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- W2093028305 abstract "Abstract A method is described for estimating the rms phase variation due to atmospheric turbulence using a stellar light source and an astronomical telescope. It consists of measuring the angular chromatic dispersion of the speckles in the stellar image. A knowledge of the rms phase variation is required in adaptive optics and in choosing the optimum spectral bandwidth in stellar speckle interferometry. Some preliminary results are given." @default.
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- W2093028305 date "1977-04-01" @default.
- W2093028305 modified "2023-09-24" @default.
- W2093028305 title "A simple method of estimating the rms phase variation due to atmospheric turbulence" @default.
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- W2093028305 doi "https://doi.org/10.1016/0030-4018(77)90076-1" @default.
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