Static spectropolarimeter concept adapted to space conditions and wide spectrum constraints
Martin Pertenais, Coralie Neiner, Pernelle Bernardi, Jean-Michel Reess, and Pascal Petit

TL;DR
This paper introduces a static, wide-spectrum spectropolarimeter concept suitable for space applications, utilizing birefringent wedges for spatial polarization modulation, enabling single-shot full-Stokes measurements across UV to millimeter wavelengths.
Contribution
The paper presents an innovative static spectropolarimeter design that replaces temporal modulation with spatial modulation using birefringent wedges, suitable for space conditions and broad spectral ranges.
Findings
Theoretical modeling and simulations support the concept.
Laboratory validation confirms feasibility.
Application to the Arago mission demonstrates practical potential.
Abstract
The issues related to moving elements in space and instruments working in broader wavelength ranges lead to a need for robust polarimeters, efficient on a wide spectral domain, and adapted to space conditions. As part of the UVMag consortium, created to develop spectropolarimetric UV facilities in space, such as the Arago mission project, we present an innovative concept of static spectropolarimetry. We studied a static and polychromatic method for spectropolarimetry, applicable to stellar physics. Instead of modulating the polarization information temporally, as usually done in spectropolarimeters, the modulation is performed in a spatial direction, orthogonal to the spectral one. Thanks to the proportionality between phase retardance imposed by a birefringent material and its thickness, birefringent wedges can be used to create this spatial modulation. The light is then spectrally…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
