Using Time Dependent Synoptic Magnetograms to Drive Models of the Corona and Heliosphere at the CCMC

Until recently, models of the global corona and inner heliosphere have been driven by single static photospheric synoptic magnetograms. These are now being superseded by time evolving models of the global photospheric field. In this presentation we discuss how the Community Coordinated Modeling Center is redeveloping both it's `realtime' and Runs-On-Request system to make use of these improved representations of the solar field. We focus principally on their use with the WSA/ENLIL model which can now be driven either by time interpolated magnetograms or by time series produced by the ADAPT system.