
doi: 10.1063/1.42747
handle: 11858/00-001M-0000-0014-F229-2
Observations in the Earth’s magnetosphere provide the unique opportunity of investigating particle acceleration in situ. In comparison with measurements in the tail of the Earth’s magnetosphere we discuss the scaling laws of acceleration in current sheets and due to reconnection. We show how different processes provide energy gains at all observed energy levels, up to several MeV. Extrapolating the obtained scaling laws to astronomical scales we demonstrate that reconnection should be relevant for cosmic particle acceleration in general.
Sun and Heliosphere, Theory: Sim Sol Sys Plasma, Planets and Comets
Sun and Heliosphere, Theory: Sim Sol Sys Plasma, Planets and Comets
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