Design considerations for a TeV telescope at the South Pole

Details Design considerations for a TeV telescope at the South Pole Design considerations for a TeV telescope at the South Pole

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..198...20h&link_type=abstract

IN: Astrophysics in Antarctica (A92-22401 07-89). New York, American Institute of Physics, 1989, p. 20-23.

Astronomy and Astrophysics

Astronomy

Antarctic Regions, Cerenkov Radiation, Energetic Particles, Gamma Ray Astronomy, Gamma Ray Telescopes, Particle Telescopes, Atmospheric Attenuation, Auroral Irradiation, Cerenkov Counters, Cosmic Ray Showers, Photomultiplier Tubes

Scientific paper

The South Pole offers such favorable factors for atmospheric Cherenkov-technique-based gamma-ray astronomy as high elevation, constant source-elevation angle, and visibility of high negative-declination sources. Atmospheric Cherenkov telescopic optics thus sited will require protection from radiative cooling and direct exposure to blowing snow, minimum component parts consistent with high redundancy, and filters to avoid the principal auroral bands. The basic design concept proposed employs three simple telescopes on a single mount.

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