{"title":"皮埃尔·奥格天文台的结果","authors":"I. Mariş","doi":"10.1393/NCC/I2011-10722-4","DOIUrl":null,"url":null,"abstract":"Ultra high energy cosmic rays are observed at the Pierre Auger Observatory, the largest cosmic rays experiment in operation, through a hybrid technique employing fluorescence and surface detectors. We present the measurements on the evolution of the mass with energy, the energy spectrum features, photon and neutrino limits and anisotropies based on the data collected between 2004 and 2009.","PeriodicalId":81495,"journal":{"name":"Il Nuovo cimento della Societa italiana di fisica. C","volume":"33 1","pages":"45-52"},"PeriodicalIF":0.0000,"publicationDate":"2010-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Results from the Pierre Auger Observatory\",\"authors\":\"I. Mariş\",\"doi\":\"10.1393/NCC/I2011-10722-4\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Ultra high energy cosmic rays are observed at the Pierre Auger Observatory, the largest cosmic rays experiment in operation, through a hybrid technique employing fluorescence and surface detectors. We present the measurements on the evolution of the mass with energy, the energy spectrum features, photon and neutrino limits and anisotropies based on the data collected between 2004 and 2009.\",\"PeriodicalId\":81495,\"journal\":{\"name\":\"Il Nuovo cimento della Societa italiana di fisica. C\",\"volume\":\"33 1\",\"pages\":\"45-52\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2010-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Il Nuovo cimento della Societa italiana di fisica. C\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1393/NCC/I2011-10722-4\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Il Nuovo cimento della Societa italiana di fisica. C","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1393/NCC/I2011-10722-4","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Ultra high energy cosmic rays are observed at the Pierre Auger Observatory, the largest cosmic rays experiment in operation, through a hybrid technique employing fluorescence and surface detectors. We present the measurements on the evolution of the mass with energy, the energy spectrum features, photon and neutrino limits and anisotropies based on the data collected between 2004 and 2009.
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