Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Models of high-latitude electric potentials derived with a least error fit of spherical harmonic coefficients

Journal Article · · Journal of Geophysical Research
DOI:https://doi.org/10.1029/95JA01755· OSTI ID:227150
 [1]
  1. Univ. of Alaska, Fairbanks, AK (United States)
New models of the high-latitude electric potentials have been developed. These models show how the polar ionospheric electric field, or plasma convection, responds to changes in the interplanetary magnetic field (IMF) and other parameters, such as dipole tilt angle. These patterns were derived from measurements of the electric field on the DE 2 satellite, using all polar cap passes during which high-resolution IMF data were available from the ISEE 3 or IMP 8 satellites. The data are sorted according to the angle of the IMF in the GSM Y-Z plane. The measurements are further divided into different groups according to the magnitude of the IMF or the dipole tilt angle. All measurements in each group are then used to derive a model of the electric potential for the given conditions, using a new technique where the coefficients of a spherical harmonic expansion are found by least square error fits. The resulting convection patterns are very realistic and show consistent variations as the IMF B{sub Y}/B{sub Z} angle rotates. For northward IMF (positive B{sub Z}) evidently there are four convection {open_quotes}cells,{close_quotes} rather than a distortion of the two-cell pattern. Many other useful facts regarding the solar wind-ionosphere coupling can be extracted from the derived patterns, such as the relationship between the polar cap potential drop and the IMF clock angle. 32 refs., 12 figs., 1 tab.
OSTI ID:
227150
Journal Information:
Journal of Geophysical Research, Journal Name: Journal of Geophysical Research Journal Issue: A10 Vol. 100; ISSN JGREA2; ISSN 0148-0227
Country of Publication:
United States
Language:
English

Similar Records

Control parameters for polar ionospheric convection patterns during northward interplanetary magnetic field
Journal Article · Thu Mar 14 23:00:00 EST 1996 · Geophysical Research Letters · OSTI ID:245174

Ionospheric convection response to slow, strong variations in a northward interplanetary magnetic field: A case study for January 14, 1988
Journal Article · Sun Oct 31 23:00:00 EST 1993 · Journal of Geophysical Research · OSTI ID:146562

Response time of the polar ionospheric convection pattern to changes in the north-south direction of the IMF
Journal Article · Tue Feb 28 23:00:00 EST 1995 · Geophysical Research Letters · OSTI ID:183358