【作者单位】Dublin Institute for Advanced Studies；Max-Planck-Institut for Nuclear Physics；State Key Laboratory of Particle Detection and Electronics；University of Science and Technology of China；School of Physical Science and Technology，Southwest Jiaotong University；College of Physics，Sichuan University；Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center，Institute of High Energy Physics，Chinese Academy of Sciences；TIANFU Cosmic Ray Research Center；School of Astronomy and Space Science，Nanjing University；Center for Astrophysics，Guangzhou University；University of Chinese Academy of Sciences；Key Laboratory of Dark Matter and Space Astronomy，Purple Mountain Observatory，Chinese Academy of Sciences；Hebei Normal University；Key Laboratory for Research in Galaxies and Cosmology，Shanghai Astronomical Observatory，Chinese Academy of Sciences；Key Laboratory of Cosmic Rays （Tibet University），Ministry of Education；National Astronomical Observatories，Chinese Academy of Sciences；School of Physics and Astronomy & School of Physics （Guangzhou），Sun Yat-sen University；School of Physics and Astronomy，Yunnan University；Département de Physique Nucléaire et Corpusculaire，Faculté de Sciences，Université de Genève；Dipartimento di Fisica dell’Università di Napoli "Federico Ⅱ"，Complesso Universitario di Monte Sant’Angelo；Institute of Frontier and Interdisciplinary Science，Shandong University；Department of Engineering Physics，Tsinghua University
【年份】2021
【卷号】第45卷
【期号】 第4期
【页码】420-429
【ISSN】1674-1137
【摘要】 The LHAASO-WFCTA experiment,which aims to observe cosmic rays in the sub-EeV range using the fluorescence technique,uses a new generation of high-performance telescopes.To ensure that the experiment has excellent detection capability associated with ...
