@article{oai:toyama.repo.nii.ac.jp:00004397,
 author = {坂井, 純一},
 journal = {富山大学工学部紀要},
 month = {Mar},
 note = {We report on the results of plasma jet and shock formation during the current loop coalescence in solar flares. It is shown by a theoretical model based on the ideal MHD Equation that the spiral, two-sided plasma jet can be explosively driven by the plasma rotatinal motion induced during the two current loop coalescence process. The maximum velocity of the jet can exceed tte Alfven velocity, depending on the plasma β( = C_s^2/V_A^2) ratio. The acceleration time getting to the maximum jet velocity is quite short and less than 1 second. The rebound following the plasma collapse driven by magnetic pinch effect can strongly induce super-Alfvenic flow.
We present the condition of the fast magnetosonic shock formation. We briefly discuss the high energy particle acceleration during the plasma collapse as well as by the fast magnetosonic shocks., Article, 富山大学工学部紀要，40},
 pages = {127--133},
 title = {Plasma Jet and Shock Formation during Current Loop Coalescence in Solar Flares},
 volume = {40},
 year = {1989}
}