Angular distribution of auroral kilometric radiation observed by the GEOTAIL spacecraft

Details Angular distribution of auroral kilometric radiation observed by the GEOTAIL spacecraft Angular distribution of auroral kilometric radiation observed by the GEOTAIL spacecraft

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997georl..24.2483k&link_type=abstract

Geophysical Research Letters, vol. 24, p. 2483

Physics

Optics

16

Angular Distribution, Geomagnetic Tail, Atmospheric Radiation, Atmospheric Optics, Plasma Waves, Geomagnetism, Space Probes, Extraterrestrial Environments

Scientific paper

We examine the angular distribution of auroral kilometric radiation (AKR) based on a 38-month data set of GEOTAIL plasma wave observations. We show that the AKR illumination pattern becomes narrower with increasing frequency above 300 kHz. The difference is more evident in the duskside zone and when geomagnetic conditions become more disturbed. We also show that AKR is more active on the winter hemisphere especially for the higher frequency range.

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