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U.S. Department of Energy
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Stellarator physics-evaluation studies

Conference ·
OSTI ID:6801033
A wide range of stellarator/torsatron configurations is evaluated and compared using vacuum field flux surface topology, MHD equilibrium beta limits and guiding center orbit confinement as optimization criteria. The torsatron is found to be a better choice for a near term physics experiment than the modular stellarator or helical configurations studied. The best torsatron geometry has an equilibrium beta limit of <..beta..> = 4 to 5% for a plasma aspect ratio of 7 and 7 to 8% for an aspect ratio of 14. A feasible torsatron modularization scheme which retains the physics properties is shown. A wide variety of flux surface geometries can be produced due to the additional flexibility introduced by toroidally-directed windbacks and compensating coils. The effects of different methods of calculating MHD equilibrium/stability, different pressure profiles, and different vertical fields on the results are discussed. Guiding center orbit containment is a less sensitive indicator of configuration quality than is the equilibrium beta limit. Orbits for thermal and fast ions are calculated in field line (flux) coordinates using actual fields and including electric fields, pitch angle scattering and fast ion slowing down.
Research Organization:
Oak Ridge National Lab., TN (USA)
DOE Contract Number:
W-7405-ENG-26
OSTI ID:
6801033
Report Number(s):
IAEA-CN-41/Q-3; CONF-820930-18; ON: DE82022298
Country of Publication:
United States
Language:
English