PSP Bibliography


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Coronal Loop Heating by Nearly Incompressible Magnetohydrodynamic and Reduced Magnetohydrodynamic Turbulence Models

The transport of waves and turbulence beyond the photosphere is central to the coronal heating problem. Turbulence in the quiet solar corona has been modeled on the basis of the nearly incompressible magnetohydrodynamic (NI MHD) theory to describe the transport of low-frequency turbulence in open magnetic field regions. It describes the evolution of the coupled majority quasi-2D and minority slab component, driven by the magnetic carpet and advected by a subsonic, sub-Alfv\ enic flow from the lower corona. In this paper, we ...

Yalim, M.~S.; Zank, G.~P.; Asgari-Targhi, M.;

Published by: \apj      Published on: feb

YEAR: 2023     DOI: 10.3847/1538-4357/acb151

Parker Data Used; Magnetohydrodynamics; Solar coronal loops; interplanetary turbulence; 1964; 1485; 830