28 October 2003 flare: High-energy gamma emission, type II radio emission and solar particle observations

被引：10
|
作者：
Kuznetsov, SN [1 ]
Kurt, VG
Yushkov, BY
Myagkova, IN
Kudela, K
Belov, AV
Caroubalos, C
Hilaris, A
Mavromichalaki, H
Moussas, X
Preka-Papadema, P
机构：
[1] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119992, Russia
[2] Slovak Acad Sci, Inst Expt Phys, SK-04353 Kosice, Slovakia
[3] Russian Acad Sci, Inst Terr Magnetism Ionosphere & Radio Wave P, Troitsk 142092, Moscow Region, Russia
[4] Univ Athens, Dept Phys, Athens 15571, Greece
来源：
INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 2005年 / 20卷 / 29期
关键词：
solar flare; gamma-ray emission; solar energetic particles; GLE; shock wave;
D O I：
10.1142/S0217751X05029873
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
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.
引用
收藏
页码：6705 / 6707
页数：3
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