関連する実験動画
Updated: Jul 12, 2026

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Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite
Published on: March 11, 2020
ピオニア軌道探査機の赤外線遠隔感知による金星の中部大気の温度,雲の構造,動態
まとめ
新金星の発見は,回転するホットスポットと冷たい雲を囲む高緯度"二極"構造を明らかにしています. この研究は,金星の大気の特徴を明らかにしています.
科学分野:
- 惑星科学は惑星科学である.
- 大気科学 大気科学
- 金星科学 金星科学
背景:
- 金星の大気は,複雑な熱的,動的構造を示しています.
- 上層大気 (60~130km) を理解することは,大気モデルにとって極めて重要です.
研究 の 目的:
- 3D温度場,雲の構造,そして金星の上層大気の動態を特徴づけるために.
- 金星軌道探査機"パイオニア"軌道探査機の放射性温度実験 (VORTEX) の新発見を紹介する.
主な方法:
- ヴィーナス軌道探査機"パイオニア"からの放射測定温度データの分析.
- 気温と雲のデータを用いて大気現象の特徴化.
主要な成果:
- 小説の識別.
- 二極二極は二極二極である.
- 金星の高緯度にある構造物である.
- 極の周りを回転する2つの明確なホットスポットの観測.
- 二極構造に関連する寒い雲の周囲の岸の検出.
結論:
- 観測された二極構造は,金星の大気動力学に関する新しい洞察を提供します.
- これらの発見は,金星の上層大気中の気温変動と雲の形成に関する私たちの理解を深めています.
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