{"title":"超高能量宇宙射线:现在与未来","authors":"Catarina Espírito Santo","doi":"10.1080/23311940.2015.1062216","DOIUrl":null,"url":null,"abstract":"Recent progress in the field of ultra-high energy cosmic rays has been driven by the data collected by the Pierre Auger Observatory in the southern hemisphere, and also by the Telescope Array in the northern hemisphere. These hybrid observatories combine large ground arrays with fluorescence detection techniques. In this paper, selected results will be reviewed. Future challenges and prospects will be briefly addressed.","PeriodicalId":43050,"journal":{"name":"Cogent Physics","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2015-12-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1080/23311940.2015.1062216","citationCount":"1","resultStr":"{\"title\":\"Ultra-high energy cosmic rays: Present and future\",\"authors\":\"Catarina Espírito Santo\",\"doi\":\"10.1080/23311940.2015.1062216\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Recent progress in the field of ultra-high energy cosmic rays has been driven by the data collected by the Pierre Auger Observatory in the southern hemisphere, and also by the Telescope Array in the northern hemisphere. These hybrid observatories combine large ground arrays with fluorescence detection techniques. In this paper, selected results will be reviewed. Future challenges and prospects will be briefly addressed.\",\"PeriodicalId\":43050,\"journal\":{\"name\":\"Cogent Physics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2015-12-31\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1080/23311940.2015.1062216\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Cogent Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1080/23311940.2015.1062216\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Cogent Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1080/23311940.2015.1062216","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Recent progress in the field of ultra-high energy cosmic rays has been driven by the data collected by the Pierre Auger Observatory in the southern hemisphere, and also by the Telescope Array in the northern hemisphere. These hybrid observatories combine large ground arrays with fluorescence detection techniques. In this paper, selected results will be reviewed. Future challenges and prospects will be briefly addressed.
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