利用ARGO-YBJ实验对太阳活动平静时期的日影研究祝凤荣叶妮周雪梅贾焕玉西南交通大学陈松战王博何会海卢红 曹臻 中科院高能所代表ARGO-YBJ实验组第8届高能物理学会
祝凤荣 叶妮 周雪梅 贾焕玉 西南交通大学 陈松战 王博 何会海 卢红 曹臻 中科院高能所 代表ARGO-YBJ 实验组 利用ARGO-YBJ实验对太阳活动 平静时期的日影研究 第8届高能物理学会
OutlineARGO-YBJexperimentSunshadow studyExperimentData &&simulationMethod:Physical analysis resultSummary第8届高能物理学会
Outline • ARGO-YBJ experiment • Sun shadow study • Experiment Data && simulation • Method • Physical analysis result • Summary 第8届高能物理学会
ARGO-YBJcollaborationINFN and Univerista di Lecce IHEP, BeijingINFNand Universita "Federico Il di Napoli Shandong University,JinanINFN Catania,Univ. and INAF/IASF di Palermo South West Jaotong Univ.,ChengduINFNand Universita di Pavia TibetUniversity,LhasaINFN and Univ.ersita Tor Vergata"di Roma Yunnan University, KunmingINFN and Universita“Roma Tredi Roma Zhengzhou UniversityINFN and INAF/IFSI di Torino Hongkong UniversityHebei Normal UniversitySpokesmenProf.B.D'EttorrePiazzoliProf.CaoZhen第8届高能物理学会
ARGO-YBJ collaboration INFN and Univeristà di Lecce IHEP, Beijing INFN and Università “Federico II” di Napoli Shandong University,Jinan INFN Catania, Univ. and INAF/IASF di Palermo South West Jaotong Univ., Chengdu INFN and Università di Pavia Tibet University, Lhasa INFN and Univ.ersità “Tor Vergata” di Roma Yunnan University, Kunming INFN and Università “Roma Tre” di Roma Zhengzhou University INFN and INAF/IFSI di Torino Hongkong University Hebei Normal University Spokesmen Prof. B. D’Ettorre Piazzoli Prof. Cao Zhen 第8届高能物理学会
ARGO-YBJ is an Extensive Air Shower detectoroptimized to work with showers induced by primariescosmic rays of energyE > a few hundreds GevThis low energy threshold is achieved byoperating at very high altitude (4300 m)using a"full coverage" detection surface第8届高能物理学会
ARGO-YBJ is an Extensive Air Shower detector optimized to work with showers induced by primaries cosmic rays of energy E > a few hundreds GeV This low energy threshold is achieved by: ▪ operating at very high altitude (4300 m) ▪ using a “full coverage” detection surface 第8届高能物理学会
第8届高能物理学会
第8届高能物理学会