GOLD’s coating and testing facilities for ISSIS-WSO
ISSIS imager has been thought as an open purpose instrument within the World Space Observatory (WSO) international space mission. The highest priorities of ISSIS, an instrument to be developed by Spain, are to guarantee high spatial resolution and high sensitivity down to the far ultraviolet (FUV)....
Gespeichert in:
| Veröffentlicht in: | Astrophysics and space science 2011-09, Vol.335 (1), p.305-309 |
|---|---|
| Hauptverfasser: | , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 309 |
|---|---|
| container_issue | 1 |
| container_start_page | 305 |
| container_title | Astrophysics and space science |
| container_volume | 335 |
| creator | Larruquert, Juan I. Méndez, José Antonio Aznárez, José Antonio Vidal-Dasilva, Manuela García-Cortés, Sergio Rodríguez-de Marcos, Luis Fernández-Perea, Mónica |
| description | ISSIS imager has been thought as an open purpose instrument within the
World Space Observatory (WSO)
international space mission. The highest priorities of ISSIS, an instrument to be developed by Spain, are to guarantee high spatial resolution and high sensitivity down to the far ultraviolet (FUV). The paper displays the capacities of GOLD for multilayer deposition and FUV reflectometry, among other metrologies, for ISSIS optical elements.
Deposition of coatings for ISSIS–WSO will be carried out in a new UHV system with a 75-cm diameter deposition chamber. The purpose of the new laboratory is the deposition of coatings satisfying the constraints for FUV space optics. The first target coating to be developed in this new laboratory is Al protected with MgF
2
, with optimum reflectance down to ∼120 nm.
GOLD’s existing reflectometer is able to characterize flat pieces both by transmittance and reflectance, and the latter from near-normal to grazing incidence, in the range from 12 to 200 nm. Other metrologies that will be available at GOLD for ISSIS’s coatings and filters include optical thickness of filters to assure parfocality, filter wedge, and coating and filter scattering. |
| doi_str_mv | 10.1007/s10509-011-0666-1 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_899143645</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2417304101</sourcerecordid><originalsourceid>FETCH-LOGICAL-c347t-2147af9f23e9d0b92a25f1111faff5f3ad9ba9f8b54842243434c12bee748fcb3</originalsourceid><addsrcrecordid>eNp1kM9KAzEQxoMoWKsP4G3x4imaSbLZ5Cj-qYVCD6vYW8imSdmy3a3J9uDN1_D1fBJTVxAEZw4zA7_vY_gQOgdyBYQU1xFIThQmAJgIITAcoBHkBcWKi8UhGhFCOBacLI7RSYzrdCqhihHKJ_PZ3ef7R8xsZ_q6XWWmXWa9i9-7N7Zu6r52MfNdyKZlOS3xSzk_RUfeNNGd_cwxen64f7p9xLP5ZHp7M8OW8aLHFHhhvPKUObUklaKG5h5SeeN97plZqsooL6ucS04pZ6kt0Mq5gktvKzZGl4PvNnSvu_SU3tTRuqYxret2UUulgDPB80Re_CHX3S606TktJTAmqeQJggGyoYsxOK-3od6Y8KaB6H2MeohRpxj1PkYNSUMHTUxsu3Lh1_h_0Rd51HOy</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>881338284</pqid></control><display><type>article</type><title>GOLD’s coating and testing facilities for ISSIS-WSO</title><source>SpringerLink Journals</source><creator>Larruquert, Juan I. ; Méndez, José Antonio ; Aznárez, José Antonio ; Vidal-Dasilva, Manuela ; García-Cortés, Sergio ; Rodríguez-de Marcos, Luis ; Fernández-Perea, Mónica</creator><creatorcontrib>Larruquert, Juan I. ; Méndez, José Antonio ; Aznárez, José Antonio ; Vidal-Dasilva, Manuela ; García-Cortés, Sergio ; Rodríguez-de Marcos, Luis ; Fernández-Perea, Mónica</creatorcontrib><description>ISSIS imager has been thought as an open purpose instrument within the
World Space Observatory (WSO)
international space mission. The highest priorities of ISSIS, an instrument to be developed by Spain, are to guarantee high spatial resolution and high sensitivity down to the far ultraviolet (FUV). The paper displays the capacities of GOLD for multilayer deposition and FUV reflectometry, among other metrologies, for ISSIS optical elements.
Deposition of coatings for ISSIS–WSO will be carried out in a new UHV system with a 75-cm diameter deposition chamber. The purpose of the new laboratory is the deposition of coatings satisfying the constraints for FUV space optics. The first target coating to be developed in this new laboratory is Al protected with MgF
2
, with optimum reflectance down to ∼120 nm.
GOLD’s existing reflectometer is able to characterize flat pieces both by transmittance and reflectance, and the latter from near-normal to grazing incidence, in the range from 12 to 200 nm. Other metrologies that will be available at GOLD for ISSIS’s coatings and filters include optical thickness of filters to assure parfocality, filter wedge, and coating and filter scattering.</description><identifier>ISSN: 0004-640X</identifier><identifier>EISSN: 1572-946X</identifier><identifier>DOI: 10.1007/s10509-011-0666-1</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Astrobiology ; Astronomy ; Astrophysics ; Astrophysics and Astroparticles ; Coatings ; Cosmology ; Filters ; Gold ; Observations and Techniques ; Optics ; Original Article ; Physics ; Physics and Astronomy ; Reflectance ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Space telescopes ; Ultraviolet astronomy</subject><ispartof>Astrophysics and space science, 2011-09, Vol.335 (1), p.305-309</ispartof><rights>Springer Science+Business Media B.V. 2011</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c347t-2147af9f23e9d0b92a25f1111faff5f3ad9ba9f8b54842243434c12bee748fcb3</citedby><cites>FETCH-LOGICAL-c347t-2147af9f23e9d0b92a25f1111faff5f3ad9ba9f8b54842243434c12bee748fcb3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10509-011-0666-1$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10509-011-0666-1$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,777,781,27905,27906,41469,42538,51300</link.rule.ids></links><search><creatorcontrib>Larruquert, Juan I.</creatorcontrib><creatorcontrib>Méndez, José Antonio</creatorcontrib><creatorcontrib>Aznárez, José Antonio</creatorcontrib><creatorcontrib>Vidal-Dasilva, Manuela</creatorcontrib><creatorcontrib>García-Cortés, Sergio</creatorcontrib><creatorcontrib>Rodríguez-de Marcos, Luis</creatorcontrib><creatorcontrib>Fernández-Perea, Mónica</creatorcontrib><title>GOLD’s coating and testing facilities for ISSIS-WSO</title><title>Astrophysics and space science</title><addtitle>Astrophys Space Sci</addtitle><description>ISSIS imager has been thought as an open purpose instrument within the
World Space Observatory (WSO)
international space mission. The highest priorities of ISSIS, an instrument to be developed by Spain, are to guarantee high spatial resolution and high sensitivity down to the far ultraviolet (FUV). The paper displays the capacities of GOLD for multilayer deposition and FUV reflectometry, among other metrologies, for ISSIS optical elements.
Deposition of coatings for ISSIS–WSO will be carried out in a new UHV system with a 75-cm diameter deposition chamber. The purpose of the new laboratory is the deposition of coatings satisfying the constraints for FUV space optics. The first target coating to be developed in this new laboratory is Al protected with MgF
2
, with optimum reflectance down to ∼120 nm.
GOLD’s existing reflectometer is able to characterize flat pieces both by transmittance and reflectance, and the latter from near-normal to grazing incidence, in the range from 12 to 200 nm. Other metrologies that will be available at GOLD for ISSIS’s coatings and filters include optical thickness of filters to assure parfocality, filter wedge, and coating and filter scattering.</description><subject>Astrobiology</subject><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Coatings</subject><subject>Cosmology</subject><subject>Filters</subject><subject>Gold</subject><subject>Observations and Techniques</subject><subject>Optics</subject><subject>Original Article</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Reflectance</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Space telescopes</subject><subject>Ultraviolet astronomy</subject><issn>0004-640X</issn><issn>1572-946X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp1kM9KAzEQxoMoWKsP4G3x4imaSbLZ5Cj-qYVCD6vYW8imSdmy3a3J9uDN1_D1fBJTVxAEZw4zA7_vY_gQOgdyBYQU1xFIThQmAJgIITAcoBHkBcWKi8UhGhFCOBacLI7RSYzrdCqhihHKJ_PZ3ef7R8xsZ_q6XWWmXWa9i9-7N7Zu6r52MfNdyKZlOS3xSzk_RUfeNNGd_cwxen64f7p9xLP5ZHp7M8OW8aLHFHhhvPKUObUklaKG5h5SeeN97plZqsooL6ucS04pZ6kt0Mq5gktvKzZGl4PvNnSvu_SU3tTRuqYxret2UUulgDPB80Re_CHX3S606TktJTAmqeQJggGyoYsxOK-3od6Y8KaB6H2MeohRpxj1PkYNSUMHTUxsu3Lh1_h_0Rd51HOy</recordid><startdate>20110901</startdate><enddate>20110901</enddate><creator>Larruquert, Juan I.</creator><creator>Méndez, José Antonio</creator><creator>Aznárez, José Antonio</creator><creator>Vidal-Dasilva, Manuela</creator><creator>García-Cortés, Sergio</creator><creator>Rodríguez-de Marcos, Luis</creator><creator>Fernández-Perea, Mónica</creator><general>Springer Netherlands</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20110901</creationdate><title>GOLD’s coating and testing facilities for ISSIS-WSO</title><author>Larruquert, Juan I. ; Méndez, José Antonio ; Aznárez, José Antonio ; Vidal-Dasilva, Manuela ; García-Cortés, Sergio ; Rodríguez-de Marcos, Luis ; Fernández-Perea, Mónica</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c347t-2147af9f23e9d0b92a25f1111faff5f3ad9ba9f8b54842243434c12bee748fcb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Astrobiology</topic><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Astrophysics and Astroparticles</topic><topic>Coatings</topic><topic>Cosmology</topic><topic>Filters</topic><topic>Gold</topic><topic>Observations and Techniques</topic><topic>Optics</topic><topic>Original Article</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Reflectance</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Space telescopes</topic><topic>Ultraviolet astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Larruquert, Juan I.</creatorcontrib><creatorcontrib>Méndez, José Antonio</creatorcontrib><creatorcontrib>Aznárez, José Antonio</creatorcontrib><creatorcontrib>Vidal-Dasilva, Manuela</creatorcontrib><creatorcontrib>García-Cortés, Sergio</creatorcontrib><creatorcontrib>Rodríguez-de Marcos, Luis</creatorcontrib><creatorcontrib>Fernández-Perea, Mónica</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Astrophysics and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Larruquert, Juan I.</au><au>Méndez, José Antonio</au><au>Aznárez, José Antonio</au><au>Vidal-Dasilva, Manuela</au><au>García-Cortés, Sergio</au><au>Rodríguez-de Marcos, Luis</au><au>Fernández-Perea, Mónica</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>GOLD’s coating and testing facilities for ISSIS-WSO</atitle><jtitle>Astrophysics and space science</jtitle><stitle>Astrophys Space Sci</stitle><date>2011-09-01</date><risdate>2011</risdate><volume>335</volume><issue>1</issue><spage>305</spage><epage>309</epage><pages>305-309</pages><issn>0004-640X</issn><eissn>1572-946X</eissn><abstract>ISSIS imager has been thought as an open purpose instrument within the
World Space Observatory (WSO)
international space mission. The highest priorities of ISSIS, an instrument to be developed by Spain, are to guarantee high spatial resolution and high sensitivity down to the far ultraviolet (FUV). The paper displays the capacities of GOLD for multilayer deposition and FUV reflectometry, among other metrologies, for ISSIS optical elements.
Deposition of coatings for ISSIS–WSO will be carried out in a new UHV system with a 75-cm diameter deposition chamber. The purpose of the new laboratory is the deposition of coatings satisfying the constraints for FUV space optics. The first target coating to be developed in this new laboratory is Al protected with MgF
2
, with optimum reflectance down to ∼120 nm.
GOLD’s existing reflectometer is able to characterize flat pieces both by transmittance and reflectance, and the latter from near-normal to grazing incidence, in the range from 12 to 200 nm. Other metrologies that will be available at GOLD for ISSIS’s coatings and filters include optical thickness of filters to assure parfocality, filter wedge, and coating and filter scattering.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s10509-011-0666-1</doi><tpages>5</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-640X |
| ispartof | Astrophysics and space science, 2011-09, Vol.335 (1), p.305-309 |
| issn | 0004-640X 1572-946X |
| language | eng |
| recordid | cdi_proquest_miscellaneous_899143645 |
| source | SpringerLink Journals |
| subjects | Astrobiology Astronomy Astrophysics Astrophysics and Astroparticles Coatings Cosmology Filters Gold Observations and Techniques Optics Original Article Physics Physics and Astronomy Reflectance Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Space telescopes Ultraviolet astronomy |
| title | GOLD’s coating and testing facilities for ISSIS-WSO |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-18T05%3A44%3A40IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=GOLD%E2%80%99s%20coating%20and%20testing%20facilities%20for%20ISSIS-WSO&rft.jtitle=Astrophysics%20and%20space%20science&rft.au=Larruquert,%20Juan%20I.&rft.date=2011-09-01&rft.volume=335&rft.issue=1&rft.spage=305&rft.epage=309&rft.pages=305-309&rft.issn=0004-640X&rft.eissn=1572-946X&rft_id=info:doi/10.1007/s10509-011-0666-1&rft_dat=%3Cproquest_cross%3E2417304101%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=881338284&rft_id=info:pmid/&rfr_iscdi=true |