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A dissipative model of a stationary, axisymmetric plasma configuration is used to calculate the pressure and toroidal magnetic field strength as functions of the poloidal magnetic flux in Grad-Shafranov's equation. Interface and boundary conditions are considered for a configuration where the toroidal plasma column with simply-connected meridional section is encircled by a vacuum region with annular meridional section. Possible iterative procedures are suggested for solution.

Additional information

Authors: SURDO C L, ENEA, Centro Ricerche Energia Frascati, Roma (IT)
Bibliographic Reference: Report: RT/ERG/FUS/94/08 EN (1994) 23 pp.
Availability: Available from Servizio Studi e Documentazione, ENEA, Centro Ricerche Energia Frascati, C.P. 65-00044 Frascati, Roma (IT)
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