
KSTAR discharge #18594 [29] is a typical Hmode [34] discharge in a midsized tokamak. Figure 14.1 shows the equilibrium magnetic fluxsurfaces in this discharge at time ms, at which time T, m, m, and . Figures 14.2 and 14.3 show the corresponding pressure, safetyfactor, and profiles [29]. Of course, the equilibrium fluxsurfaces shown in Figure 14.1, combined with the and profiles specified in Figures 14.2 and 14.3, constitute a solution of the GradShafranov equation, (14.33). Note that the safetyfactor becomes infinite at the edge of the plasma, due to the presence of a magnetic Xpoint on the bounding magnetic fluxsurface. (See Figure 14.1.) In principle, there are an infinite number of rational surfaces lying within the plasma. However, if we truncate the plasma at (i.e., at the magnetic fluxsurface that contains 99.5% of the poloidal magnetic flux contained by the last closed fluxsurface), which is the standard approach, then there are only four such surfaces. The properties of these surfaces are listed in Table 14.1.
Table 14.2 specifies the elements of the Ematrix in KSTAR discharge #18594 at time ms, calculate according to the procedure set out in Section 14.12. As expected, it can be seen that the matrix is Hermitian. Moreover, all of the diagonal elements of the matrix are negative, which indicates that the tearing mode are all classically stable. (This is not surprising because the classical drive is absent from our calculation.) Finally, the offdiagonal elements of the matrix are all substantial, indicating that there is significant coupling between different poloidal harmonics.
In order to determine the effective tearing stability index for an toroidal tearing mode that reconnects magnetic flux at a particular rational surface in the plasma, let us assume that the responses of the other rational surfaces exhibit strong shielding. This assumption can be justified a posteriori. Our assumption implies that very little magnetic reconnection is driven at the other rational surfaces. In this case, it is reasonable to calculate the responses of these surfaces using linear theory. (The linear approximation is valid as long as the widths of the magnetic island chains driven at the other rational surfaces are less than the corresponding linear layer widths. See Section 5.16.)
According to the analysis of Chapter 5, the linear response of the th rational surface is characterized by
where(14.124)  
(14.125)  
(14.126)  
(14.127)  
(14.128)  
(14.129)  
(14.130)  
(14.131)  
(14.132)  
(14.133)  
(14.134)  
(14.135)  
(14.136)  
(14.137)  
(14.138)  
(14.139)  
(14.140) 

Equation (14.123) states that the linear response of the th rational surface to a magnetic perturbation generated at another rational surface is governed by nine dimensionless parameters. These parameters are the Lundquist number, , the normalized mode frequency, , the normalized EcrossB frequency, , the normalized electron diamagnetic frequency, , the normalized ion diamagnetic frequency, , the pressure gradient ratio parameter, , the semicollisional parameter, , and the two magnetic Prandtl numbers, and . (Note that these parameters are called , , , , , , , and , respectively, in Chapter 5.) The dimensionless layer response index, , can be calculated numerically as a function of these nine parameters by solving the Riccati differential equation, (5.121), subject to the boundary conditions (5.122) and (5.123).
Figure 14.3 shows the experimental number density, temperature, and EcrossB frequency profiles in KSTAR discharge #18594 at time ms [29]. The majority ions are deuterium, whereas the impurity ions are carbonVI (i.e., ). The majority ion and impurity ion number density profiles are calculated from the measured electron number density profile [see Equations (A.4) and (A.5)] on the assumption that the effective ion charge number, [see Equation (A.3)], takes the value throughout the plasma. (This value is a best guess based on the measured stored energy.) The impurity ions are assumed to have the same temperature as the measured temperature of the majority ions. The EcrossB frequency profile is deduced from the measured impurity ion toroidal angular velocity profile using the neoclassical theory outlined in Appendix A [15]. In particular, the impurity ion poloidal angular velocity profile is assumed to take its neoclassical value. (See Section A.7). Furthermore, the ion perpendicular momentum and perpendicular particle diffusivities are given the plausible values and , respectively, throughout the plasma [34]. Finally, the values of the various resistive layer parameters, determined from the data shown in Figure 14.3, as well as the aforementioned assumptions, are given in Table 14.3.