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Simulation of a CME-driven shock by anisotropic scattering angular distributions

Published online by Cambridge University Press:  18 July 2013

Xin Wang  and
Yi-Hua Yan
Xin Wang
Affiliation:
Key laboratory of Solar Activities, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; email: wangxin@nao.cas.cn; yyh@nao.cas.cn State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing 100080, China;
Yi-Hua Yan
Affiliation:
Key laboratory of Solar Activities, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; email: wangxin@nao.cas.cn; yyh@nao.cas.cn
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Abstract

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Observations of the interplanetary shock provide us with strong evidences of particle acceleration to multi-MeV protons in a coronal mass ejection (CME). Diffusive shock acceleration (DSA) is an efficient mechanism for cosmic ray (CR). This work presents a dynamical Monte Carlo simulation of a CME-driven shock on 14-Dec-2006 by using a series of Gaussian scattering angular distributions. With the simulated results, we find that particle energy spectrum is affected by energy injection processes under the anisotropic scattering law.

Keywords

acceleration of particlesshock wavesSun: coronal mass ejections (CMEs)solar windmethods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 583 - 584
Copyright
Copyright © International Astronomical Union 2013 

References

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