Observation and analysis of solar decimetric spike radiation

Details Observation and analysis of solar decimetric spike radiation Observation and analysis of solar decimetric spike radiation

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cha%26a..16...84w&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 16, Issue 1, p. 84-90.

Astronomy and Astrophysics

Astrophysics

Sun-Radio Burst-Spike Radiation

Scientific paper

From January, 1988 to June, 1989 the solar radio synchronous observational system with high temporal resolution of the Yunnan Observatory was used to carry out observations at a decimetric wavelength (1420 MHz), and the data are analyzed in this paper. The result shows a relation between the millisecond spike radiation of the solar decimetric radio emission and the radio bursts recorded with a time constant of one second. It also reveals the coexistence of decimetric radio millisecond spike radiations and Hα flares, type III radio bursts as well as soft X-ray bursts. A solar activity event with abundant radio millisecond spike radiations is investigated preliminarily and the relation between the duration and flux of individual spikes is discussed.

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