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Detailed Reference Information
Folkner et al. 1998
Folkner, W.M., Woo, R. and Nandi, S. (1998). Ammonia abundance in Jupiter’s atmosphere derived from the attenuation of the Galileo probe’s radio signal. Journal of Geophysical Research 103: doi: 10.1029/98JE01635. issn: 0148-0227.

The radio signal from the Galileo probe to the orbiter experienced attenuation due to ammonia in Jupiter's atmosphere during the probe descent. A profile of the ammonia content as a function of depth in the atmosphere has been derived from the measurements of the attenuation. The derived ammonia abundance rises to a molar fraction of 700¿100 parts per million for pressures greater than 7 bars, about 4 times that expected based on the solar abundance of nitrogen. ¿ 1998 American Geophysical Union

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Abstract

Keywords
Planetology, Fluid Planets, Atmospheres—composition and chemistry
Journal
Journal of Geophysical Research
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Publisher
American Geophysical Union
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