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  • American Physical Society  (340)
  • American Institute of Physics  (121)
  • American Institute of Physics (AIP)  (31)
  • 1
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 7 (2000), S. 1623-1629 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Relaxation is the result of turbulence in a plasma that behaves essentially as an ideal conducting fluid, but has a small resistivity and viscosity. These small effects are locally enhanced by the turbulence and lead to reconnection of magnetic field lines. This destroys an infinity of topological constraints, leaving only the total magnetic helicity as a valid invariant. The plasma therefore rapidly reaches a specific state of minimum energy. This minimum energy "relaxed state" can be calculated from first principles and has many striking features. These depend on the topology of the system. They include spontaneous field reversal, symmetry-breaking and current limitation in toroidal pinches, and flux generation and flux amplification in Spheromaks. In addition the relaxed states can be controlled and maintained by injection of helicity from an external circuit. These features, and the profiles of the relaxed states themselves, have been verified in many laboratory experiments.
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  • 2
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 2 (1995), S. 3925-3925 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The authors contend that incorrect inferences are drawn by Ding Li regarding the sources of error and of the basis function method used in the calculations of toroidally coupled tearing modes. (AIP)
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  • 3
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 6 (1999), S. 2425-2429 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The influence of shear-flow on stability of plasma ballooning modes is important for Tokamak experiments. In a static plasma, the growth rate of ballooning modes is readily determined using the "ballooning transformation," but this is ineffective for plasmas with flow. One then has only the quasi-static approximation. This gives the growth rate in the limit that shear velocity Ω′→0, but no other information on the effect of shear-flow. Furthermore, it is invalid in typical cases because of the intervention of the stable magnetohydrodynamic continuum. In this paper, a simple model is used to investigate the influence of shear-flow on ballooning modes. This shows that the intervention of the continuum leads to a reduction in the growth rate proportional to |Ω′| for small Ω′. This is in accord with some numerical simulations—but contrary to the (Ω′)2 variation expected from a perturbation expansion. In fact, since the effect is nonanalytic in Ω′, it cannot be obtained from a perturbation expansion in Ω′ and an alternative formalism is first developed for dealing with this problem. © 1999 American Institute of Physics.
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  • 4
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 5 (1998), S. 3065-3067 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Transport barriers and transitions between modes of low and high confinement in tokamak plasmas are often attributed to suppression of turbulence by a shear flow related to a plasma gradient, e.g., of density. However, such shear flow is also affected by the second derivative of density. When this is introduced there is no unique relation between flux and gradient—it depends on the source distribution within the plasma and on conditions at the plasma edge (e.g., imposed by the scrape-off layer). This edge gradient must lie within prescribed limits if a stationary plasma profile (which may include an improved confinement zone) is to exist.
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  • 5
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 8 (2001), S. 4062-4072 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The resistive wall mode (RWM) poses a threat to many plasma confinement devices. The continuous rotation of the wall relative to the plasma makes it appear perfectly conducting, because of the skin effect, but this is ineffective if the perturbation locks to the wall. This raises the question of whether a nonuniformly rotating wall is more effective. In this paper we discuss the effect of such nonuniform wall rotation, in both the toroidal and poloidal directions, on resonant and nonresonant RWMs. In the case of toroidal rotation it is shown that at large wall velocity both the resonant and nonresonant RWMs are stabilized, even though the nonresonant mode rotates with the maximum wall velocity. In the case of poloidal rotation RWMs do not lock to the wall and have a complicated behavior at intermediate velocities. However they are again stabilized by large wall velocity. © 2001 American Institute of Physics.
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  • 6
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Review of Scientific Instruments 63 (1992), S. 3551-3555 
    ISSN: 1089-7623
    Source: AIP Digital Archive
    Topics: Physics , Electrical Engineering, Measurement and Control Technology
    Notes: We describe a flexible, inexpensive data acquisition system built for high-precision timing observations of pulsars. The system is designed to interface with a wide variety of radio telescope receiver back ends; it permits standardized measurement techniques and data formats in work carried out at a number of different observatories. Copies of the basic "Mark III'' system are now in regular use at the Arecibo Observatory, Green Bank, and the Very Large Array. We describe the specifications, hardware, and software implementation of the system, and briefly outline some of its current applications.
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  • 7
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Review of Scientific Instruments 67 (1996), S. 2658-2659 
    ISSN: 1089-7623
    Source: AIP Digital Archive
    Topics: Physics , Electrical Engineering, Measurement and Control Technology
    Notes: An out-of-plane detector movement has been built for the detector arm of the surface x-ray diffractometer on the wiggler beam line 9.4 on the synchrotron radiation source at Daresbury Lab. For a relative small cost, it significantly increases the volume of reciprocal space that can be accessed with a corresponding improvement in the accuracy of the determination of the interatomic spacings. © 1996 American Institute of Physics.
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  • 8
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 78 (1995), S. 5356-5361 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: This study uses x-ray photoelectron spectroscopy (XPS) to investigate the nature of the oxide formed on clean Au–Sn binary alloys (ζ and δ phases) and on preforms with the eutectic composition (29 at % Sn) at low O2 pressures (〈10−3 Torr) and at high O2 pressures (up to one atmosphere) at temperatures ranging from room temperature to 200 °C. Sn Auger parameters and XPS angular-resolved data were obtained in addition to the core binding energies to identify the oxide layer. The oxidation of the Au–Sn alloys is basically similar to the oxidation of metallic Sn. The Auger parameter indicates that with low-pressure oxidation a layered oxide structure is formed consisting of SnO and a slightly tin-rich oxide at the interface. Probably a thin skin of Sn(IV) oxide exists on the outer surface of the low-pressure oxide. High-temperature and low-pressure promotes the growth of SnO. As the pressure is increased the Sn(IV) oxide grows more noticeably and with high-pressure oxidation the Sn(IV) oxide grows thicker than the Sn(II) oxide at the interface. The Sn(II) oxide at the interface appears similar to the Sn(II) oxide structure formed at low pressure. The Auger parameter indicates that the Sn(IV) oxide possesses a structure different than that of Cassiterite. © 1995 American Institute of Physics.
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  • 9
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 76 (1994), S. 5481-5491 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Valence-band as well as Si(2p) and C(1s) core-level photoemission, Auger, and near-edge x-ray-absorption fine-structure spectroscopies were used to follow the surface chemistry associated with diamond film deposition with a filament-assisted chemical-vapor-deposition reactor on atomically clean and diamond polished Si(100) and Si(111) surfaces. Raman spectroscopy and atomic force microscopy (AFM) were also used ex situ to characterize the deposited films. Within 3 min of deposition, a carbon-rich SiC layer, at least 13 A(ring) thick, was observed to develop. At early stages of growth (〈10 min of deposition), no differences were observed between the clean and diamond-polished surfaces. With additional deposition, a 20–30-A(ring)-thick amorphous carbon overlayer was deposited on the clean Si surfaces: The amorphous carbon layer did not promote diamond nucleation. Deposition of an a-C:H layer on top of the amorphous carbon layer also did not promote diamond nucleation. In contrast, ∼500 A(ring) diamond films were deposited within 45–60 min on the diamond-polished surfaces. Two types of nuclei were observed following 20 min of deposition by atomic force microscopy: (1) large (200–300 nm in diameter) nuclei, randomly distributed on the surface; and (2) smaller (50–100 nm) nuclei that show a preference for forming along the scratches. Atomic force micrographs of the originally clean surface show the formation of sharp relief structures on the surface. These structures, combined with the amorphous carbon overlayer, may be responsible for the few sites that do nucleate diamond on unpolished Si surfaces.
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  • 10
    Electronic Resource
    Electronic Resource
    Woodbury, NY : American Institute of Physics (AIP)
    Applied Physics Letters 55 (1989), S. 957-959 
    ISSN: 1077-3118
    Source: AIP Digital Archive
    Topics: Physics
    Notes: We report the x-ray absorption spectra for two hard carbon films grown by filament-assisted chemical vapor deposition in gas mixtures of 1% and 0.18% methane in hydrogen. Although the Raman spectra of these two films suggest significant differences in structure, the x-ray absorption near-edge structure and extended x-ray absorption fine structure (EXAFS) are very similar. Analyzing the EXAFS from these films with a diamond crystal as a reference gives carboncarbon bond lengths of 1.53±0.03 A(ring). This result is consistent with diamond and incompatible with graphite. We conclude that the carbon films have the same local structure as diamond.
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