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Long-distance remote comparison of ultrastable optical frequencies with 10−15 instability in fractions of a second

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Abstract

We demonstrate a fully optical, long-distance remote comparison of independent ultrastable optical frequencies reaching a short term stability that is superior to any reported remote comparison of optical frequencies. We use two ultrastable lasers, which are separated by a geographical distance of more than 50 km, and compare them via a 73 km long phase-stabilized fiber in a commercial telecommunication network. The remote characterization spans more than one optical octave and reaches a fractional frequency instability between the independent ultrastable laser systems of 3 × 10−15 in 0.1 s. The achieved performance at 100 ms represents an improvement by one order of magnitude to any previously reported remote comparison of optical frequencies and enables future remote dissemination of the stability of 100 mHz linewidth lasers within seconds.

©2010 Optical Society of America

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Figures (4)

Fig. 1
Fig. 1 Schematic setup. EDFA: bi-directional erbium doped fiber amplifier, AOM: acousto-optic modulator, OC: optical circulator, FM: Faraday mirror, PD: photodiode, ϕ-Det: phase detector, VCO: voltage-controlled oscillator.
Fig. 2
Fig. 2 Fractional Allan deviation of the beat frequency between ultrastable laser systems in more than 50 km distant laboratories. L1-L2 local measurement, L1-TL and L2-TL via a 73 km stabilized fiber link; TL: transfer laser at 1542 nm. With (filled symbols) and without (open symbols) removal of linear drifts. Also shown, estimated instability of 73 km link from independent round-trip link measurements.
Fig. 3
Fig. 3 High resolution remote optical frequency comparison L2-TL using the modified Allan deviation (ModADEV) and estimated instability of 73 km link from independent round-trip link measurements. Also shown, stability of ML-YL local comparison at PTB via 300 m of stabilized fiber [20].
Fig. 4
Fig. 4 Power spectrum of the remote transfer beat note between 73 km distant L2 and TL at 48.5 THz.

Equations (1)

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ν 2 m 2 m 1 ν 1 = ( 2 m 2 m 1 ) ν CEO m 2 m 1 ν B 1 + ν B 2 ,
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