Issue |
EAS Publications Series
Volume 55, 2012
4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges
|
|
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Page(s) | 239 - 243 | |
Section | Energetic Particles, Flares and High Energy Emission | |
DOI | https://doi.org/10.1051/eas/1255033 | |
Published online | 27 June 2012 |
Understanding Solar Activity: Advances and Challenges
M. Faurobert, C. Fang and T. Corbard (eds)
EAS Publications Series, 55 (2012) 239-243
M. Faurobert, C. Fang and T. Corbard (eds)
EAS Publications Series, 55 (2012) 239-243
On the Frequency Distributions of Solar Soft X-ray Flares
Purple Mountain Observatory, Chinese Academy of
Sciences, Nanjing
210008,
China
e-mail: wqgan@pmo.ac.cn
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.
© EAS, EDP Sciences 2012