Contributions of the low-latitude boundary layer to the finite width magnetotail convection model
Convection of plasma within the terrestrial nightside plasma sheet contributes to the structure and, possibly, the dynamical evolution of the magnetotail. In order to characterize the steady state convection process, the authors have extended the finite tail width model of magnetotail plasma sheet convection. The model assumes uniform plasma sources and accounts for both the duskward gradient/curvature drift and the earthward E [times] B drift of ions in a two-dimensional magnetic geometry. During periods of slow convection (i.e., when the cross-tail electric potential energy is small relative to the source plasma's thermal energy), there is a significant net duskward displacement of the pressure-bearing ions. The electrons are assumed to be cold, and the authors argue that this assumption is appropriate for plasma sheet parameters. They generalize solutions previously obtained along the midnight meridian to describe the variation of the plasma pressure and number density across the width of the tail. For a uniform deep-tail source of particles, the plasma pressure and number density are unrealistically low along the near-tail dawn flank. They therefore add a secondary source of plasma originating from the dawnside low-latitude boundary layer (LLBL). The dual plasma sources contribute to the plasma pressure and number density throughout the magnetic equatorial plane. Model results indicate that the LLBL may be a significant source of near-tail central plasma sheet plasma during periods of weak convection. The model predicts a cross-tail pressure gradient from dawn to dusk in the near magnetotail. They suggest that the plasma pressure gradient is balanced in part by an oppositely directed magnetic pressure gradient for which there is observational evidence. Finally, the pressure to number density ratio is used to define the plasma 'temperature.'
- Research Organization:
- Aerospace Corp., El Segundo, CA (United States)
- OSTI ID:
- 6972695
- Report Number(s):
- N-94-35392; NASA-CR-196116; NAS-1.26:196116; ATR-91(7234)-1; CNN: NAGW-2126; NSF ATM-91-15557
- Country of Publication:
- United States
- Language:
- English
Similar Records
Consequences of magnetotail ion dynamics
Generation of kinetic Alfven waves in the high-latitude near-Earth magnetotail: A global hybrid simulation
Related Subjects
GENERAL PHYSICS
MAGNETOTAIL
CONVECTION
PLASMA SHEET
BOUNDARY LAYERS
MAGNETOHYDRODYNAMICS
MATHEMATICAL MODELS
EARTH ATMOSPHERE
EARTH MAGNETOSPHERE
ENERGY TRANSFER
FLUID MECHANICS
HEAT TRANSFER
HYDRODYNAMICS
LAYERS
MASS TRANSFER
MECHANICS
661320* - Auroral
Ionospheric
& Magnetospheric Phenomena- (1992-)