マリナー9号の紫外線スペクトロメーター実験:火星のオゾン層の季節的変動
まとめ
火星の極地の大気中のオゾンは季節によって変化し,冬にはピークに達し,夏には消失します. この大気中のガスは,赤道地域では一年中存在しません.
科学分野:
- 惑星科学 惑星科学
- 大気化学 大気化学
背景:
- オゾンは惑星の大気の重要な構成要素です.
- 火星の大気動態を理解することは,将来の探査に不可欠です.
研究 の 目的:
- 火星の極地大気中のオゾンの季節的変動と分布を調査する.
- 極地フードのような火星の大気現象とオゾン存在を相関させるため.
主な方法:
- 火星の極地におけるオゾン濃度に関する観測データを分析した.
- 季節の傾向と地理的分布は,火星の季節にわたって記録された.
主要な成果:
- オゾンは,火星の極域で季節的な変動が顕著である.
- オゾンレベルは夏に最低 (<3マイクロメートル大気) で,冬に最高 (57マイクロメートル大気まで).
- オゾンは,秋の極地殻形成と関連しており,夏には消失し,赤道地域には存在しません.
結論:
- 火星の極地オゾンレベルは季節的に強く,大気現象と関連しています.
- 赤道地域のオゾンがないことは,特定の大気循環パターンを示唆しています.
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