Physics
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989stin...0000441.&link_type=abstract
Technical Report, NONP-NASA-VT-1999206990
Physics
Solar System, Flyby Missions, Voyager 2 Spacecraft, Saturn Satellites, Saturn (Planet), Uranus Satellites, Uranus (Planet), Jupiter Satellites, Jupiter (Planet), Neptune Satellites, Neptune (Planet), Computerized Simulation, Zonal Flow (Meteorology), Planetary Rings, Jet Streams (Meteorology), Atmospheric Physics
Scientific paper
The main focus of this lecture is to discuss the relative size of the planets, the formation of the solar system, details of atmospheric motion (atmospheric dynamics), the aspects of the magnetic fields, different ring systems, and the Triton satellite. The study evolves around the planets of Jupiter, Saturn, Uranus, and Neptune. Their temperature and absorption properties of the ice are discussed. Two of the chemicals being absorbed by the ice are ammonia and methane. Also discussed are the belt and zonal circulation models, jet streams, plumes and clouds, magnetic fields, planetary rings, the pressure on Triton, the atmosphere of Titan, Callisto, Aria, Ganymede, Ariel, Miranda, Io, Europa, Amalthea, Rhea, Dione, Tethys, Enceladus, Mimas, Hyperion, Oberon, Titania, and Umbriel. The lecture also contained some computerized simulation and various images from Voyager.
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