中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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Bi-STAN: bilinear spatial-temporal attention network for wearable human activity recognition 期刊论文  OAI收割
INTERNATIONAL JOURNAL OF MACHINE LEARNING AND CYBERNETICS, 2023, 页码: 17
作者:  
Gao, Chenlong;  Chen, Yiqiang;  Jiang, Xinlong;  Hu, Lisha;  Zhao, Zhicheng
  |  收藏  |  浏览/下载:19/0  |  提交时间:2023/07/12
Online Similarity Learning for Big Data with Overfitting 期刊论文  OAI收割
IEEE Transactions on Big Data, 2018, 卷号: 4, 期号: 1, 页码: 78-89
作者:  
Fan BJ(范保杰);  Zeng P(曾鹏);  Yu HB(于海斌);  Luo JB(罗杰波);  Cong Y(丛杨)
  |  收藏  |  浏览/下载:43/0  |  提交时间:2017/12/21
adaptive voice stream multicast over low-power wireless networks 会议论文  OAI收割
31st IEEE Real-Time Systems Symposium, RTSS 2010, San Diego, CA, 40850
Liqun Li; Guoliang Xing; Qi Han; Limin Sun
收藏  |  浏览/下载:21/0  |  提交时间:2011/03/31
An improved two-dimensional entropy method for star trail tracing in deep sky (EI CONFERENCE) 会议论文  OAI收割
ICO20: Optical Information Processing, August 21, 2005 - August 26, 2005, Changchun, China
作者:  
Wang Y.-J.;  Yao Z.-J.
收藏  |  浏览/下载:30/0  |  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.