Matches in SemOpenAlex for { <https://semopenalex.org/work/W975018559> ?p ?o ?g. }
- W975018559 abstract "Introduction: The High Density H-Mode (HDH) /1-3/, discovered and exploited over a wide range of conditions on the W7-AS stellarator, combines optimal core behavior along with edge parameters necessary for successful operation of an Island Divertor. Potentially this bodes well for the larger W7-X device (a/R = 0.16/2m vs. 0.5/5.5m) which represents the next step in the Wendelstein line of development. Still, the question remains if the HDH properties of high energy confinement with low impurity retention and radiation localized at the edge under steady-state conditions (ELM-free) at high densities (to 4 10 20 m -3 ) and heating powers (to 1.7MWm -3 ) can be realized on W7-X or other stellarators? Early investigations revealed that the differences in energy confinement between normal confinement- (NC) and HDH-modes were related to the much broader density profiles of HDH, in contrast to the peaked profiles of NC /1/. Further, the diminished residence time of laser-ablated aluminum in HDH compared to NC could be modeled in an ad hoc fashion by a smaller inwards impurity pinch in the core plasma /1, 4/. Neoclassical calculations indicated that temperature screening together with the flat n e -profiles could be the physical factors for this reduced pinch. However, the inwards convection associated with steep density gradients at the plasma edge for HDH would nonetheless still contrive to confine impurities within the core plasma. A postulation of enhanced impurity diffusion at the plasma edge was necessary in order to reproduce the impurity flushing features of HDH /5, 6/. It is of note that the Enhanced D H-mode (EDA) of the C-Mod tokamak has properties similar to HDH, e.g. flat n e -profiles and steady-state, ELM-free operation without impurity accumulation. A quasi-coherent (QC) mode at the plasma edge is thought to provoke impurity flushing /7-9/. In contrast, ELM-free H-modes without QC exhibit accumulation. This paper reports on dedicated experiments performed on W7-AS to compare HDH with standard ELM-free discharges (H*) ‐ which typically suffer radiation collapse as a result of impurity accumulation. A back-to-back comparison offers an excellent basis for pinpointing essential operative elements of HDH physics. Experiment: A discharge was tailored in an island-divertor configuration with P abs ~1.4MW whereby the density was ramped up until attainment of H*, and then after 60ms increased again until the HDH mode was solidly established (Fig.1). The entrance into H* is indicated by the cessation of ELM activity (seen in H of Figs. 1&2), followed by a rapid increase in" @default.
- W975018559 created "2016-06-24" @default.
- W975018559 creator A5007076618 @default.
- W975018559 creator A5015769452 @default.
- W975018559 creator A5022362966 @default.
- W975018559 creator A5028553357 @default.
- W975018559 creator A5030254993 @default.
- W975018559 creator A5036978426 @default.
- W975018559 creator A5039112187 @default.
- W975018559 creator A5046233368 @default.
- W975018559 creator A5053104990 @default.
- W975018559 creator A5057982246 @default.
- W975018559 creator A5065737425 @default.
- W975018559 creator A5072583154 @default.
- W975018559 creator A5073134012 @default.
- W975018559 creator A5073752338 @default.
- W975018559 creator A5075752553 @default.
- W975018559 creator A5079154016 @default.
- W975018559 creator A5083016710 @default.
- W975018559 creator A5085192676 @default.
- W975018559 creator A5086948911 @default.
- W975018559 creator A5062996134 @default.
- W975018559 date "2003-01-01" @default.
- W975018559 modified "2023-09-27" @default.
- W975018559 title "The Wendelstein W7-AS High Density H-Mode A Mode for the Future?" @default.
- W975018559 hasPublicationYear "2003" @default.
- W975018559 type Work @default.
- W975018559 sameAs 975018559 @default.
- W975018559 citedByCount "0" @default.
- W975018559 crossrefType "journal-article" @default.
- W975018559 hasAuthorship W975018559A5007076618 @default.
- W975018559 hasAuthorship W975018559A5015769452 @default.
- W975018559 hasAuthorship W975018559A5022362966 @default.
- W975018559 hasAuthorship W975018559A5028553357 @default.
- W975018559 hasAuthorship W975018559A5030254993 @default.
- W975018559 hasAuthorship W975018559A5036978426 @default.
- W975018559 hasAuthorship W975018559A5039112187 @default.
- W975018559 hasAuthorship W975018559A5046233368 @default.
- W975018559 hasAuthorship W975018559A5053104990 @default.
- W975018559 hasAuthorship W975018559A5057982246 @default.
- W975018559 hasAuthorship W975018559A5062996134 @default.
- W975018559 hasAuthorship W975018559A5065737425 @default.
- W975018559 hasAuthorship W975018559A5072583154 @default.
- W975018559 hasAuthorship W975018559A5073134012 @default.
- W975018559 hasAuthorship W975018559A5073752338 @default.
- W975018559 hasAuthorship W975018559A5075752553 @default.
- W975018559 hasAuthorship W975018559A5079154016 @default.
- W975018559 hasAuthorship W975018559A5083016710 @default.
- W975018559 hasAuthorship W975018559A5085192676 @default.
- W975018559 hasAuthorship W975018559A5086948911 @default.
- W975018559 hasConcept C116515362 @default.
- W975018559 hasConcept C120665830 @default.
- W975018559 hasConcept C121332964 @default.
- W975018559 hasConcept C14480152 @default.
- W975018559 hasConcept C184779094 @default.
- W975018559 hasConcept C185544564 @default.
- W975018559 hasConcept C192562407 @default.
- W975018559 hasConcept C2164484 @default.
- W975018559 hasConcept C2777017188 @default.
- W975018559 hasConcept C2779176124 @default.
- W975018559 hasConcept C2781249502 @default.
- W975018559 hasConcept C62520636 @default.
- W975018559 hasConcept C71987851 @default.
- W975018559 hasConcept C82706917 @default.
- W975018559 hasConceptScore W975018559C116515362 @default.
- W975018559 hasConceptScore W975018559C120665830 @default.
- W975018559 hasConceptScore W975018559C121332964 @default.
- W975018559 hasConceptScore W975018559C14480152 @default.
- W975018559 hasConceptScore W975018559C184779094 @default.
- W975018559 hasConceptScore W975018559C185544564 @default.
- W975018559 hasConceptScore W975018559C192562407 @default.
- W975018559 hasConceptScore W975018559C2164484 @default.
- W975018559 hasConceptScore W975018559C2777017188 @default.
- W975018559 hasConceptScore W975018559C2779176124 @default.
- W975018559 hasConceptScore W975018559C2781249502 @default.
- W975018559 hasConceptScore W975018559C62520636 @default.
- W975018559 hasConceptScore W975018559C71987851 @default.
- W975018559 hasConceptScore W975018559C82706917 @default.
- W975018559 hasLocation W9750185591 @default.
- W975018559 hasOpenAccess W975018559 @default.
- W975018559 hasPrimaryLocation W9750185591 @default.
- W975018559 hasRelatedWork W115629318 @default.
- W975018559 hasRelatedWork W1551597653 @default.
- W975018559 hasRelatedWork W1569305999 @default.
- W975018559 hasRelatedWork W1632489996 @default.
- W975018559 hasRelatedWork W1977035205 @default.
- W975018559 hasRelatedWork W2006529197 @default.
- W975018559 hasRelatedWork W2023595603 @default.
- W975018559 hasRelatedWork W2066041248 @default.
- W975018559 hasRelatedWork W2071197825 @default.
- W975018559 hasRelatedWork W2092559869 @default.
- W975018559 hasRelatedWork W2094453081 @default.
- W975018559 hasRelatedWork W2112807645 @default.
- W975018559 hasRelatedWork W2149229471 @default.
- W975018559 hasRelatedWork W2170704266 @default.
- W975018559 hasRelatedWork W2188488923 @default.
- W975018559 hasRelatedWork W617785959 @default.
- W975018559 hasRelatedWork W769653908 @default.
- W975018559 hasRelatedWork W87344455 @default.
- W975018559 hasRelatedWork W935147389 @default.