The authors produce a 3D tomographic reconstruction of Galactic cosmic-ray proton density from Fermi-LAT gamma-ray data and a gas model, finding a smooth distribution with moderate inner-Galaxy enhancement consistent with AMS-02 local measurements.
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A self-consistent model of cosmic ray transport in molecular clouds with ballistic, diffusive, and hybrid scenarios applied to Taurus shows enhanced scattering on clump scales, suppressed diffusion coefficients, and elevated ionization rates.
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A Three-Dimensional Tomographic Reconstruction of the Galactic Cosmic-Ray Proton Density
The authors produce a 3D tomographic reconstruction of Galactic cosmic-ray proton density from Fermi-LAT gamma-ray data and a gas model, finding a smooth distribution with moderate inner-Galaxy enhancement consistent with AMS-02 local measurements.
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Multiwavelength Probes of Cosmic Ray Transport in Molecular Cloud Structures
A self-consistent model of cosmic ray transport in molecular clouds with ballistic, diffusive, and hybrid scenarios applied to Taurus shows enhanced scattering on clump scales, suppressed diffusion coefficients, and elevated ionization rates.