1997
DOI: 10.1063/1.872322
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Cylindrical ideal magnetohydrodynamic equilibria with incompressible flows

Abstract: It is proved that (a) the solutions of the ideal magnetohydrodynamic equation, which describe the equlibrium states of a cylindrical plasma with purely poloidal flow and arbitrary cross sectional shape [G. N. Throumoulopoulos and G. Pantis, Plasma Phys. and Contr. Fusion 38, 1817Fusion 38, (1996] are also valid for incompressible equlibrium flows with the axial velocity component being a free surface quantity and (b) for the case of isothermal incompressible equilibria the magnetic surfaces have necessarily … Show more

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Cited by 38 publications
(53 citation statements)
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“…Since for fusion plasmas the thermal conduction along B is expected to be fast in relation to the heat transport perpendicular to a magnetic surface, equilibria with isothermal magnetic surfaces are a reasonable approximation [17,18,19,20,21,22]. In particular, the even simpler case of isothermal resistive equilibria has also been considered [23].…”
Section: B Isothermal Magnetic Surfacesmentioning
confidence: 99%
“…Since for fusion plasmas the thermal conduction along B is expected to be fast in relation to the heat transport perpendicular to a magnetic surface, equilibria with isothermal magnetic surfaces are a reasonable approximation [17,18,19,20,21,22]. In particular, the even simpler case of isothermal resistive equilibria has also been considered [23].…”
Section: B Isothermal Magnetic Surfacesmentioning
confidence: 99%
“…In particular, analytic equilibrium solutions have been obtained as solutions to generalized Grad-Shafranov equations (Refs. [3,4,6,7,9,10,11,13]). An impact of the equilibrium flow related to the convective term in the momentum equation is that the isobaric surfaces deviate from the magnetic surfaces.…”
Section: Introductionmentioning
confidence: 99%
“…On the other hand, under the simplifying condition of divergence-free flows, non field-aligned rotational equilibria could be readily solved. [23][24][25] Recently, in terms of spherical coordinates, 26 the non field-aligned equilibria have been solved under a set of transformed MHD variables. 27 With these new variables, the functional dependence of the rotational Grad-Shafranov equation, plasma pressure, normal electric field, on the plasma variables are sufficiently simple and explicit to allow an understanding of the L=H mode transition through a positive feedback cycle.…”
Section: Introductionmentioning
confidence: 99%