Statistics – Methodology
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992itmtt..40.1101j&link_type=abstract
IEEE Transactions on Microwave Theory and Techniques (ISSN 0018-9480), vol. 40, no. 6, June 1992, p. 1101-1109. Research support
Statistics
Methodology
5
Atmospheric Attenuation, Atmospheric Composition, Hydrogen Sulfide, Jupiter Atmosphere, Millimeter Waves, Absorption Spectra, Atmospheric Models, Brightness Temperature, Radiative Transfer
Scientific paper
Jupiter was observed at two wavelengths near 1.4 mm in an attempt to detect gaseous hydrogen sulfide (H2S) or place new upper limits on its abundance on Jupiter's atmosphere. Although no H2S was detected, the first brightness temperature observations of Jupiter at 1.4 mm are reported with a spectral resolution of approximately 1 GHz using Mars as a calibration standard. The methodology and results of a laboratory experiment in which H2S absorption at 1.4 mm was measured in a simulated Jovian atmosphere. The results of laboratory measurements are applied to a radiative transfer model which is used to interpret the observations of Jupiter.
Joiner Joanna
Noll Keith S.
Steffes Paul Gregory
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