Electromagnetic field for an open magnetosphere
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