Models of high mass flux disks that flare uniformly. Shapes (a), and spectral energy distributions of models with outbursting (b) and quiescent (c) inner disk sources. Lines from lower to upper represent models with ﹩z=0﹩, 1, 9/8, and 5/4 (﹩H_{d}\propto r^{z}﹩). SEDs with dotted lines represent disks with larger radii (700 AU) than standard disks (160 AU). SEDs of models in outburst are double peaked. The positions of longer wavelength maxima correspond to the temperature at the outer edge of each model disk.