I work between the observation and the model. The instrument measures polarisation; the atmosphere answers with a magnetic field, a temperature and a line-of-sight velocity. Everything I do is an attempt to get from the first to the second without losing the physics on the way.
I am a direct-entry PhD student in astronomy at Nanjing University, where the coronal-seismology work began, and a guest researcher at the Rosseland Centre for Solar Physics in Oslo, where I work on inversion, extrapolation and radiation synthesis for data-constrained MHD models of the corona.
The codes are public, SPOT and CuSP for inversion and PF2nlfff for extrapolation, because a diagnostic is only as reproducible as the code that produces it and because the fastest way to be corrected is to publish the tool.