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Lunar pole illumination and communications maps computed from GSSR elevation data

机译:根据GSSR高程数据计算出的月球照度和通讯图

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A Digital Elevation Model of the lunar south pole was produced using Goldstone Solar System RADAR (GSSR) data obtained in 2006.12 This model has 40-meter horizontal resolution and about 5-meter relative vertical accuracy [Ref 1]. This Digital Elevation Model was used to compute average solar illumination and Earth visibility with 100 km of the lunar south pole. The elevation data were converted into local terrain horizon masks, then converted into lunar-centric latitude and longitude coordinates. The horizon masks were compared to latitude, longitude regions bounding the maximum Sun and Earth motions relative to the moon. Estimates of Earth visibility were computed by integrating the area of the region bounding the Earth's motion that was below the horizon mask. Solar illumination and other metrics were computed similarly. Proposed lunar south pole base sites were examined in detail, with the best site showing yearly solar power availability of 92% and Direct-To-Earth (DTE) communication availability of about 50%. Similar analysis of the lunar south pole used an older GSSR Digital Elevation Model with 600-meter horizontal resolution. The paper also explores using a heliostat to reduce the photovoltaic power system mass and complexity.
机译:利用2006年获得的Goldstone太阳系雷达(GSSR)数据制作了月球南极数字高程模型。该模型的水平分辨率为40米,相对垂直精度为5米左右[参考文献1]。此数字高程模型用于计算月球南极100公里处的平均太阳照度和地球能见度。高程数据被转换为本地地形视线蒙版,然后转换为以月球为中心的纬度和经度坐标。将地平线蒙版与纬度,经度区域进行比较,纬度,经度区域限制了相对于月球的最大太阳和地球运动。地球能见度的估算是通过对视界蒙版下方地球运动边界区域的面积进行积分而得出的。太阳照度和其他指标的计算方法类似。详细研究了拟议的月球南极基地站点,最佳站点显示年度太阳能可用性为92%,对地(DTE)通信可用性约为50%。对月球南极的类似分析使用水平分辨率为600米的旧版GSSR数字高程模型。本文还探讨了使用定日镜降低光伏发电系统的质量和复杂性。

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  • 来源
    《IEEE Aerospace conference》|2009年|1-19|共19页
  • 会议地点 Big Sky MT(US)
  • 作者

    Bryant Scott;

  • 作者单位

    California Institute of Technology Jet Propulsion Laboratory 4800 Oak Grove Drive Pasadena 91109 USA;

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