Diapycnal eddy diffusivity: Difference between revisions

Revision as of 13:37, 14 October 2021

Short definition of Diapycnal eddy diffusivity (Diapycnal eddy diffusivity <math>K_\rho</math>)
Diapycnal eddy diffusivity (for buoyancy) is defined from the buoyancy flux <math>\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>K_\rho =\frac{\bar{w'\rho'}}{\partial \rho/\partial z}\Gamma \epsilon N^{-2}</math>

@@ Line 1: / Line 1: @@
-{{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>