太陽風による太陽フレアの加速:活性領域の磁場の影響
まとめ
太陽フレアの磁場方向は太陽風を予測する. 南向きの磁場は,地球に到達する高速太陽風のプラズマを加速させ,重大な影響を及ぼします. 北向きのフィールドは,めったにこの効果を生成しません.
科学分野:
- 太陽物理 太陽物理学
- 宇宙天気は宇宙天候である.
背景:
- 太陽フレア現象における光球磁場の役割は極めて重要です.
- 太陽風の加速メカニズムを理解することは,宇宙天候の予測の鍵です.
研究 の 目的:
- 太陽フレア地点の光球磁場方向が太陽風のプラズマ加速を予測するかどうかを判断する.
- 異なる太陽フレア磁場方向の潜在的な地上の影響を評価する.
主な方法:
- 太陽フレアに関する観測分析.
- フォトスフィアの磁場方向と,地球近くの太陽風の観測による相関に関する研究.
主要な成果:
- フレア地点にある光球磁場の南向きの成分は,地球近くの高速太陽風のプラズマの後の観測と強く相関しています.
- 磁場の北側のコンポーネントは,このような高速な太陽風の観測をめったにもたらさない.
- 南向きの磁場を持つフレアは,北向きの磁場を持つフレアと比較して,著しく大きな地上の効果と関連しています.
結論:
- 太陽フレア中の光球磁場の方向は,高速太陽風発電の信頼できる予測指標です.
- 太陽フレアの南向きの磁場は,宇宙天候に影響を与え,地球上の影響を及ぼす可能性が高い.
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