Long-wave radio emission of solar and magnetospheric origin during proton events

Details Long-wave radio emission of solar and magnetospheric origin during proton events Long-wave radio emission of solar and magnetospheric origin during proton events

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kosis..28..951v&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 28, Nov.-Dec. 1990, p. 951-955. In Russian.

Physics

Energetic Particles, Solar Flares, Solar Protons, Solar Radio Emission, Auroral Electrojets, Earth Magnetosphere, Geomagnetism, Long Wave Radiation, Prognoz Satellites

Scientific paper

Prognoz-8 observations of proton events are examined. In addition to long-wave radio-emission bursts of solar origin, low-frequency magnetospheric emission in the 114-540 kHz range was recorded with powers up to 10 to the -11th to 10 to the -12th W/sq m s Hz. The source of this emission was located in the auroral zone; the emission is characterized as auroral kilometric radiation.

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