Turner angle - Misplaced Pages

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The Turner angle Tu, introduced by Ruddick(1983) and named after J. Stewart Turner, is a parameter used to describe the local stability of an inviscid water column as it undergoes double-diffusive convection. The temperature and salinity attributes, which generally determine the water density, both respond to the water vertical structure. By putting these two variables in orthogonal coordinates, the angle with the axis can indicate the importance of the two in stability. Turner angle is defined as:

Tu(\deg )=\tan ^{-1}\left(\alpha {\frac {\partial \theta }{\partial z}}-\beta {\frac {\partial S}{\partial z}},\alpha {\frac {\partial \theta }{\partial z}}+\beta {\frac {\partial S}{\partial z}}\right)

where tan is the four-quadrant arctangent; α is the coefficient of thermal expansion; β is the equivalent coefficient for the addition of salinity, sometimes referred to as the "coefficient of saline contraction"; θ is potential temperature; and S is salinity. The relation between Tu and stability is as shown

If −45° < Tu < 45°, the column is statically stable.
If −90° < Tu < −45°, the column is unstable to diffusive convection.
If 45° < Tu < 90°, the column is unstable to salt fingering.
If −90° > Tu or Tu > 90°, the column is statically unstable to Rayleigh–Taylor instability.

Relation to density ratio

Turner angle is related to the density ratio mathematically by:

R_{\rho }=-\tan(Tu+45^{\circ })

Meanwhile, Turner angle has more advantages than density ratio in aspects of:

The infinite scale of R_ρ is replaced by a finite one running from +π to -π;
The strong fingering (1 < R_ρ < 2) and weak fingering (2 < R_ρ < ∞) regions occupy about the same space on the Tu scale;
The indeterminate value obtained when ∂_zS = 0 is well defined in terms of Tu;
The regimes and their corresponding angles are easy to remember, and symmetric in the sense that if Tu corresponds to R_ρ, then -Tu corresponds to R_ρ. This links roughly equal strengths of finger and diffusive sense convection.

Nevertheless, Turner angle is not as directly obvious as density ratio when assessing different attributions of thermal and haline stratification. Its strength mainly focuses on classification.

Physical description

Turner angle is usually discussed when researching ocean stratification and double diffusion.

Turner angle assesses the vertical stability, indicating the density of the water column changes with depth. The density is generally related to potential temperature and salinity profile: the cooler and saltier the water is, the denser it is. As the light water overlays on the dense water, the water column is stably stratified. The buoyancy force preserves stable stratification. The Brunt-Vaisala frequency (N) is a measure of stability. If N>0, the fluid is stably stratified.

A stably-statified fluid may be doubly stable. For instance, in the ocean, if the temperature decreases with depth (∂θ/∂z>0) and salinity increases with depth (∂S/∂z<0), then that part of the ocean is stably stratified with respect to both θ and S. In this state, the Turner angle is between -45° and 45°.

However, the fluid column can maintain static stability even if two attributes have opposite effects on the stability; the effect of one just has to have the predominant effect, overwhelming the smaller effect. In this sort of stable stratification, double diffusion occurs. Both attributes diffuse in opposite directions, reducing stability and causing mixing and turbulence. If the slower-diffusing component is the one that is stably-stratified, then the vertical gradient will stay smooth. If the faster-diffusing component is the one providing stability, then the interface will develop long "fingers", as diffusion will create pockets of fluid with intermediate attributes, but not intermediate density.

In the ocean, heat diffuses faster than salt. If colder, fresher water overlies warmer, saltier water, the salinity structure is stable while the temperature structure is unstable (∂θ/∂z<0, ∂S/∂z<0). In these diffusive cases, the Turner angle is -45° to -90°. If warmer, saltier water overlies colder, fresher water (∂θ/∂z>0, ∂S/∂z>0), salt fingering can be expected. This is because patchy mixing will create pockets of cold, salty water and pockets of warm, fresh water. and these pockets will sink and rise. In these fingering cases, the Turner angle is 45° to 90°.

Since Turner angle can indicate the thermal and haline properties of the water column, it is used to discuss thermohaline water structures. For instance, it can be used to define the boundaries of the subarctic front.

Characteristics

Global distribution of the meridional Turner angle Tu at the sea surface (left panel) and 300m depth (right panel). a: July–September, b: January–March, in Gall-Peters projection.

The global meridional Turner angle distributions at the surface and 300-m depth in different seasons are investigated by Tippins, Duncan & Tomczak, Matthias (2003), which indicates the overall stability of the ocean over a long-time scale. It's worth noting that 300-m depth is deep enough to be beneath the mixed layer during all seasons over most of the subtropics, yet shallow enough to be located entirely in the permanent thermocline, even in the tropics.

At the surface, as the temperature and salinity increase from the Subpolar Front towards subtropics, the Turner angle is positive, while it becomes negative due to the meridional salinity gradient being reversed on the equatorial side of the subtropical surface salinity maximum. Tu becomes positive again in the Pacific and Atlantic Oceans near the equator. A band of negative Tu in the South Pacific extends westward along 45°S, produced by the low salinities because of plenty of rainfall, off the southern coast of Chile.

In 300-m depth, it is dominated by positive Tu nearly everywhere except for only narrow bands of negative Turner angles. This reflects the shape of the permanent thermocline, which sinks to its greatest depth in the center of the oceanic gyres and then rises again towards the equator, and which also indicates a vertical structure in temperature and salinity where both decrease with depth.

Availability

The function of Turner angle is available:

For Python, published in the GSW Oceanographic Toolbox from the function gsw_Turner_Rsubrho.

For R, please reference this page Home/CRAN/gsw/gsw_Turner_Rsubrho: Turner Angle and Density Ratio.

For MATLAB, please reference this page GSW-Matlab/gsw_Turner_Rsubrho.m.

References

^ You, Yuzhu (November 2002). "A global ocean climatological atlas of the Turner angle: implications for double-diffusion and water-mass structure". Deep Sea Research Part I: Oceanographic Research Papers. 49 (11): 2075–2093. Bibcode:2002DSRI...49.2075Y. doi:10.1016/S0967-0637(02)00099-7.
^ Ruddick, Barry (October 1983). "A practical indicator of the stability of the water column to double-diffusive activity". Deep Sea Research Part A. Oceanographic Research Papers. 30 (10): 1105–1107. Bibcode:1983DSRA...30.1105R. doi:10.1016/0198-0149(83)90063-8.
"Turner angle - Glossary of Meteorology".
Vanin, N. S. (October 2013). "An experience of using the turner angle for differentiating water structures in the Northwest Pacific". Russian Meteorology and Hydrology. 38 (10): 688–693. doi:10.3103/S1068373913100063. ISSN 1068-3739. S2CID 140608455.
^ Tippins, Duncan; Tomczak, Matthias (2003-11-01). "Meridional Turner angles and density compensation in the upper ocean". Ocean Dynamics. 53 (4): 332–342. Bibcode:2003OcDyn..53..332T. doi:10.1007/s10236-003-0056-5. ISSN 1616-7341. S2CID 128706996.

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