Physics
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989icar...81..386j&link_type=abstract
Icarus (ISSN 0019-1035), vol. 81, Oct. 1989, p. 386-395.
Physics
10
Absorption Spectra, Ammonia, Jupiter Atmosphere, Microwave Attenuation, Millimeter Waves, Controlled Atmospheres, Radio Occultation, Simulation
Scientific paper
An attempt is made to infer the abundance and distribution of ammonia from RF emission measurements more accurately than heretofore, on the basis of the results of laboratory measurements for the mm-wave opacity of gaseous ammonia under simulated Jovian atmosphere conditions. The measurements were conducted at various frequencies in the 32-40 GHz range at 2 atm and 203 K; the atmospheric mixture was 88.34 percent H2, 9.81 percent He, and 1.85 percent NH3. Experimental results are found to be readily modeled by the Gross (1955) line-shape factor, rather than that of Van Vleck and Weisskopf (1945).
Jenkins Jon Michael
Joiner Joanna
Steffes Paul Gregory
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