Distributions of the Venus 1.27-μm O2 airglow and rotational temperature

S. Ohtsuki, N. Iwagami, H. Sagawa, M. Ueno, Y. Kasaba, T. Imamura, K. Yanagisawa, E. Nishihara

研究成果: Article査読

23 被引用数 (Scopus)

抄録

Imaging spectroscopic observations of the Venus 1.27-μm O2 airglow were carried out with ground-based telescopes from 2002 to 2007. Spectral image cubes were taken with the Okayama Astrophysical Observatory/infrared imaging spectrometer (superOASIS), the Gunma Astronomical Observatory/near-infrared camera and NASA's Infrared Telescope Facility/cryogenic echelle spectrograph (CSHELL). The rotational temperature shows weak positive correlation with the airglow intensity. However, there are some regions that have almost same intensities but different temperatures. The intensities tend to decrease from the anti-solar point to the terminator besides local features. These results indicate that there are local strong downward flows superimposed on the subsolar-to-antisolar circulation.

本文言語English
ページ(範囲)1391-1398
ページ数8
ジャーナルPlanetary and Space Science
56
10
DOI
出版ステータスPublished - 2008 8

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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