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Wind Evaluation Breadboard electronics and software

Wind Evaluation Breadboard electronics and software

引用

2nd conference on advanced software and control for Astronomy

作者： Nunez, Miguel Reyes, Marcos Viera, Teodora Zuluaga, Pablo Inst Astrofis Canarias Tenerife Spain

ISBN: (纸本)9780819472298

WEB, the Wind Evaluation Breadboard, is an Extremely Large telescope Primary Mirror simulator, developed with the aim of quantifying the ability of a segmented primary mirror to cope with wind disturbances. This instrument supported by the European Community (Framework Programme 6, ELT Design Study), is developed by ESO, IAC, MEDIA-ALTRAN, JUPASA and FOGALE. The WEB is a bench of about 27 tons and 7 meter diameter emulating a segmented primary mirror and its cell, with 7 hexagonal segments simulators, including electromechanical support systems. In this paper we present the WEB central control electronics and the software development which has to interface with: position actuators, auxiliary slave actuators, edge sensors, azimuth ring, elevation actuator, meteorological station and air balloons enclosure. The set of subsystems to control is a reduced version of a real telescope segmented primary mirror control system with high real time performance but emphasizing on development time efficiency and flexibility, because WEB is a test bench. The paper includes a detailed description of hardware and software, paying special attention to real time performance. The Hardware is composed of three computers and the software architecture has been divided in three intercommunicated applications and they have been implemented using Labview over Windows XP and Pharlap ETS real time operating system. The edge sensors and position actuators close loop has a sampling and commanding frequency of 1 KHz.

关键词： ELT ESO IAC WEB segmented primary mirror wind soft-ware Labview

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The NEWFIRM Observing software: From Design To Implementation

The NEWFIRM Observing Software: From Design To Implementatio...

引用

2nd conference on advanced software and control for Astronomy

作者： Daly, P. N. Buchholz, N. C. Fitzpatrick, M. J. Mills, D. Valdes, F. G. Zarate, N. Swaters, R. Probs, R. G. Dickinson, M. Natl Opt Astron Observ 950 N Cherry Ave Tucson AZ 85719 USA Univ Maryland Dept Astron College Pk MD 20742 USA

ISBN: (纸本)9780819472298

NEWFIRM is the wide-field infra-red mosaic camera just delivered and commissioned on the Mayall 4-m telescope on Kitt Peak. As with other major instrumentation projects, the software was part of a, design, development, implementation and delivery strategy. In this paper, we describe the final implementation of the NEWFIRM software from acquisition within a MONSOON controller environment, directed by the observation control system, to the quick-look functionality at the telescope and final delivery of standardized data products via the pipeline. NEWFIRM is, therefore, the culmination of several years of design and development effort on several fronts.

关键词： software control Systems Data Products Pipeline Reduction Guiding

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A Framework for the Subaru telescope Observation control System Based on the Command Design Pattern

A Framework for the Subaru Telescope Observation Control Sys...

引用

2nd conference on advanced software and control for Astronomy

作者： Jeschke, Eric Bon, Bruce Inagaki, Takeshi Streeper, Sam Natl Inst Nat Sci Natl Astron Observ Japan Subaru Telescope Hilo HI 96720 USA

ISBN: (纸本)9780819472298

Subaru telescope is developing a second-generation Observation control System (OCS) that specifically addresses some of the deficiencies of the current Subaru OCS. One area of concern is better extensibility: the current system uses a custom language for implementing commands with a complex macro processing subsystem written in C. It is laborious to improve the language and awkward for scientists to extend and use standard programming techniques. Our Generation 2 OCS provides a lightweight, object-oriented task framework based on the Command design pattern. The framework provides a base task class that abstracts services for processing status and other common infrastructure activities. Upon this are built and provided a set of "atomic" tasks for telescope and instrument commands. A set of "container" tasks based on common sequential and concurrent command processing paradigms is also included. Since all tasks share the same exact interface, it is straightforward to build up compound tasks by plugging simple tasks into container tasks and container tasks into other containers, and so forth. In this way various advanced astronomical workflows can be readily created, with well controlled behaviors. In addition, since tasks are written in Python, it is easy for astronomers to subclass and extend the standard observatory tasks with their own custom extensions and behaviors, in a high-level, full-featured programming language. In this talk we will provide an overview of the task framework design and present preliminary results on the use of the framework during two separate engineering runs.

关键词： Design Pattern Command Processing Tasks Python Framework

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An Amateur telescope control System: Towards a Generic telescope control Model

An Amateur Telescope Control System: Towards a Generic Teles...

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2nd conference on advanced software and control for Astronomy

作者： Tobar, Rodrigo J. von Brand, Horst H. Araya, Mauricio A. Lopez, Joao S. Univ Tecn Federico Santa Maria Dept Informat Valparaiso 1680 Chile

ISBN: (纸本)9780819472298

control System for an Amateur telescope (CSAT) is a distributed telescope control system model for amateur telescopes with transparent interchangeable components, built using the ALMA Common software (ACS) framework. The CSAT project has been thought as the first step towards a generic telescope control model, which will consist on a generic control framework for any telescope mount. With the ACS Container/Component model, a completely different hardware can be supported by just re-implementing the low-level components for the new setup. This way, CSAT becomes a very good example of all the features that ACS provides for building a generic telescope control framework.

关键词： CORBA ACS TCS Amateur telescope Distributed systems

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LBTI software Architecture

LBTI Software Architecture

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2nd conference on advanced software and control for Astronomy

作者： Vaitheeswaran, Vidhya Hinz, Phil Kraus, Joseph Breuninger, Andrew Univ Arizona Steward Observ 933 N Cherry Ave Tucson AZ 85721 USA South African Large Telescope Karoo South Africa

ISBN: (纸本)9780819472298

LBTI is a thermal imager and a nulling interferometer to be installed on the Large Binocular telescope (LBT). Here, we present the distributed component architecture model and its simple yet powerful software structure designed to complement the LBTI hardware model that comprises pyramid wave front sensors with its control electronic universal beam combiner, phase sensor, science imager, and all housekeeping duties to run the cryogenics, compressors, vibration monitors and the interface to the telescope control systems.

关键词： Interferometer software

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software for the EVLA, Current Status

Software for the EVLA, Current Status

引用

2nd conference on advanced software and control for Astronomy

作者： Butler, Bryan J. Harland, David Truitt, Brian Rochford, James Witz, Stephan Natl Radio Astron Observ Socorro NM 87801 USA

ISBN: (纸本)9780819472298

The Expanded Very Large Array (EVLA) project is the next generation instrument for high resolution long-millimeter to short-meter wavelength radio astronomy. It is currently funded by NSF, with completion scheduled for 2012. The EVLA will upgrade the VLA with new feeds, receivers, data transmission hardware, correlator, and a new software system to enable the instrument to achieve its full potential. This software includes both that required for controlling and monitoring the instrument and that involved with the scientific dataflow. This manuscript presents an update on the overall design, and details for the pre-observing portions of the software, including: user authentication;proposal preparation, submission, and handling;and observation preparation. It will focus particularly on the observation preparation software, describing an implementation of a web-based interface for creation of a detailed observation description, and plans to achieve common observation preparation software with the ALMA telescope.

关键词： NRAO EVLA software

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Design and realization of the real-time spectrograph controller for LAMOST based on FPGA

Design and realization of the real-time spectrograph control...

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2nd conference on advanced software and control for Astronomy

作者： Wang, Jianing Wu, Liyan Zeng, Yizhong Dai, Songxin Hu, Zhongwen Zhu, Yongtian Wang, Lei Wu, Zhen Chen, Yi Chinese Acad Sci Natl Astron Observ Nanjing Inst Astron Opt & Technol Nanjing 210042 Peoples R China

ISBN: (纸本)9780819472298

A large Schmitt reflector telescope, Large Sky Area Multi-Object Fiber Spectroscopic telescope(LA MOST), is being built in China, which has effective aperture of 4 meters and can observe the spectra of as many as 4000 objects simultaneously. To fit such a large amount of observational objects, the dispersion part is composed of a set of 16 multipurpose fiber-fed double-beam Schmidt spectrographs, of which each has about ten of moveable components real-timely accommodated and manipulated by a controller. An industrial Ethernet network connects those 16 spectrograph controllers. The light from stars is fed to the entrance slits of the spectrographs with optical fibers. In this paper, we mainly introduce the design and realization of our real-time controller for the spectrograph, our design using the technique of System On Programmable Chip (SOPC) based on Field Programmable Gate Array (FPGA) and then realizing the control of the spectrographs through NIOS ii Soft Core Embedded Processor. We seal the stepper motor controller as intellectual property (IP) cores and reuse it, greatly simplifying the design process and then shortening the development time. Under the embedded operating system mu C/OS-ii, a multi-tasks control program has been well written to realize the real-time control of the moveable parts of the spectrographs. At present, a number of such controllers have been applied in the spectrograph of LAMOST.

关键词： real-time spectrograph controller Field Programmable Gate Array (FPGA) System On Programmable Chip (SOPC) NIOS ii intellectual property (IP) stepper motor Ethernet network LAMOST

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Installation and first light of the BOOTES-IR near-IR camera

Installation and first light of the BOOTES-IR near-IR camera

引用

2nd conference on advanced software and control for Astronomy

作者： Cunniffe, R. Castro-Tirado, A. J. Kubanek, P. Jelinek, M. Vitek, S. Gorosabel, J. Postigo, A. de Ugarte Riva, A. Zerbi, F. Claret, A. Sanchez-Fernandez, C. CSIC Inst Astrofis Andalucia Granada 18008 Spain Osservetorio Astronom Brera I-23807 Merate Lc Italy ESAC Madrid Spain

ISBN: (纸本)9780819472298

BIRCAM is a near-infrared (0.8-2.5um) cryogenic camera based on a 1Kx1K HgCdTe array. It was designed for - and is now mounted at - one of the Nasmyth foci of the fast-slewing 0.6 m BOOTES-IR telescope at the Sierra Nevada Observatory (OSN) in Spain. The primary science mission is prompt Gamma Ray-Burst afterglow research, with an implied demand for extremely time-efficient operation. We describe the challenges of installing a heavy camera on a small high-speed telescope, of integrating the dithering mechanism, the filterwheel, and the array itself into a high-efficiency instrument, the design of the software to meet the requirements.

关键词： Robotic telescopes telescope software near-IR instrumentation cryogenics

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A Lightweight, Fault-Tolerant Middleware for a Subaru telescope Second Generation Observation control System

A Lightweight, Fault-Tolerant Middleware for a Subaru Telesc...

引用

2nd conference on advanced software and control for Astronomy

作者： Jeschke, Eric Bon, Bruce Inagaki, Takeshi Streeper, Sam Natl Inst Nat Sci Natl Astron Observ Japan Subaru Telescope Hilo HI 96720 USA

ISBN: (纸本)9780819472298

Subaru telescope is developing a second-generation Observation control System that specifically addresses some of the shortcomings of the current Subaru OCS. Two areas of concern are complexity and failure handling. The current system has over 1000 dedicated OCS processes spread across a dozen hosts and provides nothing in the way of automated failover. Furthermore, manual failover is so fraught with difficulty that it is rarely attempted. Our Generation 2 OCS is written almost entirely in Python and builds upon a Subaru-developed middleware based on the XML-RPC protocol. This framework offers the following benefits: has very few dependencies outside of standard Python provides a nearly seamless remote proxy object-oriented interface provides optional user/password authentication and/or SSL encryption is extremely simple to use from client applications is connectionless, and assists transparent failover of communications and distributed services on a set of hosts has reasonable performance for a wide range of needs allows multiple language bindings for dynamic languages, requires no interface stub files The "back end" (service side) of the OCS is nearing completion, and has already been used successfully during two separate OCS engineering runs. It is comprised of only a couple dozen processes, and provides automated failover capabilities on a rack of commodity x86 Linux servers. We provide an overview of the middleware use, its design and its failover capabilities. Some data on the performance of communications using the middleware protocol is included.

关键词： Middleware XML-RPC Python Framework Failover

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The control and data concept for the robotic solar telescope ChroTel

The control and data concept for the robotic solar telescope...

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2nd conference on advanced software and control for Astronomy

作者： Halbgewachs, C. Bethge, Ch. Caligari, P. Elmore, D. Kentischer, T. J. Peter, H. Sigwarth, M. Schmidt, W. Kiepenheuer Inst Sonnenphys Schoneckstr 6 D-79104 Freiburg Germany High Altitude Observ Natl Ctr Atmospher Res Boulder CO 80305 USA

ISBN: (纸本)9780819472298

The solar telescope ChroTel is designed as a robotic telescope so that no user interaction is necessary for observation. The telescope will start tracking in the morning as soon as weather conditions are appropriate and will process a user defined observation routine until sunset. Weather conditions and system status are continuously monitored to close the telescope shutter in case of bad weather or to drive to the stow position in case of an error. The ChroTel control software was programmed in LabVIEW (TM).

关键词： robotic solar telescope full disc chromosphere synoptic observations labview

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