THE ENERGY SPECTRA OF COSMIC RAY HADRONS AT MT.KAMBALA 5500m ABOVE SE LEVEL

HUO AN-XIANG; REN JING-RU; LU SUI-LING; KUANG HAO-HUAI; SU SHI; WANG CHENG-RUI; CAO PEI-YUAN; LI JIN-YU

Chinese Physics C> 1982, Vol. 6> Issue(6) : 778-780

THE ENERGY SPECTRA OF COSMIC RAY HADRONS AT MT.KAMBALA 5500m ABOVE SE LEVEL

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Abstract：
The energy spectra of cosmic ray hadrons is studied by use of mountain emulsionchambers installed on Mt. Kambala 5500 m above sea level. The power index. of theenergy spectra is 1.95±0.18 in the energy region from 3 to 50 TeV The verticalflux of hadrons with E_h^γ≥3 TeV is (145±14)/year.m².sr, their attenuation lengthin air is (101±13)g/cm², and mean interaction length in Pb is (187±51)g/cm².

References

[1]	王承瑞等, 17th ICRC, 5(1981), 251.[2] 任敬儒等, 高能物理与核物理, 5(1981), 205,[3] M. T. Fuji Collaboration ICR-Report-89-81-5.[4] Bayburina et al., Nucl. Phys. B191(1981), 28.

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[6]	LU Sui-Ling , REN Jing-Ru , SU Shi , WANG Cheng-Rui , HE Mao . Variation of Intensity of High Energy Cosmic Ray Hadrons with Altitude. Chinese Physics C, 1992, 16(5): 390-391.
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[8]	FAN Xiao-Ling , ZHANG Chun-Sheng . Application of Hadron-Hadron Nuclear Interaction Parametrization Model in the Study of Superhigh Energy Cosmic Rays. Chinese Physics C, 1992, 16(4): 289-296.
[9]	FAN Xiao-Ling , SU Shi , WANG Yi . Cosmic Ray Muon on the Altitude of 5500m Above the Sea Level. Chinese Physics C, 1991, 15(2): 103-110.
[10]	DING Lin-Kai . ON THE INELASTICITY OF SUPERHIGH ENERGY COSMIC RAY INTERACTIONS. Chinese Physics C, 1990, 14(6): 486-489.
[11]	ZHANG Nai-Jian , WANG Cheng-Rui , HE Mao , CAO Pei-Yuan , LI Jin-Yu , ZOU Bao-Tang , WANG Guang-Jun , WEI Chao . HIGH ENERGY HADRONS IN ATMOSPHERIC COSMIC RAYS OBSERVED WITH Fe EMULSION CHAMBERS. Chinese Physics C, 1989, 13(11): 961-966.
[12]	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.
[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.
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[17]	LU Sui-Ling , SU Shi , REN Jing-Ru , WANG Dian-Chen . VARIATION OF THE INTENSITY OF ULTRAHIGH ENERGY γ-RAYS WITH ALTITUDE. Chinese Physics C, 1983, 7(1): 118-120.
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[19]	Shen Chang-quan , Zhu Ai-min , Zhang Ren-qing , Yao Wei-zhong , Xu You-an . MEASUREMENT OF INTENSITY AND MOMENTUM SPECTRUM OF HORIZONTAL COSMIC RAY MUON AT 3220m ABOVE SEA LEVEL. Chinese Physics C, 1980, 4(4): 409-412.
[20]	XU CHUN-XIAN , HUO AN-XIANG , YUAN YN-KUI , GU YI-DONG , LI TI-PEI , SHEN PEI-RO , JIA GUEI-BIN , XIAO QIAN-YI , ZHANG CHENG-MO , CHEN DUAN-BAO . THE NEGATIVE-POSITIVE RATIO OF CHARGED COSMIC RAY HADRONS AT THE 3220 m ABOVE SEA-LEVEL. Chinese Physics C, 1978, 2(5): 423-427.

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HUO AN-XIANG, REN JING-RU, LU SUI-LING, KUANG HAO-HUAI, SU SHI, WANG CHENG-RUI, CAO PEI-YUAN and LI JIN-YU. THE ENERGY SPECTRA OF COSMIC RAY HADRONS AT MT.KAMBALA 5500m ABOVE SE LEVEL[J]. Chinese Physics C, 1982, 6(6): 778-780.

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Received: 1982-07-22
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

THE ENERGY SPECTRA OF COSMIC RAY HADRONS AT MT.KAMBALA 5500m ABOVE SE LEVEL

Received Date: 1982-07-22
Accepted Date: 1900-01-01
Available Online: 1982-12-05

Abstract: The energy spectra of cosmic ray hadrons is studied by use of mountain emulsionchambers installed on Mt. Kambala 5500 m above sea level. The power index. of theenergy spectra is 1.95±0.18 in the energy region from 3 to 50 TeV The verticalflux of hadrons with E_h^γ≥3 TeV is (145±14)/year.m².sr, their attenuation lengthin air is (101±13)g/cm², and mean interaction length in Pb is (187±51)g/cm².