Abstract
Global observations of the auroral x‐ray emissions during three large magnetic storms in 1998 are presented from the Polar Ionospheric X‐ray Imaging Experiment (PIXIE). The cross‐polar‐cap potential drop (ΔΦPC) remained large (>100 kV) throughout most of the stormtime periods, and most of the x‐ray emissions observed were associated with enhanced earthward convection and dawnward drift of electrons caused by substantial cross‐tail electric fields. Large increases in ΔΦPC drove impulsive disturbances termed convection enhancements that showed signatures inconsistent with substorm activity, including substantial auroral emissions in the morning sector and little activity in the premidnight sector.
Published Version (
Free)
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.