Articles | Volume 36, issue 2
Regular paper
23 Mar 2018
Regular paper |  | 23 Mar 2018

Non-Gaussianity and cross-scale coupling in interplanetary magnetic field turbulence during a rope–rope magnetic reconnection event

Rodrigo A. Miranda, Adriane B. Schelin, Abraham C.-L. Chian, and José L. Ferreira

Data sets

Cluster Science Archive ESA

Model code and software

Numerical tools for statistical analysis R. A. Miranda

Short summary
The solar wind is a tenuous turbulent plasma permeating the interplanetary space and is not well understood. A complex process called magnetic reconnection can act as a source of solar wind turbulence. Here we study this process using statistics. We demonstrate that high-order statistics of the magnetic field display a parabolic relation that is enhanced when magnetic reconnection occurs. Our results can help us understand the nature of solar wind turbulence.