Geomagnetic core field models and secular variation forecasts for the 13th International Geomagnetic Reference Field (IGRF-13)

Earth, Planets and Space

M. Mandea¹  A. Chambodut²  I. Wardinski²  E. Thébault³  D. Saturnino⁴  B. Langlais⁴  H. Amit⁴ 

[1] Centre National d’ Etudes Spatiales (CNES), Paris, France;Institut de Physique du Globe de Strasbourg, Université de Strasbourg/EOST, CNRS, UMR 7516, Strasbourg, France;Laboratoire Magmas et Volcans, Université de Clermont Auvergne, CNRS UMR 6524, Clermont Ferrand, France;Laboratoire de Planétologie et Géodynamique, Université de Nantes, Université d’Angers, CNRS, UMR 6112, Nantes, France;

关键词: The geomagnetic field;    Geomagnetic secular variation;    Geomagnetic field models;    Forecasts of the geomagnetic field;   

DOI  :  10.1186/s40623-020-01254-7

来源: Springer

【 摘 要 】

Observations of the geomagnetic field taken at Earth’s surface and at satellite altitude are combined to construct continuous models of the geomagnetic field and its secular variation from 1957 to 2020. From these parent models, we derive candidate main field models for the epochs 2015 and 2020 to the 13th generation of the International Geomagnetic Reference Field (IGRF). The secular variation candidate model for the period 2020–2025 is derived from a forecast of the secular variation in 2022.5, which results from a multi-variate singular spectrum analysis of the secular variation from 1957 to 2020.

【 授权许可】

CC BY