Search results for "Apparati di sciame"

showing 2 items of 2 documents

Search for gamma ray bursts with the ARGO-YBJ detector in scaler mode

2009

We report on the search for Gamma Ray Bursts (GRBs) in the energy range 1-100 GeV in coincidence with the prompt emission detected by satellites using the Astrophysical Radiation with Ground-based Observatory at YangBaJing (ARGO-YBJ) air shower detector. Thanks to its mountain location (Yangbajing, Tibet, P.R. China, 4300 m a.s.l.), active surface (about 6700 m**2 of Resistive Plate Chambers), and large field of view (about 2 sr, limited only by the atmospheric absorption), the ARGO-YBJ air shower detector is particularly suitable for the detection of unpredictable and short duration events such as GRBs. The search is carried out using the "single particle technique", i.e. counting all the …

Nuclear and High Energy PhysicsGamma ray burstAstrophysics::High Energy Astrophysical PhenomenaAir shower arrayAstrophysicsArgo-YbjSettore FIS/05 - Astronomia e AstrofisicaObservatoryGamma Rays ObservationsInstrumentationZenithArgoPhysicsRange (particle radiation)Apparati di sciameDetectorSettore FIS/01 - Fisica SperimentaleGamma rayGamma ray bursts Air shower arraysMode (statistics)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsRedshiftAir showerSpace and Planetary ScienceGamma Ray Bursts Gamma Ray EmissionAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burst
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Observation of the cosmic ray moon shadowing effect with the ARGO-YBJ experiment

2011

Cosmic rays are hampered by the Moon and a deficit in its direction is expected (the so-called Moon shadow). The Moon shadow is an important tool to determine the performance of an air shower array. Indeed, the westward displacement of the shadow center, due to the bending effect of the geomagnetic field on the propagation of cosmic rays, allows the setting of the absolute rigidity scale of the primary particles inducing the showers recorded by the detector. In addition, the shape of the shadow permits to determine the detector point spread function, while the position of the deficit at high energies allows the evaluation of its absolute pointing accuracy. In this paper we present the obser…

Point spread functionNuclear and High Energy PhysicsCosmic Rays Gamma Astronomy Extended Air ShowersAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodCosmic rayAstrophysics01 natural sciencesStandard deviationPhysics::GeophysicsRaggi cosmiciSettore FIS/05 - Astronomia E Astrofisicageomagnetic field0103 physical sciences010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsOmbra della lunaApparati di sciameDetectorSettore FIS/01 - Fisica SperimentaleMoon shadowAstronomyCosmic rayMagnetic fieldEarth's magnetic fieldAir shower13. Climate actionPhysics::Space Physics
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