Far-infrared spectral observations of Venus, Mars, and Jupiter

Details Far-infrared spectral observations of Venus, Mars, and Jupiter Far-infrared spectral observations of Venus, Mars, and Jupiter

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977icar...30..295w&link_type=abstract

Icarus, vol. 30, Feb. 1977, p. 295-300.

Astronomy and Astrophysics

Astronomy

5

Brightness Temperature, Far Infrared Radiation, Infrared Astronomy, Jupiter Atmosphere, Mars Atmosphere, Venus Atmosphere, Ammonia, Atmospheric Temperature, Black Body Radiation, Calibrating, Lear Jet Aircraft, Lunar Atmosphere, Signal To Noise Ratios

Scientific paper

Spectra of Venus, Mars, and Jupiter between 45 and 115 micron have been obtained at a resolving power of about 10, observing from the NASA Lear Jet at an altitude of 13.7 km. The results are calibrated with lunar observations, and show Mars and Venus to have relatively constant brightness temperatures over this wavelength region, with Venus appearing somewhat warmer at longer wavelengths. The brightness temperature of Jupiter decreases slightly toward longer wavelengths.

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