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Particle Acceleration and Heating by Turbulent Reconnection

By Loukas Vlahos and others
Turbulent flows in the solar wind, large scale current sheets, multiple current sheets, and shock waves lead to the formation of environments in which a dense network of current sheets is established and sustains "turbulent reconnection". We constructed a 2D grid on which a number of randomly chosen grid points... Show more
April 19, 2016
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Particle Acceleration and Heating by Turbulent Reconnection
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