Da Li , Yonghua Jiang , Jingyin Wang , Shaodong Wei , Guo Zhang , Huilong Wang
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引用次数: 0
Abstract
In Earth observation and planetary exploration missions, high-precision geolocation through remote sensing is crucial. However, dynamic systematic errors in satellite imagery and ancillary flight data, arising from sensor limitation and measurement technology, challenge traditional correction methods such as orientation image model and bias compensation model. This study proposes a piecewise bias matrix compensation method to improve the geolocation accuracy of linear pushbroom cameras by effectively eliminating dynamic systematic errors. The method focuses on detect orientation point exposure time utilizing the distribution characteristics of the reprojection residuals caused by dynamic system errors. This is accomplished through a stepwise strategy involving residual point cloud thinning and iterative end-point fitting algorithms, which automatically divide the sub-compensation model. Furthermore, considering the stability of the satellite’s flight attitude, a Lagrange interpolation method is introduced in the piecewise bias matrix compensation model, enhancing the internal consistency and absolute accuracy in the geometric positioning process of the optical linear pushbroom satellite. A comparison of the initial camera positioning results in the experimental dataset revealed that the reprojected errors of conjugate points in the MEX-HRSC can now achieve sub-pixel accuracy, with a maximum root mean square error of 0.54 pixels; the reprojected errors of GCPs in the XX-18 can now achieve sub-pixel accuracy, with a maximum root mean square error of 0.80 pixels. Additionally, building upon the elimination of dynamic systematic errors, this study constructs high spatial resolution DTMs of the Martian surface using high-resolution stereo imagery from the MEX-HRSC. These techniques and methods result in the intersection of corresponding rays in stereo pairs, which is crucial for subsequent 3D reconstruction.
期刊介绍:
Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered:
• Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics
• Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system
• Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating
• Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements
• Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation
• Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites
• Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind
• Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations
• Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets
• History of planetary and space research