3 edition of Quenching of the beam-plasma instability by 3-D spectra of large scale density fluctuations found in the catalog.
Quenching of the beam-plasma instability by 3-D spectra of large scale density fluctuations
|Statement||L. Muschietti, M.V. Goldman, and D. Newman.|
|Series||NASA contractor report -- NASA CR-175967.|
|Contributions||United States. National Aeronautics and Space Administration.|
|The Physical Object|
It is shown that the gas motions connected with the large scale density perturbations at z approximately must lead to the generation of secondary fluctuations of microwave background. The contribution of the rich clusters of galaxies and young galaxies to the fluctuations of microwave background is also estimated. Firehose Instability In Chap. 9 of our companion book, Basic Space Plasma Physics, we found that a plasma can support low-frequency large-scale Alfv´en and magnetosonic waves far below the electron- and ion-cyclotron frequencies, but did .
National Tech- nology Information Service, Springfield, Virginia, U55 pp. Progress Report on the Development of a Large- Scale Conditional Consistent Economic and Man- power Forecasting Model. Center for Advanced Computation, Urbana, Illinois, 31 pp. Occupational Manpower Impacts of Shifting National Priorities. As a result, the threading dislocation density, measured by large area atomic force microscopy and cathodoluminescence scans, is reduced from x10(9) to x10(7) cm(-2). This nearly two orders of magnitude reduction is attributed to dislocation blocking and bending by the unique interface between GaN and silica microspheres.
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Get this from a library. Quenching of the beam-plasma instability by 3-D spectra of large scale density fluctuations. [L Muschietti; United States. National Aeronautics and Space Administration.].
Frontiers in Dusty Plasmas (PRI). This instability is a large amplitude relaxation type oscillation of the plasma potential as well as of the plasma density.
PRI-like oscillations can be observed in any low density current carrying bounded plasma system. General relations for the correlation functions of electron density fluctuations.
Early out-of-equilibrium beam-plasma evolution M.-C. Firpo, 1 A. Lifschitz, 2 E. Lefebvre, 3 and C. Deutsch 4 1 Lab oratoir e de Physique et Te chnolo gie des Plasmas (CNRS UMR ). PDF | We perform an experimental and theoretical study to investigate the interaction between an external harmonic excitation and a self-excited | Find, read and cite all the research you need.
Work on characterizing the effect of thermal conduction on micron-scale electron beam filaments is ongoing. A characteristic of fast electrons generated by laser–solid interactions is the large angular spread they posses as they enter the solid.
Experimentally, a range of divergence half-angles have been measured, from 20° to 50° [40, An externally excited ion wave in an ion beam‐plasma system was found to grow spatially in the case where the ion beam velocity is nearly equal to an ion acoustic velocity. The phase velocity and growth rate are in good agreement with the results based on the kinetic dispersion by: 9.
Full text of "Wave Propagation in Materials for Modern Applications" See other formats. However, quantum fluctuations of these dipole moments preclude the development of conventional magnetic order even at temperature far below the scale of inter-site interactions.
The result is a quantum material with unique macroscopic properties driven by quantum coherence and entanglement. On their Allocation Year ERCAP Request Forms Principal Investigators reported 1, refereed publications (published or in press) - as well as publications submitted to refereed journals - for the preceding 12 months, based on using, at least in part, NERSC resources.
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Deng et al., Phys. Rev. Lett. 96, (). Collective instabilities and beam-plasma interactions in intense heavy ion beam, Ronald C. Davidson, et al., Phys. Rev. ST Accel.
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In: Journal of the Physical Society of Japan. 82,p. - [Electron-phonon systems, quantum phonons, quantum-fluctuation-driven.
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4. AFE0 scattering 1 theory 2 nuclear 3 magnetic 4 energy 5 effect 6 electron 7 absorption 8 resonance 9 structure 10 spectrum 11 decay 12 electrons 13 field 14 cross 15 crystals 16 effects 17 properties 18 neutrons 19 states 20 spectra 21 model 22 neutron 23 production .\\ arXiv From: Max Tegmark Date: Mon, 31 Aug GMT (kb) Title: Omniscopes: Large Area Telescope Arrays with only N log N Computational.