Diapycnal eddy diffusivity: Difference between revisions

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{{netcdfGlossary
{{DefineConcept
|parameter_name=Diapycnal eddy diffusivity
|parameter_name=Diapycnal eddy diffusivity <math>K_\rho</math>
|symbol=<math>K_\rho</math>
|description=Diapycnal eddy diffusivity (for buoyancy) is defined from the buoyancy flux <math>\bar{w'\rho'{</math>
|description=Diapycnal eddy diffusivity
|article_type=Concept
|standard_name=turbulent_diffusivity
|instrument_type=Velocity profilers
|units=m<math>^2</math> s<math>^{-1}</math>
|cf-compliant=No
|instrument_type=Velocity point-measurements, Velocity profilers, Shear probes
|standard_long_name=turbulent_diffusivity
}}
}}
<math>K_\rho =\Gamma \epsilon N^{-2}</math>
Osborn 1980 showed that <math>K_\rho =\frac{\bar{w'\rho'}}{\partial \rho/\partial z}\Gamma \epsilon N^{-2}</math>

Revision as of 13:37, 14 October 2021


Short definition of Diapycnal eddy diffusivity (Diapycnal eddy diffusivity [math]\displaystyle{ K_\rho }[/math])
Diapycnal eddy diffusivity (for buoyancy) is defined from the buoyancy flux [math]\displaystyle{ \bar{w'\rho'{ }[/math]

This is the common definition for Diapycnal eddy diffusivity, but other definitions maybe discussed within the wiki.

Osborn 1980 showed that [math]\displaystyle{ K_\rho =\frac{\bar{w'\rho'}}{\partial \rho/\partial z}\Gamma \epsilon N^{-2} }[/math]