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 magneto- plasma 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.