4.2 Article

Photon yields from nitrogen gas and dry air excited by electrons

Journal

ASTROPARTICLE PHYSICS
Volume 20, Issue 3, Pages 293-309

Publisher

ELSEVIER SCIENCE BV
DOI: 10.1016/S0927-6505(03)00192-0

Keywords

nitrogen fluorescence; air fluorescence; extensive air shower; ultrahigh-energy cosmic rays

Ask authors/readers for more resources

In order to detect ultrahigh-energy cosmic rays (UHECR), atmospheric fluorescence light from the trajectory of the extensive air shower may be measured by mirror-photosensor systems. In this type of experiment the photon yield from electrons exciting air of various densities and temperatures is most fundamental information for estimating the primary energy of UHECR. An experiment has been undertaken using a Sr-90 beta source to study the pressure dependence of photon yields, and the life times of the excited states, for radiation in nitrogen and dry air. The photon yield between 300 and 406 nm in air excited by 0.85 MeV electrons is 3.73 +/- 0.15 (+/-14% systematic) photons per meter at 1000 hPa and 20 degreesC. The air density and temperature dependence is given for application to UHECR observations. (C) 2003 Elsevier B.V. All rights reserved.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.2
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available