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Electrons traveling along magnetic field lines from Jupiter to Io, driven byquasi-linear diffusion (QLD), emit synchrotron radiation. By using the smallangle approximation, the kinematic equation for the particle distribution givesus the mean pitch angle value. We described how these ultrarelativisticelectrons emit radiation in the GHz range when subjected to external forces.

Radio emission in the Jovian magnetosphere driven by the quasi-linear diffusion