3DPD: A photogrammetric pipeline for a PUSH frame stereo cameras
| Autor: | E. Simioni, Amedeo Petrella, G. Cremonese, Teo Mudric, Stepan Tulyakov, N. Thomas, Antoine Pommerol, Cristina Re |
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| Rok vydání: | 2021 |
| Předmět: |
Image processing
Satellite images Software Digital photogrammetry Stereo matching 010504 meteorology & atmospheric sciences Computer science Pipeline (computing) Multispectral image ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION Image processing 01 natural sciences Data acquisition 0103 physical sciences Computer vision stereo matching 010303 astronomy & astrophysics Image resolution 0105 earth and related environmental sciences surface imaging-system algorithm cassis Stereo cameras software business.industry 520 Astronomy Astronomy and Astrophysics calibration 620 Engineering image processing color digital photogrammetry Photogrammetry Stereo imaging Space and Planetary Science Artificial intelligence business satellite images performance |
| DOI: | 10.48350/153439 |
| Popis: | An innovative photogrammetric pipeline has been developed by INAF-Padova for the processing of the stereo images from the CaSSIS (Colour and Stereo Imaging System) (Thomas et al., 2014). CaSSIS is the multispectral stereo push frame camera on board ExoMars TGO (Trace Gas Orbiter) which will image 1.5% of the Mars surface in stereo mode with a spatial resolution of 4.6 m/pixel: the highest resolution single pass stereo capability currently operating a Mars. Data acquisition started in April 2018. The camera is able to provide two images of the same target from two different points of view along the same orbit and within one minute. The telescope is mounted on a rotational stage and its boresight is oriented to 10 degrees with respect to nadir direction. After the acquisition of the first set of images looking forward along track, the rotational stage is rotated by 180 degrees and a second set of images (looking backward) is acquired. The stereo pairs can then be processed to provide the 3D topography of specific targets. The suite of photogrammetry and imaging tools, named 3DPD (3Dimensional reconstruction of Planetary Data) (Simioni a al. 2017), is designed for processing stereo push frame data and producing the three-dimensional data for geomorphological analysis of planetary surfaces. The workflow involves a MATLAB tool for the preparation of the inputs (the mosaicked images and the projection matrices) to be ingested into the 3DPD matching core software. The pipeline is in continuous development and routinely ingests a large number of images that CaSSIS is presently acquiring and will continue to acquire in the future. CaSSIS 3DPD products are the unique DTMs available nowadays and the stereo products have been considered in some scientific work (as described in Section 6.2). The same pipeline faces the need of a dedicated pipeline for the Mercury Global Mapping with the Spectrometers and Imagers for the Mercury Planetary Orbiter (MPO) BepiColombo Integrated Observatory SYStem (SIMBIO-SYS) (Cremonese et al., 2020). |
| Databáze: | OpenAIRE |
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