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Type II Radio Emission and Solar Particle Observations

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arxiv 1009.3646 v1 pith:XAFAWKVD submitted 2010-09-19 astro-ph.SR

S. N. Kuznetsov , V. G. Kurt , B. Yushkov , B. Yu , I. N. Myagkova , K. Kudela , A. V. Belov , C. Caroubalos
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A. Hilaris H. Mavromichalaki X. Moussas P. Preka-Papadema
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classification astro-ph.SR
keywords timeemissionhigh-energyaccelerationbeencomparedependenciesescaping
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The 28 October 2003 flare gave us the unique opportunity to compare the acceleration time of high-energy protons with the escaping time of those particles which have been measured onboard spacecraft and by neutron monitors network as GLE event. High-energy emission time scale and shock wave height and velocity time dependencies were also studied.

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