@article{oai:toyama.repo.nii.ac.jp:00004394,
 author = {坂井, 純一 and 大沢, 幸治},
 journal = {富山大学工学部紀要},
 month = {Mar},
 note = {This article reviews recent development of the theory of current loop coalescence and fast magnetosonic shock waves, giving particular attention to particle acceleration caused by these processes.
It is shown that the spiral, two sided plasma jets can be explosively driven by the plasma rotational motion induced by magnetic reconnection during the two current loop coalescence. The rebound following the plasma pinch driven by the Lorentz force can generate the fast magnetosonic shock waves.
For a weak magnetic field (ω_<ce>≪ω_<pe>), strong acceleration by the shocks occurs to proton only.
While the simultaneous acceleration of protons and electrons takes place in a rather strong magnetic field such that ω_<ce>≿ω_<pe>. Resonant protons gain relativistic energies within the order of the ion cyclotron period (much less than 1s for solar plasma parameters). The electron acceleration time is shorter than the ion cyclotron period., Article, 富山大学工学部紀要，40},
 pages = {91--102},
 title = {PARTICLE ACCELERATION BY MAGNETIC RECONNECTION AND FAST MAGNETOSONIC SHOCK WAVES IN SOLAR FLARES},
 volume = {40},
 year = {1989}
}