ソーラースピキュールとアルフェニック波の発生について
J Martínez-Sykora1,2, B De Pontieu2,3, V H Hansteen3,2
1Bay Area Environmental Research Institute, Petaluma, CA 94952, USA. juanms@lmsal.com.
まとめ
太陽の染色体内のジェットです イオン中性相互作用によって増幅される磁気圧が これらのジェットを駆動し コロナを熱し 波を生成します
科学分野:
- 太陽物理学
- プラズマ物理学
- マグネトヒドロダイナミック
背景:
- 太陽の染色体には スピキュールと呼ばれるジェットがあり プラズマを高速度でコロナに押し込みます
- 冠状熱と太陽風発電におけるスピキュルの起源と役割は,まだ十分に理解されていません.
研究 の 目的:
- 太陽のスパイクルを駆動する物理的メカニズムを調査する.
- スピキュール形成の理論モデルと観測データを接続する.
主な方法:
- マグネトヒドロダイナミック (MHD) シミュレーションと,インターフェース・リージョン・イマージング・スペクトログラフ (IRIS) とスウェーデン1m太陽望遠鏡 (SST) の観測データとの比較.
主要な成果:
- 磁気張力の増幅と上向きの輸送から発生します.
- この増幅はイオン中性相互作用または二極拡散によって起こる.
- 磁気圧の衝動的な放出は プラズマの流れを駆動し,プラズマを熱し,アルフェニック波を生成します.
結論:
- アンビポラー拡散と磁気張りは,スパイキュルの形成と進化の重要なメカニズムです.
- スピキュールは太陽の染色体からコロナにエネルギーとモメンタムを転送する上で重要な役割を果たします.
- この発見により,スピキュールの動態と,冠状熱と太陽風への貢献がより明確に理解できます.
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