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Updated: Jul 11, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Published on: November 15, 2013

中央の雲層にある金星の大気の熱構造

V M Linkin, V V Kerzhanovich, A N Lipatov

    Science (New York, N.Y.)
    |March 21, 1986
    PubMed
    まとめ

    VEGAの気球は,金星の中間雲層は主にアディアバティックであることを明らかにした. 2つの気球とパイオニア・ヴェーナスのデータとの間の気温の変動は,大気の複雑さを強調しています.

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