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