Published October 2003 | Version v1
Journal article

Blob stability and transport in the scrape-off-layer

  • 1. Lodestar Research Corporation, 2400 Central Avenue, Boulder, Colorado 80301 (United States)

Description

High-density plasma filaments extended along the magnetic field, which look like 'blobs' in the plane perpendicular to B, have been observed in the scrape-off-layer (SOL) of many plasma devices. These objects become polarized and subsequently ExB drift to the wall carrying a significant flux of particles. This mechanism may account for the observed nondiffusive, intermittent transport in the far SOL of tokamaks. Previous work has examined simple models of blob propagation and shown that the radial convective velocity ux has the scaling ux∝yb-2, where yb is the poloidal blob dimension. Thus, the radial particle flux is sensitive to the details of the blob size and shape distributions; these in turn are affected by various secondary instabilities which cause blob fragmentation. A simple model of blob instability (driven by curvature in the presence of sheath boundary conditions) is studied by 1D calculations and 2D simulations to provide insight on the stability and dynamics of blobs. It is shown that a competition between the time scales for instability and transport determines the range of allowed blob sizes and shapes and constrains the overall radial velocity

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
10
Journal Issue
10
Journal Page Range
p. 4029-4039
ISSN
1070-664X
CODEN
PHPAEN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
35052913
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
BOUNDARY LAYERS; MAGNETIC FIELDS; PLASMA; PLASMA INSTABILITY; PLASMA SCRAPE-OFF LAYER; STABILITY; TOKAMAK DEVICES; TRANSPORT
Descriptors DEC
BOUNDARY LAYERS; CLOSED PLASMA DEVICES; INSTABILITY; LAYERS; THERMONUCLEAR DEVICES

Optional Information

Notes
(c) 2003 American Institute of Physics.