Helical distributed chaos in magnetic field of solar wind
Space Physics
2019-07-11 v1 Solar and Stellar Astrophysics
Fluid Dynamics
Abstract
Helical distributed chaos in magnetic field has been studied using results of direct numerical simulations (dominated by magnetic helicity), of a laboratory experiment with plasma wind tunnel and of solar wind measurements (dominated by combined magnetic and cross helicity effects). The solar wind measurements, used for the spectral computations, were produced by Helios-1 and Ulysses missions for low and high heliolatitudes respectively and for high solar wind speed at AU (where is distance from the Sun).
Cite
@article{arxiv.1907.02425,
title = {Helical distributed chaos in magnetic field of solar wind},
author = {A. Bershadskii},
journal= {arXiv preprint arXiv:1907.02425},
year = {2019}
}