The Solar Astrophysics Research Group at Rice University uses theory, computational models, observational data analysis, and machine learning to investigate solar, space, and astrophysical plasma environments spanning solar and stellar coronae and winds, star - planet interactions, and ultracold laboratory plasma.
Our research interests in these contexts include magneto-fluid and kinetic physics, energy transport and dissipation, non-thermal and non-equilibrium processes, turbulence, plasma waves and shocks, and magnetic reconnection.
We develop and build our own numerical and forward modeling tools to facilitate our research projects.
How Are Active Region Properties and Heating Connected?
Probing Flare-Generated Slow-Mode Waves in Coronal Loops Detected by SDO/AIA
Investigating the Influence of Coronal Magnetic Geometry on the Acceleration of the Solar Wind