The radio/IR/gamma-ray correlation in galaxies is an emergent geometric property of line-of-sight integration through radially structured discs, not a signature of local cosmic-ray calorimetry.
W., Johannesson, G., et al., 2011, GAL- PROP WebRun: An internet-based service for calculating galactic cosmic ray propagation and associated photon emissions , Comp
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Numerical and analytical modeling of cosmic-ray transport attributes the long-term variation in the AMS-observed proton-to-helium ratio below 3 GV to mass-to-charge dependence in the heliospheric diffusion coefficient.
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Geometry, Not Calorimetry, Drives the Radio/Infrared/Gamma-Ray Correlation
The radio/IR/gamma-ray correlation in galaxies is an emergent geometric property of line-of-sight integration through radially structured discs, not a signature of local cosmic-ray calorimetry.
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Numerical modeling of cosmic-ray transport in the heliosphere and interpretation of the proton-to-helium ratio in Solar Cycle 24
Numerical and analytical modeling of cosmic-ray transport attributes the long-term variation in the AMS-observed proton-to-helium ratio below 3 GV to mass-to-charge dependence in the heliospheric diffusion coefficient.