Displacement interferometry is widely used for accurately characterizing nanometer and subnanometer displacements in many applications. In many modern systems, fiber delivery is desired to limit optical alignment and remove heat sources from the system, but fiber delivery can exacerbate common interferometric measurement problems, such as periodic nonlinearity, and account for fiber-induced drift. In this Letter, we describe a novel, general Joo-type interferometer that inherently has an optical reference after any fiber delivery that eliminates fiber-induced drift. This interferometer demonstrated no detectable periodic nonlinearity in both free-space and fiber-delivered variants. © 2011 Optical Society of America OCIS codes: 120.0120, 120.2650, 120.3180, 120.3930, 120.4570, 120.4820. Heterodyne displacement measuring interferometry is a widely applied tool used in gravitational wave detection and conditioning the measurement environment can mitigate the effects of laser frequency instability and refractive index fluctuations. However, periodic nonlinearity in the measurement is more difficult to eliminate because it arises from a combination of source mixing, manufacturing tolerances, and imperfect alignment. Fiber delivery will inherently decrease polarization stability and add timevarying effects, which further complicates the signal processing for interferometers susceptible to periodic nonlinearity [17].Several heterodyne interferometer configurations have been developed that limit the chances for periodic nonlinearity [18][19][20][21][22][23]. These interferometers generally use a spatially separated source and limit all reference and measurement beam overlaps until the final interfering surface prior to detection.In this Letter, we present a general, fiber-coupled Joo-type interferometer with a novel design based on previous Joo-type retroreflector (RR) and plane mirror target interferometers [21,23], which is more suitable for multiaxis systems and has the same footprint on the measurement target as a typical Michelson plane mirror interferometer. Additionally, we compare the results from periodic error analyses between fiber-and free-space-delivered variants and characterize the nominal drift from fiber-induced Doppler shifts. Figure 1 shows a schematic of the general Joo-type interferometer. Two spatially separated beams, horizontally polarized with slightly different optical frequencies ðf 1 ; f 2 Þ are used as the input. When fiber coupling is employed, the phase of the respective optical frequencies ðθ 1 ; θ 2 Þ, vary in time.Both beams enter a beamsplitter (BS), where they are split equally. The reflected beams diagonally cross in a large RR due to the RR's point symmetry. They then travel back to the BS, where they interfere with their respective measurement arms.The initially transmitted beams at the BS also transmit through the polarizing beamsplitter (PBS) and pass through the quarter-wave plate (QWP) oriented at 45°a bout the azimuthal angle. The measurement beam reflects from a mirror (M...