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Updated: Jul 12, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
まとめ
ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) とは,
科学分野:
- 惑星科学は惑星科学である.
- 大気科学 大気科学
- スペクトロスコーピーは,スペクトロスコーピーを用います.
背景:
- 金星の夜空の輝きは,主に酸化窒素の帯状で構成されています.
- 酸化窒素の帯は,窒素原子と酸素原子の再結合から生じる.
研究 の 目的:
- 金星の紫外線夜空光スペクトルを分析するために.
- トレーサーとしてエアグローを使用した昼から夜までの熱球循環を理解するために.
主な方法:
- 金星の紫外線夜空の光譜分析.
- 主要なスペクトル帯の識別とその起源.
主要な成果:
- 紫外線スペクトルは,酸化窒素のガンマとデルタ帯 (v' = 0) が支配しています.
- これらの帯は,昼側熱圏からの窒素原子と酸素原子の放射性再結合の結果である.
- エアグロウの強度は,赤道緯度や反太陽 meridian の朝側で最も高い.
結論:
- 金星の夜空の輝きは,熱球循環の重要な指標として機能します.
- 空気の輝きの分布は,金星の昼と夜の側面の間の大気動力学のパターンを明らかにします.
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