Observations of Jupiter with SWS: ammonia and hydrocarbons distributions

Details Observations of Jupiter with SWS: ammonia and hydrocarbons distributions Observations of Jupiter with SWS: ammonia and hydrocarbons distributions

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427..177f&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 177

Computer Science

2

Solar System, Jupiter

Scientific paper

ISO-SWS has observed Jupiter on May, 23rd 1997, from 2.5 to 16 μm, encompassing the spectral signatures of all the major gaseous absorbers of the planet. Here we present the results concerning the ammonia vertical distribution from 0.2 to 8 bar, the ratio isotopic ratio measured in the ammonia, the thermal profile of the stratosphere, and the vertical distributions of two hydrocarbons (ethane and acetylene).

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