Models of high mass flux disks with decreasing curvature. Shapes (a), and spectral energy distributions of models with outbursting (b) and quiescent (c) inner disk sources. Line types are the same in each panel. Solid, long‐dashed, and short‐dashed lines represent models for which ﹩z=1.5( r/ R_{0}) ^{-0.03}﹩, ﹩1.4( r/ R_{0}) ^{-0.02}﹩, and ﹩1.3( r/ R_{0}) ^{-0.015}﹩, respectively (﹩H_{d}\propto r^{z}﹩). Dot‐dashed lines represent models with α varied as described in text. Note the two‐slope behavior of outbursting SEDs with slope of ﹩a\approx -4/ 3﹩ out to several microns and a plateau region with more shallow slope (﹩a\approx 0﹩) to tens of microns.