Saturn's seasonal winds and temperature: The effect of the ring system on the troposphere and stratosphere
The radiative properties of Saturn's rings (insolation shadowing, insolation scattering, and thermal emission) were incorporated into a seasonal, zonally-averaged, radiative-dynamical model to investigate the magnitude of small seasonal fluctuations in the troposphere and stratosphere of Saturn. Although the radiative time constant is large in Saturn's troposphere and stratosphere, the rings induce significant latitudinal insolation gradients resulting in potential disturbances in the upper stratosphere. The results of the model are compared to the Pioneer and Voyager Radio Sub-System (RSS) vertical temperature profile measurements and to the Voyager Infrared Interferometric Spectrometer (IRIS) latitudinal temperature profile measurements. In the upper stratosphere (1 to 30 mBar) the heating is dominated by methane and the model can be directly compared to the Voyager data. Below the temperature minimum the radiative time constant is sufficiently long to strongly dampen seasonal variations, however, the temperature excursions seen in the IRIS data are significantly larger than those predicted by the radiative model. The thermal effects of the strong Saturnian zonal winds are simulated with a first-order dynamical model to provide some insight into the lower boundary conditions. The remaining differences between the model and the Voyager IRIS data-sets are used to estimate the quantity of aerosol required near the tropopause region. The magnitudes of the wind and temperature perturbations, caused by the radiative effects of Saturn's rings, are discussed in the context of the future Hubble Space Telescope and the planned Cassini Saturnian Orbiter missions.
- Research Organization:
- New Mexico State Univ., Las Cruces, NM (USA)
- OSTI ID:
- 5912073
- Resource Relation:
- Other Information: Ph.D. Thesis
- Country of Publication:
- United States
- Language:
- English
Similar Records
Revelations of a stratospheric circulation: The dynamical transport of hydrocarbons in the stratosphere of Uranus
Changes to Saturn's zonal-mean tropospheric thermal structure after the 2010-2011 northern hemisphere storm
Related Subjects
GENERAL PHYSICS
SATURN PLANET
PLANETARY ATMOSPHERES
TEMPERATURE DISTRIBUTION
WIND
AEROSOLS
ANNUAL VARIATIONS
BOUNDARY CONDITIONS
EXPERIMENTAL DATA
INSOLATION
STRATOSPHERE
TEMPERATURE EFFECTS
THERMAL RADIATION
TROPOSPHERE
ATMOSPHERES
COLLOIDS
DATA
DISPERSIONS
EARTH ATMOSPHERE
ELECTROMAGNETIC RADIATION
INFORMATION
NUMERICAL DATA
PLANETS
RADIATIONS
SOLS
VARIATIONS
640107* - Astrophysics & Cosmology- Planetary Phenomena