Paper
26 October 2007 An image stabilization system for solar observations
Author Affiliations +
Abstract
An image stabilization system has been developed and demonstrated for solar observations in the visible wave-length at Udaipur Solar Observatory (USO) with a 15 cm Coudé-refractor. The softwa4re and hardware components of the system are similar to that of the low cost solar adaptive optics system developed for the 1.5 m McMath-Pierce solar telescope at Kitt Peak observatory for solar observations in the infrared. The first results presented. The system has a closed loop correction bandwidth in the range of 70 to 100 Hz. The root mean by a factor of 10 to 20. The software developes and key issues concerning optimum system performance have been addressed.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
R. Sridharan, A. Raja Bayanna, Rohan Eugene Louis, Brajesh Kumar, Shibu K. Mathew, and P. Venkatakrishnan "An image stabilization system for solar observations", Proc. SPIE 6689, Solar Physics and Space Weather Instrumentation II, 66890Z (26 October 2007); https://doi.org/10.1117/12.739844
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Cited by 1 scholarly publication.
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KEYWORDS
Adaptive optics

Telescopes

Observatories

Cameras

Calibration

Mirrors

Software development

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