Type II Radio Emission and Solar Particle Observations

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)

Cited by in corpus (3)

• An Extreme Solar Event of 20 January 2005: Properties of the Flare and the Origin of Energetic Particles
• Anomalous dynamics of the extremely compressed magnetosphere during 21 January 2005 magnetic storm
• New estimation of non-thermal electron energetics in the giant solar flare on 28 October 2003 based on Mars Odyssey observations