Logo image
TRACERS Small‐Scale Field‐Aligned Currents and Intense GPS Amplitude and Phase Scintillations in the Nightside Auroral Region
Journal article   Open access   Peer reviewed

TRACERS Small‐Scale Field‐Aligned Currents and Intense GPS Amplitude and Phase Scintillations in the Nightside Auroral Region

Yangyang Shen, Robert J Strangeway, Hao Cao, James M Weygand, Jiashu Wu, Anthony McCaffrey, P. T Jayachandran, Daniel Billett, Magnus F Ivarsen, Christopher Watson, …
Geophysical research letters, Vol.53(14), e2026GL123732
07/28/2026
DOI: 10.1029/2026GL123732
url
https://doi.org/10.1029/2026GL123732View
Published (Version of record) Open Access

Abstract

We present conjugate observations of ionospheric small‐scale magnetic perturbations (dB)$(dB)$and GPS scintillations from the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) and the Canadian High Arctic Ionospheric Network (CHAIN) during a storm‐time substorm on 9 August 2025 in the nightside auroral region. Rotational transverse dB$dB$of up to ∼1,000 nT, associated with filamentary field‐aligned currents (FACs) exceeding 150 μA/m2${\upmu }\mathrm{A}/{\mathrm{m}}^{2}$on spatial scales of ∼1–16 km, were colocated with extreme, localized auroral scintillations (σϕ>${\sigma }_{\phi } > $10 rad, S4≃${S}_{4}\simeq $0.3) and ∼10 dB‐Hz intensity reduction. The most intense scintillations lasted ∼1.5 s and coincided with peaks in auroral electrojets, Pi2 pulsations, and enhanced dTEC (∼12 TECU). The sheet‐like morphology and spatiotemporal correlation with auroral electrojets suggest that Farley–Buneman processes likely play a dominant role in scintillation formation, with additional contributions from FAC‐driven and gradient‐drift instabilities.
Global Positioning Systems Ionosphere Orbits Precipitation Auroral electrojet Auroral electrojets Electrodynamics Electrojets GPS Magnetic fields Plasma Receivers & amplifiers Satellites Spacecraft Storms Tracers

Details

Metrics

1 Record Views
Logo image