Type II Radio Emission and Solar Particle Observations
S. N. Kuznetsov, V. G. Kurt, B. Yushkov, B. Yu, I. N. Myagkova, K., Kudela, A. V. Belov, C. Caroubalos, A. Hilaris, H. Mavromichalaki, X., Moussas, P. Preka-Papadema
TL;DR
This paper analyzes the timing and dynamics of solar energetic particles and radio emissions during the 2003 flare, providing insights into particle acceleration and escape processes.
Contribution
It offers a comparative analysis of proton acceleration and escape times, along with shock wave dynamics during a significant solar flare event.
Findings
Correlation between high-energy emission and particle escape times
Shock wave height and velocity profiles during the flare
Insights into particle acceleration mechanisms
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.
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