We present the precision measurements of 11 years of daily cosmic positron fluxes in the
rigidity range from 1.00 to 41.9 GV based on 3.4× 10 6 positrons collected with the Alpha …

The tentative identification of approximately ten relativistic antihelium (He¯) cosmic-ray
events at AMS-02 would, if confirmed, challenge our understanding of the astrophysical …

Galactic cosmic rays (GCRs) are the slowly varying background energetic particles that
originate outside the solar system, are modulated by the heliospheric magnetic field, and …

The cosmic-ray database, CRDB, has been gathering cosmic-ray data for the community
since 2013. We present a new release, CRDB v4. 1, providing many new quantities and …

The AMS02 experiment has published the periodic spectra of proton, helium, and helium
isotopes across the majority of solar cycle 24. These precise data exhibit temporal structures …

This work presents the results of the analysis of 27-day variations in the flux of galactic
protons registered by STEREO, SOHO, and AMS-02 in 2015–2016. We calculate variations' …

We present the precision measurements of 11 years of daily cosmic electron fluxes in the
rigidity interval from 1.00 to 41.9 GV based on 2.0× 10 8 electrons collected with the Alpha …

Galactic cosmic rays suffer from solar modulation when they propagate through the
heliosphere. The transfer of the local interstellar spectrum (LIS) to the top-of-atmosphere …

A key goal of heliophysics is to understand how cosmic rays propagate in the solar system's
complex, dynamic environment. One observable is solar modulation, ie, how the flux and …

We present a new calculation of the astronaut dose rate from the galactic cosmic rays in free
space at 1 AU. We use the unshielded isotropic fluence‐to‐dose conversion coefficients …