The intensity distributions have been computed in the dark-field images of coherently illuminated objects with periodically varying transmission. To get this dark field an obstacle is placed centrally in the back focal plane of the imaging system and the image so formed is called the diffrimoscopic image. The image is characterized by the appearance of a dark fringe at the geometric image of the edges of the object. The effect of the width of the obstacle and the aperture of the imaging system on image intensity distribution have been studied. It has been shown that the dark fringes appear exactly at the geometric image of the edges separating the light and dark regions of a rectangular wave object. The width of the dark fringe is inversely proportional to the aperture width. The position and the width of the dark fringe are independent of the width of the obstacle which affects mainly the intensity away from the dark fringe.
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