Szczegóły publikacji
Opis bibliograficzny
Control software for the $SST-1M$ small-size telescope prototype for the Cherenkov Telescope Array / V. Sliusar, [et al.], W. Bilnik, [et al.], J. KASPEREK, [et al.], K. LALIK, [et al.], P. RAJDA, [et al.], M. Więcek, [et al.] // PoS Proceedings of Science [Dokument elektroniczny]. — Czasopismo elektroniczne ; ISSN 1824-8039. — 2017 — vol. 301 art. no. 844, s. 1–8. — Wymagania systemowe: Adobe Reader. — Bibliogr. s. 8. — Publikacja dostępna online od: 2018-08-03. — ICRC2017 : 35th International Cosmic Ray Conference : the astroparticle physics conference : 12–20 July, 2017, Bexco, Busan, Korea
Autorzy (43)
Dane bibliometryczne
| ID BaDAP | 120848 |
|---|---|
| Data dodania do BaDAP | 2019-04-09 |
| Tekst źródłowy | URL |
| DOI | 10.22323/1.301.0844 |
| Rok publikacji | 2017 |
| Typ publikacji | referat w czasopiśmie |
| Otwarty dostęp |  |
| Creative Commons | |
| Czasopismo/seria | PoS Proceedings of Science |
Abstract
The SST-1M is a 4-m Davies-Cotton atmospheric Cherenkov telescope optimized to provide gamma-ray sensitivity above a few TeV. The SST-1M is proposed as part of the Small-Size Telescope array for the Cherenkov Telescope Array (CTA), the first prototype has already been deployed. The SST-1M control software of all subsystems (active mirror control, drive system, safety system, photo-detection plane, DigiCam, CCD cameras) and the whole telescope itself (master controller) uses the standard software design proposed for all CTA telescopes based on the ALMA Common Software (ACS) developed to control the Atacama Large Millimeter Array (ALMA). Each subsystem is represented by a separate ACS component, which handles the communication to and the operation of the subsystem. Interfacing with the actual hardware is performed via the OPC UA communication protocol, supported either natively by dedicated industrial standard servers (PLCs) or separate service applications developed to wrap lower level protocols (e.g. CAN bus, camera slow control) into OPC UA. Early operations of the telescope without the camera were already carried out. The camera is fully assembled and is capable to perform data acquisition using artificial light source.
