Hide metadata

dc.date.accessioned2023-02-27T18:35:08Z
dc.date.available2023-02-27T18:35:08Z
dc.date.created2023-02-06T12:24:25Z
dc.date.issued2022
dc.identifier.citationAnche, Ramya M. Maharana, Siddharth Ramaprakash, Anamparambu N. Khodade, Pravin Modi, Deepa Rajarshi, Chaitanya Kypriotakis, John A. Blinov, Dmitry Eriksen, Hans Kristian Kamfjord Ghosh, Tuhin Panopoulou, Georgia V. Pelgrims, Vincent Skalidis, Raphael Pearson, Timothy J. Gjerløw, Eirik Mandarakas, Nikolaos Pavlidou, Vasiliki Potter, Stephen B. Readhead, Anthony C. S. Tassis, Konstantinos Basyrov, Artem Papadaki, Katerina Svalheim, Trygve Leithe Wehus, Ingunn Kathrine . Stress-induced birefringence in the lenses of Wide-Area Linear Optical Polarimeter-South. Proceedings of SPIE, the International Society for Optical Engineering. 2022, 12188
dc.identifier.urihttp://hdl.handle.net/10852/100468
dc.description.abstractTwo unique wide-field and high-accuracy polarimeters named WALOP (Wide-Area Linear Optical Polarimeter)- North and WALOP-South are currently under development at the Inter-University Center for Astronomy and Astrophysics (IUCAA), India, to create a large area optical polarization map of the sky for the upcoming PASIPHAE sky survey. These instruments are designed to achieve a linear polarimetric measurement accuracy of 0.1% across a field of view (FoV) of 30×30 arcminutes. The WALOP-South instrument will be installed first on a 1 m telescope at the Sutherland Observatory, where the temperatures during the night can vary between 10 to -5°C. These temperature variations and the instrument’s pointing to various non-zenithal positions in the sky can introduce stress birefringence in the lenses, leading to time-varying instrumental polarization. This work estimates stress-induced birefringence due to thermal, and gravity stresses on WALOP-South lenses. Using the optomechanical model of the WALOP-South, we carried out Finite Element Analysis (FEA) simulations in SolidWorks software to estimate the stresses for various scenarios of temperature, telescope pointing airmass, and lens mount material (aluminum and titanium). Further, we use the stress tensor analysis to estimate the principal stresses and their directions and consequent birefringence and retardance introduced in the lenses. The stressinduced birefringence will change the optical path length for orthogonal polarization states of the beam passing through the lenses and introduce phase retardation. Overall, with the lens mount design of the instrument, we find that the retardation and consequent instrumental polarization will be within the instrumental accuracy requirements. Additionally, the stress birefringence is found to be higher for aluminum compared to titanium mounts. We further incorporated this retardance in the instrument Mueller matrix estimation to understand its effects on the polarization measurements.
dc.languageEN
dc.titleStress-induced birefringence in the lenses of Wide-Area Linear Optical Polarimeter-South
dc.title.alternativeENEngelskEnglishStress-induced birefringence in the lenses of Wide-Area Linear Optical Polarimeter-South
dc.typeJournal article
dc.creator.authorAnche, Ramya M.
dc.creator.authorMaharana, Siddharth
dc.creator.authorRamaprakash, Anamparambu N.
dc.creator.authorKhodade, Pravin
dc.creator.authorModi, Deepa
dc.creator.authorRajarshi, Chaitanya
dc.creator.authorKypriotakis, John A.
dc.creator.authorBlinov, Dmitry
dc.creator.authorEriksen, Hans Kristian Kamfjord
dc.creator.authorGhosh, Tuhin
dc.creator.authorPanopoulou, Georgia V.
dc.creator.authorPelgrims, Vincent
dc.creator.authorSkalidis, Raphael
dc.creator.authorPearson, Timothy J.
dc.creator.authorGjerløw, Eirik
dc.creator.authorMandarakas, Nikolaos
dc.creator.authorPavlidou, Vasiliki
dc.creator.authorPotter, Stephen B.
dc.creator.authorReadhead, Anthony C. S.
dc.creator.authorTassis, Konstantinos
dc.creator.authorBasyrov, Artem
dc.creator.authorPapadaki, Katerina
dc.creator.authorSvalheim, Trygve Leithe
dc.creator.authorWehus, Ingunn Kathrine
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextpostprint
cristin.qualitycode1
dc.identifier.cristin2123278
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Proceedings of SPIE, the International Society for Optical Engineering&rft.volume=12188&rft.spage=&rft.date=2022
dc.identifier.jtitleProceedings of SPIE, the International Society for Optical Engineering
dc.identifier.volume12188
dc.identifier.pagecount13
dc.identifier.doihttps://doi.org/10.1117/12.2629515
dc.subject.nviVDP::Astrofysikk, astronomi: 438
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0277-786X
dc.type.versionAcceptedVersion
cristin.articleid121882C


Files in this item

Appears in the following Collection

Hide metadata