Affiliation:
1. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder Colorado USA
2. Department of Physics and Astronomy Rice University Houston Texas USA
3. National Geophysical Data Center NOAA Boulder Colorado USA
Abstract
AbstractThe subauroral polarization stream (SAPS) is an important magnetosphere‐ionosphere (MI) coupling phenomenon that impacts a range of particle populations in the inner magnetosphere. SAPS studies often emphasize ionospheric signatures of fast westward flows, but the equatorial magnetosphere is also affected through strong radial electric fields in the dusk sector. This study focuses on a period of steady southward interplanetary magnetic field (IMF) during the 29 June 2013 geomagnetic storm where the Van Allen Probes observe a region of intense electric fields near the plasmapause over multiple consecutive outbound duskside passes. We show that the large‐amplitude electric fields near the equatorial plane are consistent with SAPS by investigating the relationship between plasma sheet ion and electron boundaries, associated field‐aligned currents, and the spatial location of the electric fields. By incorporating high‐inclination DMSP data we demonstrate the spatial and temporal variability of the SAPS region, and we suggest that discrete, earthward propagating injections are driving the observed strong electric fields at low L shells in the equatorial magnetosphere. We also show the relationship between SAPS and plasmasphere erosion, as well as a possible correlation with flux enhancements for 100s keV electrons.
Funder
NASA/Van Allen Probes ECT and EFW
NASA
NASA/THEMIS
NASA Earth and Space Sciences Fellowship (NESSF)
NASA HGC
Publisher
American Geophysical Union (AGU)
Cited by
38 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献