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

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control of the Hobby-Eberly telescope primary mirror array with the segment alignment maintenance system

Control of the Hobby-Eberly Telescope primary mirror array w...

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Palunas, P Fowler, JR Booth, JA Damm, G Ames, GH Univ Texas McDonald Observ Univ Stn 1 11402 Austin TX 78712 USA

ISBN: (纸本)0819454281

The Segment Alignment Maintenance System (SAMS) is a control system to maintain the alignment of the 91 segment Hobby-Eberly telescope (BET) primary mirror array. The system was developed by Blue-Line Engineering (Colorado Springs, CO) and NASA-Marshall Space Flight Center (Huntsville-Al). The core of the system is a set of 480 inductive edge sensors which measure relative shear between adjacent segments. The relative shear is used to calculate segment tip/tilt and piston corrections. Although the system has dramatically improved the performance of the BET it does not meet its error budget due to thermal drifts in the sensors. The system is now sufficiently stable that it routinely requires only one primary mirror alignment at the beginning of the night. We describe methods to calibrate this sensor drift.

关键词： Hobby-Eberly telescope HET SAMS edge sensors control systems

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Data acquirement and process system based on Ethernet for Multi Channel Solar telescope

Data acquirement and process system based on Ethernet for Mu...

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Hu, KL Deng, YY Ma, XL CAS Natl Astron Observ Beijing 100012 Peoples R China

ISBN: (纸本)0819454281

For astronomical observations, there are many kinds of CCD cameras for different scientific purposes. Sometimes, this even happens in one telescope. Traditionally, a CCD camera has an individual image grabber, data process unit, and corresponding control computer. Consequently, this brings some inconvenience and problems not only to the system management but also to the updating of the system. This paper presents a resolution to this problem for the Multi-Channel Solar telescope (MCST). All CCD cameras are connected in an Ethernet through an Ethernet interface. A server is needed to send commands to all cameras and transfer data through TCP/IP. Each CCD camera has an embedded system to control the camera, receive commands from the server and signals from the camera, process, and store the data. This paper describes the design of an Ethernet controlled camera. The camera is PULNIX TM1010, which is controlled by an Altera embedded system by Cyclone EP1C20F400C7 FPGA, which embedded with a Nios processor.

关键词： FPGA NIOS Ethernet embedded system Multi-Channel Solar telescope

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TALON - The telescope alert operation network system: Intelligent linking of distributed autonomous robotic telescopes

TALON - The telescope alert operation network system: Intell...

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： White, RR Wren, J Davis, H Galassi, M Starr, D Vestrand, WT Wozniak, P Los Alamos Natl Lab Los Alamos NM 87545 USA

ISBN: (纸本)0819454281

The internet has brought about great change in the astronomical community, but this interconnectivity is just starting to be exploited for use in instrumentation. Utilizing the internet for communicating between distributed astronomical systems is still in its infancy, but it already shows great potential. Here we present an example of a distributed network of telescopes that performs more efficiently in synchronous operation than as individual instruments. RAPid telescopes for Optical Response (RAPTOR) is a system of telescopes at LANL that has intelligent intercommunication, combined with wide-field optics, temporal monitoring software, and deep-field follow-up capability all working in closed-loop real-time operation. The telescope ALert Operations Network (TALON) is a network server that allows intercommunication of alert triggers from external and internal resources and controls the distribution of these to each of the telescopes on the network. TALON is designed to grow, allowing any number of telescopes to be linked together and communicate. Coupled with an intelligent alert client at each telescope, it can analyze and respond to each distributed TALON alert based on the telescopes needs and schedule.

关键词： robotic telescope communication distributed sensor optical transient network servers

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The use of object-oriented techniques and CORBA in astronomical instrumentation control systems

The use of object-oriented techniques and CORBA in astronomi...

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conference on advanced software, control and Communication Systems for Astronomy

作者： Dipper, NA Blackburn, C Univ Durham Dept Phys Ctr Adv Instrumentat Sci Labs Durham DH1 3LE England

ISBN: (纸本)0819454281

control software for astronomy matches the ever increasing complexity of new large instrumentation projects. In order to speed the development cycle, object-oriented techniques have been used to generate loosely coupled software objects and larger scale components that can be reused in future projects. Such object-oriented systems provide for short development cycles which can respond to changing requirements and allow for extension. The Unified Modeling Language (UML) has been used for the analysis, design and implementation of this software. A distributed system is supported by the use of an object broker such as CORBA. These techniques are being applied to the development of an instrument control system for the UK spectrograph within FMOS (Fiber-fed Multi-Object Spectrograph). This is a second generation instrument for the Subaru telescope of the National Astronomical Observatory of Japan.

关键词： object-oriented Python CORBA UML design patterns control systems FMOS

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Generic control of robotic telescopes

Generic control of robotic telescopes

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conference on advanced software, control and Communication Systems for Astronomy

作者： Granzer, T Inst Astrophys Potsdam Germany

ISBN: (纸本)0819454281

Fully robotic observatories open a cheap, but nevertheless compelling window for scientific research. Though the telescopes are small and from the engineering point of view mostly simple, the challenging part lies in the software necessary for robotic action. If one carefully plans the development and tries to be as generic as possible, it is appropriate to create a basic software package that has the capabilities to be used on almost any robotic observatory. The aim of this article is to introduce the software used on the STELLA robotic telescope, operated by the Astrophysikalisches Institut Potsdam. Emphasis is put on issues addressing adaptation of the software to different robotic telescopes. The entire package is written in Sun's Java 1.3. It is expected to be released under the GNU public license later this year.

关键词： robotic telescopes Java XML software

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Active optics and auto-guiding control for VISTA

Active optics and auto-guiding control for VISTA

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conference on advanced software, control and Communication Systems for Astronomy

作者： Terrett, DL Bissonauth, N Graffagnino, V Stewart, M Sutherland, W Rutherford Appleton Lab Dept Space Sci Didcot OX11 0QX Oxon England

ISBN: (纸本)0819454281

The VISTA wide field survey telescope will use the ESO telescope control System as used on the VLT and NTT. However the sensors for both auto-guiding and active optics are quite different and so the ESO TCS will require some significant modifications. VISTA will use large format CCDs at fixed locations in the focal plane for auto-guiding and a pair of curvature sensors, also fixed in the focal plane, for wave-front sensing. As a consequence, three reference stars are required for each science observation in contrast to the VLT which uses a single star for both auto-guiding and active optics. This paper will outline the reasons for adopting this design, review how it differs from the VLT/NTT and describe the modifications that are being made to the ESO TCS to enable it to be used for VISTA. It will describe the software that implements auto-guiding and active optics in the VLT TCS and how the design has been adapted to the different requirements of VISTA. This will show how the modular and distributed design of the ESO TCS has enabled it to be adapted to a new telescope with radically different design choices whilst maintaining the existing architecture and the bulk of the existing implementation.

关键词： active-optics auto-guiding software engineering TCS VISTA VLT

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The VISTA IR camera software design

The VISTA IR camera software design

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Beard, S McLay, S Stewart, M Bissonauth, N Bierechel, P UK Astron Ctr Royal Observ Edinburgh EH9 3HJ Midlothian Scotland

ISBN: (纸本)0819454281

VISTA is a wide-field survey telescope with a 1.6degrees field of view, sampled with a camera containing a 4 x 4 array of 2K x 2K pixel infrared detectors. The detectors are spaced so an image of the sky can be constructed without gaps by combining 6 overlapping observations, each part of the sky being covered at least twice, except at the tile edges. Unlike a typical ESO-VLT instrument, the camera also has a set of on-board wavefront sensors. The camera has a filter wheel, a collection of pressure and temperature sensors, and a thermal control system for the detectors and the cryostat window, but the most challenging aspect of the camera design is the need to maintain a sustained data rate of 26.8 Mb/second from the infrared detectors. The camera software needs to meet the requirements for VISTA, to fit into the ESO-VLT software architecture, and to interface with an upgraded MACE system being developed by ESO-VLT. This paper describes the design for the VISTA camera software and discusses the software development process. It describes the solutions we have adopted to achieve the desired data rate, maximise survey speed, meet ESO-VLT standards, interface to the IRACE software and interface the on-board wavefront sensors to the VISTA telescope software.

关键词： VISTA instrumentation wide-field infrared camera software design

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The Goodman spectrograph control system

The Goodman spectrograph control system

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Crain, JA Clemens, JC Bayliss, M Univ N Carolina Dept Phys & Astron Chapel Hill NC 27514 USA

ISBN: (纸本)0819454281

The Goodman spectrograph is an all-refracting articulated-camera high-throughput imaging spectrograph for the SOuthern Astrophysical Research telescope (SOAR). It is designed to take advantage of Volume Phase Holographic (VPH) gratings. Due to the high level of mechanical complexity, a fully graphical control system with parallel motor control was developed. We have developed a software solution in LabVIEW that functions as a control system, component management tool, and engineering platform. A modular software design allows other instrument projects to easily adopt our approach. Distinguishing features of the control system include automated configuration changes, remote capability, and PDA control for component swaps.

关键词： instrument control control system distributed control LabVIEW Silvermax remote observing

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An enterprise software architecture for the green bank telescope (GBT)

An enterprise software architecture for the green bank teles...

引用

conference on advanced software, control and Communication Systems for Astronomy

作者： Radziwill, NM Mello, M Sessoms, E Shelton, A Natl Radio Astron Observ Green Bank WV 24944 USA

ISBN: (纸本)0819454281

The enterprise architecture presents a view of how software utilities and applications are related to one another under unifying rules and principles of development. By constructing an enterprise architecture, an organization will be able to manage the components of its systems within a solid conceptual framework. This largely prevents duplication of effort, focuses the organization on its core technical competencies, and ultimately makes software more maintainable. In the beginning of 2003, several prominent challenges faced software development at the GBT. The telescope was not easily configurable, and observing often presented a challenge, particularly to new users. High priority projects required new experimental developments on short time scales. Migration paths were required for applications which had proven difficult to maintain. In order to solve these challenges, an enterprise architecture was created which includes five layers: 1) the telescope control system, and the raw data produced during an observation, 2) Low-level Application Programming Interfaces (APIs) in C++, for managing interactions with the telescope control system and its data, 3) High-Level APIs in Python, which can be used by astronomers or software developers to create custom applications, 4) Application Components in Python, which can be either standalone applications or plug-in modules to applications, and 5) Application Management Systems in Python, which package application components for use by a particular user group (astronomers, engineers or operators) in terms of resource configurations. This presentation describes how these layers combine to make the GBT easier to use, while concurrently making the software easier to develop and maintain.

关键词： architecture application programming interface API scheduling block execution block GUI

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Flexible pointing models for large Arecibo type optical telescopes

Flexible pointing models for large Arecibo type optical tele...

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conference on advanced software, control and Communication Systems for Astronomy

作者： Schalekamp, H Swart, G SALT Fdn Observ ZA-7925 Cape Town South Africa

ISBN: (纸本)0819454281

The modern day computing power to cost ratio has allowed flexible yet complex mathematical models to be implemented in various arenas. A current example is the Southern African Large telescope and the Hobby-Eberly telescope, Arecibo-type large optical telescopes, which have a moving prime focus confined to a spherical surface. The complexity of the moving tracking mechanism, a stationary self-aligning mirror and the scales of the structures involved in such telescopes have led to the requirement of more flexible telescope mount models. In this way the combination of low cost and a requirement for flexibility has led to the design of new mathematical models for telescopes of this type. A case in point is the Southern African Large telescope, due to the specific design 6 and calibration requirements during the design and commissioning of the telescope, an adaptable mathematical model is required. Such a model should have multiple easily accessible entry points and flexibility of conversion paths between the various coordinate systems involved. In this paper the authors present an overview of the special requirements for the Southern African Large telescope and the eventual design and implementation of a mathematical model to cope with these requirements. Some of the topics that will be discussed include: tracking challenges on SALT;layering of complexity of the mathematical model;software design and access to mathematical parameters;analytical and statistical tools for model design;and design consistency between coordinate conversions.

关键词： pointing SALT mathematical modeling software extremely large telescopes

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