  AMS-02 on board the ISS provides precise measurements of Cosmic Rays (CR)
near Earth, while Voyager measures CR in the local interstellar medium, beyond
the effects of solar modulation. Based on these data, we test and revise
various CR propagation scenarios under standard assumptions: pure diffusion,
diffusion with convection, diffusion with reacceleration, and diffusion with
reacceleration and convection. We report on the scenarios' performance against
CR measurements, aiming to limit the number of model parameters as much as
possible. For each scenario we find parameters that are able to reproduce
Voyager and AMS-02 data for the entire energy band for all the CR species
tested. Above several GV we observe a similar injection spectral index for He
and C, with He harder than H. Some scenarios previously disfavored are now
reconsidered. For example, contrary to usual assumptions, we find that the pure
diffusion scenario does not need an upturn in the diffusion coefficient at low
energy, while it needs the same number of low-energy breaks in the injection
spectrum as diffusive-reacceleration scenarios. We show that scenarios differ
in modeled spectra of one order of magnitude for positrons at around 1 GeV and
of a factor of 2 for antiprotons at several GV. The force-field approximation
describes well the AMS-02 and Voyager spectra analyzed, except antiprotons. We
confirm the excess around 10 GeV in the antiproton spectrum for all scenarios.
Also, for all scenarios, the resulting solar modulation should be stronger for
positrons than for nuclei, with reacceleration models requiring much larger
modulation.
