What Characteristic Length Should Be Used for Fluids in Low Gravity?

AI Thread Summary
In low gravity, the natural oscillation frequency of fluids is influenced by surface tension and density, with the characteristic length denoted as L. For different geometries, such as spheres or channels, the appropriate characteristic length can vary; for spheres, it may be the diameter or radius, while for channels, it could depend on dimensions like length, width, or height. The choice of characteristic dimension is crucial as it directly affects the vibration modes and their corresponding frequencies. Understanding these relationships is essential for accurate modeling of fluid behavior in low gravity environments. Clarification on the distinction between using radius versus diameter remains a point of confusion.
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Hi PF!

Fluids in low gravity have a natural oscillation frequency ##\lambda = \sqrt{\sigma / (\rho L^3)}##, where ##\sigma## is surface tension, ##\rho## density, ##L## characteristic length.

Then given a particular object, say a sphere, is ##L=D## or ##L=r##? How about a channel; would ##L## be the length, width, or height, or what about, say, half-width? Any help is greatly appreciated!
 
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The characteristic dimension will depend on the vibration mode. For example, look here.

https://saviot.cnrs.fr/lamb/index.en.html
A sphere has entire families of vibration modes. Each one will have a different frequency because it involves different masses doing different things.
 
DEvens said:
The characteristic dimension will depend on the vibration mode. For example, look here.

https://saviot.cnrs.fr/lamb/index.en.html
A sphere has entire families of vibration modes. Each one will have a different frequency because it involves different masses doing different things.
Thanks for responding. I don't really see how to distinguish between using the radius vs diameter though.
 
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