Temporal characteristics of the Jovian atmosphere

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Annual Variations, Atmospheric Models, Jupiter Atmosphere, Temperature Gradients, Radiation Absorption, Solar Radiation, Stratosphere, Time Dependence, Jupiter, Atmosphere, Wavelengths, Temperatures, Stratosphere, Models, Troposphere, Voyager 1, Asymmetry, Absorption, Aerosols, Time Dependency, Radiation, Methane, Observations, Pressure, Comparisons, Saturn, Seasons, Polar Regions, Thermal Structure, Equatorial Regions

Scientific paper

Drift scans along the central meridian of Jupiter have been obtained at wavelengths of 7.9, 17.8, and 19.7 microns. These observations indicate a significant north-south temperature asymmetry within the Jovian stratosphere but not within its troposphere, results which agree with the recent Voyager 1 observations. Employing a time-dependent stratospheric model, it is found that the observed north-south asymmetry is consistent with seasonal stratospheric variability. In the model, the primary cause for this variability is the time-dependent absorption of sunlight by aerosols.

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