抄録
Rapid magnetic reconnection was experimentally observed to occur within a microsecond timescale, leading to the field-reversed configuration (FRC) comprising a single closed magnetic field structure. The compressibility of the plasma within the FRC played a crucial role in accelerating the coalescence process, making it considerably faster than the resistive process. A strong similarity between the observed experimental results and those of the coalescence of solar flare loops indicates that astrophysical phenomena and laboratory plasmas are governed by a common physics.
本文言語 | 英語 |
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論文番号 | 0177975 |
ジャーナル | Physics of Plasmas |
巻 | 31 |
号 | 1 |
DOI | |
出版ステータス | 出版済み - 1月 2024 |