Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Univ. Estadual de Caminas, Sao Paulo, Brazil
Univ. Estadual de Campinas
Instituto de Física, Universidade Federal Fluminense, 24020-130 Niteroi, Rio de Janeiro, Brazil
Instituto de Física Gleb Wataghin-UNICAMP, 13083-970 Campinas, São Paulo, Brazil
Instituto de Física, Universidade Estadual de Campinas, 13081-970, Campinas, SP, Brazil
Instituto de Física, Universidade Federal Fluminense, 24210-340, Niterói, Rio de Janeiro, Brazil
Instituto de Física, Universidade Estadual de Campinas, 13081-970, Campinas, Sao Paulo, Brazil
Instituto de Fisica Gleb Wataghin, Universidade Estadual de Campinas, Campinas, S.P.N. M.AmatoF. M. OliveiraCastroCentro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJR. H. C.MaldonadoInstitute de Fisica, Universidade Federal Fluminence, Niteroi, RJH.AokiY.FujimotoY.FunayamaS.HasegawaH.KumanoH.SembaT.TabukiM.TamadaK.TanakaS.YamashitaScience and Engineering Research Laboratory, Waseda University, Shinjuku, TokyoN.ArataT.ShibataK.YokoiDepartment of Physics, Aoyama Gakuin University, Setagaya, TokyoA.OhsawaInstitute for Cosmic-Ray Research, University of Tikyo, Tanashi, Tokyo
Instituto de Física, Universidade Estadual de Campinas, 13081-970, Campinas, São Paulo, Brazil
DRCC-IFGW-UNICAMP, P.O. 6165, Campinas 13081-970, SP, BrasilM.LuksysDF-CCEN-UFPB, P.O. 5008, João Pessoa 58059-900, PB, BrasilM. D. O.MarquesDRCC-IFGW-UNICAMP, P.O. Box 6165, Campinas 13081-970, SP, BrasilC.Navia OIF-UFF, Niteroi 24020-050, RJ, BrasilR.OliveiraF. R. A.RevolloE. H.ShibuyaDRCC-IFGW-UNICAMP, P.O. 6165, Campinas 13081-970, SP, Brasil
Instituto de Fisica, Universidade Federal Fluminense 24020, Niteroi, Rj, BrasilE. H.ShibuyaInstituto de Fisica, Universidade Estadual de Campinas 13081, Campinas, SP, Brazil
Instituto de Fisica Gleb Wataghin, Universidade Estadual de Campinas, Sao Paulo, Brasil
Universidad Andina Simon Bolivar, LaPazNicolasMartinicInst. Investigaciones Fisicas, Universidad Mayor de San Andres, La Pa
A new phenomenological model of multiple particle production to describe data of emulsion chambers and air showers
A phenomenological model of multiple particle production and highest energy air showers
Algorithms based on isotropic azimuthal angle distribution of interaction secondaries
Analysis of one hadron rich event
Atmospheric Phenomena of High Energy Cosmic Rays at Mt. Chacaltaya. (Abstract)
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