solar-corona 3
- EXTENSION OF THE MURAM RADIATIVE MHD CODE FOR CORONAL SIMULATIONS (Rempel, 2017)
- A model for heating the super-hot corona in solar active regions (Lu et al., 2024)
- What determines the brightness of magnetically open solar corona?: Insights from three-dimensional radiative MHD simulations and observations (Iijima, H., 2025)