Full text: Reports and invited papers (Part 3)

    
   
   
    
    
   
   
   
   
   
  
  
    
   
   
  
  
   
   
   
  
   
   
   
  
  
   
  
    
The output is independent of the partial coherence of the 
source; 
There are fewer focusing and alignment problems; 
Because there is no sampling slit, the overall system 
transfer function is improved; 
The measurement of singly diffuse density makes interlabora- 
tory comparison easier. 
5.9.2.2 Interferometric Methods: 
Interferometric testing essentially measures the pupil 
function from which the optical transfer function, the spread function, 
and aberration coefficients may be computed. The pupil function 
must be used to evaluate cascaded optical systems and systems employing 
coherent or partially coherent illumination. 
Most quantitative interferometric testing systems are expensive, 
time-consuming, and require operational expertise. The application 
of the Wavefront Shearing Interferometer (WSI) developed at the 
U. S. Bureau of Standards?2 eliminates some of these undesirable 
features, employing an interferometric cube into which the adjustments 
are fixed. The WSI into which the cube is installed is portable 
and easily set up on an optical bench. 
The resulting inteferograms, however, cannot be interpreted 
by simple inspection in terms of wavefront aberrations. Hence the 
major cost of testing goes into data reduction and analysis. 
The cube interferometer operates by amplitude dividing the 
incoming wavefront into two equal parts and introducing a small 
angular shear into one of the beams. For two 45? -90? -45? prisms 
contacted along the diagonals to form a cube, the pivot point of 
rotation lies in the plane of the back face of the cube. A small 
shear is then introduced. 
As the cube is not used in parallel light, corrections 
are made for the known aberrations which are introduced by the 
optical path differences. 
Working with photographic transparencies of the interfero- 
grams, the test data is supplied in fringe-peak locations. The 
technique of autoconvolving the fringe density profile in the vicinity 
of a maximum or minimum was used to locate the fringe-peaks. (Peak 
of the autoconvolution function corresponds to the fringe-peak.) 
This method has the advantage of averaging grain noise effects during 
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