The Viability of Ohmic Dissipation as a Coronal Heating Source

• 1 October 1996
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 470, 1192
• https://doi.org/10.1086/177942

Abstract

Keywords

• THREE DIMENSIONAL
• MAGNETIC FIELD
• CURRENT DENSITY
• RADIATIVE TRANSFER
• CORONA SUN
• NUMERICAL SIMULATION
• STEADY STATE