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Experiment 7: The Geophysical Fluid Flow Cell Experiment on USML-2The Geophysical Fluid Flow Cell (GFFC) experiment performed visualizations of thermal convection in a rotating differentially heated spherical shell of fluid. In these experiments dielectric polarization forces are used to generate a radially directed buoyancy force. This enables the laboratory simulation of a number of geophysically and astrophysically important situations in which sphericity and rotation both impose strong constraints on global scale fluid motions. During USML-2 a large set of experiments with spherically symmetric heating were carried out. These enabled the determination of critical points for the transition to various forms of non-axisymmetric convection and, for highly turbulent flows, the transition latitudes separating the different modes of motion. This paper presents a first analysis of these experiments as well as data on the general performance of the instrument during the USML-2 flight.
Document ID
19990018875
Acquisition Source
Marshall Space Flight Center
Document Type
Other
Authors
Hart, John E.
(Colorado Univ. Boulder, CO United States)
Ohlsen, Daniel R.
(Colorado Univ. Boulder, CO United States)
Kittleman, Scott
(Colorado Univ. Boulder, CO United States)
Leslie, Fred W.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Miller, Timothy L.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Date Acquired
August 19, 2013
Publication Date
August 1, 1998
Publication Information
Publication: Second United States Microgravity Laboratory: One Year Report
Volume: 1
Subject Category
Fluid Mechanics And Heat Transfer
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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