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°S, 68°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 105 cm-3 and a thickness of ∼200 km. At egress (43°S, 28°W), the main peak is centered near 2000 km altitude, with a peak density of 2×104 cm-3 and a thick-ness of ∼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. Copyright 1997 by the American Geophysical Union.
CITATION STYLE
Hinson, D. P., Flasar, F. M., Kliore, A. J., Schinder, P. J., Twicken, J. D., & Herrera, R. G. (1997). Jupiter’s ionosphere: Results from the first Galileo radio occultation experiment. Geophysical Research Letters, 24(17), 2107–2110. https://doi.org/10.1029/97GL01608
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