The optical ruler has two coordinates
The spacing alone leaves the starting point of the ruler unknown.
L18 · Calibrate the optical ruler
What must you measure before a frequency comb can work as a ruler for light? The tooth spacing and their common offset. The spacing equals the pulse repetition rate. Doubling a low-frequency tooth and beating it against the tooth with twice its index isolates the offset. An unknown laser also needs an identified tooth and the sign of its beat relative to that tooth.
Count repetition and offset signals, then reconstruct a target frequency. Compare missing overlap, a short record and an ambiguous tooth index.
Physics tutorial
BackgroundA regular train of pulses contains a comb of equally spaced optical frequencies. Knowing the spacing does not tell you where the comb starts.
Why it mattersTo use the comb as a ruler for light, you need the repetition frequency, the carrier-envelope offset (CEO) frequency and the integer index of the tooth you are using.
Start with the essentials
The spacing alone leaves the starting point of the ruler unknown.
Each pulse envelope repeats the last one, but the carrier under it can shift forward in phase.
Both original teeth must lie inside the comb's spectrum. The frequency doubling is treated as ideal.
The counter interpolates the upward zero crossings. If the record is too short, the frequency is reported as unresolved.
Here the beat and its sign are given as an ideal input. Because the tooth index is large, a small counting error in the repetition frequency becomes a large optical frequency error.
The pulse snapshots use the exact finite sum. The pulse-width readout uses the continuum limit for many teeth.
Typical misconceptionKnowing the tooth spacing is enough to know every optical frequency.
Better mental modelThe whole comb can slide without changing its spacing. The CEO frequency tells you how far it has slid.
Typical misconceptionThe size of the beat frequency tells you which side of the tooth the target is on.
Better mental modelA photodiode gives the same beat for a target the same distance above or below the tooth. This ideal model supplies the sign; a real instrument needs an extra discriminator to find it.
Select Half-cycle phase slip and compare the three pulse snapshots.
What to observe: The envelopes repeat, but the carrier flips sign from one pulse to the next.Compare the loaded Supported self-reference record with Missing octave.
What to observe: Unless a tooth and its doubled-index partner both lie in the spectrum, no CEO beat is recorded.Read the default counted RF values, then choose Record too short. Use Acquire RF record to repeat the acquisition.
What to observe: With too few zero crossings, the offset cannot be resolved.Try Ambiguous tooth index, then reduce the Coarse prior half-width.
What to observe: A precise RF beat alone does not tell you which optical tooth the target is next to.Probes and measurement · Reading path
Articles on this path that use this experiment, followed by the other experiments they suggest.