1976The Astrophysical JournalRequires access

The 800-1200 inverse centimeter absorption spectrum of Jupiter

S. T. Ridgway, Lynne Wallace, Gerald Ray Smith

Open publisher page 100 citations

Abstract

Synthetic spectra computed from radiative models of the Jovian thermal structure are compared with observed spectra. The results imply a subsaturated NH3 abundance near the temperature minimum, and an additional opacity source near 1100 kaysers. Evidence is found for the presence of PH3 consistent with a solar P abundance.

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What this paper is about

Synthetic spectra computed from radiative models of the Jovian thermal structure are compared with observed spectra. The results imply a subsaturated NH3 abundance near the temperature minimum, and an additional opacity source near 1100 kaysers. Evidence is found for the presence of PH3 consistent with a solar P abundance.

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Available abstract

Synthetic spectra computed from radiative models of the Jovian thermal structure are compared with observed spectra. The results imply a subsaturated NH3 abundance near the temperature minimum, and an additional opacity source near 1100 kaysers. Evidence is found for the presence of PH3 consistent with a solar P abundance.

Key concepts: Physics, Jupiter (rocket family), Astrophysics, Jovian, Spectral line, Astronomy, Opacity, Radiative transfer

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