| タイトル | Voyager 2 radio science observations of the Uranian system Atmosphere, rings, and satellites |
| 著者（英） | Lindal, G. F.; Campbell, J. K.; Marouf, E. A.; Tyler, G. L.; Anderson, J. D.; Hinson, D. P.; Sweetnam, D. N.; Eshleman, V. R.; Simpson, R. A.; Levy, G. S. |
| 著者所属（英） | Stanford Univ.|Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 1986-07-04 |
| 言語 | eng |
| 内容記述 | The results of preliminary analyses of radio occultation data obtained by Voyager 2 as it passed Uranus are described. The occultations took place between 2-7 deg S latitude and yielded atmospheric temperature profiles between pressure levels of 10-900 mbar, an altitude range of 100 km. The mole fractions of hydrogen and helium in the tropopause were estimated, in conjunction with IR data, to about 0.85 and 0.10-0.20, respectively. Radio signal intensity data indicated the presence of a cloud deck of CH4 ice at a pressure level of 1300 mbar and a temperature of 81 K, implying a CH4 mole fraction of 0.02 at very low altitudes. The ionosphere extended upward, in two levels, to more than 10,000 km altitude. The ring system was different than the one around Saturn and possessed cylindrical substructures. The radio data also permitted mass density estimates for the five major moons, i.e., about 1.40 gr/cu cm, a value which rules out cometary origins. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 86A44257 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/383598 |
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