Image Instabilities and Polarization Crosstalk

We expand on our previous study of the impact of atmospheric seeing on polarization crosstalk, and show how the formalism that was developed in that work can be applied to treat the case of spatial modulators of polarization. Beside formally demonstrating how the problem of crosstalk is fully elimin...

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Main Authors: R. Casini, A. G. de Wijn
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adc68b
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author R. Casini
A. G. de Wijn
author_facet R. Casini
A. G. de Wijn
author_sort R. Casini
collection DOAJ
description We expand on our previous study of the impact of atmospheric seeing on polarization crosstalk, and show how the formalism that was developed in that work can be applied to treat the case of spatial modulators of polarization. Beside formally demonstrating how the problem of crosstalk is fully eliminated in such devices, we also gain insight on the meaning of polarimetric noise of temporal modulation schemes in the limit of very high modulation frequency. We also describe the problem of spectrograph instabilities, and how the spectral gradients that are naturally associated with a line spectrum feed into the problem of polarimetric errors induced by mechanical vibrations, thermal drifts, and pointing jitter. Finally, we show how this formalism can be used to estimate the contribution of polarization crosstalk to the errors on the elements of the 4 × 4 Stokes response matrix, for the purpose of producing realistic error budgets for polarimetric instrumentation.
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spelling doaj-art-ed4d6397b4264105a4e3506c0766bfda2025-08-20T01:55:38ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01985216710.3847/1538-4357/adc68bImage Instabilities and Polarization CrosstalkR. Casini0https://orcid.org/0000-0001-6990-513XA. G. de Wijn1https://orcid.org/0000-0002-5084-4661HAO , NSF NCAR, P.O. Box 3000, Boulder, CO 80307-3000, USAHAO , NSF NCAR, P.O. Box 3000, Boulder, CO 80307-3000, USAWe expand on our previous study of the impact of atmospheric seeing on polarization crosstalk, and show how the formalism that was developed in that work can be applied to treat the case of spatial modulators of polarization. Beside formally demonstrating how the problem of crosstalk is fully eliminated in such devices, we also gain insight on the meaning of polarimetric noise of temporal modulation schemes in the limit of very high modulation frequency. We also describe the problem of spectrograph instabilities, and how the spectral gradients that are naturally associated with a line spectrum feed into the problem of polarimetric errors induced by mechanical vibrations, thermal drifts, and pointing jitter. Finally, we show how this formalism can be used to estimate the contribution of polarization crosstalk to the errors on the elements of the 4 × 4 Stokes response matrix, for the purpose of producing realistic error budgets for polarimetric instrumentation.https://doi.org/10.3847/1538-4357/adc68bSpectropolarimetry
spellingShingle R. Casini
A. G. de Wijn
Image Instabilities and Polarization Crosstalk
The Astrophysical Journal
Spectropolarimetry
title Image Instabilities and Polarization Crosstalk
title_full Image Instabilities and Polarization Crosstalk
title_fullStr Image Instabilities and Polarization Crosstalk
title_full_unstemmed Image Instabilities and Polarization Crosstalk
title_short Image Instabilities and Polarization Crosstalk
title_sort image instabilities and polarization crosstalk
topic Spectropolarimetry
url https://doi.org/10.3847/1538-4357/adc68b
work_keys_str_mv AT rcasini imageinstabilitiesandpolarizationcrosstalk
AT agdewijn imageinstabilitiesandpolarizationcrosstalk