Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24295
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Galy, Camille | en_US |
dc.contributor.author | FINESCHI, Silvano | en_US |
dc.contributor.author | Galano, Damien | en_US |
dc.contributor.author | Howard, R. A. | en_US |
dc.contributor.author | Kintziger, C. | en_US |
dc.contributor.author | Kirschner, V. | en_US |
dc.contributor.author | Koutchmy, Serge | en_US |
dc.contributor.author | Lamy, Philippe | en_US |
dc.contributor.author | Mazzoli, A. | en_US |
dc.contributor.author | Melich, R. | en_US |
dc.contributor.author | Mestreau-Garreau, Agnes | en_US |
dc.contributor.author | Renotte, Etienne | en_US |
dc.contributor.author | Servaye, J. S. | en_US |
dc.contributor.author | Stockman, Y. | en_US |
dc.contributor.author | Thizy, Cedric | en_US |
dc.contributor.author | Zhukov, Andrei | en_US |
dc.date.accessioned | 2020-04-28T16:59:24Z | - |
dc.date.available | 2020-04-28T16:59:24Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.isbn | 9781628417708 | en_US |
dc.identifier.issn | 0277-786X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24295 | - |
dc.description.abstract | In the framework of development of ASPIICS (Association of Spacecraft for Polarimetric and Imaging Investigation of the Corona of the Sun), the Centre Spatial de Liege is responsible of the optical design of the coronagraph and the optics will be manufactured by TOPTEC. The particularity of this coronagraph is to have an external occulter located 150 m ahead of the first imaging lens. This external occulter is re-imaged on an internal occulter which function is - as in a classical externally occulted Lyot coronagraph - to block the sun light diffracted by the external occulter and to reduce the straylight on the detector. The selection of this configuration is driven by the requirement to observe the corona as close as possible to the solar limb (i.e. 1 R<SUB>Sun</SUB>) without imaging the limb itself. A requirement of 1.08 R<SUB>Sun</SUB> is specified at optical design level to grant 1.2 R<SUB>sun</SUB> at instrument level. The coronograph instrument is designed to have a field of view of 1.6° x 1.6° with a resolution of less than 6 arcsec. Its performances are limited by diffraction in a 530 - 590 nm wavelength range. This paper presents the optical design and demonstrates that by design the requirements are fulfilled within the misalignment, manufacturing and thermo-elastic error contributions. | en_US |
dc.language.iso | eng | en_US |
dc.title | Design and modelisation of ASPIICS optics | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1117/12.2188404 | en_US |
dc.identifier.scopus | 2-s2.0-84951335425 | en_US |
dc.identifier.isi | 000366021400009 | en_US |
dc.identifier.url | https://www.spiedigitallibrary.org/conference-proceedings-of-spie/9604/96040B/Design-and-modelisation-of-ASPIICS-optics/10.1117/12.2188404.short | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 9604 | en_US |
dc.relation.firstpage | 96040B | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 16 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | BEL | en_US |
dc.relation.alleditors | Fineschi, Silvano; Fennelly, Judy | en_US |
dc.relation.ispartofbook | Solar Physics and Space Weather Instrumentation VI | en_US |
dc.publisher.name | SPIE | en_US |
dc.publisher.place | Bellingham, WA | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Solar Physics and Space Weather Instrumentation VI | en_US |
dc.relation.conferenceplace | San Diego, CA, USA | en_US |
dc.relation.conferencedate | 9-13 August, 2015 | 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 | 2015SPIE.9604E..0BG | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | sì | 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 | O.A. Torino | - |
crisitem.author.orcid | 0000-0002-2789-816X | - |
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 | |
---|---|---|---|---|
2015_SPIE_Renotte_Design status of ASPIICS-PROBA-3.pdf | pdf editoriale | 1.32 MB | Adobe PDF | View/Open |
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