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Workstation software Framework

Workstation Software Framework

引用

2nd conference on advanced software and control for Astronomy

作者： Andolfato, L. Karban, R. ESO Garching Germany

ISBN: (纸本)9780819472298

The Workstation software Framework (WSF) is a state machine model driven development toolkit designed to generate event driven applications based on ESO VLT software. State machine models are used to generate executables. The toolkit provides versatile code generation options and it supports Mealy, Moore and hierarchical state machines. Generated code is readable and maintainable since it combines well known design patterns such as the State and the Template patterns. WSF promotes a development process that is based on model reusability through the creation of a catalog of state machine patterns.

关键词： Model driven development State machines Catalog of state patterns Design patterns

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The Large Binocular telescope azimuth and elevation encoder system

The Large Binocular Telescope azimuth and elevation encoder ...

引用

2nd conference on advanced software and control for Astronomy

作者： Ashby, David S. Sargent, Tom Cox, Dan Rosato, Jerry Brynnel, Joar G. Univ Arizona Large Binocular Telescope Observ Tucson AZ 85721 USA Univ Arizona Steward Observ Tucson AZ 85721 USA

ISBN: (纸本)9780819472298

A typical high-resolution encoder interpolator relies on careful mechanical alignment of the encoder read-heads and tight electrical tolerances of the signal processing electronics to ensure linearity. As the interpolation factor increases, maintaining these tight mechanical and electrical tolerances becomes impractical. The Large Binocular telescope (LBT) is designed to utilize strip-type encoders on the main axes. Because of the very large scale of the telescope, the accumulative length of the azimuth and elevation encoder strips exceeds 80 meters, making optical tape prohibitively expensive. Consequently, the designers of the LBT incorporated the far less expensive Farrand controls Inductosyn (R) linear strip encoder to encode the positions of the main axes and the instrument rotators. Since the cycle pitch of these encoders is very large compared to that of optical strip encoders, the interpolation factor must also be large in order to achieve the 0.005 arcsecond encoder resolution as specified. The authors present a description of the innovative DSP-based hardware / software solution that adaptively characterizes and removes common systematic cycle-to-cycle encoder interpolation errors. These errors can be caused by mechanical misalignment, encoder manufacturing flaws, variations in electrical gain, signal offset or cross-coupling of the encoder signals. Simulation data are presented to illustrate the performance of the interpolation algorithm, and telemetry data are presented to demonstrate the actual performance of the LBT main-axis encoder system.

关键词： LBT MCS control encoder interpolation Inductosyn DSP

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FPGA based control system for space instrumentation

FPGA based control system for space instrumentation

引用

2nd conference on advanced software and control for Astronomy

作者： Di Giorgio, Anna. M. Irelli, Pasquale Cerulli Nuzzolo, Francesco Orfei, Renato Spinoglio, Luigi Liu, Giovanni S. Saraceno, Paolo INAF Ist Fis Spazio Interplanetario Via Fosso Cavaliere 100 I-00143 Rome Italy

ISBN: (纸本)9780819472298

The prototype for a general purpose FPGA based control system for space instrumentation is presented, with particular attention to the instrument control application software. The system HW is based on the LEON3FT processor, which gives the flexibility to configure the chip with only the necessary HW functionalities, from simple logic up to small dedicated processors. The instrument control SW is developed in ANSI C and for time critical (< 10 mu s) commanding sequences implements an internal instructions sequencer, triggered via an interrupt service routine based on a HW high priority interrupt.

关键词： instrument control FPGA Real Time Applications Sequencer

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The GIANO control software system

The GIANO control software system

引用

2nd conference on advanced software and control for Astronomy

作者： Rossetti, Emanuel Oliva, Ernesto Origlia, Livia Osservatorio Astron Bologna INAF Via Ranzani 1 I-40127 Bologna Italy INAF Osserv Astrofisico Arcetri I-50125 Florence Italy INAF Telescopio Nazl Galileo Santa Cruz De La Palma TF Spain

ISBN: (纸本)9780819472298

GIANO is an ultra-stable IR echelle spectrometer, optimized for both low (R similar or equal to 400) and high (R similar or equal to 50, 000) resolution, that will be installed at the Nasmyth-B focus of the Italian national telescope (TNG). At the beginning of this year the assembling phase of GIANO has started, at the Infrared Laboratory of INAF-Arcetri, and is currently in progress. We describe, here, the general control software structure of the instrument concerning both the user interface and the controls of all subsystems. We present also the software interface which provides the communication with the cryogenic system of the instrument and is handled by means of a Programmable Logic controller.

关键词： control software PLC infrared spectrometer

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CADOR and TAROT: A Virtual Observatory

CADOR and TAROT: A Virtual Observatory

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2nd conference on advanced software and control for Astronomy

作者： Bourez-Laas, Myrtille Vachier, Frederic Klotz, Alain Damerdji, Yassine Boer, Michel CNRS Observ Haute Provence F-04870 St Michel France CNRS OPM Inst Mecanique Celeste & calcul Ephemerides F-75014 Paris France CNRS UPS Ctr Etude Spatiale Rayonnements F-31028 Toulouse France Univ Liege Lab Astrophys & Geophys B-4000 Liege Belgium

ISBN: (纸本)9780819472298

TAROT (telescope Action Rapide pour les Objets Transitoires - Rapid Action telescope for Transient Objects) is a network of two robotic ground based telescopes. The telescopes are fully automated, from the scheduling of the observation requests to the processing of the data. All the applications use a specific automated processing pipeline which has been continuously improved. CADOR, (Coordination et Analyse des Donnees d'Observatoires Robotises - Coordination and Data Analysis of Robotic Observatories) is a set of data base servers which manage TAROT telescopes. CADOR is the prime interface to request new observations from TAROT and to access all images saved with the possibility to make additional processing and analysis. Tarot and Cador are compliant with Virtual Observatory standard and protocols.

关键词： automated telescope data base virtual observatory

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A component based astronomical visualization tool for instrument control

A component based astronomical visualization tool for instru...

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2nd conference on advanced software and control for Astronomy

作者： Briegel, Florian Berwein, Jurgen Kittmann, Frank Pavlo, Alex(ey) Max Planck Inst Astron D-69117 Heidelberg Germany

ISBN: (纸本)9780819472298

For various astronomical instruments developed at the Max-Planck-Institute-Heidelberg there was a need for a highly flexible display and control tool. Many display tools (ximtool, DS9, skycat,..) are available for astronomy, but. all this applications are monolitic and can't be easily enriched by plugins for interaction with the graphical display, and other functionalities for remote access and control of the instrument and data pipepline. It was developed on top of Trolltechs Cross-Platform Rich Client Development Framework Qt,(1) the modern middleware Internet Communications Engine(2) from ZeroC and the template based SOA developer framework for astronomical instrumentation NICE.(3) The display tool is used on the Calar Alto Observatory (Spain) as a guider for wide field imager and guider at the Wise Observatory (Israel) and for the LBT interferometer Linc-Nirvana, (USA).

关键词： Cameras Astronomy Human-machine interfaces Observatories CCD cameras Visualization control systems Astronomical instrumentation Imaging systems Internet

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The STELLA robotic observatory: first two years of high-resolution spectroscopy

The STELLA robotic observatory: first two years of high-reso...

引用

2nd conference on advanced software and control for Astronomy

作者： Weber, Michael Granzer, Thomas Strassmeier, Klaus G. Woche, Manfred Astrophys Inst Potsdam An Der Sternwarte 16 D-14482 Potsdam Germany

ISBN: (纸本)9780819472298

The STELLA project consists of two robotic 1.2m telescopes to simultaneously monitor stellar activity with a high resolution echelle spectrograph on one telescope, and a photometric imaging instrument on the other telescope. The STELLA observatory is located at the Observatorio del Teide on the Canary island of Tenerife. The STELLA Echelle spectrograph (SES) has been operated in robotic mode for two years now, and produced approximately 10,000 spectra of the entire optical range between 390 and 900nm at a spectral resolution of 55,000 with a peak shutter-open time of 93%. Although we do not use an iodine cell nor an actively stabilized chamber, its average radial velocity precision over the past two years was 60 to 150 m/s rms, depending on target. The Wide-Field STELLA Imaging Photometer (WIFSIP) is currently being tested and will enter operation early 2009. In this paper, we present an update report on the first two years of operation.

关键词： Spectrographs Robotic telescope

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software in the CARMA Heterogeneous Millimeter-wave Array

Software in the CARMA Heterogeneous Millimeter-wave Array

引用

2nd conference on advanced software and control for Astronomy

作者： Scott, Stephen L. CALTECH Owens Valley Radio Observ Big Pine CA 93513 USA

ISBN: (纸本)9780819472298

The Combined Array for Research in Millimeter-wave Astronomy (CARMA) is a 15 element heterogeneous millimeter-wave array developed and operated by a university consortium that will be expanded to 23 elements in 2008. Commissioning began in August 2005 after completion of the relocation of antennas from the Owens Valley Radio Observatory (OVRO) and the Berkeley-Illinois-Maryland Association (BIMA) arrays to a new high site and initial scientific operations began in April 2006. The array operates in the 3-mm and 1-mm bands and has a maximum resolution of 0.15 arc seconds. Most of the software and computing infrastructure for the array is new, allowing modem technology to be introduced and to provide a common interface for the disparate antenna types. The new system is proving to be both easy to use for routine observations and yet capable enough for the development of new observing techniques by the experienced astronomer. Some of the details of the computing and software are described here, with emphasis on the control system.

关键词： CARMA millimeter-wave interferometry radio astronomy control systems software

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Beating the cost curve and redefining the scientific telescope utility using 0.4-Meter Robotic Cluster Network

Beating the cost curve and redefining the scientific telesco...

引用

conference on Ground-Based and Airborne instrumentation for Astronomy ii

作者： Dubberley, Matthew A. Walker, Zachary A. Haldeman, Benjamin J. Las Cumbres Observ Global Telescope Goleta CA 93117 USA

ISBN: (纸本)9780819472229

Las Cumbres Observatory Global telescope (LCOGT) is redefining the function of robotic telescopes by deploying 0.4 meter telescopes that act as a highly networked intelligent instrument. The 0.4 meter telescopes, (P4) are optimized for quick and accurate object acquisition and tracking. This minimizes response time and enables the leveraging of the instrument. A single P4 can independently execute multiple science programs concurrently or team up with other P4s for deeper or multi-color observations of a single target. The intelligent control software will optimize the observation schedule for each individual telescope and the entire network. LCOGT is deploying 6 networked clusters consisting of four P4s around the world, providing capacity and versatility beyond the classical observatory. Each P4 has zero slippage, no backlash friction systems, and is currently achieving 20 deg/s slewing. Blind pointing is currently 8 arcsec RMS. Using the AG acquisition routine, the drive will have repeatable pointing to within 0.6 arcsec within 12 seconds from anywhere on the sky. Other features include wind buffet correction, rapid thermalization, dual autoguiders, novel scanning flat fielding device, large 20 kg instrument capacity, high speed instrument changer, and a stiff split ring mount.

关键词： Robotic telescope Network Cost Friction Drive Direct Drive

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The RTS2 protocol

The RTS2 protocol

引用

2nd conference on advanced software and control for Astronomy

作者： Kubanek, Petr Jelinek, Martin French, John Prouza, Michal Vitek, Stanislav Castro-Tirado, Alberto J. Reglero, Victor GACE Valencia Valencia Spain Inst Astrofis Andalucia IAA CSIC Granada Spain Univ Coll Dublin Dublin Ireland Fyzikalni Ustav Akad Ved Prague Czech Republic

ISBN: (纸本)9780819472298

Remote telescope System 2nd version (RTS2) is an open source project aimed at developing a software environment to control a fully robotic observatory. RTS2 consists of various components, which communicate via an ASCii based protocol. As the protocol was from the beginning designed is an observatory control system, it provides some unique features, which are hard to find in the other communication systems. These features include advanced synchronisation mechanisms and strategies for setting variables. This presentation describes the protocol and its unique features. It also assesses protocol performance, and provides examples how the RTS2 library can be used to quickly build an observatory control system.

关键词： telescopes Binary data Observatories Cameras Image processing Telecommunications control systems Optical filters Robotics software development

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