
Variation of Azimuth Angle Distribution of EAS, With Slope of the Detector Array Plane – A Examination by Semi-Montecarlo Simulation
Publication year - 2019
Publication title -
international journal of innovative technology and exploring engineering
Language(s) - English
Resource type - Journals
ISSN - 2278-3075
DOI - 10.35940/ijitee.b1194.1292s219
Subject(s) - azimuth , plane (geometry) , detector , monte carlo method , isotropy , pitch angle , optics , physics , horizontal plane , distribution (mathematics) , vertical plane , computational physics , geodesy , geometry , geology , mathematics , computer science , mathematical analysis , telecommunications , geophysics , statistics
The azimuth angle distribution of EAS is expected, as Cosmic Rays are isotropic. It is seen that, if the plane of the detectors is not horizontal, the azimuth angle distribution becomes non-uniform. In such cases it is necessary to make proper correction for this non-uniformity, when one attempts to use the EAS data collected in such array, for source search. An attempt is made to correlate the extent of non- uniformity with the slope of the array plane, using simulation.