Environmental Testing of the Front-End Electronics for the Auger Observatory Surface Detector

Details Environmental Testing of the Front-End Electronics for the Auger Observatory Surface Detector Environmental Testing of the Front-End Electronics for the Auger Observatory Surface Detector

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....2..887c&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The Pierre Auger Observatory Surface Array uses mixed analog/digital low noise electronics for the detection of the highest energy cosmic rays. The southern site, which has a targeted operational life of 20 years, contains 1600 stations spread over 3000 k m2 of difficult to access terrain with a wide range of local temperatures. The production of a very large outdo or array necessitates a quality assurance plan. This includes both functional testing of the electronics to verify compliance with specification and environmental stress screening ranging from -20° C to 70° C. The production test rig, testing procedures and performance of the front-end electronics will be discussed.

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