Wm. Folkner et al., Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signal, J GEO R-PLA, 103(E10), 1998, pp. 22847-22855
The radio signal from the Galileo probe to the orbiter experienced attenuat
ion due to ammonia in Jupiter's atmosphere during the probe descent. A prof
ile of the ammonia content as a function of depth in the atmosphere has bee
n derived from the measurements of the attenuation. The derived ammonia abu
ndance rises to a molar fraction of 700 +/- 100 parts per million for press
ures greater than 7 bars, about 4 times that expected based on the solar ab
undance of nitrogen.