Year: 2025
Type: article
Abstract: Many planets, including Earth, possess a global dipolar magnetic field. To diagnose the interior source of the dipolar field, researchers usually adopt a dipole model consisting of six parameters to fit the observed dataset of the magnetic field. However, the simultaneous fitting of these parameters often leads to multiple local optimum parameter sets. To address this fitting dilemma, a current loop model was recently developed by Rong et al.(2021). This technique can separate and invert the loop parameters successively. Here, we further show how this technique can be reduced and modified to fit a dipole model. The applications of this reduced technique to the model of the International Geomagnetic Reference Field and the Martian crustal field model highlight its unique ability to diagnose both the planetary global dipolar field and the local crustal field anomaly, a capability that sets it apart from existing methods. This technique's potential impact on geomagnetism and planetary magnetism is significant, given its unique ability to diagnose both the planetary global dipolar field and the local crustal field anomaly.
Source: Earth and Planetary Physics
DOI: 10.26464/epp2025078
Authors: Rong ZhaoJin, Wei Yong, He Fei, Klinger Lucy, Yang YanYan, Gao JiaWei, Shi Zhen, Wang HuaPei, Cai ShuHui, Qin HuaFeng, Zhu RiXiang
Institutions: Chinese Academy of Sciences, Institute of Geology and Geophysics, University of Chinese Academy of Sciences, Fudan University, Shanghai Institute for Mathematics and Interdisciplinary Sciences, National Institute of Natural Hazards, China University of Geosciences, State Key Laboratory of Lithospheric Evolution
Language: English
Subfield: Molecular Biology
Domain: Life Sciences
Open Access status: gold
Estimated APC paid: $2,324
OpenAlex ID: W4411527954
