Development of a Precise Polarization Modulator for UV Spectropolarimetry
Shin-nosuke Ishikawa, Toshifumi Shimizu, Ryouhei Kano, Takamasa Bando,, Ryohko Ishikawa, Gabriel Giono, Saku Tsuneta, Satoshi Nakayama, Takao Tajima

TL;DR
This paper presents a newly developed polarization modulation unit (PMU) for UV spectropolarimetry, demonstrating high precision in rotating waveplates with minimal errors, suitable for solar magnetic field observations.
Contribution
The paper introduces a novel PMU with high rotation uniformity, reducing measurement errors in UV spectropolarimetry for solar magnetic field studies.
Findings
Scale error and crosstalk <0.01% due to rotation non-uniformity
PMU successfully tested for the CLASP rocket experiment
Demonstrated high performance and suitability for spectropolarimetric measurements
Abstract
We developed a polarization modulation unit (PMU) to rotate a waveplate continuously in order to observe solar magnetic fields by spectropolarimetry. The non-uniformity of the PMU rotation may cause errors in the measurement of the degree of linear polarization (scale error) and its angle (crosstalk between Stokes-Q and -U), although it does not cause an artificial linear polarization signal (spurious polarization). We rotated a waveplate with the PMU to obtain a polarization modulation curve and estimated the scale error and crosstalk caused by the rotation non-uniformity. The estimated scale error and crosstalk were <0.01 % for both. This PMU will be used as a waveplate motor for the Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP) rocket experiment. We confirmed that the PMU has the sufficient performance and function for CLASP.
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