GCRAS candidate field models for IGRF-14 | Research Square window.SnipcartSettings = { analytics: { enabled: false } }; (function() { var accessVector = localStorage.getItem('access_vector') || ''; window.dataLayer = window.dataLayer || []; if (accessVector) { window.dataLayer.push({ user: { profile: { profileInfo: { snid: accessVector } } } }); } })(); (function(w,d,s,l,i){w[l]=w[l]||[];w[l].push({'gtm.start':new Date().getTime(),event:'gtm.js'});var f=d.getElementsByTagName(s)[0],j=d.createElement(s),dl=l!='dataLayer'?'&l='+l:'';j.async=true;j.src='https://www.googletagmanager.com/gtm.js?id='+i+dl;f.parentNode.insertBefore(j,f);})(window,document,'script','dataLayer','GTM-K279D39R'); Browse Preprints In Review Journals COVID-19 Preprints AJE Video Bytes Research Tools Research Promotion AJE Professional Editing AJE Rubriq About Preprint Platform In Review Editorial Policies Our Team Advisory Board Help Center Sign In Submit a Preprint Cite Share Download PDF Research Article GCRAS candidate field models for IGRF-14 Ilya Firsov, Dmitry Kudin, Anatoly Soloviev, Roman Krasnoperov, and 1 more This is a preprint; it has not been peer reviewed by a journal. https://doi.org/ 10.21203/rs.3.rs-6966906/v1 This work is licensed under a CC BY 4.0 License Status: Published Journal Publication published 05 Dec, 2025 Read the published version in Earth, Planets and Space → Version 1 posted 4 You are reading this latest preprint version Abstract We present candidate models for the 14th generation of the International Geomagnetic Reference Field (IGRF-14), specifically the Definitive Geomagnetic Reference Field (DGRF) for epoch 2020.0 and the IGRF for epoch 2025.0. These models were developed using high-quality magnetic measurements from the European Space Agency's Swarm satellite mission, including data from three low-Earth orbiting satellites equipped with Absolute Scalar Magnetometers and Vector Field Magnetometers. These models are part of the CAMPUS project, which is devoted to the construction of a series of Earth’s magnetic field models. Our methodology employs rigorous data selection criteria to minimize contamination from external sources and with strict scalar-vector consistency constraints. The internal magnetic field is parameterized using spherical harmonic functions up to degree 13, with coefficients determined through a two-stage inversion process involving linear inversion of vector measurements followed by nonlinear refinement including absolute scalar intensity data. For the DGRF 2020 model, we utilized data collected between January 2019 and December 2020, while the IGRF 2025 model incorporates measurements from January 2023 to September 2024. Comparison between the models indicates changes in field structure over the five-year interval, particularly in the South Atlantic Anomaly region. These candidate models effectively capture the main features of Earth's core-generated magnetic field and are consistent with long-term trends observed in previous IGRF generations, contributing to the collective scientific effort to maintain accurate descriptions of Earth's magnetic field. IGRF DGRF geomagnetism geomagnetic field modeling CAMPUS models CAMPUS-C Full Text Supplementary Files visualabstract.png Cite Share Download PDF Status: Published Journal Publication published 05 Dec, 2025 Read the published version in Earth, Planets and Space → Version 1 posted Reviewers agreed at journal 20 Jul, 2025 Reviewers invited by journal 18 Jul, 2025 Editor assigned by journal 17 Jul, 2025 First submitted to journal 09 Jul, 2025 You are reading this latest preprint version Research Square lets you share your work early, gain feedback from the community, and start making changes to your manuscript prior to peer review in a journal. As a division of Research Square Company, we’re committed to making research communication faster, fairer, and more useful. We do this by developing innovative software and high quality services for the global research community. Our growing team is made up of researchers and industry professionals working together to solve the most critical problems facing scientific publishing. Also discoverable on Platform About Our Team In Review Editorial Policies Advisory Board Help Center Resources Author Services Accessibility API Access RSS feed Manage Cookie Preferences © Research Square 2026 | ISSN 2693-5015 (online) Privacy Policy Terms of Service Do Not Sell My Personal Information {"props":{"pageProps":{"initialData":{"identity":"rs-6966906","acceptedTermsAndConditions":true,"allowDirectSubmit":false,"archivedVersions":[],"articleType":"Research Article","associatedPublications":[],"authors":[{"id":487505594,"identity":"2e1d126e-4329-44e7-bb87-94f9a6031704","order_by":0,"name":"Ilya Firsov","email":"data:image/png;base64,iVBORw0KGgoAAAANSUhEUgAAAZAAAAAyAQMAAABI0h/eAAAABlBMVEX///8AAABVwtN+AAAACXBIWXMAAA7EAAAOxAGVKw4bAAAA5klEQVRIiWNgGAWjYBAC9mYwJSHHz958AMhgJqyF5zCYsjCW7DmWQKSWA2CqInHDDR8DIrWw8z7+8LFNAqiF55vEzx3WcgYHeJ9J4NXCzG4mObNNwnjm7d5tkr1n0o0lG9jN8GqxZ2ZjY+Y5IyHbd+fsNgnetsOJ/QxsbARsYWP+DNTC2HAj55nk37bD9W1EaGGQ5qmQUJxwI4dNGmhLAj8RWtgkZ1RIgALZ2Fq2Ld1wZjMbswVeLfzHmD98MKgDReXDm2/brOUNjrcx3sCnBRmwQNxDRNTAAfMHEhSPglEwCkbBCAIAHnA/ubKQe4MAAAAASUVORK5CYII=","orcid":"https://orcid.org/0000-0002-7283-9679","institution":"Geophysical Center of the Russian Academy of Sciences","correspondingAuthor":true,"prefix":"","firstName":"Ilya","middleName":"","lastName":"Firsov","suffix":""},{"id":487505595,"identity":"07214452-ea3f-4d01-866a-53c72a8e7ac4","order_by":1,"name":"Dmitry Kudin","email":"","orcid":"","institution":"GCRAS","correspondingAuthor":false,"prefix":"","firstName":"Dmitry","middleName":"","lastName":"Kudin","suffix":""},{"id":487505596,"identity":"a372f5bb-8991-44f0-aea6-8080ec705402","order_by":2,"name":"Anatoly Soloviev","email":"","orcid":"","institution":"GCRAS","correspondingAuthor":false,"prefix":"","firstName":"Anatoly","middleName":"","lastName":"Soloviev","suffix":""},{"id":487505597,"identity":"f3a20f2b-1055-4c47-924d-677b5dd51517","order_by":3,"name":"Roman Krasnoperov","email":"","orcid":"","institution":"GCRAS","correspondingAuthor":false,"prefix":"","firstName":"Roman","middleName":"","lastName":"Krasnoperov","suffix":""},{"id":487505598,"identity":"f7cc51e0-d4d0-4c70-ab90-a2e2a1288839","order_by":4,"name":"Mikhail Dobrovolsky","email":"","orcid":"","institution":"GCRAS","correspondingAuthor":false,"prefix":"","firstName":"Mikhail","middleName":"","lastName":"Dobrovolsky","suffix":""}],"badges":[],"createdAt":"2025-06-24 14:42:01","currentVersionCode":1,"declarations":"","doi":"10.21203/rs.3.rs-6966906/v1","doiUrl":"https://doi.org/10.21203/rs.3.rs-6966906/v1","draftVersion":[],"editorialEvents":[{"content":"https://doi.org/10.1186/s40623-025-02318-2","type":"published","date":"2025-12-05T15:57:42+00:00"}],"editorialNote":"","failedWorkflow":false,"files":[{"id":97724568,"identity":"4164bdbf-9f8c-472e-a910-4a5cef4eaee2","added_by":"auto","created_at":"2025-12-08 16:12:38","extension":"pdf","order_by":1,"title":"","display":"","copyAsset":false,"role":"manuscript-pdf","size":1536996,"visible":true,"origin":"","legend":"","description":"","filename":"IGRFcandidate5.pdf","url":"https://assets-eu.researchsquare.com/files/rs-6966906/v1_covered_e1f1c629-2250-4e9b-83fb-b803c01e3ab2.pdf"},{"id":87255214,"identity":"80eed4f3-4049-4204-9844-f61646532ff5","added_by":"auto","created_at":"2025-07-22 05:45:31","extension":"png","order_by":10,"title":"","display":"","copyAsset":false,"role":"supplement","size":122914,"visible":true,"origin":"","legend":"","description":"","filename":"visualabstract.png","url":"https://assets-eu.researchsquare.com/files/rs-6966906/v1/db2d9d7771810b927cc7909d.png"}],"financialInterests":"","formattedTitle":"GCRAS candidate field models for IGRF-14","fulltext":[],"fulltextSource":"","fullText":"","funders":[],"hasAdminPriorityOnWorkflow":false,"hasManuscriptDocX":false,"hasOptedInToPreprint":true,"hasPassedJournalQc":"","hasAnyPriority":false,"hideJournal":false,"highlight":"","institution":"","isAcceptedByJournal":true,"isAuthorSuppliedPdf":true,"isDeskRejected":"","isHiddenFromSearch":false,"isInQc":false,"isInWorkflow":true,"isPdf":true,"isPdfUpToDate":true,"isWithdrawnOrRetracted":false,"journal":{"display":true,"email":"
[email protected]","identity":"earth-planets-and-space","isNatureJournal":false,"hasQc":true,"allowDirectSubmit":false,"externalIdentity":"epsp","sideBox":"Learn more about [Earth, Planets and Space](http://earth-planets-space.springeropen.com)","snPcode":"","submissionUrl":"https://www.editorialmanager.com/epsp/default.aspx","title":"Earth, Planets and Space","twitterHandle":"@SpringerOpen","acdcEnabled":true,"dfaEnabled":true,"editorialSystem":"em","reportingPortfolio":"BMC/SO AJ","inReviewEnabled":true,"inReviewRevisionsEnabled":true},"keywords":"IGRF, DGRF, geomagnetism, geomagnetic field modeling, CAMPUS models, CAMPUS-C","lastPublishedDoi":"10.21203/rs.3.rs-6966906/v1","lastPublishedDoiUrl":"https://doi.org/10.21203/rs.3.rs-6966906/v1","license":{"name":"CC BY 4.0","url":"https://creativecommons.org/licenses/by/4.0/"},"manuscriptAbstract":"We present candidate models for the 14th generation of the International Geomagnetic Reference Field (IGRF-14), specifically the Definitive Geomagnetic Reference Field (DGRF) for epoch 2020.0 and the IGRF for epoch 2025.0. These models were developed using high-quality magnetic measurements from the European Space Agency's Swarm satellite mission, including data from three low-Earth orbiting satellites equipped with Absolute Scalar Magnetometers and Vector Field Magnetometers. These models are part of the CAMPUS project, which is devoted to the construction of a series of Earth’s magnetic field models. Our methodology employs rigorous data selection criteria to minimize contamination from external sources and with strict scalar-vector consistency constraints. The internal magnetic field is parameterized using spherical harmonic functions up to degree 13, with coefficients determined through a two-stage inversion process involving linear inversion of vector measurements followed by nonlinear refinement including absolute scalar intensity data. For the DGRF 2020 model, we utilized data collected between January 2019 and December 2020, while the IGRF 2025 model incorporates measurements from January 2023 to September 2024. Comparison between the models indicates changes in field structure over the five-year interval, particularly in the South Atlantic Anomaly region. These candidate models effectively capture the main features of Earth's core-generated magnetic field and are consistent with long-term trends observed in previous IGRF generations, contributing to the collective scientific effort to maintain accurate descriptions of Earth's magnetic field.","manuscriptTitle":"GCRAS candidate field models for IGRF-14","msid":"","msnumber":"","nonDraftVersions":[{"code":1,"date":"2025-07-22 05:29:26","doi":"10.21203/rs.3.rs-6966906/v1","editorialEvents":[{"type":"communityComments","content":0},{"type":"reviewerAgreed","content":"","date":"2025-07-20T13:19:07+00:00","index":0,"fulltext":""},{"type":"reviewersInvited","content":"","date":"2025-07-18T14:25:30+00:00","index":"","fulltext":""},{"type":"editorAssigned","content":"","date":"2025-07-17T10:42:12+00:00","index":"","fulltext":""},{"type":"submitted","content":"Earth, Planets and Space","date":"2025-07-09T11:47:45+00:00","index":"","fulltext":""}],"status":"published","journal":{"display":true,"email":"
[email protected]","identity":"earth-planets-and-space","isNatureJournal":false,"hasQc":true,"allowDirectSubmit":false,"externalIdentity":"epsp","sideBox":"Learn more about [Earth, Planets and Space](http://earth-planets-space.springeropen.com)","snPcode":"","submissionUrl":"https://www.editorialmanager.com/epsp/default.aspx","title":"Earth, Planets and Space","twitterHandle":"@SpringerOpen","acdcEnabled":true,"dfaEnabled":true,"editorialSystem":"em","reportingPortfolio":"BMC/SO AJ","inReviewEnabled":true,"inReviewRevisionsEnabled":true}}],"origin":"","ownerIdentity":"2ef75aa4-3cbf-4a09-97e6-ba79d2b2db0e","owner":[],"postedDate":"July 22nd, 2025","published":true,"recentEditorialEvents":[],"rejectedJournal":[],"revision":"","amendment":"","status":"published-in-journal","subjectAreas":[],"tags":[],"updatedAt":"2025-12-08T16:08:30+00:00","versionOfRecord":{"articleIdentity":"rs-6966906","link":"https://doi.org/10.1186/s40623-025-02318-2","journal":{"identity":"earth-planets-and-space","isVorOnly":false,"title":"Earth, Planets and Space"},"publishedOn":"2025-12-05 15:57:42","publishedOnDateReadable":"December 5th, 2025"},"versionCreatedAt":"2025-07-22 05:29:26","video":"","vorDoi":"10.1186/s40623-025-02318-2","vorDoiUrl":"https://doi.org/10.1186/s40623-025-02318-2","workflowStages":[]},"version":"v1","identity":"rs-6966906","journalConfig":"researchsquare"},"__N_SSP":true},"page":"/article/[identity]/[[...version]]","query":{"redirect":"/article/rs-6966906","identity":"rs-6966906","version":["v1"]},"buildId":"8U1c8b4HqxoKbykW_rLl7","isFallback":false,"isExperimentalCompile":false,"dynamicIds":[84888],"gssp":true,"scriptLoader":[]}
Text is read by the "Ask this paper" AI Q&A widget below.
Extraction quality varies by source — PMC NXML preserves structure
cleanly, OA-HTML may include some navigation residue, and OA-PDF can
have broken hyphenation. The publisher copy
(via DOI)
is the canonical version.