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Showing 1 to 16 of 16 for “"wave-particle interactions"”.

  1. Wave-particle interactions in the solar wind and solar flares

    <p>Resonant interactions between particles and plasma waves play an important role in both the solar wind and solar flares. The dynamics of plasma turbulence in these settings controls the strength of the interactions, by determining the amplitudes of the small-scale electromagnetic fluctuations …

    unh-thes Repository record for Wave-particle interactions in the solar wind and solar flares (opens in a new tab)

  2. Analysis of wave-particle interactions in a beam plasma system

    Submitted by Megan O'Donnell (mnodonn2@illinois.edu) on 2012-04-19T21:35:39Z No. of bitstreams: 1 1974_winske.pdf: 5484975 bytes, checksum: 7a34a5388d0ccccc4a5eb68ad137fc0e (MD5)

    uiuc Repository record for Analysis of wave-particle interactions in a beam plasma system (opens in a new tab)

  3. Wave-particle interactions and the dynamics of the solar wind.

    Thesis. 1978. Ph.D.--Massachusetts Institute of Technology. Dept. of Physics.

    mit Repository record for Wave-particle interactions and the dynamics of the solar wind. (opens in a new tab)

  4. Experimental study of wave-particle interactions in a beam-plasma system

    Submitted by William Weathers (weathrs2@illinois.edu) on 2012-04-22T20:39:41Z No. of bitstreams: 1 1975_taylor.pdf: 2603581 bytes, checksum: 6f514d312a0be59d2f3d34753c73e36b (MD5)

    uiuc Repository record for Experimental study of wave-particle interactions in a beam-plasma system (opens in a new tab)

  5. STABILITY OF UPGOING AURORAL ION BEAMS AT 33 R(E) (PLASMA, MAGNETOSPHERE, WAVE-PARTICLE INTERACTIONS)

    … ions having been decelerated. This suggests wave-particle interactions at lower altitudes enabled the transfer of energy from the hydrogen to the oxygen. Maxwellian fits to the beam distributions are used to study the stability of the beams with respect to various low frequency …

    unh-thes Repository record for STABILITY OF UPGOING AURORAL ION BEAMS AT 33 R(E) (PLASMA, MAGNETOSPHERE, WAVE-PARTICLE INTERACTIONS) (opens in a new tab)

  6. Electron acceleration and loss caused by wave-particle interactions in the Van Allen radiation belts

    … the interaction between electrons and plasma waves. The most important plasma waves are chorus, plasmaspheric hiss, and EMIC waves. Here, new statistical models of the diffusion coefficients for these waves are presented, which considerably improve existing models. Among others, they benefit …

    the-open-u Repository record for Electron acceleration and loss caused by wave-particle interactions in the Van Allen radiation belts (opens in a new tab)

  7. Harmonic generation and parametric excitation in a beam-plasma system

    Harmonic generation by wave-wave and wave-particle interactions and parametric excitation of plasma and ion-acoustic waves by a beam-plasma instability are studied, theoretically and experimentally, in a cold beam-plasma system. The dispersion relations for plasma and ion-acoustic waves are …

    uiuc Repository record for Harmonic generation and parametric excitation in a beam-plasma system (opens in a new tab)

  8. Remote sensing of Jupiter's magnetospheric dynamics

    … hot plasma injections. It was suggested that wave-particle interactions are responsible for the scattering of electrons in this region. A third study investigated the auroral response to co-rotating interaction regions and solar wind compression. It was shown that in there are both high …

    lancaster Repository record for Remote sensing of Jupiter's magnetospheric dynamics (opens in a new tab)

  9. Modeling of Outer Radiation Belt Electron Scattering due to Spatial and Spectral Properties of ULF Waves

    The research presented in this thesis covers wave-particle interactions for relativistic (0.5-10 MeV) electrons in Earth's outer radiation belt (r = 3-7 RE, or L-shells: L = 3-7) interacting with magnetospheric Pc-5 (ULF) waves. This dissertation focuses on ideal models for short and long term …

    wvu Repository record for Modeling of Outer Radiation Belt Electron Scattering due to Spatial and Spectral Properties of ULF Waves (opens in a new tab)

  10. Controlled precipitation of energetic Van Allen belt protons by electromagnetic ion cyclotron (EMIC) waves : scientific and engineering implications

    … storms, cosmic rays and other processes. These particles can rapidly damage the space systems orbiting the inner region, limiting access to Low Earth Orbit (LEO). Decades of modeling and observations, however, show that naturally generated ULF/VLF waves have the capability of precipitating …

    mit Repository record for Controlled precipitation of energetic Van Allen belt protons by electromagnetic ion cyclotron (EMIC) waves : scientific and engineering implications (opens in a new tab)

  11. Occurrence Statistics and Driving Mechanisms of Ionospheric Ultra-Low Frequency Waves Observed by SuperDARN Radars

    Ultra-low frequency (ULF; 1 mHz - 1 Hz) waves are known to play an important role in the transfer of energy from the solar wind to Earth's magnetosphere and ionosphere. The Super Dual Auroral Radar Network (SuperDARN) is an international network consisting of 35 low-power high frequency (HF: 3-30 …

    vt Repository record for Occurrence Statistics and Driving Mechanisms of Ionospheric Ultra-Low Frequency Waves Observed by SuperDARN Radars (opens in a new tab)

  12. Nonlinear Evolution of Mirror Instability in the Earth's Magnetosheath in PIC Simulations

    … of mirror instability using expanding box Particle-in-Cell simulations. We change the plasma conditions by artificially enlarging the simulation box over time to make the plasma mirror stable and investigate the final nonlinear state of the mirror structures. We show that the direct …

    unh-thes Repository record for Nonlinear Evolution of Mirror Instability in the Earth's Magnetosheath in PIC Simulations (opens in a new tab)

  13. Understanding how low energy electrons control the variability of the Earth's electron radiation belts

    … On the timeframe of hours, both the energy and particle flux of the radiation belts can change by orders of magnitude. Variations in the high energy relativistic electron flux depend on transport, acceleration, loss processes, and importantly, on the lower energy seed (10s – 100s keV) …

    cambridge Repository record for Understanding how low energy electrons control the variability of the Earth's electron radiation belts (opens in a new tab)

  14. Impacts of Anisotropy, Wave Heating, and Neutral Winds on High-Latitude Ionospheric Dynamics

    … transverse ion acceleration by broadband ELF waves can give the upflowing ions sufficient energy for the mirror force to propel these ions to escape into the magnetosphere (ion outflow). In order to accurately examine the connection between upflow and outflow processes, a new two dimensional, …

    embry-riddle Repository record for Impacts of Anisotropy, Wave Heating, and Neutral Winds on High-Latitude Ionospheric Dynamics (opens in a new tab)