Submitted to Cornell University’s online archive www.arxiv.org in 1999 by Chihwa Song Post-print sourced from www.arxiv.org Copyright © 2000 Elsevier Science B.V.We use the CORSIKA air shower simulation program to review the method for assigning energies to ultra-high energy cosmic rays viewed with the air fluorescence technique. This technique uses the atmosphere as a calorimeter, and we determine the corrections that must be made to the calorimetric energy to yield the primary cosmic-ray energy.C. Song, Z. Cao, B. R. Dawson, B. E. Fick, P. Sokolsky, X. Zhanghttp://www.elsevier.com/wps/find/journaldescription.cws_home/523319/description#descriptio
Cosmic rays with energy exceeding ???1018 eV are referred to as ultra-high energy cosmic rays (UHECR...
High-energy cosmic rays are detected as extensive air showers, and properties of the primary cosmic ...
The uorescence technique has been successfully used to detect ultrahigh energy cosmic rays by indire...
ManuscriptWe use the CORSIKA air shower simulation program to review the method for assigning energi...
The experimental technique of fluorescence light measurement is used for indirect observations of co...
A precise measurement of the energy is essential for the study of ultra-high energy cosmic rays. Bas...
Ultra-high-energy cosmic rays can be measured by short radio pulses in the MHz regime emitted by ext...
Measurements of cosmic ray particles at energies above E = 5 x 10^{14} eV are performed by large are...
Journal ArticleWe report a measurement of the ultrahigh-energy cosmic-ray spectrum using an atmosphe...
This work investigates the processes used to reconstruct extensive air showers induced in the atmosp...
Copyright © 2008 Elsevier B.V. All rights reserved. Submitted to Cornell University’s online archive...
A new method of a primary cosmic particle energy measurement with the extensive air shower (EAS) tec...
An accurate knowledge of the fluorescence yield and its dependence on atmospheric properties such as...
ManuscriptMeasurements are reported on the fluorescence of air as a function of depth in electromagn...
Air shower simulation programs are essential tools for the analysis of data from cosmic ray experime...
Cosmic rays with energy exceeding ???1018 eV are referred to as ultra-high energy cosmic rays (UHECR...
High-energy cosmic rays are detected as extensive air showers, and properties of the primary cosmic ...
The uorescence technique has been successfully used to detect ultrahigh energy cosmic rays by indire...
ManuscriptWe use the CORSIKA air shower simulation program to review the method for assigning energi...
The experimental technique of fluorescence light measurement is used for indirect observations of co...
A precise measurement of the energy is essential for the study of ultra-high energy cosmic rays. Bas...
Ultra-high-energy cosmic rays can be measured by short radio pulses in the MHz regime emitted by ext...
Measurements of cosmic ray particles at energies above E = 5 x 10^{14} eV are performed by large are...
Journal ArticleWe report a measurement of the ultrahigh-energy cosmic-ray spectrum using an atmosphe...
This work investigates the processes used to reconstruct extensive air showers induced in the atmosp...
Copyright © 2008 Elsevier B.V. All rights reserved. Submitted to Cornell University’s online archive...
A new method of a primary cosmic particle energy measurement with the extensive air shower (EAS) tec...
An accurate knowledge of the fluorescence yield and its dependence on atmospheric properties such as...
ManuscriptMeasurements are reported on the fluorescence of air as a function of depth in electromagn...
Air shower simulation programs are essential tools for the analysis of data from cosmic ray experime...
Cosmic rays with energy exceeding ???1018 eV are referred to as ultra-high energy cosmic rays (UHECR...
High-energy cosmic rays are detected as extensive air showers, and properties of the primary cosmic ...
The uorescence technique has been successfully used to detect ultrahigh energy cosmic rays by indire...