1989
DOI: 10.1088/0029-5515/29/12/005
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Finite-beta equilibrium magnetic field perturbations in stellarator plasmas

Abstract: Magnetic field perturbations due to finite-beta operation in stellarators have been simulated by using the three-dimensional free-boundary equilibrium code VMEC to overcome the limitations imposed by averaged equilibrium and fixed-boundary methods. Results of these computations have been compared with analytic predictions for cylindrical stellarator models and confirm a linear relationship between the average beta and the plasma dipole moment. Only a weak sensitivity of the computations to details of the press… Show more

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Cited by 21 publications
(14 citation statements)
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“…It should be noted that the dependence is nearly the same as that in Ref. [3], where a set of zero net current stellarator equilibria for the ATF torsatron has been studied. In the presence of the unidirectional current the amplitude of the m = 1 harmonic is practically independent of the current density profile.…”
Section: Results Of Numerical Calculationsmentioning
confidence: 77%
“…It should be noted that the dependence is nearly the same as that in Ref. [3], where a set of zero net current stellarator equilibria for the ATF torsatron has been studied. In the presence of the unidirectional current the amplitude of the m = 1 harmonic is practically independent of the current density profile.…”
Section: Results Of Numerical Calculationsmentioning
confidence: 77%
“…From the viewpoint of magnetic diagnostics, typical (or standard) configurations in conventional stellarators are not so different from those ideal cases integrally independent from the pressure. This has been proved, in particular, by direct calculations for real systems showing that the plasma shape and the measured magnetic signals respond weakly to variations of pressure profile [39][40][41]. The same features can, in fact, be seen in Refs [6][7][8]: the dependence of the calculated magnetic quantities on the profiles of the plasma pressure is very weak.…”
Section: Conventional Stellarators Configurations Independent From Pmentioning
confidence: 73%
“…But this is more of an excuse and is not the main reason for the present article, which is that with growing interest in magnetic diagnostics in stellarators [37][38][39][40][41][63][64][65][66][67] and with excessive orientation of the modern theory towards numerical simulation there arises a natural necessity for a general evaluation of the problem and for stating physically clear general criteria for evaluating any particular result. We would like to emphasize the simple idea that the measured magnetic signals are integral by their nature, and in interpreting experimental results we must take this into account.…”
Section: Resultsmentioning
confidence: 99%
“…For systems with high shear the pressure distribution can be determined by measuring the dipole moment of the poloidal flux. However, even in the low 0 case, this dependence is rather weak and practically disappears as 0 increases [12].…”
Section: Introductionmentioning
confidence: 92%