This paper describes the holographic measurement system planned for accommo
dation in the ESA Fluid Science Laboratory (FSL), a new Facility under deve
lopment for the Columbus Orbital Facility of the International Space Statio
n. The FSL provides research opportunities for experiments with fluids and
transparent media under microgravity conditions. One of the diagnostic tool
s for experimental analysis is a holographic interferometer.
Holography is a method used to record and reconstruct wavefronts. The metho
d has a broad spectrum of applications in the field of fluid physics resear
ch on Earth and in a microgravity environment. The size, location and veloc
ity of (tracer) particles inside a fluid volume can be analysed by holograp
hy. and refractive index fields and corresponding temperature or concentrat
ion profiles can be investigated by holographic interferometry. A number of
different techniques/materials are available for hologram recording and re
construction, e.g. photographic emulsions, thermoplastic films, photorefrac
tive crystals and, recently, direct hologram recording with CCD sensors and
numerical reconstruction (digital holography). This paper provides a surve
y of these methods, defines selection criteria for the FSL and describes th
e principal geometry of the FSL holographic set-up under development.