木星の5ミクロンのホットスポットの非線形シミュレーション
1National Research Council (NRC)/NASA Ames Research Center, Mail Stop 245-3, Moffett Field, CA 94035-1000, USA. showman@humbabe.arc.nasa.gov
まとめ
シミュレーションにより,木星の5ミクロンのホットスポットは,沈没につながる長寿構造によって引き起こされていることが明らかになりました. これらの構造は,観測された乾燥と低い曇りの説明であり,ガリレオ探査機のデータと一致しています.
科学分野:
- 惑星科学は惑星科学である.
- 流体力学 流体力学とは
- 大気物理学 大気物理学
背景:
- 木星の5ミクロンのホットスポットは,低い曇りと乾燥が特徴です.
- 以前のモデルは,これらの特徴の形成と動態を完全に説明できませんでした.
研究 の 目的:
- 大規模な非線形シミュレーションを使用して木星の5ミクロンのホットスポットをシミュレートする.
- 乾燥度,低曇度を含むホットスポットの観測された特徴を説明するために.
主な方法:
- 木星の大気の大規模な非線形シミュレーション.
- シミュレートされたコヒーレント構造とその動的性質の分析.
主要な成果:
- シミュレーションにより,地域の沈殿に起因する,長寿命の一貫した構造が生成されました.
- これらの構造は,観測されたホットスポットに匹敵する特徴を示しています:赤道上の閉じ込め,周期的な間隔,西への伝播,半球的な閉じ込め,および反サイクロン回転.
- シミュレートされたホットスポットの南端で,最大70m/sの縦断風が観測されました.
結論:
- シミュレートされたコヒーレント構造は,木星の5ミクロンのホットスポットについて実行可能な説明を提供します.
- この発見は,ガリレオ探査機による測定結果と一致し,乾燥度,低雲度,ドップラー風実験結果などを説明している.
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