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

Coronal Loop Heating by Nearly Incompressible Magnetohydrodynamic and Reduced Magnetohydrodynamic Turbulence ModelsDOI: info:10.3847/1538-4357/acb151v. 944119
Yalim, M. S., Zank, G. P., and Asgari-Targhi, Mahboubeh. 2023. "Coronal Loop Heating by Nearly Incompressible Magnetohydrodynamic and Reduced Magnetohydrodynamic Turbulence Models." The Astrophysical Journal, 944 119. https://doi.org/10.3847/1538-4357/acb151.
ID: 168367
Type: article
Keywords: SAO