Spectral structures of type 'line' in the microwave burst emission at the sun

Details Spectral structures of type 'line' in the microwave burst emission at the sun Spectral structures of type 'line' in the microwave burst emission at the sun

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..138..201k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 138, March 1992, p. 201-203.

Physics

Solar Radio Bursts, Solar Spectra, Emission Spectra, Radio Spectra, Solar Flares, Solar Magnetic Field

Scientific paper

Observational results of radioburst spectra in the range of 2.0-4.0 GHz
are presented. It is shown that the narrow-band spectral structures of
the type 'line' with line widths of Df/f not greater than 0.1 and
intensity DF/F greater than 10 percent are observed in the impulsive
phase of the bursts.

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