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共 329 条记录，以下是171-180 订阅

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Integrating JSky into the large millimeter telescope monitor and control system

Integrating JSky into the large millimeter telescope monitor...

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Malin, D Souccar, K Wallace, G Univ Massachusetts Dept Astron Large Millimeter Telescope Amherst MA 01003 USA

ISBN: (纸本)0819454281

The Large Millimeter telescope monitor and control system (LMTMC) is an automatically generated software system that is implemented using XML and Java. One of the requirements of the system is catalog support. Rather than developing new catalog navigation techniques and building them into the automatically generated code, we chose to use JSky. JSky is a set of Java components providing catalog and image support for Astronomy. The JSky classes are extended to form new classes with additional capabilities that tighten the integration with the LMTMC system. Not only can users navigate local and web hosted catalogs, they can also direct output from catalogs into the control panels of the system eliminating error-prone typing or cut and paste operations. In addition, users can retrieve digital sky survey images from the catalogs, and superimpose scientific data on them to verify correct operation.

关键词： Large Millimeter telescope JSky catalog support reusable monitor and control XML Java automatically generated image support

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A secure and reliable monitor and control system for remote observing with the large millimeter telescope

A secure and reliable monitor and control system for remote ...

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Wallace, G Souccar, K Malin, D Univ Massachusetts Dept Astron Amherst MA 01003 USA

ISBN: (纸本)0819454281

Remote access to telescope monitor and control capabilities necessitates strict security mechanisms to protect the telescope and instruments from malicious or unauthorized use, and to prevent data from being stolen, altered, or corrupted. The Large Millimeter telescope (LMT) monitor and control system (LMTMC) utilizes the Common Object Request Broker Architecture (CORBA) middleware technology to connect remote software components. The LMTMC provides reliable and secure remote observing by automatically generating SSLIOP enabled CORBA objects. TAO, the ACE open source Object Request Broker (ORB), now supports secure communications by implementing the Secure Socket Layer Inter-ORB Protocol (SSLIOP) as a pluggable protocol. This capability supplies the LMTMC with client and server authentication, data integrity, and encryption. Our system takes advantage of the hooks provided by TAO SSLIOP to implement X.509 certificate based authorization. This access control scheme includes multiple authorization levels to enable granular access control.

关键词： Large Millimeter telescope monitor and control security authentication authorization encryption CORBA SSLIOP

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An implementation of the ATST virtual instrument model

An implementation of the ATST virtual instrument model

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Wampler, S Goodrich, B Natl Solar Observ Tucson AZ 85726 USA

ISBN: (纸本)0819454281

The advanced Technology Solar telescope (ATST) is intended to be the premier facility for experimental solar physics. A premium has been placed on operating ATST as a laboratory-style observatory to maximize the flexibility available to solar physicists. In particular, the main observation platform is a rotating coude platform supporting eight optical benches on which instruments may be assembled from available components. The Virtual Instrument Model has been developed to formalize the operation of a facility where instruments may exist for a single experiment before components are reassembled into a new instrument. The model allows the laboratory-style operation to fit easily within a typical modern telescope control system. This paper presents one possible implementation of the Virtual Instrument Model that is based on the container/component model becoming increasing popular in software development.

关键词： control systems solar astronomy instrument software

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Time to go H_∞?

Time to go H<sub>∞</sub>?

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Erm, T Hurák, Z Bauvir, B CALTECH Dept Astron Pasadena CA 91125 USA

ISBN: (纸本)0819454281

Traditionally telescope main axes controllers use a cascaded PI structure. We investigate the benefits and limitations of this and question if better performance can be achieved with modern control techniques. Our interest is mainly to improve disturbance rejection since the tracking performance normally is easy to achieve. Comparison is made to more advanced controller structures using H-infinity design. This type of controller is more complex and needs a mathematical model of the telescope dynamics. We discuss how to obtain this model and also how to reduce it to a more manageable size using state of the art model reduction techniques. As a design example the VLT altitude axis is chosen.

关键词： Very Large telescope H-infinity optimal control cascaded PI disturbance rejection

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Remote observing capability with Subaru telescope

Remote observing capability with Subaru Telescope

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conference on advanced software, control and Communication Systems for Astronomy

作者： Kosugi, G Sasaki, T Yagi, M Ogasawara, R Mizumoto, Y Noumaru, J Kawai, JA Koura, N Kusumoto, T Yamamoto, T Watanabe, N Ukawa, K NAOJ Subaru Telescope Hilo HI 96720 USA

ISBN: (纸本)0819454281

We've implemented remote observing function to Subaru telescope Observation software system (SOSs). Subaru telescope has three observing-sites, i.e., a telescope local-site and two remote observing- sites, Hilo base facility in Hawaii and Mitaka NAOJ headquarter in Japan. Our remote observing system is designed to allow operations not only from one of three observing-sites, but also from more than two sites concurrently or simultaneously. Considering allowance for delay in observing operations and a bandwidth of the network between the telescope-site and the remote observing-sites, three types of interfaces (protocols) have been implemented. In the remote observing mode, we use socket interface for the command and the status communication, vnc for ready-made applications and pop-up windows, and ftp for the actual data transfer. All images taken at the telescope-site are transferred to both of two remote observing-sites immediately after the acquisition to enable the observers' evaluation of the data. We present the current status of remote observations with Subaru telescope.

关键词： remote observing observation control operation software

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Application of real time database to LAMOST control system

Application of real time database to LAMOST control system

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conference on advanced software, control and Communication Systems for Astronomy

作者： Xu, LZ Xu, XQ Chinese Acad Sci Nanjing Inst Astron Opt & Technol Natl Astron Observ Nanjing 210042 Peoples R China

ISBN: (纸本)0819454281

The QNX based real time database is one of main features for Large sky Area Multi-Object fiber Spectroscopic telescope's (LAMOST) control system, which serves as a storage and platform for data flow, recording and updating timely various status of moving components in the telescope structure as well as environmental parameters around it. The database joins harmonically in the administration of the telescope control System (TCS). The paper presents methodology and technique tips in designing the EMPRESS database GUI software package, such as the dynamic creation of control widgets, dynamic query and share memory. The seamless connection between EMPRESS and the graphical development tool of QNX's Photon Application Builder (PhAB) has been realized, and so have the Windows look and feel yet under Unix-like operating system. In particular, the real time feature of the database is analyzed that satisfies the needs of the control system.

关键词： astronomical telescope real time database GUI dynamic query share memory LAMOST

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telescope networking and user support via remote telescope markup language

Telescope networking and user support via remote telescope m...

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Hessman, FV Pennypacker, C Romero-Colmenero, E Tuparev, G Univ Gottingen D-37093 Gottingen Germany

ISBN: (纸本)0819454281

Remote telescope Markup Language (RTML) is an XML-based interface/document format designed to facilitate the exchange of astronomical observing requests and results between investigators and observatories as well as within networks of observatories. While originally created to support simple imaging telescope requests (Versions 1.0-2.1), RTML Version 3.0 now supports a wide range of applications, from request preparation, exposure calculation, spectroscopy, and observation reports to remote telescope scheduling, target-of-opportunity observations and telescope network administration. The elegance of RTML is that all of this is made possible using a public XML Schema which provides a general-purpose, easily parsed, and syntax-checked medium for the exchange of astronomical and user information while not restricting or otherwise constraining the use of the information at either end. Thus, RTML can be used to connect heterogeneous systems and their users without requiring major changes in existing local resources and procedures. Projects as very different as a number of advanced amateur observatories, the global Hands-On Universe(TM) project, the MONET network (robotic imaging), the STELLA consortium (robotic spectroscopy), and the 11-m Southern African Large telescope are now using or intending to use RTML in various forms and for various purposes.

关键词： software interfaces service-observing robotic telescopes telescope networks XML

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Performance of the Lowell Observatory instrumentation System

Performance of the Lowell Observatory Instrumentation System

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conference on advanced software, control and Communication Systems for Astronomy

作者： Taylor, BW Dunham, EW Elliot, JL Lowell Observ Flagstaff AZ 86001 USA

ISBN: (纸本)0819454281

The Lowell Observatory instrumentation System (LOIS) is an instrument control software system with a common interface that can control a variety of instruments. Its user interface includes GUI-based, scripted, and remote program C control interfaces, and supports operational paradigms ranging from traditional direct observer interaction to fully automated operation. Currently LOIS controls a total of ten instruments built at Lowell Observatory (including one for SOFIA), NASA Ames Research Center, MIT (for Magellan), and Boston University. Together, these instruments include optical and near-IR imaging, spectroscopic, and polarimetric capability. This paper reviews the actual design of LOIS in comparison to its original design requirements and implementation approaches, and evaluates its strengths and weaknesses relative to operational performance, user interaction and feedback, and extensibility to new instruments.

关键词： software CCD IR telescope SOFIA MCS SCL

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control of the Hobby-Eberly telescope primary mirror array with the segment alignment maintenance system

Control of the Hobby-Eberly Telescope primary mirror array w...

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conference on advanced software, control and Communication Systems for Astronomy

作者： Palunas, P Fowler, JR Booth, JA Damm, G Ames, GH Univ Texas McDonald Observ Univ Stn 1 11402 Austin TX 78712 USA

ISBN: (纸本)0819454281

The Segment Alignment Maintenance System (SAMS) is a control system to maintain the alignment of the 91 segment Hobby-Eberly telescope (BET) primary mirror array. The system was developed by Blue-Line Engineering (Colorado Springs, CO) and NASA-Marshall Space Flight Center (Huntsville-Al). The core of the system is a set of 480 inductive edge sensors which measure relative shear between adjacent segments. The relative shear is used to calculate segment tip/tilt and piston corrections. Although the system has dramatically improved the performance of the BET it does not meet its error budget due to thermal drifts in the sensors. The system is now sufficiently stable that it routinely requires only one primary mirror alignment at the beginning of the night. We describe methods to calibrate this sensor drift.

关键词： Hobby-Eberly telescope HET SAMS edge sensors control systems

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Data acquirement and process system based on Ethernet for Multi Channel Solar telescope

Data acquirement and process system based on Ethernet for Mu...

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conference on advanced software, control and Communication Systems for Astronomy

作者： Hu, KL Deng, YY Ma, XL CAS Natl Astron Observ Beijing 100012 Peoples R China

ISBN: (纸本)0819454281

For astronomical observations, there are many kinds of CCD cameras for different scientific purposes. Sometimes, this even happens in one telescope. Traditionally, a CCD camera has an individual image grabber, data process unit, and corresponding control computer. Consequently, this brings some inconvenience and problems not only to the system management but also to the updating of the system. This paper presents a resolution to this problem for the Multi-Channel Solar telescope (MCST). All CCD cameras are connected in an Ethernet through an Ethernet interface. A server is needed to send commands to all cameras and transfer data through TCP/IP. Each CCD camera has an embedded system to control the camera, receive commands from the server and signals from the camera, process, and store the data. This paper describes the design of an Ethernet controlled camera. The camera is PULNIX TM1010, which is controlled by an Altera embedded system by Cyclone EP1C20F400C7 FPGA, which embedded with a Nios processor.

关键词： FPGA NIOS Ethernet embedded system Multi-Channel Solar telescope

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