0000000000802801

AUTHOR

Shu Xin Wang

showing 2 related works from this author

Observations of Forbush Decreases of cosmic ray electrons and positrons with the Dark Matter Particle Explorer

2021

The Forbush Decrease (FD) represents the rapid decrease of the intensities of charged particles accompanied with the coronal mass ejections (CMEs) or high-speed streams from coronal holes. It has been mainly explored with ground-based neutron monitors network which indirectly measure the integrated intensities of all species of cosmic rays by counting secondary neutrons produced from interaction between atmosphere atoms and cosmic rays. The space-based experiments can resolve the species of particles but the energy ranges are limited by the relative small acceptances except for the most abundant particles like protons and helium. Therefore, the FD of cosmic ray electrons and positrons have …

Dark Matter cosmic raysAstrophysics::High Energy Astrophysical PhenomenaDark matterCoronal holeFOS: Physical sciencesCosmic rayAstrophysicsdisturbancesCoronal mass ejectionForbush decreaseNeutronplastic scintillator detectorPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Neutron monitordriftSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsdependenceForbush decrease cosmic rayscalibrationsolarCharged particlemodulationSpace and Planetary SciencetransportPhysics::Space PhysicsintensityAstrophysics - High Energy Astrophysical Phenomenaenergy
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The DArk Matter Particle Explorer mission

2017

The DArk Matter Particle Explorer (DAMPE), one of the four scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese Academy of Sciences, is a general purpose high energy cosmic-ray and gamma-ray observatory, which was successfully launched on December 17th, 2015 from the Jiuquan Satellite Launch Center. The DAMPE scientific objectives include the study of galactic cosmic rays up to $\sim 10$ TeV and hundreds of TeV for electrons/gammas and nuclei respectively, and the search for dark matter signatures in their spectra. In this paper we illustrate the layout of the DAMPE instrument, and discuss the results of beam tests and calib…

Physics - Instrumentation and DetectorsSatellite launchesGamma ray observatoriesAstrophysicsGalactic cosmic rays01 natural sciencesCosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ObservatoryDetectors and Experimental TechniquesCosmic rays dark matter space experiments010303 astronomy & astrophysicsphysics.ins-detSpace science missionsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)CosmologyCosmology Galaxies Gamma rays Tellurium compounds Chinese Academy of Sciences Dark matter particles Explorer missions Galactic cosmic rays Gamma ray observatories Satellite launches Scientific objectives Space science missions Cosmic raysSpace ScienceAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaParticle Physics - ExperimentAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic raydark matterTellurium compounds0103 physical sciencesCosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)010308 nuclear & particles physicshep-exGamma raysAstronomyAstronomy and AstrophysicsGalaxiesChinese academy of sciencesGalaxyScientific objectivesDark matter particlesChinese Academy of SciencesSatellitespace experimentsExplorer missionsastro-ph.IM
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