太陽の全角磁場の8ヶ月の進化を観察する
Zihao Yang1,2, Hui Tian1,3, Steven Tomczyk2,4
1School of Earth and Space Sciences, Peking University, Beijing 100871, People's Republic of China.
まとめ
太陽の8ヶ月の磁場進化を明らかにした. これらの観測は 太陽の磁場動力学と エネルギー貯蔵に関する 前例のない洞察をもたらします
科学分野:
- 太陽物理学
- マグネトヒドロダイナミック
- プラズマ物理学
背景:
- 太陽のコロナは磁場にエネルギーを蓄え 太陽の噴火とプラズマの加熱を促します
- 以前の世界的な冠状磁場測定は,まれなスナップショットに限定されていました.
研究 の 目的:
- 地球の冠状磁場を継続的に長期にわたって観測する
- 高度による磁場分布を決定し,時間と緯度による磁場の進化を監視する.
主な方法:
- 強化された冠状多チャンネル極光計 (UCOMP) を利用して114の磁気図を記録した.
- 約8ヶ月間,太陽の上の地球上のコロナを観測した.
- 磁場強度と分布を様々な高度と緯度で分析した.
主要な成果:
- 測定された冠状磁場強度は,太陽半径1.05〜1.60の1〜20ガウスである.
- 異なる緯度における磁場の進化を観測した.
- コロナ磁場測定で 活動的な長さのサインを検出した
結論:
- この研究は,冠状磁場動態を理解するための包括的なデータセットを提供します.
- 冠状のモデルは一般的に観測値と一致し,高緯度地域では不一致が認められる.
- この発見は 太陽のコロナにおける エネルギー貯蔵と放出の仕組みの理解を 強化するものです
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