CRWriteup
15th Baikal Summer SchoolAnna Morozova, Atmospheric neutrinos1 Sources of atmospheric electron neutrinos A.D. Morozova, S.I.Sinegovsky 15 th Baikal Summer.
1 The Pierre Auger Observatory Capturing Messengers from the Extreme Universe A new cosmic ray observatory designed for a high statistics study of the.
What we do know about cosmic rays at energies above 10 15 eV?
The Experimental Program of the “FLASH” Experiment.
CONTENT
Rapporteur Talk: HE 1.1- Extensive Air Shower Observation
Interpretation of KASCADE-Grande Data using MC Energy spectrum with QGSJET, SIBYLL, EPOS
The High Resolution Fly’s Eye
Rapporteur Talk: HE 1.1- Extensive Air Shower Observation for Energy < 10 17 eV HE 1.2 - Theory and Simulation (In atmosphere) HE 1.5 - Instrumentation.
A crude (lower limit) estimation of resolution and event rate Development and Construction of an Extensive Air Shower Array in HOU Antonis Leisos, Hellenic.
Constraints of hadronic interaction models from the cosmic muon observations. L.G. Dedenko, A.V. Lukyashin, G.F. Fedorova, T.M. Roganova M.V. Lomonosov.
