Speaker
Paolo Zuccon
(Universita degli Studi di Trento and INFN (IT))
Description
Deuterons are the most abundant secondary nuclei in cosmic rays and precise measurement of their properties will allow to test and constrain various cosmic ray propagation models.
The precision measurement of deuteron flux with kinetic energy per nucleon from 0.2 GeV/n to 9 GeV/n based on 15 million deuterons collected by Alpha Magnetic Spectrometer during first 10 years of operation on International Space Station is presented. The deuteron-to-proton and deuteron-to-4helium flux ratios are also shown, together with their time evolution over a almost complete solar cycle.
| Submitted on behalf of a Collaboration? | Yes |
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Authors
Dr
Francesco Dimiccoli
(Universita degli Studi di Trento and INFN (IT))
Paolo Zuccon
(Universita degli Studi di Trento and INFN (IT))
