Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signal

Citation
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
Citations number
27
Categorie Soggetti
Space Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
ISSN journal
21699097 → ACNP
Volume
103
Issue
E10
Year of publication
1998
Pages
22847 - 22855
Database
ISI
SICI code
0148-0227(19980925)103:E10<22847:AAIJAD>2.0.ZU;2-Q
Abstract
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.