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Alfven resonances, forced magnetic reconnection and model of solar flares

C Uberoi2003年Plasma Physics and Controlled FusionIF 2.2出版社

This paper briefly reviews the surface-wave-induced-magnetic reconnection (SWIMR) model based on the Alfven resonance theory near the neutral point. Extending this model to magnetosonic waves it is seen that it not only has features of formation of current sheets and plasmoids as in the incompressible case but in addition energy considerations show the triggering of solar flares by the catastrophic loss of equilibrium. The similarity of SWIMR model to the emerging flux and plasmoid induced magnetic reconnection model for solar flares is discussed.This article was scheduled to appear in issue 5 of Plasma Phys. Control. Fusion. To access this Special issue please follow this link: http://www.iop.org/EJ/toc/0741-3335/45/5

日本語訳

本論文は、中性点近傍におけるアルヴェン共鳴理論に基づく表面波誘起磁気リコネクション(SWIMR)モデルを簡潔に概説する。このモデルを磁気音波に拡張すると、非圧縮性の場合と同様に電流シートやプラズモイドの形成という特徴を示すだけでなく、エネルギー考察により、平衡状態の破壊的喪失による太陽フレアのトリガーが示される。SWIMRモデルと、太陽フレアに対する浮上磁束およびプラズモイド誘起磁気リコネクションモデルとの類似性について議論する。本論文は、Plasma Phys. Control. Fusionの第5号に掲載される予定であった。この特別号にアクセスするには、次のリンクを参照されたい:http://www.iop.org/EJ/toc/0741-3335/45/5

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Alfvén waveMagnetic reconnection
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