Energy Partition of Thermal and Nonthermal Particles in Magnetic Reconnection

被引:5
|
作者
Hoshino, Masahiro [1 ]
机构
[1] Univ Tokyo, Dept Earth & Planetary Sci, Tokyo 1130033, Japan
来源
ASTROPHYSICAL JOURNAL | 2023年 / 946卷 / 02期
关键词
ELECTRON ACCELERATION; RELATIVISTIC RECONNECTION; SIMULATIONS; VARIABILITY; SPECTRA; MODEL; FIELD; ION;
D O I
10.3847/1538-4357/acbfb5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Magnetic reconnection has long been known to be the most important mechanism for quick conversion of magnetic field energy into plasma kinetic energy. In addition, energy dissipation by reconnection has gained attention not only as a plasma heating mechanism, but also as a plasma mechanism for accelerating nonthermal particles. However, the energy partitioning of thermal and nonthermal plasmas during magnetic reconnection is not understood. Here, we studied energy partition as a function of plasma sheet temperature and guide magnetic field. In relativistic reconnection with an antiparallel magnetic field or a weak guide magnetic field, it was found that the nonthermal energy density can occupy more than 90% of the total kinetic plasma energy density, but strengthening the guide magnetic field suppresses the efficiency of the nonthermal particle acceleration. In nonrelativistic reconnection for an antiparallel magnetic field, most dissipated magnetic field energy is converted into thermal plasma heating. For a weak guide magnetic field with a moderate value, however, the nonthermal particle acceleration efficiency was enhanced, but strengthening the guide field beyond the moderate value suppresses the efficiency.
引用
收藏
页数:9
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