1970年3月7日の日食からのロケットUVフラッシュスペクトル
R J Speer1, W R Garton, J F Morgan
1Imperial College of Science and Technology, London.
Nature
|April 18, 1970
まとめ
完全日食の際に初めて,極紫外線閃光スペクトルが捉えられた. この画期的な成果は,太陽のダイナミックな外側の大気に関する新しい洞察を提供します.
科学分野:
- 太陽物理 太陽物理学
- 天文学 天文学
- 天体物理学 天体物理学
背景:
- 完全日食は,太陽のコロナを研究するためのユニークな機会を提供します.
- 極紫外線 (EUV) の観測は,太陽の大気動態を理解するために極めて重要です.
研究 の 目的:
- 完全日食のすべての相の間に極紫外線フラッシュスペクトルを取得し,分析する.
- 日食中に太陽のコロナとクロモスフィアのスペクトル特性を調査する.
主な方法:
- 特殊な器具を用いて,極紫外線の高解像度スペクトルを撮影する.
- すべての相をカバーするために,日食の全体期間中に調整された観測.
主要な成果:
- 完全日食の間,極紫外線で前例のないフラッシュスペクトルを成功裏に取得しました.
- 分析は,日食の異なる相に対応する明確なスペクトル特徴を明らかにした.
結論:
- この研究は,完全な日食の間にEUVフラッシュスペクトルの取得を初めて示しています.
- 得られたデータは,太陽の大気プロセスと進化の理解を大幅に前進させるでしょう.
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