about
The TOTEM Experiment at the CERN Large Hadron ColliderPAMELA Measurements of Cosmic-Ray Proton and Helium SpectraGeomagnetically trapped, albedo and solar energetic particles: Trajectory analysis and flux reconstruction with PAMELAMeasurement of boron and carbon fluxes in cosmic rays with the PAMELA experimentMeasurements of Ground-Level Muons at Two Geomagnetic LocationsMeasurement of the flux of atmospheric muons with the CAPRICE94 apparatusSearch for slowly moving magnetic monopoles with the MACRO detectorObservation of an anomalous positron abundance in the cosmic radiationTime Dependence of the Electron and Positron Components of the Cosmic Radiation Measured by the PAMELA Experiment between July 2006 and December 2015.Double diffractive cross-section measurement in the forward region at the LHC.Luminosity-independent measurement of the proton-proton total cross section at √s=8 TeV.The discovery of geomagnetically trapped cosmic-ray antiprotonsAn evaluation of the exposure in nadir observation of the JEM-EUSO missionThe mass-hierarchy and CP-violation discovery reach of the LBNO long-baseline neutrino experimentThe TOTEM detector at LHCMeteor studies in the framework of the JEM-EUSO programStudies of a full-scale mechanical prototype line for the ANTARES neutrino telescope and tests of a prototype instrument for deep-sea acoustic measurementsThe ANTARES optical beacon systemThe data acquisition system for the ANTARES neutrino telescopeFirst results of the Instrumentation Line for the deep-sea ANTARES neutrino telescopeStudy of large hemispherical photomultiplier tubes for the ANTARES neutrino telescopeTransmission of light in deep sea water at the site of the Antares neutrino telescopeMeasurements of primary cosmic-ray hydrogen and helium by the WiZard collaborationThe Cosmic‐Ray Antiproton Flux between 0.62 and 3.19 GeV Measured Near Solar Minimum ActivityIdentification of cosmic ray electrons and positrons by neural networksPerformance of the CAPRICE RICH detector during the 1994 balloon flightWiZard SiW imaging calorimeter: a preliminary study on its particle identification capability during a balloon flight in 1993Cosmic ray oriented performance studies for the JEM-EUSO first level triggerThe cosmic ray primary composition between 1015 and 1016 eV from Extensive Air Showers electromagnetic and TeV muon dataThe cosmic ray proton, helium and CNO fluxes in the 100 TeV energy region from TeV muons and EAS atmospheric Cherenkov light observations of MACRO and EAS-TOPStudy of the primary cosmic ray composition around the knee of the energy spectrumMeasurement of electromagnetic and TEV muon components of extensive air showers by eas-top and MACRO experimentsSimultaneous observation of extensive air showers and deep-underground muons at the Gran Sasso LaboratoryCalibration aspects of the JEM-EUSO missionErratum to: Ultra high energy photons and neutrinos with JEM-EUSOGround-based tests of JEM-EUSO components at the Telescope Array site, “EUSO-TA”JEM-EUSO observational technique and exposureJEM-EUSO: Meteor and nuclearite observationsErratum to: Performances of JEM-EUSO: angular reconstructionPerformances of JEM-EUSO: angular reconstruction
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P50
description
hulumtues
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onderzoeker
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հետազոտող
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F. Cafagna
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F. Cafagna
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Francesco Cafagna
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Francesco Cafagna
@co
Francesco Cafagna
@da
Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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F. Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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Francesco Cafagna
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P106
P21
P31
P496
0000-0002-7450-4784