Development of fluctuations in local solar radio sources, and the growth of sunspot groups

Details Development of fluctuations in local solar radio sources, and the growth of sunspot groups Development of fluctuations in local solar radio sources, and the growth of sunspot groups

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5...42g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Jan. 1979, p. 42-46.) Soviet Astronomy Letters, vol. 5, Jan.-Feb. 1979, p. 24-26. Tr

Physics

1

Power Spectra, Solar Radio Emission, Solar Spectra, Sunspots, Interferometry, Solar Physics

Scientific paper

The time characteristics of the radio fluctuations of local solar sources at wavelengths of 3.5 and 3.9 cm are investigated. Fluctuation components of periods longer than 20 min are observed to strengthen when the leading sunspot in a group is growing larger. The oscillations tend to appear episodically. Peaks in the power spectrum often recur at the same value of the period.

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