Experiment

Experiment
A.019

Experiment
Density distribution for the near critical fluids in microgravity.

Primary investigator
Michels, A.C.

Co-investigator
Krop, H.W.

Contact point
Van der Waals laboratory, University of Amsterdam

Category
Fluid Sciences

Main research area
Critical Point Phenomena

Abstract
Critical point research is recognized as a major item in the field of microgravity fluid physics research. Especially for experiments on a one-component fluid system the relevance of microgravity is easily demonstrated. When a system approaches its critical point it shows a strong increase of density fluctuations in the sample as well as a strong increase in the overall isothermal compressibility. The strongly increasing density dictates an experimental requirement of a rather large sample of uniform density, since its dimensions should exceed the characteristic correlation length (5) by some orders of magnitude; the strongly increasing compressibility leads to a strong compression of a near critical fluid in a gravity field under its own weight and hence to a strong vertical density gradient. This makes it impossible to obtain uniform samples in a 1-g gravity field close to the critical point.
Over the past years, a number of critical-point research groups proposed and developed microgravity experiments for a one component system. Two of these were carried out during the Spacelab D1 mission, with remarkable results; they show neither a homogeneous density distribution, nor the expected non-analytic critical behaviour. These results have been explained as being primarily due to strongly enhanced thermal relaxation times. However, other mechanisms may also be of importance. For instance the influence of density gradients induced at the put constraints on the design of sample cells for future studies; a motive for the present study.

Objectives
The objective of our experiment, was to put a sealed sample of critical density through a number of near critical states by slow or stepwise change of temperature and to observe its response to the change in the acceleration field. The lay-out of the apparatus is shown in Figs. 4.14 and 4.15. The SF fluid samples, with T = 45C, are contained in glass tubes with a diameter of 5.35 mm and about 7 cm long.

Experiment procedure
Due to divergence of relaxation times in a fluid sample when the critical point is approached the study of critical phenomena typically requires long waiting time (in the order of hours) before the actual measurement is performed. However, in studying relaxation mechanisms, the quenching technique has proved to be very useful. In these experiments the sample is equilibrated in the one-phase region and then "quenched" to two-phase "conditions" by suddenly changing the temperature or the pressure. The ensuing relaxation phenomena can then be observed until two-phase equilibrium is attained.
Some information - be it qualitative - is already obtained in the first seconds after the quench. This has led to the assumption that some information on the preferred density distribution in microgravity can be obtained by " gravity-quenching", i.e. bringing a sample in equilibrium under normal gravity conditions and then abruptly put it in microgravity environment, for instance in a parabolic airplane flight.

Results
The experiment was flown on the ESA KC-135 campaign in Houston. A video camera recorded clear pictures of the g-quench behaviour of the sample in the temperature range of Tc + 250 mK to Tc - 2400 mK. The data rveal the following general behaviour. At low temperatures (Tc -T>500 mK) the liquid spreads over the glass surface, directly after the onset of the microgravity phase.
This surface layer seems rather sensitive to residual gravity and vibrations. Closer to Tc the fluid layer also develops, but at a slower rate and with much turbulence. At high temperature ( T-Tc >200 mK) there is no significant change of density distribution during the microgravity phase; there is an indication of redistribution during the high-g phase.
Interesting phenomena appear for T-Tc 30 mK. At this temperature the overall density difference in the sample at 1g is a few percent, which is not shown by the laser beam since it propagates parallel to the density gradient. Beam bending and reflection is observed, a few seconds after the onset of the microgravity phase indicating the build up of a layer of unexpected high density along the tube walls. This layer seems to move around with the residual g-jitter, but regular wave patterns can also be observed. The delay time for the onset of this effect is quite different for various parabolas. The temperature stability however, does not allow to correlate this time to the value of T-Tc .

Funding agency
ESA

Launcher
ESA KC-135

Mission
ESA parabolic flight campaign 88.08.08

Success
Although not all results of the campaign have been completely analyzed yet, we observed that the reaction of the sample to the disappearance of the gravity field strongly depends on the distance from the critical point, even in the one-phase region. Also the influence of the walls is quite apparent. The arrangement chosen for the experiment seems well suited to obtain better information. Therefore we propose to repeat the experiment in a future flight with minor modifications to further improve the equipment.

Pictures

Exchangeable thermostat core with sample cell


Layout of the critical-point experiment


Extracted from a prototype of the Dutch Microgravity Compact Disc