AbstractIn this paper, we report the statistical analysis of flare events observed by NoRH during 1992–2005 and NoRP during 1994–2005. We give the power law indices for the frequency distribution of peak brightness temperature which is 1.87±0.05 for 17GHz observation and is 1.64±0.04 for 34GHz observation. We also present the frequency variation of power law indices for peak flux and total energy of flare for NoRP observation, which is mono-increasing from 1 to 17GHz.
A tentative statistical analysis of flare events observed by NoRH and NoRP
Advances in Space Research ; 41 , 8 ; 1188-1190
2007-08-30
3 pages
Article (Journal)
Electronic Resource
English
A tentative statistical analysis of flare events observed by NoRH and NoRP
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