Energy Estimation of Ultra High Energy Cosmic Hadrons by Lateral Distribution Functions of Extensive Air Showers

Statistics – Methodology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

The determination of energy of Ultra High Energy Cosmic Rays (E ≥ 5×1019 eV) is one of the important issues concerning these particles. For this purpose, Monte Carlo simulations are used to create a large number of vertical and inclined extensive air showers in order to estimate the primary energy based on the lateral distribution function of recorded electrons and muons. This methodology could be applied to all cosmic ray experiments using a surface array of Cerenkov detectors, like, for example, the P. Auger Observatory.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Energy Estimation of Ultra High Energy Cosmic Hadrons by Lateral Distribution Functions 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 Energy Estimation of Ultra High Energy Cosmic Hadrons by Lateral Distribution Functions of Extensive Air Showers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energy Estimation of Ultra High Energy Cosmic Hadrons by Lateral Distribution Functions of Extensive Air Showers will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-954075

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.