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First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeVHigh Statistics Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–500 GeV with the Alpha Magnetic Spectrometer on the International Space StationElectron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space StationPrecision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station.Antiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station.Precision Measurement of the Helium Flux in Primary Cosmic Rays of Rigidities 1.9 GV to 3 TV with the Alpha Magnetic Spectrometer on the International Space Station.Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station.Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station.Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station.Precision Measurement of the (e^{+}+e^{-}) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space StationHelMod in the Works: From Direct Observations to the Local Interstellar Spectrum of Cosmic-Ray ElectronsSolution of Heliospheric Propagation: Unveiling the Local Interstellar Spectra of Cosmic-ray SpeciesLatitudinal Dependence of Cosmic Rays Modulation at 1 AU and Interplanetary Magnetic Field Polar CorrectionRecent progress of GEANT4 electromagnetic physics for LHC and other applicationsOn the forward-backward-in-time approach for Monte Carlo solution of Parker's transport equation: One-dimensional caseCosmic Rays in the Earth Magnetosphere: the importance of the External Field models in trajectory reconstruction with AMS-02 dataEVALUATION OF ENERGETIC PROTON PRESSURE DURING SOLAR EVENTS AND POSSIBLE EFFECTS ON THE MAGNETOSPHERENIEL DOSE DEPENDENCE FOR SOLAR CELLS IRRADIATED WITH ELECTRONS AND PROTONSSolar Modulation along last solar minimumAn expression for the Mott cross section of electrons and positrons on nuclei with Z up to 118Effects of solar modulation on the cosmic ray positron fractionSystematic investigation of solar modulation of galactic protons for solar cycle 23 using a Monte Carlo approach with particle drift effects and latitudinal dependence
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P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
M. Tacconi
@nl
Mauro Tacconi
@en
Mauro Tacconi
@es
type
label
M. Tacconi
@nl
Mauro Tacconi
@en
Mauro Tacconi
@es
altLabel
M. Tacconi
@en
prefLabel
M. Tacconi
@nl
Mauro Tacconi
@en
Mauro Tacconi
@es
P106
P1153
54899147500
P21
P31
P496
0000-0002-9344-6305