Realistic calculations of daily total insolation over the crater topography were made by time integration from the theoretical calculations of instantaneous solar radiation at two-minute intervals from astronomical sunrise to astronomical sunset. The calculations account for atmospheric attenuation of the direct solar beam as it passes through the earth's atmosphere, and for diffuse radiation. Estimates of atmospheric attenuation and diffuse radiation were obtained from measurements taken in Colorado's Brush Creek Valley in 1984. Because the interior south wall of the crater is in shadow during much of the day, large spatial differences in daily total radiation are seen across the interior of the crater. Important variations in total daily radiation are also seen around the crater's periphery. We plan to test the model simulations further using radiation data that will be collected in a major meteorological experiment (METCRAX - the Meteor Crater Experiment) to be conducted in the crater in the fall of 2006. The methods used to model solar radiation and shadow propagation at the Meteor Crater can be readily extended to other topographical situations.