Speaker
Jiahui WEI
(Shandong Institute of Advanced Technology (SDIAT))
Description
Beryllium nuclei are expected to be mainly produced by the fragmentation of primary cosmic rays (CR) during their propagation. Therefore, their measurement is essential in the understanding of cosmic ray propagation and sources. In particular, the $^{10}$Be/$^9$Be ratio can be used as a radioactive clock providing the measurement of CR residence time in the Galaxy. In this contribution, the measurement of the $^7$Be, $^9$Be, and $^{10}$Be fluxes and ratios based on data collected by AMS are presented.
| In-person participation | Yes |
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Primary authors
Jiahui WEI
(Shandong Institute of Advanced Technology (SDIAT))
Fernando DE CARVALHO BARAO
(LIP - Laboratório de Instrumentação e Física Experimental de Partículas)
Laurent YVES MARIE DEROME
(LPSC Laboratoire de Physique Subatomique et de Cosmologie (LPSC))
Mercedes PANICCIA
(Université de Genève)
