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Length Sensing and Control of a Prototype Advanced Interferometric Gravitational Wave Detector

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Figure

Figure 2.1: Effect of a GW on a circle of test particles. Shown are the effects of a + polarized wave and a× polarized wave, for a wave passing into the plane of the page
Figure 3.1: Input and output fields of a mirror mass. The mirror is composed of a substrate (grayish block)and a reflective coating (dark blue)
Figure 3.2: Michelson based interferometer topologies for gravitational wave detection.
Figure 3.13: Measurement of the opto-mechanical RSE response. The magnitude has been scaled so theoptical resonance is at 0 dB.
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