A self-consistent turbulent model for solar coronal heating

• 1 May 1992
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 390, 297-308
• https://doi.org/10.1086/171280

Abstract

Keywords

• MAGNETOHYDRODYNAMIC TURBULENCE
• PLASMA HEATING
• SOLAR CORONA
• TURBULENCE MODELS
• HEAT FLUX
• HYDRODYNAMIC EQUATIONS
• MAGNETOHYDRODYNAMIC FLOW
• PHOTOSPHERE