Chinese Physics C > 1996, Vol. 20 > Issue(12): 1068-1072

A Model for Enhancement of the Flux of Very High EnergyParticles During Large Solar Flares

Huo Anxiang^,,
Kuang Haohuai

Institute of High Enigh Physics,The Chinese Academy of Sciences,Beijing 100039

Abstract
HTML
Reference
Related

PDF

Abstract：
In recent years,some short time enhancements of cosmic ray paticles during large solar flares(GLE)were recorded by neutron monitor at sea level and underground muon detector at different depths.The energy regions concerned were in several hundred GeV,even in few TeV.It is disccused in this paper,that the flux enhancemengt in TeV region may be due to the re-acceleration of the galactic cosmic rays in the period of large solar flares.Because of the very steep energy spectrum of cosmic rays,if only 10% cosmic ray paticles are re-accelerated with energy increment of several hundred GeV,the cosmic ray flux in TeV region could increase considerably.

References

[1]	T.Kono,22nd ICRC,3（IWI）125.[2] Filippov,A.T.et al.,22nd ICRC3（1991）113.[3] Alexeyev,EN,Karpov,S.N,23rd ICRC3（1993）167.[4] Kolomeets,E.V et al,24th ICRC4（IWS）240[5] 霍安祥、戴义方、袁余奎，高能物理与核物理，14（1990）862.[6] M.Amenomori,Z.Cao et al,Phys Rev.Letlers,68（1992）2488.

[1]	WANG Gang,Declan Keane,Aihong Tang,Sergei A. A Method for Measuring Event-by-Event Elliptic Flow Fluctuations with the First-Order Event Plane in Heavy-Ion Collisions. Chinese Physics C, 2007, 31(12): 1165-1169.
[2]	ZHAO Xiao-Yan,ZHENG Jian-Hua,WANG Yi-Fang,ZHAO Zhi-Zheng,ZU Kai-Ling. A New Detecting System of the Beam Profile. Chinese Physics C, 2004, 28(11): 1184-1187.
[3]	PAN Feng. An Extended Pairing Model and Its Applications to Well-Deformed Nuclei. Chinese Physics C, 2004, 28(12): 1370-1372.
[4]	WANG Rui-Guang,YU Zhong-Qiang,DING Lin-Kai,MA Yu-Qian,ZHU Qing-Qi. Estimation of the Flux Upper Limit for a Solar Energetic Proton Beam. Chinese Physics C, 2004, 28(10): 1017-1020.
[5]	MA Xin-Hua,ZHOU Xun-Xiu,WU Mei,ZHU Qing-Qi. Very High Energy Gamma Rays from Gamma Ray Bursts. Chinese Physics C, 2003, 27(11): 973-977.
[6]	PENG Hong-An,DUAN Chun-Gui,YAN Zhan-Yuan,HE Zhen-Min. An Alternative Mechanism of Glueball Production in the J/ψ Radiative Decays. Chinese Physics C, 2002, 26(8): 747-752.
[7]	ZHANG JiLong,BAO KeZhi,DING LinKai,Cai Dong,DAI BenZhong,FENG ZhenYong,FU Yu,GUO HongWei,HE Mao,HUANG Qing,HUO AnXiang,JIA HuanYu,,,,,. An Observation of Solar Flare Neutrons Using Yangbajing Solar Cosmic Ray Detector. Chinese Physics C, 2000, 24(12): 1081-1087.
[8]	Liang Zuotang. Spin Effects and High Energy Reaction Mechanisms. Chinese Physics C, 1999, 23(2): 195-198.
[9]	Peng Zhaoran,Li Jing,Ma Xinhua,Wang Wei,Zhu Qingqi,Shen Changquan,Jing Cailiu,Deng Yuju,Yuan Yukui,Huo Anxiang. A Very High Energy GLE Event Possibly Associated With the X Solar Flare of 15th June 1991. Chinese Physics C, 1999, 23(11): 1033-1038.
[10]	Zhang Li,Dai Benzhong,Mu Jun. Solar Flares and Solar High Energy Particles. Chinese Physics C, 1996, 20(10): 877-884.
[11]	Jia Huanyu,Cao Zhen,Zhang Huimin. The Study of Meteorological Effects on TeV Cosmic Ray Flux. Chinese Physics C, 1994, 18(9): 788-793.
[12]	SHENG Hong,HE Guo-Zhu. An Interpretation of Sub-Barrier Fusion Reaction Based on α Transfer Mechanism. Chinese Physics C, 1993, 17(2): 161-165.
[13]	HUO An-Xiang,DAI Yi-Fang,YUAN Yu-Kui. VERY HIGH-ENERGY PARTICLE EMISSION FROM THE SOLAR COSMIC RAY FLARES. Chinese Physics C, 1990, 14(9): 862-864.
[14]	XIE Qu-Bing,LIU Xi-Ming. THE YIELDS OF FINAL PARTICLES IN HIGH ENERGY HADRON REACTION. Chinese Physics C, 1987, 11(4): 476-482.
[15]	YANG Xin-E. THE COMPOSITE MODEL OF LEPTON AND QUARK WITH ONLY ONE CONSTITUENT SCALAR. Chinese Physics C, 1985, 9(5): 537-541.
[16]	XU Shu-Wei,WU Guo-Hua,MIAO Rong-Zhi,HAN Fei. A PROBABLE NEW TYPE OF REACTION MECHANISM —DOUBLE α DIRECT TRANSFER PROCESS. Chinese Physics C, 1983, 7(2): 217-222.
[17]	Wei Kai-yu,Lin Zhen-hua. A COMPUTATIONAL METHOD FOR THE DESIGN ENERGY HIGH INTENSITY BEAM TRANSPORT SYSTEMS. Chinese Physics C, 1980, 4(5): 555-562.
[18]	XU SHU-WEI. A PHENOMENOLOGICAL NUCLEAR FRICTION MECHANISM IN HEAVY ION REACTIONS. Chinese Physics C, 1979, 3(6): 769-771.
[19]	WANG CHENG-CHIH. ON MESON RATIOS IN MULTIPARTICLE PRODUCTION AT HIGH ENERGY——A STATISTICAL QUARK MODEL. Chinese Physics C, 1979, 3(1): 122-126.
[20]	WU YONG-SHI,LEE HWA-CHUNG,KUO SHUO-HUNG,HSEEN TING-CHANG. ON A PSEUDO-PARTICLE SOLUTION OF THE YANG-MILLS FIELD. Chinese Physics C, 1978, 2(4): 371-373.

Access

Get Citation

Huo Anxiang and Kuang Haohuai. A Model for Enhancement of the Flux of Very High EnergyParticles During Large Solar Flares[J]. Chinese Physics C, 1996, 20(12): 1068-1072.

Huo Anxiang and Kuang Haohuai. A Model for Enhancement of the Flux of Very High EnergyParticles During Large Solar Flares[J]. Chinese Physics C, 1996, 20(12): 1068-1072. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 1900-01-01
Revised: 1900-01-01

Article Metric

Article Views(5177)
PDF Downloads(522)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者:陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

A Model for Enhancement of the Flux of Very High EnergyParticles During Large Solar Flares

Huo Anxiang^,
Kuang Haohuai

Corresponding author:Huo Anxiang,

Institute of High Enigh Physics,The Chinese Academy of Sciences,Beijing 100039

Received Date:1900-01-01
Accepted Date:1900-01-01
Available Online:1996-12-05

Abstract:In recent years,some short time enhancements of cosmic ray paticles during large solar flares(GLE)were recorded by neutron monitor at sea level and underground muon detector at different depths.The energy regions concerned were in several hundred GeV,even in few TeV.It is disccused in this paper,that the flux enhancemengt in TeV region may be due to the re-acceleration of the galactic cosmic rays in the period of large solar flares.Because of the very steep energy spectrum of cosmic rays,if only 10% cosmic ray paticles are re-accelerated with energy increment of several hundred GeV,the cosmic ray flux in TeV region could increase considerably.