Abstract
The design considerations that are necessary to optimize the performance of a
tilting-filter photometer are presented. Such a photometer is described, and
some typical measurements of aurora and airglow illustrate the application of
this technique to low light level spectrophotometry. The digital approach used
with photomultipliers at these low light levels is also discussed. Comparison of
the tilting-filter photometer with other spectral scanning instruments reveals a
superiority for many applications. A final section discusses possible space
applications.
© 1969 Optical Society of America
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