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Updated: Jul 12, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
まとめ
ヴィーナス・ネフェロメーター実験のパイオニアは,バックスキャッタリングデータと周囲の放射線測定を明らかにした. 観測結果は,高さに伴い放射力が低下し,下層大気圏では745nmよりも530nmでより速く減少していることを示しています.
科学分野:
- 惑星科学は惑星科学である.
- 大気科学 大気科学
- 放射能の移転について
背景:
- ピオニア・ベーナスミッションは,探査機を使って,金星の大気に関するインシトゥデータを収集した.
- ネフェロメトリーは,大気中の粒子の性質と光の散乱を理解するために不可欠です.
研究 の 目的:
- パイオニア・ベーナス・ネフェロメーターの実験からの包括的なバックスキャッタリングデータを提示する.
- 周囲の放射線を分析し,大気の絶滅特性を推測する.
主な方法:
- ネフェロメーター実験は,パイオニア・ベーナス探査機で実施されています.
- 近紫外線および可視波長の環境放射線の測定.
- 背散信号と高さによる放射能変動の分析.
主要な成果:
- 探査機が到達した最高高度まで収集されたバックスキャッティングデータ.
- メインクラウドデッキの下の小さな信号の検出.
- 高度による紫外線付近の絶滅の推論された変動.
- 周囲の放射線は,下層大気圏の745nmと比較して530nmでより急速に減少しました.
結論:
- この研究は,金星の有価な大気データを提供します.
- 放射能と絶滅の変動を理解することは,大気モデリングの鍵です.
- この発見は,金星の大気組成と光学特性の特徴づけに寄与する.
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06:27Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer
Published on: May 29, 2019
09:00Indoor Experimental Assessment of the Efficiency and Irradiance Spot of the Achromatic Doublet on Glass (ADG) Fresnel Lens for Concentrating Photovoltaics
Published on: October 27, 2017
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