International Geomagnetic Reference Field: the thirteenth generation

P. Alken; E. Thébault; C. D. Beggan; H. Amit; J. Aubert; J. Baerenzung; T. N. Bondar; W. J. Brown; S. Califf; A. Chambodut; A. Chulliat; G. A. Cox; C. C. Finlay; A. Fournier; N. Gillet; A. Grayver; M. D. Hammer; M. Holschneider; L. Huder; G. Hulot; T. Jager; C. Kloss; M. Korte; W. Kuang; A. Kuvshinov; B. Langlais; J. M. Léger; V. Lesur; P. W. Livermore; F. J. Lowes; S. Macmillan; W. Magnes; M. Mandea; S. Marsal; J. Matzka; M. C. Metman; T. Minami; A. Morschhauser; J. E. Mound; M. Nair; S. Nakano; N. Olsen; F. J. Pavón-Carrasco; V. G. Petrov; G. Ropp; M. Rother; T. J. Sabaka; S. Sanchez; D. Saturnino; N. R. Schnepf; X. Shen; C. Stolle; A. Tangborn; L. Tøffner-Clausen; H. Toh; J. M. Torta; J. Varner; F. Vervelidou; P. Vigneron; I. Wardinski; J. Wicht; A. Woods; Y. Yang; Z. Zeren; B. Zhou

doi:10.1186/s40623-020-01288-x

International Geomagnetic Reference Field: the thirteenth generation

P. Alken^*, E. Thébault, C. D. Beggan, H. Amit, J. Aubert, J. Baerenzung, T. N. Bondar, W. J. Brown, S. Califf, A. Chambodut, A. Chulliat, G. A. Cox, C. C. Finlay, A. Fournier, N. Gillet, A. Grayver, M. D. Hammer, M. Holschneider, L. Huder, G. HulotT. Jager, C. Kloss, M. Korte, W. Kuang, A. Kuvshinov, B. Langlais, J. M. Léger, V. Lesur, P. W. Livermore, F. J. Lowes, S. Macmillan, W. Magnes, M. Mandea, S. Marsal, J. Matzka, M. C. Metman, T. Minami, A. Morschhauser, J. E. Mound, M. Nair, S. Nakano, N. Olsen, F. J. Pavón-Carrasco, V. G. Petrov, G. Ropp, M. Rother, T. J. Sabaka, S. Sanchez, D. Saturnino, N. R. Schnepf, X. Shen, C. Stolle, A. Tangborn, L. Tøffner-Clausen, H. Toh, J. M. Torta, J. Varner, F. Vervelidou, P. Vigneron, I. Wardinski, J. Wicht, A. Woods, Y. Yang, Z. Zeren, B. Zhou

^*Autor/a de correspondencia de este trabajo

Producción científica: Artículo en revista indizada › Artículo › revisión exhaustiva

707 Citas (Scopus)

Resumen

In December 2019, the International Association of Geomagnetism and Aeronomy (IAGA) Division V Working Group (V-MOD) adopted the thirteenth generation of the International Geomagnetic Reference Field (IGRF). This IGRF updates the previous generation with a definitive main field model for epoch 2015.0, a main field model for epoch 2020.0, and a predictive linear secular variation for 2020.0 to 2025.0. This letter provides the equations defining the IGRF, the spherical harmonic coefficients for this thirteenth generation model, maps of magnetic declination, inclination and total field intensity for the epoch 2020.0, and maps of their predicted rate of change for the 2020.0 to 2025.0 time period. [Figure not available: see fulltext.]

Idioma original	Inglés
Número de artículo	49
Publicación	Earth, Planets and Space
Volumen	73
N.º	1
DOI	https://doi.org/10.1186/s40623-020-01288-x
Estado	Publicada - dic 2021

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Alken, P., Thébault, E., Beggan, C. D., Amit, H., Aubert, J., Baerenzung, J., Bondar, T. N., Brown, W. J., Califf, S., Chambodut, A., Chulliat, A., Cox, G. A., Finlay, C. C., Fournier, A., Gillet, N., Grayver, A., Hammer, M. D., Holschneider, M., Huder, L., ... Zhou, B. (2021). International Geomagnetic Reference Field: the thirteenth generation. Earth, Planets and Space, 73(1), Artículo 49. https://doi.org/10.1186/s40623-020-01288-x

@article{0ffd280753b4422680b1a202d6a8764d,

title = "International Geomagnetic Reference Field: the thirteenth generation",

abstract = "In December 2019, the International Association of Geomagnetism and Aeronomy (IAGA) Division V Working Group (V-MOD) adopted the thirteenth generation of the International Geomagnetic Reference Field (IGRF). This IGRF updates the previous generation with a definitive main field model for epoch 2015.0, a main field model for epoch 2020.0, and a predictive linear secular variation for 2020.0 to 2025.0. This letter provides the equations defining the IGRF, the spherical harmonic coefficients for this thirteenth generation model, maps of magnetic declination, inclination and total field intensity for the epoch 2020.0, and maps of their predicted rate of change for the 2020.0 to 2025.0 time period. [Figure not available: see fulltext.]",

keywords = "Geomagnetism, IGRF, Magnetic field modeling",

author = "P. Alken and E. Th{\'e}bault and Beggan, {C. D.} and H. Amit and J. Aubert and J. Baerenzung and Bondar, {T. N.} and Brown, {W. J.} and S. Califf and A. Chambodut and A. Chulliat and Cox, {G. A.} and Finlay, {C. C.} and A. Fournier and N. Gillet and A. Grayver and Hammer, {M. D.} and M. Holschneider and L. Huder and G. Hulot and T. Jager and C. Kloss and M. Korte and W. Kuang and A. Kuvshinov and B. Langlais and L{\'e}ger, {J. M.} and V. Lesur and Livermore, {P. W.} and Lowes, {F. J.} and S. Macmillan and W. Magnes and M. Mandea and S. Marsal and J. Matzka and Metman, {M. C.} and T. Minami and A. Morschhauser and Mound, {J. E.} and M. Nair and S. Nakano and N. Olsen and Pav{\'o}n-Carrasco, {F. J.} and Petrov, {V. G.} and G. Ropp and M. Rother and Sabaka, {T. J.} and S. Sanchez and D. Saturnino and Schnepf, {N. R.} and X. Shen and C. Stolle and A. Tangborn and L. T{\o}ffner-Clausen and H. Toh and Torta, {J. M.} and J. Varner and F. Vervelidou and P. Vigneron and I. Wardinski and J. Wicht and A. Woods and Y. Yang and Z. Zeren and B. Zhou",

note = "Funding Information: The Swarm and Cryosat-2 missions are supported by the European Space Agency (ESA). The {\O}rsted mission was made possible by extensive support from the Danish government, NASA, ESA, CNES, DARA, and the Thomas B. Thriges Foundation. The CHAMP mission was sponsored by the Space Agency of the German Aerospace Center (DLR) through funds of the Federal Ministry of Economics and Technology, following a decision of the German Federal Parliament (grant code 50EE0944). The SAC-C mission was made possible by a collaboration between the Comisi{\'o}n Nacional de Actividades Espaciales (CONAE), NASA/JPL, and the Danish Space Research Institute. The CSES mission is funded by the China National Space Administration (CNSA) and the China Earthquake Administration (CEA). The international network of geomagnetic observatories is supported by numerous institutes, staff, and INTERMAGNET. The French contribution to this work was supported by the French Centre National des Etudes Spatiales (CNES) in the framework of the program “Exploitation de la mission satellitaire europ{\'e}enne Swarm.” Publisher Copyright: {\textcopyright} 2021, The Author(s).",

year = "2021",

month = dec,

doi = "10.1186/s40623-020-01288-x",

language = "English",

volume = "73",

journal = "Earth, Planets and Space",

issn = "1343-8832",

publisher = "Springer International Publishing AG",

number = "1",

}

Alken, P, Thébault, E, Beggan, CD, Amit, H, Aubert, J, Baerenzung, J, Bondar, TN, Brown, WJ, Califf, S, Chambodut, A, Chulliat, A, Cox, GA, 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, Magnes, W, Mandea, M, Marsal, S, Matzka, J, Metman, MC, Minami, T, Morschhauser, A, 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 2021, 'International Geomagnetic Reference Field: the thirteenth generation', Earth, Planets and Space, vol. 73, n.º 1, 49. https://doi.org/10.1186/s40623-020-01288-x

TY - JOUR

T1 - International Geomagnetic Reference Field

T2 - the thirteenth generation

AU - Alken, P.

AU - Thébault, E.

AU - Beggan, C. D.

AU - Amit, H.

AU - Aubert, J.

AU - Baerenzung, J.

AU - Bondar, T. N.

AU - Brown, W. J.

AU - Califf, S.

AU - Chambodut, A.

AU - Chulliat, A.

AU - Cox, G. A.

AU - Finlay, C. C.

AU - Fournier, A.

AU - Gillet, N.

AU - Grayver, A.

AU - Hammer, M. D.

AU - Holschneider, M.

AU - Huder, L.

AU - Hulot, G.

AU - Jager, T.

AU - Kloss, C.

AU - Korte, M.

AU - Kuang, W.

AU - Kuvshinov, A.

AU - Langlais, B.

AU - Léger, J. M.

AU - Lesur, V.

AU - Livermore, P. W.

AU - Lowes, F. J.

AU - Macmillan, S.

AU - Magnes, W.

AU - Mandea, M.

AU - Marsal, S.

AU - Matzka, J.

AU - Metman, M. C.

AU - Minami, T.

AU - Morschhauser, A.

AU - Mound, J. E.

AU - Nair, M.

AU - Nakano, S.

AU - Olsen, N.

AU - Pavón-Carrasco, F. J.

AU - Petrov, V. G.

AU - Ropp, G.

AU - Rother, M.

AU - Sabaka, T. J.

AU - Sanchez, S.

AU - Saturnino, D.

AU - Schnepf, N. R.

AU - Shen, X.

AU - Stolle, C.

AU - Tangborn, A.

AU - Tøffner-Clausen, L.

AU - Toh, H.

AU - Torta, J. M.

AU - Varner, J.

AU - Vervelidou, F.

AU - Vigneron, P.

AU - Wardinski, I.

AU - Wicht, J.

AU - Woods, A.

AU - Yang, Y.

AU - Zeren, Z.

AU - Zhou, B.

N1 - Funding Information: The Swarm and Cryosat-2 missions are supported by the European Space Agency (ESA). The Ørsted mission was made possible by extensive support from the Danish government, NASA, ESA, CNES, DARA, and the Thomas B. Thriges Foundation. The CHAMP mission was sponsored by the Space Agency of the German Aerospace Center (DLR) through funds of the Federal Ministry of Economics and Technology, following a decision of the German Federal Parliament (grant code 50EE0944). The SAC-C mission was made possible by a collaboration between the Comisión Nacional de Actividades Espaciales (CONAE), NASA/JPL, and the Danish Space Research Institute. The CSES mission is funded by the China National Space Administration (CNSA) and the China Earthquake Administration (CEA). The international network of geomagnetic observatories is supported by numerous institutes, staff, and INTERMAGNET. The French contribution to this work was supported by the French Centre National des Etudes Spatiales (CNES) in the framework of the program “Exploitation de la mission satellitaire européenne Swarm.” Publisher Copyright: © 2021, The Author(s).

PY - 2021/12

Y1 - 2021/12

N2 - In December 2019, the International Association of Geomagnetism and Aeronomy (IAGA) Division V Working Group (V-MOD) adopted the thirteenth generation of the International Geomagnetic Reference Field (IGRF). This IGRF updates the previous generation with a definitive main field model for epoch 2015.0, a main field model for epoch 2020.0, and a predictive linear secular variation for 2020.0 to 2025.0. This letter provides the equations defining the IGRF, the spherical harmonic coefficients for this thirteenth generation model, maps of magnetic declination, inclination and total field intensity for the epoch 2020.0, and maps of their predicted rate of change for the 2020.0 to 2025.0 time period. [Figure not available: see fulltext.]

AB - In December 2019, the International Association of Geomagnetism and Aeronomy (IAGA) Division V Working Group (V-MOD) adopted the thirteenth generation of the International Geomagnetic Reference Field (IGRF). This IGRF updates the previous generation with a definitive main field model for epoch 2015.0, a main field model for epoch 2020.0, and a predictive linear secular variation for 2020.0 to 2025.0. This letter provides the equations defining the IGRF, the spherical harmonic coefficients for this thirteenth generation model, maps of magnetic declination, inclination and total field intensity for the epoch 2020.0, and maps of their predicted rate of change for the 2020.0 to 2025.0 time period. [Figure not available: see fulltext.]

KW - Geomagnetism

KW - IGRF

KW - Magnetic field modeling

UR - http://www.scopus.com/inward/record.url?scp=85093067418&partnerID=8YFLogxK

U2 - 10.1186/s40623-020-01288-x

DO - 10.1186/s40623-020-01288-x

M3 - Article

AN - SCOPUS:85093067418

SN - 1343-8832

VL - 73

JO - Earth, Planets and Space

JF - Earth, Planets and Space

IS - 1

M1 - 49

ER -

International Geomagnetic Reference Field: the thirteenth generation

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