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- W2611410318 abstract "Electron holes are suggested to be an important source for generation of electron-cyclotron maser radiation. We demonstrate that electron holes generated in a ring-horseshoe distribution in the auroral-kilometric radiation source region have the capacity to emit sufficiently strong band-limited radiation. The radiation is calculated in the proper frame of a model hole and shown to be strictly perpendicular in this frame. Its bandwidth under auroral conditions is of the order of ∼ 1 kHz, which is a reasonable value. The growth rate of radiation emitted from a single hole is only slightly less than that from the global horseshoe distribution as estimated under conservative assumptions. The interior of the hole produces a weak absorption at slightly higher frequency than emission. The absorptivity is roughly two orders of magnitude below the growth rate thus being weak even when the emission and absorption bands overlap. Transforming to the stationary observer frame it is found that the radiation becomes oblique against the magnetic field while the frequency of emission is Doppler shifted. For approaching holes the frequencies may even exceed the local electron cyclotron frequency." @default.
- W2611410318 created "2017-05-12" @default.
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- W2611410318 date "2011-06-01" @default.
- W2611410318 modified "2023-09-27" @default.
- W2611410318 title "Electron-cylotron maser radiation from electron holes" @default.
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