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Fabry-Perot Interferometer Finesse & FSR Calculator

A Fabry-Perot interferometer consists of two parallel partially reflective mirrors forming an optical resonant cavity.

Power reflectance of the cavity mirrors (0.01 - 0.999).

Physical spacing between mirrors.

Nominal operating laser wavelength.

Refractive index inside cavity (air = 1.0).

Calculated Result
77.0

Cavity Finesse (F)

Free Spectral Range (Freq)

9.99 GHz

Free Spectral Range (Wl)

80.08 pm

Resonance Linewidth (FWHM)

129.86 MHz

Optical Q-Factor

1.49e+6

Calculation Breakdown

  1. Finesse FormulaF = π·√R / (1 - R) = π·√0.96 / (1 - 0.96) = 77.0
  2. Free Spectral RangeFSR = c / (2·n·d) = 3e8 / (2·1·15mm) = 9.99 GHz

What Is the Fabry-Perot Interferometer Finesse & FSR Calculator?

A Fabry-Perot interferometer (or etalon) is an optical resonant cavity formed by two parallel reflecting surfaces.

How Does the Fabry-Perot Interferometer Finesse & FSR Calculator Work?

Multiple reflections interfere constructively only at integer multiples of half-wavelengths, producing sharp transmission fringes.

Fabry-Perot Interferometer Finesse & FSR Calculator Formula & Variables

The core mathematical equation utilized by this calculator is expressed as:

mathcal{F} = rac{pi sqrt{R}}{1 - R}, quad ext{FSR}_ u = rac{c}{2 n d}, quad Delta u = rac{ ext{FSR}}{mathcal{F}}

Reflective finesse and cavity free spectral range frequency spacing.

How to Use the Fabry-Perot Interferometer Finesse & FSR Calculator

  1. Input mirror power reflectivity R, cavity spacing d, and laser wavelength.

Step-by-Step Example Calculation

Laser Spectroscopy Etalon

Input Values:

mirrorReflectivity:0.96
cavityLengthMm:15
centerWavelengthNm:1550
refractiveIndexMedium:1
Worked Steps: Yields Finesse = 76.9, FSR = 10.00 GHz (80.1 pm), and narrow resonance linewidth of 130.0 MHz.

Understanding Your Result

FSR is the frequency span between successive transmission peaks; finesse measures peak sharpness.

Factors That Affect the Result

  • Mirror surface flatness imperfections, absorption losses, and mirror tilt reduce effective finesse.

When Should You Use This Calculator?

  • Laser wavelength meter calibration, optical spectrum analyzers, tunable telecom filters, and gravitational wave detectors.

Assumptions & Limitations

  • Assumes perfectly parallel, lossless mirrors and planar monochromatic wave incidence.

Frequently Asked Questions

Calculation Accuracy & Reference Note

Standard Airy transmission distribution formulation.

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