Inverse problem for the current loop model: Possibilities and restrictions


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

The possibilities of determining arbitrary current loop parameters based on the spatial structures of the magnetic field components generated by this loop on a sphere with a specified radius have been considered with the use of models. The model parameters were selected such that anomalies created by current loops on a sphere with a radius of 6378 km would be comparable in value with the different-scale anomalies of the observed main geomagnetic field (MGF). The least squares method was used to solve the inverse problem. Estimates close to the specified values were obtained for all current loop parameters except the current strength and radius. The radius determination error can reach ±120 km; at the same time, the magnetic moment value is determined with an accuracy of ±1%. The resolvability of the current force and radius can to a certain degree be improved by decreasing the observation sphere radius such that the ratio of the source distance to the current loop radius would be at least smaller than eight, which can be difficult to reach when modeling MGF.

作者简介

I. Demina

Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, St. Petersburg Branch

编辑信件的主要联系方式.
Email: dim@izmiran.spb.ru
俄罗斯联邦, Universitetskaya nab. 5/b, St. Petersburg, 199034

Yu. Farafonova

Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, St. Petersburg Branch

Email: dim@izmiran.spb.ru
俄罗斯联邦, Universitetskaya nab. 5/b, St. Petersburg, 199034

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Ltd., 2016