A kinetic model with boundary-matched Coulomb diffusion plus oblique-whistler quasilinear scattering predicts the strahl distribution and a Coulomb-to-whistler broadening threshold near 200 eV at 1 AU.
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Kinetic theory of the electron strahl in the solar wind
A kinetic model with boundary-matched Coulomb diffusion plus oblique-whistler quasilinear scattering predicts the strahl distribution and a Coulomb-to-whistler broadening threshold near 200 eV at 1 AU.