HOW I DISCOVERED PHASE CONTRAST
HOW I DISCOVERED PHASE CONTRAST
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DOI:
10.1126/science.121.3141.345
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发表时间:
1955-01-01
期刊:
影响因子:
56.9
通讯作者:
ZERNIKE, F
中科院分区:
文献类型:
--
作者:
ZERNIKE, F
P HASE CONTRAST was not discovered while I was working with a microscope, but while I was working in a different part of optics. It originated in my interest in diffraction gratings, which began about 1920. A diffraction grating consists of a plane or concave mirror with a large number of equidistant grooves ruled on its surface. Small nearly unavoidable imperfections in the location of the grooves show clearly in the optical behavior of the grating. The most conspicuous error is a periodic one that repeats itself after each revolution of the screw of the ruling engine. The regularly recurring displacement of the grooves causes corresponding changes of the optical path, just as if the mirror sur-faee were wavy. Consequently the instrument behaves as if a coarse grating, with a constant of about 2 mm, were superimposed on it, with the result that each strong spectral line is accompanied to its right and left by a number of weak spurious lines, the so-called" Rowland ghosts." These lines havea remarkable effect if one looks down at thesurface of the grating, placing the eye at the position of a spectral line. A perfect grating would in this case show an evenly illuminated surface in the color of the spectral line. In reality, however, one sees a strongly striped sur-face.At the end of a 1902 paper H. S. Allen remarked that these stripes were nothing real but were simply the effect of the interference between the principal line and its ghosts. Indeed the stripes disappear when the ghosts are covered up. I remember strongly objecting to his conclusion of unreality. On the contrary, I was convinced that the striped surface gave more information about the periodic ruling errors than that obtainable by photographing the ghosts, because in the first case, the relative phases of the ghosts come into play, whereas these are lost in the second case. I kept the question in mind, planning to look further into it as soon as an opportunity arrived. About 1930 our laboratory obtained a large con-cave gratingruled by Wood and set it up in a Runge-Paschen mounting. The striped appearance of the sur-face was soon found, but because the gratingwas 6 m from the eye, I tried pointing a small telescope at it. Then the unexpected happened. The stripes could be seen very clearly, but they disappeared when the telescope was exactly focused on the surface of the grat-ing! By a succession of experiments and calculations I soon succeeded in explaining this. On looking back to this event, I am impressed by