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- W2560581640 abstract "The Cosmic Ray anisotropy is a key element in the quest to find t he origin of the enigmatic particles. A well known problem is that, although most of the likely sources are in the Inner Galaxy, the direction from which the lowest energy particles (less t han about 1 PeV) come is largely from the Outer Galaxy. We show that this can be understood taking into account a possible reflection of charged particles by ’walls’ in the Interstellar Medium or/ and as a temporary phenomenon after the shock wave from the supernova explosion passed the Earth. This effect is too subtle to be explained by an ordinary diffusion theory and becomes apparent within the frames of the non-local relativistic transport theory, which involves conception s of free motion velocity and path lengths with probability distributions of non-exponential type ta ken for a turbulent interstellar medium." @default.
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- W2560581640 date "2016-08-18" @default.
- W2560581640 modified "2023-09-23" @default.
- W2560581640 title "A Look at the Cosmic Ray Anisotropy with the Nonlocal Relativistic Transport Approach" @default.
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- W2560581640 doi "https://doi.org/10.22323/1.236.0463" @default.
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