Jupiter's ionosphere: Results from the first Galileo radio occultation experiment

被引:87
作者
Hinson, DP
Flasar, FM
Kliore, AJ
Schinder, PJ
Twicken, JD
Herrera, RG
机构
[1] NASA,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771
[2] CALTECH,JET PROP LAB,PASADENA,CA 91109
[3] CORNELL UNIV,DEPT ASTRON,ITHACA,NY 14853
关键词
D O I
10.1029/97GL01608
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The Galileo spacecraft passed behind Jupiter on December 8, 1995, allowing the first radio occultation measurements of its ionospheric structure in 16 years. At ingress (24 degrees S, 68 degrees W), the principal peak of electron density is located at an altitude of 900 km above the 1-bar pressure level, with a peak density of 10(5) cm(-3) and a thickness of similar to 200 km. At egress (43 degrees S, 28 degrees W), the main peak is centered near 2000 km altitude, with a peak density of 2x10(4) cm(-3) and a thickness of similar to 1000 km. Two thin layers, possibly forced by upwardly propagating gravity waves, appear at lower altitudes in the ingress profile. This is the first in a two-year series of observations that should help to resolve long-standing questions about Jupiter's ionosphere.
引用
收藏
页码:2107 / 2110
页数:4
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