Proper solar wind power estimation and planetary radiometric efficiencies

Details Proper solar wind power estimation and planetary radiometric efficiencies Proper solar wind power estimation and planetary radiometric efficiencies

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.314..455b&link_type=abstract

Nature (ISSN 0028-0836), vol. 314, April 25, 1985, p. 455, 456; Author's Reply, p. 456. Research sponsored by the U.S. Departmen

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Planetary Radiation, Radio Emission, Solar Planetary Interactions, Solar Wind, Earth Magnetosphere, Kilometric Waves, Planetary Magnetic Fields, Uranus (Planet)

Scientific paper

The methods, assumptions, and conclusions of a paper by Desch and Kaiser (1984), who computed the average absolute efficiencies of the radio planets for electromagnetic wave production, are criticized, and Desch and Kaiser reply. Based on a new computation of the energy entering the earth's magnetosphere, it is concluded that auroral kilometric radiation is produced with a much higher efficiency than that computed by Desch and Kaiser. It is suggested that radio emissions for unexplored planets such as Uranus may be much different from the values determined by Desch and Kaiser.

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