Speaker
Alberto Oliva
(Istituto Nazionale di Fisica Nucleare)
Description
We present high statistics measurements of AMS-02 of the secondary cosmic rays Lithium, Beryllium, Boron, and Fluorine. The properties of the secondary cosmic ray fluxes and their ratios to the primary cosmic rays Li/C, Be/C, B/C, Li/O, Be/O, B/O, and F/Si are discussed. A systematic comparison with the latest GALPROP cosmic ray model is presented.
| In-person participation | Yes |
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Primary author
Alberto Oliva
(Istituto Nazionale di Fisica Nucleare)
