Study of the fractality of magnetized plasma using an MHD shell model driven by solar wind data-Reference-Cited by-同舟云学术

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Study of the fractality of magnetized plasma using an MHD shell model driven by solar wind data

Published:2018-09 Issue:9 Volume:25 Page:092302
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Domínguez Macarena¹,Nigro Giuseppina²,Muñoz Víctor³,Carbone Vincenzo²

Affiliation:

1. Departamento de Física, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, 8370449 Santiago, Chile

2. Dipartimento di Fisica, Universita della Calabria, 87036 Rende, CS, Italy

3. Departamento de Física, Facultad de Ciencias, Universidad de Chile, 7800003 Santiago, Chile

Funder

Comisión Nacional de Investigación Científica y Tecnológica

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

http://aip.scitation.org/doi/pdf/10.1063/1.5034129

Reference61 articles.

1. Fusion, space and solar plasmas as complex systems

2. Rank-ordered multifractal spectrum for intermittent fluctuations

3. Statistics of Active Region Complexity: A Large‐Scale Fractal Dimension Survey

4. Analysis and prediction of high-latitude geomagnetic disturbances based on a self-organized criticality framework

5. Solar cycle dependence of scaling in solar wind fluctuations

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4. An Argument in Favor of Magnetic Polarity Reversals Due to Heat Flux Variations in Fully Convective Stars and Planets;The Astrophysical Journal;2022-10-01

5. Complex Network Study of Solar Magnetograms;Entropy;2022-05-26

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