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dc.contributorRAL Space, Science and Technology Facilities Council, Rutherford Appleton Laboratory, Harwell Oxford, Didcot OX11 0QX, U.K.
dc.contributorDepartment of Physics, University of Strathlyde, 107 Rottenrow, Glasgow G4 0NG, U.K.
dc.contributorCulham Centre for Fusion Energy, Culham Science Centre, Abingdon OX14 3DB, U.K.
dc.contributorArmagh Observatory, College Hill, Armagh BT61 9DG, U.K.
dc.contributor.authorGiunta, A. S.
dc.contributor.authorHenderson, S.
dc.contributor.authorO'Mullane, M.
dc.contributor.authorHarrison, J.
dc.contributor.authorDoyle, J. G.
dc.contributor.authorSummers, H. P.
dc.date.accessioned2024-07-24T13:50:55Z
dc.date.available2024-07-24T13:50:55Z
dc.date.issued2016-09-01T00:00:00Z
dc.identifier.doi10.1088/1748-0221/11/09/C09008
dc.identifier.other2016JInst..11C9008G
dc.identifier.other10.1088/1748-0221/11/09/C09008
dc.identifier.other-
dc.identifier.urihttp://hdl.handle.net/20.500.14302/2072
dc.description.abstractThis work strongly exploits the interdisciplinary links between astrophysical (such as the solar upper atmosphere) and laboratory plasmas (such as tokamak devices) by sharing the development of a common modelling for time-dependent ionisation. This is applied to the interpretation of solar flare data observed by the UVSP (Ultraviolet Spectrometer and Polarimeter), on-board the Solar Maximum Mission and the IRIS (Interface Region Imaging Spectrograph), and also to data from B2-SOLPS (Scrape Off Layer Plasma Simulations) for MAST (Mega Ampère Spherical Tokamak) Super-X divertor upgrade. The derived atomic data, calculated in the framework of the ADAS (Atomic Data and Analysis Structure) project, allow equivalent prediction in non-stationary transport regimes and transients of both the solar atmosphere and tokamak divertors, except that the tokamak evolution is about one thousand times faster.
dc.publisherJournal of Instrumentation
dc.titleDiagnosing transient plasma status: from solar atmosphere to tokamak divertor
dc.typearticle
dc.source.journalJInst
dc.source.journalJInst..11
dc.source.volume11
refterms.dateFOA2024-07-24T13:50:56Z
dc.identifier.bibcode2016JInst..11C9008G


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