Sunrise iii: The Wavefront Correction System

Abstract This paper describes the wave-front correction and image stabilisation system (CWS) developed for the Sunrise iii balloon-borne telescope, and provides information about its performance as measured during the integration into the telescope and during the 2024 science flight. The fast image stabilisation is done by a correlation tracker (CT) and a fast tip-tilt mirror, low order aberrations such as defocus and coma are measured by a six-element Shack-Hartmann wavefront sensor (WFS) and corrected by an active telescope secondary mirror for automated focus and manual coma correction. The CWS is specified to deliver a stabilised image with a precision of 0.005 arcsec (rms). The autofocus adjustment is specified to maintain a focus stability of 0.01 waves in the focal plane of the CWS.

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Publication Details

Journal
Solar Physics
Published
2026-04-01
DOI
https://doi.org/10.1007/s11207-026-02649-7
Primary Topic
Adaptive optics and wavefront sensing
Type
article
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article

Sunrise iii: The Wavefront Correction System

A. Álvarez‐Herrero, D. Orozco Suárez, Tobias Preis, Thomas Sonner et al.
Solar Physics
Adaptive optics and wavefront sensing
article

Sunrise iii: The Wavefront Correction System

A. Álvarez‐Herrero, D. Orozco Suárez, Tobias Preis, Thomas Sonner, T. L. Riethmüller, A. Lagg, F. Heidecke, Masahito Kubo, Thomas Berkefeld, P. N. Bernasconi, Yukio Katsukawa, H. N. Smitha, B. Grauf, E. Nakai, A. Gandorfer, A. Feller, Jose Carlos del Toro Iniesta, Sami K. Solanki, Reiner Volkmer, Valentin Martinez Pillet, Alexander Bell, Michael Carpenter
article en

Abstract

Abstract This paper describes the wave-front correction and image stabilisation system (CWS) developed for the Sunrise iii balloon-borne telescope, and provides information about its performance as measured during the integration into the telescope and during the 2024 science flight. The fast image stabilisation is done by a correlation tracker (CT) and a fast tip-tilt mirror, low order aberrations such as defocus and coma are measured by a six-element Shack-Hartmann wavefront sensor (WFS) and corrected by an active telescope secondary mirror for automated focus and manual coma correction. The CWS is specified to deliver a stabilised image with a precision of 0.005 arcsec (rms). The autofocus adjustment is specified to maintain a focus stability of 0.01 waves in the focal plane of the CWS.

Solar PhysicsVol. 301(4)
The Graduate University for Advanced Studies, SOKENDAI (JP), Institut für Sonnenphysik (DE), Swedish Space Corporation (SE), Johns Hopkins University Applied Physics Laboratory (US), Max Planck Institute for Solar System Research (DE), Instituto Nacional de Técnica Aeroespacial (ES), Instituto de Astrofísica de Canarias (ES), Instituto de Astrofísica de Andalucía (ES), National Astronomical Observatory of Japan (JP), The University of Tokyo (JP)
Openalex Percentile: Top 20%
Adaptive optics and wavefront sensing
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