首页> 外文OA文献 >Calibrating mars orbiter laser altimeter pulse widths at mars science laboratory candidate landing sites
【2h】

Calibrating mars orbiter laser altimeter pulse widths at mars science laboratory candidate landing sites

机译:在火星科学实验室候选着陆点校准火星轨道激光高度计脉冲宽度

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。

摘要

Accurate estimates of surface roughness allow quantitative comparisons between planetary terrains. These comparisons enable us to improve our understanding of commonly occurring surface processes, and develop a more complete analysis of candidate landing and roving sites. A (secondary) science goal of the Mars Orbiter Laser Altimeter was to map surface roughness within the laser footprint using the backscatter pulse-widths of individual pulses, at finer scales than can be derived from the elevation profiles. On arrival at the surface, these pulses are thought to have diverged to between 70 and 170 m, corresponding to surface roughness estimates at 35 and 70 m baselines respectively; however, the true baseline and relationship remains unknown. This work compares the Mars Orbiter Laser Altimeter pulse-widths to surface roughness estimates at various baselines from high-resolution digital terrain models at the final four candidate landing sites of Mars Science Laboratory. The objective was to determine the true baseline at which surface roughness can be estimated, and the relationship between surface roughness and the pulse-widths, to improve the reliability of current global surface roughness estimates from pulse-width maps. The results seem to indicate that pulse-widths from individual shots are an unreliable indicator of surface roughness, and instead, the pulse-widths should be downsampled to indicate regional roughness, with the Slope-Corrected pulse-width dataset performing best. Where Rough Patches are spatially large compared to the footprint of the pulse, pulse-widths can be used as an indicator of surface roughness at baselines of 150 to 300 m; where these patches are spatially small, as observed at Mawrth Vallis, pulse-widths show no correlation to surface roughness. This suggests that a more complex relationship exists, with varying correlations observed, which appear dependent on the distribution of roughness across the sites.
机译:对表面粗糙度的准确估计可以对行星地形之间进行定量比较。这些比较使我们能够加深对常见表面过程的理解,并对候选着陆点和流动点进行更完整的分析。 Mars Orbiter激光测高仪的一个(次要)科学目标是使用单个脉冲的反向散射脉冲宽度以比从高程分布图得出的更精细的比例绘制激光足迹内的表面粗糙度。在到达地面时,这些脉冲被认为发散在70至170 m之间,分别对应于基准线35和70 m处的表面粗糙度估计值。但是,真正的基线和关系仍然未知。这项工作将火星科学实验室的最后四个候选着陆点的高分辨率数字地形模型中的火星轨道激光测高仪脉冲宽度与表面粗糙度估算值进行了比较。目的是确定可估计表面粗糙度的真实基线,以及表面粗糙度和脉冲宽度之间的关系,以提高从脉冲宽度图进行的当前全局表面粗糙度估计的可靠性。结果似乎表明来自单个镜头的脉冲宽度是表面粗糙度的不可靠指标,而应该对脉冲宽度进行下采样以指示区域粗糙度,其中“斜率校正的脉冲宽度”数据集表现最佳。与脉冲足迹相比,粗糙斑块在空间上较大,可以将脉冲宽度用作基线在150至300 m处的表面粗糙度的指标。如Mawrth Vallis所观察到的,这些斑块的空间很小,脉冲宽度与表面粗糙度无关。这表明存在更复杂的关系,并观察到各种相关性,这些相关性似乎取决于整个站点的粗糙度分布。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
代理获取

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号