'Primary cosmic rays' diaporamas de présentation

Multiple Muons at the Far Detector

Multiple Muons at the Far Detector. Andy Blake Cambridge University Fermilab, December 2006. Introduction (1). One characteristic feature of the observed cosmic ray energy spectrum is the steepening that occurs at energies of ~10 7 GeV/nucleus.

382 views • 26 slides

Primary Cosmic Rays the multi TeV challenge

Primary Cosmic Rays the multi TeV challenge. Roberto Battiston Gamma-400 Workshop Trieste May 2-5 2013. AMS. Calorimeter (ECAL). e ?. Lead foil (1mm). Fibers ( ? 1mm). A precision, 3-D measurement of the directions and energies of light rays and electrons up to 1 TeV.

328 views • 21 slides

Victor Hess

Victor Hess.

357 views • 20 slides

SKALTA experiment

212 views • 9 slides

SKALTA experiment

185 views • 9 slides