...
首页> 外文期刊>Planetary and space science >3DPD: A photogrammetric pipeline for a PUSH frame stereo cameras
【24h】

3DPD: A photogrammetric pipeline for a PUSH frame stereo cameras

机译:3DPD:推框立体声摄像头的摄影测量管线

获取原文
获取原文并翻译 | 示例

摘要

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).
机译:通过Inaf-Padova开发了一种创新的摄影测量管线,用于从卡西斯(颜色和立体成像系统)处理立体图像(Thomas等,2014)。 Cassis是船上的MultiSpectral立体声推式框架摄像机,其上的展开TGO(痕量气体轨道器),它将在立体声模式下以4.6米/像素的空间分辨率为1.5%的火星表面:目前运行火星的最高分辨率单通立体声能力。数据采集​​于2018年4月开始。相机能够从同一轨道和一分钟内提供来自两个不同的视图相同目标的两个图像。望远镜安装在旋转阶段,并且其触摸钻在相对于Nadir方向上定向到10度。在获取沿轨道期向前期待的第一组图像之后,旋转级被获取180度旋转180度,并且获取第二组图像(向后看)。然后可以处理立体对以提供特定目标的3D地形。摄影测量和成像工具的套件,名为3DPD(行星数据的3Dimension重建)(Simioni A Al.2007),专为处理立体电框数据并产生行星表面的地貌分析的三维数据。工作流程涉及用于准备输入(镶嵌图像和投影矩阵)的MATLAB工具被摄取到3DPD匹配核心软件中。管道在持续的发展中,常规摄取了Cassis目前获取的大量图像,并将继续在未来获取。 Cassis 3DPD产品是如今可用的独特DTMS,在某些科学工作中被考虑了立体产品(如第6.2节所述)。相同的管道面临着汞全球映射的专用管道,利用汞行星轨道(MPO)Bepicolombo综合观察系统(Simbio-sys)(Simbio-sys,2020)的光谱仪和成像者。

著录项

获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号