Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF Waves

Abstract The weakly ionized plasma in the Earth's ionosphere is controlled by a complex interplay between solar and magnetospheric inputs from above, atmospheric processes from below, and plasma electrodynamics from within. This interaction results in ionosphere structuring and variability that...

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Main Authors: Yangyang Shen, Olga P. Verkhoglyadova, Anton Artemyev, Michael D. Hartinger, Vassilis Angelopoulos, Xueling Shi, Ying Zou
Format: Article
Language:English
Published: Wiley 2024-12-01
Series:AGU Advances
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Online Access:https://doi.org/10.1029/2024AV001302
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author Yangyang Shen
Olga P. Verkhoglyadova
Anton Artemyev
Michael D. Hartinger
Vassilis Angelopoulos
Xueling Shi
Ying Zou
author_facet Yangyang Shen
Olga P. Verkhoglyadova
Anton Artemyev
Michael D. Hartinger
Vassilis Angelopoulos
Xueling Shi
Ying Zou
author_sort Yangyang Shen
collection DOAJ
description Abstract The weakly ionized plasma in the Earth's ionosphere is controlled by a complex interplay between solar and magnetospheric inputs from above, atmospheric processes from below, and plasma electrodynamics from within. This interaction results in ionosphere structuring and variability that pose major challenges for accurate ionosphere prediction for global navigation satellite system (GNSS) related applications and space weather research. The ionospheric structuring and variability are often probed using the total electron content (TEC) and its relative perturbations (dTEC). Among dTEC variations observed at high latitudes, a unique modulation pattern has been linked to magnetospheric ultra‐low‐frequency (ULF) waves, yet its underlying mechanisms remain unclear. Here using magnetically conjugate observations from the THEMIS spacecraft and a ground‐based GPS receiver at Fairbanks, Alaska, we provide direct evidence that these dTEC modulations are driven by magnetospheric electron precipitation induced by ULF‐modulated whistler‐mode waves. We observed peak‐to‐peak dTEC amplitudes reaching ∼ 0.5 TECU (1 TECU is equal to 106 electrons/m2) with modulations spanning scales of ∼ 5–100 km. The cross‐correlation between our modeled and observed dTEC reached ∼ 0.8 during the conjugacy period but decreased outside of it. The spectra of whistler‐mode waves and dTEC also matched closely at ULF frequencies during the conjugacy period but diverged outside of it. Our findings elucidate the high‐latitude dTEC generation from magnetospheric wave‐induced precipitation, addressing a significant gap in current physics‐based dTEC modeling. Theses results thus improve ionospheric dTEC prediction and enhance our understanding of magnetosphere‐ionosphere coupling via ULF waves.
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spelling doaj-art-54b8b7b68d524b15abb67e6b59355fa22024-12-24T08:34:27ZengWileyAGU Advances2576-604X2024-12-0156n/an/a10.1029/2024AV001302Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF WavesYangyang Shen0Olga P. Verkhoglyadova1Anton Artemyev2Michael D. Hartinger3Vassilis Angelopoulos4Xueling Shi5Ying Zou6Department of Earth, Planetary, and Space Sciences University of California Los Angeles CA USAJet Propulsion Laboratory California Institute of Technology Pasadena CA USADepartment of Earth, Planetary, and Space Sciences University of California Los Angeles CA USADepartment of Earth, Planetary, and Space Sciences University of California Los Angeles CA USADepartment of Earth, Planetary, and Space Sciences University of California Los Angeles CA USADepartment of Electrical and Computer Engineering Virginia Tech Blacksburg VA USAJohns Hopkins University Applied Physics Laboratory Laurel MD USAAbstract The weakly ionized plasma in the Earth's ionosphere is controlled by a complex interplay between solar and magnetospheric inputs from above, atmospheric processes from below, and plasma electrodynamics from within. This interaction results in ionosphere structuring and variability that pose major challenges for accurate ionosphere prediction for global navigation satellite system (GNSS) related applications and space weather research. The ionospheric structuring and variability are often probed using the total electron content (TEC) and its relative perturbations (dTEC). Among dTEC variations observed at high latitudes, a unique modulation pattern has been linked to magnetospheric ultra‐low‐frequency (ULF) waves, yet its underlying mechanisms remain unclear. Here using magnetically conjugate observations from the THEMIS spacecraft and a ground‐based GPS receiver at Fairbanks, Alaska, we provide direct evidence that these dTEC modulations are driven by magnetospheric electron precipitation induced by ULF‐modulated whistler‐mode waves. We observed peak‐to‐peak dTEC amplitudes reaching ∼ 0.5 TECU (1 TECU is equal to 106 electrons/m2) with modulations spanning scales of ∼ 5–100 km. The cross‐correlation between our modeled and observed dTEC reached ∼ 0.8 during the conjugacy period but decreased outside of it. The spectra of whistler‐mode waves and dTEC also matched closely at ULF frequencies during the conjugacy period but diverged outside of it. Our findings elucidate the high‐latitude dTEC generation from magnetospheric wave‐induced precipitation, addressing a significant gap in current physics‐based dTEC modeling. Theses results thus improve ionospheric dTEC prediction and enhance our understanding of magnetosphere‐ionosphere coupling via ULF waves.https://doi.org/10.1029/2024AV001302total electron contentwhistler‐mode wavesmagnetosphere ionosphere couplingparticle precipitationionosphere irregularitiesionosphere scintillation
spellingShingle Yangyang Shen
Olga P. Verkhoglyadova
Anton Artemyev
Michael D. Hartinger
Vassilis Angelopoulos
Xueling Shi
Ying Zou
Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF Waves
AGU Advances
total electron content
whistler‐mode waves
magnetosphere ionosphere coupling
particle precipitation
ionosphere irregularities
ionosphere scintillation
title Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF Waves
title_full Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF Waves
title_fullStr Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF Waves
title_full_unstemmed Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF Waves
title_short Magnetospheric Control of Ionospheric TEC Perturbations via Whistler‐Mode and ULF Waves
title_sort magnetospheric control of ionospheric tec perturbations via whistler mode and ulf waves
topic total electron content
whistler‐mode waves
magnetosphere ionosphere coupling
particle precipitation
ionosphere irregularities
ionosphere scintillation
url https://doi.org/10.1029/2024AV001302
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