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evidence as to the accuracies currently obtained. Each
of the numerous laboratories now making MTF measurements
can probably repeat their data on any one lens with sat
isfactory precision, and so long as they continue to test
lenses of the same type the results will indicate the
relative qualities of the lenses in an adequate way. Thus
the requirements of production control can be satisfied.
But if measurements are made on the same lens in another
laboratory, probably using a basically different apparatus,
the results may differ widely. Also, if any laboratory
tests lenses of very different types, e.g, changes from
very large aperture to very small aperture lenses, there is
no guarantee that the results will correspond to a measure
ment of the true MTF in each case. In fact, the test des
cribed in Appendix I revealed discrepancies as great as
- at quite low spatial frequencies when one lens was
measured by several laboratories, each of which estimated
its accuracy as 3% or better.
It is unfortunately true that so far no satisfactory
techniques have been developed for the complete proving and
qualification of MTF apparatus over the whole range of con
ditions in which it is likely to be used. It is not easy to
devise suitable checks and calibrations for this purpose.
Diffraction limited lenses can be used, but this is restr
icted to small apertures and monochromatic light. Another
possibility is the design and very careful construction of a
simple (e.g, plano-convex) lens, whose MTF could be calculated
and for which all the aberrations would be very accurately
known. Within the measuring apparatus itself much can be done
to isolate sources of error. The shape and modulation of
sinusoidal masks, their scattering characteristics, uniformity
of illumination over masks, slits, and photocell apertures,
all require careful checking. The linearity of amplifiers
and recorders is another possible source of error. The
spectral response of the photocell detector should be measured
rather than assumed from representative data. In techniques
that enlarge the spread function with a microscope objective,
the abberrations of the objective, and their combination
with the aberrations of the lens being tested require examin
ation. Similar remarks apply to collimators and folding mirrors.
Problems of vibration and air turbulence are more serious than
in the less sensitive resolving power measurement. Problems
associated with the coherence of the illumination have not
received enough attention.
Overall, the aim is to ensure that each technique
genuinely measures the OTF and MTF. Unless this is achieved
different laboratories will not agree, however, consistent
each of them may be, and reliable standard data for lenses
will not become available to the prospective purchaser.