Title: | Experimental
Assessment of Dynamic Surface Deformation Effects in Transition to Oscillatory
Thermocapillary Flow in Liquid Bridge of High Prandtl Number Fluid | Team
Coordinator: |
Satoshi Matsumoto (Japan Aerospace Exploration Agency) |
Principal Investigator: |
Yasuhiro Kamotani (Case Western Reserve University
/ Japan Aerospace Exploration Agency) |
Co-Investigator: | Koichi Nishino Hiroshi
Kawamura Masahiro Kawaji Kazunori Kawasaki Nobuyuki Imaishi | | Yokohama
National University Science University of Tokyo University of Toronto IHI
Aerospace Co., Ltd Kyushu University |
| Salient
points | In the fluid science field, recent interest has focused
on high-speed turbulent flows, which produce many small vortices, instead of gentle
flow. Such turbulent flows are encountered in areas such as spacecraft design.
At the same time, surface-driven flows like thermocapillary flows are not fully
understood in spite of their importance from scientific and industrial points
of view. Microgravity experiments on thermocapillary flows are carried
out frequently. Microgravity conditions would reveal the essence of the thermocapillary
flow because buoyancy and convection are suppressed and a larger liquid bridge
can be formed. Thermocapillary flows have been investigated to contribute the
improvement of materials processing. Convection driven by both buoyancy and
thermocapillary flows are induced during material processing. Convection cannot
be adequately controlled since we do not sufficiently understand thermocapillary
flows. Therefore, fluid physics should be advanced by accumulating the results
of thermocapillary flow experiments. In Japan, thermocapillary flows
have been systematically investigated from two points of view, advancing fluid
physics by using a transparent model fluid and improving material processing techniques
by using practical materials. The visualization techniques have been developed
though Japanese sounding rocket experiments and have become some of the most advanced
experimental methods. Both internal and surface flows can be stereoscopically
visualized in a transparent model fluid. Therefore, detailed information of the
complicated three-dimensional flow enables us to understand the oscillatory flow.
Convection in an opaque fluid, such as molten metal, is usually invisible. However,
even convection in a molten semiconductor can now be visualized since X-ray radiography
observation equipment has been developed. Experiments utilizing sounding rockets
played important roles in developing the observation system and starting the systematic
investigation of oscillatory thermocapillary flows. Complex flows such
as oscillatory motion will be understood better because sophisticated experimental
techniques have been developed. There are two questions to be resolved concerning
thermocapillary flows. First, we must clarify the conditions that generate oscillatory
flows. Second we must understand why a thermocapillary flow changes from steady
to oscillatory. The microgravity experiment will resolve the first problem in
the first KIBO utilization theme. The onset of complex oscillatory flows in both
model fluid and molten semiconductor will be observed. This experiment to resolve
the second problem. The themes utilizing the International Space Station
in the early stage allow understanding the transition behavior of complicated
thermocapillary flows. The results will not only promote better understanding
of thermocapillary flow but also contribute to the advancement of fluid physics
in surface problems.
| Brief
summary | In this experiment, large liquid bridges are formed under
microgravity conditions and flow motions and surface deformations are observed
in detail to investigate the thermocapillary flow. The relation between surface
deformation and flow will be clarified, and an innovative physical model of the
oscillatory transition in a thermocapillary flow will be verified. The results
are certain to contribute both to fluid physics and to applications in materials
processing. Under the influence of a temperature gradient, the surface
is pulled from an area of lower surface tension to an area of higher surface tension.
Consequently, convection called thermocapillary flow occurs (see Fig. 1). It is
well known that a thermocapillary flow can be changed from a steady flow to a
complicated oscillatory flow by changing the temperature difference (see Fig.
2). However, the conditions leading to the onset of oscillatory flow and the associated
transition behavior have not been clarified yet.
| @ | |
Fig. 1 Thermocapillary Flow | |
Fig. 2 Transition From steady to oscillatory flow. |
Previous
investigations to clarify the oscillatory transition revealed that Dynamic Surface
Deformation (DSD), which is a surface wave phenomena, is closely related to
the flow motion (Fig. 2). A new physical model of the transition of thermocapillary
flows has been developed to illustrate the important DSD roles that trigger the
onset of oscillatory flow and maintain it. This model is essentially different
from previous models. This model predicts that oscillatory flow occurs when the
DSD amplitude exceeds a certain value. An experiment with a larger liquid
bridge is needed to verify the hypothesis. Microgravity conditions on board the
International Space Station are utilized because only a small liquid bridge can
be formed on the Earth due to gravity. This experiment uses eight liquid bridges
with different diameters and heights. DSD is precisely observed, and flow and
temperature fields are visualized in detail. The experiment results will be compared
with an advanced numerical simulation taking into account surface motion. The
behavior of DSD in the oscillatory transition and its roles will be clarified.
As a result, this study is expected to clearly explain the unsolved phenomena
related to the oscillatory transition of thermocapillary flow.
Last Updated : October 1, 2003
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