Final Report of the Haystack Orbital Debris Data Review Panel
Final Report of the Haystack Orbital Debris Data Review Panel
复制标题
海斯塔克轨道碎片数据审查小组的最终报告
DOI：
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发表时间：
1998
期刊：
影响因子：
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通讯作者：
M. Tuley
中科院分区：
文献类型：
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作者：
D. K. Barton;D. Brillinger;A. El;P. McDaniel;K. Pollock;M. Tuley
1996年12月设立了Haystack轨道碎片数据审查小组，以审议过去几年利用Haystack雷达收集的轨道碎片数据是否充分，以及用于估计这些碎片通量与大小关系的方法是否准确。小组讨论的四个具体问题是：相对于感兴趣的估计总体的观测数2.测量的雷达截面（RCS）和物体3的推断的物理尺寸之间的固有模糊性。观察每个物体时固有的视角限制及其与物体几何形状的关系4.样本数据集是否足以确定碎片群的潜在几何特征。本报告讨论了对这些问题的进一步讨论和解释，并确定了促成这些问题的详细问题。
The Haystack Orbital Debris Data Review Panel was established in December 1996 to consider the adequacy of the data on orbital debris gathered over the past several years with the Haystack radar, and the accuracy of the methods used to estimate the flux vs. size relationship for this debris. The four specific issues addressed for the Panel were: 1. The number of observations relative to the estimated population of interest 2. The inherent ambiguity between the measured radar cross section (RCS) and the inferred physical size of the object 3. The inherent aspect angle limitation in viewing each object and its relationship to object geometry 4. The adequacy of the sample data set to characterize the debris population's potential geometry. Further discussion and interpretation of these issues, and identification of the detailed questions contributing to them, are discussed in this report.