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Convective Oscillations of Cosmic Rays
Turbulent motion of the background plasma can introduce fluctuations in the spatial distribution of cosmic rays (CRs). For an ensemble-averaged Gaussian CR distribution with a width $ Λ\left( t,p \right) $ at time $ t $ and momentum $ p $, it is found that $ P_\text{s}\left( t,k,p \right) $ and $ P_
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