Journal metrics

Journal metrics

  • IF value: 1.129 IF 1.129
  • IF 5-year value: 1.519 IF 5-year 1.519
  • CiteScore value: 1.54 CiteScore 1.54
  • SNIP value: 0.798 SNIP 0.798
  • SJR value: 0.610 SJR 0.610
  • IPP value: 1.41 IPP 1.41
  • h5-index value: 21 h5-index 21
  • Scimago H index value: 48 Scimago H index 48
Definitions
Nonlin. Processes Geophys., 25, 207-216, 2018
https://doi.org/10.5194/npg-25-207-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
Volume 25, issue 1
Review article
12 Mar 2018
Evolution of fractality in space plasmas of interest to geomagnetic activity
Víctor Muñoz1, Macarena Domínguez2, Juan Alejandro Valdivia1,3, Simon Good4,5, Giuseppina Nigro6, and Vincenzo Carbone6 1Departamento de Física, Facultad de Ciencias, Universidad de Chile, Santiago, Chile
2Departamento de Física, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Santiago, Chile
3Centro para la Nanociencia y la Nanotecnología, CEDENNA, Santiago, Chile
4Department of Physics, University of Helsinki, Helsinki, Finland
5The Blackett Laboratory, Imperial College London, London, UK
6Dipartimento di Fisica, Università della Calabria, Rende, Italy
Received: 01 Aug 2017 – Discussion started: 07 Aug 2017
Revised: 31 Dec 2017 – Accepted: 03 Jan 2018 – Published: 12 Mar 2018
Abstract. 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 magnetized plasma, which may be a useful model to study geomagnetic activity under solar wind forcing. We show that the shell model is able to reproduce the relationship between the fractal dimension and the occurrence of dissipative events, but only in a certain region of viscosity and resistivity values. We also present preliminary results of the application of these ideas to the study of the magnetic field time series in the solar wind during magnetic clouds, which suggest that it is possible, by means of the fractal dimension, to characterize the complexity of the magnetic cloud structure.
Citation: Muñoz, V., Domínguez, M., Valdivia, J. A., Good, S., Nigro, G., and Carbone, V.: Evolution of fractality in space plasmas of interest to geomagnetic activity, Nonlin. Processes Geophys., 25, 207-216, https://doi.org/10.5194/npg-25-207-2018, 2018.
Publications Copernicus
Special issue
Nonlinear Waves and Chaos
Download
PDF XML
Short summary
Fractals are self-similar objects (which look the same at all scales), whose dimensions can be noninteger. They are mathematical concepts, useful to describe various physical systems, as the fractal dimension is a measure of their complexity. In this paper we study how these concepts can be applied to some problems in space plasmas, such as the activity of the Earth's magnetosphere, simulations of plasma turbulence, or identification of magnetic structures ejected from the Sun.
Fractals are self-similar objects (which look the same at all scales), whose dimensions can be...
Read more
Citation
Share