Analysis of high resolution and full disk solar images

In the last years, our group started to develop image processing procedures to analyze data coming from ground-based solar telescopes, both for observations with high spatial and spectroscopic resolution (THEMIS, DST at NSO/SP), and for full-disk observations (RISE/PSPT-OAR). The main procedures we developed to produce Advanced Calibrated Data (ACD) are the following: 1. standard digital image corrections (flat-field, dark current; global motion and oscillation filtering when requested); 2. image segmentation (identification of granules, granular and super-granular cells, and solar network); 3. non-linear fitting of spectral cubes derived from Fabry-Perot (FP) imaging spectrometer and instrumental spectral corrections; 4. image restoration (Wiener filtering, Phase Diversity Technique); 5. feature tracking (neural network, threshold method, CLT). Thanks to that, we acquired a wealth of solar data processing and display routines. In this framework we are interested in collaboration for the Visible-Light Imager and Magnetograph (VIM) data processing system. In particular we propose our participation in the realization of the analysis pipeline and graphical interface for the VIM instrument.