# Tag Info

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 ...