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Automatic detection method, forecast and alert of solar proton events

Published online by Cambridge University Press:  26 February 2010

Ganghua Lin
Ganghua Lin*
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Datun Rd. 20A, Chaoyang District, Beijing, 100012, China email: lgh@bao.ac.cn
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Abstract

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The methods of automatic solar active phenomenon or event detection have been researched and explored by people for many years, which have gone into actual services. The paper analyzes the relationship between these methods of automatic detection and the forecast or alert, using the solar short-term proton events predictions as an example. Using automatic method to conduct forecast or alert is under thinking.

Keywords

Sun: activityparticle emissionmagnetic fieldssolar-terrestrial relationsmethods: data analysisstatistical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 105 - 108
Copyright
Copyright © International Astronomical Union 2010

References

Benkhalil, A., Zharkova, V. V., Zharkov, S., & Ipson, S. 2006, Solar Phys., 235:87–106CrossRefGoogle Scholar
Curto, J. J., Blanca, M., & Martinez, E. 2008, Solar Phys., 250:411–429CrossRefGoogle Scholar
Ming, Qu, Frank, Y. Shih, Ju, Jing, & Haimin, Wang 2003, Solar Phys, 217:157–172Google Scholar
Wang, Jialong 1999, Chinese Journal of Astronomy and Astrophysics, 19, 4, 412:418Google Scholar