1994
DOI: 10.1088/0741-3335/36/7a/011
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H-mode results in ASDEX Upgrade

Abstract: The H-mode obtained in ASDEX Upgrade by three heating methods (Ohmic, NBI, ICRF) is analysed. The power threshold is shown to be relatively low compared with other tokamaks and to be independent of the heating method The operational window for the different types of H-phases, (dithering, ELMing with type-LII and I E M S , ELM-free) is given and discussed. The features of the H-mode discharges, in particular quasi-stationary ELMing phases with type I ELMs, are described and discussed. Finally, it is shown that … Show more

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Cited by 55 publications
(46 citation statements)
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“…While the ELM-free H-modes appear to fit the ASDEX-Upgrade H-mode power threshold scaling, the ELMy H-modes following lithium pellet injection occur at significantly lower input power. These results, together with previous results from other tokamaks [3][4][5], suggest that if the neB dependence of the H-mode power threshold is approximately correct, then there is also a dependence on wall conditions that can significantly lower the power threshold. Fig.…”
supporting
confidence: 75%
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“…While the ELM-free H-modes appear to fit the ASDEX-Upgrade H-mode power threshold scaling, the ELMy H-modes following lithium pellet injection occur at significantly lower input power. These results, together with previous results from other tokamaks [3][4][5], suggest that if the neB dependence of the H-mode power threshold is approximately correct, then there is also a dependence on wall conditions that can significantly lower the power threshold. Fig.…”
supporting
confidence: 75%
“…Therefore, it is possible that S should be replaced with R 2 . 5 or that the power law dependences of ne or BT are not exactly linear. Further experiments including additional heating with ICRF and direct comparisons with ASDEX-Upgrade will be performed to test this scaling in detail.…”
mentioning
confidence: 99%
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“…Summarizing, the L-H and H-L power thresholds exhibit very similar dependences and the hysteresis often does not appear clearly which is mainly caused by the rather large radiation fraction which develops during the H-mode. This contribution is significantly higher with the tungsten wall, the hysteresis was clearer in the carbon wall [47]. The investigation of the hysteresis at the H-L transition is not the only aspect of this topic which can be extended by the study of the comparison between P loss and P scal during the development of the H-mode after the L-H transition.…”
Section: Survey Of the H-mode Power Threshold And Transition Physics mentioning
confidence: 99%