The energy flux density of radio bursts from solar radio bursts is studied by statistical analysis of observations in the meter range made with the solar radio telescope at the Abastumani Astrophysical Observatory. A truncated gamma distribution is found to give a better fit to the observational data than a gamma distribution.
CITATION STYLE
Salukvadze, G., Ograpishvili, N., Maghradze, D., Japaridze, D., Mdzinarishvili, T., Chargeishvili, B., … Makandarashvili, S. (2018). Statistical Study of Solar Radio Bursts at a Frequency of 210 MHz. Astrophysics, 61(3), 347–353. https://doi.org/10.1007/s10511-018-9541-x
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