Speaker
Mark Cheung
(CSIRO)
Description
We discuss the current state of MHD modeling of solar flares and eruptions. We focus on models that yield synthetic observables accessible to current and future generations of remote sensing capabilities, such as MUSE, EUVST and ground-based observatories. A critical assessment of the successes and limitations of current models with be presented, as well as suggestions for paths going forward.
Primary author
Mark Cheung
(CSIRO)
