金星大気の近赤外線分光撮像観測

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(99) }!^- `±(018!²^³´1S. 36. Shoko OHTSUKI and Hideo SAGAWA Graduate School of Science, University of Tokyo, 7ῌ3ῌ1 Hongo, Bunkyo-ku, Tokyo 113ῌ0033, Japan Munetaka UENO Graduate School of Arts and Sciences, University of Tokyo, 3ῌ8ῌ1 Komaba, Meguro-ku, Tokyo 153ῌ8902, Japan Abstract : We present a report on our recent observations of Venus atmosphere which we have performed in infrared wavelength at Okayama Astrophysical Observatory. The data show important results on the CO distribution and on O2 IRA (0, 0) 1.27 mm airglow in the atmosphere. The infrared windows of the Venusian atmosphere are rather developing areas and will give us important information on the dynamics of Venus atmosphere.. %µ3. 2005 6 1 µ.

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