Correlation of hard X-ray and type III bursts in solar flares

Details Correlation of hard X-ray and type III bursts in solar flares Correlation of hard X-ray and type III bursts in solar flares

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...87..165p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 87, Aug. 1983, p. 165-175.

Physics

2

Solar Flares, Solar X-Rays, Type 3 Bursts, Bivariate Analysis, Correlation, Electron Acceleration, X Ray Spectra

Scientific paper

The observed correlations between X-ray and type III radio emissions from solar bursts are described by means of a bivariate distribution function. Procedures for determining the form of this distribution are described using a sample of data analyzed by Kane (1981). With the help of this distribution a model is constructed to explain the correlation between the X-ray spectral index and the ratio of X-ray to radio intensities. Implications of the model are discussed.

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