Relativistic particles trapped in a star's dipole magnetosphere with synchrotron losses fall into three classes (oscillating, freezing, precipitating), producing distinctive optical and X-ray emission maps.
Alfven,Cosmical electrodynamics (1950)
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Relativistic van Allen belts in magnetospheres of pulsars and white dwarfs
Relativistic particles trapped in a star's dipole magnetosphere with synchrotron losses fall into three classes (oscillating, freezing, precipitating), producing distinctive optical and X-ray emission maps.