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Magnetically-confined plasmas, created and heated by electromagnetic fields near the electron gyrofrequency, can support several modes of instability driven by inherent temperature anisotropy or possible loss-cone effects. If T || ≪ T ⊥ , both electrostatic and electromagnetic waves can grow in time; while if T || →T ⊥ , electrostatic waves at the hybrid frequency can be driven unstable by the loss-cone effect. Here the relevant known criteria are reviewed, and several new criteria to describe the stabilization of the temperature-anisotropy modes as T || → T ⊥ , are developed. The results of a detailed analysis of the electrostatic loss-cone mode, for which temporal growth rates greater than anticipated electron bounce frequencies are obtained only for electron densities near microwave cut-off are also reported.
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Guest et al. (1971) studied this question.
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