Some characteristics of pulsations in radio bursts at 9.375 GHz

Details Some characteristics of pulsations in radio bursts at 9.375 GHz Some characteristics of pulsations in radio bursts at 9.375 GHz

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.218..213q&link_type=abstract

Astrophysics and Space Science, vol. 218, no. 2, p. 213-222

Astronomy and Astrophysics

Astronomy

8

Pulsed Radiation, Radiant Flux Density, Radio Astronomy, Solar Activity, Solar Cycles, Solar Radio Bursts, Time Dependence, Magnetohydrodynamic Stability, Pulse Modulation, Pulse Repetition Rate, Radio Telescopes, Radiometers, Standards, Statistical Analysis

Scientific paper

A type of pulsation in a time scale of seconds superimposed on a microwave burst at 9.375 GHz has been found during the twenty-second solar active maximum period by us. This phenomenon is quite different from radio spike emission at decimeter and long centimeter wavelengths. The flux level of the bursts rises as the repetition rate of pulsations increases, following an approximate linear relationship. This feature resembles that at mm wavelength, but some other features are different. Some mechanisms for interpretation have been proposed.

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