• Title of article

    Point spread function due to multiple scattering of light in the atmosphere

  • Author/Authors

    P?kala، نويسنده , , J. and Wilczy?ski، نويسنده , , H.، نويسنده ,

  • Pages
    6
  • From page
    296
  • To page
    301
  • Abstract
    The atmospheric scattering of light has a significant influence on the results of optical observations of air showers. It causes attenuation of direct light from the shower, but also contributes a delayed signal to the observed light. The scattering of light therefore should be accounted for, both in simulations of air shower detection and reconstruction of observed events. In this work a Monte Carlo simulation of multiple scattering of light has been used to determine the contribution of the scattered light in observations of a point source of light. Results of the simulations and a parameterization of the angular distribution of the scattered light contribution to the observed signal (the point spread function) are presented.
  • Keywords
    Point spread function , Ultra-high energy cosmic rays , Extensive Air Shower , multiple scattering
  • Journal title
    Astroparticle Physics
  • Record number

    2014384