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Saturnino, Diana, Langlais, Benoit, Civet, François, Thébault, Erwan, Mandea, Mioara (2015) Main field and secular variation candidate models for the 12th IGRF generation after 10 months of Swarm measurements. Earth, Planets and Space, 67 (1) doi:10.1186/s40623-015-0262-7

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Reference TypeJournal (article/letter/editorial)
TitleMain field and secular variation candidate models for the 12th IGRF generation after 10 months of Swarm measurements
JournalEarth, Planets and Space
AuthorsSaturnino, DianaAuthor
Langlais, BenoitAuthor
Civet, FrançoisAuthor
Thébault, ErwanAuthor
Mandea, MioaraAuthor
Year2015 (December)Volume67
Issue1
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1186/s40623-015-0262-7Search in ResearchGate
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Mindat Ref. ID543170Long-form Identifiermindat:1:5:543170:4
GUID0
Full ReferenceSaturnino, Diana, Langlais, Benoit, Civet, François, Thébault, Erwan, Mandea, Mioara (2015) Main field and secular variation candidate models for the 12th IGRF generation after 10 months of Swarm measurements. Earth, Planets and Space, 67 (1) doi:10.1186/s40623-015-0262-7
Plain TextSaturnino, Diana, Langlais, Benoit, Civet, François, Thébault, Erwan, Mandea, Mioara (2015) Main field and secular variation candidate models for the 12th IGRF generation after 10 months of Swarm measurements. Earth, Planets and Space, 67 (1) doi:10.1186/s40623-015-0262-7
In(2015, December) Earth, Planets and Space Vol. 67 (1) Springer Science and Business Media LLC

See Also

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Langlais, Benoit, Mandea, Mioara (2000) An IGRF candidate main geomagnetic field model for epoch 2000 and a secular variation model for 2000–2005. Earth, Planets and Space, 52 (12) 1137-1148 doi:10.1186/bf03352344
Fournier, Alexandre, Aubert, Julien, Thébault, Erwan (2015) A candidate secular variation model for IGRF-12 based on Swarm data and inverse geodynamo modelling. Earth, Planets and Space, 67 (1) doi:10.1186/s40623-015-0245-8
Wardinski, I., Saturnino, D., Amit, H., Chambodut, A., Langlais, B., Mandea, M., Thébault, E. (2020) Geomagnetic core field models and secular variation forecasts for the 13th International Geomagnetic Reference Field (IGRF-13). Earth, Planets and Space, 72 (1). doi:10.1186/s40623-020-01254-7
Mandea, Mioara, Langlais, Benoit (2000) Use of Ørsted scalar data in evaluating the pre-Ørsted main field candidate models for the IGRF 2000. Earth, Planets and Space, 52 (12) 1167-1170 doi:10.1186/bf03352347
Mandea, Mioara (2005) Candidate main-field models for producing the 9th generation IGRF. Earth, Planets and Space, 57 (12) 1183-1189 doi:10.1186/bf03351902
Fournier, Alexandre, Aubert, Julien, Lesur, Vincent, Thébault, Erwan (2021) Physics-based secular variation candidate models for the IGRF. Earth, Planets and Space, 73 (1) doi:10.1186/s40623-021-01507-z
Thébault, Erwan, Finlay, Christopher C., Alken, Patrick, Beggan, Ciaran D., Canet, Elisabeth, Chulliat, Arnaud, Langlais, Benoit, Lesur, Vincent, Lowes, Frank J., Manoj, Chandrasekharan, Rother, Martin, Schachtschneider, Reyko (2015) Evaluation of candidate geomagnetic field models for IGRF-12. Earth, Planets and Space, 67 (1) doi:10.1186/s40623-015-0273-4
Hamilton, Brian, Ridley, Victoria A, Beggan, Ciarán D, Macmillan, Susan (2015) The BGS magnetic field candidate models for the 12th generation IGRF. Earth, Planets and Space, 67 (1) doi:10.1186/s40623-015-0227-x
Saturnino, Diana, Langlais, Benoit, Amit, Hagay, Civet, François, Mandea, Mioara, Beucler, Éric (2018) Combining virtual observatory and equivalent source dipole approaches to describe the geomagnetic field with Swarm measurements. Physics of the Earth and Planetary Interiors, 276. 118-133 doi:10.1016/j.pepi.2017.06.004
Thébault, Erwan, Vigneron, Pierre, Langlais, Benoit, Hulot, Gauthier (2016) A Swarm lithospheric magnetic field model to SH degree 80. Earth, Planets and Space, 68 (1) doi:10.1186/s40623-016-0510-5
Chambodut, Aude, Langlais, Benoit, Menvielle, Michel, Thébault, Erwan, Chulliat, Arnaud, Hulot, Gauthier (2010) Candidate models for the IGRF-11th generation making use of extrapolated observatory data. Earth, Planets and Space, 62 (10) 745-751 doi:10.5047/eps.2010.06.006
 
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