Overview of new MAST physics in anticipation of first results from MAST Upgrade

J.R. Harrison; R. Akers; S.Y. Allan; J.S. Allcock; J. O. Allen; L. Appel; M. Barnes; N. Ben Ayed; W. Boeglin; C. Bowman; J. Bradley; P. Browning; P. Bryant; M. Carr; M. Cecconello; C. Challis; S. Chapman; I.T. Chapman; G. Colyer; S. Conroy; N.J. Conway; M. Cox; G. Cunningham; R.O. Dendy; William D. Dorland; Benjamin Dudson; Luke Easy; S.D. Elmore; T. Farley; X. Feng; A.R. Field; A. Fil; G.M. Fishpool; M. Fitzgerald; K. Flesch; M.F.J. Fox; H. Frerichs; S. Gadgil; D. Gahle; Luca Garzotti; Y.-C. Ghim; S. Gibson; K.J. Gibson; S. Hall; C. Ham; N. Heiberg; S.S. Henderson; Edmund Hood Highcock; Bogdan Hnat; J. Howard; J. Huang; S.W.A. Irvine; A.S. Jacobsen; O. Jones; I. Katramados; D. Keeling; A. Kirk; I. Klimek; L. Kogan; J. Leland; B. Lipschultz; B. Lloyd; J. Lovell; B. Madsen; O. Marshall; R. Martin; G. McArdle; K. McClements; B. McMillan; A. Meakins; H.F. Meyer; F. Militello; J. Milnes; S. Mordijck; A.W. Morris; D. Moulton; D. Muir; K. Mukhi; S. Murphy-Sugrue; O. Myatra; G. Naylor; P. Naylor; Sarah Newton; T. O'Gorman; John Omotani; M.G. O'Mullane; S. Orchard; S.J.P. Pamela; L. Pangione; F. I. Parra; R.V. Perez; L. Piron; M. Price; M. Reinke; F. Riva; C. M. Roach; D. Robb; D. Ryan; S. Saarelma; M. Salewski; S. Scannell; AA Schekochihin; O. Schmitz; S. E. Sharapov; R. Sharples; S.A. Silburn; S.F. Smith; A. Sperduti; R. Stephen; N.T. Thomas-Davies; A.J. Thornton; M. Turnyanskiy; Martin Valovic; F van Wyk; R.G.L. Vann; N. R. Walkden; I. Waters; H.R. Wilson

doi:10.1088/1741-4326/ab121c

Overview of new MAST physics in anticipation of first results from MAST Upgrade
Review article, 2019

The mega amp spherical tokamak (MAST) was a low aspect ratio device (R/a = 0.85/0.65 ∼ 1.3) with similar poloidal cross-section to other medium-size tokamaks. The physics programme concentrates on addressing key physics issues for the operation of ITER, design of DEMO and future spherical tokamaks by utilising high resolution diagnostic measurements closely coupled with theory and modelling to significantly advance our understanding. An empirical scaling of the energy confinement time that favours higher power, lower collisionality devices is consistent with gyrokinetic modelling of electron scale turbulence. Measurements of ion scale turbulence with beam emission spectroscopy and gyrokinetic modelling in up-down symmetric plasmas find that the symmetry of the turbulence is broken by flow shear. Near the non-linear stability threshold, flow shear tilts the density fluctuation correlation function and skews the fluctuation amplitude distribution. Results from fast particle physics studies include the observation that sawteeth are found to redistribute passing and trapped fast particles injected from neutral beam injectors in equal measure, suggesting that resonances between the m = 1 perturbation and the fast ion orbits may be playing a dominant role in the fast ion transport. Measured D-D fusion products from a neutron camera and a charged fusion product detector are 40% lower than predictions from TRANSP/NUBEAM, highlighting possible deficiencies in the guiding centre approximation. Modelling of fast ion losses in the presence of resonant magnetic perturbations (RMPs) can reproduce trends observed in experiments when the plasma response and charge-exchange losses are accounted for. Measurements with a neutral particle analyser during merging-compression start-up indicate the acceleration of ions and electrons. Transport at the plasma edge has been improved through reciprocating probe measurements that have characterised a geodesic acoustic mode at the edge of an ohmic L-mode plasma and particle-in-cell modelling has improved the interpretation of plasma potential estimates from ball-pen probes. The application of RMPs leads to a reduction in particle confinement in L-mode and H-mode and an increase in the core ionization source. The ejection of secondary filaments following type-I ELMs correlates with interactions with surfaces near the X-point. Simulations of the interaction between pairs of filaments in the scrape-off layer suggest this results in modest changes to their velocity, and in most cases can be treated as moving independently. A stochastic model of scrape-off layer profile formation based on the superposition of non-interacting filaments is in good agreement with measured time-average profiles. Transport in the divertor has been improved through fast camera imaging, indicating the presence of a quiescent region devoid of filament near the X-point, extending from the separatrix to ψ n ∼ 1.02. Simulations of turbulent transport in the divertor show that the angle between the divertor leg on the curvature vector strongly influences transport into the private flux region via the interchange mechanism. Coherence imaging measurements show counter-streaming flows of impurities due to gas puffing increasing the pressure on field lines where the gas is ionised. MAST Upgrade is based on the original MAST device, with substantially improved capabilities to operate with a Super-X divertor to test extended divertor leg concepts. SOLPS-ITER modelling predicts the detachment threshold will be reduced by more than a factor of 2, in terms of upstream density, in the Super-X compared with a conventional configuration and that the radiation front movement is passively stabilised before it reaches the X-point. 1D fluid modelling reveals the key role of momentum and power loss mechanisms in governing detachment onset and evolution. Analytic modelling indicates that long legs placed at large major radius, or equivalently low at the target compared with the X-point are more amenable to external control. With MAST Upgrade experiments expected in 2019, a thorough characterisation of the sources of the intrinsic error field has been carried out and a mitigation strategy developed.

MAST

MAST Upgrade

spherical tokamak

Author

Culham Science Centre

Other publications Research

T. O'Gorman

Culham Science Centre

John Omotani

Culham Science Centre

0029-5515 (ISSN) 1741-4326 (eISSN)

Vol. 59 11 112011

Subject Categories

Meteorology and Atmospheric Sciences

DOI

10.1088/1741-4326/ab121c

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Latest update

11/12/2021

Overview of new MAST physics in anticipation of first results from MAST Upgrade Review article, 2019

Author

J.R. Harrison

R. Akers

S.Y. Allan

J.S. Allcock

J. O. Allen

L. Appel

M. Barnes

N. Ben Ayed

W. Boeglin

C. Bowman

J. Bradley

P. Browning

P. Bryant

M. Carr

M. Cecconello

C. Challis

S. Chapman

I.T. Chapman

G. Colyer

S. Conroy

N.J. Conway

M. Cox

G. Cunningham

R.O. Dendy

William D. Dorland

Benjamin Dudson

Luke Easy

S.D. Elmore

T. Farley

X. Feng

A.R. Field

A. Fil

G.M. Fishpool

M. Fitzgerald

K. Flesch

M.F.J. Fox

H. Frerichs

S. Gadgil

D. Gahle

Luca Garzotti

Y.-C. Ghim

S. Gibson

K.J. Gibson

S. Hall

C. Ham

N. Heiberg

S.S. Henderson

Edmund Hood Highcock

Bogdan Hnat

J. Howard

J. Huang

S.W.A. Irvine

A.S. Jacobsen

O. Jones

I. Katramados

D. Keeling

A. Kirk

I. Klimek

L. Kogan

J. Leland

B. Lipschultz

B. Lloyd

J. Lovell

B. Madsen

O. Marshall

R. Martin

G. McArdle

K. McClements

B. McMillan

A. Meakins

H.F. Meyer

F. Militello

J. Milnes

S. Mordijck

A.W. Morris

D. Moulton

D. Muir

K. Mukhi

Overview of new MAST physics in anticipation of first results from MAST Upgrade
Review article, 2019