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

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A reusable automatically generated software system for the control of the Large Millimeter telescope

A reusable automatically generated software system for the c...

引用

conference on advanced telescope and instrumentation control software ii

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

ISBN: (纸本)0819446270

A telescope system is composed of a set of real-world objects that are mapped onto software objects whose properties are described in XML configuration files. These XML files are processed to automatically generate user interfaces, underlying communication mechanisms, and extendible source code. Developers need not write user interfaces or communication methods but can focus on the production of scientific results. Any modifications or additions of objects can be easily achieved by editing or generating corresponding XML files and compiling them into the system. This framework can be utilized to implement servo controllers, device drivers, observing algorithms and instrument controllers;and is applicable to any problem domain that requires a user-based interaction with the inputs and outputs of a particular resource or program. This includes telescope systems, instruments, data reduction methods, and database interfaces. The system is implemented using Java, C++, and CORBA.

关键词： Large Millimeter telescope reusable automatically generated monitor and control XML Java CORBA

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JCMT/UKIRT telescope control system

JCMT/UKIRT telescope control system

引用

conference on advanced telescope and instrumentation control software ii

作者： Kackley, RD Rees, NP Bailey, JA Joint Astron Ctr Hilo HI 96720 USA

ISBN: (纸本)0819446270

The Joint Astronomy Centre (JAC) operates the James Clerk Maxwell telescope (JCMT), the world's largest sub-mm telescope, and the United Kingdom Infrared telescope (UKIRT), the world's largest telescope dedicated solely to infrared astronomy. Although these two telescopes investigate different regions of the electro-magnetic spectrum and have different mounting arrangements, the JAC (in collaboration with the Anglo-Australian Observatory) has developed the Portable telescope control System (PTCS) software so that it can be used on both JAC telescopes. The benefit of this work is increased efficiency, reduced maintenance time, and reduced personnel costs as a result of using a common code base on both JAC telescopes. During the next year, the PTCS will be enhanced as part of the JCMT Observatory control System (OCS) project so that configuration information can be transmitted to the PTCS via XML files. This will simplify the PTCS interface and expedite the implementation of the OCS. This paper gives an overview of the PTCS, describes its use on both telescopes, and indicates how XML files will be used to configure the telescope prior to the start of an observation.

关键词： telescope control system portable XML DRAMA

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SOAR TCS: From prototype to implementation

SOAR TCS: From prototype to implementation

引用

conference on advanced telescope and instrumentation control software ii

作者： Schumacher, G Ashe, MC SOAR Consortium La Serena Chile

ISBN: (纸本)0819446270

The SOAR telescope is in the final phases of construction. software development is progressing well, in accordance with installation of the telescope subsystems. Our original strategy, explored during the prototype phase, has been maintained and improved, resulting in a software package of great flexibility. This paper describes the implementation details that have proved to be most useful for the development of the SOAR TCS.

关键词： control system TCS software architecture LabVIEW Internet

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A rigorous algorithm for telescope pointing

A rigorous algorithm for telescope pointing

引用

conference on advanced telescope and instrumentation control software ii

作者： Wallace, P Rutherford Appleton Lab Didcot OX11 0QX Oxon England

ISBN: (纸本)0819446270

A typical modern telescope control system points,by first calculating the direction of the target in nominal mount coordinates and then applying small corrections to the demanded mount angles. The pointing refers to the rotation axis of the instrument mount, and rotator demands are calculated via parallactic angle. This simple approach works well enough when the corrections are small and the accuracy objectives are modest. However, a more rigorous approach can pay off, in the form of improved pointing, more accurate guide probe predictions, reduced residual field rotation and reliable world coordinate system information even when the detector is of axis. In this paper I propose a rigorous vector/matrix algorithm for generating pointing predictions on an imperfect telescope, with support for autoguiding, field stabilization and world coordinate systems even in difficult cases such as Nasmyth and coude.

关键词： telescope control world coordinates pointing astrometry

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The Sloan Digital Sky Survey telescope Performance Monitor

The Sloan Digital Sky Survey Telescope Performance Monitor

引用

conference on advanced telescope and instrumentation control software ii

作者： McGehee, PM Brinkmann, J Rockosi, C Long, D Snedden, SA Kleinman, SJ Nitta, A Harvanek, M Newman, PR Neilsen, EH Krzesinski, J Los Alamos Natl Lab Los Alamos NM 87545 USA

ISBN: (纸本)0819446270

The telescope Performance Monitor (TPM) installed at the Sloan Digital Sky Survey (SDSS) located at Apache Point Observatory provides access to real-time and archived engineering data. The modularity present in the underlying Experimental Physics and Industrial control System (EPICS) toolkit allows the observers and operations staff to develop their own approaches to data access and analysis. These techniques are summarized and the use of the TPM to solve critical project issues including analysis and correction of thermal management problems are presented.

关键词： SDSS EPICS diagnostics-real-time operations data archiving

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New control software of the 188cm telescope of Okayama Astrophysical Observatory

New control software of the 188cm telescope of Okayama Astro...

引用

conference on advanced telescope and instrumentation control software ii

作者： Yoshida, M Shimizu, Y Watanabe, E Yanagisawa, K Uraguchi, F Natl Astron Observ Okayama Astrophys Observ Okayama 7190232 Japan

ISBN: (纸本)0819446270

We developed the telescope control software for the 188cm telescope of Okayama Astrophysical Observatory (OAO) based on Java technology. Basically, the software consists of two processes running on separate Java virtual machines;one of which is the "Command Dispatcher (CD)" and the other is the "User Interface (UI)". Among the two, CD is the main engine/server of the telescope control, whereas UI is just a client. The "standard" UI we provide is a graphical user interface written in Java/Swing. CD communicates with the local control units (LCUs) of the telescope through RS232C. CD is a Java multi-thread program, in which a number of threads run simultaneously. The threads running in CD are the follows: UNIX socket servers for external communications, socket opener for on-demand open/close of a socket port, socket client manager, auto-guider and dome watcher, internal command dispatcher, status manager, status collector, RS232C writer and reader, logger, and control units. The above "control units" are software models ("objects") of the telescope system. We introduced four control units - "telescope", "'Dome", "Weather-Monitor", and "Pointing" - for telescope control. The first three units are simple software models of the real-worlds devices. The last one, "Pointing", is a unit which abstracts pointing procedure of the telescope. CD and UI communicate with each other using UNIX socket. The command protocol of this communication is fairly simple, and observation instruments, auto guider, or additional UI for remote observation are also able to communicate with CD through socket using this protocol. CD opens and closes socket ports for communication on demand according to the request of client process (UI, instruments etc.), so that any clients can be connected to CD dynamically.

关键词： telescope control software distributed control Java optical astronomy

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Mira - A case study

Mira - A case study

引用

conference on advanced telescope and instrumentation control software ii

作者： Kwok, SH Conrad, A WM Keck Observ Calif Assoc Res Astron Kamuela HI 96743 USA

ISBN: (纸本)0819446270

Mira is the name of a program that measures and improves the image quality of the Keck telescopes by correcting misalignments of the secondary mirror and adjusting the segments of the primary mirror. It is used regularly to achieve optimal focus calibration. Mira is completely written in Java. During the design phase, several software design patterns were followed resulting in short implementation times and a robust product. In this paper, we first discuss the operation of Mira, and then we present four examples of design patterns, describing the problem, the solution and the implementation.

关键词： software pattern mirror alignment java

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ArcVIEW: a LabVIEW-based astronomical instrument control system

ArcVIEW: a LabVIEW-based astronomical instrument control sys...

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conference on advanced telescope and instrumentation control software ii

作者： Ashe, M Bonati, M Heathcote, S SOAR Consortium La Serena Chile

ISBN: (纸本)0819446270

To meet the needs of the SOAR 4.2-m telescope first-generation instrument suite, as well as new instruments for the Blanco 4-m telescope, we developed a new camera controller system called ArcVEEW. In order to provide a strong foundation and rapid development cycle, we decided to build the system using National Instrument's LabVIEW environment. The advantages of this approach centers on the tools available for rapid prototyping, integration and testing of components. Over the past 2 years, we have taken ArcVIEW from a design document to the point of controlling two new instruments being built at CTIO. The IR imager, ISPI, will complete final testing this semester and go into use on the Blanco telescope in September 2002. The second instrument the SOAR Optical Imager, is due for completion this semester and will be the commissioning instrument for the SOAR telescope, for which first light is expected in early 2003.

关键词： instrument control LabVIEW ArcVIEW CCD optical infrared software distributed

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A distributed software correlator at the rapid prototyping array

A distributed software correlator at the rapid prototyping a...

引用

conference on advanced telescope and instrumentation control software ii

作者： Harp, GR Allen Telescope Array SETI Inst Mt View CA 94043 USA

ISBN: (纸本)0819446270

The Rapid Prototyping Array (RPA) is a toy radio telescope located 30 miles from U. C. Berkeley in Lafayette, CA. It serves primarily as a software development test bed for the Allen telescope Array (ATA). We have developed a minimally functional prototype of the ATA control system founded on C++, Java, and a CORBA-based distributed architecture. The system controls RPA pointing, electronics, and data processing, culminating in a real-time software correlator (i.e. an imaging system). This system has helped us characterize our preliminary design of the ATA control system. Overall, the distributed architecture provided successful, versatile control supporting a wide range of experiments from satellite tracking to beam characterization to celestial observation. However, some weaknesses in the CORBA communications layer were identified, and the synergies of mixing C++ and Java were balanced by paradigm mismatch between the languages. We learned that Java was as fast as C++ and supported more ready-made libraries. Based on these experiences, we changed our design to eliminate CORBA and build a pure Java system at the ATA, which is now under development.

关键词： ATA CORBA C plus Java software distributed architecture radio astronomy correlator

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software development for the Hobby-Eberly telescope's Segment Alignment Maintenance System using LabVIEW

Software development for the Hobby-Eberly Telescope's Segmen...

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conference on advanced telescope and instrumentation control software ii

作者： Hall, D Ly, W Howard, R Weir, J Rakoczy, J NASA George C Marshall Space Flight Ctr Huntsville AL 35812 USA

ISBN: (纸本)0819446270

The software development for an upgrade to the Hobby-Eberly telescope (HET) was done in LabVIEW. In order to improve the performance of the HET at the McDonald Observatory, a closed-loop system had to be implemented to keep the mirror segments aligned during periods of observation. The control system, called the Segment Alignment Maintenance System (SAMS), utilized inductive sensors to measure the relative motions of the mirror segments. software was developed in LabVIEW to tie the sensors, operator interface, and mirror-control motors together. Developing the software in LabVIEW allowed the system to be flexible, understandable, and able to be modified by the end users. Since LabVIEW is built using block diagrams, the software naturally followed the designed control system's block and flow diagrams, and individual software blocks could be easily verified. LabVIEW's many built-in display routines allowed easy visualization of diagnostic and health-monitoring data during testing. Also, since LabVIEW is a multi-platform software package, different programmers could develop the code remotely on various types of machines. LabVIEW's ease of use facilitated rapid prototyping and field-testing. There were some unanticipated difficulties in the software development, but the use of LabVIEW as the software "language" for the development of SAMS contributed to the overall success of the project.

关键词： LabVIEW software development segmented mirror mirror control HET

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