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Scientific and Technical Aerospace Reports Volume 38 July 28, 2000

Scientific and Technical Aerospace Reports Volume 38 July 28, 2000

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Pressure gradients, i.e. pressure head, <strong>and</strong> buoyancy driven convection can be greatly decreased in experimental systems by<br />

acceleration of the laboratory reference frame at a rate consistent with the acceleration due to gravity. This may be done in a number<br />

of ways, the best known of which is the use of orbiting spacecraft. Other techniques include the use of aircraft following an<br />

appropriate parabolic trajectory or drop towers. The result is an experimental condition in which fluids experience virtually no<br />

outside forces relative to the laboratory reference frame. Such conditions are appropriate for the study of processes with diffusion<br />

dominated heat <strong>and</strong>/or mass Under, the study of phase transitions in the absence of pressure gradients, the study of solutal or thermal<br />

capillary convection, or containerless processes. Ways of achieving these conditions <strong>and</strong> complexities that arise in performing<br />

experiments in this environment are discussed.<br />

Author<br />

Microgravity; Acceleration; Pressure Gradients; Buoyancy<br />

<strong>2000</strong>0067655 NASA Marshall Space Flight Center, Huntsville, AL USA<br />

A Technique for Rapidly Deploying a Concentration Gradient with Applications to Microgravity<br />

Leslie, Fred, NASA Marshall Space Flight Center, USA; Ramach<strong>and</strong>ran, Narayanan, Universities Space Research Association,<br />

USA; [<strong>2000</strong>]; 1p; In English; No Copyright; Avail: Issuing Activity; Abstract Only<br />

The latter half of the last century has seen rapid advancements in semiconductor crystal growth powered by the dem<strong>and</strong> for<br />

high performance electronics in myriad applications. The reduced gravity environment of space has also been used for crystal<br />

growth tests, especially in instances where terrestrial growth has largely been unsuccessful. While reduced gravity crystal growth<br />

affords some control of the gravity parameter, many crystals grown in space, to date, have structural flaws believed to result from<br />

convective motions during the growth phase. The character of these instabilities is not well understood but is associated with thermal<br />

<strong>and</strong> solutal density variations near the solidification interface in the presence of residual gravity <strong>and</strong> g-jitter. In order to study<br />

these instabilities in a separate, controlled space experiment, a concentration gradient would first have to be artificially established<br />

in a timely manner as an initial condition. This is generally difficult to accomplish in a microgravity environment because the<br />

momentum of the fluid injected into a test cell tends to swirl around <strong>and</strong> mix in the absence of a restoring force. The use of magnetic<br />

fields to control the motion <strong>and</strong> position of liquids has received growing interest in recent times. The possibility of using the force<br />

exerted by a non-uniform magnetic field on a ferrofluid to not only achieve fluid manipulation but also to actively control fluid<br />

motion makes it an attractive c<strong>and</strong>idate for space applications. This paper describes a technique for quickly establishing a linear<br />

or exponential fluid concentration gradient using a magnetic field in place of gravity to stabilize the deployment. Also discussed<br />

is a photometric technique for measuring the concentration profile using light attenuation. Results of the ground-based experiments<br />

indicate that the concentration distribution is within 3% of the predicted value. Although any range of concentations can<br />

be realized, photometric constraints are discussed which impose some limitations on measurements.<br />

Author<br />

Deployment; Gradients; Microgravity; Nonuniform Magnetic Fields; Concentration (Composition)<br />

<strong>2000</strong>0067686 Alabama Univ., MAE Dept., Huntsville, AL USA<br />

Frequency-Weighting Filter Selection, for H2 Control of Microgravity Isolation Systems: A Consideration of the ”Implicit<br />

Frequency Weighting” Problem<br />

Hampton, Roy David, Alabama Univ., USA; Whorton, Mark S., NASA Marshall Space Flight Center, USA; [1999]; 18p; In<br />

English<br />

Contract(s)/Grant(s): NAG8-1598; RTOP 398-96-02<br />

Report No.(s): IMTC-9184; No Copyright; Avail: CASI; A03, Hardcopy; A01, Microfiche<br />

Many space-science experiments need an active isolation system to provide them with the requisite microgravity environment.<br />

The isolation systems planned for use with the International Space Station (ISS) have been appropriately modeled using<br />

relative position, relative velocity, <strong>and</strong> acceleration states. In theory, frequency-weighting design filters can be applied to these<br />

state-space models, in order to develop optimal H2 or mixed-norm controllers with desired stability <strong>and</strong> performance characteristics.<br />

In practice, however, since there is a kinematic relationship among the various states, any frequency weighting applied to<br />

one state will implicitly weight other states. These implicit frequency-weighting effects must be considered, for intelligent frequency-weighting<br />

filter assignment. This paper suggests a rational approach to the assignment of frequency-weighting design<br />

filters, in the presence of the kinematic coupling among states that exists in the microgravity vibration isolation problem.<br />

Author<br />

Hydrogen; Microgravity; Vibration Isolators; B<strong>and</strong>pass Filters; Frequencies; Spaceborne Experiments; Weighting Functions;<br />

H-2 Control<br />

59

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