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

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《中国物理C》（英文）编辑部

2024年10月30日

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

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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.