Observations of the auroral hectometric radio emission onboard the INTERBALL-1 satellite

Details Observations of the auroral hectometric radio emission onboard the INTERBALL-1 satellite Observations of the auroral hectometric radio emission onboard the INTERBALL-1 satellite

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cosre..45..248k&link_type=abstract

Cosmic Research, Volume 45, Issue 3, pp.248-252

Physics

96.12.De

Scientific paper

The results of five-year (1995 2000) continuous observations of the auroral radio emission (ARE) in the hectometric wavelength range on the high-apogee INTERBALL-1 satellite are presented. Short intense bursts of the auroral hectometric radio emission (AHR) were observed at frequencies of 1463 and 1501 kHz. The bursts were observed predominantly at times when the terrestrial magnetosphere was undisturbed (in the quiet Sun period), and their number decreased rapidly with increasing solar activity. The bursts demonstrated seasonal dependence in the Northern and Southern hemispheres (dominating in the autumn-winter period). Their appearance probably depends on the observation time (UT). A qualitative explanation of the AHR peculiarities is given.

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