Infrared radiation of the giant planets

Details Infrared radiation of the giant planets Infrared radiation of the giant planets

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979infph..19..353e&link_type=abstract

(Swiss National Science Foundation, Eidgenoessisches Militaerdepartement, and Eidgenoessische Technische Hochschule Zuerich, Int

Physics

1

Abundance, Gas Giant Planets, Infrared Radiation, Planetary Atmospheres, Planetary Radiation, Thermal Emission, Cosmology, Far Infrared Radiation, Jupiter Atmosphere, Near Infrared Radiation, Solar Spectra

Scientific paper

The study of the giant planets is of major interest for cosmogonical and cosmological research, because their atmospheres are, in some aspects, representative of the early stage of the solar system. From the study of the planetary spectra in the near-infrared and far-infrared range, many important results have been obtained during the past 10 years, especially about the abundance ratios of elemental and isotopic species, and some physical and chemical parameters of the planetary atmospheres. These results are reviewed and discussed in detail. In particular, we conclude that the Jovian atmosphere does not seem to have significantly evolved since its origin.

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