Prediction of radio frequency power generation of Neptune's magnetosphere from generalized radiometric Bode's law

Details Prediction of radio frequency power generation of Neptune's magnetosphere from generalized radiometric Bode's law Prediction of radio frequency power generation of Neptune's magnetosphere from generalized radiometric Bode's law

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988georl..15..111m&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 15, Jan. 1988, p. 111-113.

Physics

8

Neptune Atmosphere, Planetary Magnetospheres, Radio Frequencies, Radiometers, Planetary Magnetic Fields, Solar Wind, Spin Dynamics, Neptune, Frequencies, Radio Emissions, Power, Magnetosphere, Solar Wind, Magnetic Fields, Parameters, Density, Angular Momentum, Scaling Laws, Radiometry, Analysis, Mass, Distance, Calculations, Radiation, Models, Theoretical Studies, Comparisons, Hypotheses

Scientific paper

Magnetospheric radio frequency emission power has been shown to vary as a function of both solar wind and planetary values such as magnetic field by Kaiser and Desch. Planetary magnetic fields have been shown to scale with planetary variables such as density and angular momentum by numerous researchers. This paper combines two magnetic scaling laws (Busse's and Curtis Ness') with the radiometric law to yield "Bode's"-type laws governing planetary radio emission. Further analysis allows the reduction of variables to planetary mass and orbital distance. These generalized laws are then used to predict the power output of Neptune to be about 1.6×107W; with the intensity peaking at about 3 MHz.

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