0000000000620034

AUTHOR

D. Campana

showing 3 related works from this author

Time structure of the extensive air shower front

1997

Abstract The GREX/COVER_PLASTEX experiment has measured the temporal and spatial fine structure of the EAS disc at sea level in a new and original way, using resistive plate counter detectors for direct measurements of the arrival time of each particle crossing the detector. Data were taken at EAS core distances up to 100 m for shower size N > 105 (PeV energy range). Arrival times of shower particles were measured with nanosecond accuracy. More than 450000 air shower events have been included in this analysis.

PhysicsCore (optical fiber)Nuclear physicsResistive touchscreenRange (particle radiation)ShowerAir showerDetectorParticleAstronomy and AstrophysicsNanosecondComputational physics
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Rejection Power of A Horizontal Rpc Telescope For Left and Right Coming Cosmic Muons

1993

Abstract The possibility of performing neutrino astronomy by means of a detector above the ground depends critically on the feasibility of a rejection power on the order of 10 11 required to discriminate the enormous background of cosmic downward going muons from the signal of upward going muons produced by neutrinos. In order to check whether and how this rejection is obtainable, we have built in the Physics Department of the University of Bari a horizontal cosmic muon telescope (MINI) instrumented with resistive plate counters. By performing time-of-flight measurements, we have estimated the rejection power of our telescope for left and right coming cosmic muons. The rejection dependence …

PhysicsNuclear and High Energy PhysicsResistive touchscreenCOSMIC cancer databaseMuonPhysics::Instrumentation and DetectorsSURFACE NEUTRINO DETECTORAstrophysics::High Energy Astrophysical PhenomenaTrack (disk drive)DetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyKAMIOKANDE-II DETECTORlaw.inventionTelescopeNEUTRINOSlawHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyInstrumentation
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Layout and performance of RPC used in the Argo-YBJ experiment

2006

The layout of the RPCs, used in the Argo-YBJ experiment to image with a high space-time granularity the atmospheric shower, is described in this paper. The detector has been assembled to provide both digital and analog informations in order to cover a wide particle density range with a time accuracy of 1 ns. The experimental results obtained operating the chambers in streamer mode at sea level with a standard gas mixture are presented. (c) 2006 Elsevier B.V. All rights reserved.

PhysicsNuclear and High Energy PhysicsRivelatori a gaPhysics::Instrumentation and DetectorsCosmic rays detectorAstrophysics::High Energy Astrophysical PhenomenaDetectorSettore FIS/01 - Fisica SperimentaleResistive Plate Chambers Cosmic Rays Extended Air ShowersCamere a piani resistiviRivelatori di raggi cosmiciSettore AGR/03 - Arboricoltura Generale E Coltivazioni ArboreeGas detectorRange (statistics)RPCGranularityParticle densityInstrumentationArgoRemote sensing
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