Type II Radio Emission and Solar Particle Observations
arXiv:1009.3646 · doi:10.1142/S0217751X05029873
Abstract
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.
International Journal of Modern Physics A, Volume 20, Issue 29, pp. 6705-6707 (2005)