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火星探测是当前国家高技术科技竞争力的标志,世界航天强国均研制火星大气模式为登陆选址、科学探测提供气象环境保障。然而,我国此前尚无自主研发的火星大气模式。中国科学院大气物理研究所火星研究团队基于自主研发的高分辨率大气模式动力框架,拓展其应用领域到火星大气。在此基础上,引进并耦合了美国宇航局艾姆斯研究中心的火星物理过程,构建了新一代火星大气模式Global Open Planetary atmosph...
Bright reflections observed at Mars’ south pole serve as evidence for water. But, seeing may be deceiving.
China has paid considerable attention to space exploration and made great strides in the field. The first Chinese Mars Exploration Mission will be carried out in 2020. Digital simulation has been prov...
Four NASA missions over the last forty years with onboard instruments for high-resolution orbital imaging have achieved both global coverage (with 6m CTX, 20m THEMIS-VIS and >8m Viking Orbiter cameras...
The surface of Mars has been an object of interest for planetary research since the launch of Mariner 4 in 1964. Since then different cameras such as the Viking Visual Imaging Subsystem (VIS), Mars Gl...
Understanding planetary atmosphere-surface exchange and extra-terrestrial-surface formation processes within our Solar System is one of the fundamental goals of planetary science research. There has b...
Due to the large data amount of HiRISE imagery, traditional radiometric calibration method is not able to meet the fast processing requirements. To solve this problem, a radiometric calibration system...
Currently, Mars Express HRSC imagery is an essential data source to derive high accuracy Mars topographic data. In view of the characteristics of Martian surface satellite imagery, a dense image match...
We are investigating change detection techniques to automatically detect mass movements at the steep north polar scarps of Mars, in order to improve our understanding of these dynamic processes. Here ...
The photogrammetric bundle adjustment of line scanner image data requires a precise description of the time-dependent image orientation. For this task exterior orientation parameters of discrete point...
Geomorphologists who study Earth’s surface features and the processes that formed them have long been interested in how floods, in particular catastrophic outbursts that occur when a glacial lake ice ...
This paper deals with the computation of a new global control point network of the planet Mars. The existing Mars control point net is based on Viking data and consists of a large number of ground poi...
Viking Orbiter stereo images were used to derive a geometrially precise orthoimage mosaic at 40m scale for the Mars Pathfinder landing site. Camera pointing for each images was obtained by a formal bu...
The Mars Pathfinder stereo camera (IMP) produced a set of images unique in what they show and unique in the methods they require for their analysis and processing: We first studied the ability of the ...
Described are experimental results of a first approach towards optimal shaded relief representation of the surface of Mars derived from Viking Orbiter digital imagery. The complex problem addresses ho...

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