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Ocean Density Salinity Temperature Calculator

Free Ocean density salinity temperature Calculator for oceanography & coastal science. Enter variables to compute results with formulas and detailed steps.

Reviewed by Daniel Agrici, Founder & Lead Developer

Reviewed by Daniel Agrici, Founder & Lead Developer

Formula

rho = rho_w(T) + A(T)*S + B(T)*S^(3/2) + C*S^2

Where rho is seawater density, rho_w is pure water density as a function of temperature T, S is salinity in PSU, and A B C are polynomial coefficients that depend on temperature.

Worked Examples

Example 1: Tropical Surface Water Density

Problem:Calculate the density of tropical surface seawater with temperature 28C salinity 35.5 PSU at the surface.

Solution:Pure water density at 28C: rho_w = 996.24 kg/m3\nSalinity terms: A*35.5 + B*35.5^1.5 + C*35.5^2\nFinal: rho = 1023.16 kg/m3\nSigma-t = 23.16

Result:Density: 1023.16 kg/m3 | Sigma-t: 23.16 | Sound speed: 1540 m/s

Example 2: North Atlantic Deep Water

Problem:Calculate properties of deep water at temperature 2.5C salinity 34.9 PSU at 3000 m depth.

Solution:Pure water density at 2.5C: rho_w = 999.94 kg/m3\nSalinity contribution: +27.79 kg/m3\nrho = 1027.73 kg/m3\nPotential temp = 2.5 - 0.36 = 2.14C

Result:Density: 1027.73 kg/m3 | Sigma-t: 27.73 | Potential temp: 2.14C

Frequently Asked Questions

How does temperature affect ocean water density?

Temperature has a nonlinear inverse relationship with ocean water density meaning warmer water is generally less dense than cooler water. The thermal expansion of seawater increases with temperature so a one-degree warming at 25C produces a larger density change than at 5C. At typical ocean salinities maximum density occurs at the freezing point rather than at 4C as with fresh water. The thermal contribution ranges from about 0.15 kg/m3 per degree at low temperatures to 0.35 kg/m3 per degree at high temperatures. This temperature sensitivity drives global thermohaline circulation as surface waters cool at high latitudes and sink.

What is potential temperature in oceanography?

Potential temperature is the temperature a water parcel would have if adiabatically brought to a reference pressure level typically the sea surface. As water sinks increasing hydrostatic pressure compresses it slightly causing in-situ temperature to rise without heat exchange. This adiabatic heating amounts to approximately 0.12 degrees Celsius per 1000 meters of depth. Potential temperature removes this pressure effect allowing meaningful comparison of water masses at different depths. For example Antarctic Bottom Water has potential temperature near -0.5C at the surface reference but its in-situ temperature at 4000 meters is slightly higher.

What is the Brunt-Vaisala frequency and how does it relate to density?

The Brunt-Vaisala frequency also called buoyancy frequency measures the static stability of a stratified fluid and represents the natural oscillation frequency of a vertically displaced water parcel. It is defined as N = sqrt((-g/rho) * d(rho)/dz) where g is gravitational acceleration rho is density and d(rho)/dz is the vertical density gradient. When N-squared is positive the water column is stably stratified. Typical values in the ocean thermocline range from 0.005 to 0.02 per second corresponding to periods of 5 to 20 minutes. The buoyancy frequency determines maximum frequency of internal waves and controls vertical mixing rates.

Why does seawater density matter for ocean circulation?

Seawater density is the fundamental driver of thermohaline circulation the global overturning that transports heat salt nutrients and dissolved gases throughout the world ocean. Dense water formed by cooling and brine rejection during sea ice formation sinks to the ocean floor and flows equatorward. The density difference between surface and deep waters determines vertical stratification controlling how easily wind mixing can bring nutrients to the sunlit surface. Horizontal density gradients drive geostrophic currents through the thermal wind relationship shaping major ocean gyres. Changes in density structure from melting ice sheets could weaken Atlantic Meridional Overturning Circulation.

References

Reviewed by Daniel Agrici, Founder & Lead Developer ยท Editorial policy