A method to analyze imaging radio data on solar flares

Details A method to analyze imaging radio data on solar flares A method to analyze imaging radio data on solar flares

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003soph..213..103g&link_type=abstract

Solar Physics, v. 213, Issue 1, p. 103-110 (2003).

Physics

12

Scientific paper

Microwave imaging data are widely used in analysis of solar flares. To identify essential features and study their behavior, one has to deal with large data sets of hundreds of frames. This allows a single image, a variance map, to represent the overall dynamics of the event. A method is presented that allows investigation of the detected positions of sources in both Stokes I and V using the analysis of variance maps, combined difference images, and total flux time profiles.

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