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

Abstract We present conjugate observations of ionospheric small‐scale magnetic perturbations 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 of up to ∼1,000 nT, associated with filamentary field‐aligned currents (FACs) exceeding 150 on spatial scales of ∼1–16 km, were colocated with extreme, localized auroral scintillations ( 10 rad, 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.

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Publication Details

Journal
Geophysical Research Letters
Published
2026-07-18
DOI
https://doi.org/10.1029/2026gl123732
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

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

Magnus F. Ivarsen, P. T. Jayachandran, Yangyang Shen, S. Tian et al.
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
article

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

Magnus F. Ivarsen, P. T. Jayachandran, Yangyang Shen, S. Tian, M. Øieroset, J. Wu, Anthony M. McCaffrey, R. J. Strangeway, Hao Cao, David M. Miles, Chris Watson, Daniel Billett, James M. Weygand
article en

Abstract

Abstract We present conjugate observations of ionospheric small‐scale magnetic perturbations 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 of up to ∼1,000 nT, associated with filamentary field‐aligned currents (FACs) exceeding 150 on spatial scales of ∼1–16 km, were colocated with extreme, localized auroral scintillations ( 10 rad, 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.

Geophysical Research LettersVol. 53(14)
University of New Brunswick (CA), University of Iowa (US), Planetary Science Institute (US), University of Alberta (CA), University of California, Los Angeles (US), University of Saskatchewan (CA), University of California, Berkeley (US)
National Aeronautics and Space Administration, Natural Sciences and Engineering Research Council of Canada
Life below water
Openalex Percentile: Top 8%
Ionosphere and magnetosphere dynamics
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