Cosmic Sodium and Aluminum nuclei are a combination of primaries, produced at cosmic-ray sources, and secondaries resulting from collisions of heavier primary cosmic rays with the interstellar medium. We present high statistics measurements of the Na and Al rigidity spectra. We discuss the properties and composition of their spectra and present a novel model-independent determination of their abundance ratios at the source.
The systematic comparison with the latest GALPROP cosmic ray model is presented.
Volume 414 -
41st International Conference on High Energy physics (ICHEP2022) -
Astroparticle Physics and Cosmology
Unique Properties of the 3rd Group of Cosmic Rays: Results from the Alpha Magnetic Spectrometer
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Pre-published on:
November 22, 2022
Published on:
June 15, 2023
Abstract
DOI: https://doi.org/10.22323/1.414.0090
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.