Three-component electron models with Maxwellian core and Kappa halo/strahl predict excitation and interplay of whistler and firehose heat-flux instabilities triggered by core-strahl and halo-strahl drifts, unlike two-component models.
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Modeling complex plasma instabilities in space plasmas - Three-component electron formalism of heat-flux instabilities
Three-component electron models with Maxwellian core and Kappa halo/strahl predict excitation and interplay of whistler and firehose heat-flux instabilities triggered by core-strahl and halo-strahl drifts, unlike two-component models.