skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: MHD stability of the MHH2 stellarator

Technical Report ·
DOI:https://doi.org/10.2172/334076· OSTI ID:334076
 [1]
  1. New York Univ., NY (United States). Courant Inst. of Mathematical Sciences

The NSTAB code provides a computer implementation of the variational principle of magnetohydrodynamics. Excellent resolution is obtained by combining a spectral representation in the toroidal and poloidal angles with a low order, but exceptionally accurate, finite difference scheme in the radial direction. Conservation form of the magnetostatics equations is used to capture islands and current sheets effectively on crude grids. This method enables one to discuss global stability by analyzing bifurcated solutions of the equilibrium problem. The author applies it to investigate the physics of the MHH2 stellarator, whose magnetic structure has a remarkable property of quasi-axial symmetry.

Research Organization:
Univ. of Wisconsin, Center for Plasma Theory and Computation, Madison, WI (United States)
Sponsoring Organization:
USDOE, Washington, DC (United States); National Science Foundation, Washington, DC (United States)
DOE Contract Number:
FG02-86ER53223
OSTI ID:
334076
Report Number(s):
CONF-9803121-PROC.; ON: DE99001004; TRN: 99:005152
Resource Relation:
Conference: Workshop on nonlinear MHD and extended MHD, Atlanta, GA (United States), 25-26 Mar 1998; Other Information: PBD: [1998]; Related Information: Is Part Of Proceedings of the workshop on nonlinear MHD and extended MHD; PB: [75] p.
Country of Publication:
United States
Language:
English

Similar Records

A high performance spectral code for nonlinear MHD stability
Technical Report · Tue Sep 01 00:00:00 EDT 1992 · OSTI ID:334076

A high performance spectral code for nonlinear MHD stability
Technical Report · Tue Sep 01 00:00:00 EDT 1992 · OSTI ID:334076

A high-performance spectral code for nonlinear MHD stability
Miscellaneous · Wed Jan 01 00:00:00 EST 1992 · OSTI ID:334076