Draw the Fabry–Pérot etalon with parallel mirrors and an incident beam making internal angle with their normal. Every emerging transmitted contribution has undergone one more internal round trip than its predecessor.
Figure 1.
Successive transmitted paths and a common outgoing wavefront for a tilted beam in an air-gap etalon
. Details.
The extra internal path is , but successive contributions leave at laterally separated points, a distance apart. Comparing their phases on the same outgoing wavefront subtracts the path projection . Their net optical path difference in air is
Hence, in the reflection-phase convention implicit in the supplied transmission formula,
For a gap of refractive index , replace by and use the vacuum wavelength. Coating reflection phases can add a round-trip offset; the expression above assumes that offset is absorbed in the resonance order, or is zero modulo as in the stated ideal model.
Write , keeping this coefficient distinct from the finesse . The transmission has maxima at . At a displacement from a maximum, its ratio to peak transmission is . Half maximum therefore requires
This is the half-width in wave phase; the full width at half maximum is . Successive resonances are apart, so the exact ideal-model result is
For narrow peaks, , the small-angle approximation to the inverse sine gives
Thus the formula requested in the paper is the high-reflectivity approximation, not an exact identity at arbitrary . Ordinary half-maximum peaks exist only when , or ; below that threshold the transmission minimum never reaches half the peak. The prefactor cancels from this relative-width calculation.
Let , and . Requiring the separation to be at least times the measured full width at half maximum means a width no larger than , or a resolving power of approximately .
The etalon resolving power and order overlap constraints are particularly clear in frequency. Put . At normal incidence, the free spectral range is and the instrumental width is . Thus
Avoiding ambiguity between the doublet and adjacent interference orders requires a free spectral range exceeding the doublet separation:
Together these give
Using the narrow-peak finesse from the previous part, gives , with a practical margin above that limiting value. At the exact limit, the gap between orders vanishes, so equality is not a sensible operating point.
One feasible ideal design is , , and . It has an approximate wavelength free spectral range of and instrumental width near the doublet. The doublet spacing is about widths. Even the spacing to the nearest replica of the other line exceeds widths in this example. If that latter separation is also required in general, impose the stronger condition , rather than just the two basic inequalities.
Such mirror reflectivities and submillimetre gaps are plausible for a high-quality Fabry–Pérot etalon. Flatness, parallelism, coating loss, angular spread, mechanical stability and source width limit the achieved finesse. A wavelength width of corresponds to a gap variation of order , so the ideal coating-limited estimate demands stringent uniformity. The paper expressly excludes intrinsic source broadening.
Figure 1.
Calculated etalon transmission comb and a scanned doublet spectrum for an illustrative design meeting the width and order constraints
. Details.
The first panel is the fixed etalon's transmission versus wavelength, a comb of resonances. It does not by itself have one peak at each sodium line. The second panel shows the two peaks obtained by scanning the etalon phase or gap and calibrating the scan to wavelength. A fixed-gap output spectrum is instead the incident spectrum multiplied by the transmission function. This distinction is needed to interpret a doublet measurement correctly.
A high-finesse Fabry–Pérot etalon obtains very narrow transmission peaks by summing many coherent round trips, allowing high resolving power with a compact optical path. It can transmit a substantial fraction of resonant light when coating absorption is small, and works well for precise relative line separations and narrow-line measurements. A diffraction grating may require many illuminated grooves to achieve the same resolving power.
The etalon's free spectral range is limited, and repeated orders cause ambiguity across a broad optical spectrum. It commonly needs scanning and an order-selecting optical filter or another dispersive element. Mirror alignment, flatness and illumination angle strongly affect peak positions and widths, and absorption lowers throughput. A diffraction grating instead separates a broad range of wavelengths spatially for simultaneous detection, although grating orders can also overlap. The preferred instrument depends on whether narrow-band precision or broad spectral coverage is the priority.

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