SIMIONI, EMANUELEEMANUELESIMIONIRE, CristinaCristinaREMUDRIC, TEOTEOMUDRICPETRELLA, AmedeoAmedeoPETRELLACREMONESE, GabrieleGabrieleCREMONESE2020-10-152020-10-152020http://hdl.handle.net/20.500.12386/27852http://dx.doi.org/10.20371/INAF/TechRep/41The Team at the Observatory of Padova (INAF) developed a stereo 3d reconstruction pipeline for the planetary images, by taking advantage of its know-how from the design, realization and calibration of the stereo camera STC on board the BepiColombo mission. The stereo cameras STC and CaSSIS are different in terms of optical design and stereo strategy, but they both apply the push-frame acquisition mode. In this context, an ad-hoc DTM generation software, called 3DPD, has been developed.This document describes the nowadays procedures for the internal use of the 3DPD software and the associated MATLAB tools finalized to: - update of the CaSSIS images and spice kernels - Read CaSSIS images data and projection matrices assembly - generate the stereo pair mosaic projects - generate the 3D models (DTMs) - update the OAPD Archive (https://cassis.oapd.inaf.it/archive/) All these procedures can be performed only by OAPD Workstations. Changes in the procedures will be documented in the next issues of this report.ELETTRONICOenTechnical reportINF/01 - INFORMATICAERC sectors::Physical Sciences and Engineering::PE6 Computer Science and Informatics: Informatics and information systems, computer science, scientific computing, intelligent systems::PE6_6 Algorithms, distributed, parallel and network algorithms, algorithmic game theory