Atmospheric sensing for atmospheric Cherenkov telescopes

Details Atmospheric sensing for atmospheric Cherenkov telescopes Atmospheric sensing for atmospheric Cherenkov telescopes

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..558..601c&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: International Symposium. AIP Conference Proceedings, Volume 558, pp. 601-604 (2001).

Astronomy and Astrophysics

Astronomy

X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

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. .

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