Articles | Volume 42, issue 1
https://doi.org/10.5194/angeo-42-163-2024
https://doi.org/10.5194/angeo-42-163-2024
Regular paper
 | 
27 May 2024
Regular paper |  | 27 May 2024

Permutation entropy and complexity analysis of large-scale solar wind structures and streams

Emilia K. J. Kilpua, Simon Good, Matti Ala-Lahti, Adnane Osmane, and Venla Koikkalainen

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Short summary
The solar wind is organised into slow and fast streams, interaction regions, and transient structures originating from solar eruptions. Their internal characteristics are not well understood. A more comprehensive understanding of such features can give insight itno physical processes governing their formation and evolution. Using tools from information theory, we find that the solar wind shows universal turbulent properties on smaller scales, while on larger scales, clear differences arise.