冠状の活性領域の微妙な熱構造
Fabio Reale1, Susanna Parenti, Kathy K Reeves
1Dipartimento di Scienze Fisiche ed Astronomiche, Sezione di Astronomia, Università di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy. reale@astropa.unipa.it
まとめ
太陽のコロナを研究する.
科学分野:
- 太陽物理 太陽物理学
- プラズマ物理学のプラズマ物理学
- 天体物理学 天体物理学
背景:
- 太陽の冠状熱のメカニズムを理解することは極めて重要です.
- 太陽のコロナの熱構造は,重要な診断情報を提供する.
研究 の 目的:
- 太陽のコロナの微細な熱構造を決定する.
- 先進的なイメージング技術を使用して太陽光冠状熱機構を制限する.
主な方法:
- ヒノードX線望遠鏡を使って太陽のコロナを画像化しました.
- 温度診断のために複数のパスバンドとフィルターの組み合わせを使用した.
- 5つの異なるフィルターで撮影された画像のエネルギー比を分析した.
主要な成果:
- 活発な領域で熱的に高度に構造された太陽のコロナを明らかにした.
- 芯の非常に微細な熱構造と周辺のより大きな構造を観測した.
- 冠状回路と絡み合った構造に沿った連続的な熱分布が検出されました.
- 視線に沿った熱構造の変動を発見した.
結論:
- 観測された微細な熱構造は,冠状熱の理解に不可欠である.
- マルチフィルター画像は,太陽冠の複雑な熱特性についての詳細な洞察を提供します.
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