Radio spectrum and position of two solar spike burst sources

Details Radio spectrum and position of two solar spike burst sources Radio spectrum and position of two solar spike burst sources

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..106c&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Feb. 1982, p. 106-108.) Soviet Astronomy Letters, vol. 8, Jan.-Feb. 1982, p. 54-56.

Astronomy and Astrophysics

Astronomy

Radio Spectra, Solar Radio Bursts, Solar Spectra, Spectrum Analysis

Scientific paper

A comparison is made between simultaneous observations of a pair of spike bursts during the July 19, 1971 solar noise storm, as carried out with a 151-187 MHz dynamic spectrograph and a 169-MHz radiometer at the Institute of Terrestrial Magnetism near Moscow and with a 159-179 MHz multichannel spectrograph and a 169-MHz radio heliograph at Nancay. The broadening of the noise storm source indicates that the spike sources are about 2 arcmin in diameter. They might originate from breakup of type I radio burst sources.

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