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Diagnosing transient plasma status: from solar atmosphere to tokamak divertor View all abstracts by submitter

Gerry Doyle   Submitted: 2016-10-07 07:07

This 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.

Authors: A. S. Giuntaa, S. Henderson , M. O'Mullane, J. Harrison, J. G. Doyle and H. P. Summers
Projects: IRIS

Publication Status: in press
Last Modified: 2016-10-12 12:23
Go to main E-Print page  Magnetic helicity estimations in models and observations of the solar magnetic field. Part I: Finite volume methods  Decay of Activity Complexes, Formation of Unipolar Magnetic Regions and Coronal Holes in their Causal Relation  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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