| タイトル | Thermal radio emission from Jupiter and Saturn. |
| 著者（英） | Gulkis, S.; Poynter, R. |
| 発行日 | 1972-12-01 |
| 言語 | eng |
| 内容記述 | Microwave brightness temperature calculations have been carried out for a number of model atmospheres for Jupiter and Saturn. The models considered are characterized by helium to hydrogen number mixing ratios which range from 0 to 0.2. Gaseous ammonia is assumed to be a trace constituent in all the models. The ammonia abundance below the (NH3) cloud level is a free parameter which is determined by comparing the observed thermal spectrum of Jupiter and the total spectrum of Saturn with the model calculations. The theoretical microwave spectra corresponding to those models in which the ammonia abundance is that expected from an atmosphere containing a solar abundance of elements are found to be in generally good agreement with the observations. |
| NASA分類 | SPACE SCIENCES |
| レポートNO | 73A25883 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/457867 |
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