activity
19992019
most citedProtons in near earth orbit

205 citations · 745 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.HE2019

Anisotropy of Cosmic Ray Fluxes Measured with the Alpha Magnetic Spectrometer on the ISS

M. Molero, J. Casaus, C. Mana +6

A measurement of the dipole anisotropy in galactic coordinates for different charged cosmic rays has been performed with the Alpha Magnetic Spectrometer (AMS) onboard the Internati…

astro-ph.IM2019★ 84 cited

AMS-100: The Next Generation Magnetic Spectrometer in Space -- An International Science Platform for Physics and Astrophysics at Lagrange Point 2

Stefan Schael, Alexander Atanasyan, Javier Berdugo +23

The next generation magnetic spectrometer in space, AMS-100, is designed to have a geometrical acceptance of and to be operated for at least ten ye…

astro-ph.HE2017★ 12 cited

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 Station

Manuela Vecchi

We present a precise measurement of the combined electron plus positron flux from 0.5 GeV to 1 TeV, based on the analysis of the data collected by the Alpha Magnetic Spectrometer d…

astro-ph.HE2016★ 1 cited

Precision Measurement of the Proton Flux in Primary Cosmic Rays from 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station

Cristina Consolandi

A precision measurement of the proton flux in primary cosmic rays with rigidity from 1 GV to 1.8 TV is presented based on 300 million events. The results show that the proton flux…

physics.data-an2016

Three Lectures on Probability and Statistics

Carlos Mana

Notes for a Course on Probability and Statistics: L1: Elements of Probability; L2: Bayesian Inference; L3: Monte Carlo Methods

astro-ph.IM2015

On the upper limits for dipole anisotropies in cosmic-ray positrons

J. Berdugo, J. Casaus, C. Mana +1

The excess of cosmic-ray positrons in the energy range from 10 GeV to few hundred GeV reported by PAMELA and AMS experiments is not consistent with a pure secondary origin and requ…