Editing ThreeDimensionalConfigurations/CAREs (section)

==New Idea==

Perhaps we should move away from Riemann S-type ellipsoids and attempt instead to develop an SCF technique that can be used to construct a variety of Type I Riemann ellipsoids.  This might be useful because:
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The velocity flow-field is not constrained to be independent of z.  (Although a related constraint appears to be in place.)  This would lead to significant redesign of my above-mentioned "Incomplete" on-line notes.  This state of affairs might demand that each system evolve on a viscous time scale toward a flow field that has no z-component.
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In the Type I Riemann ellipsoids, the steady-state flow-field already shows a pair of off-axis circulations &#8212; analogous to what is seen in a binary system &#8212; even though the underlying density distribution is uniform.  This flow would presumably get "locked in" as the configuration cooled and encourage/necessarily imply the development of off-axis density maxima develop.
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Given that the spin-axis of the interflow is not aligned with the spin-axis of the ellipsoidal figure, one can imagine that a binary system formed from such a configuration would have a wide range of interesting properties; the spin and orbital angular momentum axes would be different from one another, for example.  This reminds me of work that Peter Bodenheimer did in the late 70s &#8212; see [https://ui.adsabs.harvard.edu/abs/1978ApJ...224..488B/abstract P. Bodenheimer (1978, ApJ, 224, 448)] &#8212; when he used fragmentation of "rings' to estimate how multiple multiple star systems might divide up the angular momentum.
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