 ◽  
Vol 120 (1) ◽  
pp. 117-124 ◽  
Author(s):  
Jun-Ichi Sakai
Keyword(s):  
Solar Flares ◽  
Plasma Jet ◽  
Current Loop ◽  
Shock Formation

Current Loop Coalescence Model of Solar Flares: Erratum

1988 ◽  
Vol 329 ◽  
pp. 517
Author(s):  
T. Tajima ◽  
J. Sakai ◽  
H. Nakajima ◽  
T. Kosugi ◽  
F. Brunel ◽  
...  
Keyword(s):  
Solar Flares ◽  
Current Loop ◽  
Coalescence Model

Formation of fast magnetosonic shock waves during a two-current-loop collision in solar flares

Solar Physics ◽  
1994 ◽  
Vol 151 (1) ◽  
pp. 137-145 ◽  
Author(s):  
Shinji Koide ◽  
Jun-Ichi Sakai
Keyword(s):  
Shock Waves ◽  
Solar Flares ◽  
Current Loop

Coronal explosions as a signature of current loop coalescence in solar flares

Solar Physics ◽  
1989 ◽  
Vol 123 (2) ◽  
pp. 393-396 ◽  
Author(s):  
Jun-Ichi Sakai ◽  
Cornelis de Jager
Keyword(s):  
Solar Flares ◽  
Current Loop

scholarly journals 3D Simulation of Externally Driven Reconnection

1985 ◽  
Vol 107 ◽  
pp. 211-215
Author(s):  
T. Sato
Keyword(s):  
Mach Number ◽  
Plasma Jet ◽  
3D Simulation ◽  
Shock Formation ◽  
Neutral Sheet ◽  
Slow Shock ◽  
New Findings ◽  
Sheet Current ◽  
Magnetohydrodynamic Simulation ◽  
2D Model

A 3D magnetohydrodynamic simulation is presented. The essential conclusions obtained by the previous 2D model, such as the slow shock formation and the strong plasma jet generation, are reconfirmed. In addition, several new findings pertinent to three dimensionality are obtained. Among them, particularly interesting and important is the generation of field aligned currents at the slow shock associated with a local interruption of the neutral sheet current. It is also interesting to observe the generation of super–magnetosonic flows with the Mach number of 2.

Current loop coalescence model of solar flares

1987 ◽  
Vol 321 ◽  
pp. 1031 ◽  
Author(s):  
T. Tajima ◽  
J. Sakai ◽  
H. Nakajima ◽  
T. Kosugi ◽  
F. Brunel ◽  
...  
Keyword(s):  
Solar Flares ◽  
Current Loop ◽  
Coalescence Model
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