NOAA/NCEI and University of Colorado candidate models for IGRF-13

Author:

Alken P.ORCID,Chulliat A.,Nair M.

Abstract

AbstractThe International Geomagnetic Reference Field (IGRF) is a set of parameters representing the large-scale internal part of Earth’s magnetic field. The 13th generation IGRF requested candidate models for a definitive main field for 2015.0, a provisional main field for 2020.0, and a predictive secular variation covering the period 2020.0–2025.0. The University of Colorado (CU) and the National Centers for Environmental Information (NCEI), part of the National Oceanic and Atmospheric Administration (NOAA), have produced these three candidate models for consideration in IGRF-13. In this paper, we present the methodology used to derive our candidate models. Our candidates were built primarily from Swarm satellite data, and also relied on geomagnetic indices derived from the ground observatory network. The ground observatories played a crucial role as independent data in validating our candidates. This paper also provides a retrospective assessment of the CU/NCEI candidate model to the previous IGRF (IGRF-12) and discusses the impact of differences between candidate and final IGRF models on global model errors.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Geology

Reference17 articles.

1. Alken P, Maus S, Chulliat A, Manoj C (2015) NOAA/NGDC candidate models for the 12th generation International Geomagnetic Reference Field. Earth Planets Space 67:68. https://doi.org/10.1186/s40623-015-0215-1

2. Alken P, Olsen N, Finlay CC (2020a) Co-estimation of geomagnetic field and in-orbit fluxgate magnetometer calibration parameters. Earth Planets Space 72:1–32. https://doi.org/10.1186/s40623-020-01163-9

3. Alken P, Thébault E, Beggan C, Aubert J, Baerenzung J, Brown W, Califf S, Chulliat A, Cox G, Finlay CC, Fournier A, Gillet N, Hammer MD, Holschneider M, Hulot G, Korte M, Lesur V, Livermore P, Lowes F, Macmillan S, Nair M, Olsen N, Ropp G, Rother M, Schnepf NR, Toh CSH, Vervelidou F, Vigneron P, Wardinski I (2020b) Evaluation of candidate models for the 13th International Geomagnetic Reference Field. Earth Planets Space. https://doi.org/10.21203/rs.3.rs-41022/v1

4. Alken P, Thébault E, Beggan CD, Amit H, Aubert J, Baerenzung J, Bondar TN, Brown W, Califf S, Chambodut A, Chulliat A, Cox G, Finlay CC, Fournier A, Gillet N, Grayver A, Hammer MD, Holschneider M, Huder L, Hulot G, Jager T, Kloss C, Korte M, Kuang W, Kuvshinov A, Langlais B, Léger JM, Lesur V, Livermore PW, Lowes FJ, Macmillan S, Mound JE, Nair M, Nakano S, Olsen N, Pavón-Carrasco FJ, Petrov VG, Ropp G, Rother M, Sabaka TJ, Sanchez S, Saturnino D, Schnepf NR, Shen X, Stolle C, Tangborn A, Tøffner-Clausen L, Toh H, Torta JM, Varner J, Vervelidou F, Vigneron P, Wardinski I, Wicht J, Woods A, Yang Y, Zeren Z, Zhou B (2020c) International Geomagnetic Reference Field: the thirteenth generation. Earth Planets Space. https://doi.org/10.1186/s40623-020-01288-x

5. Chulliat A, Alken P, Maus S (2015) Fast equatorial waves propagating at the top of the Earth’s core. Geophys Res Lett 42(9):3321–3329

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