Neutron flux generated by cosmic-ray mouns at 5200 hg/cm2 s.r. underground. Depth-neutron intensity curve
M. Aglietta(Osservatorio Astrofisico di Torino), Г. Т. Зацепин, P. V. Kortchaguin, F. F. Khalchukov, V. A. Kudryavtsev(University of Sheffield), W. Fulgione(National Institute for Astrophysics), A. Castellina(Osservatorio Astrofisico di Torino), G. Badino(Osservatorio Astrofisico di Torino), S. Vernetto(Osservatorio Astrofisico di Torino), V. B. Kortchaguin(Russian Academy of Sciences), C. Castagnoli(Osservatorio Astrofisico di Torino), V. G. Ryasny(Russian Academy of Sciences), O. Saavedra(Osservatorio Astrofisico di Torino), P. Galeotti(Osservatorio Astrofisico di Torino), A. S. Malguin, G. Bologna(Osservatorio Astrofisico di Torino), V. F. Yakushev(Institute for Nuclear Research), G. Trinchero(Osservatorio Astrofisico di Torino), O. G. Ryazhskaya, V. L. Dadykin
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