Effect of convolution and rebinning on maps of bolometric intensity (left panels) and vertical field strength on the τ_R = 1 surface (right panels). Top row: original simulation resolution; middle row: convolved and rebinned corresponding to 1.0 m telescope apertures; bottom row: convolved and rebinned corresponding to 0.5 m telescope aperture. For clarity, we show only a 6 Mm  ×  6 Mm section of the full 24 Mm  ×  24 Mm full horizontal areas of the simulation.