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Imaging the May 2024 Extreme Aurora with Ionospheric Total Electron Content
  • +5
  • J C Foster,
  • P J Erickson,
  • Y Nishimura,
  • S R Zhang,
  • D C Bush,
  • A J Coster,
  • P E Meade,
  • E Franco-Diaz
J C Foster
Haystack Observatory, Massachusetts Institute of Technology

Corresponding Author:[email protected]

Author Profile
P J Erickson
Haystack Observatory, Massachusetts Institute of Technology
Y Nishimura
Department of Electrical and Computer Engineering and Center for Space Physics, Boston University
S R Zhang
Haystack Observatory, Massachusetts Institute of Technology
D C Bush
Missouri Skies Observatory
A J Coster
Haystack Observatory, Massachusetts Institute of Technology
P E Meade
Computational Physics Inc
E Franco-Diaz
Computational Physics Inc

Abstract

TEC maps show the intensification and spread of the 11 May 2024 extreme auroral event across the continental US over a 20-minute interval. All sky camera imagery indicates that the TEC enhancement closely matches the westward and equatorward expansion of strong red aurora. Coincident with auroral breakup, individual receiver/satellite data sets show sharp bursts of greatly elevated TEC 50 TECu above background.
01 Oct 2024Submitted to ESS Open Archive
04 Oct 2024Published in ESS Open Archive