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Adaptive Slicing Method of the Spatiotemporal Event Stream Obtained from a Dynamic Vision Sensor 期刊论文
Sensors, 2022, 卷号: 22, 期号: 7, 页码: 20
作者:  Y. S. Zhang;  Y. C. Zhao;  H. Y. Lv;  Y. Feng;  H. L. Liu and C. S. Han
收藏  |  浏览/下载:0/0  |  提交时间:2023/06/14
The Effect of Compressible Flow on Heat Transfer Performance of Heat Exchanger by Computational Fluid Dynamics (CFD) Simulation 期刊论文
Entropy, 2019, 卷号: 21, 期号: 9, 页码: 12
作者:  C.Yu;  S.C.Qin;  B.S.Chai;  S.Huang;  Y.Liu
收藏  |  浏览/下载:1/0  |  提交时间:2020/08/24
Detection of P2P botnet based on network behavior features and Dezert-Smarandache theory 期刊论文
Journal of Southeast University (English Edition), 2018, 卷号: 34, 期号: 2, 页码: 191-198
作者:  Song, Yuanzhang;  Chen, Yuan;  Wang, Junjie;  Wang, Anbang;  Li, Hongyu
收藏  |  浏览/下载:12/0  |  提交时间:2019/09/17
基于局部视觉特征的图像质量客观评价方法研究 学位论文
博士: 中国科学院大学, 2015
作者:  卢彦飞
收藏  |  浏览/下载:145/0  |  提交时间:2015/11/30
An improved two-dimensional entropy method for star trail tracing in deep sky (EI CONFERENCE) 会议论文
ICO20: Optical Information Processing, August 21, 2005 - August 26, 2005, Changchun, China
Yao Z.-J.; Wang Y.-J.; Han Q.-L.
收藏  |  浏览/下载:15/0  |  提交时间:2013/03/25
The trace of star trail is an important component of deep sky detection. The stars are low contrast targets  and their self-rotation will make their brightness change in cycle. Above all  the trail trace is vulnerable to the block and disturbance of other stars. Traditional one-dimensional maximum entropy thresholding algorithm is vulnerable to the noise  and the calculation of two-dimensional entropy methods is too large and takes too much time. This paper proposes an improved two-dimensional entropy threshold algorithm. We use recursion iteration method to eliminate the redundancy calculation  and reduce the size of two-dimensional histogram based on the deep sky stars characteristic  such as low contrast  fuzziness and the centralized histogram. We also combine our algorithm with the space trail trace model to forecast the star trace. Experiments results show  when the star are blocked or they turn dark  the method still can well extrapolate the star trace. Our method improves the capability of trailing the ebb and small star  and increases the precision of tracing. It is also robust to the noise  so there is a good application foreground for the method.  


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