Published November 1, 1990 | Version v1
Journal article

Field-aligned current signatures in the near-tail region. 2. Coupling between the region 1 and region 2 systems

  • 1. Johns Hopkins Univ., Laurel, MD (United States)
  • 2. Univ. of Tokyo (Japan)
  • 3. Los Alamos National Lab., NM (United States)
  • 4. Univ. of California, Los Angeles (United States)
  • 5. NASA Goddard Space Flight Center, Greenbelt, MD (United States)

Description

The development of the substorm-associated current system in the near-tail region is examined in the light of both experiment and theory. First, the March 28, 1979, event is examined intensively by using ground magnetometer data and satellite magnetic field and energetic particle data. The comparison of field-aligned current signatures at geosynchronous altitude and in the near-tail region indicates that the development of the region 1 system is not merely the enhancement in current intensity of the pre-existing system. This finding is consistent with the so-called current wedge model, in which the tail current is converted into a pair of field-aligned currents with the region 1 polarity at substorm onsets. Detailed inspection, however, suggests that the region 2 system is as important as the region 1 system. Statistical properties of the azimuthal magnetic component at synchronous orbit indicate that the deviation during disturbed periods is larger than expected from the enhancement of the region 1 current. These individual and statistical studies suggest that the region 2 system tends to develop in the synchronous region and that the coupling between the region 1 and the region 2 systems is important. The current closure in the magnetosphere is discussed from a viewpoint of the macroscopic behavior of plasma. It is suggested that the dawnside and the duskside region 2 currents are closed in the magnetosphere by the curvature current during the growth phase and by the magnetic gradient current during the expansion phase. The field-aligned currents of the region 1 and the region 2 systems are closed in the ionosphere by the Pedersen current. Consequently, the energy is dissipated as the Joule heating and this energy must be supplied from the magnetosphere. Therefore, the counter part of the Pedersen current, which closes the region 1 and the region 2 currents in magnetosphere, must be the dynamo current

Additional details

Publishing Information

Journal Title
Journal of Geophysical Research
Journal Volume
95
Journal Issue
A11
Series
J. Geophys. Res.
Journal Page Range
18913-18927
ISSN
0148-0227
CODEN
JGREA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
23007840
Subject category
S58: GEOSCIENCES;
Descriptors DEI
COMPARATIVE EVALUATIONS; DATA; EARTH MAGNETOSPHERE; ELECTRIC CURRENTS; ENERGY LOSSES; IONOSPHERE; JOULE HEATING; MAGNETIC BAYS; MAGNETOTAIL; MATHEMATICAL MODELS; PLASMA; STATISTICS
Descriptors DEC
CURRENTS; EARTH ATMOSPHERE; EVALUATION; HEATING; INFORMATION; MATHEMATICS