高解像度の中赤外線画像からの土星の温度場
G S Orton1, P A Yanamandra-Fisher
1Jet Propulsion Laboratory, MS 169-237, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
まとめ
土星 サターン
科学分野:
- 惑星科学 惑星科学
- 天文学 天文学
- 大気物理学 大気物理学
背景:
- 土星の大気動力学と熱的構造は,ガスの巨大惑星を理解するための鍵です.
- 以前の観測では,土星の熱的特徴の解像度が限られていた.
研究 の 目的:
- 土星の大気の熱構造を赤外線画像を用いて調査する.
- 大気温と見える雲の特徴を相関させるため.
主な方法:
- ケックI望遠鏡を用いた土星の赤外線画像.
- 8~24.5ミクロメートルの間の熱放出の分析.
- 約3000キロメートルの解像度.
主要な成果:
- 土星の大気圏で明確なゾーン温度帯を観測した.
- 温度帯と可視雲の反射性との間の相関は最小値であった.
- 南緯32度近くで100ミリバールの強いゾーン温度振動が検出されました.
- 暖かい南極点と南極点近くのコンパクトなホットスポットを特定しました.
結論:
- 土星の大気気温分布は複雑で,目に見える雲のパターンにのみ左右されるものではない.
- 南極のような特定の地域は,さらなる調査を必要とするユニークな熱特性を示しています.
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