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ESA's Use of CFD on the ISS |
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The ESA engineers used a trace gas, such as CO2, to determine if the entire ICC cabin was being washed out by the cabin fan. If there were "dead air" regions in the cabin, they would have shown up as regions of finite concentration of the gas after the cabin flow field had reached steady state. In addition, the temperature field was determined including the heat load from numerous electronics boxes and the metabolic heat from two astronauts. This also allowed the engineers to predict the "touch temperature" of hot surfaces, which depend strongly on the convective, conductive and radiative cooling.
The European Columbus laboratory will be used for conducting experiments in a microgravity environment. Such experiments, however, are sensitive to vibration. Sources of vibration on the ISS include
the acceleration and deceleration of moving parts (pumps, fans, motors...), impact forces (opening or closing of valves), or they can be of fluid-dynamic origin.
One source of fluid-dynamic vibration is the venting of gases from Columbus' payload chamber. The exhaust outlet is designed to produce minimal thrust, however, the high velocity plume can impact other modules and the resulting forces are not easy to predict.
CFD can be used to calculate the exhaust plume and the resulting impingement forces. Furthermore, the CFD model can be used to evaluate different venting scenarios with the control valves being opened in a controlled way to minimize any disturbances.
CFD has been shown to be a valuable tool in the design of the ISS. Furthermore, the versatility of CFD allows it to be coupled with other analysis methods allowing for a more complete design.
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