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Investigating Correlations Between Day-to-Day Variability in Pre-Reversal Enhancement in Equatorial Electron Drifts and Neutral Winds

Fatima
Yousuf
UC Berkeley Space Sciences Laboratory
Abstract text

The pre-reversal enhancement (PRE) of the equatorial zonal electric field arises from the F-layer neutral wind dynamo and is a driver of equatorial spread-F. Yet, the drivers of the PRE's day-to-day variability remain uncertain. We investigate the altitude- and local-time-dependent sensitivity of the daily variability of the PRE to neutral wind perturbations using observations from the Ionospheric Connection Explorer (ICON) and simulations with WACCM-X. We present correlation studies to identify local times and altitudes of neutral winds that may drive day-to-day variability in PRE. ICON orbits separated by 24 ± 0.25 hours are paired to minimize longitudinal effects and to isolate short-term changes in PRE strength and neutral winds. WACCM-X simulations reveal alternating-sign correlations between PRE variability and E-region zonal neutral winds, with positive correlations near ~90–110 km, negative correlations near ~120–150 km, and weakly positive correlations above ~180 km, most pronounced near sunset. Observations exhibit a similar but weaker structure. In contrast, F-region winds above ~150 km show predominantly weakly positive correlations in WACCM-X and limited coherence in observations.

Authors
Brian Harding, UC Berkeley Space Sciences Laboratory
Claire Gasque, UC Berkeley Space Sciences Laboratory
Colin Triplett, UC Berkeley Space Sciences Laboratory
Thomas Immel, UC Berkeley Space Sciences Laboratory
Yen‐Jung Joanne Wu, UC Berkeley Space Sciences Laboratory
Gilda Gonzalez, UC Berkeley Space Sciences Laboratory
Student in poster competition
Poster category
EQIT - Equatorial Ionosphere or Thermosphere
Poster number
6