My primary research interest lies in the field of solar astrophysics. Over the past five years, I have been primarily working on numerical magnetohydrodynamic (MHD) simulations and forward modeling of magnetic reconnection and thermal instability. My goal is to understand the coupled nature of these two processes and how they drive eruptions while contributing to the Sun's multi-thermal characteristics. This remains an open problem, offering significant opportunities to expand our current understanding from both theoretical and observational perspectives.

Some of my recent theoretical simulation models, developed in collaboration with colleagues, have gained recognition in the community for addressing the missing link in this phenomenon within the solar corona. Moreover, due to the scale-free nature of MHD, these models can be extrapolated to much larger scales, encompassing the heliosphere, stars, galaxies, and the universe as a whole.

In this forum, I look forward to presenting my work, exchanging ideas with fellow researchers, and discussing future perspectives in this exciting field.