The central laser facility at the Pierre Auger Observatory

F. Arqueros, J. Bellido, C. Covault, D. D'Urso, C. Di Giulio, P. Facal, B. Fick, F. Guarino, M. Malek, J. A.J. Matthews, J. Matthews, R. Meyhandan, M. Monasor, Miguel Alejandro Mostafa, P. Petrinca, M. Roberts, P. Sommers, P. Travnicek, L. Valore, V. VerziL. Wiencke

Research output: Contribution to conferencePaperpeer-review

7 Scopus citations

Abstract

The Central Laser Facility is located near the middle of the Pierre Auger Observatory in Argentina. It features a UV laser and optics that direct a beam of calibrated pulsed light into the sky. Light scattered from this beam produces tracks in the Auger optical detectors which normally record nitrogen fluorescence tracks from cosmic ray air showers. The Central Laser Facility provides a "test beam" to investigate properties of the atmosphere and the fluorescence detectors. The laser can send light via optical fiber simultaneously to the nearest surface detector tank for hybrid timing analyses. We describe the facility and show some examples of its many uses.

Original languageEnglish (US)
Pages335-338
Number of pages4
StatePublished - Jan 1 2005
Event29th International Cosmic Ray Conference, ICRC 2005 - Pune, India
Duration: Aug 3 2005Aug 10 2005

Other

Other29th International Cosmic Ray Conference, ICRC 2005
CountryIndia
CityPune
Period8/3/058/10/05

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics

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