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The layered system is heated from below, the upper (fluid) surface is free to the atmosphere, and convection driven by surface tension is allowed for.
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With continued microwave heating, the density of the bottom fluid dropped below the density of the upper fluid, creating a Rayleigh–Taylor unstable configuration, and, subsequently, buoyancy driven mixing.
Above this layer is a region of free-flowing fluid which we refer to as the upper fluid layer.
Specifically, we explore the effect of fluid shear stress on cell yield and distribution, via changes in the fluid flux into the upper fluid layer.
Below, the upper part of the OMZ is generally almost free of organisms.
(3.1a), (3.3b) and (3.4a) across the lumen, cell layer and upper fluid layer.
The fluid level was adjusted to just below the upper edge of the gel to expose the gel surface to air.
Free convection takes place at the up side of the upper plate and forced convection below the upper plate.
The mixing takes place in the vertical section of the well below the upper lateral.
In magnetized plasma, we also could observe the sheath waves below the Upper Hybrid Resonance frequency.
Below the upper clouds, Venus has a hostile atmosphere containing clouds of sulfuric acid droplets.
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