タイトル | The Use of Ferrofluids to Model Materials Processing (MSFC Center Director's Discretionary Fund) |
本文(外部サイト) | http://hdl.handle.net/2060/20000092062 |
著者(英) | Leslie, F.; Ramachandran, N. |
著者所属(英) | NASA Marshall Space Flight Center |
発行日 | 2000-07-01 |
言語 | eng |
内容記述 | Many crystals grown in space have structural flaws believed to result from convective motions during the growth phase. The character of these instabilities is not well understood but is associated with thermal and solutal density variations near the solidification interface in the presence of residual gravity and g-jitter. To study these instabilities in a separate, controlled space experiment, a concentration gradient would first have to be artificially established in a timely manner as an initial condition. This is generally difficult to accomplish in a microgravity environment because the momentum of the fluid injected into a test cell tends to swirl around and mix in the absence of a restoring force. The use of magnetic fields to control the motion and position of liquids has received recent, growing interest. The possibility of using the force exerted by a non-uniform magnetic field on a ferrofluid to not only achieve fluid manipulation but also to actively control fluid motion makes it an attractive candidate for space applications. This paper describes a technique for quickly establishing a linear or exponential fluid concentration gradient using a magnetic field in place of gravity to stabilize the deployment. Also discussed is a photometric technique for measuring the concentration profile using light attenuation. Although any range of concentrations can be realized, photometric constraints impose some limitations on measurements. Results of the ground-based experiments indicate that the species distribution is within 3 percent of the predicted value. |
NASA分類 | Fluid Mechanics and Thermodynamics |
レポートNO | NASA/TP-2000-210386 NAS 1.60:210386 M-985 |
権利 | No Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/94029 |