On solar decimeter radio fluctuations

Details On solar decimeter radio fluctuations On solar decimeter radio fluctuations

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990an....311..363a&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 311, no. 6, 1990, p. 363-365.

Astronomy and Astrophysics

Astrophysics

2

Decimeter Waves, Solar Oscillations, Solar Radio Emission, Maximum Entropy Method, Periodic Variations, Power Spectra

Scientific paper

Results are reported from a search for periodic fluctuations in solar radio emission in the dm band (755 MHz). Data obtained at Riga Radioastrophysical Observatory and at Tremsdorf Solar Radio Observatory (separated by about 850 km) during a 15-day period in October-November 1987 are presented in graphs and briefly characterized on the basis of a maximum-entropy analysis. Although most of the dm fluctuations seem to be of nonsolar origin, as reported by Benz and Fuerst (1987) for 4.75 GHz, some discrete signals with the same periods (in the range 3-200 sec) were found at the two stations. The potential value of further coordinated observations using widely separated telescopes is indicated.

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