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Measure used in calculating seawater density gradient

Density ratio

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The density ratio of a column of seawater is a measure of the relative contributions of temperature and salinity in determining the density gradient. At a density ratio of 1, temperature and salinity are said to be compensated: their density signatures cancel, leaving a density gradient of zero. The formula for the density ratio, {\displaystyle R_{\rho }}, is:

{\displaystyle R_{\rho }={\frac {\alpha d\theta /dz}{\beta dS/dz}}}

where

When a water column is "doubly stable"—both temperature and salinity contribute to the stable density gradient—the density ratio is negative (a doubly unstable water column would also have a negative density ratio but does not commonly occur). When either the temperature- or salinity-induced stratification is statically unstable, while the overall density stratification is statically stable, double-diffusive instability exists in the water column. Double-diffusive instability can be separated into two different regimes of statically stable density stratification: a salt fingering regime (warm salty overlying cool fresh) when the density ratio is greater than 1, and a diffusive convection regime (cool fresh overlying warm salty) when the density ratio is between 0 and 1.

Density ratio may also be used to describe thermohaline variability over a non-vertical spatial interval, such as across a front in the mixed layer.

Diffusive density ratio

In place of the density ratio, sometimes the diffusive density ratio {\displaystyle R_{\rho }^{*}} is used, which is defined as

{\displaystyle R_{\rho }^{*}={\frac {1}{R_{\rho }}}={\frac {\beta dS/dz}{\alpha d\theta /dz}}}

Turner Angle

If the signs of both the numerator and denominator are reversed, the density ratio remains unchanged. A related quantity which avoids this ambiguity as well as the infinite values possible when the denominator vanishes is the Turner angle, {\displaystyle Tu}, which was introduced by Barry Ruddick and named after Stewart Turner. It is defined by

{\displaystyle Tu={\frac {3\pi }{4}}-\mathrm {arg} \left(\beta {\frac {dS}{dz}}+i\alpha {\frac {d\theta }{dz}}\right).}

The Turner angle is related to the density ratio by

{\displaystyle R_{\rho }=-\tan \left(Tu+{\frac {\pi }{4}}\right).}

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Text from Wikipedia, CC BY-SA 4.0 · Source article