检索结果-内蒙古大学图书馆

您好，读者！请登录

内蒙古大学图书馆

首页
概况
党建
资源
服务
科研支持
- 论文收录引用证明
- 科技查新
知识产权
档案馆
帮助

咨询与建议

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

您的常用邮箱：*

您的手机号码：*

问题描述：

当前已输入0个字，您还可以输入200个字

全部搜索
期刊论文
图书
学位论文
标准
纸本馆藏
外文资源发现
数据库导航
超星发现

高级检索

时间限定

出版年份：

文献类型

图书期刊文献学位论文多媒体

馆藏选择

电子馆藏纸本馆藏

核心期刊

全部期刊 SCI 收录期刊 SSCI 收录期刊 EI 收录期刊 CSCD 收录期刊 CSSCI 收录期刊

语言

中文英文

文献类型

期刊文献图书学位论文标准纸本馆藏

帮助

文字说明：

T=题名（书名、题名），A=作者（责任者），K=主题词，P=出版物名称，PU=出版社名称，O=机构（作者单位、学位授予单位、专利申请人），L=中图分类号，C=学科分类号，U=全部字段，Y=年（出版发行年、学位年度、标准发布年）

检索规则说明：

AND代表“并且”；OR代表“或者”；NOT代表“不包含”；(注意必须大写,运算符两边需空一格)

检索范例：

范例一：(K=图书馆学 OR K=情报学) AND A=范并思 AND Y=1982-2016
范例二：P=计算机应用与软件 AND (U=C++ OR U=Basic) NOT K=Visual AND Y=2011-2016

分类表

所选分类

>> <<

限定检索结果

文献类型

1,156 篇 会议
31 篇 期刊文献
3 册 图书

馆藏范围

1,190 篇 电子文献
0 种 纸本馆藏

日期分布

学科分类号

968 篇 工学
- 575 篇 仪器科学与技术
- 332 篇 软件工程
- 328 篇 控制科学与工程
- 294 篇 计算机科学与技术...
- 119 篇 电气工程
- 117 篇 航空宇航科学与技...
- 54 篇 机械工程
- 40 篇 光学工程
- 36 篇 信息与通信工程
- 31 篇 测绘科学与技术
- 29 篇 电子科学与技术（可...
- 25 篇 动力工程及工程热...
- 23 篇 材料科学与工程（可...
- 22 篇 核科学与技术
- 12 篇 化学工程与技术
- 11 篇 土木工程
- 8 篇 安全科学与工程
- 7 篇 力学（可授工学、理...
- 7 篇 交通运输工程
815 篇 理学
- 567 篇 物理学
- 521 篇 天文学
- 36 篇 数学
- 26 篇 地球物理学
- 15 篇 化学
- 10 篇 系统科学
- 7 篇 统计学（可授理学、...
51 篇 管理学
- 47 篇 管理科学与工程(可...
- 20 篇 工商管理
28 篇 医学
- 28 篇 临床医学
8 篇 教育学
- 8 篇 教育学
4 篇 经济学
2 篇 军事学
1 篇 法学

主题

111 篇 control systems
94 篇 software
77 篇 telescopes
54 篇 adaptive optics
51 篇 telescope
45 篇 instruments
44 篇 control software
43 篇 control system
35 篇 mirrors
34 篇 instrumentation
32 篇 control
32 篇 process control
29 篇 hardware
28 篇 active optics
27 篇 data acquisition
25 篇 observatories
24 篇 telescope contro...
22 篇 astronomy
22 篇 application soft...
22 篇 computer archite...

机构

19 篇 european so obse...
18 篇 nasa goddard spa...
13 篇 space telescope ...
11 篇 space telescope ...
10 篇 natl radio astro...
8 篇 max planck inst ...
7 篇 joint astron ctr...
7 篇 univ arizona ste...
6 篇 chinese acad sci...
6 篇 natl inst nat sc...
6 篇 chinese acad sci...
5 篇 osserv astron tr...
5 篇 univ massachuset...
5 篇 univ calif los a...
5 篇 natl solar obser...
5 篇 natl astron obse...
5 篇 nasa ames res ct...
5 篇 natl res council...
5 篇 ball aerosp & te...
5 篇 inaf osservatori...

作者

9 篇 kosugi g
9 篇 drory niv
9 篇 soummer remi
8 篇 perrin marshall ...
8 篇 guyon olivier
8 篇 mancini d
8 篇 sasaki t
7 篇 pueyo laurent
7 篇 anon
7 篇 schipani p.
7 篇 briegel florian
6 篇 lee hanshin
6 篇 ramsey jason
6 篇 hill gary j.
6 篇 jeschke eric
6 篇 chiozzi g
6 篇 vuerli c
6 篇 wirenstrand k
6 篇 martinache frant...
6 篇 schipani p

语言

1,176 篇 英文
10 篇 其他
4 篇 中文

检索条件"任意字段=Conference on Advanced Telescope and Instrumentation Control Software"

共 1190 条记录，以下是581-590 订阅

全选清除本页清除全部题录导出标记到"检索档案"

详细简洁

排序：

The WIYN One Degree Imager: An Update

The WIYN One Degree Imager: An Update

引用

conference on Ground-Based and Airborne instrumentation for Astronomy II

作者： Harbeck, Daniel R. Jacoby, George H. Muller, Gary Sawyer, Dave Harmer, Charles Yeatts, Andrey Cavin, John Corson, Charles Univ Wisconsin 475 N Charter St Madison WI 53706 USA WIYN Observat Tucson AZ 85719 USA Natl Opt Astron Observ Tucson AZ 85719 USA

ISBN: (纸本)9780819472243

The WIYN Consortium is building the One Degree Imager (ODI) for its 3.5m telescope, located at Kitt Peak, Arizona (USA). ODI will utilize both the excellent image quality and the one degree field of view of the WIYN telescope. Image quality will be actively improved by localised tip/tilt image motion stabilisation using a novel concept of Orthogonal Transfer Array (OTA) CCDs, which are a new detector type jointly developed with the PanSTARRS project. Its anticipated median image quality of <= 0.55" in the R band will make ODI a unique and competitive instrument in the landscape of the next generation of large field imagers. A conceptual design of ODI was presented earlier at SPIE.(1) In the meantime, this concept matured, the ODI project has been fully funded, and it has entered the construction phase. A prototype camera (QUOTA) with a field of view of 16' x 16' has already seen first star light in fall 2006. In this paper we report on the evolution of ODI's definition, the design of its components, the status of the OTA detector development, and the path towards first light in early 2010. In accompanying papers we detail the design of the ODI's optical corrector, the mechanical structures, and the software & instrument system control design.

关键词： Ground based telescope instrumentation wide-field imaging One Degree Imager Orthogonal Transfer Array CCD WIYN telescope

来源：评论

学校读者我要写书评

暂无评论

Applications of high-rate data logging to telescope system development and operations

Applications of high-rate data logging to telescope system d...

引用

2nd conference on advanced software and control for Astronomy

作者： Carter, Christopher J. Rippa, Mathew J. Gemini Observ Elect & Instrumentat Grp 670 North Aohoku PlUniv Pk Hilo HI 96720 USA Gemini Observ Software Grp Hilo HI 96720 USA

ISBN: (纸本)9780819472298

The Gemini Secondary Mirror Tip/tilt Systems (M2TS) have greatly benefited from the availability of software-based data logging-to-disk of internal variables at servo loop rates, enabling efficient testing and troubleshooting. Similar 'fast-logging-to-disk' systems are now being considered for other Gemini subsystems. We describe how this technique was successfully applied to the M2TS, solving intractable tuning problems;a forward look will show how extensive & fully integrated logging and diagnostic capabilities are at the heart of the new design for the M2TS-2. Designers of new and ever-larger and more complex telescope systems are challenged to consider the benefits of including such systems in their own designs at an early stage - and to consider the costs in terms of ease of performing diagnostics and loss of maintainability of not doing so.

关键词： data logging high-rate sampling systems diagnostics analysis troubleshooting commissioning time domain frequency domain Bode

来源：评论

学校读者我要写书评

暂无评论

Optical Modeling Activities for NASA's James Webb Space telescope (JWST): V. Operational Alignment Updates

Optical Modeling Activities for NASA's James Webb Space Tele...

引用

conference on Modeling, Systems Engineering and Project Management for Astronomy III

作者： Howard, Joseph M. Ha, Kong Q. Shiri, Ron Smith, J. Scott Mosier, Gary Muheim, Danniella NASA Goddard Space Flight Ctr Greenbelt MD USA

ISBN: (纸本)9780819472274

This paper is part five of a series on the ongoing optical modeling activities for the James Webb Space telescope (JWST). The first two papers discussed modeling JWST on-orbit performance using wavefront sensitivities to predict line of sight motion induced blur, and stability during thermal transients. The third paper investigates the aberrations resulting from alignment and figure compensation of the controllable degrees of freedom (primary and secondary mirrors), which may be encountered during ground alignment and on-orbit commissioning of the observatory, and the fourth introduced the software toolkits used to perform much of the optical analysis for JWST. The work here models observatory operations by simulating line-of-sight image motion and alignment drifts over a two-week period. Alignment updates are then simulated using wavefront sensing and control processes to calculate and perform the corrections. A single model environment in Matlab is used for evaluating the predicted performance of the observatory during these operations.

关键词： Optical Modeling Integrated Modeling telescopes Phase Retrieval Jitter Thermal Stability

来源：评论

学校读者我要写书评

暂无评论

Distributed Modeling and control of a Segmented Mirror Surface

Distributed Modeling and Control of a Segmented Mirror Surfa...

引用

2nd conference on advanced software and control for Astronomy

作者： Kerley, Dan A. Park, Edward J. Dunn, Jennifer Natl Res Council Canada Herzberg Inst Astrophys 5071 W Saanich Rd Victoria BC V9E 2E7 Canada Univ Victoria Dept Mech Engn Victoria BC V8W 2Y2 Canada

ISBN: (纸本)9780819472298

The next generation of ground-based optical telescopes will employ increasingly large primary mirrors to achieve superior resolution and light collecting abilities. Many of these large mirror surfaces will be segmented into an array of hundreds of smaller mirror segments. The corresponding number of required sensors and actuators will be in the order of thousands, which creates a challenging control problem to stabilize and align each segment from external disturbances wind shake, gravity forces, thermal effects, seismic effects and induced vibrations from surrounding equipment and telescope motion - so that the telescope's image quality requirements can be met. The use of a centralized control scheme may be infeasible due to the large number of inputs and outputs of the resulting control system, while a decentralize control scheme would lack global performance. An attractive alternative approach is an interconnected network of distributed controllers that provide global control with a highly scalable design and implementation. A segmented mirror can be considered as an interconnected system comprised of many similar discrete subsystems, where each subsystem represents an individual mirror segments and its dynamics are coupled directly to its neighboring segments. The resulting distributed controller network of controller subsystems are similarly coupled and working cooperatively to achieve the desired global performance.

关键词： Distributed Modeling Distributed control Segmented Mirror telescope control Decentralized control

来源：评论

学校读者我要写书评

暂无评论

Enabling technologies and constraints for software sharing in large astronomy projects

Enabling technologies and constraints for software sharing i...

引用

2nd conference on advanced software and control for Astronomy

作者： Chiozzi, Gianluca Bridger, Alan Gillies, Kim Goodrich, Bret Johnson, Jimmy McCann, Kevin Schumacher, German Wampler, Steve European Southern Observ Karl Schwarzschild Str 2 D-8046 Garching Germany UK Astron Technol Ctr Edinburgh Midlothian Scotland Space Telescope Sci Inst Baltimore MD USA Natl Solar Observ Silver Spring MD USA WM Keck Observ Kamuela HI USA Natl Opt Astron Observ La Serena Chile

ISBN: (纸本)9780819472298

The new observatories currently being built, upgraded or designed represent a big step up in terms of complexity (laser guide star, adaptive optics, 30/40m class telescopes) with respect to the previous generation of ground-based telescopes. Moreover, the high cost of observing time imposes challenging requirements on system reliability and observing efficiency as well as challenging constraints in implementing major upgrades to operational observatories. Many of the basic issues are common to most of the new projects, while each project also brings an additional set of very specific challenges, imposed by the unique characteristics and scientific objectives of each telescope. Finding ways to share the solution and the risk for these common problems would allow the teams in the different projects to concentrate more resources on the specific challenges, while at the same time realizing more reliable and cost efficient systems. In this paper we analyze the many dimensions that might be involved in sharing and re-using observatory software (e.g. components, design, infrastructure frameworks, applications, toolkits, etc.). We also examine observatory experiences and technology trends. This work is the continuation of an effort started in the middle of 2007 to analyze the trends in software for the control systems of large astronomy projects[ I].

关键词： observatory software software sharing technology trends infrastructure frameworks control system

来源：评论

学校读者我要写书评

暂无评论

ESPRESSO control software and Electronics

ESPRESSO Control Software and Electronics

引用

2nd conference on advanced software and control for Astronomy

作者： Di Marcantonio, P. Santin, P. Coretti, I. Cirami, R. Comari, M. Osserv Astron Trieste INAF I-34143 Trieste Italy

ISBN: (纸本)9780819472298

The Astrophysical Technology Group of the INAF-AOT, as part of a consortium led by ESO, has carried out a feasibility study for the control software and Electronics of a new generation optical spectrograph, named ESPRESSO. ESPRESSO has been conceived as a high-efficient, high-resolution, fiber-fed spectrograph of high mechanical and thermal stability to be located at the Coude Combined Laboratory of the VLT. These features together with its ability to gather light from 4-UT simultaneously made ESPRESSO a very challenging instrument. This paper presents an overview of the control software and electronics concept design focusing on the more critical and innovative aspects of the spectrograph.

关键词： VLT control software echelle spectrograph astronomical instrumentation

来源：评论

学校读者我要写书评

暂无评论

Inspector: the GTC graphical user interface

Inspector: the GTC graphical user interface

引用

2nd conference on advanced software and control for Astronomy

作者： Macias, R. Filgueira, J. M. Inst Astrofis Canarias GTC Project Tenerife 38200 Spain

ISBN: (纸本)9780819472298

The Inspector is the graphical user interface of the GTC control System. It is implemented in Java and gives a unified view of the whole system by representing it as hierarchical browser of distributed objects. The ability to resolve at runtime the domain objects running distributed on the real time systems and use that domain information to dynamically generate different views of the system. Using the exact same set of tools and edition capabilities, it is as simple to create an engineering view of the GCS as it is to create a science view. Such flexibility and simplicity, have made the Inspector be, not only the interface of the final system, but also one of the most important tools used by the engineers from very early in the development process to test the functionality of their respective components. Persistency of dynamically created views, commands execution flows, visualization of system alarms and logs, are also important aspects of the Inspector which will be explained in this paper.

关键词： GUI interface software control GTC

来源：评论

学校读者我要写书评

暂无评论

Design, construction, and performance of VIRUS-P: the prototype of a highly replicated integral-field spectrograph for HET

Design, construction, and performance of VIRUS-P: the protot...

引用

conference on Ground-Based and Airborne instrumentation for Astronomy II

作者： Hill, Gary. J. MacQueen, Phillip J. Smith, Michael P. Tufts, Joseph R. Roth, Martin M. Kelz, Andreas Adams, Joshua J. Drory, Niv Grupp, Frank Barnes, Stuart I. Blanc, Guillermo A. Murphy, Jeremy D. Altmann, Werner Wesley, Gordon L. Segura, Pedro R. Good, John M. Booth, John A. Bauer, Svend-Marian Popow, Emil Goertz, John A. Edmonston, Robert D. Wilkinson, Christopher P. Univ Texas Austin McDonald Observ 1 Univ Stn C1402 Austin TX 78712 USA Univ Texas Austin Dept Astron Austin TX 78712 USA Las Cumbres Observ Goleta CA 93117 USA Astrophys Inst Potsdam D-14482 Potsdam Germany Max Planck Inst Extraterr Phys D-85748 Garching Germany Konstruct Buro Werner Altmann D-94113 Haselbach Tiefenbach Germany

ISBN: (纸本)9780819472243

We describe the design, construction, and performance of VIRUS-P (Visible Integral-field Replicable Unit Spectrograph - Prototype), the prototype for 150+ identical fiber-fed integral field spectrographs for the Hobby-Eberly telescope Dark Energy Experiment (HETDEX double dagger). VIRUS-P was commissioned in 2007, is in regular service on the McDonald Observatory 2.7 m Smith telescope, and offers the largest field of any integral field spectrograph. The 246-fiber IFU uses a densepak-type fiber bundle with a 1/3 fill factor. It is fed at f/3.65 through a telecentric, two-group dioptric focal reducer. The spectrograph's double-Schmidt optical design uses a volume phase holographic grating at the pupil between the articulating f/3.32 folded collimator and the f/1.33 cryogenic prime focus camera. High on-sky throughput is achieved with this catadioptric system by the use of high reflectivity dielectric coatings, which set the 340-670 nm bandwidth. VIRUS-P is gimbal-mounted on the telescope to allow short fibers for high UV throughput, while maintaining high mechanical stability. The instrument software and the 18 square arcmin field, fixed-offset guider provide rapid acquisition, guiding, and precision dithering to fill in the IFU field. Custom software yields Poisson noise limited, sky subtracted spectra. The design characteristics are described that achieved uniformly high image quality with low scattered light and fiber-to-fiber cross talk. System throughput exceeds requirements and peaks at 40%. The observing procedures are described, and example observations are given.

关键词： telescopes Hobby-Eberly telescope, Astronomical instrumentation: Spectrographs VIRUS, Dark Energy

来源：评论

学校读者我要写书评

暂无评论

The Micro-displacement Worktable control System of Mirror Detection

The Micro-displacement Worktable Control System of Mirror De...

引用

2nd conference on advanced software and control for Astronomy

作者： Ye, Yu Zhang, Zhenchao Li, Aihua Chinese Acad Sci Nanjing Inst Astron Opt & Technol Natl Astron Observ Nanjing 210042 Peoples R China

ISBN: (纸本)9780819472298

This paper mainly introduces hardware design and control method of the system which is used for detecting the MA segmented mirrors In the LAMOST. According to the demand of sub-aperture stitching interferometer, the system adopts a control card to control the stepping motor to drive the worktable moving on the X-Y. The MA sub-mirror surface will be changed through active optical correction and add-subtract power of force actuators. The detection result of the M(A) segmented mirror of 14 shows that root mean square (RMS) of surface accuracy error is 21.387 nm less than 0.035 lambda (lambda = 632.8 nm). It is demonstrated that the control system can work very well and shorten the time of detection.

关键词： mirror detection micro-displacement worktable control system

来源：评论

学校读者我要写书评

暂无评论

A first generation software product line for data acquisition systems in astronomy

A first generation software product line for data acquisitio...

引用

2nd conference on advanced software and control for Astronomy

作者： Lopez-Ruiz, J. C. Heradio, Rube Cerrada Somolinos, Jose Antonio Coz Fernandez, Jose Ramon Ramos, Pablo Lopez Instituto de Astrofísica de Canarias (Spain) Univ. Nacional a Distancia (Spain) Univ. de La Laguna (Spain)

ISBN: (纸本)9780819472298

This article presents a case study on developing a software product line for data acquisition systems in astronomy based on the Exemplar Driven Development methodology and the Exemplar Flexibilization Language tool. The main strategies to build the software product line are based on the domain commonality and variability, the incremental scope and the use of existing artifacts. It consists on a lean methodology with little impact on the organization, suitable for small projects, which reduces product line start-up time. software Product Lines focuses on creating a family of products instead of individual products. This approach has spectacular benefits on reducing the time to market, maintaining the know-how, reducing the development costs and increasing the quality of new products. The maintenance of the products is also enhanced since all the data acquisition systems share the same product line architecture.

关键词： software Product Lines methodologies reuse software architecture

来源：评论

学校读者我要写书评

暂无评论

没有更多数据了...

全选清除本页清除全部题录导出标记到“检索档案”

共119页 << < 55 56 57 58 59 60 61 62 63 64 > >>

检索报告对象比较合并检索0

隐藏清空

合并搜索

回到顶部

执行限定条件

内容：

评分：

请选择保存的检索档案：

请选择收藏分类：

订阅名称：

通借通还

温馨提示：

图书名称：

借书校区：

取书校区：

手机号码：

邮箱地址：

一卡通帐号：

电话和邮箱必须正确填写，我们会与您联系确认。

联系人：

所在院系：

联系邮箱：

联系电话：

内蒙古自治区呼和浩特市赛罕区大学西街235号邮编: 010021

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：