dc.contributor.author
Petereit, Johannes
dc.contributor.author
Saynisch-Wagner, Jan
dc.contributor.author
Morschhauser, Achim
dc.contributor.author
Pick, Leonie
dc.contributor.author
Thomas, Maik
dc.date.accessioned
2022-05-20T08:29:39Z
dc.date.available
2022-05-20T08:29:39Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/35092
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-34809
dc.description.abstract
Periodic tidal ocean currents induce electric currents and, therefore, magnetic field signals that are observable using spaceborne and ground-based observation techniques. In theory, the signals can be used to monitor oceanic temperature and salinity variations. Tidal magnetic field amplitudes and phases have been extracted from magnetometer measurements in the past. However, due to uncertainties caused by a plentitude of influencing factors, the shape and temporal variation of these signals are only known to a limited extent. This study uses past extraction methods to characterize seasonal variations and long-term trends in the ten year magnetometer time series of three coastal island observatories. First, we assess data processing procedures used to prepare ground-based magnetometer observations for tidal ocean dynamo signal extraction to demonstrate that existing approaches, i.e., subtraction of core field models or first-order differencing, are unable to reliably remove low-frequency contributions. We hence propose low-frequency filtering using smoothing splines and demonstrate the advantages over the existing approaches. Second, we determine signal and side peak magnitudes of the M2 tide induced magnetic field signal by spectral analysis of the processed data. We find evidence for seasonal magnetic field signal variations of up to 25% from the annual mean. Third, to characterize the long-term behavior of tidal ocean dynamo signal amplitudes and phases, we apply different signal extraction techniques to identify tidal ocean-dynamo signal amplitudes and phases in sub-series of the ten-year time series with incrementally increasing lengths. The analyses support three main findings: (1) trends cause signal amplitude changes of up to ≈1 nT and phase changes are in the order of O(10∘) within the observation period; (2) at least four years of data are needed to obtain reliable amplitude and phase values with the extraction methods used and (3) signal phases are a less dependent on the chosen extraction method than signal amplitudes.
en
dc.format.extent
16 Seiten
dc.rights.uri
https://creativecommons.org/licenses/by/4.0/
dc.subject
Ocean-tide induced magnetic fields
en
dc.subject
Tidal ocean dynamo
en
dc.subject
Signal extraction
en
dc.subject
Magnetometer Observations
en
dc.subject
Data Processing
en
dc.subject.ddc
500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::550 Geowissenschaften
dc.title
On the characterization of tidal ocean-dynamo signals in coastal magnetic observatories
dc.type
Wissenschaftlicher Artikel
dcterms.bibliographicCitation.articlenumber
67
dcterms.bibliographicCitation.doi
10.1186/s40623-022-01610-9
dcterms.bibliographicCitation.journaltitle
Earth, Planets and Space
dcterms.bibliographicCitation.number
1
dcterms.bibliographicCitation.volume
74
dcterms.bibliographicCitation.url
https://doi.org/10.1186/s40623-022-01610-9
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Institut für Meteorologie
refubium.resourceType.isindependentpub
no
dcterms.accessRights.openaire
open access
dcterms.isPartOf.eissn
1880-5981
refubium.resourceType.provider
WoS-Alert