中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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浏览/检索结果: 共34条,第1-10条 帮助

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Antisaturation Finite-Time Attitude Tracking Control Based Observer for a Quadrotor 期刊论文  OAI收割
IEEE TRANSACTIONS ON CIRCUITS AND SYSTEMS II-EXPRESS BRIEFS, 2021, 卷号: 68
作者:  
Liu, Kang;  Wang, Xingxian;  Wang, Rujing;  Sun, Guowei;  Wang, Xiaodong
  |  收藏  |  浏览/下载:46/0  |  提交时间:2021/08/31
The features and mechanisms of the North Shandong Coastal Current: a case study in 2014 期刊论文  OAI收割
JOURNAL OF OCEANOGRAPHY, 2021, 页码: 16
作者:  
Zheng, Xiangyang;  Zhang, Hua;  Li, Yanfang;  Zou, Tao;  Liu, Xin
  |  收藏  |  浏览/下载:24/0  |  提交时间:2021/06/07
A nonlinear model for aerodynamic configuration of wake behind horizontal-axis wind turbine 期刊论文  OAI收割
APPLIED MATHEMATICS AND MECHANICS-ENGLISH EDITION, 2019, 卷号: 40, 期号: 9, 页码: 1313-1326
作者:  
Li DS;  Guo T;  Li RN;  Yang CX;  Cheng ZX
  |  收藏  |  浏览/下载:59/0  |  提交时间:2019/10/21
Wind velocity distribution reconstruction using CFD database with Tucker decomposition and sensor measurement 期刊论文  OAI收割
ENERGY, 2019, 卷号: 167, 页码: 1236-1250
作者:  
Qin L;  Liu S;  Kang Y;  Yan SA;  Schlaberg HI
  |  收藏  |  浏览/下载:70/0  |  提交时间:2019/01/09
Analysis on Wind Resistance Index of Multi-rotor UAV 会议论文  OAI收割
Nanchang, China, June 3-5, 2019
作者:  
Hou YQ(侯永强);  Huang W(黄微);  Zhou H(周浩);  Gu F(谷丰);  Chang YC(常彦春)
  |  收藏  |  浏览/下载:13/0  |  提交时间:2019/11/13
Interaction between the atmospheric boundary layer and a standalone wind turbine in Gansu-Part I: Field measurement 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2018, 卷号: 61, 期号: 9, 页码: 94711
作者:  
  |  收藏  |  浏览/下载:42/0  |  提交时间:2018/10/30
EFDC模型在不同水体类型中的应用研究 学位论文  OAI收割
北京: 中国科学院生态环境研究中心, 2018
作者:  
陈晓枫
  |  收藏  |  浏览/下载:238/0  |  提交时间:2019/06/27
A New Set of Parameters of High-Mass X-ray Binaries Found with their Cyclotron Lines 期刊论文  OAI收割
arXiv e-prints, 2018
作者:  
Zhang, Chengmin;  Taani, Ali;  Chaty, Sylvain;  Karino, Shigeyuki;  Song, Liming
  |  收藏  |  浏览/下载:75/0  |  提交时间:2019/07/12
Astrophysics - High Energy Astrophysical Phenomena  Abstract: We have derived new physical quantities for several High-Mass X-ray Binaries (HMXBs) with supergiant (SG) companions through their cyclotron lines. The parameters are: the terminal velocity of the wind, the mass loss rate of the donor, the effective temperature and the magnetic fields. These parameters influence significantly the improvement of the model of accretion. In spite of the variety of their observational properties, the corresponding magnetic field is around B ~ 10^12 G. This result can be constrained by the effects on stellar evolution. In addition, we have performed a segmentation in the parameter space of donors intended for several SG-HMXB listed in our sample set. The parameter space can be categorized into five regimes depending on the possibility of disk formation associated with accretion from the stellar wind. This can give a quantitative clarification of the observed variability and the properties of these objects. We show that, when these systems come into the direct accretion region, systems with corresponding parameters can emit X-rays.  
Simulation research and theoretical study on measurement of atmospheric optical turbulence and wind profile using the correlation of gradient-tilt 期刊论文  OAI收割
ACTA PHYSICA SINICA, 2017, 卷号: 66, 期号: 10
作者:  
Peng Zhe;  Jing Xu;  Hou Zai-Hong;  Wu Yi
收藏  |  浏览/下载:30/0  |  提交时间:2018/07/27