Low Solar Coronal Thermal Structure Derived from Magnetohydrostatic Model

Abstract

By assuming the Sun in quiet condition we derived coronal thermal structure for low solar coronal magnetoplasma atmosphere. Ideal gas law in a static equilibrium configuration in coronal magnetic plasma state is derived and the solution may be directed to figure-out the thermal structure in mixed plasma and magnetic fields within the low corona. The results show that corona may have hot and ‘cool’ solution in low corona under the condition when the Sun in quiet condition.