Chinese Physics C > 1984, Vol. 8 > Issue(4): 502-507

A SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10¹⁴TO 5×10¹⁶eV

SUN Luo-Rui^,

Zhengzhou University

Abstract
HTML
Reference
Related

PDF

Abstract：
Energy spectrum of cosmic rays ranging from 6×10 ¹⁴to 5×10 ¹⁶eV is studied. The work is done automatically by employing a computer as well as fast and efficient electronics. The results of the experiment show that: The integral spectrum of the primary cosmic rays can be represented as I= K.(E/E ₀) ^－γThe value of γ is changed from 1.15±0.04 to 1.19±0.08 at energy around 3×10 ¹⁵eV.

References

[1]

P. Bassi, G. Clark, and B. Rossi, Phys. Rev., 92 (1953), 441.[2] G. Clark, H. Bradt, and M. La Pointe, Proc. 8th Int. Cosmic Ray Conf., Jaipur 4 (1963), 65.[3] C. B. A. McCuslcer, Proc. 8th Int. Cosmic ray Conf., Jaipur 4 (1963), 35.[4] S. Hayakawa, Cosmic Ray Physics, Wiley-Interscience (1969). ,[5] Ph. Catz et al., Proc. 14th Int. Cosmic Rag Conf., Munich 12 (1975),4329.[6] F. Ashton et al., Proc. 16th Tnt. Cosmic Ray Conf., Kyoto 13 (1979),243.[7] P. C. Crouch et al., Nucl. Instr. and Meth., 179(1981), 467.[8] C. B. A. McCusker and M. M. Winn, Nucl. Phys., 5(1979), 159.

[1]	RUAN Xi-Chao,ZHOU Zu-Ying,CHEN Guo-Chang,QI Bu-Jia,LI Xia,HUANG Han-Xiong,ZHONG Qi-Ping,TANG Hong-Qing,JIANG Jing,XIN Biao,BAO Jie,CHEN Lin,ZHANG Jing-Shang. Measurements of Neutron Emission Spectra for Neutron Induced Reactions on⁹Be and^6,7Li. Chinese Physics C, 2007, 31(5): 442-447.
[2]	XIE Wan,OUYANG Qun,XIE Yi-Gang,ZHENG Shu-Cheng,HAN Hong-Guang,CHENG Shao-Chen,YANG Yi. Performance Study of Monitored Drift Tube Chambers with Cosmic Rays. Chinese Physics C, 2007, 31(11): 1056-1061.
[3]	LU Xiao,LIU Guang-Dong,SHEN Peng-Nian. Study about the Binding Energy of Light Double Hypernuclei ^6_ΛΛHe,^5_ΛΛHe,^5_ΛΛH,^4_ΛΛHe,and ^4_ΛΛH Based on Chiral SU(3) Quark Model. Chinese Physics C, 2006, 30(11): 1074-1077.
[4]	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.
[5]	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.
[6]	JIA Huan-Yu,WANG Shun-Jin. Study of the Time Variation of 10TeV Cosmic Ray. Chinese Physics C, 2001, 25(4): 277-282.
[7]	Gu Jianhui,Yu Zhongqiang. Muon Sample Selection from Cosmic Ray Events for BES. Chinese Physics C, 1996, 20(1): 26-31.
[8]	Li Xungui. The Ground State Energy of the Hypernucleus Λ6Li. Chinese Physics C, 1994, 18(1): 81-84.
[9]	CHEN Feng-Zhi,NIE Chuan-Hui,WANG Ping. The Source of Anomalous Positrons in the Cosmic Rays Above 10GeV. Chinese Physics C, 1991, 15(6): 504-509.
[10]	CAO Yu-Fang,PAN Feng,PAN Zhen-Yong. SOME ISOSCALAR FACTORS FOR THE GROUP CHAINSO(6)SO(5). Chinese Physics C, 1988, 12(1): 123-129.
[11]	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.
[12]	JIANG Yin-Lin,YUAN Yu-Kui,LI Yan-Guo,CHEN Duan-Bao,ZHENG Rong-Ting,SONG Jian-Ning. RESEARCH FOR THE POSSIBILITY ON DETECTING COSMIC RAY PARTICLES BY ACOUSTIC WAY. Chinese Physics C, 1986, 10(1): 9-14.
[13]	WANG Yun-Xin. ENERGY SPECTRUM OF SUPER HIGH ENERGY COSMIC RAY MUON SHOWERS OF LARGE ZENITH ANGLES. Chinese Physics C, 1986, 10(2): 245-248.
[14]	HE Yu-Dong,ZHOU Wen-De,HE Ren-Dao,MU Jun,DING Lin-Kai,ZHU Qing-Qi,JING Cai-Liu,JING Gui-Ru. AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER. Chinese Physics C, 1986, 10(6): 641-646.
[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]	ZHU Pei-Yu,CAO Yu-Fang,WU You-Shi.U(5) LIMIT OFU(6/20) SUPERSYMMETRY IN NUCLEI. Chinese Physics C, 1985, 9(4): 405-411.
[17]	XU Chun-Xian. THE ANISOTROPY OF COSMIC RAY PARTICLES IN THE ENERGY RANGE 10¹¹—10¹⁹eV. Chinese Physics C, 1985, 9(4): 385-390.
[18]	CHEN Ying-Xuan,HE Chang-Xiao,XIAO Qian-Yi,WANG Li-Xiang. THE TIME DISTRIBUTION OF EAS WITHE>10¹⁴eV. Chinese Physics C, 1985, 9(4): 391-396.
[19]	JING Cai-Liu,JING Gui-Ru,DING Lin-Kai,ZHU Qing-Qi. ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV. Chinese Physics C, 1985, 9(2): 134-141.
[20]	DING LIN-KAI,ZHU QING-QI,GUO KE-ZHUN. CLUSTER PHENOMENA OBSERVED IN EMULSION CHAMBER EXPERIMENTS IN ENERGY REGION OF 10¹⁵—10¹⁶eV AND HADRON JETS WITH LARGE TRANSVERSE MOMENTA. Chinese Physics C, 1982, 6(6): 657-664.

Access

Get Citation

SUN Luo-Rui. A SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10 ¹⁴TO 5×10 ¹⁶eV[J]. Chinese Physics C, 1984, 8(4): 502-507.

SUN Luo-Rui. A SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10 ¹⁴TO 5×10 ¹⁶eV[J]. Chinese Physics C, 1984, 8(4): 502-507. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Article Metric

Article Views(5015)
PDF Downloads(416)
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 SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10¹⁴TO 5×10¹⁶eV

SUN Luo-Rui^,

Corresponding author:SUN Luo-Rui,

Zhengzhou University

Received Date:1900-01-01
Accepted Date:1900-01-01
Available Online:1984-06-05

Abstract:Energy spectrum of cosmic rays ranging from 6×10¹⁴to 5×10¹⁶eV is studied. The work is done automatically by employing a computer as well as fast and efficient electronics. The results of the experiment show that: The integral spectrum of the primary cosmic rays can be represented asI=K.(E/E₀)^－γThe value of γ is changed from 1.15±0.04 to 1.19±0.08 at energy around 3×10¹⁵eV.