Interferometric surface mapping of a spherical proof mass for ultra precise inertial reference sensors.

In the context of our investigations on novel inertial reference sensors for space applications, we have explored a design utilizing an optical readout of a spherical proof mass. This concept enables full drag-free operations, hence reducing proof mass residual acceleration noise to a minimum. The main limitations of this sensor are errors in position determination of the center of mass of the proof mass due to the surface topography and the involved path length changes upon rotation. One solution is to apply a surface map for correction of the measurement data, thus improving the precision of position determination. This article presents the results of our one-dimensional interferometric surface topography measurements of a sphere, achieving uncertainties of ≈10  nm, as a first step to realize a complete surface map. The measurement setup consists of two heterodyne interferometers positioned in an opposing configuration, which measure the surface topography while the sphere is continuously rotated by a rotation stage.

[1]  J. P. López-Zaragoza,et al.  Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results. , 2016, Physical review letters.

[2]  D. DeBra,et al.  Precision spheres for the Gravity Probe B experiment , 2015 .

[3]  Badr N. Alsuwaidan,et al.  The Gravity Probe B test of general relativity , 2015 .

[4]  Ulrich Johann,et al.  Design of a dual species atom interferometer for space , 2014, 1412.2713.

[5]  D. DeBra,et al.  Invited article: advanced drag-free concepts for future space-based interferometers: acceleration noise performance. , 2009, The Review of scientific instruments.

[6]  Martin Gohlke,et al.  Interferometric characterization and modeling of pathlength errors resulting from beamwalk across mirror surfaces in LISA. , 2013, Applied optics.

[7]  Walter Fichter,et al.  The LISA Pathfinder interferometry—hardware and system testing , 2011 .

[8]  Michael Krystek,et al.  Volume determination of the Avogadro spheres of highly enriched 28Si with a spherical Fizeau interferometer , 2011 .

[9]  I Busch,et al.  Determination of the Avogadro constant by counting the atoms in a 28Si crystal. , 2010, Physical review letters.

[10]  Martin Gohlke,et al.  Picometer and nanoradian optical heterodyne interferometry for translation and tilt metrology of the LISA gravitational reference sensor , 2009 .

[11]  Walter Fichter,et al.  LISA Pathfinder: the experiment and the route to LISA , 2009 .

[12]  John Conklin,et al.  Determination of Spherical Test Mass Kinematics with Modular Gravitational Reference Sensor , 2008 .

[13]  Ulrich Johann,et al.  Novel Payload Architectures for LISA , 2006 .

[14]  Robert L. Byer,et al.  Advanced gravitational reference sensor for high precision space interferometers , 2005 .

[15]  Ulrich Johann,et al.  Interferometry for the LISA technology package (LTP) aboard SMART-2 , 2003 .

[16]  J. Fu,et al.  Heterodyne interferometer with two spatial-separated polarization beams for nanometrology , 2002 .

[17]  B. Lange Managing spherical proof masses in drag-free satellites with application to the LISA experiment , 2001 .

[18]  L. Ek,et al.  Heterodyne profiling instrument for the angstrom region. , 1986, Applied optics.

[19]  G E Sommargren,et al.  Optical heterodyne profilometry. , 1981, Applied optics.

[20]  Benjamin Lange,et al.  The Drag-Free Satellite , 1964 .