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Type II Radio Emission and Solar Particle Observations View all abstracts by submitter

Alexander Hillaris   Submitted: 2014-06-10 13:59

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.

Authors: Kuznetsov, S. N.; Kurt, V. G.; Yushkov, B. Yu.; Myagkova, I. N.; Kudela, K.; Belov, A. V.; Caroubalos, C.; Hilaris, A.; Mavromichalaki, H.; Moussas, X.; Preka-Papadema, P.
Projects: None

Publication Status: International Journal of Modern Physics A, Volume 20, Issue 29, pp. 6705-6707 (2005).
Last Modified: 2014-06-11 09:54
Go to main E-Print page  Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks  ARTEMIS IV Radio Observations of the 14 July 2000 Large Solar Event  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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