Free spectral range

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Free spectral range (FSR) is the spacing in optical frequency or wavelength between two successive reflected or transmitted optical intensity maxima or minima of an interferometer or diffractive optical element.[1]

The FSR is not always represented by or , but instead is sometimes represented by just the letters FSR. The reason is that these different terms often refer to the bandwidth or linewidth of an emitted source respectively.

In general[edit]

The free spectral range (FSR) of a cavity in general is given by

where is the roundtrip length of the cavity (which is twice the physical length of the cavity), is the group index of the media within the cavity, and is the speed of light. A simple intuitive interpretation of the FSR is that it is the inverse of the roundtrip time :

In wavelength, the FSR is given by

where is the vacuum wavelength of light. For a linear cavity, such as the Fabry-Pérot discussed below, , where is the distance travelled by light in one roundtrip around the closed cavity, and is the length of the cavity.

Diffraction gratings[edit]

The free spectral range of a diffraction grating is the largest wavelength range for a given order that does not overlap the same range in an adjacent order. If the (m + 1)-th order of and m-th order of lie at the same angle, then

Fabry–Pérot interferometer[edit]

In a Fabry–Pérot interferometer or etalon, the wavelength separation between adjacent transmission peaks is called the free spectral range of the etalon and is given by

where λ0 is the central wavelength of the nearest transmission peak, n is the index of refraction of the cavity medium, is the angle of incidence, and is the thickness of the cavity. More often FSR is quoted in frequency, rather than wavelength units:

The transmission of an etalon as a function of wavelength. A high-finesse etalon (red line) shows sharper peaks and lower transmission minima than a low-finesse etalon (blue). The free spectral range is Δλ (shown above the graph).

The FSR is related to the full-width half-maximum δλ of any one transmission band by a quantity known as the finesse:

where is the coefficient of finesse, and R is the reflectivity of the mirrors.

This is commonly approximated (for R > 0.5) by


  1. ^ Eugene., Hecht,. Optics. ISBN 9780133977226. OCLC 953709783.