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Mapping Mars: Geodetic and cartographic aspects

机译:火星测绘:大地测量和制图方面

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This paper presents a review of geodetic and cartographic aspects involved in the mapping of Mars and in the handling of planetary data returned and available from different team missions. It focuses on the reference system adopted for the planet, the main coordinate systems being used and main projection systems adopted when representing the data in a map. Several returned data are available in two different coordinate systems, the planetographic and the planetocentric. Errors in latitude and longitude when taking one system for another are addressed and quantified. As an example, the difference between planetographic and planetocentric latitudes can reach up to similar to 0.35 degrees. Errors involving equirectangular, sinusoidal and stereographic map projections, which are among the most common projections used to represent Mars data, are studied. Angular, linear and areal distortions are calculated for all three projections and the results are discussed. For the given examples, the maximum angular distortion and the distortion along parallels for a typical HiRISE image were similar to 0.6 degrees and similar to 1.009, respectively. For the MOC image used in the examples, the maximum angular distortion and the distortion along meridians were similar to 0.02 degrees and similar to 1.00000005, respectively. And for the stereographic projection the distortion along meridians was similar to 1.049150. (C) 2014 Elsevier Ltd. All rights reserved.
机译:本文介绍了与火星测绘有关的大地测量学和制图学方面的情况,并涉及了从不同团队任务获得并返回的行星数据的处理方法。它着重于为行星表示的参考系统,在地图中表示数据时使用的主要坐标系和主要的投影系统。在两个不同的坐标系中,可以得到几个返回的数据,这两个坐标系是行星学的和平面中心的。解决和量化将一个系统用于另一个系统时的经度和纬度误差。举例来说,行星和纬向平面的纬度之差可以达到约0.35度。研究了涉及等角,正弦和立体地图投影的误差,这些误差是用来表示火星数据的最常见投影。计算所有三个投影的角,线性和面畸变,并对结果进行讨论。对于给定的示例,典型的HiRISE图像的最大角度失真和沿平行方向的失真分别类似于0.6度和1.009。对于示例中使用的MOC图像,最大角度变形和沿子午线的变形分别类似于0.02度和1.00000005。对于立体投影,沿子午线的变形类似于1.049150。 (C)2014 Elsevier Ltd.保留所有权利。

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