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Magnetic Fields and Magnetic Diagnostics for Tokamak Plasmas

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<strong>Magnetic</strong> fields <strong>and</strong> tokamak plasmas<br />

Alan Wootton<br />

Figure 1.10. The poloidal flux ψ in the plane z = 0 <strong>for</strong> a circular current loop,<br />

radius 1 m, current I = 1/µ 0 . The solid line is the exact solution, the long dash line<br />

is the far field solution, <strong>and</strong> the short dash line is the very near field solution (zero<br />

order in ρ/R terms only).<br />

ψ<br />

exact<br />

very near<br />

zero order<br />

first order<br />

Radius R (m)<br />

Figure 1.11 The poloidal flux ψ in the plane z = 0 <strong>for</strong> a circular current loop,<br />

radius 1 m, current I = 1/µ 0 . The solid line is the exact solution, the short dash line<br />

is the first order expansion in ρ/R 0 solution keeping terms of order ρ/R 0 , <strong>and</strong> the<br />

long dash line is the very near field solution (zero order in ρ/R terms only).<br />

We can also compare the zero order, first order <strong>and</strong> exact solutions by plotting contours of ψ in<br />

(R,z) space. This is done in Figure 1.12, <strong>for</strong> the conditions described in the caption of Figure<br />

1.11. We see that it is very important to include the first order in ρ/R 0 terms; even then the<br />

solution contours are significantly different from the exact solution contours. This is very<br />

different from the case of the vector potential, where the zero order solution was accurate.<br />

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