Abstract
Speckle images have been formed in the optical laboratory with a linear pupil (its length was 10 times its width) viewing through a fluctuating medium which introduced severe seeing. The images were recorded with a microprocessor-controlled CCD-camera system interfaced to a minicomputer. By slightly modifying several established processing techniques and combining them into a new synthesis procedure, faithful versions of diffraction-limited true images of simulated astronomical objects are reconstructed from sequences of speckle images.
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© 1982 Springer-Verlag Berlin Heidelberg
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Böhme, S. et al. (1982). Astronomical Instruments and Techniques. In: Böhme, S., et al. Astronomy and Astrophysics Abstracts. Astronomy and Astrophysics Abstracts, vol 31. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-12334-8_6
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DOI: https://doi.org/10.1007/978-3-662-12334-8_6
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-662-12336-2
Online ISBN: 978-3-662-12334-8
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