Measurement of air fluorescence light yield induced by an electromagnetic shower

For most of the Ultra High Energy Cosmic Ray (UHECR) experiments and projects (HiRes, AUGER, TA, JEM-EUSO, TUS,...), the detection technique of Extensive Air Showers (EAS) is based, at least, on the measurement of the air fluorescence induced signal. The knowledge of the Fluorescence Light Yield (FL...

Descripción completa

Detalles Bibliográficos
Autores principales: Colin, Pierre, Chukanov, A., Grebenyuk, V., Naumov, D., Nedelec, P., Nefedov, Yu., Onofre, A., Porokhovoi, S., Sabirov, B., Tkatchev, L.
Lenguaje:eng
Publicado: 2007
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1016/j.astropartphys.2008.10.005
http://cds.cern.ch/record/1021844

Internet

https://dx.doi.org/10.1016/j.astropartphys.2008.10.005
http://cds.cern.ch/record/1021844

Ejemplares similares