  We present mid-infrared interferometric observations of the Herbig Ae star R
CrA obtained with MIDI at the VLTI using several projected baselines in the
UT2-UT3 configuration. The observations show resolved circumstellar emission in
the wavelength range 8-13 micron on a ~6 AU scale with a non-symmetric
intensity distribution, providing support for an inclined disk geometry.
Visibilities are best fitted using a uniform ring model with outer radius in
the range 6-10 AU, in the wavelength range 8-13 micron. The inclination of the
ring with respect to the plane of the sky is found to be ~45 deg., consistent
with the 40 deg. suggested from near-infrared imaging polarimetry (Clark et al.
2000, MNRAS, 319, 337).
