Published February 1979 | Version v1
Journal article

Time-dependent configuration changes of the magnetotail and plasma sheet thinning

Creators

  • 1. Kean Coll. of New Jersey, Union (USA). Dept. of Earth and Planetary Environments

Description

The configuration of the magnetotail magnetic field has been calculated for a situation where a disruption of a portion of the tail current system develops. The decrease of the current in a localised region of the magnetotail leads to a collapse of the magnetic field in that vicinity. The calculated configuration of the field resembles what is predicted by reconnection models with the field lines moving toward the neutral sheet and then connecting and either moving toward or away from the earth. Associated with this changing magnetic field there is an induced electric field which will then influence the motion of the plasma in the magnetotail via E x B drifts. The calculations show that the induced electric field of a time-dependent magnetic field is able to explain certain observed features of the plasma sheet motions. Also, this agreement suggests that the assumption that there is no charge separation contribution to the electric field may be reasonable during situations of large scale and rapid current disruptions in the magnetotail. (author)

Additional details

Publishing Information

Journal Title
Planet. Space Sci.
Journal Volume
27
Journal Issue
2
Series
Planet. Space Sci.
Journal Page Range
103-112
ISSN
0032-0633

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
10469568
Subject category
S58: GEOSCIENCES;
Descriptors DEI
ELECTRIC CURRENTS; ELECTRIC FIELDS; GEOMAGNETIC FIELD; MAGNETIC BAYS; MAGNETIC FIELD CONFIGURATIONS; MAGNETIC STORMS; MAGNETOTAIL; MATHEMATICAL MODELS; PLASMA DRIFT; PLASMA SHEET; TIME DEPENDENCE
Descriptors DEC
CURRENTS; MAGNETIC FIELDS