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- W2072290980 abstract "The anisotropy introduced by the motion of an observer with velocity V through a particle or photon flux is derived from the Lorentz-invariance of distribution functions in phase space. The invariance of the black-body distribution function leads to a ≅1 + (V/c) cos θ dependence of the temperature of the 3°K thermal background radiation. For massive particles whose speed, ν, is much greater than V, the Compton-Getting anisotropy — (d(lnƒ)/ d(ln p))V/ν is added to the angular part of the distribution function, and the isotropic part is unchanged, to order V/ν. The cosmic-ray proton spectrum at solar minimum is observed to have a region where the Compton-Getting anisotropy is zero. The Lorentz-invariance of the volume element in phase space, and the consequent invariance of distribution functions, is demonstrated in the Appendix." @default.
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- W2072290980 date "1970-01-01" @default.
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- W2072290980 title "The compton-getting effect for cosmic-ray particles and photons and the Lorentz-invariance of distribution functions" @default.
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- W2072290980 doi "https://doi.org/10.1016/0032-0633(70)90064-4" @default.
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