Consequences of using simple analytical functions for the high-latitude convection electric field
Journal Article
·
· Journal of Geophysical Research; (USA)
- Air Force Geophysics Lab., Hanscom Air Force Base, Bedford, MA (USA)
The authors have developed analytical functions to represent the convection electric field of Heppner and Maynard (1987), which are realistic representations of the field. The functions include an explicit variability with geomagnetic activity for southward interplanetary magnetic field (IMF). They have used a simple computer algorithm to model the ionosphere and investigate the consequences of using the Heppner-Maynard analytical functions for the high-latitude convection electric field. The Heelis et al (1982) model, which has been widely used by investigators with computer simulations of the magnetosphere, ionosphere and/or thermosphere, is used here to provide a comparison. The Heppner-Maynard functions improve on the simple Heelis function for southward IMF. The Heppner-Maynard functions yield reasonable configurations and magnitude for Joule heating and field-aligned currents for a southward IMF. The Heelis model may or may not yield reasonable results depending on the input parameters. The major differences between the Heppner-Maynard functions and the Heelis function for southward IMF are for regions near (1) the dayside cusp, (2) the Harang discontinuity and (3) the subauroral latitudes. In general, the Heppner-Maynard functions yield results that more closely compare with other investigators. For northward IMF, the functional representations of the Heppner-Maynard do not reproduce the field-aligned currents in the polar cap which have been referred to as the NBZ current system.
- OSTI ID:
- 5831946
- Journal Information:
- Journal of Geophysical Research; (USA), Journal Name: Journal of Geophysical Research; (USA) Vol. 94:A4; ISSN 0148-0227; ISSN JGREA
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640201* -- Atmospheric Physics-- Auroral
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANALYTICAL SOLUTION
AURORAL OVAL
COMPARATIVE EVALUATIONS
COMPUTERIZED SIMULATION
CONVECTION
EARTH ATMOSPHERE
ELECTRIC FIELDS
ELECTRIC HEATING
ENERGY TRANSFER
GEOGRAPHICAL VARIATIONS
GEOMAGNETIC FIELD
HARANG DISCONTINUITY
HEAT TRANSFER
HEATING
INTERPLANETARY MAGNETIC FIELDS
IONOSPHERE
JOULE HEATING
LATITUDE EFFECT
MAGNETIC FIELDS
MASS TRANSFER
MATHEMATICAL MODELS
PLANETARY IONOSPHERES
PLASMA HEATING
POLAR CUSP
POLAR REGIONS
RESISTANCE HEATING
SIMULATION
VARIATIONS
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANALYTICAL SOLUTION
AURORAL OVAL
COMPARATIVE EVALUATIONS
COMPUTERIZED SIMULATION
CONVECTION
EARTH ATMOSPHERE
ELECTRIC FIELDS
ELECTRIC HEATING
ENERGY TRANSFER
GEOGRAPHICAL VARIATIONS
GEOMAGNETIC FIELD
HARANG DISCONTINUITY
HEAT TRANSFER
HEATING
INTERPLANETARY MAGNETIC FIELDS
IONOSPHERE
JOULE HEATING
LATITUDE EFFECT
MAGNETIC FIELDS
MASS TRANSFER
MATHEMATICAL MODELS
PLANETARY IONOSPHERES
PLASMA HEATING
POLAR CUSP
POLAR REGIONS
RESISTANCE HEATING
SIMULATION
VARIATIONS