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Using EPICS and VxWorks for real-time motion control of the Altair adaptive optics instrument for Gemini.

Using EPICS and VxWorks for real-time motion control of the ...

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conference on advanced telescope and instrumentation control software ii

作者： Ebbers, AW Dunn, J

ISBN: (纸本)0819446270

The Instrument Group in the National Research Council of Canada's Herzberg Institute of Astrophysics develops instrumentation for large Astronomical telescopes including Altair (Gemini's ALTitude conjugate Adaptive optics for the InfraRed). This paper discusses how we responded to a need for adaptive intelligence and complex choreography and sequencing of mechanisms in the design of Altair's motion control systems. Our primary goal has been to maximize code reusability without sacrificing performance or flexibility.

关键词： EPICS VxWorks software real-time motion control Altair Gemini

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Command system architecture for NGST

Command system architecture for NGST

引用

conference on advanced telescope and instrumentation control software ii

作者： Balzano, VA Rehm, KD Space Telescope Sci Inst AURA Baltimore MD 21218 USA

ISBN: (纸本)0819446270

NGST ground software and flight software will enable exciting scientific research programs that will address fundamental questions about the structure of the universe and the evolution of galaxies, stars and planets. The design of the spacecraft and instrument command system architecture acknowledges from project start that the ground software and flight software are parts of a single integrated system. A layered architecture is presented where the ground system software provides descriptions of "what to do" with the spacecraft and science instruments, while the flight software provides the detailed "how to do" rules required to execute these requests. All specific knowledge about onboard computer memory structures, hardware device communication rules, and spacecraft/science instrument operational sequences will be encapsulated onboard the spacecraft. The ground system will simply supply high-level alphanumeric requests that the flight software knows how to interpret and perform.

关键词： scientific spacecraft software layered software architecture spacecraft software automation

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Upgraded control, acquisition program and user interface for the Manchester Echelle Spectrometer at San Pedro Martir.

Upgraded control, acquisition program and user interface for...

引用

conference on advanced telescope and instrumentation control software ii

作者： Gutiérrez, L Murillo, J Quiroz, F Pedrayes, MH Meaburn, J López, JA Univ Nacl Autonoma Mexico Observ Astron Nacl Ensenada Baja California Mexico

ISBN: (纸本)0819446270

We describe the recent upgrade of the Manchester Echelle Spectrometer, currently in use at San Pedro Martir. This upgrade has included a user interface and a new CCD acquisition software. The spectrometer control is now done by a microcontroller, whose inputs are new sensors and encoders installed inside the spectrometer. The instrument control is now fully carried out from a graphical user interface running in a personal computer. The acquisition computer sends the images to the GUI through an ethernet link. In this paper, we present the general scheme and the programs developed for Linux (in C++ and Tcl/Tk) that permits an easy integral operation of the instrument, as well as the creation of scripts intended to the optimization of the observing run and the future interaction with the telescope and the guider. This upgraded system has been operated successfully during several campaigns in the 2.1-meter telescope at Observatorio Astronomico Nacional in San Pedro MdAir.

关键词： spectrometer GUI sequences

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The Ultracam camera control and data acquisition system

The Ultracam camera control and data acquisition system

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conference on advanced telescope and instrumentation control software ii

作者： Beard, S Vick, A Atkinson, D Dhillon, V Marsh, T McLay, S Stevenson, M Tierney, C UK Astron Technol Ctr Edinburgh EH9 3HJ Midlothian Scotland

ISBN: (纸本)0819446270

Ultracam is a high speed, three channel CCD camera designed to provide imaging photometry at high temporal resolution, allowing the study of rapidly changing astronomical phenomena such as eclipses, rapidly flickering light curves and occultation events. It is designed to provide frame rates up to 500 Hz with minimum inter-frame dead time and to time-tag each frame to within 1 millisecond of UT. The high data rates that this instrument produces, together with its use as a visitor instrument at a number of observatories, have lead to a highly modular design. Each major service (camera, control, sequencing, data handlers, etc.) is a separate process that communicates using XML documents via HTTP transport, allowing the services to be redeployed or reconfigured with minimal effort. The use of XML and HTTP also allows a web browser to act as a front end for any of the services, as well as providing easy access to services from other control systems. The overall design allows for simple re-engineering for a variety of imaging systems, and is already expected to provide control of IR arrays for the UKIRT Wide-Field Camera project. The instrument has been successfully commissioned on the William Herschel telescope.

关键词： instrumentation ultracam time resolution imaging photometry

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ALMA software architecture

ALMA software architecture

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conference on advanced telescope and instrumentation control software ii

作者： Schwarz, J Raffi, G European So Observ D-85748 Garching Germany

ISBN: (纸本)0819446270

The Atacama Large Millimeter Array (ALMA) is a joint project involving astronomical organizations in Europe and North America. ALMA will consist of at least 64 12-meter antennas operating in the millimeter and sub-millimeter range. It will be located at an altitude of about 5000m in the Chilean Atacama desert. The primary challenge to the development of the software architecture is the fact that both its development and runtime environments will be distributed. Groups at different institutes will develop the key elements such as Proposal Preparation tools, Instrument operation, On-line calibration and reduction, and Archiving. The Proposal Preparation software will be used primarily at scientists' home institutions (or on their laptops), while Instrument Operations will execute on a set of networked computers at the ALMA Operations Support Facility. The ALMA Science Archive, itself to be replicated at several sites, will serve astronomers worldwide. Building upon the existing ALMA Common software (ACS), the system architects will prepare a robust framework that will use XML-encoded entity objects to provide an effective solution to the persistence needs of this system, while remaining largely independent of any underlying DBMS technology. Independence of distributed subsystems will be facilitated by an XML- and CORBA-based pass-by-value mechanism for exchange of objects. Proof of concept (as well as a guide to subsystem developers) will come from a prototype whose details will be presented.

关键词： corba XML ALMA

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CORBA-based Common software for the ALMA project

CORBA-based Common Software for the ALMA project

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conference on advanced telescope and instrumentation control software ii

作者： Chiozzi, G Gustafsson, B Jeram, B Plesko, M Sekoranja, M Tkacik, G Zagar, K European So Observ D-85748 Garching Germany

ISBN: (纸本)0819446270

The Atacama Large Millimeter Array (ALMA) is a joint project between astronomical organizations in Europe and North America. ALMA will consist of at least 64 12-meter antennas operating in the millimeter and sub-millimeter range, with baselines up to 14 km. It will be located at an altitude above 5000m in the Chilean Atacama desert. The ALMA Common software (ACS) provides a software infrastructure common to all partners and consists of a documented collection of common patterns and of components that implement those patterns. The heart of ACS is an object model based on Distributed Objects (DOs), implemented as CORBA objects. The teams responsible for the control system development use DOs as the basis for components and devices such as an antenna mount control. ACS provides common CORBA-based services such as logging, error and alarm management, configuration database and lifecycle management. A code generator creates a Java Bean for each DO. Programmers can write Java client applications by connecting those Beans with data-manipulation and visualization Beans. ACS is based on the experience gained in the astronomical and particle accelerator domains, and reuses and extends proven concepts and components. Although designed for ALMA, ACS can be used in other new control systems, since it implements proven design patterns using state of the art, stable and reliable technology. This paper presents the architecture of ACS and its status, detailing the object model and major services.

关键词： CORBA control software ALMA

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Distributed framework for dynamic telescope and instrument control

Distributed framework for dynamic telescope and instrument c...

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conference on advanced telescope and instrumentation control software ii

作者： Ames, TJ Case, L NASA Goddard Space Flight Ctr Greenbelt MD 20771 USA

ISBN: (纸本)0819446270

Traditionally, instrument command and control systems have been developed specifically for a single instrument. Such solutions are frequently expensive and are inflexible to support the next instrument development effort. NASA Goddard Space Flight Center is developing an extensible framework, known as Instrument Remote control (IRC) that applies to any kind of instrument that can be controlled by a computer. IRC combines the platform independent processing capabilities of Java with the power of the Extensible Markup Language (XML). A key aspect of the architecture is software that is driven by an instrument description, written using the Instrument Markup Language (IML). IML is an XML dialect used to describe graphical user interfaces to control and monitor the instrument, command sets and command formats, data streams, communication mechanisms, and data processing algorithms. The IRC framework provides the ability to communicate to components anywhere on a network using the JXTA protocol for dynamic discovery of distributed components. JXTA (see http://***) is a generalized protocol that allows any devices connected by a network to communicate in a peer-to-peer manner. IRC uses JXTA to advertise a device's IML and discover devices of interest on the network. Devices can join or leave the network and thus join or leave the instrument control environment of IRC. Currently, several astronomical instruments are working with the IRC development team to develop custom components for IRC to control their instruments. These instruments include: High resolution Airborne Wideband Camera (HAWC), a first light instrument for the Stratospheric Observatory for Infrared Astronomy (SOFIA);Submillimeter And Far Infrared Experiment (SAFIRE), a Principal Investigator instrument for SOFIA;and Fabry-Perot Interferometer Bolometer Research Experiment (FIBRE), a prototype of the SAFIRE instrument, used at the Caltech Submillimeter Observatory (CSO). Most recently, we have been w

关键词： astronomy infrared astronomy XML instrument : description telescope : control SOFIA NASA : GSFC Java IML

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Receiver control for the Submillimeter Array

Receiver control for the Submillimeter Array

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conference on advanced telescope and instrumentation control software ii

作者： Hunter, TR Wilson, RW Kimberk, R Leiker, PS Christensen, R Harvard Smithsonian Ctr Astrophys Cambridge MA 02138 USA

ISBN: (纸本)0819446270

Efficient operation of a submillimeter interferometer requires remote (preferably automated) control of mechanically tuned local oscillators, phase-lock loops, mixers, optics, calibration vanes and cryostats. The present control system for these aspects of the Submillimeter Array (SMA) will be described. Distributed processing forms the underlying architecture. In each antenna cabin, a serial network of up to ten independent 80C196 microcontroller boards attaches to the real-time PowerPC computer (running LynxOS). A multi-threaded, gcc-compiled program on the PowerPC accepts top-level requests via remote procedure calls (RPC), subsequently dispatches tuning commands to the relevant microcontrollers, and regularly reports the system status to optical-fiber-based reflective memory for common access by the telescope monitor and error reporting system. All serial communication occurs asynchronously via encoded, variable-length packets. The microcontrollers respond to the requested commands and queries by accessing non-volatile, rewriteable lookup-tables (when appropriate) and executing embedded software that operates additional electronic devices (DACs, ADCs, etc.). Since various receiver hardware components require linear or rotary motion, each microcontroller also implements a position servo via a one-millisecond interrupt service routine which drives a DC-motor/encoder combination that remains standard across each subsystem.

关键词： Submillimeter receiver microcontroller interferometry Gunn oscillator multiplier DC servo motor digital PLL

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VIMOS Instrument control software design:: an Object Oriented Approach

VIMOS Instrument Control Software design:: an Object Oriente...

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conference on advanced telescope and instrumentation control software ii

作者： Brau-Nogué, S Lucuix, C Observatoire Midi-Pyrénées (France)

ISBN: (纸本)0819446270

The Franco-Italian VIMOS instrument is a VIsible imaging Multi-Object Spectrograph with outstanding multiplex capabilities, allowing to take spectra of more than 800 objects simultaneously, or integral field spectroscopy mode in a 54x54 arcsec area. VIMOS is being installed at the Nasmyth focus of the third Unit telescope of the European Southern Observatory Very Large telescope (VLT) at Mount Paranal in Chile. This paper will describe the analysis, the design and the implementation of the VIMOS Instrument control System, using UML notation. Our control group followed an Object Oriented software process while keeping in mind the ESO VLT standard control concepts. At ESO VLT a complete software library is available. Rather than applying waterfall lifecycle, ICS project used iterative development, a lifecycle consisting of several iterations. Each iteration consisted in: capture and evaluate the requirements, visual modeling for analysis and design, implementation, test, and deployment. Depending of the project phases, iterations focused more or less on specific activity. The result is an object model (the design model), including use-case realizations. An implementation view and a deployment view complement this product. An extract of VIMOS ICS UML model will be presented and some implementation, integration and test issues will be discussed.

关键词： VLT Instrument control software Object Oriented Iterative Development UML 2TUP

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Computing design principles for robotic telescopes

Computing design principles for robotic telescopes

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conference on advanced telescope and instrumentation control software ii

作者： Bowman, MK Ford, MJ Lett, RDJ McKay, DJ Mücke-Herzberg, D Norbury, MA Telescope Technol Ltd Birkenhead CH41 1NQ Merseyside England

ISBN: (纸本)0819446270

telescopes capable of making observing decisions independent of human supervision have become a reality in the 21st century. These new telescopes are likely to replace automated systems as the telescopes of choice. A fully robotic implementation offers not only reduced operating costs, but also significant gains in scientific output over automated or remotely operated systems. The design goals are to maximise the telescope operating time and minimise the cost of diagnosis and repair. However, the demands of a robotic telescope greatly exceed those of its remotely operated counterpart, and the design of the computing system is key to its operational performance. This paper outlines the challenges facing the designer of these computing systems, and describes some of the principles of design which may be applied. Issues considered include automatic control and efficiency, system awareness, robustness and reliability, access, security and safety, as well as ease-of-use and maintenance. These requirements cannot be considered simply within the context of the application software. Hence, this paper takes into account operating system, hardware and environmental issues. Consideration is also given to accommodating different levels of manual control within robotic telescopes, as well as methods of accessing and overriding the system in the event of failure.

关键词： robotic telescope software design control computing security automatic robust efficiency

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