Computer Science
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989stin...9024215h&link_type=abstract
Presented at the IAGA Scientific Assembly Symposium on Planetary Magnetospheres, Exeter, England, 24 Jul. - 4 Aug. 1989
Computer Science
Auroral Irradiation, Ionospheric Ion Density, Ohmic Dissipation, Planetary Atmospheres, Planetary Magnetospheres, Resistance Heating, Solar Planetary Interactions, Earth (Planet), Jupiter (Planet), Mars (Planet), Saturn (Planet), Uranus (Planet)
Scientific paper
Observed characteristics of the interactions of the magnetospheres on the planetary atmospheres of Earth, Mars, Jupiter, Uranus and Saturn are summarized. Tables containing the estimated order of magnitude of power associated with auroral particle precipitation and Joule heating and of ionospheric ion outward fluxes arrived at are given. Measurements from Viking, Phobos and Voyager missions are used. The auroral emission intensity of Earth is second only to that of Jupiter which is extreme in most respects. For planets with a corotating plasmasphere extending to the magnetopause, the Joule heating power is small compared with the precipitating particle power.
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