大气湍流相位屏数字孪生模型
Pengjia
这是大气湍流相位屏数字孪生模型的示例代码，该代码权重及相位屏尺度被锁死，最大可生成128*128像素500副相位屏，可以为各类算法测试提供参考。深度定制的相位屏模拟代码（包括可变r0 L0和boiling effect），以及其他介质内的光波相位扰动可以联系论文作者贾鹏（邮箱robinmartin@126.com或robinmartin20@gmail.com）。
文件
IFATS_code.zip
285.53 MB
论文信息
论文标题:
Digital Twin of Atmospheric Turbulence Phase Screens Based On Deep Neural Networks
发表期刊:
Optics Express
标识符
CSTR:
11379.11.101110
DOI:
10.12149/101110
VO Identifier:
ivo://China-VO/paperdata/OE/jiapeng2022/101110
发布时间:
2022-05-24
使用统计
总下载量
421
引用
Pengjia et al. 2022. Code for Digital Twin of Atmospheric Turbulence Phase Screens Based On Deep Neural Networks. 版本 1.0. https://doi.org/10.12149/101110
@misc{10.12149/101110,
doi = {10.12149/101110},
url = {https://doi.org/10.12149/101110},
author = {Pengjia},
title = {Code for Digital Twin of Atmospheric Turbulence Phase Screens Based On Deep Neural Networks},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
doi = {10.12149/101110},
url = {https://doi.org/10.12149/101110},
author = {Pengjia},
title = {Code for Digital Twin of Atmospheric Turbulence Phase Screens Based On Deep Neural Networks},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
版本