Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images

This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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Autores: Bailén, Francisco Javier, Orozco Suárez, David, Rodríguez, J. Blanco, Toro, José Carlos del, Strecker, H., Moreno Vacas, Alejandro, Santamarina, Pablo, Hirzberger, J., Albert, K., Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Gandorfer, A., Germerott, D., Guerrero, L., Gutierrez-Marques, P., Kahil, F., Kolleck, M., Solanki, S. K., Volkmer, R., Woch, J., Fiethe, B., Cama, J. M.Gómez, Pérez-Grande, I., Kilders, E. Sanchis, Balaguer Jiménez, M., Bellot Rubio, Luis R., Calchetti, D., Alonso Carmona, M. Isabel, Deutsch, W., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., Parejo, P. García, Blesa, J. L.Gasent, Gizon, L., Grauf, B., Heerlein, K., Korpi-Lagg, A., Lange, T., López Jiménez, A. C., Maue, T., Meller, R., Michalik, H., Müller, R., Nakai, E., Schmidt, W., Schou, J., Schühle, U., Staub, J., Torralbo, I., Valori, G.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/369622
Acceso en línea:http://hdl.handle.net/10261/369622
https://api.elsevier.com/content/abstract/scopus_id/85183753946
Access Level:acceso abierto
Palabra clave:Instrumentation: polarimeters
Sun: magnetic fields
Sun: photosphere
Techniques: image processing
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dc.title.none.fl_str_mv Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images
title Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images
spellingShingle Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images
Bailén, Francisco Javier
Instrumentation: polarimeters
Sun: magnetic fields
Sun: photosphere
Techniques: image processing
title_short Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images
title_full Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images
title_fullStr Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images
title_full_unstemmed Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images
title_sort Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images
dc.creator.none.fl_str_mv Bailén, Francisco Javier
Orozco Suárez, David
Rodríguez, J. Blanco
Toro, José Carlos del
Strecker, H.
Moreno Vacas, Alejandro
Santamarina, Pablo
Hirzberger, J.
Albert, K.
Jorge, N. Albelo
Appourchaux, T.
Alvarez-Herrero, A.
Gandorfer, A.
Germerott, D.
Guerrero, L.
Gutierrez-Marques, P.
Kahil, F.
Kolleck, M.
Solanki, S. K.
Volkmer, R.
Woch, J.
Fiethe, B.
Cama, J. M.Gómez
Pérez-Grande, I.
Kilders, E. Sanchis
Balaguer Jiménez, M.
Bellot Rubio, Luis R.
Calchetti, D.
Alonso Carmona, M. Isabel
Deutsch, W.
Feller, A.
Fernandez-Rico, G.
Fernández-Medina, A.
Parejo, P. García
Blesa, J. L.Gasent
Gizon, L.
Grauf, B.
Heerlein, K.
Korpi-Lagg, A.
Lange, T.
López Jiménez, A. C.
Maue, T.
Meller, R.
Michalik, H.
Müller, R.
Nakai, E.
Schmidt, W.
Schou, J.
Schühle, U.
Staub, J.
Torralbo, I.
Valori, G.
author Bailén, Francisco Javier
author_facet Bailén, Francisco Javier
Orozco Suárez, David
Rodríguez, J. Blanco
Toro, José Carlos del
Strecker, H.
Moreno Vacas, Alejandro
Santamarina, Pablo
Hirzberger, J.
Albert, K.
Jorge, N. Albelo
Appourchaux, T.
Alvarez-Herrero, A.
Gandorfer, A.
Germerott, D.
Guerrero, L.
Gutierrez-Marques, P.
Kahil, F.
Kolleck, M.
Solanki, S. K.
Volkmer, R.
Woch, J.
Fiethe, B.
Cama, J. M.Gómez
Pérez-Grande, I.
Kilders, E. Sanchis
Balaguer Jiménez, M.
Bellot Rubio, Luis R.
Calchetti, D.
Alonso Carmona, M. Isabel
Deutsch, W.
Feller, A.
Fernandez-Rico, G.
Fernández-Medina, A.
Parejo, P. García
Blesa, J. L.Gasent
Gizon, L.
Grauf, B.
Heerlein, K.
Korpi-Lagg, A.
Lange, T.
López Jiménez, A. C.
Maue, T.
Meller, R.
Michalik, H.
Müller, R.
Nakai, E.
Schmidt, W.
Schou, J.
Schühle, U.
Staub, J.
Torralbo, I.
Valori, G.
author_role author
author2 Orozco Suárez, David
Rodríguez, J. Blanco
Toro, José Carlos del
Strecker, H.
Moreno Vacas, Alejandro
Santamarina, Pablo
Hirzberger, J.
Albert, K.
Jorge, N. Albelo
Appourchaux, T.
Alvarez-Herrero, A.
Gandorfer, A.
Germerott, D.
Guerrero, L.
Gutierrez-Marques, P.
Kahil, F.
Kolleck, M.
Solanki, S. K.
Volkmer, R.
Woch, J.
Fiethe, B.
Cama, J. M.Gómez
Pérez-Grande, I.
Kilders, E. Sanchis
Balaguer Jiménez, M.
Bellot Rubio, Luis R.
Calchetti, D.
Alonso Carmona, M. Isabel
Deutsch, W.
Feller, A.
Fernandez-Rico, G.
Fernández-Medina, A.
Parejo, P. García
Blesa, J. L.Gasent
Gizon, L.
Grauf, B.
Heerlein, K.
Korpi-Lagg, A.
Lange, T.
López Jiménez, A. C.
Maue, T.
Meller, R.
Michalik, H.
Müller, R.
Nakai, E.
Schmidt, W.
Schou, J.
Schühle, U.
Staub, J.
Torralbo, I.
Valori, G.
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author
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author
author
author
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dc.contributor.none.fl_str_mv Ministerio de Ciencia e Innovación (España)
European Commission
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Instrumentation: polarimeters
Sun: magnetic fields
Sun: photosphere
Techniques: image processing
topic Instrumentation: polarimeters
Sun: magnetic fields
Sun: photosphere
Techniques: image processing
description This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
publishDate 2024
dc.date.none.fl_str_mv 2024
2024
2024
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http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
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status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/369622
https://api.elsevier.com/content/abstract/scopus_id/85183753946
url http://hdl.handle.net/10261/369622
https://api.elsevier.com/content/abstract/scopus_id/85183753946
dc.language.none.fl_str_mv Inglés
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info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2021-001131-S
Astronomy and Astrophysics
http://dx.doi.org/10.1051/0004-6361/202346019

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spelling Determination of the SO/PHI-HRT wavefront degradation using multiple defocused imagesBailén, Francisco JavierOrozco Suárez, DavidRodríguez, J. BlancoToro, José Carlos delStrecker, H.Moreno Vacas, AlejandroSantamarina, PabloHirzberger, J.Albert, K.Jorge, N. AlbeloAppourchaux, T.Alvarez-Herrero, A.Gandorfer, A.Germerott, D.Guerrero, L.Gutierrez-Marques, P.Kahil, F.Kolleck, M.Solanki, S. K.Volkmer, R.Woch, J.Fiethe, B.Cama, J. M.GómezPérez-Grande, I.Kilders, E. SanchisBalaguer Jiménez, M.Bellot Rubio, Luis R.Calchetti, D.Alonso Carmona, M. IsabelDeutsch, W.Feller, A.Fernandez-Rico, G.Fernández-Medina, A.Parejo, P. GarcíaBlesa, J. L.GasentGizon, L.Grauf, B.Heerlein, K.Korpi-Lagg, A.Lange, T.López Jiménez, A. C.Maue, T.Meller, R.Michalik, H.Müller, R.Nakai, E.Schmidt, W.Schou, J.Schühle, U.Staub, J.Torralbo, I.Valori, G.Instrumentation: polarimetersSun: magnetic fieldsSun: photosphereTechniques: image processingThis is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.Context. The Polarimetric and Helioseismic Imager on board the Solar Orbiter mission (SO/PHI) offers refocusing capabilities to cope with the strongly varying thermal environment of the optical system along the spacecraft's elliptical orbit. The series of images recorded during in-flight focus calibrations can be employed for phase diversity analyses.Aims. In this work we infer the wavefront degradation caused by the thermo-optical effects in the High Resolution Telescope (HRT) from images taken during the fine and coarse focus scans performed in the commissioning phase of the instrument. The difference between these two series of images are mainly related to the employed defocused step (smaller for the fine scans) and the signal-to-noise ratio (higher for the coarse scans). We use the retrieved wavefronts to reconstruct the original scene observed during the calibration of the instrument.Methods. We applied a generalized phase diversity algorithm that allowed us to use several images taken with different amounts of defocus to sense the wavefront degradation caused by the instrument. The algorithm also uses information from both the inferred wavefront and the series of images to restore the solar scene.Results. We find that most of the retrieved Zernike coefficients tend to converge to the same value when increasing the number of images employed for PD for both the fine and the coarse focusing scans. The restored scenes also show signs of convergence, and the merit function is minimized more as K increases. Apart from a defocus, the inferred wavefronts are consistent for the two datasets (λ/10 − λ/11). For the fine scan images, the quiet-sun contrast improves from 4.5% for the original focused image up to about 10%. For the coarse scan images, the contrast of the restored scene is as high as 11%. © The Authors 2024.Solar Orbiter is a space mission of international collaboration between ESA and NASA, operated by ESA. We are grateful to the ESA SOC and MOC teams for their support. The German contribution to SO/PHI is funded by the BMWi through DLR and by MPG central funds. The Spanish contribution is funded by FEDER/AEI/MCIU (ESP-2016-77548-C5-1-R and RTI2018-096886-C5), Grant PID2021-125325OB-C51 funded by MCIN/AEI/ 10.13039/501100011033 and by “ERDF A way of making Europe”, by the “European Union”, a “Center of Excellence Severo Ochoa” award to IAA-CSIC (CEX2021-001131-S), and a Ramón y Cajal fellowship awarded to DOS. The French contribution is funded by CNES.With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).Peer reviewedEDP SciencesMinisterio de Ciencia e Innovación (España)European CommissionConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202420242024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/369622https://api.elsevier.com/content/abstract/scopus_id/85183753946reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP-2016-77548-C5-1-Rinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/RTI2018-096886-B-C51info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-125325OB-C51info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2021-001131-SAstronomy and Astrophysicshttp://dx.doi.org/10.1051/0004-6361/202346019Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3696222026-05-22T06:33:51Z
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