Solution

ID: past-exam-of-the-physics-of-atmospheres-and-oceans-course-of-the-university-of-oxford/2022/4/a/solution

A Michelson interferometer uses a beam splitter to divide collimated input light between a fixed mirror and a moving mirror. Returning beams recombine at the beam splitter; one output reaches a photodetector. A compensator plate can equalize the glass traversed in the two arms. Moving one mirror by changes the optical path difference by .
The usual nominal Fourier transform spectroscopy specification is , where is the maximum optical path difference measured from equal arms. It gives
This is a nominal spectral resolution element convention.[ref] A symmetric rectangular scan from to instead has a sinc instrumental line shape with first-zero offset . Quoting that first-zero criterion would give cm; interferogram apodization and other linewidth criteria change the numerical factor. An exact mathematical minimum requires such a criterion.
In the measurement chain, the Michelson interferometer is the spectral analyzer or modulator, between the collection optics and the photodetector. It encodes the incoming radiation spectrum into an interferogram; detector electronics digitize that signal and a Fourier transform reconstructs the radiation spectrum. It does not itself turn radiant power into an electrical signal.

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