| タイトル | Laboratory measurements and modeling of microwave absorption by ammonia in gas mixtures applicable to giant planet atmospheres |
| 本文（外部サイト） | http://hdl.handle.net/2060/19900017434 |
| 著者（英） | Spilker, T. R. |
| 著者所属（英） | Stanford Univ. |
| 発行日 | 1990-05-01 |
| 言語 | eng |
| 内容記述 | Accurate knowledge of the microwave absorption behavior of ammonia is critical to the correct interpretation of radio astronomical and radio occultation data from the giant planets. New cavity resonator techniques developed at the Stanford Center for Radar Astronomy have allowed accurate laboratory measurements of the microwave absorptivity and refractivity spectra of gas mixtures containing trace amounts of ammonia. A parameterized version of the modified Ben-Reuven formalism of Berge and Bulkis was optimized to fit the new data. The new formalism produced by this method predicts ammonia absorptivity much more accurately than previous formalism over a significant range of conditions. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 90N26750 |
| 権利 | No Copyright |
