| タイトル | The atmosphere of Jupiter - An analysis of the Voyager radio occultation measurements |
| 著者（英） | Hotz, H. B.; Doms, P. E.; Buckles, B. J.; Levy, G. S.; Wood, G. E.; Sweetnam, D. N.; Lindal, G. F.; Eshleman, V. R.; Holmes, D. P.; Anderson, J. D. |
| 著者所属（英） | Stanford Univ.|Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 1981-09-30 |
| 言語 | eng |
| 内容記述 | Coherently related S and X band signals of 2.3 and 8.4 GHz, respectively, which were transmitted from Voyagers 1 and 2 were used to probe the Jovian atmosphere. Height profiles of the gas refractivity, molecular number density, pressure, temperature, and microwave absorption in the troposphere and stratosphere were observed at latitudes ranging from 0 to 70 deg S. At 1000 mbar, the temperature was + or - 5 K and the lapse rate was equal to the adiabatic value of 2.1 K/km within the resolution of the measurements. The ammonia abundance in this region was 0.022 + or - 0.008%, which is in good agreement with values derived from cosmic abundance considerations. The tropopause at the 140 mbar level had a temperature of 110 K, which increased with increasing altitude, reaching 160 + or - 20 K in the 10 to 1 mbar region. Significant horizontal density variations were detected in the stratosphere, which implies a nonuniform temperature and aerosol distribution across the Jovian disk or across high- and low-pressure regions due to local atmospheric dynamics. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 82A12374 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/413253 |
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