附录A:使用多个传感器进行地面观测

C. Elachi, J. V. Zyl
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引用次数: 0

摘要

对行星表面或大气的详细研究需要同时使用覆盖大部分电磁波谱的多个传感器。这是由于任何单个传感器只覆盖频谱的一小部分,其中波-物质相互作用机制是由有限数量的介质特性驱动的。例如,对于固体表面,x射线传感器提供放射性物质含量的信息,可见光和近红外传感器提供表面化学成分的信息,热红外传感器测量近表面热性能,雷达传感器主要对表面物理性能(地形、粗糙度、湿度和介电常数)敏感。同样,在大气的情况下,为了覆盖范围广泛的可能的化学成分,探测和表征大气颗粒(包括雨),并探测大气的物理特性,将需要一套覆盖可见光、红外、毫米和微波光谱区域选定波段的传感器。为了说明如何共同使用多个传感器来提高解释器在研究行星表面时的能力,本文介绍了一组覆盖加州东部死亡谷地区的数据产品。图A.1显示了用三种不同仪器在可见光/近红外(图A.1a)、热红外(图A.1b)和雷达(图A.1c)光谱波段拍摄的三幅死亡谷图像。利用地形数据库,可以生成虚假照明图像来突出地表地形(图A.2)。然后,该地形数据库可以与多光谱图像数据(图a .1)共同注册,并用于从各种观测方向生成透视图像,如图a .3和a .4所示。观测方向、垂直夸张、光谱带和颜色编码可以由解释器选择并立即显示在监视器上。这实际上相当于将研究地点带入实验室进行详细的“解剖”和分析。当然,总是需要进行直接地表观测的实地工作,但上述数据库将在发展对地表性质的基本理解方面发挥很大作用。507
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Appendix A: Use of Multiple Sensors for Surface Observations
The detailed study of a planetary surface or atmosphere requires the simultaneous use of multiple sensors covering a large part of the electromagnetic spectrum. This is a result of the fact that any individual sensor covers only a small part of the spectrum in which the wave–matter interaction mechanisms are driven by a limited number of the medium properties. For example, in the case of solid surfaces, x-ray sensors provide information on the content of radioactive materials, visible and near-infrared sensors provide information about the surface chemical composition, thermal infrared sensors measure the near-surface thermal properties, and radar sensors are mainly sensitive to the surface physical properties (topography, roughness, moisture, and dielectric constant). Similarly, in the case of the atmosphere, in order to cover the wide range of possible chemical constituents, detect and characterize atmospheric particles (including rain), and sound the physical properties of the atmosphere, a suite of sensors covering selected bands in the visible, infrared, millimeter, and microwave spectral regions will be needed. To illustrate howmultiple sensors can be used collectively to enhance the ability of an interpreter in the study of a planetary surface, a set of data products covering the area of Death Valley in eastern California are presented. Figure A.1 shows three images of Death Valley acquired with three separate instruments in the visible/near IR (Figure A.1a), thermal IR (Figure A.1b), and radar (Figure A.1c) spectral bands. With the topography database, false illumination images can be generated to highlight the surface topography (Fig. A.2). This topography database can then be coregistered to the multispectral image data (Fig. A.1) and used to generate perspective images from a variety of observing directions, as illustrated in Figures A.3 and A.4. The observing direction, the vertical exaggeration, the spectral bands, and the color coding can be selected by the interpreter and displayed on a monitor instantaneously. This will effectively be equivalent to bringing the study site into the laboratory for detailed “dissection” and analysis. Of course, there will always be the need to do field work for direct surface observation, but the above-described database will go a long way in developing a basic understanding of the surface properties. 507
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Appendix D: Compression of a Linear FM Chirp Signal Appendix A: Use of Multiple Sensors for Surface Observations Atmospheric Remote Sensing in the Microwave Region Nature and Properties of Electromagnetic Waves Appendix B: Summary of Orbital Mechanics Relevant to Remote Sensing
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