In electromagnetically driven kinetic plasmas, super-Debye turbulence yields universal v^{-5} tails via Debye screening, producing kappa-like distributions that invert temperature profiles in the solar corona.
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Non-thermal particle acceleration in multi-species kinetic plasmas: universal power-law distribution functions and temperature inversion in the solar corona
In electromagnetically driven kinetic plasmas, super-Debye turbulence yields universal v^{-5} tails via Debye screening, producing kappa-like distributions that invert temperature profiles in the solar corona.