Solving the system of Radiation Magnetohydrodynamics

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The book introduces a Finite-Volume scheme designed for radiation magnetohydrodynamics, crucial for modeling solar plasma dynamics. It begins with a basic conservation laws framework, analyzing convergence with a model problem. Essential modifications enhance the scheme's accuracy by accommodating various equations of state, correcting magnetic field divergence errors, and improving equilibrium state approximations. Additionally, it addresses radiation intensity in solar photosphere simulations, emphasizing the significance of solving the radiation transport equation for realistic atmospheric modeling.