Fraction excitations as a driving mechanism for the self-organized dynamical structuring in the solar wind

DOI10.1023/A:1002450525201zbMath0974.85009OpenAlexW4249929880MaRDI QIDQ1574507

N. Delaunay

Publication date: 12 December 2001

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1002450525201

zbMATH Keywords

interplanetary magnetic fieldself-organized fractal geometry

Mathematics Subject Classification ID

Astronomy and astrophysics (85A99)

Related Items (2)

Non-extensive statistical analysis of magnetic field during the March 2012 ICME event using a multi-spacecraft approach ⋮ Tsallis non-extensive statistics and solar wind plasma complexity

This page was built for publication: Fraction excitations as a driving mechanism for the self-organized dynamical structuring in the solar wind