Edge-localized modes and edge transport in spherical tokamaks
Creators
- 1. Institute for Research in Electronics and Applied Physics, University of Maryland, Maryland 20742-3511 (United States)
Description
Turbulent energy transport in numerical simulations of the edge region of spherical tokamaks with small toroidal aspect ratio A=1.5 is directly compared to that in conventional tokamaks with larger aspect ratio A=3. Depending upon the aspect ratio of the torus, the energy flux can vary greatly. While a tokamak plasma with aspect ratio A=3 is in the high (H) mode where the transport rate is small, an otherwise identical tokamak plasma with small aspect ratio A=1.5 exhibits extremely poor confinement. The magnitude of the energy flux in these two cases differs by a multiplicative factor larger than 50. However, good H mode confinement in small aspect ratio spherical tokamaks can be obtained by a further increase in the edge density gradient. Confinement is then dominated by bursts of ballooning modes which periodically transport energy to large major radius. The periodic bursts in the numerical simulations are similar to the periodic radiation bursts that characterize edge-localized modes in tokamaks
Additional details
Identifiers
- DOI
- 10.1063/1.1914806;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 12
- Journal Issue
- 5
- Journal Page Range
- p. 052518-052518.5
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37034591
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ASPECT RATIO; BALLOONING INSTABILITY; EDGE LOCALIZED MODES; H-MODE PLASMA CONFINEMENT; PLASMA DENSITY; PLASMA SIMULATION; TOKAMAK DEVICES; TURBULENCE
- Descriptors DEC
- CLOSED PLASMA DEVICES; CONFINEMENT; DIMENSIONLESS NUMBERS; INSTABILITY; MAGNETIC CONFINEMENT; PLASMA CONFINEMENT; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; SIMULATION; THERMONUCLEAR DEVICES
Optional Information
- Notes
- (c) 2005 American Institute of Physics