Periodicities in the lambda 10 CM solar flux

Details Periodicities in the lambda 10 CM solar flux Periodicities in the lambda 10 CM solar flux

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...71..259h&link_type=abstract

Solar Physics, vol. 71, June 1981, p. 259-268.

Physics

26

Centimeter Waves, Periodic Variations, Solar Flux Density, Solar Rotation, Sunspot Cycle, Error Analysis, Solar Neutrinos, Solar Spectra

Scientific paper

An analysis is conducted on the 10-cm radiation from the sun, for which data is now available over the past 32 years. Not only is this data believed to be a reliable indicator of solar activity, but it is more amenable to physical interpretation than are other types of data, since its origin is more easily understood. The data are examined to see if there are any periodicities that persist throughout the 32 years, in particular, if there is any sign of those claimed by Dicke and Goldenberg (1967). A search is conducted for the longer periodicities, of about 1000 days, as suggested by Sakurai (1979). The results are presented as spectra of the radiation covering periods of from about 5 days to about 2000 days, the upper limit being determined by the finite amount of data (11658 days) and the large amplitude of the sunspot cycle.

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