Paper
29 August 2022 Assembling and integration of the ALMA hardware in the loop simulation environment
Tzu-Chiang Shen, Alejandro Saez, Rodrigo Cabezas, Mark Gallilee, José L. Ortíz, Carlos Boza, Yoshiharu Asaki, Claudio Follert, Martin Tourneboeuf, Soledad Fuica, Johnny Reveco, Ruben Soto, Jorge Ibsen, Norikazu Mizuno, Stuartt Corder
Author Affiliations +
Abstract
The Atacama Large Millimeter/submillimeter Array (ALMA) has been working in the operations regime since 2013. After almost 10 years of successful operation, obsolescence of hardware and software emerged. On the other hand, the ALMA 2030 plan will add new disrupting capabilities to the ALMA telescope. Both efforts will require an increased amount of technical time for testing in order to minimize the risks to introduce instability in the operation when new equipment and software are integrated into the telescope. Therefore, a process to design and implement a new simulation environment, which must be comparable to the production environment, was started in 2017 and passed the Critical Design and Manufacturing Review (CDMR) in 2020. In this paper, the current status of the project was reviewed focusing on the assembling and integration period, and use cases that are started to be built on top of this testing facility.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Tzu-Chiang Shen, Alejandro Saez, Rodrigo Cabezas, Mark Gallilee, José L. Ortíz, Carlos Boza, Yoshiharu Asaki, Claudio Follert, Martin Tourneboeuf, Soledad Fuica, Johnny Reveco, Ruben Soto, Jorge Ibsen, Norikazu Mizuno, and Stuartt Corder "Assembling and integration of the ALMA hardware in the loop simulation environment", Proc. SPIE 12189, Software and Cyberinfrastructure for Astronomy VII, 121891C (29 August 2022); https://doi.org/10.1117/12.2629194
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KEYWORDS
Antennas

Telescopes

Signal processing

Control systems

Data modeling

Observatories

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