Flux density distribution in solar type III radio bursts

Details Flux density distribution in solar type III radio bursts Flux density distribution in solar type III radio bursts

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnt...16..241y&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 16, no. 3, p. 241-244

Mathematics

Probability

Scientific paper

It is shown that the estinate of the energy emission probability described by the distribution of the inverse quantity 1/P rather than the distribution of the flux density P itself. The application of this result to the analysis of the empirical histograms of type III bursts showed that the bursts with a peak flux of the order of 100\cdot10-22 W/m2 Hz contain 10 times more energy than the total energy of all short tracks with a flux of 10\cdot10-22 W/m2 Hz each. Therefore, the radio sources emit the is energy mainly in the form of powerful bursts rather than in the form of numerous weak bursts.

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