Statistical analysis of fluctuations of solar decimeter radio emission and active longitudes

Details Statistical analysis of fluctuations of solar decimeter radio emission and active longitudes Statistical analysis of fluctuations of solar decimeter radio emission and active longitudes

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..368i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Mar.-Apr. 1989, p. 368-376. In Russian.

Astronomy and Astrophysics

Astronomy

Decimeter Waves, Periodic Variations, Solar Longitude, Solar Radio Emission, Statistical Analysis, Autocorrelation, Solar Rotation, Sunspots

Scientific paper

Ottawa data on the F10.7 radio emission flux for 1949-1986 are used for an autocorrelation analysis of fluctuations of the solar decimeter emission with characteristic times of several dozen days. Such fluctuations are usually modulated by radio emission regions (RERs) developing and traveling over the solar disk. It is shown that successive RERs appear at neighboring longitudes to form an RER complex with an average lifetime of about 10 solar rotations, the maximum lifetime sometimes reaching 40 rotations.

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