Drifting pulsations in a solar radio noise storm

Details Drifting pulsations in a solar radio noise storm Drifting pulsations in a solar radio noise storm

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56..867a&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, July-Aug. 1979, p. 867-871. In Russian.

Astronomy and Astrophysics

Astronomy

Drift Rate, Electromagnetic Pulses, Noise Storms, Solar Radio Bursts, Unsteady Flow, Alternations, Frequency Ranges, Wavelengths

Scientific paper

Observational data obtained at IZMIRAN in the frequency ranges from 45 to 90, 93 to 186, and 180 to 230 MHz are used to analyze pulsations in a meter-wavelength noise storm. The main characteristic of the event is shown to be the alternation of groups of pulsations with opposite frequency drift. The results are compared with radio-emission records obtained at two widely spaced points at frequencies of 68 and 200 MHz. It is concluded that the pulsations in the present case are of solar origin.

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