Published 1984 | Version v1
Book

Electromagnetic field for an open magnetosphere

  • 1. Texas Univ., Richardson

Description

The boundary-layer-dominated models of the earth EM field developed by Heikkila (1975, 1978, 1982, and 1983) and Heikkila et al. (1979) to account for deficiencies in the electric-field descriptions of quasi-steady-state magnetic-field-reconnection models (such as that of Cowley, 1980) are characterized, reviewing the arguments and indicating the most important implications. The mechanisms of boundary-layer formation and field direction reversal are explained and illustrated with diagrams, and it is inferred that boundary-layer phenomena rather than magnetic reconnection may be the cause of large-scale magnetospheric circulation, convection, plasma-sheet formation and sunward convection, and auroras, the boundary layer acting basically as a viscous process mediating solar-wind/magnetosphere interactions. 23 references

Additional details

Publishing Information

Publisher
American Geophysical Union.
Imprint Place
Washington, DC (USA)
Imprint Title
Magnetic reconnection in space and laboratory plasmas; Proceedings of the Chapman Conference on Magnetic Reconnection, Los Alamos, NM, October 3-7, 1983
Journal Page Range
p. 39-44.

Conference

Title
Chapman conference on magnetic reconnection.
Dates
3-7 Oct 1983.
Place
Los Alamos, NM (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
17082083
Subject category
S58: GEOSCIENCES;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CONVECTION; EARTH MAGNETOSPHERE; ELECTRIC FIELDS; ELECTROMAGNETIC FIELDS; MAGNETIC FIELD CONFIGURATIONS; MAGNETOPAUSE; PLASMA; SOLAR WIND
Descriptors DEC
EARTH ATMOSPHERE; ENERGY TRANSFER; HEAT TRANSFER; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS