| タイトル | Radiative forcing of the Venus mesosphere. II - Thermal fluxes, cooling rates, and radiative equilibrium temperatures |
| 著者（英） | Crisp, David |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech.|Princeton Univ. |
| 発行日 | 1989-02-01 |
| 言語 | eng |
| 内容記述 | A radiative heat-transfer model is presently used to ascertain the way in which radiative forcing contributes to the up to 20 K higher temperature of the Venus polar regions, by comparison with the tropics, in the 60-100 km mesospheric levels. Model global-mean radiative equilibrium temperatures for 55-100 km are compared with observations to show how each opacity source contributes to the thermal structure. The results obtained from latitude-dependent radiative equilibrium experiments indicate that meridional variations in radiative forcing obliterate observed mesospheric temperature gradients and yield polar temperatures up to 40 K cooler than the tropics. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 89A33320 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/364279 |
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