Clearer circulation on Uranus
Abstract
Discoveries made with the Voyager 2 flyby concerning the atmospheric circulation on Uranus are discussed. The lack of horizontal thermal constrast with latitude is explained in terms of a circulation similar to the Hadley circulation on earth. Uranus appears to be unique in the solar system in possessing a retrograde equatorial jet near the top of its atmosphere. The pattern of zonal winds on Uranus, as on Jupiter and Saturn, decays with height above the visible clouds. The solar-driven component is the dominant energy source driving the upper-level circulation of the atmosphere of Uranus. The entire circulation pattern of Uranus seems to be displaced along the rotation axis toward the (dark) north pole.
- Publication:
-
Nature
- Pub Date:
- January 1987
- DOI:
- 10.1038/325197a0
- Bibcode:
- 1987Natur.325..197R
- Keywords:
-
- Atmospheric Circulation;
- Atmospheric Models;
- Uranus Atmosphere;
- Voyager Project;
- Energy Budgets;
- Planetary Environments;
- Solar Radiation;
- Lunar and Planetary Exploration; Uranus;
- URANUS;
- ATMOSPHERE;
- CIRCULATION;
- VOYAGER 2;
- SPACECRAFT OBSERVATIONS;
- THERMAL PROPERTIES;
- HEATING;
- RADIATION;
- SOLAR RADIATION;
- DIAGRAMS;
- LATITUDE;
- IRIS;
- INFRARED INTERFEROMETER SPECTROMETER;
- POLAR REGIONS;
- EQUATORIAL REGIONS;
- COMPARISONS;
- PATTERNS;
- ROTATION;
- MOTION;
- WINDS