| タイトル | Laser heterodyne spectroscopy |
| 著者（英） | Betz, A. L.; Mcalary, C. W.; Mclaren, R. A.; Sutton, E. C. |
| 著者所属（英） | Toronto Univ. Ontario|California Univ. |
| 発行日 | 1978-01-01 |
| 言語 | eng |
| 内容記述 | High-resolution heterodyne spectroscopic studies of the atmosphere of Venus are surveyed with attention to Doppler shifts in the 10-micron CO2 lines. While the C-12(O-16)2 emission lines formed in the mesosphere near 115 km indicate that the winds are distinctly subsolar to antisolar, C-13(O-16)2 absorption lines for the stratosphere at about 75 km confirm that the pattern is a strong retrograde rotation with an average equatorial velocity of 90 plus or minus 7 m/sec. It is concluded that the winds change from retrograde to subsolar-to-antipolar between 80 and 115 km. |
| NASA分類 | ASTRONOMY |
| レポートNO | 79A13106 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/429572 |
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