The objective of this study is to refine the understanding of micro-fluidics subject to micro-gravity in an attempt to support future space exploration efforts. A combination of experimental and numerical approaches were utilized to build a validated assessment approach. A quasi-pore geometry, inspired by CT scans of rat bones, was used in lieu of human bone structures. A quasi-1D assessment of the conservation of momentum was used to identify the dominant forces acting on the fluid at the operating length-scales. The dominant forces were surface tension, gravity, and shear stress. Experiments were conducted to visualize the flow moving through the quasi-pore geometry. Computational Fluid Dynamics (CFD) was used to create a corresponding model of the experiments in order to illicit further insight. The CFD models were validated by using micro-fluidic experiments. Once validated, the CFD model was also used to study micro-fluids in micro-gravity conditions. The results showed that gravity has a significant effect on the flow pattern of fluids through micro-fluidic porous features. The results can be correlated to the fluid flow through bone pores on Earth versus in micro-gravity. This suggests that interstitial fluid flow is influenced by the effects of micro-gravity leading to physiological changes in astronaut bones.
| Identifer | oai:union.ndltd.org:ucf.edu/oai:stars.library.ucf.edu:etd2020-2241 |
| Date | 01 January 2022 |
| Creators | Le Henaff, Sylvain |
| Publisher | STARS |
| Source Sets | University of Central Florida |
| Language | English |
| Detected Language | English |
| Type | text |
| Format | application/pdf |
| Source | Electronic Theses and Dissertations, 2020- |
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