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Reduction of the field‐aligned potential drop in the polar cap during large geomagnetic storms
Author(s) -
Kitamura N.,
Seki K.,
Nishimura Y.,
Hori T.,
Terada N.,
Ono T.,
Strangeway R. J.
Publication year - 2013
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/jgra.50450
Subject(s) - earth's magnetic field , geomagnetic storm , polar , ionosphere , atmospheric sciences , geophysics , physics , magnetic field , astronomy , quantum mechanics
We have studied photoelectron flows and the inferred field‐aligned potential drop in the polar cap during five large geomagnetic storms, which occurred in the periods when the photoelectron observations in the polar cap are available near the apogee of the Fast Auroral SnapshoT satellite (~4000 km) at solar maximum, and the footprint of the satellite paths in the polar cap was under sunlit conditions most of the time. In contrast to the ~20 V potential drop during geomagnetically quiet periods at solar maximum identified by Kitamura et al. (2012), the field‐aligned potential drop frequently became smaller than ~5 V during the main and early recovery phases of the large geomagnetic storms. This result indicates that the acceleration of ions by a field‐aligned potential drop in the polar cap and the lobe region is smaller during the main and early recovery phases of large geomagnetic storms compared to during geomagnetically quiet periods. Since ions with large flux originating from the cusp/cleft ionosphere convect into the polar cap during geomagnetic storms, the net escaping electron number flux should increase to balance the enhanced ion outflows under small field‐aligned current conditions. The magnitude of the field‐aligned potential drop would be reduced to let larger part of photoelectrons escape.