Narrow-band radiation component in the flash phase of a microwave burst

Details Narrow-band radiation component in the flash phase of a microwave burst Narrow-band radiation component in the flash phase of a microwave burst

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989raf....32..516l&link_type=abstract

Radiofizika (ISSN 0021-3462), vol. 32, April 1989, p. 516-519. In Russian.

Computer Science

4

Microwave Spectra, Solar Radio Bursts, Solar Spectra, Dynamic Characteristics, Error Analysis, Spectrum Analysis

Scientific paper

The spectral and temporal characteristics of the sun's radio emission bursts were studied in the frequency range 8-12 GHz in order to investigate the dynamics of the flash component of the radiation. Elementary flash events are identified which can be accounted for in terms of a quasi-linear plasma generation mechanism. It is shown that the obervation of the 'plasma line', a narrow-band drifting-frequency component, makes it possible to predict such parameters as plasma inhomogeneity scales and plasma concentration in the radiation source region and the transverse dimensions of the energy release region.

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