Figure 1: What Dante sees in a typical VisRad
halfraum simulation, progressively
zoomed in. Emission temperature is shown here.
The question: DANTE sees a different proportion of
hot spots, wall,
low-albedo witness plate, and LEH/vacuum than does the witness plate. How do the radiation temperatures and
spectra incident
on DANTE and the witness plate compare?
How does beam pointing affect the temperatures? How important is it to
model these
effects when analyzing hohlraum/halfraum data from OMEGA?
