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基于卷积曲面的动态实时星图模拟

闫劲云 刘慧 赵伟强 江洁

闫劲云, 刘慧, 赵伟强, 等 . 基于卷积曲面的动态实时星图模拟[J]. 北京航空航天大学学报, 2019, 45(4): 681-686. doi: 10.13700/j.bh.1001-5965.2018.0425
引用本文: 闫劲云, 刘慧, 赵伟强, 等 . 基于卷积曲面的动态实时星图模拟[J]. 北京航空航天大学学报, 2019, 45(4): 681-686. doi: 10.13700/j.bh.1001-5965.2018.0425
YAN Jinyun, LIU Hui, ZHAO Weiqiang, et al. Dynamic real-time star map simulation based on convolution surface[J]. Journal of Beijing University of Aeronautics and Astronautics, 2019, 45(4): 681-686. doi: 10.13700/j.bh.1001-5965.2018.0425(in Chinese)
Citation: YAN Jinyun, LIU Hui, ZHAO Weiqiang, et al. Dynamic real-time star map simulation based on convolution surface[J]. Journal of Beijing University of Aeronautics and Astronautics, 2019, 45(4): 681-686. doi: 10.13700/j.bh.1001-5965.2018.0425(in Chinese)

基于卷积曲面的动态实时星图模拟

doi: 10.13700/j.bh.1001-5965.2018.0425
基金项目: 

国家自然科学基金 61505191

国家自然科学基金 61725501

质量技术监督能力提升专项 ANL1805

详细信息
    作者简介:

    闫劲云 男, 博士, 助理研究员。主要研究方向:星敏感器技术、光度计量

    江洁 女, 博士, 教授, 博士生导师。主要研究方向:星敏感器技术、图像处理

    通讯作者:

    江洁, E-mail: jiangjie@buaa.edu.cn

  • 中图分类号: V448.25

Dynamic real-time star map simulation based on convolution surface

Funds: 

National Natural Science Foundation of China 61505191

National Natural Science Foundation of China 61725501

Project for Improvement of Quality and Technical Supervision Capacity ANL1805

More Information
  • 摘要:

    多星模拟器可动态刷新显示变化的星空,是星敏感器测试的关键设备。在动态条件下星点成像发生拖尾,要求星模拟器能够准确、实时仿真拖尾星图。建立了动态拖尾星点的卷积曲面模型。该模型是星点光斑弥散函数与权重函数沿着星点运动轨迹的卷积,可描述以任意形式运动产生的拖尾星点。提出了一种基于卷积曲面的像素离散算法,解决了星图仿真实时性不够的问题。先将星点轨迹分割为多段,再计算得到每段轨迹对应形成的星点光斑的像素值,将所有星点光斑累加。所提算法将多重积分化简,使得仿真速度提高了一个数量级,多星模拟器的刷新率达30 Hz。

     

  • 图 1  拖尾星点光斑成像过程

    Figure 1.  Imaging process of smeared star spot

    图 2  拖尾星点光斑仿真精度对比

    Figure 2.  Simulation accuracy comparison of smeared star spots

    图 3  不同算法仿真耗时直方图

    Figure 3.  Histogram of simulation time consumption for different algorithm

    图 4  星图仿真耗时与星图中星点数量的关系

    Figure 4.  Star map simulation time consumption vs. star number of star image

    图 5  剔除暗星后仿真耗时直方图

    Figure 5.  Histogram of simulation time consumption after dark star is excluded

    表  1  不同划分间隔下的星点灰度误差

    Table  1.   Star grayscale error under different steps

    划分间隔/像素 0.02 0.05 0.10 0.20
    最大灰度误差 0.005 3 0.012 9 0.026 0 0.052 5
    灰度RMS误差 0.001 1 0.002 7 0.005 4 0.010 9
    下载: 导出CSV
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出版历程
  • 收稿日期:  2018-07-13
  • 录用日期:  2018-10-15
  • 网络出版日期:  2019-04-20

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