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| The reference cavity is locked using a 21.5Mhz signal from a rack mounted board (FSS REF - Crystal Frequency Reference [http://www.ligo.caltech.edu/docs/D/D980353-C.pdf]) | The reference cavity was locked using a 21.5 MHz signal from a rack mounted board (FSS REF - Crystal Frequency Reference http://www.ligo.caltech.edu/docs/D/D980353-C.pdf). That turned out to have many problems and we removed it completely from the system circa 2008 with a fixed 21.5 MHz OCXO from Wenzel and an RF Amplifier (see [[http://nodus.ligo.caltech.edu:8080/40m/986|elog]]). |
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| See also [[Frequency Stabilization Servo]]. | We got the design parameters for the reference cavity from [[http://www.ligo.caltech.edu/docs/D/D980670-00.pdf|D980670]] || Spacer Material || Fused Silica (Corning?) || || Mirror Material || Fused Silica || || Mirror T_HR || 300 +/- 30 ppm || || Mirror R_AR || < 500 ppm || || Mirror RoC || 500 mm || || Cavity Length || 8" (203.2 mm) || || Cavity Finesse || 10000 || || Cavity g-factor (g1*g2) || 0.352 || || Cavity waist || 0.218 mm || || Cavity FSR || 737.7 MHz || || Cavity pole || 35.2 kHz || Some FEA of the LIGO/40m reference cavity using COMSOL: [[/FEA]] ---- See also [[Frequency Stabilization Servo]]. |
The reference cavity was locked using a 21.5 MHz signal from a rack mounted board (FSS REF - Crystal Frequency Reference http://www.ligo.caltech.edu/docs/D/D980353-C.pdf). That turned out to have many problems and we removed it completely from the system circa 2008 with a fixed 21.5 MHz OCXO from Wenzel and an RF Amplifier (see elog).
We got the design parameters for the reference cavity from D980670
Spacer Material |
Fused Silica (Corning?) |
Mirror Material |
Fused Silica |
Mirror T_HR |
300 +/- 30 ppm |
Mirror R_AR |
< 500 ppm |
Mirror RoC |
500 mm |
Cavity Length |
8" (203.2 mm) |
Cavity Finesse |
10000 |
Cavity g-factor (g1*g2) |
0.352 |
Cavity waist |
0.218 mm |
Cavity FSR |
737.7 MHz |
Cavity pole |
35.2 kHz |
Some FEA of the LIGO/40m reference cavity using COMSOL: /FEA
See also Frequency Stabilization Servo.
