Frequency distribution model for geomagnetic SYM-H fluctuations

被引：0
|
作者：
Ewin Sánchez
Pedro Vega-Jorquera
机构：
[1] Intituto de Investigación Mutidisciplinar en Ciencia y Tecnología de la Universidad de La Serena,Departamento de Física, Facultad de Ciencias
[2] Universidad de La Serena,undefined
来源：
Acta Geodaetica et Geophysica | 2020年 / 55卷
关键词：
Geomagnetic storm; Frequency–magnitude distribution; Bayesian model;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
A model describing the frequency distribution of geomagnetic field fluctuations has been developed, allowing a better understanding of the influence of the solar magnetic field on the geomagnetic variations. The constructed model is analogous to the one presented by same authors in 2018 to describe the frequency distribution of seismic magnitudes. A similarity between seismic and geomagnetic systems is exposed from this point of view. Applications to data corresponding to four different years where the most intense fluctuations have occurred are presented.
引用
收藏
页码：555 / 566
页数：11
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