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长春光学精密机械与物... [5]
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期刊论文 [3]
会议论文 [1]
学位论文 [1]
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专题:长春光学精密机械与物理研究所
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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
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浏览/下载:0/0
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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
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浏览/下载:1/0
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提交时间:2020/08/24
water cooled charge air cooler (WCAC),compressible flow,computational,fluid dynamics (CFD),heat transfer,plate-fin,Physics
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
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  |  
浏览/下载:12/0
  |  
提交时间:2019/09/17
Peer to peer networks
Botnet
Entropy
Feature extraction
Kalman filters
Network protocols
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
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浏览/下载:145/0
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提交时间:2015/11/30
人类视觉系统
局部信息失真
Riesz变换
韦伯定律
差异激励
视觉显著性
单演相位一致性
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.
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浏览/下载:15/0
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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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