Study of the fractality in a magnetohydrodynamic shell model forced by solar wind fluctuations

<p>The description of the relationship between interplanetary plasma and geomagnetic activity requires complex models. Drastically reducing the ambition of describing this detailed complex interaction and, if we are interested only in the fractality properties of the time series of its charact...

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Bibliographic Details
Main Authors: M. Domínguez, G. Nigro, V. Muñoz, V. Carbone, M. Riquelme
Format: Article
Language:English
Published: Copernicus Publications 2020-04-01
Series:Nonlinear Processes in Geophysics
Online Access:https://www.nonlin-processes-geophys.net/27/175/2020/npg-27-175-2020.pdf