Skip to Main content Skip to Navigation
Poster communications

An iterative unfolding method dedicated to the measure of cosmic-ray fluxes with AMS-02

Abstract : The measurement of cosmic-ray fluxes gives an indirect access to the source spectra, the abundances of different species and to the propagation processes in the Galaxy. Due to the finite energy resolution of the detectors, the measured fluxes differ from the physical ones. The process to compute the true flux from the measured one is called unfolding. The method presented here was developed in the context of the AMS-02 experiment, in particular for the analysis of the proton spectrum.
Complete list of metadata

http://hal.in2p3.fr/in2p3-01011887
Contributor : Emmanuelle Vernay Connect in order to contact the contributor
Submitted on : Tuesday, June 24, 2014 - 9:07:04 PM
Last modification on : Thursday, November 19, 2020 - 12:59:02 PM

Identifiers

  • HAL Id : in2p3-01011887, version 1

Collections

IN2P3 | LPSC | CNRS | GEPI | UGA

Citation

A. Ghelfi. An iterative unfolding method dedicated to the measure of cosmic-ray fluxes with AMS-02. Cosmic Rays & their Interstellar Medium Environment (CRISM-2014), Jun 2014, Montpellier, France. Proceedings of Science, CRISM2014, pp.013. ⟨in2p3-01011887⟩

Share

Metrics

Record views

155