Development of Fast and Precise Scan Mirror Mechanism for an Airborne Solar Telescope
Takayoshi Oba, Toshifumi Shimizu, Yukio Katsukawa, Masahito Kubo,, Yusuke Kawabata, Hirohisa Hara, Fumihiro Uraguchi, Toshihiro Tsuzuki,, Tomonori Tamura, Kazuya Shinoda, Kazuhide Kodeki, Kazuhiko Fukushima, Jos\'e, Miguel Morales Fern\'andez, Antonio S\'anchez G\'omez

TL;DR
This paper presents a newly developed scan mirror mechanism (SMM) for airborne solar telescopes that offers rapid, precise, and stable imaging capabilities, enabling advanced solar observations with high accuracy and speed.
Contribution
The paper introduces a novel SMM with a closed-loop control system, achieving high linearity, stability, and speed, suitable for precise solar spectroscopic measurements.
Findings
Achieved 0.08% scan-step linearity across ±1005 arcsec
Demonstrated high stability with 0.1 arcsec precision
Achieved fast stepping speed of 26 ms
Abstract
We developed a scan mirror mechanism (SMM) that enable a slit-based spectrometer or spectropolarimeter to precisely and quickly map an astronomical object. The SMM, designed to be installed in the optical path preceding the entrance slit, tilts a folding mirror and then moves the reflected image laterally on the slit plane, thereby feeding a different one-dimensional image to be dispersed by the spectroscopic equipment. In general, the SMM is required to scan quickly and broadly while precisely placing the slit position across the field-of-view (FOV). These performances are highly in demand for near-future observations, such as studies on the magnetohydrodynamics of the photosphere and the chromosphere. Our SMM implements a closed-loop control system by installing electromagnetic actuators and gap-based capacitance sensors. Our optical test measurements confirmed that the SMM fulfils…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Adaptive optics and wavefront sensing · Astronomical Observations and Instrumentation
