Readout for intersatellite laser interferometry: Measuring low frequency phase fluctuations of HF signals with microradian precision
arXiv:1504.08266 · doi:10.1063/1.4927071
Abstract
Precision phase readout of optical beat note signals is one of the core techniques required for intersatellite laser interferometry. Future space based gravitational wave detectors like eLISA require such a readout over a wide range of MHz frequencies, due to orbit induced Doppler shifts, with a precision in the order of at frequencies between and . In this paper, we present phase readout systems, so-called phasemeters, that are able to achieve such precisions and we discuss various means that have been employed to reduce noise in the analogue circuit domain and during digitisation. We also discuss the influence of some non-linear noise sources in the analogue domain of such phasemeters. And finally, we present the performance that was achieved during testing of the elegant breadboard model of the LISA phasemeter, that was developed in the scope of an ESA technology development activity.
submitted to Review of Scientific Instruments on April 30th 2015
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- Investigation and mitigation of noise contributions in a compact heterodyne interferometer
- Frequency planning for LISA
- Quasi-monolithic heterodyne laser interferometer for inertial sensing
- Single-element dual-interferometer for precision inertial sensing
- Towards the LISA Backlink: Experiment design for comparing optical phase reference distribution systems
- Performance analysis of sequential carrier- and code-tracking receivers in the context of high-precision space-borne metrology systems
- Space-based Gravitational Wave Observatories