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

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Design and implementation of the primary and secondary mirror control system for NST - art. no. 62740Z

Design and implementation of the primary and secondary mirro...

引用

conference on advanced software and control for Astronomy

作者： Yang, G. New Jersey Inst Technol Newark NJ 07104 USA

ISBN: (纸本)0819463396

The 1.6-meter New Solar telescope (NST) will replace the 65 cm reflector that is currently being used at Big Bear Solar Observatory (BBSO). Some technologies new to solar telescopes, including Active Optics, will be employed in NST project. The goal of Active Optics is to correct the low frequency telescope aberrations by adjusting the figure of primary mirror and the position of the secondary mirror. The Active Optics control Subsystem (AOCS) is part of the telescope control System (TCS) for NST. The AOCS will cooperate with the Wavefront Sensing control Subsystem to correct the lower order aberrations of the telescope system. When fully developed, it will work in close-loop. The wavefront aberration information will be obtained from the wavefront sensor and corresponding corrections will be applied to the primary mirror and the secondary mirror. In this paper, the design and the implementation of the AOCS will be described in detail.

关键词： active optics control software object-oriented XML Java

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RTS2:: a powerful robotic observatory manager

RTS2:: a powerful robotic observatory manager

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conference on advanced software and control for Astronomy

作者： Kubanek, Petr Jelinek, Martin Vitek, Stanislav Postigo, Antonio de Ugarte Nekola, Martin French, John Astron Akad Ceske Republ Ondrejov Czech Republic

ISBN: (纸本)0819463396

RTS2, or Remote telescope System, 2nd Version, is an integrated package for remote telescope control under the Linux operating system. It is designed to run in fully autonomous mode, picking targets from a database table, storing image meta data to the database, processing images and storing their WCS coordinates in the database and offering Virtual-Observatory enabled access to them. It is currently running on various telescope setups world-wide. For control of devices from various manufacturers we developed an abstract device layer, enabling control of all possible combinations of mounts, CCDs, photometers, roof and cupola controllers. We describe the evolution of RTS2 from Python-based RTS to C and later C++ based RTS2, focusing on the problems we faced during development. The internal structure of RTS2, focusing on object layering, which is used to uniformly control various devices and provides uniform reporting layer, is also discussed.

关键词： robotic telescopes telescope software

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Remir-NCS -: The new control software for RemIr camera

Remir-NCS -: The new control software for RemIr camera

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conference on advanced software and control for Astronomy

作者： D'Alessio, F. Vitalia, F. Testa, V. Antonelli, L. A. Molinari, E. Chincarini, G. Zerbi, F. M. Rodono, M. Covino, S. Tosti, G. Conconi, P. Malaspina, G. Palazzif, E. Osserv Astron Roma INAF I-00040 Monte Porzio Catone Italy

ISBN: (纸本)0819463396

REMIR is the NIR camera of the automatic REM (Rapid Eye Mount) telescope located at ESO La Silla Observatory Chile and dedicated to monitor the afterglow of Gamma Ray Burst events. The REMIR camera is composed by a set of sub systems: the array controller, the cooling system, the temperature and the pressure monitors, the filter wheel controller, the dither wedge controller. During 2005, a complete re-writing of the REMIR software control system started in order to optimize the system performances: the new configuration will adopt a client server architecture, where a supervisor system accepts via socket the data acquisition queries from AQUA (the acquisition data suite), manages the several components of the camera and the communication with the telescope control system. Here we describe in particular the philosophy adopted to realize the general control system, the sub systems and the communication protocols.

关键词： control software near infrared instrumentation

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Event-driven James Webb Space telescope operations using on-board JavaScripts - art. no. 62740A

Event-driven James Webb Space Telescope operations using on-...

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conference on advanced software and control for Astronomy

作者： Balzano, V. Zak, D. Space Telescope Sci Inst Baltimore MD 21218 USA

ISBN: (纸本)0819463396

The James Webb Space telescope (JWST) will use an event-driven system architecture to provide efficient and flexible operations as initiated by a simplified, high-level ground command interface. Event-driven operations is provided through the use of an on-board COTS JavaScript engine hosted within the payload flight software. After presenting the overall software architecture, we summarize the trade study that led to the selection of a commercial JavaScript interpreter and review our experiences developing scripts over the past year. Our script development approach is based upon the process successfully used at Space telescope Science Institute for the last six Hubble Space telescope science instruments. The major characteristics of our process are 1) coordinated development of the operational scripts and the flight software, 2) an incremental buildup of the operational requirements, and 3) recurring integrated testing. Our iterative script implementation process addresses how to gather requirements from a geographically dispersed team, and then how to design, build, and test the script software to accommodate the changes that are inevitable as Right hardware is built and tested. The concurrent development of the operational scripts and the flight software enables early and frequent "test- as-you-will-fly" verification, thus reducing the risk of on-orbit software problems.

关键词： event-driven operations software development concepts space science operations

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Active remote observing system for the 1-m telescope at Tonantzintla observatory

Active remote observing system for the 1-m telescope at Tona...

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conference on advanced software and control for Astronomy

作者： Bernal, Abel Martinez, Luis A. Hernandez, Hector Garfias, Fernando Angeles, Fernando Natl Autonomous Univ Mexico Inst Astron Mexico City 04510 DF Mexico

ISBN: (纸本)0819463396

We have designed and installed a new active remote observing system for the 1-m, f/15 telescope at the Tonantzintla Observatory. This remote system is operated in real-time through the Internet, allowing an observer to control the building, the telescope (pointing, guiding and focusing) and the CCD image acquisition at the main and finder telescopes from the Instituto de Astronomia headquarters in Mexico City (150 KM away). The whole system was modeled within the Unified Modeling Language (UML) and the design has proved to be versatile enough for a variety of astronomical instruments. We describe the system architecture and how different subsystems (telescope control, main telescope and finder image acquisition, weather station, videoconference, etc.) that are based on different operative system platforms (Linux, Windows, uIP) have been integrated. We present the first results of an IPv6 over IPv4 tunnel. Recent remote direct imaging and spectroscopic observations have been used to test the astronomical site. We conclude that this remote system is an excellent tool for supporting research and graduated observational astronomy programs.

关键词： active remote observing UML telescopes

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LUCIFER VR:: a virtual instrument for the LBT

LUCIFER VR:: a virtual instrument for the LBT

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conference on advanced software and control for Astronomy

作者： Polsterer, Kai L. Juette, Marcus Knierim, Volker Lehmitz, Michael Mandel, Holger Ruhr Univ Bochum Inst Astron D-44780 Bochum Germany

ISBN: (纸本)0819463396

Lucifer VR is a virtually realized instrument that was build in order to allow improved pre-integration software tests, training of observers as well as providing educational access. Beside testing the instrument hardware in combination with e.g. a telescope simulator, software tests need to be done. A virtual instrument closes the gap between regression tests and testing the control software with the integrated instrument. Lucifer VR allows much earlier tests and reduces the amount of time needed to combine the software with the hardware. By modeling the instrument in a simulator, motion times can be calculated very easily and the position of all instrument units can be traced. Especially when using complex mechanisms like a MOS unit a virtual instrument makes software development less time consuming. Lucifer VR consists of three parts;one for handling the communication, another to simulate the hardware and finally a part to visualize the whole instrument in three dimensions.

关键词： LBT instrumentation infrared spectrograph MOS simulator control software software test methods

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Auto-alignment and image tracking system for the SUNRISE telescope

Auto-alignment and image tracking system for the SUNRISE tel...

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conference on advanced software and control for Astronomy

作者： Schmidt, W. Berkefeld, T. Feger, B. Friedlein, R. Gerber, K. Heidecke, F. Kentischer, T. von der Luehe, O. Sigwarth, M. Soltau, D. Waelde, E. Kiepenheuer Inst Sonnenphys D-79104 Freiburg Germany

ISBN: (纸本)0819463396

The 1m balloon-borne solar telescope SUNRISE will be equipped with a wave-front sensing system for automatic in-flight focusing and alignment of the telescope and for high-precision image tracking. A six-element wavefront sensor measures low order aberrations of the telescope, including defocus and coma. The correction is achieved by moving the focusing mirror and the telescope secondary, respectively, in a closed-loop circuit. The same system measures image motion. The instrument requirements for the tracking are a dynamical range of about 30 Hz and a precision of about 0.005 arcs in the sky. The image motion signal feeds a closed-loop control system that drives both the tip-tilt mirror assembly and the mirrors that are needed for focusing and alignment. The tip-tilt unit is a dual-stage system, built at the Kiepenheuer-Insitut, consisting of a slow component with a large range of about 60 arcs and a fast component with a short range and high bandwidth. A breadboard-version of the Correlating Wavefront Sensor has been successfully tested at the German Vacuum Tower telescope on Tenerife in summer of 2005. A closed-loop bandwidth of 80 Hz was measured for the tracking system. The wave-front sensor detected image aberrations pre-set by the telescope's adaptive optics system with the required accuracy. SUNRISE will be flown in long duration stratospheric balloon flights, with a first scientific flight in 2009.

关键词： Sun robotic alignment wave-front sensing active optics

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The Java based control software of the LUCIFER instrument

The Java based control software of the LUCIFER instrument

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conference on advanced software and control for Astronomy

作者： Juette, Marcus Polsterer, Kai Knierim, Volker Luks, Thomas Ruhr Univ Bochum Inst Astron D-44780 Bochum Germany

ISBN: (纸本)0819463396

The LUCIFER instrument is a near infrared spectroraph/imager with MOS for the Large Binocular telescope. Here we present the final software design, the interrelation of the software packages and the used hardware architecture. The software package is completely running under Java using intensively its Remote Method Invocation (RMI) mechanisms in a distributed system environment. The use of Java helped us to cope with a small amount of available manpower for the SW development, providing many native built-in Java methods and classes, which speed up the development process a lot. The control software will be finally installed on a Solaris OS, hosted on a Sun Fire V880 server, which results from a specific hardware constraint. For testin g purposes a standard Linux environment is used. This shows another big Java advantage, the platform independency. The "First Light" of LUCIFER 1 is estimated for summer/fall 2007, following LUCIFER 2 one year later.

关键词： near-infrared LBT object-oriented Java instrument software distributed system

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Interconnecting astronomical networks: Evolving from single networks to meta-networks - art. no. 627409

Interconnecting astronomical networks: Evolving from single ...

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conference on advanced software and control for Astronomy

作者： White, R. R. Allan, A. Evans, S. Vestrand, W. T. Wren, J. Wozniak, P. Los Alamos Natl Lab ISR Div Los Alamos NM 87545 USA

ISBN: (纸本)0819463396

Over the past four years we have seen continued advancement in network technology and how those technologies are beginning to enable astronomical science. Even though some sociological aspects are hindering full cooperation between most observatories and telescopes outside of their academic or institutional connections, an unprecedented step during the summer of 2005 was taken towards creating a world-wide interconnection of astronomical assets. The telescope Alert Operations Network System (TALONS), a centralized server/client bi-directional network developed and operated by Los Alamos National Laboratory, integrated one of its network nodes with a node from the eScience telescopes for Astronomical Research (eSTAR), a peer-to-peer agent based network developed and operated by The University of Exeter. Each network can act independently, providing support for their direct clients, and by interconnection provide local clients with access to;outside telescope systems, software tools unavailable locally, and the ability to utilize assets far more efficiently, thereby enabling science on a world-wide scale. In this paper we will look at the evolution of these independent networks into the worlds first heterogeneous telescope network and where this may take astronomy in the future. We will also examine those key elements necessary to providing universal communication between diverse astronomical networks.

关键词： robotic telescope communication interconnection network servers clients

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The active optics control software for the VST telescope

The active optics control software for the VST telescope

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conference on advanced software and control for Astronomy

作者： Schipani, P. Brescia, M. Marty, L. Osserv Astron Capodimonte INAF I-80131 Naples Italy

ISBN: (纸本)0819463396

The VST active optics software must basically provide the analysis of the image coming from the wavefront sensor (a 10x10 subpupils Shack Hartmann device) and the calculation of primary mirror forces and secondary mirror displacements to correct the intrinsic aberrations of the optical system and the ones originated for thermal or gravity reasons. The software architecture, the simulation code to validate the results and the status of work are here described.

关键词： active optics image analysis VST telescope control software

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