Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975p%26ss...23.1344s&link_type=abstract
Planetary and Space Science, vol. 23, Sept. 1975, p. 1344-1346.
Astronomy and Astrophysics
Astronomy
6
Astronomical Models, Electromagnetic Noise, Microwave Emission, Noise Storms, Solar Radiation, Decametric Waves, Imp, Lines Of Force, Solar Magnetic Field, Spaceborne Astronomy, Sunspots
Scientific paper
The relationship between metric noise continuum storms and the S-component of solar microwave emissions is examined by considering the properties of a solar active region and its relation to LF radio burst emissions observed by IMP 6. It is noted that the development of radio noise continuum sources in metric frequencies or less is usually preceded by the appearance of an S-emission source, which is formed in complex sunspot groups such as beta-gamma and gamma types. A model for the development of radio noise continuum sources in metric and decametric frequencies is proposed in which the development of relationships between emissions is closely connected to the growth of magnetic-field lines above associated sunspot groups into complex configurations.
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