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共 329 条记录，以下是141-150 订阅

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Object-oriented communications for the New Solar telescope's telescope control System: design and implementation - art. no. 62741Q

Object-oriented communications for the New Solar Telescope's...

引用

conference on advanced software and control for Astronomy

作者： Shumko, Sergiy Yang, Guo Big Bear Solar Observ Big Bear City CA 92314 USA

ISBN: (纸本)0819463396

Big Bear Solar Observatory (BBSO) is building the 1.6 meter New Solar telescope (NST). The telescope control System (TCS) of NST consists of many systems and applications and heterogeneous computer platforms. It is a critical task to design a robust, flexible and reliable - yet not over-complicated - communications for TCS. This paper describes the design and implementation of NST's communication software and protocols. The software is based on the Internet communication engine (Ice) middleware and uses eXtensible Markup Language (XML) for messaging.

关键词： NST telescope control software communications XML middleware

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software control of the 3 active surfaces of the Thirty-Meter telescope - art. no. 62740F

Software control of the 3 active surfaces of the Thirty-Mete...

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conference on advanced software and control for Astronomy

作者： Daly, P. N. Marshall, R. E. Sirota, M. J. Jared, R. C. Natl Opt Astron Observ New Initiat Off Tucson AZ 85719 USA

ISBN: (纸本)0819463396

The Thirty Meter telescope (TMT) is a collaborative project between the California Institute of Technology (CIT), the University of California (UC), the Association of Universities for Research in Astronomy (AURA) and the Association of Canadian Universities for Research in Astronomy (ACURA). Current activity is focused on the design and development phase (DDP) of all systems. For the TMT to achieve seeing and diffraction limited performance, the telescope-related software systems will have to work in concert to precisely control all 738 primary mirror (M1) segments along with the active secondary mirror (M2) and an articulated tertiary mirror (M3). In this paper we discuss the conceptual design of the software control systems for these surfaces and their integration into a cohesive whole.

关键词： TMT control systems software AO WFS

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The telescope control system of the new solar telescope at big bear solar observatory - art. no. 62741Y

The telescope control system of the new solar telescope at b...

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conference on advanced software and control for Astronomy

作者： Yang, G. Varsik, J. R. Shumko, S. Denker, C. Choi, S. Verdonia, A. P. Wang, H. New Jersey Inst Technol Newark NJ 07104 USA

ISBN: (纸本)0819463396

The New Solar telescope (NST) is an advanced solar telescope at Big Bear Solar Observatory (BBSO). It features a 1.6-m clear aperture with an off-axis Gregorian configuration. An open structure will be employed to improve the local seeing. The NST telescope control System (TCS) is a complex system, which provides powerful and robust control over the entire telescope system. At the same time, it needs to provide a simple and clear user interface to scientists and observers. We present an overview of the design and implementation of the TCS as a distributed system including its several subsystems such as the telescope Pointing and Tracking Subsystem, Wavefront Sensing Subsystem etc. The communications between different subsystems are handled by the Internet Communication Engine (Ice) middleware.

关键词： solar telescopes control systems distributed communication middleware XML

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A standard python environment for software applications at the Robert C. Byrd Green Bank telescope (GBT) - art. no. 627405

A standard python environment for software applications at t...

引用

conference on advanced software and control for Astronomy

作者： Radziwill, Nicole M. Shelton, Amy L. Natl Radio Astron Observ Green Bank WV 24944 USA

ISBN: (纸本)0819463396

Since 2003, the monitor and control software systems for the Robert C. Byrd Green Bank telescope (GBT) have been substantially redesigned to make the telescope easier to use. The result is the release of the Astronomer's Integrated Desktop (Astrid), an observation management platform used to create and submit scheduling blocks, monitor their progress on the telescope, and provide a real time, quick look data display. Using Astrid, the astronomer launches one application and has access to all of the software, documentation, and feedback facilities that are required to conduct an interactive observing session. These systems together provide a common look and feel for GBT software applications, enable offline observation preparation, and facilitate dynamic scheduling and remote observing.

关键词： architecture scheduling block python framework quick look plotting quick look pipeline

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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...

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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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