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dc.contributor.CRUESPUNIVERSIDADE DE ESTADUAL DE CAMPINASpt_BR
dc.typeArtigo de periódicopt_BR
dc.titleAn Eas Event Observed In The Early Stage Of Developmentpt_BR
dc.contributor.authorBarroso S.L.C.pt_BR
dc.contributor.authorBeggio P.C.pt_BR
dc.contributor.authorde Carvalho A.O.pt_BR
dc.contributor.authorChinellato J.A.pt_BR
dc.contributor.authorMariano A.pt_BR
dc.contributor.authorde Oliveira R.pt_BR
dc.contributor.authorShibuya E.H.pt_BR
unicamp.authorde Carvalho, A.O., Instituto de Física 'Gleb Wataghin', UNICAMP, 13083-970 Campinas, SP, Brazilpt_BR
unicamp.authorChinellato, J.A., Instituto de Física 'Gleb Wataghin', UNICAMP, 13083-970 Campinas, SP, Brazilpt_BR
unicamp.authorMariano, A., Instituto de Física 'Gleb Wataghin', UNICAMP, 13083-970 Campinas, SP, Brazilpt_BR
unicamp.authorde Oliveira, R., Instituto de Física 'Gleb Wataghin', UNICAMP, 13083-970 Campinas, SP, Brazilpt_BR
unicamp.authorShibuya, E.H., Instituto de Física 'Gleb Wataghin', UNICAMP, 13083-970 Campinas, SP, Brazilpt_BR
unicamp.author.externalBarroso, S.L.C., Centro Brasileiro de Pesquisas Físicas, 22290-180 Rio de Janeiro, RJ, Brazilpt
unicamp.author.externalBeggio, P.C., Laboratório de Ciências Matemáticas, UENF, Campos de Goytacazes, RJ, Brazilpt
dc.description.abstractSince 1969 the experiments of Brazil-Japan Collaboration showed the occurrence of a series of events, showing a region with a high concentration of electromagnetic particles, surrounded by isolated and/or groups of showers. These events were named "halo events" or "super-families". Currently, we have more than a dozen of such events. The first of them, due to its aspect, was named "Andromeda". We present here the main characteristics of a similar halo event, named C21S087I075. It has a halo region with many high energy showers in its border. Other small energy showers spread over the central and surrounding blocks (S088, S100, S101, I074). These isolated showers, classified as of hadronic or electromagnetic origin, present a fractional energy distribution compatible with that of a Centauro candidate event (C16S087I037), reported at this symposium [S.L.C. Barroso, P.C. Beggio, J.A. Chinellato, A.O. Carvalho, A. Mariano, R. Oliveira, E.H. Shibuya, in this issue of XIV ISVHECRI]. Moreover, the lateral distribution in the halo region is similar to that observed in other 3 halo events. © 2007 Elsevier B.V. All rights reserved.en
dc.relation.ispartofNuclear Physics B - Proceedings Supplementspt_BR
dc.date.issued2008pt_BR
dc.identifier.citationNuclear Physics B - Proceedings Supplements. , v. 175-176, n. SUPPL.: COMPLETE, p. 182 - 185, 2008.pt_BR
dc.language.isoenpt_BR
dc.description.volume175-176pt_BR
dc.description.issuenumberSUPPL.: COMPLETEpt_BR
dc.description.firstpage182pt_BR
dc.description.lastpage185pt_BR
dc.rightsfechadopt_BR
dc.sourceScopuspt_BR
dc.identifier.issn9205632pt_BR
dc.identifier.doi10.1016/j.nuclphysbps.2007.10.031pt_BR
dc.identifier.urlhttp://www.scopus.com/inward/record.url?eid=2-s2.0-37649016300&partnerID=40&md5=71192944e83d7f709f07f56ff0c0ec8cpt_BR
dc.date.available2015-06-30T19:33:37Z
dc.date.available2015-11-26T14:45:30Z-
dc.date.accessioned2015-06-30T19:33:37Z
dc.date.accessioned2015-11-26T14:45:30Z-
dc.description.provenanceMade available in DSpace on 2015-06-30T19:33:37Z (GMT). No. of bitstreams: 1 2-s2.0-37649016300.pdf: 732175 bytes, checksum: 02d44414140b26f0b37ec3065e1b8f53 (MD5) Previous issue date: 2008en
dc.description.provenanceMade available in DSpace on 2015-11-26T14:45:30Z (GMT). No. of bitstreams: 1 2-s2.0-37649016300.pdf: 732175 bytes, checksum: 02d44414140b26f0b37ec3065e1b8f53 (MD5) Previous issue date: 2008en
dc.identifier.urihttp://www.repositorio.unicamp.br/handle/REPOSIP/106655
dc.identifier.urihttp://repositorio.unicamp.br/jspui/handle/REPOSIP/106655-
dc.identifier.idScopus2-s2.0-37649016300pt_BR
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dc.description.referenceYamashita, S., (1985) J. Phys. Soc. of Japan, 54 (2), pp. 529-543pt_BR
dc.description.referenceOhta, I., Mizutani, K., Kasahara, K., Kobayashi, T., Mikumo, E., Mito, I., Ohsawa, A., Takahashi, Y., (1979) Nucl. Inst. & Meth., 161, pp. 35-53pt_BR
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