Journal of Plasma and Fusion Research
Print ISSN : 0918-7928
Volume 78, Issue 6
Displaying 1-14 of 14 articles from this issue
Rapid Communications
  • Iwao MORIMOTO, Sunao KAWASAKI, Kazuhiko HORIOKA, Xiaodong ZHENG, Sunao ...
    2002 Volume 78 Issue 6 Pages 493-494
    Published: 2002
    Released on J-STAGE: December 08, 2005
    JOURNAL FREE ACCESS
    The dependence of the backward wave oscillator's (BWO's) microwave output power on the number of corrugations is observed experimentally. The slow-wave structure (SWS) of the BWO has been designed to operate at 9.8 GHz . The SWS consists of detachable corrugated modules, and the corrugation number N can be changed from 1 up to 10. The BWO is driven by the high current electron accelerator LAX-1 (850 keV, 3 kA). The dependence of power on corrugation number is not monotonic; with 3 modules, a small output signal of 20kW level is observed; with 4 modules, a rapid increase of output power of the level of 10 MW is observed, and from 5 to 10 modules the output power appears to saturate at the power level of 100MW. These results are analyzed with a PIC Code called Magic.
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  • Hitoshi HOJO, Tsuguhiro WATANABE, Kazuhiro AKIMOTO
    2002 Volume 78 Issue 6 Pages 495-496
    Published: 2002
    Released on J-STAGE: December 08, 2005
    JOURNAL FREE ACCESS
    Stationary solitary electromagnetic waves generated in ultraintense relativistic laser-plasma interactions are studied numerically. For one-dimensional stationary propagation with circular polarization, subcycle solitary waves moving with finite velocity are obtained for a given value of wave velocity and nonlinear frequency shift, and it is shown that the solitary-wave amplitude increases for the larger nonlinear frequency shift. A new type of solitary-wave solution, a paired solution of positive and negative solitary waves, is also shown.
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Commentary
  • Hiromoto SHIBAHASHI
    2002 Volume 78 Issue 6 Pages 497-507
    Published: 2002
    Released on J-STAGE: December 08, 2005
    JOURNAL FREE ACCESS
    There has been a long-standing discrepancy between the number of neutrinos expected from the sun and the number we actually detect. One possible way to account for this is that our theoretical solar model is inaccurate. However, recent progress in helioseismology has shown that the real sun is very close to the latest solar models. On the other hand, very recent experiments of neutrino detection provided us evidence for neutrino oscillation. I discuss what we should do and what we can do in this situation for the neutrino physics from the astrophysical side.
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  • Takashi MAEKAWA
    2002 Volume 78 Issue 6 Pages 508-520
    Published: 2002
    Released on J-STAGE: December 08, 2005
    JOURNAL FREE ACCESS
    Recent progress in electron Bernstein wave physics for electron cyclotron heating and electron cyclotron emission measurement in over-dense toroidal plasmas such as spherical tokamaks are reviewed. First, the theoretical bases of mode-conversion processes including X-B and O-X-B processes are described and discussed. Second, basic characteristics of electron Bernstein waves are described, and their propagation and absorption characteristics in toroidal plasmas including N// up-shift are described and discussed. Finally, recent experimental studies and efforts are reviewed.
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Special Topic Article : Particle Beam Application - Present Status and Future Prospects
Lecture Note : Relativistic Plasma Physics
  • Ken-ichi NAKASHIMA, Thomas E. COWAN
    2002 Volume 78 Issue 6 Pages 568-574
    Published: 2002
    Released on J-STAGE: December 08, 2005
    JOURNAL FREE ACCESS
    Electron-positron plasmas are believed to exist around the center of galaxy and compact stars. This relativistic electron-positron pair plasma has special features different from normal plasmas. The equilibrium conditions are given to solve the rate equation for pair creations and pair annihilation. The limit of temperature exists around 15 MeV under the condition that electron-positron plasma stays in equilibrium. In addition to the astrophysical plasmas, the dense electron-positron plasmas are produced by ultra-intense lasers in alaboratory.The studies of the relativistic electron-positron plasmas become important subjects in both astrophysics and laboratory plasma physics.
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  • Akira MIZUTA, Tatsuya YAMASAKI
    2002 Volume 78 Issue 6 Pages 575-581
    Published: 2002
    Released on J-STAGE: December 08, 2005
    JOURNAL FREE ACCESS
    Relativistic flows have been observed in jets and gamma-ray bursts. Such phenomena are not fully understood. In order to study such flows, we need to consider relativistic effects. In this paper, we first explain relativistic hydrodynamic equations. Some characteristics relativistic flows are discussed, namely, the adiabatic exponent and sound speed for high temperature fluid, and shock jump conditions. Second, we show relativistic jets as an example of relativistic flows. Observations of jets and theoretical models for acceleration, collimation, and propagation of jets are given.
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Contributed Paper
  • Shinichiro TODA, Kimitaka ITOH
    2002 Volume 78 Issue 6 Pages 582-590
    Published: 2002
    Released on J-STAGE: December 08, 2005
    JOURNAL FREE ACCESS
    The structure of the electric field is studied by use of the theoretical model for the anomalous transport diffusivities. In this analysis, the thermal diffusivity is employed based on the theory of self-sustained turbulence due to the balooning mode and the interchange mode, both driven by the current diffusivity. Multiple solutions of Er for the ambipolar condition are obtained in the structure of the radial electric field. The reduction of the anomalous transport coeffient is examined due to the strong gradient of the radial electric field in the phase diagram of the external sources.
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Review Paper
  • Teruo SAITO, Yoshinori TATEMATSU, Isao KATANUMA, Kiyoshi YATSU
    2002 Volume 78 Issue 6 Pages 591-598
    Published: 2002
    Released on J-STAGE: December 08, 2005
    JOURNAL FREE ACCESS
    In GAMMA 10, the plasma potential at the plug region, which is generated by fundamental ECRH, is linked to the end plate potential. There are two factors in this linkage. One is the field-aligned flow of warm electrons driven into the loss cone by ECRH. The other is a finite current through the end plate. This current is connected to an ion current, which is detected on annular electrodes in the end mirror cell where the plug potential is formed. An experimental attempt to externally control this current was performed by varying the resistance connecting the end plate to the vacuum vessel, and a picture of current circulation was obtained. In this circuit, ECRH generates an electromotive force by driving the axial flow of electrons. This electromotive force is divided into the positive plug potential and the negative end plate potential, respectively as measured from the vacuum vessel to meet the condition of a closed circuit.
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