A DEDUCTION ON PRIMARY COSMIC PAY COMPOSITION AND SPECTRA ABOVE 10<SUP>14</SUP>eV

JING Cai-Liu; DING Lin-Kai; ZHU QiNG-Qi; JING Gui-Ru

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《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 1986, Vol. 10> Issue(5) : 636-640

A DEDUCTION ON PRIMARY COSMIC PAY COMPOSITION AND SPECTRA ABOVE 10¹⁴eV

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Abstract：
The spectra of primary cosmic ray nuclei are fitted from experimental data under 10¹⁴eV and extrapolated to their bending energies. The primary cosmic ray composition above 10¹⁴eV is deduced according to the rigidity cut off model by selecting an appropriate bending energy for proton so that the sum of various nucleus components is consistent with the experimental total particle spectrum. The method used is independent on the behaviour of hadronic interaction.

References

[1]

A. M. Hillas Proc. of the Cosmic Ray Workshop, Uni. of Utah (1983) 1.[2] J. P.W efel Proc. of the Cosmic Ray Workshop, Uni. of Z.Jtah (1983), 188.[3] R. K.Sood, Nature 301(1983), 44.[4] M.Siman et al., Astrophys. J., 239(1980), 712.[5] JACEE Collaboration Proc. of Inter. Symp. on Cosmic Rays and Particles Phys. Tokyo, (1984).468.[6] W. R. Webber in Composition and Origin of Cosmic Rays D. Reidel Publishing Company, Dordrecht, (1983).[7] M. Anienomori et al. Proc, of Inter. Symp.on Cosmic Rays and Particles Phys. Tokyo, (1984),494.[8] N. Nagano et al., J. Phys. G: Nucl. Phys., 10(1984), 1295.

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JING Cai-Liu, DING Lin-Kai, ZHU QiNG-Qi and JING Gui-Ru. A DEDUCTION ON PRIMARY COSMIC PAY COMPOSITION AND SPECTRA ABOVE 10¹⁴eV[J]. Chinese Physics C, 1986, 10(5): 636-640.

JING Cai-Liu, DING Lin-Kai, ZHU QiNG-Qi and JING Gui-Ru. A DEDUCTION ON PRIMARY COSMIC PAY COMPOSITION AND SPECTRA ABOVE 10¹⁴eV[J]. Chinese Physics C, 1986, 10(5): 636-640. shu

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

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1.
沈阳化工大学材料科学与工程学院沈阳 110142

A DEDUCTION ON PRIMARY COSMIC PAY COMPOSITION AND SPECTRA ABOVE 10¹⁴eV

Corresponding author: JING Cai-Liu,

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1986-10-05

Abstract: The spectra of primary cosmic ray nuclei are fitted from experimental data under 10¹⁴eV and extrapolated to their bending energies. The primary cosmic ray composition above 10¹⁴eV is deduced according to the rigidity cut off model by selecting an appropriate bending energy for proton so that the sum of various nucleus components is consistent with the experimental total particle spectrum. The method used is independent on the behaviour of hadronic interaction.