Astronomy and Astrophysics – Astrophysics – Instrumentation and Methods for Astrophysics
Scientific paper
2009-01-22
Astropart.Phys.34:699-704,2011
Astronomy and Astrophysics
Astrophysics
Instrumentation and Methods for Astrophysics
published, and superseded by arXiv:1103.0662
Scientific paper
10.1016/j.astropartphys.2011.01.
Cosmic rays have valuable information about universe surroundings us. Finding energy, mass and arrival direction of primary cosmic ray particle are the most important aspects of extensive air shower studies. In order to determine these parameters, arrival direction and core position of extensive air showers should be determined at first. In this article, a new method has been introduced that utilizes arrival time information of secondary particles of extensive air showers for finding their core location and correcting plane wave front approximation so that calculate the arrival direction of extensive air showers. This method does not need number sensitive detectors-detectors which are sensitive to the number of crossing particles- and consequently there is no need for lateral distribution models. This model has been developed by analysis of simulated events generated by CORSIKA package.
Anvari A.
Bahmanabadi Mahmoud
Ghomi Mehdi Khakian
Hedayati H. Kh.
Samimi Jalal
No associations
LandOfFree
New Simple Method for Analysis of Extensive Air Showers does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with New Simple Method for Analysis of Extensive Air Showers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New Simple Method for Analysis of Extensive Air Showers will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-190096