• [1]

    J. R. Ren et al., Phys. Rev., D38(1988), 1404.[2] Pamir Collaboration, Proceedings of International Symposium on Cosmic Ray Superhigh Energy Interactions,Beijing (1986), 3-1.[3] Chacaltaya and Pamir Collaboration, ICRR-Report-216-90-9.[4] G, Coccni, Nucl. Phys., B28(1971), 341[5] R. P. Feynman, Phys. Rev, Lett., Vol. 23(1969), 1451,[6] J. Wdowczyk and A. W. Wolfendale, Nature (London) 306(1983), 347; J, Phys.G13(1987),411.[7] L. K. Ding et al., Proceedings of the International Symposium on Cosmic Ray and Particle Physics, Tokyo,Japan, 1984, P142.[8] M, Dunaevsky, Proceedings of International Symposium on Cosmic Ray Superhigh Energy Interactions, Beijing(1986), 1-103.[9] L. K. Ding et al., Proceedings of International Symposium on Cosmic Ray Superhigh Energy Interactions, Beijing (1986), 3-49.[10] Q. Q. Zhu et al., Proceedings of International Symposium on Cosmic Ray Superhigh Energy Interactions, Beijing(1986), 7-1.[11] 汤田利典,《用乳胶室研究超高能核作用》,1983,P19,任敬儒译.[12] M. Haguenauer et al., 21th ICRC, Austrilia, 8(1990), 209.[13] J. G. Rushbrooke, CERN-EP/85-124, 1985.[14] A. Ohsawa, Prog. Thero. Phys., Vol. 84, No. 1(1990), 50.[15] 王承瑞,第五届全国宇宙线会议文集,武汉(1990),p.l.[16] K. Alpgard et al,Phys. Lett., 121B(1983), 209.[17] G. J. Alner et al., Phys. Lett., 160B(1985), 193.[18] G. Giacomelli and M, Jacob, Phys. Reports, 55(1979), 1-132.[19] 范晓般,张春生,强子—强子核相互作用参数化模型在超高能字宙线研究中的应用,高能物理与核物理,待发表.