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dc.contributor.author
Zenhäusern, Géraldine
dc.contributor.author
Kuvshinov, Alexey
dc.contributor.author
Guzavina, Martina
dc.contributor.author
Maute, Astrid
dc.date.accessioned
2021-07-05T15:19:04Z
dc.date.available
2021-07-04T03:19:34Z
dc.date.available
2021-07-05T15:19:04Z
dc.date.issued
2021
dc.identifier.issn
1343-8832
dc.identifier.issn
1880-5981
dc.identifier.other
10.1186/s40623-021-01455-8
en_US
dc.identifier.uri
http://hdl.handle.net/20.500.11850/492892
dc.identifier.doi
10.3929/ethz-b-000492892
dc.description.abstract
The electromagnetic (EM) field variations capable of probing the electrical conductivity of the upper mantle and mantle transition zone have a period range between a few hours and 1 day. At these periods, the dominant source of the EM signals is the ionospheric current system, which has a complex spatial and temporal structure. A concept of global-to-local (G2L) transfer functions can handle spatially complex source by relating global source expansion coefficients with locally measured magnetic (or/and electric) fields. When estimating the G2L transfer functions, the source is commonly expanded into spherical harmonics (SH). In this paper, we explore an alternative parametrization of the source based on a principal component analysis (PCA) of the Fourier transformed output from the physics-based Thermosphere Ionosphere Electrodynamics General Circulation Model (TIE-GCM). Specifically, we investigate whether magnetic fields computed in the realistic three-dimensional conductivity model of Earth excited by the PCA-based source agree better with observatory data than those computed in the same model but induced by the SH-based source. Using PCA to capture the source current compared to SH parametrization, we find that agreement with the observatory data is better during magnetically disturbed times and at shorter periods. Vice versa, it is poorer during magnetically quiet times and at longer periods.
en_US
dc.format
application/pdf
en_US
dc.language.iso
en
en_US
dc.publisher
Springer
en_US
dc.rights.uri
http://creativecommons.org/licenses/by/4.0/
dc.subject
Electromagnetic induction
en_US
dc.subject
Ionospheric current systems
en_US
dc.subject
Magnetic field variations
en_US
dc.subject
Principal component analysis
en_US
dc.title
Towards probing Earth’s upper mantle with daily magnetic field variations: exploring a physics-based parametrization of the source
en_US
dc.type
Journal Article
dc.rights.license
Creative Commons Attribution 4.0 International
dc.date.published
2021-06-25
ethz.journal.title
Earth, Planets and Space
ethz.journal.volume
73
en_US
ethz.journal.issue
1
en_US
ethz.journal.abbreviated
Earth Planets Space
ethz.pages.start
136
en_US
ethz.size
16 p.
en_US
ethz.version.deposit
publishedVersion
en_US
ethz.identifier.wos
ethz.identifier.scopus
ethz.publication.place
Heidelberg
en_US
ethz.publication.status
published
en_US
ethz.leitzahl
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02330 - Dep. Erdwissenschaften / Dep. of Earth Sciences::02506 - Institut für Geophysik / Institute of Geophysics::03476 - Giardini, Domenico / Giardini, Domenico
ethz.leitzahl
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02330 - Dep. Erdwissenschaften / Dep. of Earth Sciences::02506 - Institut für Geophysik / Institute of Geophysics::03734 - Jackson, Andrew / Jackson, Andrew
ethz.leitzahl.certified
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02330 - Dep. Erdwissenschaften / Dep. of Earth Sciences::02506 - Institut für Geophysik / Institute of Geophysics::03476 - Giardini, Domenico / Giardini, Domenico
ethz.leitzahl.certified
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02330 - Dep. Erdwissenschaften / Dep. of Earth Sciences::02506 - Institut für Geophysik / Institute of Geophysics::03734 - Jackson, Andrew / Jackson, Andrew
ethz.date.deposited
2021-07-04T03:19:45Z
ethz.source
SCOPUS
ethz.eth
yes
en_US
ethz.availability
Open access
en_US
ethz.rosetta.installDate
2021-07-05T15:19:11Z
ethz.rosetta.lastUpdated
2024-02-02T14:15:52Z
ethz.rosetta.versionExported
true
ethz.COinS
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