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- W2076970448 abstract "[1] This paper describes results from ensembles of hybrid simulations of steady, homogeneous, collisionless plasmas characterized by average solar wind parameters near 1 AU upon which damped, resonant Alfven-cyclotron fluctuations are imposed. The applied fluctuations propagate parallel to the background magnetic field B o . The ensembles yield late-time proton and alpha particle responses to such fluctuations as functions of the initial magnitude of the applied fluctuating magnetic field energy and the initial ν αp /ν A (where ν αp is the alpha/proton relative speed and ν A is the Alfven speed). The simulations show a strong, consistent negative correlation between the alpha temperature anisotropy T? α /T ∥α (where the directional subscripts refer to directions perpendicular and parallel to By) and ν αp /ν A . On average the simulations also show a weaker, positive correlation between the proton temperature anisotropy and ν αp /ν A . Both correlations are in agreement with statistical observations from the solar wind near 1 AU, thereby confirming earlier conclusions that such observations are signatures of Alfvencyclotron scattering of ions in the solar wind." @default.
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- W2076970448 date "2006-01-01" @default.
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- W2076970448 title "Alfvén-cyclotron scattering of solar wind ions: Hybrid simulations" @default.
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- W2076970448 doi "https://doi.org/10.1029/2005ja011552" @default.
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