How does the U-shaped potential close above the acceleration region? A study using Polar data

We present a statistical study of Polar electric field observations using auroral oval passes over Scandinavia above the acceleration region. We are especially interested in seeing whether we can find large perpendicular electric fields associated with an upward extended classical U-shaped poten...

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Main Authors: P. Janhunen, A. Olsson, F. S. Mozer, H. Laakso
Format: Article
Language:English
Published: Copernicus Publications 1999-10-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/17/1276/1999/angeo-17-1276-1999.pdf
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author P. Janhunen
A. Olsson
A. Olsson
F. S. Mozer
H. Laakso
author_facet P. Janhunen
A. Olsson
A. Olsson
F. S. Mozer
H. Laakso
author_sort P. Janhunen
collection DOAJ
description We present a statistical study of Polar electric field observations using auroral oval passes over Scandinavia above the acceleration region. We are especially interested in seeing whether we can find large perpendicular electric fields associated with an upward extended classical U-shaped potential drop for these passes, during which Polar is in the northern hemisphere usually at about 4 <i>R<sub>E</sub></i> altitude. We also use Polar magnetic field data to infer the existence of a field-aligned current (FAC) and conjugate ground-based magnetometers (the IMAGE magnetometer network) to check whether the event is substorm-related or not. We find several events with a FAC but only weak perpendicular electric fields at Polar. In those rare cases where the Polar electric field was large, its direction was mostly found to be incompatible with the U-shaped potential model, or it was associated with disturbed conditions (substorms), where one cannot easily distinguish between inductive and static perpendicular electric fields. We found only two cases which are compatible with the upward extended U-shaped potential picture, and even in those cases the potential value is quite small (1-2 kV). To check the validity of the analysis method we also estimate the perpendicular electric field on the southern hemisphere, where Polar flies within or below the acceleration region, and we found a large number of inverted-V-type signatures as expected from previous studies. To explain the lack of perpendicular electric fields at high altitudes we suggest an O-shaped potential model instead of the U-shaped one.<br><br><b>Key words. </b>Ionosphere (particle acceleration) · Magnetospheric physics (auroral phenomena; magnetosphere · ionosphere interactions)
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spelling doaj.art-cff0cb58e7c4404396da3523de10cf292022-12-22T03:54:15ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05761999-10-01171276128310.1007/s00585-999-1276-xHow does the U-shaped potential close above the acceleration region? A study using Polar dataP. Janhunen0A. Olsson1A. Olsson2F. S. Mozer3H. Laakso4Finnish Meteorological Institute, Geophysical Research, Helsinki, FinlandFinnish Meteorological Institute, Geophysical Research, Helsinki, FinlandSwedish Institute of Space Physics, Uppsala Division, Uppsala, SwedenSpace Sciences Laboratory, University of California, Berkeley, USAFinnish Meteorological Institute, Geophysical Research, Helsinki, FinlandWe present a statistical study of Polar electric field observations using auroral oval passes over Scandinavia above the acceleration region. We are especially interested in seeing whether we can find large perpendicular electric fields associated with an upward extended classical U-shaped potential drop for these passes, during which Polar is in the northern hemisphere usually at about 4 <i>R<sub>E</sub></i> altitude. We also use Polar magnetic field data to infer the existence of a field-aligned current (FAC) and conjugate ground-based magnetometers (the IMAGE magnetometer network) to check whether the event is substorm-related or not. We find several events with a FAC but only weak perpendicular electric fields at Polar. In those rare cases where the Polar electric field was large, its direction was mostly found to be incompatible with the U-shaped potential model, or it was associated with disturbed conditions (substorms), where one cannot easily distinguish between inductive and static perpendicular electric fields. We found only two cases which are compatible with the upward extended U-shaped potential picture, and even in those cases the potential value is quite small (1-2 kV). To check the validity of the analysis method we also estimate the perpendicular electric field on the southern hemisphere, where Polar flies within or below the acceleration region, and we found a large number of inverted-V-type signatures as expected from previous studies. To explain the lack of perpendicular electric fields at high altitudes we suggest an O-shaped potential model instead of the U-shaped one.<br><br><b>Key words. </b>Ionosphere (particle acceleration) · Magnetospheric physics (auroral phenomena; magnetosphere · ionosphere interactions)https://www.ann-geophys.net/17/1276/1999/angeo-17-1276-1999.pdf
spellingShingle P. Janhunen
A. Olsson
A. Olsson
F. S. Mozer
H. Laakso
How does the U-shaped potential close above the acceleration region? A study using Polar data
Annales Geophysicae
title How does the U-shaped potential close above the acceleration region? A study using Polar data
title_full How does the U-shaped potential close above the acceleration region? A study using Polar data
title_fullStr How does the U-shaped potential close above the acceleration region? A study using Polar data
title_full_unstemmed How does the U-shaped potential close above the acceleration region? A study using Polar data
title_short How does the U-shaped potential close above the acceleration region? A study using Polar data
title_sort how does the u shaped potential close above the acceleration region a study using polar data
url https://www.ann-geophys.net/17/1276/1999/angeo-17-1276-1999.pdf
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