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The European Solar ...
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Quintero Noda, C.University of La Laguna (ULL)
(author)
The European Solar Telescope
- Article/chapterEnglish2022
Publisher, publication year, extent ...
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2022-09-30
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EDP Sciences,2022
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printrdacarrier
Numbers
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LIBRIS-ID:oai:DiVA.org:su-211140
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https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-211140URI
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https://doi.org/10.1051/0004-6361/202243867DOI
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https://lup.lub.lu.se/record/e96d404b-b5b4-4367-82a6-be6f45a81f01URI
Supplementary language notes
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Language:English
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Summary in:English
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Classification
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Subject category:ref swepub-contenttype
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Subject category:art swepub-publicationtype
Notes
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The European Solar Telescope (EST) is a project aimed at studying the magnetic connectivity of the solar atmosphere, from the deep photosphere to the upper chromosphere. Its design combines the knowledge and expertise gathered by the European solar physics community during the construction and operation of state-of-the-art solar telescopes operating in visible and near-infrared wavelengths: the Swedish 1m Solar Telescope, the German Vacuum Tower Telescope and GREGOR, the French Télescope Héliographique pour l’Étude du Magnétisme et des Instabilités Solaires, and the Dutch Open Telescope. With its 4.2 m primary mirror and an open configuration, EST will become the most powerful European ground-based facility to study the Sun in the coming decades in the visible and near-infrared bands. EST uses the most innovative technological advances: the first adaptive secondary mirror ever used in a solar telescope, a complex multi-conjugate adaptive optics with deformable mirrors that form part of the optical design in a natural way, a polarimetrically compensated telescope design that eliminates the complex temporal variation and wavelength dependence of the telescope Mueller matrix, and an instrument suite containing several (etalon-based) tunable imaging spectropolarimeters and several integral field unit spectropolarimeters. This publication summarises some fundamental science questions that can be addressed with the telescope, together with a complete description of its major subsystems.
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Löfdahl, Mats G.,1961-Stockholms universitet,Institutionen för astronomi(Swepub:su)lofda
(author)
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Leenaarts, JorritStockholms universitet,Institutionen för astronomi(Swepub:su)jleen
(author)
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de la Cruz Rodríguez, Jaime,1983-Stockholms universitet,Institutionen för astronomi(Swepub:su)jade0464
(author)
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Danilovic, SanjaStockholms universitet,Institutionen för astronomi(Swepub:su)sdani
(author)
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Díaz Baso, Carlos JoséStockholms universitet,Institutionen för astronomi(Swepub:su)cada4215
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Kiselman, Dan,1963-Stockholms universitet,Institutionen för astronomi(Swepub:su)dan
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Lindberg, BoStockholms universitet,Institutionen för astronomi
(author)
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Pastor Yabar, AdurStockholms universitet,Institutionen för astronomi(Swepub:su)adpa7375
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Scharmer, GöranStockholms universitet,Institutionen för astronomi(Swepub:su)scharmer
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Sliepen, GuusStockholms universitet,Institutionen för astronomi(Swepub:su)gslil
(author)
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Sütterlin, PeterStockholms universitet,Institutionen för astronomi(Swepub:su)pets
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Collados, M.University of La Laguna (ULL)
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González, J.B.Lund University,Lunds universitet,MAX IV-laboratoriet,MAX IV Laboratory(Swepub:lu)jo0832go
(author)
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University of La Laguna (ULL)Institutionen för astronomi
(creator_code:org_t)
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et al.
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In:Astronomy and Astrophysics: EDP Sciences6660004-63611432-0746
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Collados, M.
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