Spectro-polarimeters in solar astronomy usually require splitting different wavebands into separate monochromatic arms that operate as independent sub-instruments. We demonstrate a concept for a polarimeter that operates at two wavebands simultaneously, using a single channel of optical components and a single detector. By using chromatic zero-order waveplates, polarized light propagates differently through the instrument depending on its wavelength, allowing to measure the polarization in both wavebands simultaneously. We present Stokes vectors measurements with ∼ 1% relative error using standard off-the-shelf components, thus demonstrating the relevance of this concept for fields like solar astronomy and space instrumentation.
No takes yet. Share an insight, caveat, or question.
Huber et al. (2024) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: