Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-05T16:44:25.134Z Has data issue: false hasContentIssue false
  • English
  • Français

An intelligent method for solar flare observation

Published online by Cambridge University Press:  18 July 2013

Jia Ben Lin ,
Juan Guo  and
Yuan Yong Deng
Jia Ben Lin*
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, CAS
Juan Guo
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, CAS
Yuan Yong Deng
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, CAS
*
email: jiabenlin@bao.ac.cn
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

To capture the fine structure of the flare kernel during it's explosive phase, we design a real time flare onset detecting algorithm named Near Saturation Area Threshold(NSAT), And an automatic CCD parameters control algorithm for the observing software. All the data from CCD, 48f/s, could be saved to the hard disk, and the GPS time of the flare onset also be saved in the log. These methods could avoid the data overflow and grab the fine structure data of the flare kernel. The simulation experiment works well and the software will be put into use in Huairou Solar Observatory soon.

Keywords

flareintelligentdetectionautomatic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 503 - 504
Copyright
Copyright © International Astronomical Union 2013 

References

Wang, H et al. 2000, ApJ, 1080, 1087, 542 Google Scholar
Ji, H. S. et al. 2004, ApJ, 938, 605 Google Scholar
Hu, X. H. 2007, National astronomical observatory doctoral dissertation Google Scholar
Veronig, A., Stenegger, M. 2000, ESA SP-463 Google Scholar
Temmer, M. 2001, Hvar Obs. Bull., 185, 194 Google Scholar
Borda, D. Mininni 2002, Solar Physics, 347, 357, 206 Google Scholar
Qu, M. et al. 2004, Solar Physics, 5137, 149, 222 Google Scholar