Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28157
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Schühle, Udo | en_US |
dc.contributor.author | Teriaca, Luca | en_US |
dc.contributor.author | Aznar Cuadrado, Regina | en_US |
dc.contributor.author | Heerlein, Klaus | en_US |
dc.contributor.author | USLENGHI, MICHELA | en_US |
dc.contributor.author | Werner, Stephan | en_US |
dc.date.accessioned | 2020-11-05T11:03:30Z | - |
dc.date.available | 2020-11-05T11:03:30Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.isbn | 9781510619517 | en_US |
dc.identifier.isbn | 9781510619524 | en_US |
dc.identifier.issn | 0277-786X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28157 | - |
dc.description.abstract | Two instruments aboard the Solar Orbiter mission, the Extreme Ultraviolet Imager and the Metis coronagraph, are using cameras of similar design to obtain images in the Lyman alpha line of hydrogen at 121.6 nm. Each of these cameras is based on an APS sensor used as readout of a single microchannel plate intensifier unit whose output current is converted into visible light photons through a phosphor screen. Before integration on the respective instruments, both detector's flight models have been characterized and calibrated. In this paper, we describe the two camera systems, the results of qualification tests, and report their performance characteristics. | en_US |
dc.language.iso | eng | en_US |
dc.title | The solar orbiter Metis and EUI intensified CMOS-APS detectors: concept, main characteristics, and performance | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1117/12.2313800 | en_US |
dc.identifier.scopus | 2-s2.0-85051861365 | en_US |
dc.identifier.isi | 000452819200074 | en_US |
dc.identifier.url | https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10699/1069934/The-solar-orbiter-Metis-and-EUI-intensified-CMOS-APS-detectors/10.1117/12.2313800.full | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 10699 | en_US |
dc.relation.firstpage | 1069934 | en_US |
dc.relation.numberofpages | 7 | en_US |
dc.type.referee | REF_3 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | DEU | en_US |
dc.relation.alleditors | den Herder, Jan-Willem A.; Nikzad, Shouleh; Nakazawa, Kazuhiro | en_US |
dc.relation.ispartofbook | Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray | en_US |
dc.relation.conferenceplace | Austin, Texas, USA | en_US |
dc.relation.conferencedate | 10-15 June, 2018 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | PROCEEDINGS OF SPIE | en_US |
dc.identifier.adsbibcode | 2018SPIE10699E..34S | en_US |
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 | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0002-7585-8605 | - |
crisitem.journal.journalissn | 0277-786X | - |
crisitem.journal.ance | E136238 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1069934 (1).pdf | Pdf editoriale | 649.78 kB | Adobe PDF | View/Open |
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