APF Light Sources for the Auger Southern Observatory

Details APF Light Sources for the Auger Southern Observatory APF Light Sources for the Auger Southern Observatory

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....2..873m&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 air fluorescence signal from extensive air showers includes backgrounds from scattered Cherenkov light and from multiple scattered light. The dominant limitations in estimating, and thus correcting for, these backgrounds come from uncertainties in the aerosol attenuation length and in the aerosol differential scattering cross section. This paper discusses dedicated light sources used to measure the aerosol differential scattering cross section every hour during Auger fluorescence data taking.

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