  We present a speckle analysis of the active galactic nucleus (AGN) inside the
archetype Seyfert type 2 galaxy NGC 1068. This study is based on 12.8 microns
images obtained with the burst mode of VISIR (the Very Large Telescope Imager
and Spectrometer in the InfraRed). The interferometric processing allows to
push the resolution far below the diffraction limit of a 8m telescope in the
N-band and to trace two main contributions to the mid-IR flux inside the
nucleus. It also allows to partially fill the lack of visibility points at low
spatial frequencies. The confrontation with VLT/MIDI (the Mid-InfrareD
Interferometer) data points helps to establish the link between dust in the
vicinity of the central engine and inside the ionisation cone to get a
multi-scale picture of mid-IR sources emitting in the nucleus of NGC 1068.
