26 July 2016 The software architecture to control the Cherenkov Telescope Array
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Proceedings Volume 9913, Software and Cyberinfrastructure for Astronomy IV; 991303 (2016); doi: 10.1117/12.2232520
Event: SPIE Astronomical Telescopes + Instrumentation, 2016, Edinburgh, United Kingdom
Abstract
The Cherenkov Telescope Array (CTA) project is an initiative to build two large arrays of Cherenkov gamma- ray telescopes. CTA will be deployed as two installations, one in the northern and the other in the southern hemisphere, containing dozens of telescopes of different sizes. CTA is a big step forward in the field of ground- based gamma-ray astronomy, not only because of the expected scientific return, but also due to the order-of- magnitude larger scale of the instrument to be controlled. The performance requirements associated with such a large and distributed astronomical installation require a thoughtful analysis to determine the best software solutions. The array control and data acquisition (ACTL) work-package within the CTA initiative will deliver the software to control and acquire the data from the CTA instrumentation. In this contribution we present the current status of the formal ACTL system decomposition into software building blocks and the relationships among them. The system is modelled via the Systems Modelling Language (SysML) formalism. To cope with the complexity of the system, this architecture model is sub-divided into different perspectives. The relationships with the stakeholders and external systems are used to create the first perspective, the context of the ACTL software system. Use cases are employed to describe the interaction of those external elements with the ACTL system and are traced to a hierarchy of functionalities (abstract system functions) describing the internal structure of the ACTL system. These functions are then traced to fully specified logical elements (software components), the deployment of which as technical elements, is also described. This modelling approach allows us to decompose the ACTL software in elements to be created and the ow of information within the system, providing us with a clear way to identify sub-system interdependencies. This architectural approach allows us to build the ACTL system model and trace requirements to deliverables (source code, documentation, etc.), and permits the implementation of a flexible use-case driven software development approach thanks to the traceability from use cases to the logical software elements. The Alma Common Software (ACS) container/component framework, used for the control of the Atacama Large Millimeter/submillimeter Array (ALMA) is the basis for the ACTL software and as such it is considered as an integral part of the software architecture.
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I. Oya, M. Füßling, P. Oliveira Antonino, V. Conforti, L. Hagge, D. Melkumyan, A. Morgenstern, G. Tosti, U. Schwanke, J. Schwarz, P. Wegner, J. Colomé, E. Lyard, "The software architecture to control the Cherenkov Telescope Array", Proc. SPIE 9913, Software and Cyberinfrastructure for Astronomy IV, 991303 (26 July 2016); doi: 10.1117/12.2232520; https://doi.org/10.1117/12.2232520
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KEYWORDS
Telescopes

Control systems

Data acquisition

Computer architecture

Atmospheric Cherenkov telescopes

Chemical elements

Systems modeling

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