{"title":"皮埃尔·奥格天文台的AugerPrime表面探测器电子学升级的片上系统架构","authors":"E. Lagorio","doi":"10.1109/NSSMIC.2016.8069731","DOIUrl":null,"url":null,"abstract":"The Pierre Auger Observatory, located near the town of Malargüe, Argentina, is the world's largest cosmic ray observatory. It has for objectives to probe the origin and characteristics of ultrahigh-energy cosmic rays (UHECRs). The results obtained by the Pierre Auger Collaboration provide important information on key aspects of the UHECR field, leading to new questions and open challenges which call for an upgrade of the Observatory. In the upgrade program, called AugerPrime, the 1660 surface detector stations will be improved in particular by implementing new electronics with higher performance. The new electronics aims to increase the number of analog channels and their dynamic range, to get a higher sampling rate and better timing accuracy. It is designed with a new generation of component, called SOC for System On Chip. A Linux system must be integrated for higher access development. First prototypes of the new electronics have been built and deployed at the Pierre Auger Observatory.","PeriodicalId":184587,"journal":{"name":"2016 IEEE Nuclear Science Symposium, Medical Imaging Conference and Room-Temperature Semiconductor Detector Workshop (NSS/MIC/RTSD)","volume":"20 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2016-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"System on chip architecture for AugerPrime surface detector electronics upgrade of the pierre auger observatory\",\"authors\":\"E. Lagorio\",\"doi\":\"10.1109/NSSMIC.2016.8069731\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Pierre Auger Observatory, located near the town of Malargüe, Argentina, is the world's largest cosmic ray observatory. It has for objectives to probe the origin and characteristics of ultrahigh-energy cosmic rays (UHECRs). The results obtained by the Pierre Auger Collaboration provide important information on key aspects of the UHECR field, leading to new questions and open challenges which call for an upgrade of the Observatory. In the upgrade program, called AugerPrime, the 1660 surface detector stations will be improved in particular by implementing new electronics with higher performance. The new electronics aims to increase the number of analog channels and their dynamic range, to get a higher sampling rate and better timing accuracy. It is designed with a new generation of component, called SOC for System On Chip. A Linux system must be integrated for higher access development. First prototypes of the new electronics have been built and deployed at the Pierre Auger Observatory.\",\"PeriodicalId\":184587,\"journal\":{\"name\":\"2016 IEEE Nuclear Science Symposium, Medical Imaging Conference and Room-Temperature Semiconductor Detector Workshop (NSS/MIC/RTSD)\",\"volume\":\"20 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2016-10-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2016 IEEE Nuclear Science Symposium, Medical Imaging Conference and Room-Temperature Semiconductor Detector Workshop (NSS/MIC/RTSD)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/NSSMIC.2016.8069731\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2016 IEEE Nuclear Science Symposium, Medical Imaging Conference and Room-Temperature Semiconductor Detector Workshop (NSS/MIC/RTSD)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/NSSMIC.2016.8069731","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 2
摘要
位于阿根廷malarg镇附近的皮埃尔·奥格天文台是世界上最大的宇宙射线天文台。它的目标是探索超高能宇宙射线(uhecr)的起源和特征。皮埃尔·奥格合作项目获得的结果提供了关于UHECR领域关键方面的重要信息,引发了新的问题和公开的挑战,要求对天文台进行升级。在名为AugerPrime的升级计划中,1660个地面监测站将通过安装性能更高的新电子设备得到改进。新的电子器件旨在增加模拟通道的数量及其动态范围,以获得更高的采样率和更好的定时精度。它是用新一代元件设计的,称为SOC (System On Chip)。为了进行更高级别的访问开发,必须集成Linux系统。新电子设备的第一个原型已经建成并部署在皮埃尔·奥格天文台。
System on chip architecture for AugerPrime surface detector electronics upgrade of the pierre auger observatory
The Pierre Auger Observatory, located near the town of Malargüe, Argentina, is the world's largest cosmic ray observatory. It has for objectives to probe the origin and characteristics of ultrahigh-energy cosmic rays (UHECRs). The results obtained by the Pierre Auger Collaboration provide important information on key aspects of the UHECR field, leading to new questions and open challenges which call for an upgrade of the Observatory. In the upgrade program, called AugerPrime, the 1660 surface detector stations will be improved in particular by implementing new electronics with higher performance. The new electronics aims to increase the number of analog channels and their dynamic range, to get a higher sampling rate and better timing accuracy. It is designed with a new generation of component, called SOC for System On Chip. A Linux system must be integrated for higher access development. First prototypes of the new electronics have been built and deployed at the Pierre Auger Observatory.