It is well known that the size of the superbananas in stellarators scales with the minor radius. Thus, in some stellarator configurations superbananas may not be confined. To improve stellarator confinement, a theory is developed to include the effects of the magnetic well and the radial gradient of the radial electric field to squeeze superbananas. It is found that the size of the superbananas is reduced by a factor of S-1/2, where S is the superbanana squeezing factor that depends on the magnetic well depth and the radial gradient of the radial electric field. The corresponding fraction of the superbanana is increased by a factor of S-1/2. The diffusive loss is thus reduced by a factor of S-3/2. (C) 2002 American Institute of Physics.
机构:
MIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USAMIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USA
Catto, Peter J.
Tolman, Elizabeth A.
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Inst Adv Study, Princeton, NJ 08540 USA
Flatiron Inst, Ctr Computat Astrophys, 162 Fifth Ave, New York, NY 10010 USAMIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USA
Tolman, Elizabeth A.
Parra, Felix I.
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Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08540 USAMIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USA