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Background Info The first thing to do is to consider the relativistic gyrofrequency, given by: $$ \Omega_{cs} = \frac{ Z_{s} \ e \ B_{o} }{ \gamma \ m_{s} } $$ where $Z_{s}$ is the charge state of species $s$, $e$ is the fundamental charge, $B_{o}$ is the quasi-static magnetic field magnitude, $\gamma$ is the relativistic Lorentz factor, and $m_{s}$ is the ...

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