Characteristic features in Venus’ nightside cloud-top temperature obtained by Akatsuki/LIR

書誌事項

公開日
2012-05
資源種別
journal article
権利情報
  • https://www.elsevier.com/tdm/userlicense/1.0/
DOI
  • 10.1016/j.icarus.2012.01.024
公開者
Elsevier BV

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説明

Abstract Mid-infrared images of almost the entire Venus nightside hemisphere obtained by the Longwave Infrared Camera (LIR) onboard Akatsuki on December 9 and 10, 2010 reveal that the brightness temperature of the cloud-top ranges from 237 K in the cold polar collars to 243 K in the equatorial region, significantly higher than the values obtained by Venera 15. Other characteristic features of the temperature distributions observed are zonal belt structures seen in the middle and low latitudes and patchy temperature structures or quasi-periodic streaks extending in a north–south direction in the northern middle latitudes and southern low latitudes.

収録刊行物

  • Icarus

    Icarus 219 (1), 502-504, 2012-05

    Elsevier BV

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