CM5, a pre-Swarm comprehensive geomagnetic field model derived from over 12 yr of CHAMP, Ørsted, SAC-C and observatory data

dc.contributor.authorSabaka, Terence J.
dc.contributor.authorOlsen, Nils
dc.contributor.authorTyler, Robert H.
dc.contributor.authorKuvshinov, Alexey
dc.date.accessioned2023-07-26T20:01:28Z
dc.date.available2023-07-26T20:01:28Z
dc.date.issued2015-02-04
dc.description.abstractA comprehensive magnetic field model named CM5 has been derived from CHAMP, Ørsted and SAC-C satellite and observatory hourly-means data from 2000 August to 2013 January using the Swarm Level-2 Comprehensive Inversion (CI) algorithm. Swarm is a recently launched constellation of three satellites to map the Earth's magnetic field. The CI technique includes several interesting features such as the bias mitigation scheme known as Selective Infinite Variance Weighting (SIVW), a new treatment for attitude error in satellite vector measurements, and the inclusion of 3-D conductivity for ionospheric induction. SIVW has allowed for a much improved lithospheric field recovery over CM4 by exploiting CHAMP along-track difference data yielding resolution levels up to spherical harmonic degree 107, and has allowed for the successful extraction of the oceanic M₂ tidal magnetic field from quiet, nightside data. The 3-D induction now captures anomalous Solar-quiet features in coastal observatory daily records. CM5 provides a satisfactory, continuous description of the major magnetic fields in the near-Earth region over this time span, and its lithospheric, ionospheric and oceanic M₂ tidal constituents may be used as validation tools for future Swarm Level-2 products coming from the CI algorithm and other dedicated product algorithms.en_US
dc.description.sponsorshipWe thank Vincent Lesur and an anonymous reviewer for valuable comments that improved the quality of the paper. The NASA Center for Climate Simulation at Goddard Space Flight Center provided computational resources. TJS and RHT are supported by the NASA Earth Surface and Interior program.en_US
dc.description.urihttps://academic.oup.com/gji/article/200/3/1596/633332en_US
dc.format.extent31 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2tup0-rinu
dc.identifier.citationTerence J. Sabaka and others, CM5, a pre-Swarm comprehensive geomagnetic field model derived from over 12 yr of CHAMP, Ørsted, SAC-C and observatory data, Geophysical Journal International, Volume 200, Issue 3, March 2015, Pages 1596–1626, https://doi.org/10.1093/gji/ggu493en_US
dc.identifier.urihttps://doi.org/10.1093/gji/ggu493
dc.identifier.urihttp://hdl.handle.net/11603/28863
dc.language.isoen_USen_US
dc.publisherOxford University Pressen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Joint Center for Earth Systems Technology
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleCM5, a pre-Swarm comprehensive geomagnetic field model derived from over 12 yr of CHAMP, Ørsted, SAC-C and observatory dataen_US
dc.typeTexten_US

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