Sketch of the inner disk structure around CTTSs indicating our three component model. The unocculted part of the stellar disk is denoted with A. The upper disk layer causes reddening of part the stellar disk (part B of the stellar disk). Stellar emission from the region denoted with C is subject to opaque (gray) extinction by the lower disk layers. We also show the inner disk radius r, the viewing inclination i, and the height h of the inner disk warp with respect to the disk midplane.