Danielle M. R. Wuchenich
Australian National University
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Featured researches published by Danielle M. R. Wuchenich.
Optics Express | 2009
Glenn de Vine; D. S. Rabeling; Bram Slagmolen; Timothy T.-Y. Lam; S. Chua; Danielle M. R. Wuchenich; D. E. McClelland; Daniel A. Shaddock
Digitally enhanced heterodyne interferometry is a laser metrology technique employing pseudo-random codes phase modulated onto an optical carrier. We present the first characterization of the techniques displacement sensitivity. The displacement of an optical cavity was measured using digitally enhanced heterodyne interferometry and compared to a simultaneous readout based on conventional Pound-Drever-Hall locking. The techniques agreed to within 5 pm/ radicalHz at 1 Hz, providing an upper bound to the displacement noise of digitally enhanced heterodyne interferometry. These measurements employed a real-time signal extraction system implemented on a field programmable gate array, suitable for closed-loop control applications. We discuss the applicability of digitally enhanced heterodyne interferometry for lock acquisition of advanced gravitational wave detectors.
Optics Letters | 2011
Danielle M. R. Wuchenich; Timothy T.-Y. Lam; Jong H. Chow; D. E. McClelland; Daniel A. Shaddock
Digitally enhanced interferometry (DI) can be used to distinguish between interferometric signals and simultaneously monitor in-line object displacements with subnanometer sensitivity. In contrast to conventional interferometry-where these signals interfere with each other and degrade performance-we experimentally show that by using DI, each of these signals can be isolated and measured at the same time. We present what we believe to be the first demonstration of DIs signal multiplexing capabilities, showing simultaneous length sensing of three sections of an optical fiber. The cross talk between length measurements was less than 2.6×10(-3) with a displacement noise floor of 200 pm/√Hz, which corresponds to a strain sensitivity of less than 80 picostrain(pϵ) in each sensor. We also enhance our systems displacement sensitivity at low frequencies by combining information from multiple lengths to suppress errors due to laser frequency noise.
Classical and Quantum Gravity | 2014
R. L. Ward; Roland Fleddermann; Suzanne Francis; C. M. Mow-Lowry; Danielle M. R. Wuchenich; Mary M Elliot; F Gilles; Mark Herding; Kolja Nicklaus; J Brown; James E. Burke; Svetlana Dligatch; David I. Farrant; K L Green; Jeffrey A. Seckold; M Blundell; R Brister; Craig R. Smith; Karsten Danzmann; Gerhard Heinzel; D Schutze; Benjamin Sheard; William M. Klipstein; D. E. McClelland; Daniel A. Shaddock
The Gravity Recovery and Climate Experiment (GRACE) mission, launched in 2002, is nearing an end, and a continuation mission (GRACE Followon) is on a fast-tracked development. GRACE Follow-on will include a laser ranging interferometer technology demonstrator, which will perform the first laser interferometric ranging measurement between separate spacecraft. This necessitates the development of lightweight precision optics that can operate in this demanding environment. In particular, this beam routing system, called the triple mirror assembly, for the GRACE Follow-on mission presents a significant manufacturing challenge. Here we report on the design and construction of a prototype triple mirror assembly for the GRACE Follow-on mission. Our constructed prototype has a co-alignment error between the incoming and
Optics Express | 2014
Danielle M. R. Wuchenich; Christoph Mahrdt; Benjamin Sheard; Samuel P. Francis; Robert E. Spero; J. D. B. Miller; C. M. Mow-Lowry; R. L. Ward; William M. Klipstein; Gerhard Heinzel; Karsten Danzmann; D. E. McClelland; Daniel A. Shaddock
We experimentally demonstrate an inter-satellite laser link acquisition scheme for GRACE Follow-On. In this strategy, dedicated acquisition sensors are not required-instead we use the photodetectors and signal processing hardware already required for science operation. To establish the laser link, a search over five degrees of freedom must be conducted (± 3 mrad in pitch/yaw for each laser beam, and ± 1 GHz for the frequency difference between the two lasers). This search is combined with a FFT-based peak detection algorithm run on each satellite to find the heterodyne beat note resulting when the two beams are interfered. We experimentally demonstrate the two stages of our acquisition strategy: a ± 3 mrad commissioning scan and a ± 300 μrad reacquisition scan. The commissioning scan enables each beam to be pointed at the other satellite to within 142 μrad of its best alignment point with a frequency difference between lasers of less than 20 MHz. Scanning over the 4 alignment degrees of freedom in our commissioning scan takes 214 seconds, and when combined with sweeping the laser frequency difference at a rate of 88 kHz/s, the entire commissioning sequence completes within 6.3 hours. The reacquisition sequence takes 7 seconds to complete, and optimizes the alignment between beams to allow a smooth transition to differential wavefront sensing-based auto-alignment.
Optics Letters | 2013
David John Bowman; Malcolm J King; Andrew Sutton; Danielle M. R. Wuchenich; R. L. Ward; Emmanuel Malikides; D. E. McClelland; Daniel A. Shaddock
Extending phased array techniques to optical frequencies is challenging because of the considerably smaller wavelengths and the difficulty of stabilizing the optical path lengths of multiple emitters to this level of precision. This is especially true under real-world conditions where thermal and vibrational disturbances cause path length variations that are considerable in relation to the wavelength. Earlier attempts have relied on an external mechanism to sense and compensate for any unwanted variations in the outgoing beams. Here we propose and demonstrate a method that does not rely on any external components. The method combines a pseudo-random noise phase modulation scheme together with conventional heterodyne interferometry to simultaneously measure phase variations between emitters. This information is then used to control the relative phases between the emitters and compensate for any unwanted disturbance. Experimental results are presented that support the viability of this design.
Classical and Quantum Gravity | 2014
Roland Fleddermann; R. L. Ward; M Elliot; Danielle M. R. Wuchenich; F Gilles; Mark Herding; Kolja Nicklaus; J Brown; James E. Burke; Svetlana Dligatch; David I. Farrant; K L Green; Jeffrey A. Seckold; M Blundell; R Brister; Craig R. Smith; Benjamin Sheard; Gerhard Heinzel; Karsten Danzmann; B. Klipstein; D. E. McClelland; Daniel A. Shaddock
We report on the successful testing of the GRACE follow-on triple mirror assembly (TMA) prototype. This component serves to route the laser beam in a proposed follow-on mission to the Gravity Recovery and Climate Explorer (GRACE) mission, containing an optical instrument for space-based distance measurement between satellites. As part of this, the TMA has to meet a set of stringent requirements on both the optical and mechanical properties. The purpose of the TMA prototype testing is to establish the feasibility of the design, materials choice and fabrication techniques. Here we report on co-alignment testing of this device to the arc second (5 μrad) level and thermal alignment stability testing to 1 .
Applied Optics | 2014
Lyle E. Roberts; R. L. Ward; Andrew Sutton; Roland Fleddermann; Glenn de Vine; Emmanuel Malikides; Danielle M. R. Wuchenich; D. E. McClelland; Daniel A. Shaddock
Coherent combination of multiple lasers using an optical phased array (OPA) is an effective way to scale optical intensity in the far field beyond the capabilities of single fiber lasers. Using an actively phase locked, internally sensed, 2D OPA we demonstrate over 95% fringe visibility of the interfered beam, λ/120 RMS output phase stability over a 5 Hz bandwidth, and quadratic scaling of intensity in the far field using three emitters. This paper presents a new internally sensed OPA architecture that employs a modified version of digitally enhanced heterodyne interferometry (DEHI) based on code division multiplexing to measure and control the phase of each emitter. This internally sensed architecture can be implemented with no freespace components, offering improved robustness to shock and vibration exhibited by all-fiber devices. To demonstrate the concept, a single laser is split into three channels/emitters, each independently controlled using separate electro-optic modulators. The output phase of each channel is measured using DEHI to sense the small fraction of light that is reflected back into the fiber at the OPAs glass-air interface. The relative phase between emitters is used to derive the control signals needed to stabilize their relative path lengths and maintain coherent combination in the far field.
australian conference on optical fibre technology | 2011
Andrew Sutton; Danielle M. R. Wuchenich; Timothy T.-Y. Lam; Daniel A. Shaddock
We present a novel technique for optical interrogation of multiplexed displacement sensors with homodyne detection. Based upon the Digitally Enhanced Interferometry, we propose the use of a complex (IQ) modulation to reduce sensitivity to scattered light and provide multiplexing capabilities. Results of initial prototype testing are presented.
Proceedings of SPIE - The International Society for Optical Engineering | 2011
Timothy T.-Y. Lam; Danielle M. R. Wuchenich; Jong H. Chow; D. E. McClelland; Daniel A. Shaddock
The resolution of fiber optic interferometry sensors is often limited by frequency noise in the laser. For this reason, prestabilization techniques have been used to reduce laser frequency fluctuations and improve signal resolution. However, for multi-element systems this becomes cumbersome and difficult to implement. In this paper, we demonstrate the use of digitally-enhanced interferometry for the interrogation of a multi-element sensing system. Over 50 dB of cross-talk rejection was found, with displacement resolutions of ~ 100 pm. Furthermore, using this technique, sub-frequency noise displacement resolution was obtained without the need for high performance sensors.
Optics Express | 2018
Tiehui Su; Guangyao Liu; Katherine E Badham; Samuel T. Thurman; Richard L. Kendrick; Alan J. Duncan; Danielle M. R. Wuchenich; Chad Ogden; Guy Chriqui; Shaoqi Feng; Jaeyi Chun; Weicheng Lai; S. J. B. Yoo