The phase problem solving by the use of optical correlation algorithm for reconstructing phase skeleton of complex optical fields

Author(s):  
C. Y. Zenkova ◽  
M. P. Gorsky ◽  
P. A. Ryabyi
2014 ◽  
Vol 22 (5) ◽  
pp. 6186 ◽  
Author(s):  
O. V. Angelsky ◽  
M. P. Gorsky ◽  
S. G. Hanson ◽  
V. P. Lukin ◽  
I. I. Mokhun ◽  
...  

1993 ◽  
Vol 18 (2) ◽  
pp. 90 ◽  
Author(s):  
O. V. Angelsky ◽  
P. P. Maksimyak ◽  
T. O. Perun

1995 ◽  
Vol 167 ◽  
pp. 221-229 ◽  
Author(s):  
Didier Queloz

The measurement of some physical parameters of astronomical objects can only be carried out with high resolution spectra. Unfortunately the high dispersion of the light on the detector restricts such observations to relatively bright sources. However, some spectral information can be concentrated into a single spectral “line” by a cross-correlation algorithm, allowing the observation of fainter objects. Such a technique, taken from the CORAVEL optical correlation, is presented. A complete description of the errors of the correlation function parameters is given and the minimum signal-to-noise ratio is also discussed. Finally, a short investigation of the best resolution needed to observe efficiently radial velocities and velocity broadenings is made.


1991 ◽  
Vol 55 (5) ◽  
pp. 327-331 ◽  
Author(s):  
GT Chiodo ◽  
WW Bullock ◽  
HR Creamer ◽  
DI Rosenstein
Keyword(s):  

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