Range of frequency drift of the solar type III bursts

Details Range of frequency drift of the solar type III bursts Range of frequency drift of the solar type III bursts

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001izkry..97...56y&link_type=abstract

Izvestiya Krymskoj Astrofizicheskoj Observatorii, Tom 97, p. 56 - 59 (2001)

Mathematics

Probability

Solar Radio Bursts

Scientific paper

It is shown that an evaluation of probability of emission of energy inside a frequency bandwidth B is being described by the distribution of inverse value 1/B but not by the distribution of variable B itself. The application of this result for analysis of empirical histograms of type III bursts shows that the long tracks of bursts with size of 600 MHz occupied 10 times bigger interval of frequency than a summarized range occupied by all short tracks with a size of 45 MHz everyone. Therefore, the radio source emits the energy mainly in the form of long tracks.

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