A SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10<SUP>14</SUP> TO 5×10<SUP>16</SUP>eV

SUN Luo-Rui

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

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

SUN Luo-Rui ^,

Zhengzhou University

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Abstract：
Energy spectrum of cosmic rays ranging from 6×10¹⁴ to 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 as I=K.(E/E₀)^－γ The value of γ is changed from 1.15±0.04 to 1.19±0.08 at energy around 3×10¹⁵eV.

References

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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.

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SUN Luo-Rui. A SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10¹⁴ TO 5×10¹⁶eV[J]. Chinese Physics C, 1984, 8(4): 502-507.

SUN Luo-Rui. A SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10¹⁴ TO 5×10¹⁶eV[J]. Chinese Physics C, 1984, 8(4): 502-507. shu

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Received: 1900-01-01
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

A SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10¹⁴ TO 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 6×10¹⁴ to 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 as I=K.(E/E₀)^－γ The value of γ is changed from 1.15±0.04 to 1.19±0.08 at energy around 3×10¹⁵eV.