Beam‐plasma interaction in randomly inhomogeneous plasmas and statistical properties of small‐amplitude Langmuir waves in the solar wind and electron foreshock

Beam‐plasma interaction in randomly inhomogeneous plasmas and statistical properties of small‐amplitude Langmuir waves in the solar wind and electron foreshock

Source :

• Journal of Geophysical Research: Space Physics [ 0148-0227 ] ; 2007-10.

Descripteurs français

• Pascal (Inist)
  • Amont onde choc, Amplitude, Densité spectrale, Diffusion onde, Diffusion(transport), Distribution densité, Etude expérimentale, Faisceau électronique, Fluctuation densité, Inhomogénéité, Instabilité, Interaction faisceau plasma, Modèle numérique, Onde électrostatique, Paquet onde, Particule, Perturbation densité, Planète Terre, Plasma hétérogène, Plasma inhomogène, Propagation onde, Résonance, Simulation numérique, Vent solaire.
• Wicri :
  • topic : Simulation, énergie des vagues.

English descriptors

• KwdEn :
  • Absolute value, Amplitude, Amplitude distribution, Angular diffusion, Angular width, Astrophys, Atmospheric physics, Beam plasma interaction, Beam speed, Blue curve, Blue line, Blue lines, Cairn, Central limit theorem, Clumpy langmuir waves, Cluster spacecraft, Corresponding data point, Corresponding thresholds, Czech republic, Density distribution, Density fluctuation, Density fluctuations, Density perturbation, Density perturbations, Different factors, Different values, Differential equation, Diffusion, Diffusion coefficient, Diffusion effect, Dimensionless parameters, Distribution function, Earth, Effective growth rate, Effective number, Electric field, Electron beam, Electron foreshock, Electrostatic wave, Empirical distribution, Empirical distributions, Error function, Experimental data, Finite regions, First test, Fluctuation, Foreshock, Foreshock boundary, Foreshock langmuir waves, Frequency range, General case, Geophys, Green curve, Green line, Group velocity, Growth rate, Gurnett, High frequencies, Impulse rate, Inhomogeneity, Inhomogeneous, Inhomogeneous plasma, Inhomogeneous plasmas, Instability, Integral equation, Intense langmuir waves, Intensive studies, Interplanetary medium, Isee propagation experiment, Kellogg, Krasnoselskikh, Langmuir, Langmuir wave amplitudes, Langmuir wave packets, Langmuir waves, Large amplitude, Large amplitudes, Lett, Linear interaction, Logarithm, Lognormal distribution, Magnetic field, Main reason, Maximum likelihood, Middle panel, Middle panels, Model distributions, Moment technique, Nimp, Nonlinear, Nonlinear processes, Normal distribution, Normal distributions, Null hypothesis, Numerical model, Numerical modeling, Numerical simulations, Other hand, Packet, Parameter, Pearson curves, Pearson diagram, Pearson distributions, Pearson parameters, Pearson technique, Pearson type, Plasma, Plasma density, Plasma density profile, Plasma inhomogeneities, Plasma oscillations, Plasma waves, Positive growth rate, Present paper, Previous section, Probability density function, Probability distribution, Probability distributions, Radio sources, Random density inhomogeneities, Random inhomogeneities, Relative role, Shot noise, Significance level, Similar problem, Simulation, Small ratios, Solar physics, Solar radio bursts, Solar wind, Spacecraft, Spatial evolution, Spatial scales, Spatial variations, Spectral density, Spectral density distributions, Spectral energy density, Statistical ensemble, Statistical properties, Statistical scatter, Stochastic, Stochastic growth, Stochastic growth theory, Stochastic process, Stochastic wave growth, Terrestrial electron foreshock, Typical conditions, Typical value, Unstable plasma, Upstream shock wave, Wave, Wave amplitude, Wave amplitudes, Wave energies, Wave energy, Wave energy density, Wave intensity, Wave numbers, Wave packet, Wave packets, Wave propagation, Wave spectra, Wave statistics, Wave vector, amplitude, digital simulation, experimental studies, inhomogeneity, instability, numerical models, particles, resonance, solar wind, wave scattering.
• Teeft :
  • Absolute value, Amplitude, Amplitude distribution, Angular diffusion, Angular width, Astrophys, Atmospheric physics, Beam speed, Blue curve, Blue line, Blue lines, Cairn, Central limit theorem, Clumpy langmuir waves, Cluster spacecraft, Corresponding data point, Corresponding thresholds, Czech republic, Density fluctuations, Density perturbations, Different factors, Different values, Differential equation, Diffusion coefficient, Diffusion effect, Dimensionless parameters, Distribution function, Effective growth rate, Effective number, Electric field, Electron beam, Electron foreshock, Empirical distribution, Empirical distributions, Error function, Experimental data, Finite regions, First test, Fluctuation, Foreshock, Foreshock boundary, Foreshock langmuir waves, Frequency range, General case, Geophys, Green curve, Green line, Group velocity, Growth rate, Gurnett, High frequencies, Impulse rate, Inhomogeneity, Inhomogeneous, Inhomogeneous plasma, Inhomogeneous plasmas, Instability, Integral equation, Intense langmuir waves, Intensive studies, Interplanetary medium, Isee propagation experiment, Kellogg, Krasnoselskikh, Langmuir, Langmuir wave amplitudes, Langmuir wave packets, Langmuir waves, Large amplitude, Large amplitudes, Lett, Linear interaction, Logarithm, Lognormal distribution, Magnetic field, Main reason, Maximum likelihood, Middle panel, Middle panels, Model distributions, Moment technique, Nimp, Nonlinear, Nonlinear processes, Normal distribution, Normal distributions, Null hypothesis, Numerical model, Numerical modeling, Numerical simulations, Other hand, Packet, Parameter, Pearson curves, Pearson diagram, Pearson distributions, Pearson parameters, Pearson technique, Pearson type, Plasma, Plasma density, Plasma density profile, Plasma inhomogeneities, Plasma oscillations, Plasma waves, Positive growth rate, Present paper, Previous section, Probability density function, Probability distribution, Probability distributions, Radio sources, Random density inhomogeneities, Random inhomogeneities, Relative role, Shot noise, Significance level, Similar problem, Simulation, Small ratios, Solar physics, Solar radio bursts, Solar wind, Spacecraft, Spatial evolution, Spatial scales, Spatial variations, Spectral density distributions, Spectral energy density, Statistical ensemble, Statistical properties, Statistical scatter, Stochastic, Stochastic growth, Stochastic growth theory, Stochastic process, Stochastic wave growth, Terrestrial electron foreshock, Typical conditions, Typical value, Unstable plasma, Wave, Wave amplitude, Wave amplitudes, Wave energies, Wave energy, Wave energy density, Wave intensity, Wave numbers, Wave packet, Wave packets, Wave propagation, Wave spectra, Wave statistics, Wave vector.

Abstract

• https://api.istex.fr/document/AB59685298F9E5662A9D6717EF2164D52E1E1F5F/fulltext/pdf

Affiliations:

• Australie, France, République tchèque, États-Unis
• Bohême centrale, Centre-Val de Loire, Iowa, Nouvelle-Galles du Sud, Région Centre
• Iowa City, Orléans, Prague, Sydney
• Université d'Orléans, Université de Sydney, Université de l'Iowa

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