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On the Frequency Distributions of Solar Soft X-ray Flares

Published online by Cambridge University Press:  27 June 2012

M. Faurobert ,
C. Fang ,
T. Corbard ,
W.Q. Gan ,
Y.P. Li  and
L. Feng
W.Q. Gan
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China. e-mail: [email protected]
Y.P. Li
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China. e-mail: [email protected]
L. Feng
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China. e-mail: [email protected]
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Abstract

By giving three different definitions of peak flux(original peak flux, corrected peak flux, and scaled peak flux), we analyze the frequency distributions of 14057 flares recorded by GOES from 2000 to 2005. We find a significant result that the frequency distribution of the scaled peak flux for all the sample flares can be approximated by a perfect power-law function with an index of 2.18, without any usually deviating from the power-law at the lower fluxes.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 55: 4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges , 2012 , pp. 239 - 243
Copyright
© EAS, EDP Sciences 2012

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