Optical interferometers sharpen views of the sky

Science ◽  
2018 ◽  
Vol 361 (6397) ◽  
pp. 12-13
Author(s):  
Adam Mann
1995 ◽  
Author(s):  
Fabrizio Barone ◽  
Enrico Calloni ◽  
Luciano DiFiore ◽  
Aniello Grado ◽  
Leopoldo Milano ◽  
...  

1997 ◽  
Vol 36 (28) ◽  
pp. 7162 ◽  
Author(s):  
Timothy B. Carlson ◽  
Steven M. Denzer ◽  
Thomas R. Greenlee ◽  
Robert P. Groschen ◽  
Richard W. Peterson ◽  
...  

1994 ◽  
Vol 33 (34) ◽  
pp. 7846 ◽  
Author(s):  
Fabrizio Barone ◽  
Rosario De Rosa ◽  
Luciano Di Fiore ◽  
Francesco Fusco ◽  
Aniello Grado ◽  
...  

2018 ◽  
Vol 85 (11) ◽  
pp. 680-690
Author(s):  
Yinan Li ◽  
Markus Kästner ◽  
Eduard Reithmeier

Abstract Optical interferometers as non-contact measurement devices are very desirable for the measurement of surface roughness and topography. Compared to phase shifting interferometers (PSIs) with a limited measurement range and a scan step of maximum λ/4, the optical interferometers like low coherence interferometers (LCIs) evaluating the degree of fringe coherence allow a larger vertical measurement range. Their vertical measurement range is only limited by the scan length allowed by the linear piezo stage and the coherence length of the light source. To evaluate the obtained data for a large range, the common LCIs require much computation time. To overcome this drawback, we present an evaluation algorithm based on the Hilbert-Transform and curve fitting (Levenberg–Marquardt algorithm) using Compute Unified Device Architecture (CUDA) technology, which allows parallel and independent data evaluation on General Purpose Graphics Processing Unit (GPGPU). Firstly, the evaluation algorithm is implemented and tested on an in-house developed LCI, which is based on Michelson configurations. Furthermore, we focus on the performance optimization of the GPU-based program using the different approaches to further achieve efficient and accurate massive parallel computing. Finally, the performance comparison for evaluating measurement data using different approaches is discussed in this paper.


1989 ◽  
Vol 8 ◽  
pp. 559-560
Author(s):  
S.T. Ridgway

During the last three years significant results have been obtained from several operational, long baseline optical interferometers. Precision stellar angular diameters (accuracy of order 2% and better) have been reported in the infrared (DiBenedetto and Rabbia, 1987) and in the visible (Davis and Tango, 1986). Astrometric precision of order 20 milliarcsec has been demonstrated over large angles (Shao et al, in press). Spectro-spatial resolution of the disk of a Be star in the hydrogen emission line (Thom et al., 1986) suggests spectacular imaging science to come with many-telescope coherent and phased optical arrays.


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