  We present synthetic images of disks around T Tauri stars. We calculate
visibility curves in order to study the possibility of directly detecting
thermal emission from T Tauri disks. Total fluxes of T Tauri disks are compared
to the sensitivity of VISA, the interferometric sub-array of the European Very
Large Telescope. We conclude that thermal emission from circumstellar disk
around T Tauri stars is detectable with current or soon-to-be interferometric
techniques at wavelengths longer than 2.2 microns.
