Upper limits on hydrogen halides in Jupiter from Cassini/CIRS observations

Details Upper limits on hydrogen halides in Jupiter from Cassini/CIRS observations Upper limits on hydrogen halides in Jupiter from Cassini/CIRS observations

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004icar..170..237f&link_type=abstract

Icarus, Volume 170, Issue 1, p. 237-241.

Computer Science

5

Atmosphere, Composition, Atmospheres

Scientific paper

We have determined the following upper limits for the mole fraction of hydrogen halides in Jupiter's atmosphere from Cassini/CIRS observations: [HF]<2.7×10-11, [HCl]<2.3×10-9, [HBr]<1.0×10-9, [HI]<7.6×10-9. These limits are smaller than solar composition for HF and HCl, and support the halogens' condensation in ammonium salts predicted by thermochemical models for the upper jovian troposphere.

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