昨天和今天的地球感应能力

P. Razzhivalov, N. Korobova, S. Shatalova
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引用次数: 0

摘要

目前,地球遥感卫星轨道星座的扩容仍在继续。成像设备的技术特性正在不断改进。本文讨论了地球遥感数据引用不准确的主要原因,即轨道参数测量误差和航天器方位误差。已经确定的是,glonass / GPS系统是造成第一个错误的原因,而确定恒星坐标的设备(由恒星定位的传感器)是造成第二个错误的原因。分析了世界知名公司的现代航天器恒星坐标测定装置的特点。已经确定,在图像的几何校正中必须考虑这些系统和设备的测量结果。已查明与这些装置的研制、生产和性能控制试验阶段有关的问题。这些问题的解决将使为地球遥感航天器配备星敏感器成为可能,星敏感器与成像设备一起工作,将能够提供所需的图像特征,其空间分辨率小于40-50厘米,空间参考精度为2-3米。确定恒星坐标的测量装置的精度直接影响到地球遥感图像绑定的精度。研究发现,俄罗斯科学院空间研究所的传感器精度特性在1弧秒范围内。最大可达2弧秒。造成误差的主要原因是借助确定恒星坐标的设备进行的测量的标准偏差(随机误差)。关键词:遥感,星敏感器,误差,定位。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Earth sensing capabilities yesterday and today
At present, the expansion of the orbital constellation of Earth remote sensing satellites continues. Thetechnical characteristics of the imaging equipment are being improved. The article discusses the mainreasons for the inaccurate referencing of Earth remote sensing data, namely, the errors in measuring theparameters of the orbit and the error in the orientation of the spacecraft. It has been established that theGlonass / GPS systems are responsible for the first error, and the devices for determining the coordinatesof stars (orientation sensors by stars) are responsible for the second. The analysis of the modern devicescharacteristics for determining the stars coordinates of spacecraft from well-known world companies hasbeen carried out.It has been established that the results of measurements of these systems and devices must be taken intoaccount in the geometric correction of images. The problems associated with the stages of development,production and control tests of the performance of these devices have been identified. The solution of theseproblems will make it possible to equip spacecraft for remote sensing of the Earth with star sensors, which,working in conjunction with imaging equipment, will be able to provide the required characteristics of theimages obtained with a spatial resolution of less than 40-50 cm and a spatial reference accuracy of 2-3 m.The accuracy of devices measurement for determining the coordinates of stars affects the accuracy of theimages binding of Earth remote sensing. It was found that the accuracy sensor characteristics of the SpaceResearch Institute of Russian Academy of Sciences are in the range from 1 arc.sec. up to 2 arc.sec. Themain contribution to the error is made by the standard deviation of measurements carried out with the helpof devices for determining the coordinates of the stars (random error). Key words: remote sensing, star sensor, error, orientation.
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