Description
We present a newly updated version of SPHERLS, which can be used for modelling the interaction of convection and pulsation in radial pulsators. We present preliminary calculations to verify performance for RR Lyrae stars, as well as extensions to Cepheids. SPHERLS will be made publicly available, and is expected to have applications to a number of outstanding problems in understanding RR Lyrae and classical Cepheids.
