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Published byMillicent Mills Modified over 9 years ago
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Ergodic heat transport analysis in non-aligned coordinate systems S. Günter, K. Lackner, Q. Yu IPP Garching Problems with non-aligned coordinates? Description of new scheme First results
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Problems with non-aligned coordinates Radial heat transport in multiple helicity magnetic fields enhanced by stochasticity For large || / (realistic values for hot plasmas ~ 10 10 ) careful treatment of parallel heat flux required
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Problems with non-aligned coordinates Usually coordinate system aligned with magnetic field lines used, see e.g. Runov et al. (for static magnetic field) But for non-linear MHD calculations dynamically evolving magnetic fields need to be considered! For large || / (realistic values for hot plasmas ~ 10 10 ): small gradient along magnetic field lines cause large errors in temperature profile
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An example: Interaction of NTMs with different helicities No simultaneous large NTMs of different helicities observed in experiments j BS p
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Analytic theory: for NTMs stabilising effect of additional helical field can be proven for small values of || / (incomplete temperature flattening) effect vanishes for || / Is there an effect remaining for realistic values of || / ? If so: new stabilisation method for NTMs can be propsed: stabilisation by external helical perturbation fields An example: Interaction of NTMs with perturbation fields Many other problems, but: so far no non-linear MHD code can deal with realistic || /
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Proposal for a solution in non-aligned coordinate system In the following, for simplicity (not in the code): Cartesian coordinates in radial direction, Fourier decomposition within the unperturbed flux surface, only one perturbation field component Heat conduction equation for different Fourier components of temperature: … … To close the equations one should not truncate the Fourier series in T, but in q heat flux along perturbed magnetic field line remains finite (nearly vanishing temperature gradients)
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Fourier decomposition for perturbation To lowest order (for explanation): include only terms up to first order in q T 2 adjusts itself such that q ||1 becomes small In the following, for simplicity (not in the code): Cartesian coordinates in radial direction, Fourier decomposition within the unperturbed flux surface, only one perturbation field component Heat conduction equation for different Fourier components of temperature:
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Fourier decomposition for perturbation If one truncates in T (just as example, holds for any order): Cut after lowest order in temperature Enhancement of radial transport (T 1 would adjust to cancel the first term) To close the equations one should not truncate the Fourier series in T, but in q heat flux along perturbed magnetic field line remains finite (nearly vanishing temperature gradients)
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What about the radial derivatives? perturbation field: Introduces an additional error or order ( r) 2, but equations for each grid point ensure vanishing temperature gradients along perturbed field lines simplest discretisation at i’s grid point new scheme
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Convergence properties: single magnetic island || / = 10 8 Still convergence only ( r) -2 But: relative error reduced by factor of 10 Improvement increases for larger || / (~ ( || / ) 1/2 ) -2
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Example: Magnetic islands of two helicities
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|| / = 10 10 Magnetic islands seen in temperature contours, but still strong gradient in ergodic region Example: Magnetic islands of two helicities
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|| / = 10 12 Temperature gradient vanishes in ergodic region due to increased radial transport along magnetic field lines Example: Magnetic islands of two helicities
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Coming back to: Interaction of NTMs with different helicities Is there an effect remaining for realistic values of || / ? If so: new stabilisation method for NTMs can be propsed: stabilisation by external helical perturbation fields (next talk) YES!
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Summary and conclusion New scheme for solving heat conduction equation in non-aligned coordinates developed Successful test for realistic (and even higher) values of || / Method can be used in general (toroidal) non-linear MHD codes Generalisation to 3d Cartesian grid straightforward
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