2001
DOI: 10.13182/fst01-a11963456
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Analysis of MHD Behaviour by Using Optical Detectors in the GAMMA 10 Tandem Mirror

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Cited by 3 publications
(5 citation statements)
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“…It has been reported that the electrostatic fluctuations were suppressed by MLO experimentally in GAMMA10 [10], which is consistent with the stability criterion (14) or (19).…”
supporting
confidence: 83%
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“…It has been reported that the electrostatic fluctuations were suppressed by MLO experimentally in GAMMA10 [10], which is consistent with the stability criterion (14) or (19).…”
supporting
confidence: 83%
“…The plasma escaping from the central cell touches the MLO, because the plasma radius is 0.18 m at the central cell. Thus, the MLO is heated by high-energy ions and electrons, so that it can emit a secondary electron current easily and can contribute the line-tying effects on the interchange instability [10].…”
Section: Introductionmentioning
confidence: 99%
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“…From the above-described experimental evidence, the observed rigid rotational phenomena for both bulk electrons and ions are consistently interpreted in terms of a flute interchange mode driven by the pressure difference [17,18,20] between the central cell and the anchor region caused by the anchor cold gas puffing. This is also consistent with the results from previously reported electrostatic probe measurements in the peripheral plasma regions of the central cell and the anchor [17,18,20]; i.e. fluctuations having an azimuthal mode number of m = −1 (i.e.…”
Section: Experimental Results and Physics Interpretationsmentioning
confidence: 73%
“…In this paper, the detailed data on the internal core plasma structural behaviour during the MHD destabilization are presented by the use of the developed x-ray diagnostics in comparison to the previous reports with probe measurements and H α diagnostics dominated over the peripheral plasma region [17,18], as well as the mode identification with microwave scattering and reflectometor diagnostics [16,19], since the requirement of the direct observations of interior plasma structural behaviour including the plasma temperature profiles during the MHD instability have still remained as an unsolved issue in order to construct the overall view of the MHD phenomena.…”
Section: Introductionmentioning
confidence: 99%