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Journal articles
Temperature and humidity dependence of air fluorescence yield measured by AIRFLY
M. Ave
M. Bohacova
B. Buonomo
N.G. Busca
1, 2
L. Cazon
S. D. Chemerisov
M. E. Conde
R. A. Crowell
P. Di Carlo
C. Di Giulio
M. Doubrava
A. Esposito
P. Facal
F. J. Franchini
J. Hörandel
M. Hrabovsky
M. Iarlori
T. E. Kasprzyk
B. Keilhauer
H. Klages
M. Kleifges
S. Kuhlmann
G. Mazzitelli
L. Nozka
A. Obermeier
M. Palatka
S. Petrera
P. Privitera
J. Ridky
V. Rizi
G. Rodriguez
F. Salamida
P. Schovanek
H. Spinka
E. Strazzeri
A. Ulrich
Z. M. Yusof
V. Vacek
P. Valente
V. Verzi
T. Waldenmaier
T. Waldenmaier
Author
1
APC (UMR_7164) - AstroParticule et Cosmologie (APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : DRF/IRFU (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- UPD7 - Université Paris Diderot - Paris 7 : UMR_7164 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7164 (France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
2
University of Chicago (Edward H. Levi Hall 5801 South Ellis Avenue Chicago, Illinois 60637 - United States)
Abstract : The fluorescence detection of ultra high energy cosmic rays requires a detailed knowledge of the fluorescence light emission from nitrogen molecules over a wide range of atmospheric parameters, corresponding to altitudes typical of the cosmic ray shower development in the atmosphere. We have studied the temperature and humidity dependence of the fluorescence light spectrum excited by MeV electrons in air. Results for the 313.6, 337.1, 353.7 and 391.4 nm bands are reported in this paper. We found that the temperature and humidity dependence of the quenching process changes the fluorescence yield by a sizeable amount (up to 20% for the temperature dependence in the 391.4 nm band) and its effect must be included for a precise estimation of the energy of ultra high energy cosmic rays.
Document type :
Journal articles
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http://hal.in2p3.fr/in2p3-00706780
Contributor : Nicolás Busca Connect in order to contact the contributor
Submitted on : Monday, June 11, 2012 - 3:28:11 PM
Last modification on : Thursday, November 18, 2021 - 3:57:15 AM
Contributor : Nicolás Busca Connect in order to contact the contributor
Submitted on : Monday, June 11, 2012 - 3:28:11 PM
Last modification on : Thursday, November 18, 2021 - 3:57:15 AM
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Identifiers
- HAL Id : in2p3-00706780, version 1
- ARXIV : 0711.4583
- BIBCODE : 2008NIMPA.597...50A
- DOI : 10.1016/J.NIMA.2008.08.050
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IN2P3 | OBSPM | CEA | UNIV-PARIS7 | APC | CNRS | IRFU-APC | DSM-IRFU | CEA-DRF | UNIV-PARIS | UP-SCIENCES | PSL
Citation
M. Ave, M. Bohacova, B. Buonomo, N.G. Busca, L. Cazon, et al.. Temperature and humidity dependence of air fluorescence yield measured by AIRFLY. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2008, 597, pp.50-54. ⟨10.1016/J.NIMA.2008.08.050⟩. ⟨in2p3-00706780⟩
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