Detecting low-latitude outer core-surface waves with 25 years of satellite secular variation data

Fluid motion in the Earth’s liquid outer core generates most of the geomagnetic field, and its time changes over timescales of one year or longer, the secular variation (SV). Data from the satellite missions Ørsted, CHAMP, CryoSat-2 and Swarm, together with data from ground observatories, were combined to yield a SV dataset spanning from late 1997 to early 2023. These SV data were inverted for time-varying core surface fluid velocity assuming it is purely advective, with the main field specified by the CHAOS-7.16 field model. The inversion was regularised both in time and in space. In time, the difference in velocity between individual epochs was minimised. In space, small-scale velocity structures were penalised. Flow acceleration was then calculated from first differences of velocities at successive epochs. Time-longitude diagrams of azimuthal acceleration show sloping features at low latitudes, interpreted as signatures of propagating waves. Waves propagating both eastwards and westwards were observed, with propagation velocities of approximately 1700 km/yr which is in agreement with previous inferences of fast core waves. Power spectral density plots reveal that the energy is concentrated in modes with periods of 6–7 years, and azimuthal wavenumbers −5, −2 and 2, where negative wave numbers indicate westward motion. There is a higher energy content in the westward propagating waves than in those travelling eastwards. Finally, we find intermittent low-latitude standing waves, which coincide with times of recent equatorial geomagnetic jerks, consistent with inferences of magneto-Coriolis and Alfvén waves from other studies. • Low latitude standing and propagating waves inferred from core surface flow acceleration • Waves travel west- and eastwards at periods of 6–7 years, with more energy westwards • Consistent with inferences of magneto-Coriolis and Alfvén waves from other studies • Acceleration changes coincide with times of geomagnetic jerks

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Publication Details

Journal
Physics of The Earth and Planetary Interiors
Published
2025-08-22
DOI
https://doi.org/10.1016/j.pepi.2025.107435
Citations
3
Primary Topic
Geochemistry and Geologic Mapping
Type
article
Field-Weighted Citation Impact
7.44
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article

Detecting low-latitude outer core-surface waves with 25 years of satellite secular variation data

3 citations
Physics of The Earth and Planetary Interiors
Geochemistry and Geologic Mapping
7.44
article

Detecting low-latitude outer core-surface waves with 25 years of satellite secular variation data

article en
3 citations

Abstract

Fluid motion in the Earth’s liquid outer core generates most of the geomagnetic field, and its time changes over timescales of one year or longer, the secular variation (SV). Data from the satellite missions Ørsted, CHAMP, CryoSat-2 and Swarm, together with data from ground observatories, were combined to yield a SV dataset spanning from late 1997 to early 2023. These SV data were inverted for time-varying core surface fluid velocity assuming it is purely advective, with the main field specified by the CHAOS-7.16 field model. The inversion was regularised both in time and in space. In time, the difference in velocity between individual epochs was minimised. In space, small-scale velocity structures were penalised. Flow acceleration was then calculated from first differences of velocities at successive epochs. Time-longitude diagrams of azimuthal acceleration show sloping features at low latitudes, interpreted as signatures of propagating waves. Waves propagating both eastwards and westwards were observed, with propagation velocities of approximately 1700 km/yr which is in agreement with previous inferences of fast core waves. Power spectral density plots reveal that the energy is concentrated in modes with periods of 6–7 years, and azimuthal wavenumbers −5, −2 and 2, where negative wave numbers indicate westward motion. There is a higher energy content in the westward propagating waves than in those travelling eastwards. Finally, we find intermittent low-latitude standing waves, which coincide with times of recent equatorial geomagnetic jerks, consistent with inferences of magneto-Coriolis and Alfvén waves from other studies. • Low latitude standing and propagating waves inferred from core surface flow acceleration • Waves travel west- and eastwards at periods of 6–7 years, with more energy westwards • Consistent with inferences of magneto-Coriolis and Alfvén waves from other studies • Acceleration changes coincide with times of geomagnetic jerks

Physics of The Earth and Planetary InteriorsVol. 367
British Geological Survey (GB), University of Edinburgh (GB)
Openalex Percentile: Top 3%
Geochemistry and Geologic Mapping
7.44
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