Astrophysics (Index)About

speckle imaging

(method of combining short-term images to yield better resolution)

Speckle imaging indicates use of techniques maximize the resolution of a telescope's images in the face of atmospheric distortion from seeing issues (a type of speckle). A speckle imager is an imager (camera) designed for such imaging.

A basic method uses numerous images are taken at relatively short exposures and uses image processing to produce a more detailed image likely to match what the image would be without the distortion. A straightforward process called shift-and-add aka image stacking can be used, or a type of interferometry called speckle masking. Lucky imaging is a variant.


(telescopes,optics,method)
Further reading:
https://en.wikipedia.org/wiki/Speckle_imaging
https://en.wikipedia.org/wiki/Lucky_imaging
https://physicstoday.scitation.org/doi/10.1063/PT.3.4077
https://archive.ll.mit.edu/publications/journal/pdf/vol02_no2/2.2.4.speckleimaging.pdf
http://www2.lowell.edu/workshops/speckle2014/presentations/03-01%20horch_lsw1.pptx.pdf
https://noirlab.edu/public/programs/kitt-peak-national-observatory/wiyn-35m-telescope/nessi/

Referenced by page:
WIYN 3.5m Telescope

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