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
Link To Document :
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