The possibility of classifying local sources of solar-radio emission according to fluctuation power spectra

Details The possibility of classifying local sources of solar-radio emission according to fluctuation power spectra The possibility of classifying local sources of solar-radio emission according to fluctuation power spectra

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..907b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, Nov.-Dec. 1990, p. 907-910. In Russian.

Physics

Microwave Emission, Power Spectra, Solar Activity, Solar Radio Emission, Annual Variations, Solar Atmosphere, Solar Corona, Solar Flares, Variations

Scientific paper

An analysis is made of fluctuations of the microwave emission of solar active regions, flocculae, the quiet atmosphere, and coronal holes. It is shown that these types of emission sources differ in terms of the degree of fluctuation-energy concentration in the long-period part of their power spectrum. It is noted that numerical series of these characteristics can be used for the prediction of solar activity.

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