Articles | Volume 25, issue 1
https://doi.org/10.5194/npg-25-207-2018
Special issue:
https://doi.org/10.5194/npg-25-207-2018
Review article
 | 
12 Mar 2018
Review article |  | 12 Mar 2018

Evolution of fractality in space plasmas of interest to geomagnetic activity

Víctor Muñoz, Macarena Domínguez, Juan Alejandro Valdivia, Simon Good, Giuseppina Nigro, and Vincenzo Carbone

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AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Victor Munoz on behalf of the Authors (29 Nov 2017)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (03 Dec 2017) by Gurbax S. Lakhina
RR by Anonymous Referee #1 (12 Dec 2017)
ED: Publish subject to minor revisions (review by editor) (21 Dec 2017) by Gurbax S. Lakhina
AR by Victor Munoz on behalf of the Authors (31 Dec 2017)  Author's response    Manuscript
ED: Publish as is (03 Jan 2018) by Gurbax S. Lakhina
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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.