Paper Review 7
- EXTENSION OF THE MURAM RADIATIVE MHD CODE FOR CORONAL SIMULATIONS (Rempel, 2017)
- A Comparative Analysis of High-resolution Shock-capturing Schemes for Two-dimensional Magnetohydrodynamic Simulation of Flux Emergence in the Solar Atmosphere (Son et al., 2025)
- A model for heating the super-hot corona in solar active regions (Lu et al., 2024)
- Which Component of Solar Magnetic Field Drives the Evolution of Interplanetary Magnetic Field over the Solar Cycle? (Yoshida, 2023)
- Convective Magnetic Flux Emergence Simulations from the Deep Solar Interior to the Photosphere: Comprehensive Study of Flux Tube Twist (Toriumi et al., 2024)
- What determines the brightness of magnetically open solar corona?: Insights from three-dimensional radiative MHD simulations and observations (Iijima, H., 2025)
- Studying the Spheromak Rotation in Data-constrained Coronal Mass Ejection Modeling with EUHFORIA and Assessing Its Effect on the Bz Prediction (Sarkar, R., et al., 2024)