During the last decade, a number of studies have shown that turbulent processes in the plasma sheet are very important for the analysis of the formation of quasi‐stable plasma …
V Munoz, M Dominguez, G Nigro, M Riquelme… - Journal of Atmospheric …, 2021 - Elsevier
Abstract The Gledzer-Yamada-Ohkitani MHD shell model is used to describe dissipative events that take place in magnetized plasmas. In this review we summarize a series of works …
The magnetosphere is a multi-scale spatio-temporal complex dynamical system. In this context, we have analyzed the multifractal behavior of the AL index, as a proxy for an energy …
V Muñoz, M Domínguez, JA Valdivia… - Nonlinear Processes …, 2018 - npg.copernicus.org
We studied the temporal evolution of fractality for geomagnetic activity, by calculating fractal dimensions from the Dst data and from a magnetohydrodynamic shell model for turbulent …
M Domínguez, V Muñoz… - Journal of Geophysical …, 2014 - Wiley Online Library
The study of complexity in two aspects of the magnetic activity in the Sun‐Earth system is presented. We compare the temporal evolution of the magnetic fluctuations in the Earth's …
GL Delzanno, JE Borovsky - Frontiers in Astronomy and Space …, 2022 - frontiersin.org
This perspective advocates for the need of a combined system science approach to global magnetospheric models and to spacecraft magnetospheric data to answer the question “Do …
A magnetohydrodynamic (MHD) shell model is used to describe the dissipative events which take place in magnetized plasmas. A scatter plot box-counting fractal dimension D is …
V Pinto, M Stepanova, EE Antonova… - Journal of atmospheric …, 2011 - Elsevier
We have studied the turbulent processes in the central plasma sheet using the tailward alignments of THEMIS satellites. Fluctuations of the plasma bulk velocity and corresponding …