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D. Grassi, R. Politi, N. I. Ignatiev, C. Plainaki, S. Lebonnois, P. Wolkenberg, L. Montabone, A. Migliorini, G. Piccioni and P. Drossart The Venus nighttime atmosphere as observed by the VIRTIS-M instrument. Average fields from the complete infrared data set Journal of Geophysical Research: Planets 119

Article first published online: 17 APR 2014 | DOI: 10.1002/2013JE004586

Key Points

  • Venus air temperatures above clouds are driven by atmosphere dynamics
  • Cloud altitude increases toward the equator also on the nightside
  • [CO] at 65-70 km increases from 40S to 60S

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