関連する実験動画
Updated: Jul 12, 2026
07:00
Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite
Published on: March 11, 2020
木星の熱帯圏の気温の空間的組織と時間的依存性,1980年から1993年
Science (New York, N.Y.)
|July 29, 1994
まとめ
木星,木星,木星,木星,木星,木星,木星,木星,木星,木星,木星,木星,木星,木星,木星
科学分野:
- 惑星科学は惑星科学である.
- 大気物理学 大気物理学
- 木星研究 木星研究
背景:
- 木星の大気温は250ミリバールの圧力に近いので,木星の気候動態を理解する上で極めて重要です.
- 以前の研究では,気温と雲のパターンの間の相関が示されましたが,全面的な木星の1年間の分析は欠けていました.
研究 の 目的:
- 完全な木星年における木星の気温の空間的および時間的変動を調査するために.
- 温度パターンを季節的フォースと見える雲の構造と相関させるため.
- 木星の大気帯域内の特定の熱現象を特定するために.
主な方法:
- 木星の温度場をマッピングするために,18マイクロメートルの熱放出をイメージする.
- 1年の木星年にわたって収集された温度データを分析した.
- 温度データを可視雲のフィールド観測と相関させる.
主要な成果:
- 木星の温度場は,その可視雲場と密接に関連した帯状組織を示しています.
- 準周期的な気温振動が赤道地帯で検出されました.
- トロポスフィアの波とストラトスフィアの波は,北赤道帯で相関していることが判明しました.
- 北と南の赤道帯では,ゆっくりと移動する熱的特徴が観察されました.
結論:
- 季節的な放射能強制は木星の大気温に大きな影響を与えます.
- 赤道地帯と北赤道帯のような特定の地域は,ダイナミックな熱行動を示しています.
- 温度の変化は,木星の軸対称帯のアルベドの変化と一貫して相関しない.
関連する概念動画
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