Design and Preparation of a Particle Dynamics Space Flight Experiment, SHIVA

• Published in: Annals of the New York Academy of Sciences 2004-11, Vol.1027 (1), p.550-566
• Main Authors: TROLINGER, JAMES D., L'ESPERANCE, DREW, RANGEL, ROGER H., COIMBRA, CARLOS F.M., WITHEROW, WILLIAM K.
• Format: Article
• Language: English
• Subjects: Acceleration; Cosmic Radiation; Gravitation; Holography; microgravity; Microscopy, Video; particle dynamics; Physics - methods; Pressure; Space Flight; Spacecraft; Stokes flow; Weightlessness; Weightlessness Simulation
• ISSN: 0077-8923; 1749-6632
• DOI: 10.1196/annals.1324.042

: This paper describes the flight experiment, supporting ground science, and the design rationale for a project on spaceflight holography investigation in a virtual apparatus (SHIVA). SHIVA is a fundamental study of particle dynamics in fluids in microgravity. Gravitation effects and steady Stokes drag often dominate the equations of motion of a particle in a fluid and consequently microgravity provides an ideal environment in which to study the other forces, such as the pressure and viscous drag and especially the Basset history force. We have developed diagnostic recording methods using holography to save all of the particle field optical characteristics, essentially allowing the experiment to be transferred from space back to Earth in what we call the “virtual apparatus” for microgravity experiments on Earth. We can quantify precisely the three‐dimensional motion of sets of particles, allowing us to test and apply new analytic solutions developed by members of the team. In addition to employing microgravity to augment the fundamental study of these forces, the resulting data will allow us to quantify and understand the ISS environment with great accuracy. This paper shows how we used both experiment and theory to identify and resolve critical issues and to produce an optimal experimental design that exploits microgravity for the study. We examined the response of particles of specific gravity from 0.1 to 20, with radii from 0.2 to 2 mm, to fluid oscillation at frequencies up to 80 Hz with amplitudes up to 200 microns. To observe some of the interesting effects predicted by the new solutions requires the precise location of the position of a particle in three dimensions. To this end we have developed digital holography algorithms that enable particle position location to a small fraction of a pixel in a CCD array. The spaceflight system will record holograms both on film and electronically. The electronic holograms can be downlinked providing real‐time data, essentially acting like a remote window into the ISS experimental chamber. Ground experiments have provided input to a flight system design that can meet the requirements for a successful experiment on ISS. Moreover the ground experiments have provided a definitive, quantitative observation of the Basset history force over a wide range of conditions. Results of the ground experiments, the flight experiment design, preliminary flight hardware design, and data analysis procedures are reported.