Periodicities in the Daily Proton Fluxes from 2011 to 2019 Measured by the Alpha Magnetic Spectrometer on the International Space Station from 1 to 100 GV

In the following tables we present the daily proton flux $\Phi_p$ as a function of rigidity at the top of AMS. The fluxes are in units of $[{\rm m}^2 \cdot {\rm sr} \cdot {\rm s} \cdot {\rm GV}]^{-1}$. The errors include statistics ($\sigma_{\rm stat.}$), time-dependent systematic errors ($\sigma_{\rm time}$) and the total systematic error ($\sigma_{\rm syst.}$). Contributions to the time-dependent systematic errors ($\sigma_{\rm time}$) are from: the trigger efficiency and the reconstruction efficiencies. Contributions to the total systematic error ($\sigma_{\rm syst.}$) are from: the time-dependent systematic error, the background evaluation, the geomagnetic cutoff, the acceptance calculation, the rigidity resolution function, and the absolute rigidity scale.

The days are defined as UTC time 00:00:00 – 23:59:59. The daily collection time of the proton fluxes is $(1.6 - 3.7) \times 10^3 {\rm s}$ at 1 GV, $(4.5 - 7.5) \times 10^3 {\rm s}$ at 2 GV, $(1.8 - 2.3) \times 10^4 {\rm s}$ at 5 GV, $(3.3 - 3.8) \times 10^4 {\rm s}$ at 10 GV, $(6.1 - 7.0) \times 10^4 {\rm s}$ at 20 GV, and, above 0 GV, reaches $(6.7 - 7.3) \times 10^4 {\rm s}$ out of $8.64 \times 10^4 {\rm s}$ per day.