Atmospheric sensing for atmospheric Cherenkov telescopes

被引：0
|
作者：
Chadwick, PM [1 ]
Daniel, MK [1 ]
Lyons, K [1 ]
McComb, TJL [1 ]
McKenny, JM [1 ]
Nolan, SJ [1 ]
Orford, KJ [1 ]
Osborne, JL [1 ]
Rayner, SM [1 ]
机构：
[1] Univ Durham, Dept Phys, Sci Labs, Durham DH1 3LE, England
来源：
HIGH ENERGY GAMMA-RAY ASTRONOMY | 2001年 / 558卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The atmospheric Cherenkov technique is unique in that the atmosphere is an integral part of the detector. A realistic goal for the next generation of telescopes is to make energy assignments and flux determinations to better than 10%. We discuss the requirements for atmospheric monitoring that will be necessary to achieve this and look forward to how these requirements can be implemented.
引用
收藏
页码：601 / 604
页数：4
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