AtmoHEAD 2013 研讨会：高能天体粒子探测器的大气监测
天体物理仪器与方法
2014-03-20 v1 高能天体物理现象
高能物理 - 实验
大气与海洋物理
摘要
本次为期三天的国际研讨会聚焦于面向下一代设施的高能天体粒子探测器的大气监测与校准。大气是许多高能天体粒子探测器的组成部分。成像大气切伦科夫望远镜和宇宙射线广延大气簇射探测器是推动甚高能及超高能天体物理学领域快速发展的两大仪器。在这些仪器中，大气被用作巨大的量热计，宇宙射线和伽马射线在其中沉积能量并引发广延大气簇射（EAS）；它也是产生的切伦科夫光传播的介质。实时大气条件的不确定性以及固定大气模型的不确定性通常主导了所有其他系统误差。随着 H.E.S.S.-II 和 MAGIC-II 等升级后的成像大气切伦科夫望远镜（IACTs）以及切伦科夫望远镜阵列（CTA）和 JEM-EUSO 等未来设施灵敏度的提高，统计误差预计将显著降低，从而使大气成为确定天体粒子能谱的限制因素。多变的天气条件 necessitate 开发合适的大气监测方案，并将其整合到包括蒙特卡洛模拟在内的整体仪器校准中。鉴于专业知识分布在多个合作组和科学领域，本次跨学科研讨会旨在推动这一关键且及时议题的进展。
引用
@article{arxiv.1403.4816,
title = {AtmoHEAD 2013 workshop / Atmospheric Monitoring for High-Energy Astroparticle Detectors},
author = {K. Bernlöhr and G. Bellassai and O. Blanch and M. Bourgeat and P. Bruno and M. Buscemi and C. Cassardo and P. M. Chadwick and R. Chalme-Calvet and F. Chouza and M. Cilmo and M. Coco and J. Colombi and M. Compin and M. K. Daniel and R. De Los Reyes and J. Ebr and R. D'Elia and C. Deil and A. Etchegoyen and M. Doro and S. Ferrarese and M. Fiorini and LL. Font and D. Garrido and H. Gast and M. Gaug and F. Gonzales and A. Grillo and F. Guarino and J. Hahn and M. Hrabovsky and K. Kosack and P. Krüger and G. La Rosa and G. Leto and Y. T. E. Lo and A. López-Oramas and K. Louedec and M. C. Maccarone and D. Mandat and V. Marandon and E. Martinetti and M. Martinez and M. de Naurois and A. Neronov and S. J. Nolan and L. Otero and M. Palatka and J. Pallotta and M. Pech and G. Puhlhofer and M. Prouza and E. Quel and D. Raul and P. Ristori and M. D. Rodriguez Frias and S. Rivoire and C. B. Rulten and P. Schovanek and A. Segreto and G. Sottile and L. Stringhetti and J. -P. Tavernet and A. S. Tonachini and S. Toscano and P. Travnicek and L. Valore and G. Vasileiadis and S. Vincent and S. Wada and L. Wiencke and M. Will},
journal= {arXiv preprint arXiv:1403.4816},
year = {2014}
}
备注
Proceedings of the Atmospheric Monitoring for High-Energy Astroparticle Detectors (AtmoHEAD) Conference, Saclay (France), June 10-12, 2013