Atmospheric Sensing for Ground-Based Gamma-Ray Telescopes

Details Atmospheric Sensing for Ground-Based Gamma-Ray Telescopes Atmospheric Sensing for Ground-Based Gamma-Ray Telescopes

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....7.2859a&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The atmospheric Cherenkov telescope 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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