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- W2019901730 abstract "Using Lerche's turbulent kinematic-dynamo equations we calculate the mean square displacement of the fluctuating component of the galactic magnetic field and hence the cosmic-ray diffusion coefficient. We find that the radial variation of the diffusion coefficient thus calculated agrees well with that deduced from the γ-ray observations, provided we use a mean velocity field which includes a compressional component, which according to Burton is also responsible for the observed peaking of H II regions, CO, supernova remnants and γ-rays at about 6 kpc from the Galactic Centre." @default.
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- W2019901730 date "1979-05-01" @default.
- W2019901730 modified "2023-09-27" @default.
- W2019901730 title "Cosmic-ray diffusion and the turbulent galactic magnetic field" @default.
- W2019901730 doi "https://doi.org/10.1093/mnras/187.1.23" @default.
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