Type II Radio Emission and Solar Particle Observations

Authors :: Kuznetsov, S. N.
Kurt, V. G.
Yushkov, B.
Yu, B.
Myagkova, I. N.
Kudela, K.
Belov, A. V.
Caroubalos, C.
Hilaris, A.
Mavromichalaki, H.
Moussas, X.
Preka-Papadema, P.
Source :: 2005IJMPA..20.6705K
Publication Year :: 2010
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.<br />Comment: International Journal of Modern Physics A, Volume 20, Issue 29, pp. 6705-6707 (2005)