Solar and Heliospheric Modeling Activities at the CCMC

The CCMC currently hosts a number of different MHD and semi-empirical models of the corona and heliosphere. These models are frequently updated as the developers improve their models, adding new features and improving their accuracy and robustness. In particular the models in this community are transitioning from modes in which they support runs driven by synoptic photospheric magnetograms, to modes which include transient events and numerical experimentation through the use of user defined inputs. In this presentation we report on these upgrade activities and on the evolution of the models to support this new experimentation. In addition we report on use of our in-house data formatting and interpolation tool to design a comprehensive magnetogram construction tool.