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金星の大気圏の夜間雲の循環
Kiichi Fukuya1, Takeshi Imamura2, Makoto Taguchi3
1Department of Earth and Planetary Science, The University of Tokyo, Tokyo, Japan.
Nature
|July 22, 2021
まとめ
ヴィーナス
科学分野:
- 惑星科学
- 大気科学
- 航空学
背景:
- 金星の大気循環は 特に夜側では 十分に理解されていません
- 以前の研究では,すべての局所時間帯にわたる包括的な風力データはありませんでした.
- 金星の大気動態を理解することは 地球上の惑星の進化を理解する鍵です
研究 の 目的:
- 熱潮とハドリー循環を含む 金星の大気循環を特徴づけるため
- 金星の大気の超回転の 原因を調査するために
- 金星の雲の頂点を 総合的な風データセットにします
主な方法:
- 熱赤外線画像を利用した アカツキの金星軌道探査機
- 約65kmの高度で風速を測定する雲追跡技術を採用した.
- 夜間も含めて データを集めました
主要な成果:
- 恒星の夜側で赤道に向かって 流れているのが観測された.
- ハドリー循環の影響なしに熱潮の速度構造を決定した.
- 半日間の潮の振幅が 大気の超回転を維持するのに 十分だと分かった
結論:
- ハドリー循環の極端の分岐は 雲の頂上にあり 赤道への分岐は 雲の中にあります
- 熱潮は金星の大気の超回転を維持する上で重要な役割を果たします
- これらの発見は,他の天体における大気の超回転についての洞察を提供します.
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