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  2. Seawater - Wikipedia

    en.wikipedia.org/wiki/Seawater

    The density of surface seawater ranges from about 1020 to 1029 kg/m 3, depending on the temperature and salinity. At a temperature of 25 °C, the salinity of 35 g/kg and 1 atm pressure, the density of seawater is 1023.6 kg/m 3. [7] [8] Deep in the ocean, under high pressure, seawater can reach a density of 1050 kg/m 3 or higher. The density of ...

  3. TEOS-10 - Wikipedia

    en.wikipedia.org/wiki/TEOS-10

    TEOS-10 (Thermodynamic Equation of Seawater - 2010) is the international standard for the use and calculation of the thermodynamic properties of seawater, humid air and ice. It supersedes the former standard EOS-80 (Equation of State of Seawater 1980). [ 1 ]

  4. Sigma-t - Wikipedia

    en.wikipedia.org/wiki/Sigma-t

    Sigma-t is a quantity used in oceanography to measure the density of seawater at a given temperature. [1] σ T is defined as ρ(S,T)-1000 kg m −3, where ρ(S,T) is the density of a sample of seawater at temperature T and salinity S, measured in kg m −3, at standard atmospheric pressure.

  5. Potential density - Wikipedia

    en.wikipedia.org/wiki/Potential_density

    The potential density of a fluid parcel at pressure is the density that the parcel would acquire if adiabatically brought to a reference pressure , often 1 bar (100 kPa). Whereas density changes with changing pressure, potential density of a fluid parcel is conserved as the pressure experienced by the parcel changes (provided no mixing with ...

  6. Oceanic physical-biological process - Wikipedia

    en.wikipedia.org/wiki/Oceanic_physical...

    Due to the higher density of sea water (1,030 kg m −3) than air (1.2 kg m −3), the force exerted by the same velocity on an organism is 827 times stronger in the ocean. When waves crash on the shore, the force exerted on littoral organisms can be equivalent to several tons.

  7. Haline contraction coefficient - Wikipedia

    en.wikipedia.org/wiki/Haline_contraction_coefficient

    Τhe haline contraction coefficient is defined as: [1] = |, where ρ is the density of a water parcel in the ocean and S is the absolute salinity.The subscripts Θ and p indicate that β is defined at constant potential temperature Θ and constant pressure p.

  8. Displacement (ship) - Wikipedia

    en.wikipedia.org/wiki/Displacement_(ship)

    To calculate the weight of the displaced water, it is necessary to know its density. Seawater (1,025 kg/m 3) is more dense than fresh water (1,000 kg/m 3); [5] so a ship will ride higher in salt water than in fresh. The density of water also varies with temperature.

  9. Neutral density - Wikipedia

    en.wikipedia.org/wiki/Neutral_density

    The neutral density ( ) or empirical neutral density is a density variable used in oceanography, introduced in 1997 by David R. Jackett and Trevor McDougall. [1] It is a function of the three state variables ( salinity , temperature , and pressure ) and the geographical location ( longitude and latitude ).