Chemical Composition of Galactic Cosmic Rays with Space Experiments
arXiv:1208.1406 · doi:10.1016/j.astropartphys.2012.05.007
Abstract
The origin and properties of the cosmic radiation are one of the most intriguing question in modern astrophysics. The precise measurement of the chemical composition and energy spectra of the cosmic rays provides fundamental insight into these subjects. In this paper we will review the existing experimental data. Specifically, we will analyse results collected by space-born experiments discussing the experimental uncertainties and challenges with a focus on the PAMELA experiment.
42 pages, 13 figures. In Press Astrop. Phys. (2012)
References in corpus (16)
- Observation of an anomalous positron abundance in the cosmic radiation
- Measurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope
- PAMELA - A Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics
- Discrepant hardening observed in cosmic-ray elemental spectra
- Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations
- Cosmic-ray positron fraction measurement from 1 to 30 GeV with AMS-01
- The origin of the positron excess in cosmic rays
- Anisotropy and Corotation of Galactic Cosmic Rays
- Constraints on WIMP Dark Matter from the High Energy PAMELA data
- Measurements of cosmic-ray secondary nuclei at high energies with the first flight of the CREAM balloon-borne experiment
- The Large Scale Cosmic-Ray Anisotropy as Observed with Milagro
- Galactic electrons and positrons at the Earth:new estimate of the primary and secondary fluxes
- Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
- Measurement of the Anisotropy of Cosmic Ray Arrival Directions with IceCube
- Measurement of cosmic-ray low-energy antiproton spectrum with the first BESS-Polar Antarctic flight
- Moon Shadow by Cosmic Rays under the Influence of Geomagnetic Field and Search for Antiprotons at Multi-TeV Energies