检索结果-内蒙古大学图书馆

arXiv 2019年

作者： Nolan, M.C. Howell, E.S. Scheeres, D.J. McMahon, J.W. Golubov, O. Hergenrother, C.W. Emery, J.P. Noll, K.S. Chesley, S.R. Lauretta, D.S. Lunar and Planetary Laboratory University of Arizona TucsonAZ United States Department of Aerospace Engineering Sciences University of Colorado BoulderCO80309 United States V. N. Karazin Kharkiv National University 4 Svobody Sq. Kharkiv61022 Ukraine Earth and Planetary Science Department Planetary Geosciences Institute University of Tennessee KnoxvilleTN37996 United States NASA Goddard Space Flight Center Solar System Exploration Division GreenbeltMD20770 United States Jet Propulsion Laboratory California Institute of Technology 4800 Oak Grove Drive PasadenaCA91109 United States Institute of Astronomy of V. N. Karazin Kharkiv National University 35 Sumska Str. Kharkiv61022 Ukraine

We observed the near-Earth asteroid (101955) Bennu from the ground in 1999 and 2005, and with the Hubble space Telescope in 2012, to constrain its rotation rate. The data reveal an acceleration of 2.64 ± 1.05 ×10-6 deg day-2, which could be due to a change in the moment of inertia of Bennu or to spin up from the YORP effect or other source of angular momentum. The best solution is within 1 sigma of the period determined by Nolan et al. (2013). The OSIRIS-REx mission will determine the rotation state independently in 2019. Those measurements should show whether the change in rotation rate is a steady increase (due, for example, to the YORP effect) or some other phenomenon. The precise shape and surface properties measured by the OSIRIS-REx science team will allow for a better understanding of variations in rotation rate of small asteroids. Copyright © 2019, The Authors. All rights reserved.

关键词： Rotation rate

来源：评论

学校读者我要写书评

暂无评论

Wind-CHP generation aggregation with storage capability of district heating network

Wind-CHP generation aggregation with storage capability of d...

引用

2017 IEEE Conference on Energy Internet and Energy system Integration, EI2 2017

作者： Yu, Jing Shen, Xinwei Sheng, Tongtian Sun, Hongbin Xiong, Wen Tang, Lei Shenzhen Environmental Science and New Energy Technology Engineering Laboratory Tsinghua-Berkeley Shenzhen Institute Tsinghua University Shenzhen China State Key Lab of Control and Simulation of Power System and Generation Equipments Department of Electrical Engineering Tsinghua University Beijing China Guangzhou Power Grid Company Guangzhou China Beijing Qingda Gaoke System Control Company Beijing China

ISBN: (纸本)9781538614273

The strong coupling of electricity and heat of combined heat and power (CHP) unit in cold season results in the loss of flexibility, which may cause massive wind power curtailment if they are in the same system. This issue could be handled with the thermal storage capability of a district heating network (DHN) that could supply flexibility for CHP to decouple the strong coupling of heat and electric power supplies. In this paper, a wind-CHP generation aggregation(WCGA) model is formulated, which motivates CHP to increase wind power integration by increasing total profit of the system, while considering the additional flexibility supplied by DHN. In WCGA model, DHN is formulated as an energy-storage-like (ESL) model that considers the storage capability of DHN based on dynamic characteristics of temperature and time delay effect of DHN. The potential benefits of the proposed model have been demonstrated by case study in terms of enhancing, wind power integration as well as total profit. © 2017 IEEE.

关键词： District heating

来源：评论

学校读者我要写书评

暂无评论

Publisher Correction: Firn on ice sheets

引用

Nature Reviews Earth & Environment 2024年 330页

作者： Charles Amory Christo Buizert Sammie Buzzard Elizabeth Case Nicole Clerx Riley Culberg Rajashree Tri Datta Devon Dunmire Jan T. M. Lenaerts Megan Thompson-Munson Nander Wever Rahul Dey Reinhard Drews Falk M. Oraschewski Clare Eayrs Nicolaj Hansen Sebastian B. Simonsen Angelika Humbert Athul Kaitheri Kaitlin Keegan Ian McDowell Peter Kuipers Munneke Stef Lhermitte Sophie de Roda Husman Bert Wouters Doug Mair Jessica Mejia Colin R. Meyer Elizabeth Morris Dorothea Moser Elizabeth R. Thomas Emma Pearce Nicole-Jeanne Schlegel Timm Schultz C. Max Stevens Institut des Géosciences de l’Environnement University Grenoble Alpes CNRS Grenoble France College of Earth Ocean and Atmospheric Sciences Oregon State University Corvallis OR USA School of Earth and Environmental Sciences Cardiff University Cardiff UK Department of Geography and Environmental Sciences Northumbria University Newcastle upon Tyne UK Department of Earth and Environmental Sciences Columbia University NY USA Department of Geosciences Université de Fribourg Fribourg Switzerland Department of Earth and Atmospheric Sciences Cornell University Ithaca NY USA Department of Atmospheric and Oceanic Sciences University of Colorado Boulder Boulder CO USA Cooperative Institute for Research in Environmental Sciences (CIRES) University of Colorado Boulder Boulder CO USA WSL Institute for Snow and Avalanche Research SLF Davos Switzerland National Centre for Polar and Ocean Research (NCPOR) Ministry of Earth Sciences Vasco da Gama Goa India Department of Geosciences University of Tübingen Tübingen Germany Center for Global Sea Level Change New York University Abu Dhabi Abu Dhabi UAE Department of Glacial Environment Research Korea Polar Research Institute Incheon Republic of Korea Geodesy and Earth Observation DTU Space Technical University of Denmark Kongens Lyngby Denmark Danish Meteorological Institute Copenhagen Denmark Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research Bremerhaven Germany Faculty of Geosciences University of Bremen Bremen Germany Observatoire de la Côte d’Azur Université Côte d’Azur CNRS Valbonne France Department of Geological Sciences and Engineering University of Nevada Reno USA Graduate Program of Hydrologic Sciences University of Nevada Reno NV USA Institute for Marine and Atmospheric Research (IMAU) Utrecht University Utrecht The Netherlands Department of Earth and Environmental Sciences KU Leuven Leuven Belgium Department of Geoscience and Remote Sensing Delft University of Technology (TUDel

来源：评论

学校读者我要写书评

暂无评论

Quantitative Evaluation of Actual LOE Fault Diagnosability for Dynamic systems

引用

Zidonghua Xuebao/Acta Automatica Sinica 2017年第11期43卷 1941-1949页

作者： Fu, Fang-Zhou Wang, Da-Yi Li, Wen-Bo Beijing Institute of Control Engineering Beijing100190 China Beijing Institute of Spacecraft System Engineering Beijing100190 China Science and Technology on Space Intelligent Control Laboratory Beijing100190 China

Due to the lack of efficient approaches to quantify actual loss of effect (LOE) fault diagnosability in dynamic systems, a novel presented is presented in this paper. Discrete-time state space models are modified into dynamic models with time window of certain length, and the similarity of different multivariate distributions, instead of fault diagnosability evaluation, is analyzed. The definitions of detectability and isolability of LOE fault are given. Diagnosability performance is quantified by the method based on minimum Bhattacharyya distance. Least-squares method is utilized to enhance applicability of the novel proposed approach. In addition, a simulation example is employed to show the validity of the proposed approach and to analyze maximum effectiveness coefficient of LOE fault in dynamic systems. Copyright © 2017 Acta Automatica Sinica. All rights reserved.

关键词： State space methods

来源：评论

学校读者我要写书评

暂无评论

Economic analysis of multi-energy virtual power plant considering market information

Economic analysis of multi-energy virtual power plant consid...

引用

2017 IEEE Conference on Energy Internet and Energy system Integration, EI2 2017

作者： Wang, Jiazhen Shen, Xinwei Guo, Qinglai Xiong, Wen Tang, Lei Shenzhen Environmental Science and New Energy Technology Engineering Laboratory Tsinghua-Berkeley Shenzhen Insitute Tsinghua University Shenzhen China State Key Lab of Control and Simulation of Power System and Generation Equipments Department of Electrical Engineering Tsinghua University Beijing China Guangzhou Power Grid Company Guangzhou Lei Tang Beijing Qingda Gaoke System Control Company Beijing China Beijing Qingda Gaoke System Control Company Beijing China

ISBN: (纸本)9781538614273

Integrated Energy system is beneficial for promoting the distributed renewable energy (DRE) consumption, thereby alleviating environmental pollution and energy shortage. In this paper, we propose a virtual power plant (VPP) structure considering the feature of heat and electric power system integration, which is defined as Multi-energy Virtual Power Plant (MVPP). MVPP is allowed to participate in the electricity market;and price information from bulk power market can affect heating system through the coupling devices, thus optimizing the co-operation of electric and heat system. MVPP is also involved in the auxiliary service market, a penalty term is designed for the Utility to charge MVPP service fee so that power fluctuation on transmission line can be reduced. The case study proved the effectiveness of the penalty term and MVPP is able to provide reserve service for Utility in peak load hours by multi-energy flow coupling under the regulation of feed-in tariff. © 2017 IEEE.

关键词： Virtual Power Plants

来源：评论

学校读者我要写书评

暂无评论

Observations of energetic-particle population enhancements along intermittent structures near the sun from parker solar probe

arXiv

引用

arXiv 2019年

作者： Bandyopadhyay, Riddhi Matthaeus, W.H. Parashar, T.N. Chhiber, R. Ruffolo, D. Goldstein, M.L. Maruca, B.A. Chasapis, A. Qudsi, R. McComas, D.J. Christian, E.R. Szalay, J.R. Joyce, C.J. Giacalone, J. Schwadron, N.A. Mitchell, D.G. Hill, M.E. Wiedenbeck, M.E. McNutt, R.L. Desai, M.I. Bale, Stuart D. Bonnell, J.W. Wit, Thierry Dudokde Goetz, Keith Harvey, Peter R. MacDowall, Robert J. Malaspina, David M. Pulupa, Marc Velli, M. Kasper, J.C. Korreck, K.E. Stevens, M. Case, A.W. Raouafi, N. Department of Physics and Astronomy University of Delaware NewarkDE19716 United States Bartol Research Institute University of Delaware NewarkDE19716 United States NASA Goddard Space Flight Center GreenbeltMD20771 United States Department of Physics Faculty of Science Mahidol University Bangkok10400 Thailand University of Maryland Baltimore County BaltimoreMD21250 United States Laboratory for Atmospheric and Space Physics University of Colorado Boulder BoulderCO80303 United States Department of Astrophysical Sciences Princeton University PrincetonNJ08544 United States University of Arizona TucsonAZ85721 United States University of New Hampshire DurhamNH03824 United States Johns Hopkins University Applied Physics Laboratory LaurelMD20723 United States California Institute of Technology PasadenaCA91125 United States University of Texas of San Antonio San AntonioTX78249 United States Physics Department University of California BerkeleyCA94720-7300 United States Space Sciences Laboratory University of California BerkeleyCA94720-7450 United States Blackett Laboratory Imperial College London LondonSW72AZ United Kingdom School of Physics and Astronomy Queen Mary University of London LondonE14NS United Kingdom LPC2E CNRS University of Orleans Orleans France School of Physics and Astronomy University of Minnesota MinneapolisMN55455 United States Solar System Exploration Division NASA Goddard Space Flight Center GreenbeltMD20771 United States Laboratory for Atmospheric and Space Physics University of Colorado BoulderCO80303 United States Department of Earth Planetary and Space Sciences University of California Los AngelesCA90095 United States Climate and Space Sciences and Engineering University of Michigan Ann ArborMI48109 United States Smithsonian Astrophysical Observatory CambridgeMA02138 United States

Observations at 1 au have confirmed that enhancements in measured energetic particle uxes are sta-tistically associated with rough" magnetic fields, i.e., fields having atypically large spatial derivatives or increments, as measured by the Partial Variance of Increments (PVI) method. One way to interpret this observation is as an association of the energetic particles with trapping or channeling within mag-netic ux tubes, possibly near their boundaries. However, it remains unclear whether this association is a transport or local effect;i.e., the particles might have been energized at a distant location, perhaps by shocks or reconnection, or they might experience local energization or re-acceleration. The Parker Solar Probe (PSP), even in its first two orbits, offers a unique opportunity to study this statistical correlation closer to the corona. As a first step, we analyze the separate correlation properties of the energetic particles measured by the ISfiIS instruments during the first solar encounter. The distribu-tion of time intervals between a specific type of event, i.e., the waiting time, can indicate the nature of the underlying process. We find that the ISfiIS observations show a power-law distribution of waiting times, indicating a correlated (non-Poisson) distribution. Analysis of low-energy ISfiIS data suggests that the results are consistent with the 1 au studies, although we find hints of some unexpected be-havior. A more complete understanding of these statistical distributions will provide valuable insights into the origin and propagation of solar energetic particles, a picture that should become clear with future PSP orbits. Copyright © 2019, The Authors. All rights reserved.

关键词： Probes

来源：评论

学校读者我要写书评

暂无评论

Corrigendum to: The TianQin project: current progress on science and technology

引用

Progress of Theoretical and Experimental Physics 2021年第5期2021卷

作者： Mei, Jianwei Bai, Yan-Zheng Bao, Jiahui Barausse, Enrico Cai, Lin Canuto, Enrico Cao, Bin Chen, Wei-Ming Chen, Yu Ding, Yan-Wei Duan, Hui-Zong Fan, Huimin Feng, Wen-Fan Fu, Honglin Gao, Qing Gao, TianQuan Gong, Yungui Gou, Xingyu Gu, Chao-Zheng Gu, De-Feng He, Zi-Qi Hendry, Martin Hong, Wei Hu, Xin-Chun Hu, Yi-Ming Hu, Yuexin Huang, Shun-Jia Huang, Xiang-Qing Jiang, Qinghua Jiang, Yuan-Ze Jiang, Yun Jiang, Zhen Jin, Hong-Ming Korol, Valeriya Li, Hong-Yin Li, Ming Li, Pengcheng Li, Rongwang Li, Yuqiang Li, Zhu Li, Zhulian Li, Zhu-Xi Liang, Yu-Rong Liang, Zheng-Cheng Liao, Fang-Jie Liu, Qi Liu, Shuai Liu, Yan-Chong Liu, Li Liu, Pei-Bo Liu, Xuhui Liu, Yuan Lu, Xiong-Fei Lu, Yang Lu, Ze-Huang Luo, Yan Luo, Zhi-Cai Milyukov, Vadim Ming, Min Pi, Xiaoyu Qin, Chenggang Qu, Shao-Bo Sesana, Alberto Shao, Chenggang Shi, Changfu Su, Wei Tan, Ding-Yin Tan, Yujie Tan, Zhuangbin Tu, Liang-Cheng Wang, Bin Wang, Cheng-Rui Wang, Fengbin Wang, Guan-Fang Wang, Haitian Wang, Jian Wang, Lijiao Wang, Panpan Wang, Xudong Wang, Yan Wang, Yi-Fan Wei, Ran Wu, Shu-Chao Xiao, Chun-Yu Xu, Xiao-Shi Xue, Chao Yang, Fang-Chao Yang, Liang Yang, Ming-Lin Yang, Shan-Qing Ye, Bobing Yeh, Hsien-Chi Yu, Shenghua Zhai, Dongsheng Zhang, Caishi Zhang, Haitao Zhang, Jian-dong Zhang, Jie Zhang, Lihua Zhang, Xin Zhang, Xuefeng Zhou, Hao Zhou, Ming-Yue Zhou, Ze-Bing Zhu, Dong-Dong Zi, Tie-Guang Luo, Jun TianQin Research Center for Gravitational Physics & School of Physics and Astronomy Sun Yat-sen University (Zhuhai Campus) Zhuhai 519082 P.R. China Centre for Gravitational Experiments School of Physics MOE Key Laboratory of Fundamental Physical Quantities Measurement & Hubei Key Laboratory of Gravitation and Quantum Physics PGMF Huazhong University of Science and Technology Wuhan 430074 P.R. China SISSA Via Bonomea 265 34136 Trieste Italy and INFN Sezione di Trieste & IFPU – Institute for Fundamental Physics of the Universe Via Beirut 2 34014 Trieste Italy Former Faculty Politecnico di Torino Corso Duca degli Abruzzi 24 10129 Torino Italy Yunnan Observatories Chinese Academy of Sciences Kunming 650011 China School of Physical Science and Technology Southwest University Chongqing 400715 China Beijing Institute of Control Engineering Beijing 100094 P.R. China SUPA School of Physics and Astronomy University of Glasgow Glasgow G12 8QQ UK DFH Satellite Co. Ltd. Beijing 100094 P.R. China National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China School of Astronomy and Space Science University of Chinese Academy of Sciences Beijing 100049 China School of Physics and Astronomy University of Birmingham Birmingham B15 2TT United Kingdom Center for High Energy Physics & Department of Physics and State Key Laboratory of Nuclear Physics and Technology Peking University No. 5 Yiheyuan Rd Beijing 100871 P.R. China Lomonosov Moscow State University Sternberg Astronomical Institute Moscow 119992 Russia Dipartimento di Fisica “G. Occhialini” Universitá degli Studi Milano Bicocca Piazza della Scienza 3 I-20126 Milano Italy School of Aeronautics and Astronautics Shanghai Jiao Tong University Shanghai 200240 China Purple Mountain Observatory Chinese Academy of Sciences Nanjing 210023 & School of Astronomy and Space Science University of Science and Technology of China Hefei Anhui 230026 P.R. China Max-Planck-Institut für Gravitationsphysik (Al

来源：评论

学校读者我要写书评

暂无评论

Bifurcation Control for a Duffing Oscillator with Delayed Velocity Feedback

引用

International Journal of Automation and computing 2016年第6期13卷 596-606页

作者： Chang-Jin Xu Yu-Sen Wu Guizhou Key Laboratory of Economics System Simulation Guizhou University of Finance and Economics Guiyang 550004 China School of Mathematics and Statistics Henan University of Science and Technology Luoyang 471023 China

In this paper, a Duffing oscillator model with delayed velocity feedback is considered. Applying the time delayed feedback control method and delayed differential equation theory, we establish some criteria which ensure the stability and the existence of Hopf bifurcation of the model. By choosing the delay as bifurcation parameter and analyzing the associated characteristic equation,the existence of bifurcation parameter point is determined. We found that if the time delay is chosen as a bifurcation parameter,Hopf bifurcation occurs when the time delay is changed through a series of critical values. Some numerical simulations show that the designed feedback controllers not only delay the onset of Hopf bifurcation, but also enlarge the stability region for the model.

关键词： bifurcation oscillator Feedback asymptotically dynamical Velocity enlarge perturbation imaginary unstable

来源：评论

学校读者我要写书评

暂无评论

The JWST Early Release science Program for the Direct Imaging & Spectroscopy of Exoplanetary systems

arXiv

引用

arXiv 2022年

作者： Hinkley, Sasha Carter, Aarynn L. Ray, Shrishmoy Skemer, Andrew Biller, Beth Choquet, Elodie Millar-Blanchaer, Maxwell A. Sallum, Stephanie Miles, Brittany Whiteford, Niall Patapis, Polychronis Perrin, Marshall Pueyo, Laurent Schneider, Glenn Stapelfeldt, Karl Wang, Jason Ward-Duong, Kimberly Bowler, Brendan P. Boccaletti, Anthony Girard, Julien H. Hines, Dean Kalas, Paul Kammerer, Jens Kervella, Pierre Leisenring, Jarron Pantin, Eric Zhou, Yifan Meyer, Michael Liu, Michael C. Bonnefoy, Mickael Currie, Thayne McElwain, Michael Metchev, Stanimir Wyatt, Mark Absil, Olivier Adams, Jea Barman, Travis Baraffe, Isabelle Bonavita, Mariangela Booth, Mark Bryan, Marta Chauvin, Gael Chen, Christine Danielski, Camilla De Furio, Matthew Factor, Samuel M. Fitzgerald, Michael P. Fortney, Jonathan J. Grady, Carol Greenbaum, Alexandra Henning, Thomas Hoch, Kielan K.W. Janson, Markus Kennedy, Grant Kenworthy, Matthew Kraus, Adam Kuzuhara, Masayuki Lagage, Pierre-Olivier Lagrange, Anne-Marie Launhardt, Ralf Lazzoni, Cecilia Lloyd, James Marino, Sebastian Marley, Mark Martinez, Raquel Marois, Christian Matthews, Brenda Matthews, Elisabeth C. Mawet, Dimitri Mazoyer, Johan Phillips, Mark Petrus, Simon Quanz, Sascha P. Quirrenbach, Andreas Rameau, Julien Rebollido, Isabel Rickman, Emily Samland, Matthias Sargent, B. Schlieder, Joshua E. Sivaramakrishnan, Anand Stone, Jordan M. Tamura, Motohide Tremblin, Pascal Uyama, Taichi Vasist, Malavika Vigan, Arthur Wagner, Kevin Ygouf, Marie University of Exeter Astrophysics Group Physics Building Stocker Road ExeterEX4 4QL United Kingdom Department of Astronomy & Astrophysics University of California Santa CruzCA95064 United States SUPA Institute for Astronomy The University of Edinburgh Royal Observatory Blackford Hill EdinburghEH9 3HJ United Kingdom Aix Marseille Univ. CNRS CNES LAM Marseille France Department of Physics University of California Santa Barbara Santa BarbaraCA United States Department of Physics and Astronomy University of California Irvine IrvineCA United States Department of Astrophysics American Museum of Natural History Central Park West at 79th Street NY10024 United States Institute for Particle Physics & Astrophysics ETH Zurich Zurich8092 Switzerland Space Telescope Science Institute 3700 San Martin Drive BaltimoreMD21218 United States Steward Observatory University of Arizona 933 N. Cherry Ave TucsonAZ85721-0065 United States Jet Propulsion Laboratory California Institute of Technology M/S 321-100 4800 Oak Grove Drive PasadenaCA91109 United States Department of Astronomy California Institute of Technology PasadenaCA91125 United States Department of Physics and Astronomy Northwestern University EvanstonIL60208 United States Department of Astronomy Smith College NorthamptonMA01063 United States Department of Astronomy The University of Texas at Austin 2515 Speedway Boulevard Stop C1400 AustinTX78712 United States LESIA Observatoire de Paris Université PSL CNRS Sorbonne Université Université Paris Cité 5 place Jules Janssen Meudon92195 France Department of Astronomy University of California BerkeleyCA94720 United States IRFU/DAp Département D’Astrophysique CE Saclay Gif-sur-Yvette France Department of Astronomy University of Michigan Ann ArborMI48109 United States Institute of Astronomy University of Hawaii 2860 Woodlawn Drive HonoluluHI96822 United States Université Grenoble Alpes CNRS Institut de Planétologie et d’As

The direct characterization of exoplanetary systems with high contrast imaging is among the highest priorities for the broader exoplanet community. As large space missions will be necessary for detecting and characterizing exo-Earth twins, developing the techniques and technology for direct imaging of exoplanets is a driving focus for the community. For the first time, JWST will directly observe extrasolar planets at mid-infrared wavelengths beyond 5 µm, deliver detailed spectroscopy revealing much more precise chemical abundances and atmospheric conditions, and provide sensitivity to analogs of our solar system ice-giant planets at wide orbital separations, an entirely new class of exoplanet. However, in order to maximise the scientific output over the lifetime of the mission, an exquisite understanding of the instrumental performance of JWST is needed as early in the mission as possible. In this paper, we describe our 55-hour Early Release science Program that will utilize all four JWST instruments to extend the characterisation of planetary mass companions to ∼15 µm as well as image a circumstellar disk in the mid-infrared with unprecedented sensitivity. Our program will also assess the performance of the observatory in the key modes expected to be commonly used for exoplanet direct imaging and spectroscopy, optimize data calibration and processing, and generate representative datasets that will enable a broad user base to effectively plan for general observing programs in future cycles. © 2022, CC BY.

关键词： Extrasolar planets

来源：评论

学校读者我要写书评

暂无评论

Geoacoustic inversion using ship noise vector field

引用

Harbin Gongcheng Daxue Xuebao/Journal of Harbin Engineering University 2018年第2期39卷 236-240页

作者： Ren, Qunyan Piao, Shengchun Ma, Li Guo, Shengming Liao, Tianjun Institute of Acoustics Chinese Academy of Sciences Beijing100190 China Key Laboratory of Underwater Acoustics Environment Chinese Academy of Sciences Beijing100190 China Science and Technology on Underwater Acoustic Laboratory Harbin Engineering University Harbin150001 China State Key Laboratory of Complex System Simulation Beijing100101 China

Seabed geoacoustic parameters and associated uncertainties are important for sonar performance prediction and related applications, and the feasibility of jointly using pressure and vector fields to increase geoacoustic inversion reliability is discussed. The matching field inversion algorithm is used to process ship noise data collected by a single-vector hydrophone, and the estimation value and posterior probability distribution is derived. Theoretical analysis and a numerical simulation suggest that the component of the vertical particle velocity provides more abundant acoustic signal transmission characteristics than when using the acoustic pressure field only, and more consolidated estimates can be obtained through using pressure and vector fields jointly than by treating them individually. © 2018, Editorial Department of Journal of HEU. All right reserved.

关键词： Uncertainty analysis

来源：评论

学校读者我要写书评

暂无评论

建议与咨询留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

时间限定

文献类型

馆藏选择

核心期刊

语言

文献类型

帮助

文字说明：

检索规则说明：

检索范例：

分类表

所选分类

限定检索结果

文献类型

馆藏范围

日期分布

学科分类号

主题

机构

作者

语言

请选择保存的检索档案：

请选择收藏分类：

通借通还

建议与咨询 留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

时间限定

文献类型

馆藏选择

核心期刊

语言

文献类型

帮助

文字说明：

检索规则说明：

检索范例：

分类表

所选分类

限定检索结果

文献类型

馆藏范围

日期分布

学科分类号

主题

机构

作者

语言

请选择保存的检索档案： 新增检索档案 确定 取消

请选择收藏分类： 新增自定义分类 确定 取消

通借通还

建议与咨询留下您的常用邮箱和电话号码，以便我们向您反馈解决方案和替代方法

请选择保存的检索档案：

请选择收藏分类：