Published 1988
| Version v1
Book
Polar wind
Creators
Description
The classical polar wind is considered to be an ambipolar outflow of thermal plasma from the terrestrial ionosphere at high latitudes. The paper reviews the characteristic features of this flow, with emphasis placed on recent theoretical predictions. Consideration is given to H(+) and He(+) outflow characteristics both with and without convection electric field effects, the collisionless polar wind characteristics (including the formation of temperature anisotropies), and the time-dependent polar wind behavior in response to localized density perturbations and localized heat sources. 29 references
Additional details
Publishing Information
- Publisher
- American Geophysical Union.
- Imprint Place
- Washington, DC (USA)
- Imprint Title
- Modeling magnetospheric plasma; Proceedings of the First Huntsville Workshop on Magnetosphere/Ionosphere Plasma Models, Guntersville, AL, Oct. 14-16, 1987
- Journal Page Range
- p. 219-228.
Conference
- Title
- 1. Huntsville workshop on magnetosphere/ionosphere plasma models.
- Dates
- 14-16 Oct 1987.
- Place
- Guntersville, AL (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20033429
- Subject category
- S58: GEOSCIENCES;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CATIONS; EARTH MAGNETOSPHERE; ELECTRIC FIELDS; HELIUM IONS; HOT PLASMA; HYDROGEN IONS; INTERACTIONS; ION DENSITY; ION TEMPERATURE; IONIC COMPOSITION; IONOSPHERE; POLAR REGIONS; SOLAR WIND; TIME DEPENDENCE; WIND
- Descriptors DEC
- CHARGED PARTICLES; EARTH ATMOSPHERE; IONS; PLASMA; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS