05 HiRes / MIA Measurements of Extensive Air Shower Development between 10 17 and 10 18 eV : Detector Description and Performance

T. Abu-Zayyad, K. Belov,D. J. Bird, J. Boyer, Z. Cao, M. Catanese,G. F. Chen,R. W. Clay,C. E. Covault,J. W. Cronin, H. Y. Dai,B. R. Dawson,J. W. Elbert, B. E. Fick, L. F. Fortson, J. W. Fowler, K. G. Gibbs, M. A. K. Glasmacher,K. D. Green, Y. Ho, A. Huang, C. C. Jui,M. J. Kidd,D. B. Kieda,B. C. Knapp, S. Ko,C. G. Larsen,W. Lee,E. C. Loh, E. J. Mannel,J. Matthews,J. N. Matthews, B. J. Newport, D. Nitz, T. A. O’Halloran,R. A. Ong, K. M. Simpson,J. D. Smith,D. Sinclair,P. Sokolsky, P. Sommers, C. Song, J. K. K. Tang,S. B. Thomas, J. C. van der Velde, L. R. Wiencke,C. R. Wilkinson, S. Yoshida,X. Z. Zhang

semanticscholar（1999）

引用 0|浏览0

暂无评分

摘要

The HiRes prototype detector was operated for almost three years in coincidence with the CASA and MIA EAS arrays. We are able to extract mass composition information from the HiRes data (the shower depth of maximum) and from the MIA data (the muon content). In this paper we describe the detectors and their ability to measure mass composition parameters. Physics conclusions and their sensitivity to systematic effects are described in an accompanying paper (Abu-Zayyad et al. 1999).

查看译文

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要