2013年4月成功发射的GF-1卫星是中国高分系列卫星的首发星,影像在中国农情遥感监测业务中得到了广泛应用,已成为大宗农作物种植面积遥感监测的主要数据源之一。高精度几何位置的配准是卫星农情定量化应用的基础与前提,该文提出了一种基...2013年4月成功发射的GF-1卫星是中国高分系列卫星的首发星,影像在中国农情遥感监测业务中得到了广泛应用,已成为大宗农作物种植面积遥感监测的主要数据源之一。高精度几何位置的配准是卫星农情定量化应用的基础与前提,该文提出了一种基于区域网平差方法修正GF-1卫星WFV(wide field view,WFV)影像RPC(rational polynomial coefficients,RPC)参数,获取更高几何定位精度的校正方法,形成了模式化的业务处理流程,为该影像在农情遥感监测中的应用奠定了基础。算法流程包括2个部分,首先是基于像面间仿射变换关系及有理多项式RFM(rational function model,RFM)模型构建轨道间的区域网平差数学模型,其次是根据影像连接点及少量控制点输入求解所有参与平差的卫星影像定向参数,获取亚像元级的校正结果。平差参数的解算是通过两步求解完成的,初始平差参数是根据连接点及对应的DEM高程值进行平差迭代至收敛,结果平差参数是将初始平差参数作为初始值代入区域网平差模型,并以逐点消元方式约化法方程,解算出各影像的仿射变换参数。该文在求解平差参数过程中,直接使用DEM(digital elevation model)上获取的高程值作为约束条件,消除了平面坐标与高程的相关性,保证了区域网平差模型能够解算。混合地形、平原、山区3种情况下区域网平差结果表明,全连接点平差结果具有较高的相对定位精度,其行方向的中误差分别为0.3046、0.4674、0.3365像元,列方向的中误差分别为0.3677、0.2849、0.2889像元;而结合少量控制点的区域网平差则同时具有很高的绝对定位精度,其行方向的中误差分别为0.3648、0.5041、0.3605像元,列方向的中误差分别为0.4954、0.4039、0.6323像元,整体达到了亚像素级。最后,在农业应用基础控制底图的支持下,分别对原始影像、RPC校正影像、区域网平差后的影像进行几何配准,�展开更多
This paper completely introduces the basic idea of the EFP (Equivalent Frame Photo) aerial triangulation, EFP image point coordinate calculation and the function model of adjustment as well as the digital simulation o...This paper completely introduces the basic idea of the EFP (Equivalent Frame Photo) aerial triangulation, EFP image point coordinate calculation and the function model of adjustment as well as the digital simulation of the satellite photogrammetry. Then, the free framework + the control points adjustment, the adjustment with the observations of the exterior orientation element, detection the constant error of the observations of the exterior orientation element and the block adjustment are calculated and analysed using the simulated data. Through experiments and analysis, the conclusions are: The strip length of the three baselengths can be built up a stable model of the three-line array CCD image strip adjustment; The control points can be arranged on the start and the end of the strip. The elevation accuracy of the twofold area is lower about a factor of 1.4 than the threefold area; The observations of the exterior orientation element are the necessary data for the three-line array CCD image bundle adjustment. By the adjustment, the elevation accuracy can be improved in variant levels. Even if the accuracy of the observations of the exterior orientation elements are so high now, the elevation accuracy of the bundle adjustment is higher than the only forward intersection, so the three-line array CCD camera is more advantageous than single-line and double-line cameras in global satellite photogrammetry without control points or the exterior planet photogrammetry.展开更多
文摘2013年4月成功发射的GF-1卫星是中国高分系列卫星的首发星,影像在中国农情遥感监测业务中得到了广泛应用,已成为大宗农作物种植面积遥感监测的主要数据源之一。高精度几何位置的配准是卫星农情定量化应用的基础与前提,该文提出了一种基于区域网平差方法修正GF-1卫星WFV(wide field view,WFV)影像RPC(rational polynomial coefficients,RPC)参数,获取更高几何定位精度的校正方法,形成了模式化的业务处理流程,为该影像在农情遥感监测中的应用奠定了基础。算法流程包括2个部分,首先是基于像面间仿射变换关系及有理多项式RFM(rational function model,RFM)模型构建轨道间的区域网平差数学模型,其次是根据影像连接点及少量控制点输入求解所有参与平差的卫星影像定向参数,获取亚像元级的校正结果。平差参数的解算是通过两步求解完成的,初始平差参数是根据连接点及对应的DEM高程值进行平差迭代至收敛,结果平差参数是将初始平差参数作为初始值代入区域网平差模型,并以逐点消元方式约化法方程,解算出各影像的仿射变换参数。该文在求解平差参数过程中,直接使用DEM(digital elevation model)上获取的高程值作为约束条件,消除了平面坐标与高程的相关性,保证了区域网平差模型能够解算。混合地形、平原、山区3种情况下区域网平差结果表明,全连接点平差结果具有较高的相对定位精度,其行方向的中误差分别为0.3046、0.4674、0.3365像元,列方向的中误差分别为0.3677、0.2849、0.2889像元;而结合少量控制点的区域网平差则同时具有很高的绝对定位精度,其行方向的中误差分别为0.3648、0.5041、0.3605像元,列方向的中误差分别为0.4954、0.4039、0.6323像元,整体达到了亚像素级。最后,在农业应用基础控制底图的支持下,分别对原始影像、RPC校正影像、区域网平差后的影像进行几何配准,�
文摘This paper completely introduces the basic idea of the EFP (Equivalent Frame Photo) aerial triangulation, EFP image point coordinate calculation and the function model of adjustment as well as the digital simulation of the satellite photogrammetry. Then, the free framework + the control points adjustment, the adjustment with the observations of the exterior orientation element, detection the constant error of the observations of the exterior orientation element and the block adjustment are calculated and analysed using the simulated data. Through experiments and analysis, the conclusions are: The strip length of the three baselengths can be built up a stable model of the three-line array CCD image strip adjustment; The control points can be arranged on the start and the end of the strip. The elevation accuracy of the twofold area is lower about a factor of 1.4 than the threefold area; The observations of the exterior orientation element are the necessary data for the three-line array CCD image bundle adjustment. By the adjustment, the elevation accuracy can be improved in variant levels. Even if the accuracy of the observations of the exterior orientation elements are so high now, the elevation accuracy of the bundle adjustment is higher than the only forward intersection, so the three-line array CCD camera is more advantageous than single-line and double-line cameras in global satellite photogrammetry without control points or the exterior planet photogrammetry.
