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土星の上層大気圏における予期せぬ冷却効果.

C G A Smith1, A D Aylward, G H Millward

  • 1Department of Physics and Astronomy, University College London, WC1E 6BT, UK.

Nature
|January 26, 2007
PubMed
まとめ

巨大惑星の大気はエネルギー危機に瀕しており,太陽熱だけでは温度が高すぎます. モデルでは,極性エネルギー投入が実際に低緯度地域を冷却することを示し,土星の大気加熱の唯一の解決策としてそれらを排除しています.

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