Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29995
DC Field | Value | Language |
---|---|---|
dc.contributor.author | OLMI, LUCA | en_US |
dc.contributor.author | BOLLI, Pietro | en_US |
dc.contributor.author | CARBONARO, LUCA | en_US |
dc.contributor.author | CRESCI, Luca | en_US |
dc.contributor.author | MARONGIU, Pasqualino | en_US |
dc.contributor.author | NESTI, Renzo | en_US |
dc.contributor.author | PANELLA, Dario | en_US |
dc.contributor.author | RODA, JURI | en_US |
dc.contributor.author | ZACCHIROLI, GIAMPAOLO | en_US |
dc.contributor.author | Mugnai, Daniela | en_US |
dc.contributor.author | Natale, Enzo | en_US |
dc.date.accessioned | 2021-01-26T10:16:47Z | - |
dc.date.available | 2021-01-26T10:16:47Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.isbn | 978-90-82598-73-5 | en_US |
dc.identifier.isbn | 978-1-5386-3764-7 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29995 | - |
dc.description.abstract | Toraldo Pupils (TPs) can improve the angular resolving power of an optical instrument beyond the classical diffrac- tion limit (hence the term super-resolution) using a filter consisting of finite-width concentric coronae with differ- ent amplitude and phase transmittance. The first success- ful laboratory test of TPs in 2003 suggested that these de- vices could represent a viable approach to achieve super- resolution in Radio Astronomy. We have therefore started a project devoted to an exhaustive study of TPs and how they could be implemented on a radio telescope. In this work we present a summary of the design and laboratory tests of an optical module based on TPs that we plan to field-test on the Medicina 32-m radio telescope. | en_US |
dc.language.iso | eng | en_US |
dc.title | Design and Test of a Toraldo Pupil Optical Module for the Medicina Radio Telescope | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.23919/URSI-AT-RASC.2018.8471525 | en_US |
dc.identifier.scopus | 2-s2.0-85051939771 | en_US |
dc.identifier.url | http://www.ursi.org/proceedings/procAT18/papers/paperATRASC2018v2.pdf | en_US |
dc.identifier.url | https://ieeexplore.ieee.org/document/8471525 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.type.referee | REF_4 | en_US |
dc.relation.ispartofbook | 2018 2nd URSI Atlantic Radio Science Conference (AT-RASC) | en_US |
dc.relation.conferencename | 2018 2nd URSI Atlantic Radio Science Conference (AT-RASC) | en_US |
dc.relation.conferenceplace | Gran Canaria, Spain | en_US |
dc.relation.conferencedate | 28 May – 1 June, 2018 | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | reserved | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0002-1162-7947 | - |
crisitem.author.orcid | 0000-0001-8770-8316 | - |
crisitem.author.orcid | 0000-0003-1492-1591 | - |
crisitem.author.orcid | 0000-0003-0314-7801 | - |
crisitem.author.orcid | 0000-0003-0303-839X | - |
crisitem.author.orcid | 0000-0001-7554-2056 | - |
crisitem.author.orcid | 0000-0003-3544-4114 | - |
crisitem.author.orcid | 0000-0002-2066-2330 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | Existing users please |
---|---|---|---|---|
OLMI_ATRASC2018_Editorial.pdf | [Administrators only] | 5.71 MB | Adobe PDF |
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