Spectral resolved Measurement of the Nitrogen Fluorescence Emissions in Air induced by Electrons
arXiv:0709.1494 · doi:10.1016/j.astropartphys.2008.01.004
Abstract
For the calorimetric determination of the primary energy of extensive air showers, measured by fluorescence telescopes, a precise knowledge of the conversion factor (fluorescence yield) between the deposited energy in the atmosphere and the number of emitted fluorescence photons is essential. The fluorescence yield depends on the pressure and the temperature of the air as well as on the water vapor concentration. Within the scope of this work the fluorescence yield for the eight strongest nitrogen emission bands between 300 nm and 400 nm has been measured using electrons from a Sr-90 source with energies between 250 keV and 2000 keV. Measurements have been performed in dry air, pure nitrogen, and a nitrogen-oxygen mixture at pressures ranging from 2 hPa to 990 hPa. Furthermore the influence of water vapor has been studied. A new approach for the parametrization of the fluorescence yield was used to analyze the data, leading to a consistent description of the fluorescence yield with a minimal set of parameters. The resulting absolute accuracies for the single nitrogen bands are in the order of 15%. In the investigated energy range, the fluorescence yield proved to be independent of the energy of the ionizing electrons.
arXiv commentAccepted by Astroparticle Physics, 19 pages, 21 figures
References in corpus (4)
- New measurement on photon yields from air and the application to the energy estimation of primary cosmic rays
- Measurement of the pressure dependence of air fluorescence emission induced by electrons
- Photon yields from nitrogen gas and dry air excited by electrons
- Atmospheric Profiles at the Southern Pierre Auger Observatory and their Relevance to Air Shower Measurement
Cited by in corpus (12)
- Cosmic Rays from the Knee to the Highest Energies
- A Study of the Effect of Molecular and Aerosol Conditions in the Atmosphere on Air Fluorescence Measurements at the Pierre Auger Observatory
- Air Fluorescence Relevant for Cosmic-Ray Detection - Summary of the 5th Fluorescence Workshop, El Escorial 2007
- Precise measurement of the absolute fluorescence yield of the 337 nm band in atmospheric gases
- On the absolute value of the air-fluorescence yield
- Geometry reconstruction of fluorescence detectors revisited
- Nitrogen fluorescence in air for observing extensive air showers
- Comparison of available measurements of the absolute fluorescence yield
- Improved model for the analysis of air fluorescence induced by electrons
- The impact of the air-fluorescence yield on the reconstructed shower parameters of ultra-high energy cosmic rays
- Measurement of air fluorescence light yield induced by an electromagnetic shower
- On the energy deposition by electrons in air and the accurate determination of the air-fluorescence yield