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ETFP Krakow, 11.9.2006 Edge plasma turbulence theory: the role of magnetic topology Alexander Kendl Bruce D. Scott Institute for Theoretical Physics Max-Planck-Institut für Plasmaphysik, University of Innsbruck, Austria Garching, Germany. → g mn → ?.
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ETFP Krakow, 11.9.2006 Edge plasma turbulence theory: the role of magnetic topology Alexander Kendl Bruce D. Scott Institute for Theoretical Physics Max-Planck-Institut für Plasmaphysik, University of Innsbruck, Austria Garching, Germany → gmn → ?
Influence of magnetic topology on plasma edge turbulence Paradigm for plasma edge turbulence: - resistive electromagnetic gyrofluid drift (-Alfven) wave turbulence - driven by pressure gradient: density + temperature gradients (hi ~ 2 in pedestal) - nonlinear drive, saturation and sustainment Toroidal magnetic topology: - axial-symmetric tokamaks - „three-dimensional“ stellarators Flux-surface shaping: elongation, triangularity, Shafranov shift, D-shape, X-point,... → enters into (nonlinear, gyro-fluid) drift wave equations by: Metric description: |B|, mag. shear, curvature, metric tensor,... (preferably in field-aligned coordinates, e.g. flux-tube representation) → computationally determine influence on fully developed turbulence and flows → identify and understand mechanisms → use understanding to optimise tokamaks and stellarators for turbulent transport reduction / transport barrier formation
„2D“ and „3D“ toroidal magnetic topology Flux-surface shape: elongation, triangularity, Shafranov shift, D-shape, X-point,... Tokamak: axial symmetry elongation: k= b/a triangularity: d = (c+d)/(2a) Stellarator here Wendelstein 7-X: five-fold periodicity (contours: left: local shear, right: |B| ) Geometric quantities on a flux surface: e.g. here local magnetic shear (left) and |B| (right)
Electromagnetic gyrofluid model: two-moment GEM3 equations (B. Scott) { Electrons { Ions Poisson + Ampere equation: Geometric factors: ri ~ 1/B BÑ ||B-1= ∂zbz Ñ || = bz∂z
Metric representation in a field-aligned system Differentiation operators: expression in general curvilinear coordinates - Preferentially: field-aligned (flux-tube) coordinates (u1,u2,u3) = (r,x,h) = (Y,x,h) = (x,y,z) - General definitions: - Laplacian: - Perp. Components: - Parallel grad components: - Parallel divergences:
Metric representation: magnetic field strength |B| |B| acts mainly as scaling factor for some terms: - B(z): in vE ~ 1/B , and ri / FLR-effects contained in gyrofluid polarisation equation - bz = B·Ñ z = Y'/(BJ) in parallel derivatives New physics due to B(z): TEM - particle trapping in magnetic field wells (not discussed in this talk) Influence of flux-surface shaping on |B| effects: - toroidicity effects due to scaling by |B| comparable in moderately shaped tokamaks, but may vary significantly for different stellarator configurations - effects of variation of |B| included in curvature terms (see curvature effects)
Metric representation: local and global magnetic shear Global magnetic shear: Local magnetic shear: - enters into perp. Laplacian as relation between off-diagonal and radial derivatives: - global and local magnetic shear damping of edge turbulence: Kendl & Scott PRL 03
Metric representation: normal and geodesic curvature Definition: magnetic curvature: - low beta: - normal curvature: with - geodesic curvature: with - flux-tube:
Metric representation: dependence on flux-surface shaping - Metric quantities gxx(z), |B|(z), ... etc for various tokamak plasma shapes: simple circular torus (k = 1, d = 0) / shaped torus (k = 2, d = 0.4) / AUG (k = 1.7, d = 0.3, LSN Div)
Computational set-up: flux-tube approximation Codes: - GEM (B. Scott, IPP Garching): full 6 moments or 2-moment model GEM3 - TYR (V. Naulin, Risoe Denmark): drift-Alfvén Fluxtube approximation of toroidal geometry: - field-aligned coordinate transformation - local approximation of metric, shear-shift transformation (see Scott ...) 3D computational grid (flux-tube): radial - perp - parallel x y z 64 256 16-64 ExB convection in (x,y), parallel coupling in z → efficient parallelisation in z (8-128 procs, domain decomposition, MPI) ca. 106 grid point, 105 time steps (run into saturated, equilibrated state) grid resolution: x,y: ~ mm (drift scale), z ~ m t ~ 0.05 Ln/cs < µs
Theoretical expectations: Normal curvature: - defines ballooning region: Ñ p·Ñ B > 0 destabilises interchange drive (ITG/ETG) and catalyses resistive drift wave turbulence Geodesic curvature: - determines geodesic transfer: coupling of zonal flows to turbulence (cf. GAM oscillation) (Scott PLA 03; Kendl & Scott PoP 05) - energetics: GT couples energy for edge turbulence out of flows (e.g. Naulin, Kendl et al PoP 05) Local and global magnetic shear (LMS / GMS): - limits ballooning region - twists vortices: nonlinear decorrelation, general damping mechanism for turbulence - enhances zonal flows (Kendl & Scott PRL 03) Elongation: - enhances magnetic shear: LMS stronger at ballooning boundaries, GMS stronger if other parameters fixed - reduces geodesic curvature at upper / lower regions Triangularity: - slight enhancement of LMS at outboard midplane (little influence on ballooning region) Divertor X-point: - stronger LMS, more reduced geod. curvature
Computational results: Results from model geometries and realistic tokamak + stellarator MHD equilibria Normal curvature: - catalysing for edge turbulence (phase shift properties); ballooning depends on parameters; linear properties determine only long wavelenghts (Scott PoP 05) - sets with beta the ideal MHD ballooning boundary Geodesic curvature: - geodesic transfer effect (Scott PLA 03) scales with geod. curvature (Kendl & Scott PoP 05) - (strong) elongation and X-point shaping enhances GTE (Kendl & Scott PoP 06) Local and global magnetic shear: - general damping effect (nonlinear decorrelation, smaller vortices, lower transport) - LMS relevant even if GMS=0, e.g. in adv. stellarator (Kendl & Scott PRL 03) - strong shear (s > 1) enhances zonal flows (max ZF kx smaller)
General results: flux-surface shaping effects on tokamak edge turbulence - Elongation is always favourable (lower transport, stronger Zfs): simulation transport scaling agrees with empirically found scaling laws (Bateman et al PoP 98) c ~ k-4 - Triangularity has only slight effect - X-point shaping similar effects as strong elongation (shear flow enhancement stronger if ITG dynamics is active, hi ~ 2 → role of ITG crit for L-H threshold, if ZF trigger mean flow?) - Stellarator: general statements difficult, specific computations necessary for each configuration (Kendl & Scott PoP 03) - Strong potential for low-transport / strong shear flow optimisation of tokamaks and stellarators! Next steps: - include dynamic equilibrium coupling for realistic shaping - include radial variations of geometry (esp. important near X-point) - annulus simulations of stellarators instead of flux-tube approximation - try transport optimisation of flux surfaces → large number of simulations necessary
eddies vy(x) vy(x) Computational results: zonal flows, Reynolds stress and geodesic transfer V0: mean flow vxvy: Reynolds stress BxBy: Maxwell stress n sin z: geodesic transfer V0
Computational results: Shear flow generation and energetics (beta dependence) Relative importance of transfer mechanisms: Reynolds stress, Maxwell stress, transfer Flow energy: 0 5 10 15 20 [ Naulin, Kendl, Garcia, Nielsen, Rasmussen, Phys. Plasmas 12, 052515 (2005) ]
Computational results: Influence of elongation and triangularity Elongation reduces edge turbulence and transport. Major mechanisms: magnetic shear damping and shear flow enhancement - Flux surface shaping effects on tokamak edge turbulence and flows: Kendl, Scott; Phys. Plasmas 13, 012504 (2006) - Plasma turbulence in complex magnetic field structures: Kendl; J. Plasma Phys. 41, (2005); in print
Computational results: Influence of X-point shaping on zonal flows X-point shaping enhances zonal flows for ITG turbulence - relevance for L-H transition? (zonal flow triggers mean flow?) - threshold linked to (nonlinear) ITG critical gradient ? - Flux surface shaping effects on tokamak edge turbulence and flows: Kendl, Scott; Phys. Plasmas 13, 012504 (2006) - Plasma turbulence in complex magnetic field structures: Kendl; J. Plasma Phys. 41, (2005); in print