A mechanism to produce a dawn-dusk component of plasma flow during magnetic reconnection in the magnetotail
Journal Article
·
· Journal of Geophysical Research
- Univ. of Alaska, Fairbanks, AK (United States); and others
Magnetic reconnection between antiparallel field lines in the magnetotail is generally thought to produce plasma acceleration in the earthward-tailward direction. However, measurements of the plasma velocity in the magnetotail during substorm activity sometimes reveal a dawn-dusk component of plasma flow. In this paper, the authors show that a dawn-dusk component of plasma acceleration may be produced during reconnection if the neutral line is not perpendicular to the magnetic field. In this case, MHD simulations show that reconnection between antiparallel field lines will initially produce plasma acceleration that is nearly parallel to the neutral line because the magnetic tension force is not opposed by a pressure gradient force in this direction. As the magnetic field topology evolves to a steady state, the plasma flow direction rotates until it is nearly parallel to the plane that initially contained the antiparallel magnetic field lines before reconnection (hereafter referred to as the initial field plane). However, the time required to reach a steady state (typically several hundred seconds in the magnetotail region) may be greater than the time during which the reconnection process is active. Consequently, bursts of plasma flow with a dawn-dusk component may occur in the magnetotail. The initial acceleration along the neutral line depends on the angle ({theta}{sub B}) between the neutral line and the initial field plane, with the largest burst of plasma flow along the neutral line occurring when {theta}{sub B}=45{degrees}. 11 refs., 8 figs., 1 tab.
- OSTI ID:
- 121250
- Journal Information:
- Journal of Geophysical Research, Journal Name: Journal of Geophysical Research Journal Issue: A4 Vol. 99; ISSN JGREA2; ISSN 0148-0227
- Country of Publication:
- United States
- Language:
- English
Similar Records
Magnetotail reconnection: Current diversion and field-aligned currents
Southward magnetic field in the neutral sheet produced by wavy motions propagating in the dawn-dusk direction
Three-dimensional computer modeling of dynamic reconnection in the geomagnetic tail
Journal Article
·
Sun Mar 31 23:00:00 EST 1991
· Geophysical Research Letters (American Geophysical Union); (United States)
·
OSTI ID:5187414
Southward magnetic field in the neutral sheet produced by wavy motions propagating in the dawn-dusk direction
Journal Article
·
Tue Oct 31 23:00:00 EST 1989
· Geophysical Research Letters (American Geophysical Union); (USA)
·
OSTI ID:7188527
Three-dimensional computer modeling of dynamic reconnection in the geomagnetic tail
Journal Article
·
Sat Aug 01 00:00:00 EDT 1981
· J. Geophys. Res.; (United States)
·
OSTI ID:5800988