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  • 1
    Digitale Medien
    Digitale Medien
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 73 (1993), S. 4181-4196 
    ISSN: 1089-7550
    Quelle: AIP Digital Archive
    Thema: Physik
    Notizen: The resistive hose instability can disrupt propagation of self-pinched beams in dense gas. To reduce growth of the instability, beams can be conditioned prior to propagation. The objectives of beam conditioning are to center the beam in order to reduce initial transverse perturbations which seed the hose instability, and to "tailor'' the beam emittance in order to detune the head-to-tail coherence of the instability. Emittance tailoring can be performed by transporting the beam through a "passive ion-focused regime'' (IFR) cell, a low-pressure gas cell that induces a head-to-tail taper of the beam radius. The radius taper is then converted to an emittance taper by passing the beam through a thick exit foil which scatters the beam. Beam centering can be accomplished by transporting the beam through either: (i) a passive IFR cell that is narrow enough to provide wall guiding, or (ii) a laser-ionized "active'' IFR cell, or (iii) a wire cell in which the centering is provided by a current-carrying wire. Axisymmetric particle simulation studies of IFR tailoring cells, alone and in tandem with each of these types of centering cells, and also the effect of supplementary focusing lenses and conducting foils are reported. The parameter choices that are conducive to effective beam conditioning are discussed. The emphasis is on conditioning configurations and beam parameters that have actually been tested in experiments with the Advanced Test Accelerator and SuperIBEX accelerator.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
    Digitale Medien
    Digitale Medien
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 7 (2000), S. 3851-3861 
    ISSN: 1089-7674
    Quelle: AIP Digital Archive
    Thema: Physik
    Notizen: Dust grains in plasma acquire a large negative charge, and can constitute a strongly coupled system. If the plasma is stationary, the plasma-mediated electrostatic potential around a single grain can be calculated by orbital-motion-limited (OML) theory, including ion absorption at the grain surface. This potential is repulsive at all ranges, and falls off as r−2 at long range. Nonlinear modifications occur when there are several grains, but the interaction is still repulsive. If the plasma is streaming by the grains, each grain generates a wake field potential which can be calculated via linear response theory, and which attracts other grains to stationary points behind the grain. There is in addition an attractive force between grains, due to ion-impact momentum deposition. In certain parameter regimes, this "shadowing" force can yield a weak net attraction at long range. Trapped-ion effects are significant at high plasma density, but have not yet been calculated. © 2000 American Institute of Physics.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 3
    Digitale Medien
    Digitale Medien
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 75 (1994), S. 3278-3293 
    ISSN: 1089-7550
    Quelle: AIP Digital Archive
    Thema: Physik
    Notizen: The electron beams used commercially for welding and materials processing operate either in vacuum or at very short range in air, which limits system productivity and the types of applications allowed. We show here that these restrictions can be relaxed considerably by raising both the beam energy and current, from under 200 keV to a few MeV and from under 1 A to a few kA, respectively, with the beam chopped into short pulses to preserve average beam power. This technology is made possible by the recent development of high-power generators that produce low-emittance beams with radii as small as 1 mm, pulse lengths of tens of ns, and pulse repetition rates up to several kHz. After studying the constraints imposed by gas scattering and the resistive hose instability, we conclude that high-power beams can propagate and remain tightly pinched over tens of cm in ambient air, without need of external guide fields. Equally important, the propagation requirements can be significantly relaxed by using a narrow conducting pipe filled with air or another gas to guide the beam to the workpiece.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 4
    Digitale Medien
    Digitale Medien
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 62 (1987), S. 1171-1180 
    ISSN: 1089-7550
    Quelle: AIP Digital Archive
    Thema: Physik
    Notizen: A relativistic electron beam propagating in a dense gas typically ionizes the gas weakly, and the resulting plasma conductivity evolution strongly influences beam stability properties. We note in this paper that the electric field E and the plasma electron temperature Te usually decrease with distance ζ behind the beam head; as a result, the plasma electron neutral collision frequency νm decreases with ζ, which depresses the conductivity σ in the front of the beam and increases σ further back in the beam. We find that this variation of νm, which has generally been ignored in previous models, substantially modifies beam instability evolution. Hose instability growth tends to increase very rapidly in the beam head and taper off to an asymptotic value for large ζ, in contrast to the pure power law growth seen when νm and dσ/dζ are assumed to be constant. A second effect arises from local decreases in the perturbed conductivity σ, produced by perturbed electric field driven increases in the local collision frequency. This destabilizing effect causes the beam to behave as if the monopole conductivity σ0 were replaced by σ*=σ0 [1−(E/νm)(∂νm/∂E)]≡σ0(1−q¯). Analytical models for the case of constant q¯ illustrate the pattern of rapid hose instability growth in the beam head followed by a "plateau'' in hose amplitudes that is also observed in hose simulations with the VIPER model. The destabilizing effect of variable νm on the perturbed conductivity also occurs for the resistive sausage instability. However, the model calculation presented here shows that the threshold for sausage instability is not likely to be reached for reasonable beam and plasma parameters.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 5
    Digitale Medien
    Digitale Medien
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 3 (1991), S. 1521-1531 
    ISSN: 1089-7666
    Quelle: AIP Digital Archive
    Thema: Physik
    Notizen: A solvable model is developed for the linearized sausage mode within the context of resistive magnetohydrodynamics. The model is based on the assumption that the fluid motion of the plasma is self-similar, as well as several assumptions pertinent to the limit of wavelength long compared to the pinch radius. The perturbations to the magnetic field are not assumed to be self-similar, but rather are calculated. Effects arising from time dependences of the z-independent perturbed state, e.g., current rising as tα, Ohmic heating, and time variation of the pinch radius, are included in the analysis. The formalism appears to provide a good representation of "global'' modes that involve coherent sausage distortion of the entire cross section of the pinch, but excludes modes that are localized radially, and higher radial eigenmodes. For this and other reasons, it is expected that the model underestimates the maximum instability growth rates, but is reasonable for global sausage modes. The net effect of resistivity and time variation of the unperturbed state is to decrease the growth rate if α(approximately-less-than)1, but never by more than a factor of about 2. The effect is to increase the growth rate if α(approximately-greater-than)1.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 6
    Digitale Medien
    Digitale Medien
    [S.l.] : American Institute of Physics (AIP)
    Physics of Fluids 31 (1988), S. 2349-2361 
    ISSN: 1089-7666
    Quelle: AIP Digital Archive
    Thema: Physik
    Notizen: A relativistic electron beam propagating through dense gas may evolve into a variety of current density profiles Jb(r) depending on the beam temperature T and plasma current profile Jp(r). Four broad classes of equilibria are discernible in particle simulations: (1) Bennett-like or compact, (2) core and halo, (3) on-axis hollowed, and (4) off-axis hollowed. The qualitative features of each class are reproduced in a simple analytical model that assumes an isothermal beam and a Bennett plasma current profile and iterates about an initial ansatz of a Bennett beam current profile. Bennett-like equilibria are produced when the return current fraction f is small or when T/TB=1−f, where TB=eIb/2c is the Bennett temperature. For T/TB 〉1−f and moderate or high f, the equilibrium consists of a compact core surrounded by a halo, which may contain most of the beam current. In extreme cases (T/TB(very-much-greater-than)1−f and f close to unity) an off-axis density minimum occurs. (This is also referred to as off-axis hollowing.) For T/TB〈1−f and moderate or high f, the beam core is broader than the plasma current profile, and on-axis hollowing results. Simulations with the ultrarelativistic sarlac simulation code [Bull. Am. Phys. Soc. 31, 1429 (1986); Phys. Fluids 29, 3056 (1986)] exhibit all of these types of equilibria. sarlac also treats transverse beam distortion arising from the resistive hose instability. Hose instability growth appears to be strongly enhanced when halos are generated.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 7
    Digitale Medien
    Digitale Medien
    New York, NY : American Institute of Physics (AIP)
    Physics of Fluids 5 (1993), S. 1888-1901 
    ISSN: 1089-7666
    Quelle: AIP Digital Archive
    Thema: Physik
    Notizen: A relativistic electron beam, propagating in an underdense ion-focusing channel that is embedded within a broad region of underdense plasma, is shown to be subject to a hose instability due to coupling with plasma electrons at the edge of the pure-ion region. The instability is studied by means of linearized analytic calculations of dispersion relations and asymptotic growth, numerical integrations of the linearized dynamical equations, and three-dimensional particle simulations of the full nonlinear evolution. Three cases are considered: (1) If the plasma density ni0(r), prior to the introduction of the beam, is uniform, the instability is absolute, grows very rapidly, and does not saturate nonlinearly until the thrashing of the beam carries it into the quasineutral plasma region. Thus the instability prevents orderly beam propagation. (2) If ni0(r) consists of a central channel with constant density, surrounded by lower density plasma, the instability is again absolute, but with a reduced growth rate. Over a limited range, propagation without significant disturbance is possible. If the propagation range is long, the instability is stabilized by phase mixing when the beam leaves the channel. The beam then is recentered, with consequent emittance growth. (3) If ni0(r) consists of a central channel with a rounded density profile, surrounded by lower density plasma, the instability is convective in the beam frame. If parameters are chosen correctly, the instability does not significantly inhibit long range propagation.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 8
    Digitale Medien
    Digitale Medien
    Springer
    Journal of fusion energy 12 (1993), S. 403-404 
    ISSN: 1572-9591
    Quelle: Springer Online Journal Archives 1860-2000
    Thema: Energietechnik
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 9
    Publikationsdatum: 1968-06-05
    Print ISSN: 0031-899X
    Digitale ISSN: 1536-6065
    Thema: Physik
    Publiziert von American Physical Society
    Standort Signatur Erwartet Verfügbarkeit
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  • 10
    Publikationsdatum: 2001-06-04
    Print ISSN: 0031-9007
    Digitale ISSN: 1079-7114
    Thema: Physik
    Publiziert von American Physical Society
    Standort Signatur Erwartet Verfügbarkeit
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