Computer Science – Performance
Scientific paper
Mar 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999evga.conf..278s&link_type=abstract
13th Working Meeting on European VLBI for Geodesy and Astrometry, p. 278 - 284
Computer Science
Performance
Scientific paper
Large Ring lasers are not yet used for geophysical applications. C-II is a prototype for such a device and has a square optical path with side 1 m. One difference with the earlier C-I laser testbed - and similarity to an aircraft gyro - is its monolithic construction. It is housed 30 m underground in a New Zealand military bunker. The measured ringdown time of 0.20 ms corresponds to a quality factor 6e+11 and a finesse 9.4e+4. For the observed exit beam power of 10 pW, this gives an angular rotation sensitivity 4 × 10-9 rad/s/sqrt(Hz). C-II performance limits therefore rival those of Sagnac matter-wave gyroscopes (2 × 10-8 rad/s/sqrt(Hz)). This also corresponds to a quantum noise line width of 220 microhertz, consistent with that observed (172 microhertz) in the direct spectrum and with the coefficient of inverse time in the Allan variance plot.
Schluter Wolfgang
Schneider Manfred
Schreiber Urs
Stedman Geoffrey E.
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