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

页码：601 / 604

页数：4

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