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Radiated power and impurity concentrations in the EXTRAP-T2R reversed-field pinch
KTH, Skolan för teknikvetenskap (SCI), Fysik, Atom- och molekylfysik.ORCID-id: 0000-0001-7389-5501
Vise andre og tillknytning
2005 (engelsk)Inngår i: Physica Scripta, ISSN 0031-8949, E-ISSN 1402-4896, Vol. 71, nr 5, s. 523-531Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

A numerical and experimental study of the impurity concentration and radiation in the EXTRAP-T2R device is reported. The experimental setup consists of an 8-chord bolometer system providing the plasma radiated power and a vacuum-ultraviolet spectrometer providing information on the plasma impurity content. The plasma emissivity profile as measured by the bolometric system is peaked in the plasma centre. A one dimensional Onion Skin Collisional-Radiative model (OSCR) has been developed to compute the density and radiation distributions of the main impurities. The observed centrally peaked emissivity profile can be reproduced by OSCR simulations only if finite particle confinement time and charge-exchange processes between plasma impurities and neutral hydrogen are taken into account. The neutral hydrogen density profile is computed with a recycling code. Simulations show that recycling on metal first wall such as in EXTRAP-T2R (stainless steel vacuum vessel and molybdenum limiters) is compatible with a rather high neutral hydrogen density in the plasma centre. Assuming an impurity concentration of 10% for oxygen and 3% for carbon compared with the electron density, the OSCR calculation including lines and continuum emission reproduces about 60% of the total radiated power with a similarly centrally peaked emmissivity profile. The centrally peaked emissivity profile is due to low ionisation stages and strongly radiating species in the plasma core, mainly O4+ (Be-like) and C3+ (Li-like).

sted, utgiver, år, opplag, sider
2005. Vol. 71, nr 5, s. 523-531
Emneord [en]
vuv spectroscopy, tore-supra, t2r rfp, confinement, transport, profiles, plasma, mode, emission, rotation
Identifikatorer
URN: urn:nbn:se:kth:diva-14783ISI: 000229429800017Scopus ID: 2-s2.0-18844446151OAI: oai:DiVA.org:kth-14783DiVA, id: diva2:332824
Merknad
QC 20100525Tilgjengelig fra: 2010-08-05 Laget: 2010-08-05 Sist oppdatert: 2017-12-12bibliografisk kontrollert

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