Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27433
DC Field | Value | Language |
---|---|---|
dc.contributor.author | MARASSI, Alessandro | en_US |
dc.contributor.author | Kotze, Jan | en_US |
dc.contributor.author | Steyn, T.J. | en_US |
dc.contributor.author | van Niekerk, C | en_US |
dc.contributor.author | RIGGI, Simone | en_US |
dc.contributor.author | SCHILLIRO', FRANCESCO | en_US |
dc.contributor.author | Smit, George | en_US |
dc.date.accessioned | 2020-09-17T07:12:42Z | - |
dc.date.available | 2020-09-17T07:12:42Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.isbn | 978-3-95450-193-9 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27433 | - |
dc.description.abstract | The Square Kilometre Array (SKA) project is responsible for developing the SKA Observatory, the world's largest radio telescope ever built: eventually two arrays of radio antennas - SKA1-Mid and SKA1-Low - will be installed in the South Africa's Karoo region and Western Australia's Murchison Shire respectively, each covering a different range of radio frequencies. In particular, the SKA1-Mid array will comprise of 133 15m diameter dish antennas observing in the 350 MHz-14 GHz range, each locally managed by a Local Monitoring and Control (LMC) system and remotely orchestrated by the SKA Telescope Manager (TM) system. All control system functionality run on the Tango Controls platform. The Dish Single Pixel Feed (SPF) work element will design the combination of feed elements, orthomode transducers (OMTs), and low noise amplifiers (LNAs) that receive the astronomical radio signals. Some SPFs have cryogenically cooled chambers to obtain the sensitivity requirements. This paper gives a status update of the SKA Dish SPF and LMC interaction design, focusing on SPF, LMC simulators and engineering/operational user interfaces, prototypes being developed and technological choices. | en_US |
dc.language.iso | eng | en_US |
dc.title | The SKA Dish SPF and LMC Interaction Design: Interfaces, Simulation, Testing and Integration | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.18429/JACoW-ICALEPCS2017-THPHA142 | en_US |
dc.identifier.url | http://accelconf.web.cern.ch/icalepcs2017/doi/JACoW-ICALEPCS2017-THPHA142.html | en_US |
dc.identifier.url | http://accelconf.web.cern.ch/icalepcs2017/ | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.type.referee | REF_3 | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | ZAF | en_US |
dc.relation.ispartofbook | Proceedings of the 16th International Conference on Accelerator and Large Experimental Control Systems | en_US |
dc.relation.conferencename | 16th International Conference on Accelerator and Large Experimental Physics Control Systems (ICALEPCS 2017) | en_US |
dc.relation.conferenceplace | Barcelona, Spain | en_US |
dc.relation.conferencedate | October 8-13, 2017 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.languageiso639-1 | en | - |
item.openairetype | Conference paper | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.orcid | 0000-0001-9585-9974 | - |
crisitem.author.orcid | 0000-0001-6368-8330 | - |
crisitem.author.orcid | 0000-0001-5106-2277 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
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thpha142.pdf | Pdf editoriale | 526.3 kB | Adobe PDF | View/Open |
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