论文信息 - First astronomical application of postdetection turbulence compensation: images of alpha Aurigae, nu Ursae Majoris, and alpha Geminorum using self-referenced speckle holography. - 字舞流文

First astronomical application of postdetection turbulence compensation: images of alpha Aurigae, nu Ursae Majoris, and alpha Geminorum using self-referenced speckle holography.

We describe a postdetection turbulence compensation technique for obtaining high resolution imagery through the atmosphere. We present preliminary results fromfield experiments.

D G Voelz | J D Gonglewski | D. Voelz | J. Gonglewski | D. Dayton | B. Spielbusch | J. Fender | R. Pierson | J S Fender | D C Dayton | B K Spielbusch | R E Pierson

[1] B. McGlamery. Restoration of Turbulence-Degraded Images* , 1967 .

[2] G. Weigelt,et al. Speckle holography measurements of the stars Zeta Cancri and ADS 3358. , 1978, Applied optics.

[3] J. C. Dainty,et al. Stellar Speckle Interferometry , 1976 .

[4] J. Hardy,et al. Real-time atmospheric compensation , 1977 .

[5] R. Bates,et al. Speckle Interferometry Gives Holograms of Multiple Star Systems , 1973 .

[6] A. Labeyrie. Attainment of diffraction limited resolution in large telescopes by Fourier analysing speckle patterns in star images , 1970 .

[7] K. Knox,et al. Recovery of Images from Atmospherically Degraded Short-Exposure Photographs , 1974 .

[8] J. Fontanella. Wavefront sensing deconvolution and adaptive optics , 1985 .

[9] Horace W. Babcock,et al. THE POSSIBILITY OF COMPENSATING ASTRONOMICAL SEEING , 1953 .

[10] A. Lohmann,et al. High resolution image formation through the turbulent atmosphere , 1973 .

[11] David L. Fried,et al. Statistics of a Geometric Representation of Wavefront Distortion: Errata , 1965 .