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) | 263 - 266 | |
Section | Energetic Particles, Flares and High Energy Emission | |
DOI | https://doi.org/10.1051/eas/1255037 | |
Published online | 27 June 2012 |
M. Faurobert, C. Fang and T. Corbard (eds)
EAS Publications Series, 55 (2012) 263-266
Temporal properties of decimetric spikes in solar flares
Key Laboratory of Solar Activity / National Astronomical
Observatories of China, Chinese Academy of Sciences China
e-mail: wsj@nao.cas.cn
An analysis of the temporal properties of a group of spikes in the solar flares is presented recorded by the 1–2 GHz spectrometer of National Astronomical observatories of China (NAOC) on 27 October 2003. The time profile of each single spike was fitted and analyzed. In particular, we determine the e-folding rise and decay times corresponding to the ascending and decaying parts of the time profile, respectively. Several important correlations have studied and compared with the results in earlier literature, i.e. those between duration and frequency, e-folding rise time and decay time, e-folding decay time and duration, and e-folding decay time and peak flux. Plasma temperatures of source region are also estimated and the possible decaying mechanism is discussed.
© EAS, EDP Sciences 2012