Galactic Turbulence and the Origins of Cosmic Rays and the Galactic Magnetic Field

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Abstract
A new absorption mechanism is discussed in relation to the turbulence of the interstellar gas in the presence of a magnetic field. It is evaluated and compared with ordinary viscous absorption in different types of interstellar gas. Wherever there is a proportion, even though very small, of neutral atoms (helium being most likely) the new mechanism predominates for waves of length comparable with one parsec or more.

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