Type II Radio Emission and Solar Particle Observations

Details Type II Radio Emission and Solar Particle Observations Type II Radio Emission and Solar Particle Observations

2010-09-19

arxiv.org/abs/1009.3646v1

2005IJMPA..20.6705K

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

International Journal of Modern Physics A, Volume 20, Issue 29, pp. 6705-6707 (2005)

Scientific paper

10.1142/S0217751X05029873

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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