The angular distribution of auroral kilometric radiation

Details The angular distribution of auroral kilometric radiation The angular distribution of auroral kilometric radiation

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jgr....82.1825g&link_type=abstract

Journal of Geophysical Research, vol. 82, May 1, 1977, p. 1825-1838. Navy-NSF-supported research;

Physics

22

Angular Distribution, Atmospheric Radiation, Auroral Zones, Night Sky, Radiation Distribution, Radio Emission, Auroral Electrojets, Cones, Diurnal Variations, Earth Magnetosphere, Power Spectra, Satellite Observation, Symmetry

Scientific paper

A study based on data from Hawkeye 1, Imp 6 and Imp 8 satellites has shown that the intense kilometric radio emissions generated over the nightside auroral regions are beamed into a cone-shaped region whose axis of symmetry is tilted away from the magnetic axis of the earth, toward evenings, by about 20 deg. The solid angle of this emission cone increases systematically with increasing frequency, varying from about 1.1 sr at 56.2 kHz to about 3.5 sr at 178 kHz.

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