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33条,第1-10条 帮助

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Interpretable data-driven chemometric approach for predicting non-optically active water quality parameters using ultraviolet-visible-near infrared absorption spectroscopy and physical-chemical measurements 期刊论文  OAI收割
SPECTROCHIMICA ACTA PART A-MOLECULAR AND BIOMOLECULAR SPECTROSCOPY, 2025, 卷号: 331, 页码: 125768
作者:  
Zhao, Yubo;  Zhang, Zhou;  Hu, Bingliang;  Liu, Jiacheng;  Wang, Xueji
  |  收藏  |  浏览/下载:5/0  |  提交时间:2025/03/18
A GSD-driven approach to deriving stochastic soil strength parameters under hybrid machine learning models 期刊论文  OAI收割
EUROPEAN JOURNAL OF SOIL SCIENCE, 2024, 卷号: 75, 期号: 6, 页码: 18
作者:  
Jiang, Hu;  Li, Yong;  Zou, Qiang;  Zhang, Jun;  Cui, Junfang
  |  收藏  |  浏览/下载:4/0  |  提交时间:2025/01/15
X-ray emission of contact binary variables within 1 kpc 期刊论文  OAI收割
Astronomy & Astrophysics, 2022, 卷号: 663, 页码: A115
作者:  
(1)Department of Astronomy, Xiamen University, Xiamen, Fujian 361005, PR China;  (2)Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang 830011, PR China;  (3)University of Chinese Academy of Sciences, Beijing 100049, PR China
  |  收藏  |  浏览/下载:17/0  |  提交时间:2023/06/19
Optimization of the Physical and Mechanical Properties of Grouting Material for Non-Soil-Squeezing PHC Pipe Pile 期刊论文  OAI收割
CRYSTALS, 2022, 卷号: 12, 期号: 1, 页码: 21
作者:  
Hou, Zhenkun;  Tang, Mengxiong;  Liang, Shihua;  Zhu, Yi
  |  收藏  |  浏览/下载:31/0  |  提交时间:2022/04/11
Analysis of lithium-ion battery thermal models inaccuracy caused by physical properties uncertainty 期刊论文  OAI收割
APPLIED THERMAL ENGINEERING, 2021, 卷号: 198, 页码: 13
作者:  
Dong, Ti;  Wang, Yiwei;  Cao, Wenjiong;  Zhang, Weijiang;  Jiang, Fangming
  |  收藏  |  浏览/下载:88/0  |  提交时间:2021/11/01
Photometric Study and Absolute Parameter Estimation of Six Totally Eclipsing Contact Binaries 期刊论文  OAI收割
Astronomical Journal, 2021, 卷号: 162, 期号: 1, 页码: 13
作者:  
Li, Kai;  Xia, Qi-Qi;  Kim, Chun-Hwey;  Gao, Xing;  Hu, Shao-Ming
  |  收藏  |  浏览/下载:28/0  |  提交时间:2022/06/30
Influence of non-ideal gas characteristics on working fluid properties and thermal cycle of space nuclear power generation system 期刊论文  OAI收割
ENERGY, 2021, 卷号: 222
作者:  
Xu, Chi;  Kong, Fanli;  Yu, Dali;  Yu, Jie;  Khan, Muhammad Salman
  |  收藏  |  浏览/下载:33/0  |  提交时间:2021/05/06
A full-disk image standardization of the chromosphere observation at Huairou Solar Observing Station 期刊论文  OAI收割
ADVANCES IN SPACE RESEARCH, 2020, 卷号: 65, 期号: 3, 页码: 1054-1061
作者:  
Suo, Liu
  |  收藏  |  浏览/下载:12/0  |  提交时间:2021/09/26
Lunar surface potential and electric field 期刊论文  OAI收割
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2019, 卷号: 19, 期号: 6, 页码: 77
作者:  
Li, Lei;  Lhang, Yi-Teng;  Zhou, Bin;  Feng, Yong-Yong
  |  收藏  |  浏览/下载:55/0  |  提交时间:2019/07/10
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:76/0  |  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.