Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle

International Letters of Chemistry, Physics and Astronomy

doi 10.18052/www.scipress.com/ilcpa.67.21

Full Text

Abstract

Available in

Date

Authors

Publisher

SciPress Ltd

Related search

Tunka-133: The New EAS Cherenkov Light Array for Cosmic Ray Study

2011English

The Instrument Response Function Format for the Cherenkov Telescope Array

2016English

The Cosmic Ray Nuclear Composition Measurement Performance of the Non-Imaging CHErenkov Array (NICHE)

2016English

The Cosmic Ray Background as a Tool for Relative Calibration of Atmospheric Cherenkov Telescopes

Astroparticle Physics
AstrophysicsAstronomy
2003English

The Truncated Lognormal Distribution as a Luminosity Function for SWIFT-BAT Gamma-Ray Bursts

Galaxies
AstrophysicsAstronomy
2016English

Ray Tracing the Wigner Distribution Function for Optical Simulations

Optical Engineering
EngineeringOpticsAtomicMolecular Physics,
2018English

Implied Distribution as a Function of the Volatility Smile

SSRN Electronic Journal
2011English

Estimating Smooth Distribution Function in the Presence of Heteroscedastic Measurement Errors

Computational Statistics and Data Analysis
StatisticsProbabilityApplied MathematicsComputational TheoryComputational MathematicsMathematics
2010English

Investigation of the Electromagnetic Calorimeter Response Function by Cosmic Muons

EPJ Web of Conferences
AstronomyPhysics
2019English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy