太陽光スペキュルの生成とその後の大気加熱
Tanmoy Samanta1, Hui Tian2, Vasyl Yurchyshyn3
1School of Earth and Space Sciences, Peking University, Beijing 100871, People's Republic of China.
まとめ
磁場相互作用により 太陽の表面から発する スピキュールと呼ばれる小さな太陽ジェットです これらの現象は 太陽の上層大気であるコロナの加熱と関連しています
科学分野:
- 太陽物理学
- プラズマ天体物理学
- マグネトヒドロダイナミック
背景:
- スピキュールは,太陽の染色体の中で観察された動的,微細なプラズマジェットです.
- スピキュルの起源と大気の加熱の役割はよくわかっていない.
- スピキュルの理解は 太陽の大気動態の理解に不可欠です
研究 の 目的:
- 太陽の粒子の起源を調査する
- 太陽の大気を暖める スピクルスの役割を決定する.
- 磁場ダイナミクスと スピキュール形成の関係を探る
主な方法:
- ビッグベア太陽観測所のグード太陽望遠鏡を用いた観測.
- 磁気流の発生とスパイキュールの分析
- 太陽ダイナミクス天文台データを用いて,スピキュールイベントと太陽のコロナ加熱を相関させる.
主要な成果:
- 反対の極性磁気流が現れた直後に 突起が現れた.
- 磁場相互作用,おそらく磁気再接続は,太陽の低い大気圏で観察されました.
- 太陽のコロナで発生した熱は,スピキュールの出現に伴い検出されました.
結論:
- 部分的にイオン化された太陽の大気中の磁場ダイナミクスは スピクルスを生み出します
- スピキュール生成は太陽のコロナの加熱に関連しています.
- この研究は,太陽の大気加熱を駆動するメカニズムの洞察を提供します.
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