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Detailed Reference Information |
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. |
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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 |
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Keywords
Planetology, Fluid Planets, Atmospheres—composition and chemistry |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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