Page 96 - Fundamentals of Magnetic Thermonuclear Reactor Design
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80     Fundamentals of Magnetic Thermonuclear Reactor Design


            In terms of surface coordinates ξ and η a radius-vector of any point on the quad-
            rilateral surface can be taken in the form

                                           4
                                   r ξη = ∑  N ( ξ n,) r
                                        )
                                    (,
 r(ξ,η)=∑i=14Ni(ξ,n)ri−1≤ξ, η≤1,              i     i
                                           = i 1
                                          −≤  ξη ≤1,
                                               ,
                                           1
 Ni(ξ,η)=1/4(1+ξiξ)(1+ηiη),
                                            ξη =±1.
                     ξη =)1 /4(1
 ξi,ηi=±1.  where  N (,        +  ξξ)(1 +  ηη),   i ,  i
                   i
                                  i
                                        i
               We use the same shape functions  N (,
                                             ξη) to approximate the B distribution
                                           i
 Ni(ξ,η)    on the quadrilateral surface. Then the final equation for the magnetic flux will
            take the form
 Φ=1/2{(r14×r23)⋅B +1/3(r14×∆  Φ = 1/ 2{( r ×  r ) ⋅ B +1/ 3( r ×∆ B +  r × ∆ B )  r ⋅  ξη },
                                             14
                             14
                                 23
                                      0
                                                       23
                                                   23
                                                             14
 0
 B23+r23×∆B14)⋅rξη},
                         r
 ,
 i
 B
 B =1/4(B +B +B rij=rj−ri,  where  r =  r − , B∆ ij  =  B −  B , i    B = 1/ 4( B +  B +  B +  B ),
 =+B ),
 j
                                                      2
                                                               4
                                                  1
                                                           3
                                          0
                   ij
                      j
                                  j
                         i
 −
 B 4
 ∆Bij 3
 1
 0
 2
                                                          r
                           r = 1/ 4  ξη r = 1 /4( r − r −  r + ).
 rξη=1/4∑ξiηiri=1/4(r −r −r +  ξη  ∑ i  i i     1  2   3  4
 3
 2
 1
 r ).          Software modules enabling the implementation of this approach have
 4
            been incorporated, as post-processing tools, in the computer codes intended
            to simulate 3D magnetostatic fields. The user can control the computation ac-
            curacy determining the balance of magnetic fluxes coming through any closed
            surfaces.
               A complex system design has to account for the interaction of different
            functional components. As to the ITER design, the stray field of the reactor,
            affected by the building steel rebar and ferromagnetic surroundings, influ-
            ence the operation of the neutral beam injectors, turbomolecular pumps, and
            diagnostic equipment. The modelling of such problems is often complicated
            by the fact that each MS would be well described by a local FE mesh. How-
            ever,  common  meshing  is  a  very  laborious  task. The  common  mesh  gets
            so sizable, that the problem cannot be solved in principle or in reasonable
            time, while the mutual effect of the functional components is often specified
            analytically or in a tabulated form, rather than described in terms of the FE
            approach.
               To solve the problem, field H , generated by external sources, should be
                                       ext
            applied and adjusted at the next stage to find a self-consistent solution in the
            regions of interest.
               Let a static magnetic field be described by vectors B, H, M and j. The vec-
            tors are related by Eqs. (4.1)–(4.3). We introduce the field H  that may be
                                                               ext
            determined, particularly, as a field generated by current sources j in vacuum.
            This field fits
 ∇×Hext=j,  ∇⋅µ Hext=0.         ∇×  H ext  =  j,  ∇  µ ⋅  0 H ext  = 0.
 0
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