Flux-rope-mediated Turbulent Magnetic Reconnection
We present a new model of magnetic reconnection in the presence of turbulence. The new model differs from the Lazarian–Vishniac turbulent reconnection theory by emphasizing the role of locally coherent magnetic structures, whose existence is shown to be permitted by the properties of magnetic field...
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フォーマット: | 論文 |
言語: | English |
出版事項: |
IOP Publishing
2025-01-01
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シリーズ: | The Astrophysical Journal |
主題: | |
オンライン・アクセス: | https://doi.org/10.3847/1538-4357/adac61 |