AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10<SUP>14</SUP>eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER

HE Yu-Dong; ZHOU Wen-De; HE Ren-Dao; MU Jun; DING Lin-Kai; ZHU Qing-Qi; JING Cai-Liu; JING Gui-Ru

Chinese Physics C> 1986, Vol. 10> Issue(6) : 641-646

AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER

Abstract
HTML
Reference
Related

PDF

Abstract：
The characteristics of electromagnetic and hadronic components in high energy cosmic rays at mountain altitude are studied by analysing single-shower events observed by mountain emulsion chamber. The chemical composition of primary cosmic rays in the energy region around 10¹⁴eV is studied by using Monte-Carlo simulation. The simulated power indices of energy spectra and attenuation lengths in air in agreement with the experimental data. The analysis of their vertical intensities indicates that the chemical composition of primary cosmic rays at energies around 10¹⁴eV is not contradicted to the simple extrapolation from lower energies and the abundance of protons can not be less than 30% and that of the nuclei with A≥2 not larger than 70%.

References

[1]

例如 A. M. Hillas, Proceedings of Cosmic Ray Workshop, University of Utah, 1983, P. 1.[2] Wang. C. R et al., 17 th ICRC, 5 (1981), 251.[3] 霍安祥等, 高能物理与核物理, 6 (1982), 778.[4] Ren. J. R et al., 18 th ICRC,5 (1983), 285.[5] 曹培园等, 第四届全国宇宙线会议论文(重庆建工学院学报, 1985年增刊, p.105).[6] 木钧等, 云南大学学报, 7 (1985), 289.[7] Ren. J. R et al., 19 th ICRC, 5(1985), 204.[8] 张春生等, 高能物理与核物理, 9 (1985), 649.[9] 例如,A. G. Ekspong, CERN-EP/84-43, (1984); J. G. Rushbrooke, CERN-EP/85-124, (1985) 及其有关引文.[10] 丁林惶等, 科学通报, (待发表).[11] 任敬儒等, 高能物理与核物理, 5 (1981), 205.[12] 和煌东等, 云南大学学报, (待发表).[13] L. W. Jones, 18 th ICRC, 5 (1983), 17.[14] T. K. Gaisser et al., 18 th ICRC, 5 (1983), 174.[15] 例如 M. A. Faessler, CERN-EP/84-64, (1984).[16] 丁林恺等, 高能物理与核物理, 7 (1983),129.[17] 经才骆等, 高能物理与核物理, 10 (1986), 636.

[1]	LAN Xiao-Gang , HOU Yan , ZHOU Xun-Xiu , JIA Huan-Yu , CAO Zhen , DING Lin-Kai . Study of p-Air Inelastic Cross Section with Directly Arrived Protons at Yangbajing. Chinese Physics C, 2007, 31(6): 513-517.
[2]	YANG Hong-Tao , LIU Jun , GENG Qing-Xi , LIU Chang-Qin , ZHANG Pin , GAO Xiao-Yu , ZHA Min , JING Gui-Ru , JING Cai-Liu , ZHU Qing-Qi , Cheung T , Leung K , NG L . The Study of Primary Cosmic Ray Mass Composition Around the. Chinese Physics C, 2006, 30(6): 497-500.
[3]	LI Li , ZHANG Feng , WANG Rui-Guang , CHEN He-Sheng , MA Yu-Qian . Track Finding of Cosmic Multi-muon Events in the L3+C Muon Detector. Chinese Physics C, 2004, 28(7): 749-752.
[4]	WANG Kong-Sen , WANG He , HUANG Xing-Tao , MA Lian-Liang , MA Li-Na , WANG Yong-Gang , XUE Liang , FENG Cun-Feng , ZHANG Xue-Yao , LI Jin-Yu , ZHANG Nai-Jian , HE Mao , WANG Cheng- , , . Study on the Production Characteristics of Cosmic Ray High Energy Family Events with Simulation and Experiment. Chinese Physics C, 2004, 28(3): 232-238.
[5]	LIU Jun , GENG Qing-Xi , YANG Hong-Tao , LIU Chang-Qin , ZHANG Pin , GAO Xiao-Yu , JING Cai-Liu , ZHA Min , JING Gui-Ru , ZHU Qing-Qi , Cheung T , Ng L . Study of EAS Local Muon Density Spectrum and the Knee in the Energy Spectrum of Primary Cosmic Rays. Chinese Physics C, 2003, 27(2): 109-112.
[6]	FENG Gun-Feng , ZHANG Xue-Yao , WANG Yong-Gang , XUE Liang , MA Li-Na , LI Jin-Yu , ZHANG Nai-Jian . Identification of Primary Y-Rays by the Characteristics of Time-Space Structure of the Cosmic-Ray Air Showers. Chinese Physics C, 2003, 27(11): 969-972.
[7]	WANG He , WANG Yong-Gang , DAI Zhi-Qiang , XUE Liang , FENG Cun-Feng , ZHANG Xue-Yao , LI Jin-Yu , ZHANG Nai-Jian , HE Mao , WANG Cheng-Rui , REN Jing-Ru , LU Sui-Ling . Lateral Distribution of Shower Particles in High Energy Family Events of Cosmic Rays. Chinese Physics C, 2003, 27(4): 299-303.
[8]	WANG Yong-Gang , XUE Liang , FENG Cun-Feng , FU Yu , LI Jie , ZHANG Xue-Yao , LI Jin-Yu , ZHANG Nai-Jian , HE Mao , WANG Cheng-Rui , REN Jing-Ru , LU Sui-Ling . Adjustment of Parameters of Primary Cosmic Ray Energy Spectrum with Recent Direct Measurments. Chinese Physics C, 2002, 26(2): 108-115.
[9]	XUE Liang , DAI ZhiQiang , LI Jinyu , ZHANG Xueyao , FENG CunFeng , FU Yu , ZHANG NaiJian , REN JingRu , LU SuiLing . Phenomenon of Alignment in Cosmic Ray High Energy Family Events. Chinese Physics C, 2000, 24(11): 979-984.
[10]	Ding Linkal , Zhu Qingqi , Shen Changquan , Yao Zhiguo , Cheung Tsang , Matti Vallinkoski . An Approach to Study the Cosmic Ray ‘Knee’Composition From Underground Multimuon Events at a Shallower Depth. Chinese Physics C, 1999, 23(6): 584-588.
[11]	Luo Guangxuan , Tan Youheng , Zhang Chunsheng , Dong Yuju , Yuan Peng , Zhang Huimin , Wang Hui , Yuan Yukui , Li Jing . Primary Energy Spectrum of Cosmic Ray at the. Chinese Physics C, 1995, 19(9): 769-774.
[12]	CAI Xu , ZHOU Dai-Cui , QIAN Wan-Yan , LUO Lai-Qi . A HIGH MULTIPLICITY COSMIC PAY EVENT OBSERVED IN CHINESE SATELLITE EMULSION. Chinese Physics C, 1988, 12(2): 150-154.
[13]	XU Ke-Zun , ZHANG Zhen-Hua , TANG Zi-Zhou , WANG Ming-Qian . MEASUREMENT OF THE ENERGY SPECTRUM OF PRIMARY COSMIC PAYS. Chinese Physics C, 1987, 11(1): 1-5.
[14]	ZOU Bao-Tang , WANG Cheng-Rui , REN Jing-Ru . A COSMIC RAY SUPER HIGH ENERGY MULTIJET FAMILY EVENT. Chinese Physics C, 1986, 10(4): 393-399.
[15]	JING Cai-Liu , DING Lin-Kai , ZHU QiNG-Qi , JING Gui-Ru . A DEDUCTION ON PRIMARY COSMIC PAY COMPOSITION AND SPECTRA ABOVE 10¹⁴eV. Chinese Physics C, 1986, 10(5): 636-640.
[16]	XU Chun-Xian . THE ANISOTROPY OF COSMIC RAY PARTICLES IN THE ENERGY RANGE 10¹¹—10¹⁹eV. Chinese Physics C, 1985, 9(4): 385-390.
[17]	LU Chang-Guo , LU Wei-Da , ZHOU Yue-Hua , ZHANG Yu , GU Wei-Xin . TESTING RESULTS ON THE PROTOTYPE OF SHOWER COUNTER WITH COSMIC RAYS. Chinese Physics C, 1985, 9(4): 397-404.
[18]	CHANG KONG-LIANG . DIMENSIONAL METHOD TO SOLVE THE DIFFUSION CONVECTION EQUATION OF SOLAR COSMIC RAYS. Chinese Physics C, 1978, 2(3): 200-210.
[19]	LUO LIAU-FU , LU TAN . HIGH SPIN MESONS AND UNEXPLAINED MULTIPHOTON PHENOMENA. Chinese Physics C, 1978, 2(6): 562-565.
[20]	YUAN YU-KUI , HUO AN-XIANG , ZHANG CHANG-CHUN , QIN KE-YU , ZHU AI-MIN , ZHANG REN-QING , GUO KE-ZUN , YANG CHANG-TOU , LI QIN-LIAN , FAN SHI-HE . PRELIMINARY MEASUREMENT OF THE ANTIPROTON COMPONENT IN COSMIC RAYS AT A 3220m ALTITUDE. Chinese Physics C, 1978, 2(5): 478-480.

Access

Get Citation

HE Yu-Dong, ZHOU Wen-De, HE Ren-Dao, MU Jun, DING Lin-Kai, ZHU Qing-Qi, JING Cai-Liu and JING Gui-Ru. AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER[J]. Chinese Physics C, 1986, 10(6): 641-646.

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Article Metric

Article Views(2123)
PDF Downloads(392)
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

AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER

Corresponding author: HE Yu-Dong,

Received Date: 1900-01-01

Accepted Date: 1900-01-01

Available Online: 1986-12-05

Abstract: The characteristics of electromagnetic and hadronic components in high energy cosmic rays at mountain altitude are studied by analysing single-shower events observed by mountain emulsion chamber. The chemical composition of primary cosmic rays in the energy region around 10¹⁴eV is studied by using Monte-Carlo simulation. The simulated power indices of energy spectra and attenuation lengths in air in agreement with the experimental data. The analysis of their vertical intensities indicates that the chemical composition of primary cosmic rays at energies around 10¹⁴eV is not contradicted to the simple extrapolation from lower energies and the abundance of protons can not be less than 30% and that of the nuclei with A≥2 not larger than 70%.

HTML

Reference (1)

AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER

Corresponding author: HE Yu-Dong,

HTML

目录

AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 1014eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 1014eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER

Corresponding author: HE Yu-Dong,

HTML

目录

AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER

AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER