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Clear widens the field for observations of the Sun with multi-conjugate adaptive optics

dc.contributor.authorSchmidt, Dirk
dc.contributor.authorGorceix, Nicolas
dc.contributor.authorGoode, Philip R.
dc.contributor.authorMarino, José
dc.contributor.authorRimmele, Thomas R.
dc.contributor.authorBerkefeld, Thomas H.
dc.contributor.authorWöger, Friedrich
dc.contributor.authorZhang, Xianyu
dc.contributor.authorRigaut, Francois
dc.contributor.authorVon Der Lühe, Oskar F.
dc.date.accessioned2020-12-20T20:51:52Z
dc.date.available2020-12-20T20:51:52Z
dc.date.issued2017
dc.date.updated2020-11-23T10:19:17Z
dc.description.abstractThe multi-conjugate adaptive optics (MCAO) pathfinder Clear on the New Solar Telescope in Big Bear Lake has provided the first-ever MCAO-corrected observations of the Sun that show a clearly and visibly widened corrected field of view compared to quasi-simultaneous observations with classical adaptive optics (CAO) correction. Clear simultaneously uses three deformable mirrors, each conjugated to a different altitude, to compensate for atmospheric turbulence. While the MCAO correction was most effective over an angle that is approximately three times wider than the angle that was corrected by CAO, the full 53′′ field of view did benefit from MCAO correction. We further demonstrate that ground-layer-only correction is attractive for solar observations as a complementary flavor of adaptive optics for observational programs that require homogenous seeing improvement over a wide field rather than diffraction-limited resolution. We show illustrative images of solar granulation and of a sunspot obtained on different days in July 2016, and present a brief quantitative analysis of the generalized Fried parameters of the images
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/217910
dc.language.isoen_AUen_AU
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.titleClear widens the field for observations of the Sun with multi-conjugate adaptive optics
dc.typeJournal article
local.contributor.affiliationSchmidt, Dirk, National Solar Observatory
local.contributor.affiliationGorceix, Nicolas, Big Bear Solar Observatory
local.contributor.affiliationGoode, Philip R., Big Bear Solar Observatory
local.contributor.affiliationMarino, José, National Solar Observatory
local.contributor.affiliationRimmele, Thomas R., National Solar Observatory
local.contributor.affiliationBerkefeld, Thomas H., Kiepenheuer-Institut fur Sonnenphysik
local.contributor.affiliationWöger, Friedrich, National Solar Observatory
local.contributor.affiliationZhang, Xianyu, Large Binocular Telescope Observatory
local.contributor.affiliationRigaut, Francois, College of Science, ANU
local.contributor.affiliationVon Der Lühe, Oskar F., Kiepenheuer-Institut fur Sonnenphysik
local.contributor.authoruidRigaut, Francois, u5090915
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationa383154xPUB6339
local.identifier.citationvolume597
local.identifier.doi10.1051/0004-6361/201629970
local.identifier.scopusID2-s2.0-85009260900
local.identifier.thomsonID000392392900147
local.type.statusPublished Version

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