Nonlinear response of a neoclassical four-field magnetic reconnection model to localized current drive
Creators
- 1. Istituto di Fisica del Plasma CNR, Euratom-ENEA-CNR Association, Via R. Cozzi 53, Milan 20125 (Italy)
- 2. Department of Mathematics, Politecnico di Milano, Piazza L. da Vinci 32, Milan 20133 (Italy)
Description
In tokamaks magnetic islands arise from an unstable process of tearing and reconnecting of helical field lines across rational surfaces. After a linear stage the magnetic instability develops through three characteristic nonlinear stages where increasingly complex topological alterations occur in the form of the magnetic islands. The problem of response of reconnection process to the injection of an external current suitably localized is addressed using a four-field model in a plane slab plasma, with a novel extension to account consistently of the relevant neoclassical effects, such as bootstrap current and pressure anisotropy. The results found have implications on the interpretation of the possible mechanism of present day experimental results on neoclassical tearing modes as well as on the concepts for their control or avoidance.
Additional details
Identifiers
- DOI
- 10.1063/1.3428676;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 17
- Journal Issue
- 5
- Journal Page Range
- p. 052509-052509.7
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41101579
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- BOOTSTRAP CURRENT; MAGNETIC ISLANDS; MAGNETIC RECONNECTION; MAGNETOHYDRODYNAMICS; MODE RATIONAL SURFACES; NONLINEAR PROBLEMS; TEARING INSTABILITY; TOKAMAK DEVICES
- Descriptors DEC
- CLOSED PLASMA DEVICES; CURRENTS; ELECTRIC CURRENTS; FLUID MECHANICS; HYDRODYNAMICS; INSTABILITY; MAGNETIC FIELD CONFIGURATIONS; MAGNETIC SURFACES; MECHANICS; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; THERMONUCLEAR DEVICES
Optional Information
- Notes
- (c) 2010 American Institute of Physics