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Updated: Jul 12, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
まとめ
以前,マイクロ波干渉測定によって示唆された金星の極地における実質的な冷却は,疑わしい. その他のマイクロ波データは,金星全体で最小の温度変動を示している.
科学分野:
- 惑星科学は惑星科学である.
- ラジオ天文学 ラジオ天文学
- 金星科学 金星科学
背景:
- 以前のマイクロ波干渉計は,金星の極地が著しく冷却されていることを示唆していた.
- 金星の大気温分布を理解することは,気候モデリングに不可欠です.
研究 の 目的:
- 金星の極地冷却の証拠を再評価する.
- 金星の温度に関する既存のマイクロ波測定の信頼性を評価する.
主な方法:
- 波長10.6cmのマイクロ波インターフェロメトリーデータの分析.
- 金星の熱プロファイルの他の利用可能なマイクロ波測定値との比較.
主要な成果:
- マイクロ波インターフェロメトリーデータの解釈は,実質的な極地冷却を示唆していることに異議を唱える.
- 他のマイクロ波観測では,極の方向に有意な温度梯度を示す証拠はほとんどない.
結論:
- 金星の極地での有意な冷却の存在は不確実である.
- 現存するマイクロ波データは,金星の赤道と極の間の大きな温度差を強く支持していない.
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