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  • 1
    Electronic Resource
    Electronic Resource
    Search for fine Moiré fringes representing the (010), (100) and (013) planes in aligned unit cells of YBa2Cu2.7Sn0.3O7-y superconducting crystals (1994)
    Springer
    Journal of materials science 13 (1994), S. 647-649 
    Details
    ISSN: 1573-4811
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00271222
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  • 2
    Electronic Resource
    Electronic Resource
    Evaluation of Energy Utilization Efficiencies for SO2 and NO Removal by Pulsed Corona Discharge Process (1998)
    Springer
    Plasma chemistry and plasma processing 18 (1998), S. 535-550 
    Details
    ISSN: 1572-8986
    Keywords: Pulsed corona discharge ; energy transfer efficiency ; energy utilization efficiency ; SO2 ; NO
    Source: Springer Online Journal Archives 1860-2000
    Topics: Chemistry and Pharmacology , Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics , Technology
    Notes: Abstract Pulsed corona discharge process was applied to the removal of sulfur dioxide and nitrogen oxides from simulated flue gas. The energy transfer efficiency of the pulse generation circuit and the energy utilization efficiencies for SO 2 and NO removal are evaluated and discussed. When the pulse-forming capacitance was five times larger than the geometric capacitance of the reactor, the energy utilization efficiency was maximized, and the energy requirements for NO and SO 2 removal could be lowered. With regard to radical utilization efficiency, producing small amounts of radicals frequently was found to be more advantageous than producing large amounts of radicals less frequently. Removal efficiency of SO 2 increased with the applied peak voltage, but the energy utilization efficiency was nearly independent of the peak voltage when the peak field intensity was high enough to induce corona discharge (above 10 kV cm −1 in this system).
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1023/A:1021863300810
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  • 3
    Electronic Resource
    Electronic Resource
    Efficient Energy Delivery Condition from Pulse Generation Circuit to Corona Discharge Reactor (2000)
    Springer
    Plasma chemistry and plasma processing 20 (2000), S. 353-364 
    Details
    ISSN: 1572-8986
    Keywords: Corona discharge ; pulse-forming capacitor ; optimum energy transfer
    Source: Springer Online Journal Archives 1860-2000
    Topics: Chemistry and Pharmacology , Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics , Technology
    Notes: Abstract The energy transfer efficiency from pulse generation circuit to corona discharge reactor was investigated. To find the optimum energy transfer condition, we varied the value of the pulse-forming capacitor in pulse generation circuit. Maximum energy transfer from pulse generation circuit to corona discharge reactor was achieved when the ratio of the pulse-forming capacitance to the geometric capacitance of the reactor was around 3.0. From the analyses of the voltage and current waveforms, we found that the capacitance of the reactor increases about three times, due to the corona development. This increase is the reason why the maximum energy transfer occurs when the pulse-forming capacitance is three times larger than the initial capacitance of the reactor. The energy consumption for removal of nitric oxide was also minimized at this capacitance ratio.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1023/A:1007044328066
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  • 4
    Electronic Resource
    Electronic Resource
    Prominence condensation and magnetic levitation in a coronal loop (1992)
    Springer
    Solar physics 140 (1992), S. 269-287 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We describe the results of a model dynamic simulation of the formation and support of a narrow prominence at the apex of a coronal magnetic loop or arcade. The condensation process proceeds via an initial radiative cooling and pressure drop, and a secondary siphon flow from the dense chromospheric ends. The anti-buoyancy effect as the prominence forms causes a bending of the confining magnetic field, which propagates toward the semi-rigid ends of the magnetic loop. Thus, a wide magnetic ‘hammock’ or well (of the normal-polarity Kippenhahn-Schlüter-type) is formed, which supports the prominence at or near the field apex. The simplicity of this 1.5-dimensional model, with its accompanying diagnostics, allows one to comprehend the various contributions to the nonlinear dynamics of prominence condensation and levitation.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00146313
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  • 5
    Electronic Resource
    Electronic Resource
    The thermal stability of coronal loops numerical simulations (1991)
    Springer
    Solar physics 132 (1991), S. 95-108 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We have studied the radiative stability of thermally isolated coronal loops with free-flow boundary conditions by nonlinear numerical simulation. We first establish a chromosphere-to-corona loop equilibrium (including the option of a deep chromosphere) by following the nonlinear evolution from an initial isothermal state with rigid boundaries. We then change the end conditions, to allow free flow and to fix the temperature, and investigate the response to non-isobaric perturbations. Within a family of loops of the same pressure, we find long hot loops to be stable and short cool loops to be unstable to the thermal chromosphericexpansion mode. The stable cases remain so, even when long chromospheric ends and/or gravity are added. In those cases which are unstable, we follow the subsequent nonlinear evolution which exhibits swelling of the chromosphere until the entire loop becomes cool and dense.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00159132
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  • 6
    Electronic Resource
    Electronic Resource
    The thermal structure of the magnetized solar transition region (1993)
    Springer
    Solar physics 146 (1993), S. 5-17 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The detailed thermal structure of the magnetized solar transition region, as measured by itsdifferential emission measure [DEM(T)], is unknown. Proposals have been made that envision a significant lower-temperature contribution to the energy balance from cross-field (ion) heat flux. In this paper, we describe a self-consistent, 2-D, MHD simulation (including the full effects of anisotropic thermal conduction) of a conceptual model due to Athay (1990). We display the detailed, irregular, thermal and magnetic structure of the transition region, and demonstrate that the predicted DEM agrees with observations, particularly in theT 〈 105 K regime where previous theories had difficulty.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00662166
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  • 7
    Electronic Resource
    Electronic Resource
    The solar-surface boundary conditions of coronal magnetic loops (1995)
    Springer
    Solar physics 161 (1995), S. 67-81 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The dynamical properties of a realisticthermal-structure interface between a coronal loop and the chromosphere/photosphere are investigated by numerical simulations using acoustic and Alfvénic excitations. These properties are relevant to the end conditions seen by coronal MHD perturbations (e.g., waves or instabilities), in the absence of much slower energetics effects. Analytic studies of coronal-loop hydromagnetics have often made simplifying assumptions about the boundary conditions at the loop base in order to make their calculations tractable. However, in the presence of a transition region and chromosphere with rapidly varying plasma conditions, it is not clear how valid these heuristic assumptions are. In this study, we find that the discontinuous fluid-density model approximately represents the reflection/ transmission scaling with respect to varying transition-region density and temperature (i.e., dynamic impedance) ratios, although it does not quantitatively predict the chromospheric response to wave-like coronal activity. This disagreement is partially due to the finite width of the corona-to-photosphere transition.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00732085
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  • 8
    Electronic Resource
    Electronic Resource
    The differential emission measure of nested hot and cool magnetic loops (1993)
    Springer
    Solar physics 147 (1993), S. 199-202 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The detailed thermal structure of the magnetized solar transition region, as measured by itsdeferential emission measure [DEM(T)], is poorly known. Building on the fact that the solar surface is strongly magnetized and thereby structured, proposals have been made that envision a significant lower-temperature contribution to the energy balance from (ion) heat fluxacross an arcade of different temperature loops. In this paper, we describe aself-consistent, 2-D, MHD simulation, which includes the full thermal effects of parallel stability and anisotropic conduction, of a nested-loop model of the thermal and magnetic structure of the transition region. We then demonstrate that the predicted DEM agrees with observations in the conceptually elusiveT 〈 105K regime.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00675494
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  • 9
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    Superheating of ice crystals in antifreeze protein solutions (2010)
    National Academy of Sciences
    Details
    Publication Date: 2010-03-09
    Print ISSN: 0027-8424
    Electronic ISSN: 1091-6490
    Topics: Biology , Medicine , Natural Sciences in General
    Published by National Academy of Sciences
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  • 10
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    Internal magnetic field measurements of translated and merged field-reversed configuration plasmas in the FAT-CM device (2018)
    American Institute of Physics
    Details
    Publication Date: 2018-10-01
    Print ISSN: 0034-6748
    Electronic ISSN: 1089-7623
    Topics: Electrical Engineering, Measurement and Control Technology , Physics
    Published by American Institute of Physics
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