scholarly journals Measurement of the plasma boundary shift and approximation of the magnetic surfaces on the IR-T1 Tokamak

2010 ◽  
Vol 40 (3) ◽  
pp. 323-326 ◽  
Author(s):  
A. Salar Elahi ◽  
M. Ghoranneviss

For quantitative predictions the tokamak plasma has to be modelled as a consistent entity. Distinguishing features of fusion plasma theory are the simultaneous importance of a large number of effects, essential multidimensionality in geometrical and velocity space, and a high degree of nonlinearity in the interaction between these effects. Only computational methods, mainly based on linearization, iteration and on procedures for solving huge systems of linear equations, are widely applicable, and provide quantitative ‘point results’ of the ‘numerical experiment’ type. The practical limitations of computer capacity and cost of computing time impose severe limits on details which can be taken into account in computational plasma models. For plasmas of tokamaks such as JET, the models are set up as initial boundary value problems on several time scales, and composed of a cluster of interdependent computer codes. The basic magnetic field-plasma configuration is determined from a one-fluid (magnetohydrodynamic) theory in two dimensions. The macroscopic stability of these configurations is checked. For stable plasmas the secular evolution of a sequence of equilibria is computed by ‘transport codes’. In these the balance equations for the conservation quantities (mass, momentum, energy) are solved for fluxes between, and sources and sinks on, the magnetic surfaces (as determined from equilibrium). These are multifluid equations in one spatial dimension for all charged plasma species including impurities. Important source terms such as electromnetic wave heating, injected particles, and fusion x-particles must be calculated kinetically with at least one additional velocity-space coordinate. At least at the plasma boundary, neutral atoms cannot be neglected. Their distribution is calculated by Monte-Carlo methods in three spatial dimensions (and velocity space). The bulk plasma is usually surrounded by magnetic surfaces or field lines that cross solid walls. Here also, for the transport of charged particles, propagation in two dimensions must be calculated. The consistent combination of these major elements is considered.


1971 ◽  
Vol 5 (2) ◽  
pp. 229-238 ◽  
Author(s):  
J. H. Williamson

Local imperfections in the magnetic field can alter the topology of the magnetic surfaces, thereby allowing plasma to escape. A modest longitudinal magnetic field will maintain the nested surfaces near the plasma boundary, so that the residual topological changes near the separatrix become unimportant.


1998 ◽  
Vol 59 (2) ◽  
pp. 303-314 ◽  
Author(s):  
G. N. THROUMOULOPOULOS

The equilibrium of a resistive axisymmetric plasma with purely toroidal flow surrounded by a conductor is investigated within the framework of nonlinear magnetohydrodynamic theory. It is proved that (a) the poloidal current-density vanishes and (b) apart from an idealized case, the pressure profile should vanish on the plasma boundary. For the cases of isothermal magnetic surfaces, isentropic magnetic surfaces and magnetic surfaces with constant density, the equilibrium states obey an elliptic partial differential equation for the poloidal magnetic flux function, which is identical in form to the corresponding equation governing ideal equilibria. The conductivity, which can be neither uniform nor a surface quantity, results, however, in a restriction of the possible classes of equilibrium solutions; for example for the cases considered, the only possible equilibria with Spitzer conductivity are of cylindrical shape.


1998 ◽  
Vol 398 (1-2) ◽  
pp. 84-90 ◽  
Author(s):  
A. Närmann ◽  
M. Dirska ◽  
J. Manske ◽  
G. Lubinski ◽  
M. Schleberger ◽  
...  

1985 ◽  
Vol 40 (10) ◽  
pp. 959-967
Author(s):  
A. Salat

The equivalence of magnetic field line equations to a one-dimensional time-dependent Hamiltonian system is used to construct magnetic fields with arbitrary toroidal magnetic surfaces I = const. For this purpose Hamiltonians H which together with their invariants satisfy periodicity constraints have to be known. The choice of H fixes the rotational transform η(I). Arbitrary axisymmetric fields, and nonaxisymmetric fields with constant η(I) are considered in detail.Configurations with coinciding magnetic and current density surfaces are obtained. The approach used is not well suited, however, to satisfying the additional MHD equilibrium condition of constant pressure on magnetic surfaces.


2021 ◽  
Vol 87 (2) ◽  
Author(s):  
Arthur Carlton-Jones ◽  
Elizabeth J. Paul ◽  
William Dorland

Coil complexity is a critical consideration in stellarator design. The traditional two-step optimization approach, in which the plasma boundary is optimized for physics properties and the coils are subsequently optimized to be consistent with this boundary, can result in plasma shapes which cannot be produced with sufficiently simple coils. To address this challenge, we propose a method to incorporate considerations of coil complexity in the optimization of the plasma boundary. Coil complexity metrics are computed from the current potential solution obtained with the REGCOIL code (Landreman, Nucl. Fusion, vol. 57, 2017, 046003). While such metrics have previously been included in derivative-free fixed-boundary optimization (Drevlak et al., Nucl. Fusion, vol. 59, 2018, 016010), we compute the local sensitivity of these metrics with respect to perturbations of the plasma boundary using the shape gradient (Landreman & Paul, Nucl. Fusion, vol. 58, 2018, 076023). We extend REGCOIL to compute derivatives of these metrics with respect to parameters describing the plasma boundary. In keeping with previous research on winding surface optimization (Paul et al., Nucl. Fusion, vol. 58, 2018, 076015), the shape derivatives are computed with a discrete adjoint method. In contrast with the previous work, derivatives are computed with respect to the plasma surface parameters rather than the winding surface parameters. To further reduce the resolution required to compute the shape gradient, we present a more efficient representation of the plasma surface which uses a single Fourier series to describe the radial distance from a coordinate axis and a spectrally condensed poloidal angle. This representation is advantageous over the standard cylindrical representation used in the VMEC code (Hirshman & Whitson, Phys. Fluids, vol. 26, 1983, pp. 3553–3568), as it provides a uniquely defined poloidal angle, eliminating a null space in the optimization of the plasma surface. In comparison with previous spectral condensation methods (Hirshman & Breslau, Phys. Plasmas, vol. 5, 1998, p. 2664), the modified poloidal angle is obtained algebraically rather than through the solution of a nonlinear optimization problem. The resulting shape gradient highlights features of the plasma boundary that are consistent with simple coils and can be used to couple coil and fixed-boundary optimization.


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