Quantifying dynamical complexity of magnetic storms and solar flares via nonextensive Tsallis entropy

31Citations
Citations of this article
22Readers
Mendeley users who have this article in their library.

Abstract

Over the last couple of decades nonextensive Tsallis entropy has shown remarkable applicability to describe nonequilibrium physical systems with large variability and multifractal structure. Herein, we review recent results from the application of Tsallis statistical mechanics to the detection of dynamical changes related with the occurrence of magnetic storms. We extend our review to describe attempts to approach the dynamics of magnetic storms and solar flares by means of universality through Tsallis statistics. We also include a discussion of possible implications on space weather forecasting efforts arising from the verification of Tsallis entropy in the complex system of the magnetosphere. © 2011 by the authors.

Cite

CITATION STYLE

APA

Balasis, G., Daglis, I. A., Papadimitriou, C., Anastasiadis, A., Sandberg, I., & Eftaxias, K. (2011). Quantifying dynamical complexity of magnetic storms and solar flares via nonextensive Tsallis entropy. Entropy, 13(10), 1865–1881. https://doi.org/10.3390/e13101865

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free