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Nonlinear Plasma Theory
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The article was published on 1969-01-01 and is currently open access. It has received 1030 citations till now. The article focuses on the topics: Ion acoustic wave & Acoustic wave equation.read more
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Drift-wave spectra in plasmas with magnetic shear
André Rogister,Günter Hasselberg +1 more
TL;DR: The nonlinear radial eigenmode equation governing the evolution of drift waves in a weakly turbulent state is obtained under the assumption that ion nonlinear scattering (nonlinear ion Landau damping) is the dominant saturation mechanism as mentioned in this paper.
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Artificial Aurora Experiments and Application to Natural Aurora
TL;DR: In this paper, a review of the effects observed during injections of powerful electron beams from sounding rockets into the upper atmosphere is given, where data come from in situ particle and wave measurements near a beam emitting rocket and ground-based optical, wideband radiowave, and radar observations.
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Modulational instability of strongly dispersive drift waves and formation of convective cells
TL;DR: In this paper, the two-dimensional self-modulation instability of strongly dispersive drift waves is investigated in order to explain convective cell excitation in drift wave turbulence, and it is shown that the nonlinear evolution of the convective cells can lead to anomalous particle losses.
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Anomalous cooling of coronal loops with turbulent suppression of thermal conduction
TL;DR: In this article, the authors investigate the impact of turbulent suppression of parallel heat conduction on the cooling of post-flare coronal loops and identify four main cooling scenarios depending on the value of the mean free path lT associated with the turbulent scattering process.
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On the origin of the drifting subpulses in radio pulsars
TL;DR: In this paper, a model for the radio emission of pulsars with well-organized drifting subpulses is presented, where drift waves are generated at shorter wavelengths, and their non-linear evolution favours accumulation in a specific azimuthal eigenmode with an integral number, m, of nodes encircling the magnetic pole.