Numerical modeling of cosmic-ray transport in the heliosphere and interpretation of the proton-to-helium ratio in Solar Cycle 24

Author:

Tomassetti Nicola,Barão Fernando,Bertucci Bruna,Fiandrini Emanuele,Orcinha Miguel

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference58 articles.

1. Time dependence of the proton flux measured by PAMELA during the 2006 July - 2009 December solar minimum;Adriani;Astrophys. J.,2013

2. Observation of fine time structures in the cosmic proton and helium fluxes with the alpha magnetic spectrometer on the International Space Station;Aguilar;Phys. Rev. Lett.,2018

3. Observation of complex time structures in the cosmic-ray electron and positron fluxes with the alpha magnetic spectrometer on the International Space Station;Aguilar;Phys. Rev. Lett.,2018

4. Observation of new properties of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer on the International Space Station;Aguilar;Phys. Rev. Lett.,2018

5. Precision measurement of the proton flux in primary cosmic rays from Rigidity 1 GV to 1.8 TV with the alpha magnetic spectrometer on the International Space Station;Aguilar;Phys. Rev. Lett.,2015

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