The Protons in Primary Cosmic Rays in the Energy Range 1015-1017 eV According to Data from the PAMIR Experiment

机译：根据PAMIR实验获得的数据，能量范围为1015-1017 eV的主要宇宙射线中的质子

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Adjusted data on the fraction of protons in the mass composition of primary cosmic rays (PCRs) in theof the X-ray emulsion chamber in the PAMIR experiment. It is demonstrated that the fraction of protons in a PCR is

机译：在PAMIR实验中，X射线乳化室中主要宇宙射线（PCR）的质量组成中质子分数的调整数据。结果表明，PCR中质子的比例为

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《Proceedings of the 32nd International Cosmic Ray Conference》|2011年|1-3|共3页
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R.M.MARTIROSOV; A.P.GARYAKA; H.S.VARDANYAN; A.D.ERLYKIN; N.M.NIKOLSKAYA; Y.A.GALLANT; L.W.JONES; H.A.BABAYAN;
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中图分类宇宙射线强度变化;
关键词
cosmic rays, mass composition, PAMIR experiment;

机译：宇宙射线，质量成分，PAMIR实验;
入库时间 2022-08-26 15:08:32

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专利

1. Fraction of protons in primary cosmic rays according to data from the PAMIR experiment in consideration of the response of X-ray emulsion chambers [J] . Puchkov V.S., Borisov A.S., Guseva Z.M., Bulletin of the Russian Academy of Sciences. Physics . 2011,第3期

机译：根据来自PAMIR实验的数据，考虑到X射线乳化室的响应，原生宇宙射线中的质子分数
2. MASS COMPOSITION OF PRIMARY COSMIC RAYS AT ENERGIES ￡0 = l-10PeV ACCORDING TO DATA OF X-RAY EMULSION CHAMBERS IN PAMIR EXPERIMENT [J] . A.S.Borisov, A.V. Vargasov, Z.M. Guseva, Bulletin of the Russian Academy of Sciences. Physics . 2005,第3期

机译：根据PAMIR实验中X射线乳化室的数据，能量为TO0 = 1-10PeV的主要宇宙射线的质量组成
3. Processing of High-Energy Proton Events using a New Method for Searching Primary Cosmic Ray Particles in X-ray Emulsion Chambers (According to the RUNJOB Experiment Data) [J] . I. S. Zayarnaya Bulletin of the Lebedev Physics Institute . 2013,第11期

机译：使用新方法在X射线乳化室中搜索主要宇宙射线粒子的处理高能质子事件（根据RUNJOB实验数据）
4. The Protons in Primary Cosmic Rays in the Energy Range 1015-1017 eV According to Data from the PAMIR Experiment [C] . R.M.MARTIROSOV, A.P.GARYAKA, H.S.VARDANYAN, International Cosmic Ray Conference . 2011

机译：初级宇宙射线中的质子在能量范围内的1015-1017 EV根据PAMIR实验的数据
5. THE NATURE OF LOW-ENERGY INTERPLANETARY HEAVY NUCLEI DOWN TO ENERGIES OF 50 KEV/AMU FROM AN ANALYSIS OF SOLID STATE ETCHED-TRACK DETECTORS FROM THE SURVEYOR III SPACECRAFT AND THE APOLLO 16 AND 17 COSMIC RAY EXPERIMENTS. [D] . WOODS, RICHARD THOMAS. 1974

机译：低能级星际重核的性质，直至能量为50 KEV / AMU，这是通过对来自于Surveyyor III航天器和APOLLO 16和17宇宙射线实验的固态电迹检测器的分析得出的。
6. Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite [O] . DAMPE Collaboration, Q. An, R. Asfandiyarov, 2019

机译：用DAMPE卫星测量40 GeV至100 TeV的宇宙射线质子光谱
7. Cosmic ray proton plus helium energy spectrum measured by the ARGO-YBJ experiment in the energy range 3–300 TeV [O] . Bartoli, B., Bernardini, P., Bi, X. j., 2015

机译：通过aRGO-YBJ实验测量的宇宙射线质子加氦能谱在3-300 TeV的能量范围内

The Protons in Primary Cosmic Rays in the Energy Range 1015-1017 eV According to Data from the PAMIR Experiment

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