Abstract
An image stabilizer has been inserted into the optical path of the THEMIS solar telescope. THEMIS is a Ritchey–Chretien reflector telescope using an altazimuthal mount and closely tied to its spectrograph. The optical and mechanical design, implementation and system tests are described, and emphasis is put on the complexity of situations that this stabilizer must accept, including the scanning of the solar surface while stabilizing. The current closed-loop crossover frequency of the device is 65 Hz at − 3 dB on all typical solar scenes.
Similar content being viewed by others
References
Hill, F., Beckers, J., Brandt, P., Briggs, J., Brown, T., Brown, W., Collados, M., Denker, C., Fletcher, S., Hegwer, S., Horst, T., Komsa, M., Kuhn, J., Lecinski, A., Lin, H., Oncley, S., Penn, M., Radick, R., Rimmele, T., Socas-Navarro, H., Streander, K.: In: Stepp, L.M. (ed.) Ground-based and Airborne Telescopes. Proceedings of the SPIE, vol. 6267, 62671T (2006)
Aulanier, G., Gigan, P., Malherbe, J.-M., Molodij, G.: Projet de stabilisation d’image pour le télescope THEMIS. Report to the THEMIS Scientific Advisory Council (2003)
Ballesteros Ramirez, E.: Estabilizador bidimensional optimizado para imágenes solares. Ph.D. Thesis, U. La Laguna (1996)
Ballesteros, et al.: Two dimensional, high spatial resolution, solar spectroscopy using a correlation tracker. Astron. Astrophys. Suppl. Ser. 115, 353–365 (1996)
Cruvellier, et al.: T.A.O.: Themis adaptive optics. Report to the THEMIS Scientific Advisory Council (unpublished) (2003)
Darvan, T.A., Dunn, R.B.: Influence of seeing on measurements of horizontal flows in the solar photosphere. In: High Spatial Resolution Solar Observations, Proceedings of the 10th Sacramento Peak Summer Workshop, p. 502, Sunspot, New Mexico, August 22–26, 1988 (1989)
Edwards, C.G., Levay, M., Gilbreth, C.W., Tarbell, T.D., Title, A.M., Wolfson, C.J., Torgerson, D.D.: The correlation tracker image stabilization system for HRSO. Bull. Am. Astron. Soc. 19, 929 (1987)
Judge, P.G., Elmore, D.L., Lites, B.W., Keller, C.U., Rimmele, T.: Evaluation of seeing induced crosstalk in tip-tilt corrected solar polarimetry. Appl. Opt. 43(19), 3817–3828 (2004)
Labeyrie, A.: Attainment of diffraction limited resolution in large telescope by Fourier analysing speckle patterns in star images. Astron. Astrophys. 6, 85–87 (1970)
Knox, K.T., Thompson, B.J.: Recovery of images from atmospherically degraded short-exposure photographs. Astrophys. J. 193, L45 (1974)
Molodij, G., Rayrole, J., Madec, P.-Y., Colson, F.: Performance analysis for THEMIS image stabilizer optical system I. Astron. Astrophys. Suppl. Ser. 188, 169–179 (1996)
Rimmele, Th., Von der Lühe, O., Wiborg, P.H., Widener, A.L., Dunn, R.B., Spence, G.: Solar feature correlation tracker. In: Active and Adaptive Optical Systems. Proceedings of the Meeting, pp. 186–193. San Diego, CA, July 22–24, 1991 (A93-39451 15-74) (1991)
Ricort, G., Aime, C., Roddier, F., Borgnino, J.: Determination of Fried's parameter r 0 prediction for the r.m.s. contrast in solar granulation. Sol. Phys. 69, 223 (1981)
Von der Lühe, et al.: Solar feature correlation tracker for ground based telescopes. Astron. Astrophys. 224, 351 (1989)
Von der Lühe, O.: Speckle imaging of solar small scale structure. Astron. Astrophys. 268, 374–390 (1993)
Acknowledgements
THEMIS is operated on the Island of Tenerife by the Centre National de la Recherche Scientifique (CNRS, France), the Institut National des Sciences de l’Univers (INSU, France) and the Consiglio Nazionale delle Ricerche (CNR, Italy) in the Spanish Observatorio del Teide of the Instituto de Astrofisica de Canarias.
The authors wish to thank O. Von Der Lühe and Friedrich Vogler for making available the KISIP V speckle imaging software from the Kiepenheuer-Institut für Sonnenphysics (KIS), and for the test run on our data.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Gelly, B., Le Men, C., López Ariste, A. et al. Design and implementation of an image stabilization device at the THEMIS solar telescope. Exp Astron 22, 67–85 (2008). https://doi.org/10.1007/s10686-007-9083-4
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10686-007-9083-4