The design of the local monitor and control system of SKA dishes

F. Schillirò; V. Baldini; U. Becciani; R. Cirami; A. Costa; A. Ingallinera; A. Marassi; G. Nicotra; C. Nocita; S. Riggi; C. Trigilio

doi:10.1117/12.2232567

9 August 2016 The design of the local monitor and control system of SKA dishes

F. Schillirò, V. Baldini, U. Becciani, R. Cirami, A. Costa, A. Ingallinera, A. Marassi, G. Nicotra, C. Nocita, S. Riggi, C. Trigilio

Author Affiliations +

Proceedings Volume 9906, Ground-based and Airborne Telescopes VI; 99065V (2016) https://doi.org/10.1117/12.2232567
Event: SPIE Astronomical Telescopes + Instrumentation, 2016, Edinburgh, United Kingdom

Abstract

The Square Kilometer Array (SKA) project aims at building the world’s largest radio observatory to observe the sky with unprecedented sensitivity and collecting area. In the first phase of the project (SKA1), an array of dishes, SKA1-MID, will be built in South Africa. It will consist of 133 15m-dishes, which will include the MeerKAT array, for the 0.350-20 GHz frequency band observations. Each antenna will be provided with a local monitor and control system (LMC), enabling operations both to the Telescope Manager remote system, and to the engineers and maintenance staff; it provides different environment for the telescope control (positioning, pointing, observational bands), metadata collection for monitoring and database storaging, operational modes and functional states management for all the telescope capabilities. In this paper we present the LMC software architecture designed for the detailed design phase (DD), where we describe functional and physical interfaces with monitored and controlled sub-elements, and highlight the data flow between each LMC modules and its sub-element controllers from one side, and Telescope Manager on the other side. We also describe the complete Product Breakdown Structure (PBS) created in order to optimize resources allocation in terms of calculus and memory, able to perform required task for each element according to the proper requirements. Among them, time response and system reliability are the most important, considering the complexity of SKA dish network and its isolated placement. Performances obtained by software implementation using TANGO framework will be discussed, matching them with technical requirements derived by SKA science drivers.

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F. Schillirò, V. Baldini, U. Becciani, R. Cirami, A. Costa, A. Ingallinera, A. Marassi, G. Nicotra, C. Nocita, S. Riggi, and C. Trigilio "The design of the local monitor and control system of SKA dishes", Proc. SPIE 9906, Ground-based and Airborne Telescopes VI, 99065V (9 August 2016); https://doi.org/10.1117/12.2232567

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