Type II Radio Emission and Solar Particle Observations
classification
🌌 astro-ph.SR
keywords
timeemissionhigh-energyaccelerationbeencomparedependenciesescaping
read the original 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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