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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4ADMK3L
Repositorysid.inpe.br/mtc-m21d/2023/12.20.19.15   (restricted access)
Last Update2023:12.20.19.15.24 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2023/12.20.19.15.24
Metadata Last Update2023:12.23.13.49.32 (UTC) administrator
DOI10.1007/s11207-023-02237-z
ISSN0038-0938
1573-093X
Citation KeyJessGBLJKVDGCGB:2023:FiReOp
TitleThe Fibre Resolved OpticAl and Near-Ultraviolet Czerny–Turner Imaging Spectropolarimeter (FRANCIS)
Year2023
Access Date2024, June 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size5624 KiB
2. Context
Author 1 Jess, David B.
 2 Grant, Samuel D. T.
 3 Bate, William
 4 Liu, Jiajia
 5 Jafarzadeh, Shahin
 6 Keys, Peter H.
 7 Vieira, Luis Eduardo Antunes
 8 Dal Lago, Alisson
 9 Guarnieri, Fernando Luis
10 Christian, Damian J.
11 Gilliam, Doug
12 Banerjee, Dipankar
Resume Identifier 1
 2
 3
 4
 5
 6
 7
 8 8JMKD3MGP5W/3C9JGH3
ORCID 1 0000-0002-9155-8039
 2 0000-0001-5170-9747
 3 0000-0001-9629-5250
 4 0000-0003-2569-1840
 5 0000-0002-7711-5397
 6 0000-0001-8556-470X
 7 0000-0002-9376-475X
 8 0000-0002-4361-6492
 9 0000-0007-2353-2594
10 0000-0003-1746-3020
11
12 0000-0003-4653-6823
Group 1
 2
 3
 4
 5
 6
 7 DIHPA-CGCE-INPE-MCTI-GOV-BR
 8 DIHPA-CGCE-INPE-MCTI-GOV-BR
 9 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation 1 Queen’s University Belfast
 2 Queen’s University Belfast
 3 Queen’s University Belfast
 4 University of Science and Technology of China
 5 Max Planck Institute for Solar System Research
 6 Queen’s University Belfast
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 California State University Northridge
11 Big Bear Solar Observatory
12 Aryabhatta Research Institute of Observational Sciences
Author e-Mail Address 1 d.jess@qub.ac.uk
 2 samuel.grant@qub.ac.uk
 3 wbate02@qub.ac.uk
 4 wbate02@qub.ac.uk
 5 shahin.jafarzadeh@mps.mpg.de
 6 p.keys@qub.ac.uk
 7 luis.vieira@inpe.br
 8 alisson.dallago@inpe.br
 9 fernando.guarnieri@inpe.br
10 damian.christian@csun.edu
11 douglas.gilliam@njit.edu
12 directoraries@aries.res.in
JournalSolar Physics
Volume298
Pagese146
Secondary MarkA2_INTERDISCIPLINAR A2_GEOCIÊNCIAS A2_BIOTECNOLOGIA B1_ENGENHARIAS_IV B1_ASTRONOMIA_/_FÍSICA B2_CIÊNCIA_DA_COMPUTAÇÃO
History (UTC)2023-12-20 19:15:24 :: simone -> administrator ::
2023-12-20 19:15:28 :: administrator -> simone :: 2023
2023-12-20 19:16:59 :: simone -> administrator :: 2023
2023-12-23 13:49:32 :: administrator -> simone :: 2023
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAstronomical instrumentation
Solar atmosphere
Solar radiation
Spectrometers
Spectropolarimetry
AbstractThe solar physics community is entering a golden era that is ripe with next-generation ground- and space-based facilities, advanced spectral inversion techniques, and realistic simulations that are becoming more computationally streamlined and efficient. With everincreasing resolving power stemming from the newest observational telescopes, it becomes more challenging to obtain (near-)simultaneous measurements at high spatial, temporal and spectral resolutions, while operating at the diffraction limit of these new facilities. Hence, in recent years there has been increased interest in the capabilities integral field units (IFUs) offer towards obtaining the trifecta of high spatial, temporal and spectral resolutions contemporaneously. To date, IFUs developed for solar physics research have focused on mid-optical and infrared measurements. Here, we present an IFU prototype that has been designed for operation within the near-ultraviolet to mid-optical wavelength range, which enables key spectral lines (e.g., Ca II H/K, Hβ, Sr II, Na I D1/D2, etc.) to be studied, hence providing additional spectral coverage to the instrument suites developed to date. The IFU was constructed as a low-budget proof-of-concept for the upcoming 2 m class Indian National Large Solar Telescope and employs circular cross-section fibres to guide light into a Czerny Turner configuration spectrograph, with the resulting spectra captured using a high quantum efficiency scientific CMOS camera. Mapping of each input fibre allows for the reconstruction of two-dimensional spectral images, with frame rates exceeding 20 s−1 possible while operating in a non-polarimetric configuration. Initial commissioning of the instrument was performed at the Dunn Solar Telescope, USA, during August 2022. The science verification data presented here highlights the suitability of fibre-fed IFUs operating at near-ultraviolet wavelengths for solar physics research. Importantly, the successful demonstration of this type of instrument paves the way for further technological developments to make a future variant suitable for upcoming ground-based and space-borne telescope facilities.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > The Fibre Resolved...
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4. Conditions of access and use
Languageen
Target Files11207-023-02237-z.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2021/06.04.03.40.25
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.39.46 8
sid.inpe.br/bibdigital/2022/04.03.17.52 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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