Page 114 - Fundamentals of Magnetic Thermonuclear Reactor Design
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98     Fundamentals of Magnetic Thermonuclear Reactor Design


            conducting coils, and so on. Relevant computations are performed using the
            DINA axisymmetric plasma simulation code. The latter allows a numerical
            solution for the plasma equilibrium equation self-consistent with an external
            magnetic field, and transport equations for plasma kinetic parameters in the
            plasma and the halo regions. DINA computational models are axisymmetric.
            Because the blanket modules and divertor cassettes are not axisymmetric,
            these components are described with relevant 2D models equivalent from the
            EM point of view. In this approximation, the characteristic time needed for
            a magnetic field to penetrate conductive structures is assumed the same for
            2D and 3D models.
               Evolutions of the distributed plasma current and coil currents, obtained with
            DINA, are used for a 3D analysis of the transients. In principle, such analysis
            implies issues that cannot be covered by 2D DINA models. Although not self-
            consistent, this approach enables a desired practical accuracy for the evaluation
            of anticipated EM loads.
               Note, that the simulated data may contain rapid oscillations due to physi-
            cal processes in the plasma, as well as computational errors that inevitably
            arise during the numerical integration of relevant stiff systems of differen-
            tial equations. They a priori limit possible accuracy of modelling the EM
              transients.
               Toroidal Plasma Current: In DINA simulations, the toroidal plasma cur-
            rent is modelled as a set of movable ring-shaped current loops (typically,
              5
            10  loops). 3D models using immovable loops with given current variations
            seem to be better suited for eddy current computation. For a transition be-
            tween the models, first, coordinates R and Z sort all movable loops simu-
            lating the plasma current. If there are two loops with coordinates that fit
 R −R ≤ζ,Z −Z ≤ζ  conditions  R 1  − R 2  ≤ ζ Z 1  − Z 2  ≤  ζ , the loops are assumed coincident. For
                                ,
 2
 2
 1
 1
            the reactor, the parameter ζ is generally taken from the interval 40–60 mm.
            In this way, we obtain a set of 2000–2500 unique immovable loops used
            to simulate the plasma current over the entire observation period. In such
            approximation, a relative  error of field computations is within 0.1%. If ζ is
            close to zero, then the numbers of immovable and movable loops are practi-
            cally the same.
               This approach was applied, in particular, for the analysis of EM transients
            during a plasma current discharge in the GLOBUS tokamak [34]. Simulated
            evolutions  of  eddy  currents  induced  in  the  tokamak  vacuum  vessel  demon-
            strated a good agreement with measured data. Experimental validation of the
            numerical results allows us to draw a conclusion that the simulation accuracy is
            quite adequate for such kind of applications.
               Toroidal Magnetic Flux: In 3D models, the toroidal magnetic flux associated
            with the plasma current and obtained as DINA output can be simulated as a flux
            of a virtual toroidal solenoid. The virtual solenoid of radius r is assumed to be
            located inside the vacuum vessel at radius R of the plasma centre. The solenoid
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