The Australian SKA Pathfinder (ASKAP) Software Architecture
Identifieur interne : 000A54 ( Main/Exploration ); précédent : 000A53; suivant : 000A55The Australian SKA Pathfinder (ASKAP) Software Architecture
Auteurs : Juan C. Guzman [Australie] ; Ben Humphreys [Australie]Source :
- Proceedings of SPIE, the International Society for Optical Engineering [ 0277-786X ] ; 2010.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
The Australian SKA Pathfinder (ASKAP) is a 1% Square Kilometre Array (SKA) pathfinder radio telescope, comprising of 36 12-metre diameter reflector antennas, each with a Focal Plane Array consisting of approximately 100 dual-polarised elements operating at centimetre wavelengths and yielding a wide field-of-view (FOV) on the sky of about 30 square degrees. ASKAP is currently under construction and will be located in the remote radio-quiet desert Midwest region of Western Australia. It is expected to be fully operational in 2013. Key challenges include near real-time processing of large amount of data (˜ 4 GB/s), control and monitoring of widely distributed devices (approx. 150,000 monitoring I/O points) and remote semi-automated operations. After evaluating several software technologies we have decided to use the EPICS framework for the Telescope Operating System and the Internet Communications Engine (ICE) middleware for the high-level service bus. This paper presents a summary of the overall ASKAP software architecture, as well as describing how EPICS and ICE technologies fit in the control software design.
Affiliations:
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Le document en format XML
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<term>Control synthesis</term>
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<term>Focal plane</term>
<term>Internet</term>
<term>Middleware</term>
<term>Monitoring</term>
<term>Operating system</term>
<term>Processing time</term>
<term>Radiotelescope</term>
<term>Real time</term>
<term>Remote operation</term>
<term>Service quality</term>
<term>Sky</term>
<term>Software architecture</term>
<term>Software development</term>
<term>Telescope</term>
<term>Wavelength</term>
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<term>Temps réel</term>
<term>Temps traitement</term>
<term>Monitorage</term>
<term>Système exploitation</term>
<term>Internet</term>
<term>Intergiciel</term>
<term>Qualité service</term>
<term>Synthèse commande</term>
<term>Développement logiciel</term>
<term>Antenne</term>
<term>Plan focal</term>
<term>Longueur onde</term>
<term>Ciel</term>
<term>Téléopération</term>
<term>Diamètre</term>
<term>Télescope</term>
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<front><div type="abstract" xml:lang="en">The Australian SKA Pathfinder (ASKAP) is a 1% Square Kilometre Array (SKA) pathfinder radio telescope, comprising of 36 12-metre diameter reflector antennas, each with a Focal Plane Array consisting of approximately 100 dual-polarised elements operating at centimetre wavelengths and yielding a wide field-of-view (FOV) on the sky of about 30 square degrees. ASKAP is currently under construction and will be located in the remote radio-quiet desert Midwest region of Western Australia. It is expected to be fully operational in 2013. Key challenges include near real-time processing of large amount of data (˜ 4 GB/s), control and monitoring of widely distributed devices (approx. 150,000 monitoring I/O points) and remote semi-automated operations. After evaluating several software technologies we have decided to use the EPICS framework for the Telescope Operating System and the Internet Communications Engine (ICE) middleware for the high-level service bus. This paper presents a summary of the overall ASKAP software architecture, as well as describing how EPICS and ICE technologies fit in the control software design.</div>
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