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应用/结构英文2017被引 167

The Colour and Stereo Surface Imaging System (CaSSIS) for the ExoMars Trace Gas Orbiter

N. Thomas, G. Cremonese, R. Ziethe, M. Gerber, Mathias Brändli, G. Bruno, M. Erismann, L. Gambicorti, T. Gerber, K. Ghose, Mario Gruber, P. Gubler, H. Mischler, J. Jost, D. Piazza, A. Pommerol, Markus Rieder, V. Roloff, A. Servonet, W. Trottmann, T. Uthaicharoenpong, C. Zimmermann, Dervis Vernani, Micah Johnson, E. Pelò, Thomas Weigel, Jacques Viertl, Nicolas Roux, P. Lochmatter, G. Sutter, A. Casciello, T. Hausner, Iacopo Ficai Veltroni, Vania Da Deppo, P. Orleański, Witold Nowosielski, Tomasz Zawistowski, S. Szalaı̈, B. Sodor, Stepan Tulyakov, G. Troznai, M. Banaskiewicz, J. C. Bridges, Shane Byrne, S. Debei, M. R. El‐Maarry, Ernst Hauber, C. J. Hansen, A. B. Ivanov, L. Keszthelyi, R. L. Kirk, R. O. Kuzmin, N. Mangold, L. Marinangeli, W. J. Markiewicz, Matteo Massironi, A. S. McEwen, C. H. Okubo, L. L. Tornabene, P. Wajer, J. J. Wray · University of Bern
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期刊 / 来源Space Science Reviews
卷/期/页212 / 3-4 / 1897-1944
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摘要整理

The Colour and Stereo Surface Imaging System (CaSSIS) is the main imaging system onboard the European Space Agency’s ExoMars Trace Gas Orbiter (TGO) which was launched on 14 March 2016. CaSSIS is intended to acquire moderately high resolution (4.6 m/pixel) targeted images of Mars at a rate of 10–20 images per day from a roughly circular orbit 400 km above the surface. Each image can be acquired in up to four colours and stereo capability is foreseen by the use of a novel rotation mechanism. A typical product from one image acquisition will be a $9.5~\mbox{km} \times {\sim}45~\mbox{km}$ swath in full colour and stereo in one over-flight of the target thereby reducing atmospheric influences inherent in stereo and colour products from previous high resolution imagers. This paper describes the instrument including several novel technical solutions required to achieve the scientific requirements.

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