Soumitra is working on developing coupled models for the interaction of exoplanets with their host star's corona.
Kalpa is working on simulations of the solar wind, and particle transport in the inner heliosphere.
Chen is working on numerical simulations of exoplanets magnetospheres and ionospheres.
Chris worked on numerical simulations of stellar coronae.
Qusai developed a multi-fluid magnetohydrodynamic (MHD) code for the solar chromosphere. His model includes the collisions between ionized and neutral particles, which plays a major role in the physics of the chromosphere.
Now a postdoc at the University of Michigan
Undergraduate Students: