Published August 1979 | Version v1
Journal article

Magnetic field-line reconnexion by localised enhancement of resistivity

  • 1. Ehime Univ., Matsuyama (Japan)

Description

An examination is made as to how the process of fast reconnexion depends on the magnitude of the local resistivity enhanced in the vicinity of the magnetic neutral point. It is shown that quasi-steady Petschek-type configurations are set up, one for each of the variously imposed local resistivity enhancements. The fundamental structure of the quasi-steady configuration is largely controlled by the initially indented value of locally enhanced resistivity. It is seen that the magnitude of fast reconnexion rate has a weak dependence on the local resistivity in the diffusion region. All the numerical results are very consistent with previous theoretical work on the fast reconnexion problem, once the problem is reconsidered from another angle. It is suggested that the process of fast reconnexion should be viewed as a gross instability, inherent to the current sheet system itself, that can be triggered by some local onset of anomalous resistivity. (author)

Additional details

Additional titles

Subtitle (English)
Pt. 4. Dependence on the magnitude of resistivity

Publishing Information

Journal Title
J. Plasma Phys.
Journal Volume
22
Journal Issue
pt.1
Series
J. Plasma Phys.
Journal Page Range
1-14
ISSN
0022-3778

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
11495652
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Resource subtype / Literary indicator
Numerical Data
Descriptors DEI
COUPLING; EARTH MAGNETOSPHERE; ELECTRIC CONDUCTIVITY; GRAPHS; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC STORMS; MATHEMATICAL MODELS; SOLAR FLARES; THEORETICAL DATA
Descriptors DEC
DATA; DATA FORMS; EARTH ATMOSPHERE; ELECTRICAL PROPERTIES; INFORMATION; NUMERICAL DATA; PHYSICAL PROPERTIES; SOLAR ACTIVITY