Radar sensing of the sea surface using small spacecraft

Igor Kartsan, A. Zhukov
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引用次数: 4

Abstract

The possibility of using a constellation of small spacecraft as receiving satellites, when “highlighting” the sea surface from existing (navigational, communication) or specially created spacecraft—to form a wide-area (about 1 000 km) radar survey zone at a given resolution (about 10 m)—is under consideration. Such a constellation could provide operational monitoring of fast-moving atmospheric cyclones, measuring directly the parameters of storm waves (altitude and orbital velocity)—which would replace the existing constellation of microwave scatterometers, providing operational monitoring of the World Ocean surface in the 3 H (H—altitude of the satellite’s orbit) field of view with a resolution of about 10 km—but with calibration of the received images by wind speed and direction, which leads to huge errors when trying to introduce altitude calibration in the Small spacecraft have many advantages over large satellites. For example, they are relatively inexpensive to build, take minimal time from design to launch, are easily modified to solve a specific problem, and create less radio interference. The approach under consideration consists in redistribution of tasks to be solved between the constellation of satellites in orbit. High orbiting navigation satellites, for example, can be used as transmitter carriers (of the illumination of the surface) that use the necessary broadband signal with acceptable periodicity. Receivers of reflected signals are placed on board small spacecraft, and at formation of wide-band radar image of sea surface with necessary resolution ∼10 m (that only on order exceeds acceptable on small spacecraft size of receiving antennas)—in flight direction is necessary to use synthesized aperture of receiving antenna. This work has the character of “staged” research.
用小型航天器对海面进行雷达探测
目前正在考虑使用一组小型航天器作为接收卫星的可能性,当现有(导航、通信)或专门制造的航天器“高亮”海面时,以给定的分辨率(约10米)形成一个广域(约1000公里)的雷达测量区。这样一个星座可以提供对快速移动的大气气旋的操作监测,直接测量风暴波的参数(高度和轨道速度)——它将取代现有的微波散射仪星座,提供对世界海洋表面3h(卫星轨道的H高度)视场的操作监测,分辨率约为10公里——但需要根据风速和风向对接收到的图像进行校准。在尝试引入高度校准时,会导致巨大的误差。小型航天器比大型卫星有许多优点。例如,它们的制造成本相对较低,从设计到发射的时间最短,很容易修改以解决特定问题,并且产生较少的无线电干扰。正在考虑的办法是在轨道上的卫星群之间重新分配待解决的任务。例如,高轨道导航卫星可以用作(地表照明的)发射机载体,它使用具有可接受周期性的必要宽带信号。反射信号的接收器放置在小型航天器上,在形成必要分辨率的海面宽带雷达图像时(只有在接收天线尺寸较小的航天器上才超过可接受的分辨率),在飞行方向上需要使用接收天线的合成孔径。这项工作具有“阶段性”研究的特点。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
CiteScore
0.90
自引率
0.00%
发文量
2
审稿时长
8 weeks
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