Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators
Liquid crystal variable retarders (LCVRs) will be used for the first time in a space instrument, the Solar Orbiter mission of the European Space Agency, as polarization states analyzers (PSAs). These devices will determine the Stokes parameters of the light coming from the Sun by temporal polarizati...
| Autores: | , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2020 |
| País: | España |
| Institución: | Universidad de Barcelona |
| Repositorio: | Dipòsit Digital de la UB |
| OAI Identifier: | oai:diposit.ub.edu:2445/177604 |
| Acceso en línea: | https://hdl.handle.net/2445/177604 |
| Access Level: | acceso abierto |
| Palabra clave: | Moduladors (Electrònica) Polarització (Física nuclear) Modulators (Electronics) Polarization (Nuclear physics) |
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Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulatorsGarcia Parejo, PilarCampos Jara, AntonioGarcía Caurel, EnricArteaga Barriel, OriolÁlvarez Herrero, AlbertoModuladors (Electrònica)Polarització (Física nuclear)Modulators (Electronics)Polarization (Nuclear physics)Liquid crystal variable retarders (LCVRs) will be used for the first time in a space instrument, the Solar Orbiter mission of the European Space Agency, as polarization states analyzers (PSAs). These devices will determine the Stokes parameters of the light coming from the Sun by temporal polarization modulation, using the so-called modulation matrix O. This is a matrix constituted by the first rows of properly selected PSA Mueller matrices. Calibrating a space instrument, in particular, finding O, is a critical point because in a spacecraft there is no possibility of physical access. Due to the huge difficulty in calibrating the complete instruments in all possible scenarios, a more complete calibration of the individual components has been done in ground in order to make extrapolations to obtain O in-flight. Nevertheless, apart from the individual calibrations, the experimental errors and nonideal effects that inhibit the system to reach the designed and theoretical values must be known. In this work, description and study of these effects have been done, focusing on the nonideal effects of the LCVRs and the azimuthal misalignments between the optical components of the PSA during the mechanical assembly. The Mueller matrix of a representative LCVR has been measured and mathematically decomposed by logarithm decomposition, looking for values of circular birefringence and fast axis angle variations as a function of voltage. These effects, in the absence of other nonidealities, affect the polarimetric performance, reducing the polarimetric efficiencies in some cases until 11%. Nevertheless, in this case, they are negligible if compared to the other nonideality studied, which are the azimuthal misalignments between the PSA optical components. The study presented in this work is key to extrapolate the PSA O matrix if the expected instrumental set-point temperatures are not reached in flight and can be used for the design and implementation of other polarimetric instruments.American Vacuum Society2020info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttps://hdl.handle.net/2445/177604Articles publicats en revistes (Física Aplicada)reponame:Dipòsit Digital de la UBinstname:Universidad de BarcelonaInglésReproducció del document publicat a: https://doi.org/10.1116/1.5122749Journal of Vacuum Science & Technology B, 2020, vol. 38, num. 1https://doi.org/10.1116/1.5122749(c) American Vacuum Society, 2020info:eu-repo/semantics/openAccessoai:diposit.ub.edu:2445/1776042026-05-27T06:46:51Z |
| dc.title.none.fl_str_mv |
Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators |
| title |
Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators |
| spellingShingle |
Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators Garcia Parejo, Pilar Moduladors (Electrònica) Polarització (Física nuclear) Modulators (Electronics) Polarization (Nuclear physics) |
| title_short |
Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators |
| title_full |
Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators |
| title_fullStr |
Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators |
| title_full_unstemmed |
Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators |
| title_sort |
Nonideal optical response of liquid crystal variable retarders and its impact on their performance as polarization modulators |
| dc.creator.none.fl_str_mv |
Garcia Parejo, Pilar Campos Jara, Antonio García Caurel, Enric Arteaga Barriel, Oriol Álvarez Herrero, Alberto |
| author |
Garcia Parejo, Pilar |
| author_facet |
Garcia Parejo, Pilar Campos Jara, Antonio García Caurel, Enric Arteaga Barriel, Oriol Álvarez Herrero, Alberto |
| author_role |
author |
| author2 |
Campos Jara, Antonio García Caurel, Enric Arteaga Barriel, Oriol Álvarez Herrero, Alberto |
| author2_role |
author author author author |
| dc.subject.none.fl_str_mv |
Moduladors (Electrònica) Polarització (Física nuclear) Modulators (Electronics) Polarization (Nuclear physics) |
| topic |
Moduladors (Electrònica) Polarització (Física nuclear) Modulators (Electronics) Polarization (Nuclear physics) |
| description |
Liquid crystal variable retarders (LCVRs) will be used for the first time in a space instrument, the Solar Orbiter mission of the European Space Agency, as polarization states analyzers (PSAs). These devices will determine the Stokes parameters of the light coming from the Sun by temporal polarization modulation, using the so-called modulation matrix O. This is a matrix constituted by the first rows of properly selected PSA Mueller matrices. Calibrating a space instrument, in particular, finding O, is a critical point because in a spacecraft there is no possibility of physical access. Due to the huge difficulty in calibrating the complete instruments in all possible scenarios, a more complete calibration of the individual components has been done in ground in order to make extrapolations to obtain O in-flight. Nevertheless, apart from the individual calibrations, the experimental errors and nonideal effects that inhibit the system to reach the designed and theoretical values must be known. In this work, description and study of these effects have been done, focusing on the nonideal effects of the LCVRs and the azimuthal misalignments between the optical components of the PSA during the mechanical assembly. The Mueller matrix of a representative LCVR has been measured and mathematically decomposed by logarithm decomposition, looking for values of circular birefringence and fast axis angle variations as a function of voltage. These effects, in the absence of other nonidealities, affect the polarimetric performance, reducing the polarimetric efficiencies in some cases until 11%. Nevertheless, in this case, they are negligible if compared to the other nonideality studied, which are the azimuthal misalignments between the PSA optical components. The study presented in this work is key to extrapolate the PSA O matrix if the expected instrumental set-point temperatures are not reached in flight and can be used for the design and implementation of other polarimetric instruments. |
| publishDate |
2020 |
| dc.date.none.fl_str_mv |
2020 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
https://hdl.handle.net/2445/177604 |
| url |
https://hdl.handle.net/2445/177604 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
Reproducció del document publicat a: https://doi.org/10.1116/1.5122749 Journal of Vacuum Science & Technology B, 2020, vol. 38, num. 1 https://doi.org/10.1116/1.5122749 |
| dc.rights.none.fl_str_mv |
(c) American Vacuum Society, 2020 info:eu-repo/semantics/openAccess |
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(c) American Vacuum Society, 2020 |
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openAccess |
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application/pdf |
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American Vacuum Society |
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American Vacuum Society |
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Articles publicats en revistes (Física Aplicada) reponame:Dipòsit Digital de la UB instname:Universidad de Barcelona |
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Universidad de Barcelona |
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Dipòsit Digital de la UB |
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Dipòsit Digital de la UB |
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