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Abstract:
The method and arrangement determining the energy spectrum of primary cosmic rays by measuring the Cerenkov radiation were described. The integral power index γ=1.80±0.11 of energy spectrum of primary cosmic rays wa measured at the energy range of 2.9×1014-4.0×1015eV.
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References
[1]
|
W. Galbraith J. V. Jelley, J.Atmos. Terres. Phys. 6(1955), 250.[2] D. H. Hartman et al, Nuovo Cimersto, 51A(1979), 131.[3] V. I. Zatsepin A. E. Chudakov, Soviet Phys. JETP, 15(1962), 1176.[4] Giler et al., Proc. 13th ICCR, 3(1973), 2366.[5] Anderson et al., Bri. Jour. A. Phys. 5(1953).[6] G. Clark et al., Proc. of ICCR, 4(1963), 65.[7] Efimov, Proc. 16th ICCR, 8(1979), 154.[8] G. T. Zatsepin et al., Proc.of ICCR, 4(1963), 100.[9] C. Gerders et al., Proc. 13th ICCR, 3(1973), 219. |
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[1] |
GUO Yun-Jun
, HE Kang-Lin
. Muon Identification Using the Efficiencies Ratio Method at BESⅡ. Chinese Physics C,
2007, 31(11): 1050-1055. |
[2] |
PENG Quan-Ling
, SUN Jian
, ZHAO Guang-Yuan
, SHI Cai-Tu
. Principle and Software Design of Helmhotz Coil Measurement System. Chinese Physics C,
2001, 25(9): 920-925. |
[3] |
CHANG KONG-LIANG
. DIMENSIONAL METHOD TO SOLVE THE DIFFUSION CONVECTION EQUATION OF SOLAR COSMIC RAYS. Chinese Physics C,
1978, 2(3): 200-210. |
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