Voyager 1 Data Reveals Signatures of the Local Gas and Cosmic-Ray Source Distributions

We investigate the effects of the nearby interstellar medium (ISM) on the locally measured cosmic-ray (CR) spectra. Using the G al P rop code, we explore how variations in the local gas and source distributions affect spectral features at low energies. Comparing with recent Voyager 1 measurements taken in the local ISM, we show that for a realistic interstellar gas distribution the data favor models in which there are no significant CR sources within ∼150–200 pc of the solar system, implying that the nearest dominant contributors to the low-energy CR flux are located at distances beyond this range. We find that the modeling supports the conclusion of A. C. Cummings et al. that there is a significant fraction of primary boron in its observed spectrum at low energies. Our study shows that detailed modeling of the immediate Galactic environment is required to robustly infer Galactic CR propagation parameters from local measurements and that accounting for nearby ISM structure can alleviate tensions between direct CR data and global propagation models.