这些影像输入计算机后，通过一种天文分析算法—改进式均匀冗余阵列（MURA, modified uniformly redundant array）整合生成一个三维的图像。
These different perspectives are then combined to form into a three-dimensional image by a computer using a trick from astronomical analysis known as MURA (modified uniformly redundant array).
由于航天实验费用大，为测试星敏感器性能和星图识别算法，需在地面构建天文导航半物理仿真试验平台。
Because of high spaceflight laboratory fees, it is impractical to take star-pictures real time in order to debug star sensor and test the algorithm of star map identification.
贝尔说：“从天文上讲，根本没有任何变化，有变化的只是在人类的算法上。”
"It's nothing astronomical changing. What's changing is the human side of it," Bell said.
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