Spectral analysis of solar radio type III burst groups

Details Spectral analysis of solar radio type III burst groups Spectral analysis of solar radio type III burst groups

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acasn..32...28p&link_type=abstract

(Acta Astronomica Sinica, vol. 32, no. 1, 1991, p. 28-35) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, Sept. 19

Astronomy and Astrophysics

Astrophysics

Spectrum Analysis, Type 3 Bursts, Fourier Transformation, Frequency Distribution, Radio Telescopes

Scientific paper

Using high-time-resolution and high-sensitivity data on the intensity, polarization, position and size of type-III burst groups obtained at 5 frequencies, a careful Fourier transform spectral analysis is conducted. The study further confirms the existence of periodicity in type-III burst groups; most of the events have periods between 1 and 6 seconds and show multiple periods at a 90-percent confidence level or better. The type-III burst groups can be divided into two classes, one with weak polarization and with periods over a wide range up to 6 seconds, and the other with strong polarization and short periods of less than 2 seconds and smaller-size compact sources.

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