Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ Ocean Science © Author(s) 2010. This work is distributed under the Creative Commons Attribution 3.0 License.
Thermodynamic properties of sea air
R. Feistel1, D. G. Wright2, H.-J. Kretzschmar3, E. Hagen1, S. Herrmann3, and R. Span4 1Leibniz Institute for Baltic Sea Research, 18119 Warnemunde,¨ Germany 2Bedford Institute of Oceanography, Dartmouth, NS, Canada 3Department of Technical Thermodynamics, Zittau/Gorlitz¨ University of Applied Sciences, 02763 Zittau, Germany 4Lehrstuhl fur¨ Thermodynamik, Ruhr-Universitat¨ Bochum, 44780 Bochum, Germany Received: 6 August 2009 – Published in Ocean Sci. Discuss.: 13 October 2009 Revised: 4 January 2010 – Accepted: 13 January 2010 – Published: 1 February 2010
Abstract. Very accurate thermodynamic potential functions 1 Introduction are available for fluid water, ice, seawater and humid air cov- ering wide ranges of temperature and pressure conditions. In meteorology and oceanography, many standard textbooks They permit the consistent computation of all equilibrium present the thermodynamic properties of moist air, seawater properties as, for example, required for coupled atmosphere- or ice in the form of a collection of independently determined ocean models or the analysis of observational or experimen- correlation equations for selected quantities (e.g., Gill, 1984; tal data. With the exception of humid air, these potential Emanuel, 1994; Seinfeld and Pandis, 1998; Millero, 2001; functions are already formulated as international standards Jacobson, 2005) or by means of meteorological charts such released by the International Association for the Properties of as the Stuve¨ diagram, the emagram or the tephigram (Rogers Water and Steam (IAPWS), and have been adopted in 2009 and Yau, 1989). Often, some of these equations rely on cer- for oceanography by IOC/UNESCO. tain simplifications (e.g., ideal gas, constant heat capacity, In this paper, we derive a collection of formulas for im- constant latent heat); their uncertainty, completeness, mutual portant quantities expressed in terms of the thermodynamic consistency or range of validity is not always clearly stated. potentials, valid for typical phase transitions and composite The particular selection chosen may depend on personal pref- systems of humid air and water/ice/seawater. Particular at- erences of the author over various alternative empirical for- tention is given to equilibria between seawater and humid air, mulas available from the scientific literature. Although the referred to as “sea air” here. In a related initiative, these for- air-sea interface forms the largest contribution to the atmo- mulas will soon be implemented in a source-code library for spheric boundary layer, meteorological equations which ac- easy practical use. The library is primarily aimed at oceano- count for the ocean’s salinity are comparatively scarce and graphic applications but will be relevant to air-sea interaction apparently considered to be of marginal interest. Explicit for- and meteorology as well. mulas for fundamental quantities such as entropy are often The formulas provided are valid for any consistent set of missing (McDougall and Feistel, 2003; Pauluis et al., 2008). suitable thermodynamic potential functions. Here we adopt Even if mathematical expressions for enthalpy, entropy or potential functions from previous publications in which they chemical potential are available, without an explicit speci- are constructed from theoretical laws and empirical data; fication of their freely adjustable constants it is difficult to they are briefly summarized in the appendix. The formulas compare the results from different formulas or to consistently make use of the full accuracy of these thermodynamic poten- combine one with another (Feistel et al., 2008b). tials, without additional approximations or empirical coeffi- An alternative, systematic, theoretically more elegant and cients. They are expressed in the temperature scale ITS-90 satisfactory concept is the construction and evaluation of and the 2008 Reference-Composition Salinity Scale. thermodynamic potentials, as demonstrated by IAPWS1 in the form of its releases on fluid water (IAPWS, 2009a), ice (IAPWS, 2009b) and seawater (IAPWS, 2008). On this
Correspondence to: R. Feistel 1IAPWS: The International Association for the Properties of ([email protected]) Water and Steam, http://www.iapws.org.
Published by Copernicus Publications on behalf of the European Geosciences Union. 92 R. Feistel et al.: Thermodynamic properties of sea air basis, together with IAPWS, the SCOR2/IAPSO3 Working The short term “sea air” is used in this paper to refer to sys- Group 127 (WG127) on Thermodynamics and Equation of tems composed of humid air and seawater, freshwater or ice State of Seawater in cooperation with UNESCO-IOC4 devel- in mutual thermodynamic equilibrium, e.g. modelling prop- oped a proposal for a new international standard for oceanog- erties of a system including the ocean surface mixed layer raphy, TEOS-105 (IOC, 2010), which has replaced the cur- and the marine atmospheric boundary layer. In addition to rently valid 1980 International Equation of State of Seawa- the three thermodynamic potentials for fluid water, ice and ter (EOS-80, Fofonoff and Millard, 1983) after almost three seawater endorsed by IAPWS, potential functions for dry decades without formal updates to account for progress in air and virial coefficients for air-vapour interaction are re- this field (Feistel, 2008a, b; Feistel et al., 2008b; IAPWS, quired for the construction of a potential function for humid 2008a; IOC, 2009). air. These formulas are available from the literature as dis- All available accurate experimental thermodynamic data cussed later and are used here to construct the desired po- for a given substance can be suitably combined with each tential function. An IAPWS document on this formulation is other for the construction of a single mathematical func- in preparation (IAPWS, 2010). Combined, these four poten- tion, the thermodynamic potential (Gibbs, 1873; Fofonoff, tials permit the computation of thermodynamic properties of 1962; Feistel, 1993; Pruppacher and Klett, 1997; Tillner- the atmosphere, the ocean, clouds, ice and lakes in a com- Roth, 1998; Alberty, 2001; Hantel and Mayer, 2006; Alek- prehensive and consistent manner, valid over wide ranges in sandrov and Orlov, 2007; Feistel, 2008a; Herrmann et al., temperature, pressure and concentrations, from polar cirrus 2009; IOC, 2010), from which all thermodynamic proper- clouds at high altitudes to saline estuaries in the tropics, with ties can be derived analytically or numerically. Moreover, the highest accuracy presently available. Rather than being if the potential functions of different substances obey cer- a mere theoretical exercise, these four independent functions tain mutual consistency requirements (Feistel et al., 2008b), and numerous properties derived thereof are available from any mixtures, phase equilibria or composite systems can ad- a numerical source-code library which has currently been ditionally be described this way by rigorous thermodynamic developed, supporting the implementation of the intended methods, i.e. by appropriate algebraic combinations of par- new oceanographic TEOS-10 standard (Feistel et al., 2009; tial derivatives of the potential functions. Wright et al., 2009). The library will be available in Fortran For practical use in oceanography and meteorology, Gibbs and Visual Basic/Excel for easy use on various platforms. functions g(T , P) are the most convenient potentials because Later, versions in Matlab and C/C++ are also planned. they provide all properties as functions of temperature T and The mathematical forms of the four thermodynamic po- pressure P which are directly available from measurements tentials are briefly described in the appendix. In Sects. 3 (Tillner-Roth, 1998). If the range of validity includes a phase to 9, exploiting those potentials, mathematical formulas and transition region, Gibbs functions possess multiple values in relations are given for the computation of properties of hu- the vicinity of the phase transition line in the T −P diagram mid air and its equilibria with liquid water, ice and seawater. (Kittel, 1969; Stanley, 1971). Helmholtz functions f (T , ρ) These formulas are rigorous thermodynamic relations; they depending on temperature and density ρ are single-valued will remain valid even if the particular potential functions are even in this case and are therefore the preferred numerical updated in the future with new numerical coefficients or dif- formulation in such regions of parameter space. Enthalpy ferent algebraic structures. h(s, P) as a function of entropy s and pressure is particularly The flux of water vapour from the oceans into the air is useful for the description of adiabatic (isentropic) processes the main source of moisture for the atmospheric branch of (Feistel and Hagen, 1995; McDougall, 2003; Pauluis et al., the hydrological cycle, in which the moisture is carried by 2003; Feistel, 2008a), e.g. for the computation of potential large-scale atmospheric circulation patterns. Via precipita- temperature (v. Helmholtz, 1888; v. Bezold, 1888; Helland- tion, a great part returns directly to the ocean or indirectly Hansen, 1912; Rogers and Yau, 1996; McDougall and Feis- as riverine run-off from the continents. Spatial patterns of tel, 2003). All these potential functions are mathematically evaporation, precipitation, river discharge and overall runoff and physically equivalent; the choice of which to use depends vary substantially over time, and the oceanic circulation ad- on application requirements or numerical simplicity. justs to close the freshwater cycle on the global scale. The global freshwater balance controls the distribution of salin- ity which, via internal pressure gradients, constitutes a main driving factor for the circulation of the world ocean. Re- 2SCOR: Scientific Committee on Oceanic Research, http:// www.scor-int.org. gional exchange processes at the ocean-atmosphere interface 3IAPSO: International Association for the Physical Sciences of depend essentially on the redistribution of thermohaline wa- the Ocean, http://iapso.sweweb.net. ter properties by oceanic currents. As sufficiently advanced 4IOC: Intergovernmental Oceanographic Commission, http:// global coupled ocean-atmosphere models become available, ioc-unesco.org the remotely observed sea-surface temperature (SST) is be- 5TEOS-10: International Thermodynamic Equation of Seawater ing treated as an internal system variable rather than being 2010, http://www.teos-10.org. formulated as a boundary condition of either an atmospheric
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic properties of sea air 93 or an oceanic climate model; it is thus becoming one of the equilibrium properties of sea air with some observations of most useful and sensitive indicators for the correctness of the marine atmosphere. The appendix summarizes the details such models. Fully coupled atmosphere-ocean general cir- of the different thermodynamic potential functions, formulas culation and ice-sheet models are presently the most impor- for properties derived thereof, conversion tables between the tant tools to understand the dramatic climatic impact on at- partial derivatives of different potentials and, for reference, mospheric water content, cloud formation, ice cover and sea simplified potential functions in the ideal-gas limit. Note that level in the past and future (Trenberth et al., 2001; Lunt et al., this limit implies pressure-independent but not necessarily 2008). The feedback associated with changes in atmospheric temperature-independent heat capacities (Landau and Lifs- water content is a key process that must be accounted for in chitz, 1987). For the humid-air potential that is published predictions of global warming (Willett et al., 2007; Dressler in this form for the first time in this paper, tables with nu- et al., 2008). merical check values are provided for the verification of the A consistent description of the fluxes of seawater vapour correctness of its implementations or modifications. and latent heat, which continually pass across the ocean- To use an approach and nomenclature that are consistent atmosphere interface on different spatial and temporal scales, with oceanographic practice, some equations developed here is indispensable for models dealing with the coupled ocean- differ slightly from common meteorological practice. Pure atmosphere system. All thermodynamic quantities associ- water serves as the general reference substance, in the ocean ated with such fluxes must be formulated consistently on in liquid form, in the atmosphere in its vapour phase. Dis- both sides of the sea surface. While transport properties solved in or mixed with this fluid water are sea salt and dry themselves cannot directly be computed from the equilib- air, both being natural mixtures of various chemical species, rium properties summarized in this paper, the deviation of described by the absolute salinity, SA, as the mass fraction of measured or modelled conditions from those equilibrium salt in seawater, and the mass fraction of dry air, A, in humid properties represent the system’s distance from equilibrium air, including the limiting cases of freshwater (SA=0), dry air and estimate the thermodynamic Onsager forces (Glansdorff (A=1) or air-free vapour (A=0). and Prigogine, 1971; De Groot and Mazur, 1984) driving the The dissolution of air in water or seawater is always ne- irreversible fluxes. Consequently, standard formulas which glected in this paper. Also, problems related to metastable use measurable parameters to estimate the physical fluxes states, supersaturation or nucleation processes are not con- of energy, heat, water, or salt at the sea surface are based sidered. The fallout of condensed water or ice from the on equilibrium properties of seawater and humid air (Stull, real atmosphere depends on certain conditions such as the 2003; Weller et al., 2008). For example, the correspond- droplet size distribution. This precipitation problem is ex- ing bulk formulas for the ocean-atmosphere latent heat flux cluded from our theoretical model; in this paper we consider (Weare et al., 1981; Baosen, 1989; Wells and King-Hele, thermodynamic phase equilibria of gravity-free composite 1990) are more correctly expressed in terms of the sea-air systems regardless of the shape of the phase boundaries. specific humidity at the condensation point (Sects. 6, 12) The chemical composition of sea-salt, Table A1, is consid- rather than of saturated humid air. Measurements of the evap- ered as constant, as described by Millero et al. (2008). The oration rate of seawater at different salinities were made re- chemical composition of air, Table A2, is assumed to be fixed cently by Panin and Brezgunov (2007). as described by Picard et al. (2008), although only the per- In Sect. 2, with regard to ocean-atmosphere interaction, manent constituents of air are considered here except for the we first briefly review several vapour-pressure formulas and variable water vapour content. The symbol for pressures is equations for humid air. In Sect. 3, the IAPWS Release 2008 P with corresponding superscripts. Thus, for example, we for seawater is explained. Some recent formulations for dry use P V for the partial pressure of water vapour rather than e air are discussed in Sect. 4. The generalisation for humid as often used in meteorological texts. The symbol s is used air follows in Sect. 5. The composite system of humid air for the specific entropy rather than φ (as in the word “tephi- in equilibrium with seawater (sea air) is analyzed in Sect. 6. gram” which refers to the T -φ diagram, where φ refers to Its special case of vanishing salinity, i.e. the equilibrium be- specific entropy). Consistent with oceanography, the adia- tween pure water and saturated air is described in Sect. 7, batic lapse rate 0 is defined here as the isentropic tempera- in particular the saturation of air with respect to liquid water. ture change with respect to pressure rather than with respect Below the freezing point of seawater, ice appears in sea air as to altitude, 0 = (∂T /∂P )s, thus being immediately available a third phase; in Sect. 8 extended formulas are discussed that from e.g. the related Gibbs function as an intrinsic thermo- account for the presence of ice, and in Sect. 9 we consider dynamic property of air, independent of non-thermodynamic the related zero-salinity limit, “ice air”. In Sect. 10 we dis- parameters such as gravity or distance. cuss different definitions of relative humidity and derive its Regarding the terminology of adiabatic processes and equilibrium value for the sea surface. Introducing enthalpy lapse rates, consistent with Pruppacher and Klett (1997), we as a potential function in Sect. 11, we consider the properties refer to the lapse rate of dry air as “dry adiabatic”, of un- of a well-mixed, isentropic atmosphere in local equilibrium saturated humid air as “moist adiabatic”, of wet air (parcels with the sea surface. In the discussion, Sect. 12, we compare containing humid air and liquid water) as “wet adiabatic” and www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 94 R. Feistel et al.: Thermodynamic properties of sea air of ice air (parcels containing humid air and solid ice) as “ice The most recent and most accurate equation of state for adiabatic”. This is in contrast to textbooks such as Jacob- moist air near atmospheric pressure is the CIPM7-2007 for- son (2005) which, to some extent confusingly, link “dry” adi- mula (Picard et al., 2008), replacing its predecessor known abatic lapse rates to unsaturated moist air, and “moist” adi- as the CIPM-81/91 equation (Giacomo, 1982; Davis, 1992) abatic lapse rates to saturated parcels which condense water in particular for its corrected value of the Argon fraction. and warm up due to latent heat release during uplift. CIPM-2007 is valid in the range 0.06–0.11 MPa and 15– If not explicitly mentioned otherwise, all equations are ex- 27 ◦C for relative humidity 0–100%. Its relative combined pressed in the temperature scale ITS-906 (Preston-Thomas, standard uncertainty in density is estimated to be 22 ppm 1990) and in the new oceanographic Reference-Composition (10−6). The formulation of Hyland and Wexler (1983b) Salinity Scale (Millero et al., 2008; IOC, 2010) in g kg−1 covers dry air at 173.15–473.15 K and humid air at 173.15– rather than in Practical Salinity on the 1978 scale. As usual in 372.15 K at pressures up to 5 MPa. For an accurate construc- meteorology, in several figures the absolute pressure is given tion of humid-air formulations from separate equations for in units of hPa=100 Pa. dry air and for water vapour, Harvey and Huang (2007) re- calculated the second virial coefficient of H2O-air interaction by evaluating the statistical configuration integral. Earlier 2 Available formulations for dry air, humid air, and the second and also third virial coefficients for H2O-air-air and vapour pressure over water, seawater, or ice H2O-H2O-air three-particle interactions are available from Hyland and Wexler (1983b). In this paper we use these sec- Standard textbooks (Gill, 1983; Jacobson, 2005) provide sets ond and third cross-virial coefficients in combination with of various separate correlation equations for relevant thermo- Helmholtz functions for dry air from Lemmon et al. (2000) dynamic properties of the atmosphere such as the heat ca- and for water vapour from IAPWS-95 (Appendix D; IAPWS, pacity, the lapse rate or the latent heat. The estimated uncer- 2010). tainties in the proposed ideal-gas formulations for the den- Thermodynamic properties of water vapour including air- sity of dry and humid air are less than 0.2% under typical free saturation conditions are available from the IAPWS-95 atmospheric temperature and pressure conditions (Jacobson, formulation in the range 130 K–1273 K and pressures up to 2005). 1000 MPa in the form of a Helmholtz function. A correc- A Helmholtz function for dry air was published by Lem- tion term additional to the ideal-gas part of IAPWS-95 below mon et al. (2000), representing experimental data in the range 130 K is proposed in Appendix C of this paper, extending its 0–70 MPa and 60–873 K (reasonably predicting properties validity to 50 K, for consistency with the latest formulas for even up to 2000 MPa and 2000 K) as an extended revision the sublimation pressure and the sublimation enthalpy of ice of the previous equation by Jacobsen et al. (1990), com- Ih (Feistel and Wagner, 2007; IAPWS, 2008b). pleting it with the ideal-gas contributions for the major air constituents. The most recent ideal-gas heat capacities are An industrial humid-air description, intended for applica- available from Helmholtz function formulations for Nitrogen tions at elevated pressure and temperature, was recently pro- (Span et al., 2000, quantum rigid rotor model for 20–500 K posed by Aleksandrov and Orlov (2007), based on the dry- with 0.01% uncertainty), Oxygen (Stewart et al., 1991, from air equation of Lemmon et al. (2000) in conjunction with experimental data at 30–3000 K with a maximum deviation the IAPWS Industrial Formulation IF97 (Wagner and Kret- of 0.003 J mol−1 K−1) and Argon (Tegeler et al., 1999, us- zschmar, 2008) for fluid water and an earlier equation for ice (Feistel and Wagner, 2005), although without including virial ing the constant isobaric heat capacity cAr,id = 2.5R with an P coefficients for air-water interaction. The approach of Nelson uncertainty below 0.01% up to 10 000 K). Another equation and Sauer (Gatley, 2005) is similar. The “SKU” model of for oxygen is available from Wagner and de Reuck (1987). Herrmann et al. (2009c, 2010) also is an ideal-mixture com- We choose to use the more recent formulation of Lemmon bination of the real-gas formulation of Lemmon et al. (2000) et al. (2000) which combines the properties of the differ- with IAPWS (2009a) for water vapour (ideal mixtures are ent air constituents including their ideal-gas parts, and is models which may consider non-ideal properties of the pure expressed on the ITS-90 scale. Experimental data for the components but neglect any interaction between the parti- heat capacity of air were published by Henry (1931) at atmo- cles of different chemical species). Herrmann et al. (2009c) spheric pressure for the temperature range 20–370 ◦C, and by provide an extensive comparison of different humid-air equa- Magee (1994) for 67–300 K at pressures up to 35 MPa. The tions and experimental data. different formulas and data available are reviewed in great detail by Lemmon et al. (2000). Millero (2001, p. 291) provides a vapour pressure for- mula for seawater that uses the pure-water vapour pressure of Ambrose and Lawrenson (1972) with a pressure-independent three-term salinity correction. The related table for practical
6ITS-90: International Temperature Scale of 1990, www.bipm. 7CIPM: International Committee for Weights and Measures, org/en/publications/its-90.html. www.bipm.org/en/committees/cipm/.
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic properties of sea air 95 salinity SP=35 refers to Millero and Leung (1976), who smoke by differential evaporation and condensation is con- provide a different, two-term salinity correction. The tem- trolled by the so-called Kohler¨ equation (Kohler,¨ 1936; Sein- perature scale can be assumed to be IPTS-688, the salin- feld and Pandis, 1998; Jacobson, 2005). This relaxation pro- ity scale is PSS-789. No uncertainty estimate is given. cess is similar to the Ostwald ripening of nuclei that emerge Kennish (2001, p. 62) provides a table with reference to along with phase transitions of the first kind (Ostwald, 1896; Millero (1996), which probably means the same formula Schmelzer and Schweitzer, 1987), as e.g. encountered in as given in Millero (1983) and Millero (2001). The earlier cloud formation processes (Rogers and Yau, 1989; Prup- edition of the CRC Handbook of Marine Science (Walton pacher and Klett, 1997; Hellmuth, 2006). In this paper we Smith, 1974, p. 49) reported the vapour pressure lowering do not consider the specific properties of aerosols or simi- of seawater from Robinson (1954) and Arons and Kient- lar systems that are essentially influenced by surface-tension zler (1954). The formula is pressure-independent. Siedler effects. and Peters (1986, p. 252) refer to Millero (1983), who in turn Consistent with the Releases of IAPWS (2008b, 2009a, provides the same formula as Millero (2001). Gill (1982) 2009b), valid over the full range of ambient temperatures in- refers to empirical formulas of List (1951) and Kraus (1972) cluding conditions in the high atmosphere at high latitudes, for the vapour pressure over water and seawater. Dietrich et the vapour pressure over ice (i.e., the sublimation pressure) al. (1975, p. 68) provide a graph for the vapour pressure low- was compiled by Feistel and Wagner (2007) and is available ering based on measurements of Higashi et al. (1931) and from an IAPWS Release (IAPWS, 2008b). The vapour pres- Arons and Kientzler (1954). No uncertainty estimates are sure over sea ice (i.e. ice in equilibrium with brine pockets) given and the temperature and salinity scales are not speci- and its relation to the brine salinity is discussed in Sect. 8. fied. The formula is pressure-independent. As is evident from this brief review, numerous different Linke and Baur (1970, p. 476) provide a standard mete- formulas are in practical use for the particular properties of orological formula that is attributed to G. Hofmann (with- water, seawater and air, on different temperature scales, with out giving the reference, which probably is Hofmann, 1955, different accuracies and over different ranges of validity, with 1956) for pure water with a linear salinity correction from uncertain completeness or mutual consistency. Quantitative Defant (1961, p. 45). The latter in turn uses results from information is scarce about fundamental quantities such as Witting (1908) without specifying that reference. No uncer- entropy or enthalpy of humid air, or the latent heat of sea- tainty estimates are given, the temperature and salinity scales water. In this paper we propose to replace this inhomoge- are not reported, and the formula is pressure-independent. neous collection by consistent, thermodynamically rigorous Tetens’ (1930) formula for the saturated vapour pressure is formulas derived from a minimum set of comprehensive and also common in meteorology; a recent update was recom- most accurate thermodynamic potentials of fluid water, ice, mended by Bolton (1980). A review of vapour-pressure for- seawater (Feistel, 2008a, b; Feistel et al., 2008b) and humid mulas over pure water and ice was given by Sonntag (1982) air which provide all thermodynamic equilibrium properties with explicit conversion to the IPTS-68 temperature scale; of those substances as well as their combinations and mu- the effect of the conversion to ITS-90 on the saturation tual phase equilibria over a wide range of conditions. When vapour pressure was analysed by Sonntag (1990). Saturated an official standard formulation for humid air becomes avail- vapour pressure data and formulae since 1740 were reviewed able which covers wider ranges of conditions than the present by Sonntag (1998) who expressed his regret regarding the CIPM-2007 formula (Picard et al., 2008), the building-block lack of internationally recognised meteorological standards concept proposed here will permit its easy incorporation into for these properties. For very accurate vapour pressure for- the suggested system of equations derived by thermodynamic mulas such as that of Weiss and Price (1980) for seawater, rules. based on Robinson’s (1954) careful experiments, the tem- Simple correlation functions for particular thermodynamic perature conversion to the recent ITS-90 temperature scale properties have advantages for certain purposes; they are is essential (Feistel, 2008a). An early review on seawater easy to use and numerical implementations execute quickly. evaporation was published by Montgomery (1940). Formu- The comprehensive formulation proposed in this paper can las used for the latent heat in numerical ocean models are provide error estimates and validity limits for such existing given by Smith (1988); simple expressions for the evapo- formulas. For high-speed applications, it can be used to de- ration and sublimation heat as functions of temperature are rive from its computed data points tailored, very accurate and available from Gill (1982). consistent new correlation equations. The time it takes to Various properties of marine aerosols are reviewed by determine tailored formulae or to compute and store tabu- O’Dowd et al. (1997) and Seinfeld and Pandis (1998). The lated values in look-up tables is irrelevant for their later us- adjustment of the equilibrium droplet size distribution of sea age. The sea-air functions implemented in the library (Feis- tel et al., 2009; Wright et al., 2009) permit the computation 8IPTS-68: International Practical Temperature Scale of 1968 of look-up tables for practically any desired combination of (Goldberg and Weir, 1992). input and output properties, since the thermodynamic po- 9PSS-78: Practical Salinity Scale 1978 (Unesco, 1981). tentials provide a complete description. Real-time models www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 96 R. Feistel et al.: Thermodynamic properties of sea air require the highest computation speeds; so, we believe that In particular for the description of phase equilibria with sea- our equations may well feed such models with the most ac- water, partial specific properties are conveniently derived curate properties available. However, we recognize that for from the Gibbs function. If, for example, H SW is the en- particular applications such as in oceanographic or climate thalpy of a sample of seawater that contains the masses mW models, computation (or look-up) speed may be critical, too. of water and mS of salt, respectively, the partial specific en- SW thalpy HW of water in seawater is defined by (Glasstone, 1947) 3 Helmholtz and Gibbs functions of fluid water, ice and ! seawater ∂H SW H SW = . (3.6) W ∂mW The new standard formulation for thermodynamic properties mS,T ,P of seawater developed cooperatively by the SCOR/IAPSO S W S WG 127 (Feistel, 2008a; IOC, 2010) and IAPWS (2008) con- Transformation to the absolute salinity, SA = m /(m +m ), S SW = SW W + S sists of the saline part of the Gibbs function, g (SA, T , P) and the specific enthalpy, h H /(m m ), yields for which describes the salinity correction to the specific Gibbs the partial specific enthalpy the expression energy of pure liquid water that can be derived from the ! ∂hSW ∂S Helmholtz potential for fluid (i.e. liquid and gaseous) wa- H SW = hSW + mW +mS A W W (3.7) Ih ∂SA ∂m S ter, and a Gibbs function g (T , P) for ice (IAPWS, 2009a, T ,P m 2009b; Feistel et al., 2008b). Mathematical details of those SW ! SW ∂h correlation functions are given in the appendix. = h −SA . SW ∂SA The Gibbs function of seawater, g , T ,P gSW (S ,T,P ) = gW (T,P )+gS (S ,T,P ), (3.1) SW A A By means of Eqs. (3.5) and (3.7), HW is computed from the Gibbs function of seawater. Since H SW depends on one as a function of absolute salinity S , absolute temperature T W A freely adjustable constant (see Appendix E), the absolute en- and absolute pressure P refers to a Gibbs function of water, ergy of water, only differences between partial specific en- gW, as its zero-salinity limit, and a saline part, gS, which thalpies rather than their absolute values can be measured is explicitly available from IAPWS (2008). Rather than in thermodynamic experiments. With respect to different the Gibbs function gW, the IAPWS-95 standard provides a phases that contain water, an important example for such a Helmholtz function for fluid water, f F (T ,ρ), depending on difference is the latent heat of the related phase transition. temperature and density. Below the critical temperature, the If the Gibbs energy GSW of seawater is used in Eq. (3.6) related equation for the pressure, rather than H SW, then the related result (3.7) is the partial ∂f F specific Gibbs energy of water in seawater which equals the P = ρ2 (3.2) ∂ρ chemical potential of water in seawater (Landau and Lifs- chitz, 1987; IOC, 2010). has two different inverse functions of practical relevance, one The freely adjustable constants representing the absolute for the liquid density, ρW (T,P ), and one for the vapour energy and entropy of water and sea salt are specified by the density, ρV (T,P ), which can be computed iteratively from reference state conditions of vanishing internal energy and Eq. (3.2). With this liquid density, the Gibbs function of liq- entropy of liquid water at the triple point and zero entropy uid water is obtained from and enthalpy of seawater at the standard ocean state (Feis- tel et al., 2008b). The related terms of the Gibbs functions W = F W + W g (T,P ) f T ,ρ P /ρ , (3.3) which are determined by these conditions are independent of pressure and of order 0 and 1 in temperature and salinity, V and similarly for the Gibbs function of water vapour, g . respectively (Fofonoff, 1962; Feistel and Hagen, 1995). Together with gS available from the IAPWS Release 2008, Eq. (3.3) provides the full Gibbs function (3.1) of seawater, gSW, from which all thermodynamic properties of seawater 4 Helmholtz function for dry air are available by thermodynamic rules, as e.g. the entropy Air is a mixture of gases, Table A2, as described recently by ! ∂gSW Picard et al. (2008), with only minor variability of its com- sSW (S ,T,P ) = − (3.4) A ∂T position under ambient conditions. A Helmholtz function for SA,P dry air was published by Lemmon et al. (2000) in the form of A,mol mol or the enthalpy, the molar Helmholtz energy, f T ,ρ , depending on mol ! absolute temperature T (ITS-90) and molar air density, ρ . ∂gSW hSW (S ,T,P ) = gSW +T sSW = gSW −T (3.5) For consistency with the description of water and seawater, A ∂T S,P we will use in this paper the specific (rather than the molar)
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic properties of sea air 97
Helmholtz energy, f A, as the thermodynamic Helmholtz po- provides accurate results for higher densities if mA mV or tential, mV mA where the contributions from one component are strongly dominating and contributions from 4th and higher F A 1 ρA f A T ,ρA = = f A,mol T, , (4.1) order cross-virial terms remain negligible. The absence of mA MA,L MA,L these higher cross-virial coefficients will not relevantly af- fect the accuracy of Eq. (5.1) for meteorological applications A A which depends on the mass density of dry air, ρ = m /V . because of the smallness of non-ideal effects, Fig. 1, under For consistency we use in the conversion (4.1) the original natural atmospheric conditions of temperature, pressure and estimate of the molar mass of dry air given by Lemmon et humidity. A,L −1 al. (2000), M =28.958 6(2) g mol , rather than the latest Defining the mass of humid air by mAV = mA + mV and A −1 estimate by Picard et al. (2008), M =28.965 46 g mol (Ta- the mass fraction of dry air by A = mA/mAV, we find for the A ble A2). In Eq. (4.1), m is the mass of air contained in the Helmholtz function of humid air the expression volume V , and F A is the (extensive) Helmholtz energy of this air sample. F AV f AV A,T ,ρAV = =(1−A)f V T,(1−A)ρAV (5.2) The Helmholtz function (4.1) for dry air adopted from mAV Lemmon et al. (2000) is defined in Eq. (B1) in the Ap- A(1−A)RT +Af A T ,AρAV +2ρAV pendix. The absolute energy and the absolute entropy of MAMW dry air is specified here by the reference-state condition of 3 A (1−A) B (T )+ ρAV C (T )+ C (T ) vanishing entropy and enthalpy at the standard ocean state, AW 4 MA AAW MW AWW T0=273.15 K, P0=101 325 Pa. The related freely adjustable terms of f A(T , ρA) are independent of ρA and multiply Here, ρAV = mAV/V is the density of humid air, q = 1−A = powers 0 and 1 in T . mV/mAV is its specific humidity, (1−A)ρAV = mV/V is its Various thermophysical properties of dry air are available absolute humidity, and r = (1−A)/A = mV/mA is the hu- from the formulas given in the following section for the lim- midity ratio or mixing ratio (van Wylen and Sonntag, 1965; iting case of vanishing humidity. Gill, 1982; Emanuel, 1994; Pruppacher and Klett, 1997). The relation to relative humidity is given in Sects. 7 and 10, and Fig. 14 therein. 5 Helmholtz and Gibbs functions for humid air Later in this text, we will frequently omit for simplicity of the formulae the superscript AV at the density of humid air, The Helmholtz function f V T ,ρV of water vapour is avail- ρAV ≡ ρ, if there is no risk of confusion. able from the IAPWS-95 formulation, Sect. 3 and Ap- The use of A rather than q as the composition variable pendix C, and that of dry air, f A T ,ρA, from Appendix B of humid air is not common. This somewhat unfamiliar de- and Eq. (4.1) above. If a mass mV of vapour is mixed with cision was made independently of the typical ambient mass a mass mA of dry air in a volume V , the virial expansion ratios (q 1). The formalisms used here are very similar for of the Helmholtz energy F AV of the humid-air system up to the ocean and the atmosphere. Water in its three phases forms three-particle vapour-air interactions reads (Appendix D), the reference system; in particular its two fluid phases are de- mV mA scribed by one and the same Helmholtz potential (IAPWS- F AV mV,mA,T,V = mVf V T, +mAf A T, (5.1) V V 95) for rigorous consistency between ocean and atmosphere. RT mAmV 3 mA mV Thus, as in nature, also in this theoretical model the water is +2 B (T )+ C (T )+ C (T ) V MAMW AW 4V MA AAW MW AWW exactly “the same” on both sides of the sea surface. Added to these fluid phases of water are natural mixtures of almost In Eq. (5.1), R is the molar gas constant, and MA, MW constant composition, sea salt in the liquid and dry air in the are the molar masses of air and water, respectively. The gas phase. For these additives, their pure properties are de- second molar virial coefficient BAW(T ) is available from scribed and corrected by a density expansion with respect to Harvey and Huang (2007), and the third molar virial coef- their interaction with water. As a result, the equations for hu- ficients CAAW(T ) and CAWW(T ) of air-vapour interaction mid air look very similar to those of seawater if just the mass are reported by Hyland and Wexler (1983b). We note that fraction A of the one additive is exchanged with the other, V A the Helmholtz functions f and f that we have chosen to SA. use in Eq. (5.1) are complete expressions rather than expan- The Helmholtz potential (5.2) is formally a symmetric sions in terms of powers of density; consequently, they in- function in the fractions of air and of vapour. Its validity clude contributions corresponding to higher powers of den- is not restricted to small specific humidity, q = (1−A), such sity than included in the cross-virial terms represented by the as some 1–3% often assumed for empirical equations used in third term, see Appendix D. Eq. (5.1) is thus an inhomoge- meteorology; see for example Figs. 3 and 13 in the follow- neous approximation formula with respect to the powers of ing sections. Equation (5.2) can therefore be applied even density and the related correlation clusters. This approach to physical situations in which dry air is the minor fraction, www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 13 with respect to the particular density arguments of those functions, rather than derivatives 98with respect to the total density of humid air, ρAV , in Eq. (5.7). R. Feistel et al.: Thermodynamic properties of sea air
Non-Ideal Behaviour of Dry Air 0.03 P ρAV ∂f AV Z = = , AV AV AV (5.3) 0.02 ρ RAVT RAVT ∂ρ A,T - 1 Z 0.01 where RAV is the (effective) specific gas “constant” of humid air, as a function of the air fraction A,
0 R 1−A A 0.1 MPa R = = R + = ( −A)R +AR AV AV W A 1 W A -0.01 M M M (5.4)
CompressibilityFactor 1 MPa 10 MPa -0.02 and MAV its mean molar mass,
-0.03 −1 -80 -60 -40 -20 0 20 40 60 80 AV AV W AV A 1−A A Temperature14 t /°C M = xV M + 1−xV M = + , MW MA Non-Ideal Effect of Humidity (5.5) 0.001 AV 0 where the mole fraction xV of vapour is given by 10 MPa -0.001 (1−A)/MW r
(dry) AV 1 MPa -0.002 x = = . (5.6) Z V − W + A + W A -0.003 (1 A)/M A/M r M /M
(sat) - -0.004 The deviation of the compressibility factor ZAV, as defined in Z -0.005 Eq. (5.3), from unity is shown in Fig. 1 for dry and saturated -0.006 air for several values of T and P . Selected values for ZAV -0.007 are reported by Pruppacher and Klett (1997). The compress-
Difference -0.008 ibility factor Z of fluids is generally small in the vicinity of the critical point; the critical value is Zc=0.375 for the van- 0.1 MPa -0.009 der-Waals gas, 0.29 for noble gases (Guggenheim, 1967) and -0.01 -20 -10 0 10 20 30 40 50 60 70 80 90 100 0.23 for water (Stanley, 1971). In statistical thermodynam- Temperature t /°C ics, the compressibility factor is the logarithm of the grand
Fig. 1: Non-ideal behaviour ( ZAV – 1), Eq. (5.3), of dry (upper panel) and saturated (lower canonical partition function and therefore a thermodynamic AV − Fig.panel) 1.air forNon-ideal several values behaviour of T and P. (Z 1), Eq. (5.3), of dry (upper potential in terms of temperature, density and chemical po- panel) and saturated (lower panel) air for several values of T and P . tential (Landau and Lifschitz, 1987) which is regarded as
Computed from Eqs. (5.7) or (5.3), the ratio the Landau free energy or the Landau potential (Goodstein, 1975) divided by RT. such as condensersPM A AM ofW desalination+ (1− A)M A plants1+ r M A or/ M headspacesW over T = = TZ = TZ (5.8) subglacialv Rρ lakes.AV AV TheM mostW relevantAV restriction1+ r for the ac- For the total pressure of humid air we get from Eq. (5.2), compare Eq. (D11), curacyis known in of meteorology Eq. (5.2) as the isvirtual the temperature truncation of humid error air (Rogers of and the Yau, virial 1989; ex- pansion,Jacobson, 2005; i.e., Hantel its and omitted Mayer, 2006). subsequent terms proportional to AV ∂F 3 3 2 2 3 3 3 AThe (specific1−A entropy)ρ , ofA humid(1 −air Afollows) ρ fromand A(1−A) ρ must be neg- P = − (5.7) ∂V mA,mV,T ligibly small.1 Hyland∂F AV and Wexler∂f AV (1983b) require pressures sAV = − = − (5.9) AV AV ∂ ∂ 2 ∂f 2 h V i less than 5m MPa T for A saturatedV T humid air; this condition im- AV AV 2 2 A m ,m ,V A,V = ρ = ρ (1−A) f V +A f A plies limitations to the air density in dependence of the air ∂ρAV ρ ρ as A,T fraction. The comparison with experimentalRT data shown in 2 s AV = −()()1− A f V − Af A − 2A 1− A ρ AV × AV RT T T A W +A −A ρ the appendix, Fig. D1, suggestsM thatM the current formulation (1 ) A W ()− (5.10) M M B dB 3 AV A C dC 1 A C dC −3 of Eq.× (5.2)AW + canAW + safelyρ be usedAAW + upAAW to + densities AWW of+ 100AWW kg m T dT 4 M A T dT M W T dT A (1−A) of saturated humid air. Results remain reasonable beyond 2B (T )+3ρAV C (T )+ C (T ) AW MA AAW MW AWW this point, but the uncertain third and the missing fourth and higher cross-virial coefficients are clearly relevant beyond from which the partial pressure of vapour, P V, is obtained by 200 kg m−3. AV multiplication with xV (Guggenheim, 1967). The subscripts V Describing the deviation of the equation of state from on f and f A are meant as partial derivatives with respect ideal-gas behaviour, the compressibility factor Z of humid ρV ρA AV to the particular density arguments of those functions, rather air is defined as (van Wylen and Sonntag, 1965), than derivatives with respect to the total density of humid air, ρAV, in Eq. (5.7).
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Computed from Eqs. (5.7) or (5.3), the ratio A W A PM AM +(1−A)M ∂gAV TV = = TZAV (5.8) AV = AV + AV = AV − RρAV MW h (A,T,P ) g T s g T . (5.17) ∂T A,P 1+r MA/MW = TZAV AV = 1+r The specific isobaric heat capacity is cP ∂hAV/∂T = T ∂sAV/∂T . is known in meteorology as the virtual temperature of hu- A,P A,P mid air (Rogers and Yau, 1989; Jacobson, 2005; Hantel and In particular for the description of phase equilibria with humid air, partial specific properties are conveniently derived Mayer, 2006). AV The specific entropy of humid air follows from from the Gibbs function. If, for example, H is the en- thalpy of a sample of humid air that contains the masses mV 1 ∂F AV ∂f AV of vapour and mA of air, respectively, the partial specific en- sAV = − = − AV (5.9) AV m ∂T mA,mV,V ∂T A,V thalpy HV of water in humid air is defined by (Glasstone, as 1947) RT AV AV = − − V − A − − AV ∂H s (1 A)fT AfT 2A(1 A)ρ (5.10) H AV = . MAMW V V (5.18) ∂m A B dB 3 A C dC m ,T ,P × AW + AW + ρAV AAW + AAW T dT 4 MA T dT Transformation to the air fraction, A = mA/(mV + mA), and (1−A) C dC the specific enthalpy, hAV = H AV/(mV +mA), yields for the + AWW + AWW MW T dT partial specific enthalpy the expression and the specific enthalpy from Eqs. (3.3), (3.5) as ∂hAV ∂A H AV = hAV + mV +mA (5.19) AV AV AV AV V V h = f +P /ρ +T s . (5.11) ∂A T ,P ∂m mA AV AV AV ∂h Here, the functions f , P and s are available from = hAV −A . Eqs. (5.2), (5.7) and (5.10), respectively. ∂A T ,P Equation (5.10) is consistent with the air-vapour interac- By means of Eqs. (5.17) and (5.19), H AV is computed from tion terms of the virial formula for the entropy given by Hy- V the Gibbs function of humid air. land and Wexler (1983b, their Eqs. 2, 3 and 7). Exploiting the entropy (5.16), the (absolute) potential tem- The Gibbs function of humid air, gAV, follows from its perature θ AV(A,T ,P ) (in K) of humid air referenced to stan- Helmholtz function (5.2) via the Legendre transform dard pressure is obtained by solving (numerically) the equa- ∂f AV tion gAV = f AV +ρAV . AV (5.12) ∂ρ A,T AV AV AV s A,θ ,P0 = s (A,T,P ) (5.20) The function gAV can be written in terms of the chemical A potentials of air in humid air, µ , and of vapour in humid where P0=101 325 Pa. Equivalently, the potential tem- air, µV, as (Gibbs-Duhem equation, Landau and Lifschitz, perature follows from the entropy derivative of the en- 1987; Feistel and Marion, 2007; Feistel, 2008a; IOC, 2010) thalpy (5.11) of humid air (Feistel and Hagen, 1995; Feistel, 2008), as gAV = AµA +(1−A)µV (5.13) ∂hAV which obey the relations θ AV = , (5.21) ∂s ∂gAV A,P =P0 µA = gAV +(1−A) (5.14) ∂A T ,P where the right side is evaluated at the reference pressure, P = P0, and in-situ entropy. and AV The equivalent potential temperature θe is the potential ∂gAV µV = gAV −A . (5.15) temperature that a parcel of humid air would have if all its ∂A T ,P vapour were condensed and the latent heat released used to heat the parcel (Jacobson, 2005). If a mass fraction (1−A) From the Gibbs function (5.12), the entropy (5.9) is com- of liquid water with the initial temperature θ AV is irreversibly puted as e evaporated into dry air with the mass fraction A at the surface ∂gAV pressure P , the resulting humid air is cooled by this process sAV (A,T,P ) = − , (5.16) 0 to the temperature θ AV determined from, ∂T A,P W AV A AV AV AV and the enthalpy in the form, (1−A)h θe ,P0 +Ah θe ,P0 = h A,θ ,P0 , (5.22) www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 100 R. Feistel et al.: Thermodynamic properties of sea air because the enthalpy is conserved during an irreversible iso- coincides with the (partial) pressure of the gas in the ideal- baric and adiabatic process rather than the entropy (Landau gas limit. The fugacity fAV of humid air is and Lifschitz, 1987; IOC, 2010). This equation implicitly ! AV AV AV − AV,id provides the equivalent potential temperature θe A,θ g g fAV (A,T,P ) = P exp (5.28) as a function of the air fraction and the potential temperature RAVT of the original humid-air sample. From the Gibbs function (5.12), the specific volume vAV Here we have used the subscript AV on f to distinguish the AV AV and the density ρ of humid air at given T and P are com- fugacity fAV from the Helmholtz function f of humid air. puted as The pressure P is obtained from Eq. (5.7), the ideal-gas limit gAV,id is given in Eq. (H5). 1 ∂gAV vAV A,T,P = = . The fugacity is related to the compressibility factor, ZAV, ( ) AV (5.23) ρ ∂P A,T Eq. (5.3), by the differential equation (Glasstone, 1947; van Wylen and Sonntag, 1965), The parcel’s volume expansion during adiabatic uplift is ob- tained from the adiabatic compressibility, P ∂fAV P = ZAV = (5.29) 2 AV 2 1 ∂vAV ∂ h /∂P 1 fAV ∂P A,T ρRAVT κAV = − = − A,T = . (5.24) s vAV ∂P AV ρAVc2 A,s ∂h /∂P A,T AV AV Because g = f + ZAVRAVT , using Eqs. (5.3) and p (5.12), the fugacity (5.28) can be expressed in terms of Here, c = (∂P /∂ρ)A,s is the sound speed. The adiabatic lapse rate of humid air (recall that in some Helmholtz functions as literature this is referred to as the “dry” adiabatic lapse rate ! f AV −f AV,id rather than the “moist” adiabatic lapse rate) is computed from fAV (A,T,P ) = P exp +ZAV −1 . (5.30) the enthalpy (5.11) or the Gibbs function (5.12) as RAVT ! ∂T ∂2hAV ∂2gAV/∂T ∂P The fugacity of vapour in humid air is 0AV = = = − A (5.25) 2 AV 2 ∂P A,s ∂s∂P ∂ g /∂T ! A A,P µV −µV,id = AV or, by means of Table G2, from the Helmholtz function (5.2) fV (A,T,P ) xV P exp . (5.31) RWT at the given humid-air density, ρ = ρAV, as = W V f AV Here, RW R/M is the specific gas constant of water, µ 0AV = Tρ . (5.26) is given in Eq. (5.15) and its ideal-gas limit in Eq. (H13). 2 2 AV − AV AV + AV The saturation of air with vapour is defined by the equilib- ρ fTρ ρfTT 2fρ ρfρρ rium between humid air and liquid water and will be consid- Here, the subscripts of f AV indicate partial derivatives at ered in Sect. 7, i.e. as the limiting case for zero salinity of the fixed A. The deviation between the lapse rates of dry air sea-air properties derived in the next section. (A = 1) and of humid air (A < 1) in the atmosphere is usually less than 3% (Seinfeld and Pandis, 1998), in contrast to the 6 Gibbs function for sea air wet-air lapse rate, Eq. (7.19). Selected values of Eq. (5.26) computed at saturation humidity are displayed in Fig. 2. The Gibbs function gSW The adiabatic virtual-temperature lapse rate (Jacobson, SW W S 2005) follows from the pressure derivative of the virtual tem- g (SA,T,P ) = g (T,P )+g (SA,T,P ) (6.1) perature, Eq. (5.8), as ! of seawater (IAPWS, 2008a; Feistel, 2008a; Feistel et al., ∂T MA ∂ P vAV W AV = V = 2009; Wright et al., 2009) consist of a pure-water part, g , 0V (5.27) W ∂P A,s R ∂P available from the Helmholtz function f (T , ρ) given by A,s S the IAPWS-95 formulation, and a saline addition, g , ac- 1 AV 1 1 = T −κ = T − counting for the solute regarded as sea salt. Here, SA = V s V AV 2 P P ρ c mS/ mW +mS is the absolute salinity (Millero et al., 2008), Adiabatic compressibility and sound speed are given in expressed by the mass, mS, of salt dissolved in a mass of Eq. (5.24). liquid water, mW. In addition to the compressibility factor, Eq. (5.3), another In the composite system “sea air” consisting of seawater common measure for the non-ideal behaviour of gases or gas and humid air, these two phases are spatially separate and the mixtures is the fugacity (Glasstone, 1947; van Wylen and mutual molecular interaction (surface effects) of their parti- Sonntag, 1965; Guggenheim, 1967; IUPAC, 1997). It is de- cles will be neglected. We may imagine a portion of the sur- fined in terms of chemical potentials in such a way that it face mixed layer of the ocean in contact with the atmospheric
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Adiabatic Lapse Rate of Saturated Humid Air a) Sea-Air Specific Humidity 0.98 40
0 g/kg 0.96 35 g/kg 35 120 g/kg 0.94 30 1000 hPa 900 hPa 800 hPa 0.92 25 700 hPa 600 hPa 0.9 20 500 hPa 0.88 15
400 hPa Specific Humidity in % LapseRate K /(100in m) 0.86 10
0.84 5 300 hPa 0.82 0 0 5 10 15 20 25 30 35 40 45 50 0 10 20 30 40 50 60 70 80 90 Temperature t /°C Temperature t /°C
Fig. 2: Adiabatic lapse rate (5.26) of saturated humid air at different temperatures and Fig.pressures 2. Adiabaticas indicated by lapse the curves. rate Note (5.26) that thi ofs lapse saturated rate is termed humid “dry” air in some at differ- b) Sea-Air Relative Humidity (WMO) entliterature. temperatures For convenience, and the pressures rate is shown as per indicated 100 m altitude by thedifference curves. as common Note thatin 100 meteorology, rather than per pressure difference. For comparison, the lapse rate of wet air is 10 g/kg thisshown lapse in Fig. rate 7. is termed “dry” in some literature. For convenience, 20 g/kg 98 the rate is shown per 100 m altitude difference as common in me- 30 g/kg teorology,The adiabatic rathervirtual-temperature than per lapse pressure rate (Jacob difference.son, 2005) follows For from comparison, the pressure the 40 g/kg 96 lapsederivative rate of ofthe wetvirtual air temperature, is shown Eq. in (5.8), Fig. as 7. 50 g/kg 94 ∂T M A ∂(Pv AV ) 1 1 1 60 g/kg ΓAV = v = = T −κ AV = T − (5.27) v ∂ ∂ v s v ρ AV 2 P A,s R P P P c 70 g/kg surface boundary layer, orA droplets,s of sea spray floating in 92 80 g/kg air,Adiabatic in thermodynamiccompressibility and sound equilibrium speed are given inat Eq. their(5.24). interface. As a 90 g/kg 90 simpleIn additionexample, to the compressibility a box factor, containing Eq. (5.3), another certain common masses measure for of the water, non-ideal Relative Humidity in % 100 g/kg airbehaviour and saltof gases (in or gas any mixtures initial is the form) fugacity will (Glasstone, adjust 1947; to van its Wylen equilibrium and Sonntag, 1965; Guggenheim, 1967; IUPAC, 1997). It is defined in terms of chemical potentials in such 110 g/kg 88 statea way that in it the coincides form with of the seawater (partial) pressure and of humid the gas in air the ideal-gas after some limit. The relax- fugacity f of humid air is AV 120 g/kg 86 ation time. When the volume or the temperature of the box is changing, the related g AV − g AV, shiftedid liquid-gas equilibria can be f ()A,T, P = P exp (5.28) 0 10 20 30 40 50 60 70 80 90 AV R T computed from a Gibbs AV function of this heterogeneous sys- Temperature t /°C tem since each component has the same pressure and temper- ature. Thus, the Gibbs function gSA of sea air consists of the Fig. 3. Specific (a) and relative (b) humidity of sea air, i.e., sum of a seawater part with the mass mSW = mS +mW, and humid air in equilibrium with seawater, at sea level pressure, a humid-air part with the mass mAV = mA +mV, forming the P =101 325 Pa, as a function of temperature for different absolute total sea-air mass mSA = mSW +mAV: salinities as indicated by the curves. The equilibrium air fraction, A = Acond, at the condensation point is computed from Eq. (6.4), SA A S AV AV g w ,w ,T,P = w g (A,T,P ) (6.2) the resulting specific humidity is q=(1−A). The relative humidity RH is determined from A by the WMO definition (10.4) with + SW SW WMO w g (SA,T,P ) the saturated air fraction Asat from Eq. (7.5). Asat is displayed as Here, the independent composition variables wA = mA/mSA the zero-salinity curve “0 g/kg” in (a). and wS = mS/mSA are the mass fractions of air and of sea salt in sea air, respectively. The liquid mass fraction of the sea-air SW SW SA S composite is w = m /m = w /SA, the gaseous one is AV = AV SA = A w m /m w /A. Thus, from the mass conserva- AV SW ! AV ∂g SW ∂g tion we infer the identity g −A = g −SA . (6.4) ∂A ∂SA A S T ,P T ,P w /A+w /SA = 1 (6.3) which relates the air fraction A of humid air to the salinity From Eq. (6.4) along with (6.3), all thermodynamic prop- S of seawater at given wA and wS. erties of sea air can be computed as functions of the four A In equilibrium and in the absence of gravity, temperature independent variables wA,wS,T,P . cond and pressure in both phases are the same. The vapour-liquid For this purpose, the air fraction A = A (SA, T , P) of V W mass ratio m /m of H2O in sea air is controlled by the ther- sea air at equilibrium, i.e. of humid air at the condensation modynamic equilibrium condition of equal chemical poten- point in contact with seawater, can be computed from the tials of water in seawater and water in humid air, Eq. (5.15), condition (6.4) by Newton iteration. Converted to relative www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 102 R. Feistel et al.: Thermodynamic properties of sea air humidity using the WMO definition, Eq. (10.4), the subsat- uration of sea air as a function of temperature and salinity ∂ 2 2 AV 2 is shown in Fig. 3 at conditions ranging from cold brackish DA = −A 3AS [g] = A ∂ g /∂A , (6.8) ∂A T ,P water to hot concentrated brines. The climatological ambi- SA,T ,P ent relative humidity at the ocean surface is about 80% (Dai, and DS of seawater as the derivative with respect to absolute 2006), i.e. clearly below the equilibrium values shown in the salinity change, lower panel of Fig. 3. The equilibrium specific humidity of sea-air shown in Fig. 3 is the actual quantity to be used in la- ∂ 2 2 SW 2 DS = SA 3AS [g] = SA ∂ g /∂SA . (6.9) tent heat flow parameterisations (Wells and King-Hele, 1990) ∂SA A,T ,P T ,P that represent the tendency of the system to adjust towards From the Second Law of Thermodynamics it follows that the thermodynamic equilibrium. coefficients D and D are nonnegative (Prigogine and De- For a compact writing of formulas related to the equilib- A S fay, 1954; Ebeling and Feistel, 1982; De Groot and Mazur, rium condition (6.4) of a composite system, we define for 1984; Landau and Lifschitz, 1987; IOC, 2010). In the ideal- sea air a formal phase-transition latency operator 3 [z] of AS gas limit, D /T is independent of temperature and pressure, the two phases with the subscripts A for humid air and S for A Eq. (H15). seawater, with respect to a certain property, z, by, Because of total water conservation between the phases, AV SW ! Eq. (6.3), the differentials dA and dS at constant wA and wS AV ∂z SW ∂z A 3AS[z] = z −A −z +SA . (6.5) of sea air are not independent of each other and are related ∂A T ,P ∂SA T ,P by The operator (6.5) was originally introduced for sea ice in a wA wS slightly modified version (Feistel and Hagen, 1998), where it A+ S = . 2 d 2 d A 0 (6.10) was referred to as the “melting operator”. It turns out that for A SA humid air a similar expression is again a very useful tool. The term “latency operator” is used as a natural generalization of Thus, in Eq. (6.7), dA can be expressed in terms of dSA “melting operator”, applicable for arbitrary phase transitions or vice versa. Eliminating first dA, the Clausius-Clapeyron Eq. (6.7) reads for the total differential dSA of the first kind. The operator 3AS is commutative regarding partial differentiation, (∂/∂x)3 [z] = 3 [∂z/∂x], taken AS AS wS at constant A and SA, if x stands for either T or P . 3AS is an- DAS dSA = 3AS [s]dT −3AS [v]dP. (6.11) S2 tisymmetric in its indices, 3AS [z] = −3SA [z] = 3SA [−z]. A Evidently, in a case of three phases, A, B, C, the related op- Here, the combined chemical air-salt coefficient DAS is de- erators obey additivity in the form fined as
3AB = 3AC +3CB, (6.6) A S D D D = D + A D = A + S . (6.12) AS wA A wS S wAV wSW corresponding to the transitivity of the binary relation “equi- librium” between phases. Using this operator, the equilib- The specific entropies of the two phases appearing in 3AS[s] rium condition (6.4) takes the simple form 3 [g] = 0. Its are sAV = − ∂gAV/∂T and sSW = − ∂gSW/∂T , AS A,P SA,P total differential gives the Clausius-Clapeyron differential and vAV = ∂gAV/∂P , vSW = ∂gSW/∂P are the A,T SA,T equation of this phase transition, specific volumes of humid air and of seawater in 3AS[v]. ∂ From the exact differential (6.11) we infer the partial d3AS [g]=0= 3AS [g] dA (6.7) derivatives ∂A SA,T ,P 2 " # ∂SA S 3AS [s] ∂ ∂g = A , (6.13) + 3 [g] dS +3 dT S ∂S AS A AS ∂T ∂T wA,wS,P w DAS A A,T ,P A,SA,P " # ∂g and +3AS dP ∂P ∂S S2 3 [v] A,SA,T A = − A AS . S (6.14) which tells us how changes in one state variable must be ∂P wA,wS,T w DAS compensated by changes in some other state variable(s) in Alternatively, eliminating dSA from Eq. (6.7) by means of order to maintain thermodynamic equilibrium. Eq. (6.10), we get for the corresponding changes of the un- Evaluating the first two terms in Eq. (6.7), we define the saturated air fraction at the condensation point chemical coefficient DA of humid air as the derivative of the relative chemical potential with respect to the air fraction ∂A A2 3 [s] = − AS change, A (6.15) ∂T wA,wS,P w DAS
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ 24
∂A A2 Λ [v] = AS . (6.16) ∂ A P wA ,wS ,T w DAS
With the help of Eqs. (6.13) – (6.16) we can derive formulas for relevant sea-air properties from temperature and pressure derivatives of the sea-air Gibbs function (6.2),
A S SA ()A S = w AV ()+ w SW () g w , w ,T, P g A,T, P g SA ,T, P , (6.17) A SA
A S where A and SA are the solutions of the Eqs. (6.3) and (6.4), i.e. functions of ( w , w , T, P).
The specific entropy of sea air, sSA , is
∂gSA sSA = − = wAV sAV + wSW sSW , (6.18) ∂ T wA ,wS ,P
and the specific enthalpy of sea air, hSA , is
hSA = g SA + Ts SA = wAV hAV + wSW hSW . (6.19)
R. Feistel et al.: Thermodynamic properties of sea airIts humid-air parts sAV and hAV are plotted in Fig. 4 for different salinities and temperatures 103 at the standard surface air pressure of 101325 Pa. and a) Sea-Air Entropy at 1013.25 hPa 3000 0 g/kg 35 g/kg 2 ∂A A 3 [v] 120 g/kg 2800 = AS . A (6.16) 2600 ∂P wA,wS,T w DAS 2400 2200 With the help of Eqs. (6.13–6.16) we can derive formulas 2000 for relevant sea-air properties from temperature and pressure 1800 derivatives of the sea-air Gibbs function (6.2), 1600 1400 A S 1200 SA A S w AV w SW g w ,w ,T,P = g (A,T,P )+ g (SA,T,P ), (6.17) 1000 A SA 800
Specific Entropyin J/(kgK) 600 where A and SA are the solutions of the Eqs. (6.3) and (6.4), 400 A S i.e. functions of (w , w , T , P). Dry Air 200 The specific entropy of sea air, sSA, is 0 0 10 20 30 40 50 60 70 80 90 25 Temperature t /°C SA ! SA ∂g AV AV SW SW s = − = w s +w s , (6.18) b) Sea-Air Enthalpy at 1013.25 hPa ∂T A S 1000 w ,w ,P 0 g/kg 35 g/kg 120 g/kg 900 and the specific enthalpy of sea air, hSA, is 800 hSA = gSA +T sSA = wAVhAV +wSWhSW. (6.19) 700 600 Its humid-air parts sAV and hAV are plotted in Fig. 4 for dif- 500 ferent salinities and temperatures at the standard surface air pressure of 101 325 Pa. 400 The specific volume of sea air follows as 300 Specific Enthalpy in kJ/kg ! 200 ∂gSA vSA = = wAVvAV +wSWvSW. (6.20) 100 ∂P Dry Air wA,wS,T 0 0 10 20 30 40 50 60 70 80 90 Temperature t /°C Taking the derivatives in Eqs. (6.18) and (6.20), the prop- erty of the composite system is just the sum of the fractions AV AV Fig 4: Entropy s , panelAV a), and enthalpy h , panel b),AV of humid air in equilibrium with of the two phases. Any additional terms cancel because of Fig.seawater, 4. EntropyEq. (6.18), ats sea-level, a), andpressure enthalpy as a functionh of ,theb), sea-surface of humid temperature air in equi- (SST) libriumfor salinities with 0, 35 seawater,and 120 g/kg. Eq.The related (6.18), humi atdity sea-level is shown in pressureFig. 3. Entropy as and a func- Eq. (6.4), 3AS[g] = 0. This is no longer the case if the sec- enthalpy of dry air are plotted for comparison. ond derivatives of the Gibbs function (6.17) are involved, as tion of the sea-surface temperature (SST) for salinities 0, 35 and 120 g/kg. The related humidity is shown in Fig. 3. Entropy and for the heat capacity, compressibility or thermal expansion. The specific volume of sea air follows as SA enthalpy of dry air are plotted for comparison. The specific isobaric heat capacity of sea air, cP , is com- ∂gSA vSA = = wAV vAV + wSW vSW . (6.20) puted from Eq. (6.18), as ∂ P wA ,wS ,T ! cSA ∂sSA wA ∂sAV TheTaking last the derivatives term of in Eq.Eqs. (6.18) (6.22) and (6.20), is the the latent-heatproperty of the composite part of system the heatis just P = = (6.21) the sum of the fractions of the two phases. Any additional terms cancel because of Eq. (6.4), capacityΛ caused by the transfer of water between the liquid T ∂T A ∂T AS [g] = 0. This is no longer the case if the second derivatives of the Gibbs function (6.17) wA,wS,P A,P andare involved, the gas as for phase the heat whencapacity, thecompressibi temperaturelity or thermal is expansion. changing at con-
" A A AV # w w ∂s ∂A stantThe specific pressure. isobaric heat capacity of sea air, cSA , is computed from Eq. (6.18), as + − sAV + P SA 2 For the isothermal compressibility, κ = A A ∂A ∂T A S T T ,P w ,w ,P cSASA ∂sSA wA ∂s AVSA wA wA ∂s AV ∂A − ∂vP =/∂P = /v ,+ we− repeats AV + similar calculation ∂ wA,wS,T ∂ 2 ∂ ∂ ! " ! # T T A S A T A A A T A S S SW S S SW w ,w ,P A,P T ,P w ,w ,P w ∂s w SW w ∂s steps with the result (6.21) + + − s + wS ∂sSW wS wS ∂sSW ∂S 2 + + − sSW + A SA ∂T S SA ∂SA ∂ 2 ∂ ∂ A S T S S S T A S S,P T ,P A S ,P A A A T ,P 2 w ,w ,P SA SA AV AV AV SW SW SW (3AS [v]) ∂SA v κT = w v κT +w v κT + . (6.23) DAS ∂T wA,wS,P Using Eqs. (6.5), (6.13) and (6.15), this expression can be For the thermal expansion coefficient, αSA = SA SA rearranged to give ∂v /∂T wA,wS,P /v , we similarly obtain (3 s )2 SA AV AV SW SW AS [ ] SA SA AV AV AV SW SW SW 3AS [v]3AS [s] cP = w cP +w cP +T . (6.22) v α = w v α +w v α + . (6.24) DAS DAS www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 104 R. Feistel et al.: Thermodynamic properties of sea air
Various other thermodynamic properties of sea air are avail- the relative humidity of sea-air is, from Eq. (10.4), SA = able from these coefficients using standard thermodynamic RHWMO=98.14%, Fig. 3. The latent heat is LP relations. As an example, a property of particular interest −1 SA = 2498510Jkg , its derivatives are ∂LP /∂SA SA A,T ,P in meteorology is the adiabatic lapse rate, 0 , describing −30775Jkg−1, ∂LSA/∂T = −2379Jkg−1 K−1 and the temperature change with pressure under isentropic con- P A,SA,P ∂LSA/∂P = −0.0136Jkg−1 Pa−1. ditions, similar to Eq. (5.25), P A,SA,T
∂2gSA/∂T ∂P SA ∂T wA,wS 7 Properties of wet and saturated humid air 0 = = − . (6.25) ∂P A S AS 2 SA 2 w ,w ,s ∂ g /∂T wA,wS,P As an important special case, at zero salinity, wS=0, the From Eqs. (6.18), (6.20–6.22) and (6.24) we get Gibbs function (6.2) describes the properties of wet air, i.e. saturated air combined with liquid water, e.g. in the form of wAVvAVαAV +wSWvSWαSW +3 [v]3 [s]/D 0SA = AS AS AS (6.26) droplets as in clouds or fog. It is therefore often denoted AV AV + SW SW + 2 w cP w cP /T (3AS [s]) /DAS as “cloudy air” in meteorology. However, this Gibbs func- tion for a composite system of liquid water and humid air for air over seawater reacting to air pressure variations with in mutual equilibrium may also be applied to e.g. saturated warming or cooling caused by adiabatic expansion as well as air resting over a fresh water lake, or to the precipitation of condensation or evaporation. dew. Below the freezing point of water, in the formulas de- To obtain an appropriate expression for the latent heat, AS rived here the properties of liquid water must be replaced LP , of isobaric evaporation from the sea surface, we di- with those of ice. 2 vide the latent heat-capacity term, T 3AS[s] /DAS, from The Gibbs function of wet air, gAW, follows from Eq. (6.2) Eq. (6.22) by the related isobaric evaporation rate, Eq. (6.15), as gAW wA,T,P = gSA wA,0,T,P (7.1) ∂wAV wA ∂A 3 [s] = − = AS . AV AV W SW 2 (6.27) = w g (A,T,P )+w g (0,T,P ) ∂T wA,wS,P A ∂T wA,wS,P DAS and the related latency operator reads Under consideration of 3AS [g] = 0, Eq. (6.4), we eventually arrive at the formula for the latent heat, ∂zAV 3 [z] = zAV −A −zW. (7.2) AW ∂A ∂hAV T ,P LSA = T 3 [s] = 3 [h] ≡ hAV −A (6.28) P AS AS AV ∂A T ,P The mass fractions are w = ! mA +mV/ mA +mV +mW for the humid air in the ∂hSW SW W W A V W −h +SA . wet air, w = m / m +m +m for the liquid wa- ∂SA T ,P ter in the wet air, and wA = mA/ mA +mV +mW, A = A A V This expression does not depend on the absolute enthalpies m / m +m for the dry air content, which together obey V W of H2O, air, and sea salt. On the contrary, the simple en- mass conservation of water, m +m , between vapour and thalpy difference, 1h = hAV −hSW, between the gaseous and liquid, i.e. the identity the liquid component depends on the arbitrary values of the wA absolute enthalpies of air and of salt. Only in the special case +wW = wAV +wW = 1. (7.3) A of pure water, SA = 0, A = 0, does this difference equal the latent heat of evaporation (Kirchhoff’s law). Thus, the Gibbs function (7.1) can be written in the form AV − AV From Eq. (6.28) it is reasonable to refer to h AhA as A SW SW AW A w AV the specific enthalpy of water in humid air, and h −SAh g w ,T,P = g (A,T,P ) (7.4) SA A(T,P ) as the specific enthalpy of water in seawater, or the par- wA tial specific enthalpies (Glasstone, 1947; Pruppacher and + 1− gW (T,P ) Klett, 1997), Eqs. (3.7) and (5.19). In the ideal-gas limit, A(T,P ) hAV − AhAV equals the enthalpy of vapour, Eq. (H12), as A as a linear function of the given air fraction, wA, of the wet one would expect. The latent heat, Eq. (6.28), is an al- air. most linear function of temperature and depends only weakly As a function of T and P , the saturated air fraction of hu- on salinity, air fraction and pressure (Fig. 5). For illustra- mid air, Asat (T,P ), is obtained from the equilibrium condi- tion we give the values for the standard ocean surface state AW −1 tion (TSO=273.15 K, PSO=101 325 Pa, SSO=35.16504 g kg ). At AV this state, the air fraction of sea-air is ASO=0.996293, AV ∂g W sat 3AW[g] = g −A −g = 0. (7.5) the saturated air fraction would be A =0.996223, i.e. ∂A T ,P
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic properties of sea air 105 28
Latent Heat of Water and Seawater potentials of the two phases, e.g., Eq. (8.1). An approximate 2550 analytical solution P (T ) can be derived analytically and rep-
2500 resents a reasonable estimate, for example, for the sublima- 120 g/kg tion curve of ice (Feistel and Wagner, 2007). In the special 2450 case when no air is present, A = 0, dA = 0, the generalized 40 g/kg 2400 form, Eq. (7.6), reduces to the familiar Clausius-Clapeyron 101 325 Pa equation for the liquid-vapour transition. Geometrically, any 40 g/kg 2350 5 M displacement (dA, dT , dP) which obeys Eq. (7.6) is tangen- Pa tial to the phase transition surface defined by Eq. (7.5) in the 1 2300 0 M Pa (A, T , P) phase space, while the coefficients of (dA, dT , 0 g/kg 2250 dP) in Eq. (7.6) form a “normal vector”.
Evaporation Enthalpy in kJ/ kg Reading Eq. (7.6) as an exact differential for dA, we infer 0 g/kg 2200 for the partial derivatives of A, i.e., for changes of the air 0 g/kg 2150 fraction with temperature, -10 0 10 20 30 40 50 60 70 80 90 100 Temperature t /°C sat ∂A 3 [s] AW AW sat AW δP = − = AAW , (7.7) Fig. 5: Isobaric evaporation enthalpy of water, indicated by “0 g/kg”, and of seawater with ∂T DA Fig.salinity 5. 120Isobaric g kg –1 at 101325 evaporation Pa and 40 g enthalpykg –1 at 5 MPa of and water,10 MPa, computed indicated from Eq. by P (6.28). The salinity dependence is very weak in either case. At− 1high pressure the validity “0 g/kg”, and of seawater with salinity 120 g kg at 101 325 Pa and–1 or pressure, of the− current1 Gibbs function of seawater (3.1) is restricted to maxima of only 40 g kg 40 gand kg 40 °C,at but 5at MPaatmospheric and pressure 10 MPa, it is computedvalid up to 120 from g kg –1 and Eq. 80 (6.28). °C (IAPWS, The sat salinity2008; Feistel, dependence 2008). The is lower very temperature weak inbounds either are the case. particular At freezing high pressure points of ∂A 3AW [v] water or seawater. AW = − AW = − sat the validity of the current Gibbs function of seawater (3.1) is re- δT AAW , (7.8) ∂P T DA stricted to maxima of only 40 g kg−1 and 40 ◦C, but at atmospheric 7. Properties of wet and saturated humid−1 air ◦ pressure it is valid up to 120 g kg and 80 C (IAPWS, 2008; Feis- due to condensation or evaporation. The coefficient DA is tel,As an 2008). important The special lower case, temperatureat zero salinity, w boundsS = 0, the Gibbs are the function particular (6.2) describes freezing the defined in Eq. (6.8). The right-hand sides of Eqs. (7.7) and properties of wet air, i.e. saturated air combined with liquid water, e.g. in the form of droplets pointsas in clouds of or water fog. It oris therefore seawater. often denoted as “cloudy air” in meteorology. However, this (7.8) depend only on the air fraction A of the humid-air com- Gibbs function for a composite system of liquid water and humid air in mutual equilibrium A may also be applied to e.g. saturated air resting over a fresh water lake, or to the precipitation ponent rather than on the air fraction w of the total sample, of dew. Below the freezing point of water, in the formulas derived here the properties of i.e. they are independent of the mass of liquid water present. Throughoutliquid water must be this replaced section, with those if of not ice. explicitly stated otherwise, A They can therefore be regarded as the isothermal and isobaric AW sat equalsThe Gibbs thefunction saturation of wet air, g value, followsA fromAW Eq., Fig. (6.2) as 8, since humid air in drying rates of humid air, i.e. the decrease of its saturated air equilibriumAW A with liquidSA A waterAV isAV always saturated.W SW sat g (w ,T, P)= g (w ,0, T, P)= w g (A,T, P)+ w g ( ,0 T, P) (7.1) fraction A due to heating or compression, corresponding sat AW The function AAW (T,P ) is different from the saturation to a lowering of the relative humidity at constant specific hu- andsat the related latency operator reads A AI (T,P ) of humid air with respect to ice, Sect. 8. Both midity of an unsaturated sample at constant P or T , respec- functions take the same values on the freezing curve because tively. Below the freezing point, different drying rates δAI W Ih g equals g under the equilibrium conditions, Eq. (7.5) and must be applied with respect to the sublimation equilibrium, its counterpart for ice air, Eq. (8.7). Sect. 8. Solving Eq. (7.5) for either T (A, P) or P (A, T) provides From Eqs. (7.7), (7.8), the adiabatic drying rate of humid the saturation point (SP) temperature TSP or pressure PSP, air with respect to increasing pressure is computed by means also known as the isentropic condensation level (ICL), i.e. of the chain rule as the saturation level for an unsaturated parcel lifted moist- sat adiabatically (Stull, 2003; Jacobson, 2005). This is consid- AW ∂AAW AW AV AW δs = − = δT +0 δP . (7.9) ered in more detail below, see Eq. (7.25) and following. ∂P s The total differential of the phase equilibrium condi- Here, the adiabatic lapse rate of humid air, 0AV = tion (7.5) is the related Clausius-Clapeyron differential equa- (∂T /∂P ) , is given by Eq. (5.25). tion, A,s Returning to wet air, we find for the entropy, Eq. (6.18), ∂3AW [g] d3 [g] = 0 = dA (7.6) ∂gAW AW AW A = − = AV AV + W W ∂A T ,P s w ,T,P w s w s , (7.10) ∂T A " # " # w ,P ∂g ∂g +3AW dT +3AW dP, and the specific volume, Eq. (6.20), ∂T A,P ∂P A,T AW AW A ∂g AV AV W W which represents a special case of Eq. (6.7). v w ,T,P = = w v +w v . (7.11) ∂P A Commonly, the Clausius-Clapeyron differential equation w ,T for a two-phase system such as water-vapour or ice-vapour The entropy of wet air, Eq. (7.10), is plotted in Fig. 6 (“tephi- takes the form dP/dT = 1s/1v, obtained by taking the to- gram”) as a function of temperature, pressure and the dry- tal differential of the equilibrium condition of equal chemical air fraction wA between the freezing point and complete www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 31
∂g AW v AW ()wA ,T,P = = wAV v AV + wWvW . (7.11) ∂ P wA ,T
The entropy of wet air, Eq. (7.10), is plotted in Fig. 6 (“tephigram”) as a function of temperature, pressure and the dry-air fraction wA between the freezing point and complete evaporation of the liquid component. Evidently, the temperature range of validity of Eq. (7.10) depends strongly on the pressure and the air fraction, given by the condition A ≤ sat ( ) = sat ( ) 106w AAW R.T, P Feistel from Eq. et(7.3) al.: and ThermodynamicA AAW T, P computed from properties Eq. (7.5), as of shown sea in air Fig. 8. evaporation of the liquid component. Evidently, the tem- a) Entropy of Wet Air at 1013.25 hPa 7000 perature range of validity of Eq. (7.10) depends strongly 10% on the pressure and the air fraction, given by the condition 20% ) 6000 A sat sat -1 w ≤ A (T,P ) from Eq. (7.3) and A = A (T,P ) com- 30% AW AW K puted from Eq. (7.5), as shown in Fig. 8. -1 40% 5000 Similar to Eq. (5.20), the potential temperature of wet air 50% / (J kg follows from the equation, s 4000 60% sAW wA,θ AW,P = sAW wA,T,P . (7.12) 3000 0 70% or, equivalently, from the enthalpy, hAW, 80% 2000 AW 90%
∂g Specific Entropy 1000 hAW = gAW −T (7.13) ∂T A w ,P 0 0 10 20 30 40 50 60 70 80 90 100 as its isobaric entropy derivative (Feistel and Hagen, 1995; Temperature32 t /°C
Feistel, 2008a) taken at the in-situ entropy s and the surface pressure P0 as the reference pressure, b) Entropy of Wet Air at 500 hPa 7000 10% AW AW ∂h 20% θ = . (7.14) ) 6000 ∂s A -1 30% w ,P =P0 K -1 Equation (7.14) is the formal solution of the implicit 40% 5000 Eq. (7.12) for θ AW which can be inferred from the total dif- 50% / (J kg
AW A s 4000 ferential of the enthalpy potential function, h (w , s, P), 60% obtained from Eqs. (7.13) and (7.5), as, 70% 3000 dhAW = µAVdwA +T ds +vdP, (7.15) 80% 2000 AV A V where the relative chemical potential, µ = µ −µ , of hu- 90% mid air is given by Eqs. (5.14), (5.15). Specific Entropy 1000 Equations (7.12) and (7.14) are meaningful only if liquid 0 water is still present at the reference pressure P0, i.e. if the 0 10 20 30 40 50 60 70 80 90 100 Temperature t /°C dewpoint pressure (ICL) is higher than P0. Otherwise, one AW Fig. 6: Entropy of wet air, Eq. (7.10), as a function of temperature at 1013.25 hPa has to insert the conserved entropy s = s computed from (Panel a) and 500 hPa (Panel b) between the freezing point and complete evaporation A Fig. 6.of Entropythe liquid component of wet for air, dry-air Eq. fractions (7.10), w asA of a wet function air, Eq. (7.3), of temperaturebetween 10% and Eq. (7.10) and the conserved air fraction A = w into the en- W AV at 1013.2590% as hPaindicated(a) byand the curves. 500 hPa The related(b) between liquid mass the fractions freezing w of wet point air, Eq. and thalpy h (A, s, P0) of unsaturated humid air and compute (7.3), are shown in Fig. 9. complete evaporation of the liquid component for dry-air fractions the related potential temperature from Eq. (5.21). w A of wet air, Eq. (7.3), between 10% and 90% as indicated by the In analogy to Eqs. (6.22–6.28) we compute the heat capac- W curves. The related liquid mass fractions w of wet air, Eq. (7.3), ity, as, areSimilar shown to Eq. in(5.20), Fig. the 9. potential temperature of wet air follows from the equation,
AW AW A AW AW A s (w ,θ , P )= s (w ,T, P). (7.12) AW ∂s AV AV W W 0 cP = T = w cP +w cP (7.16) ∂T A AW w ,P Theor, equivalently, adiabatic from lapse the enthalpy, rate h of, wet air, often regarded as the “sat- 2 T (3 [s]) ∂ AW AV AW urated”AW lapseAW rate, g is computed from Eqs. (7.16) and (7.18) + h = g − T (7.13) w , ∂ T A DA as w ,P
AW as its isobaric entropy derivative (Feistel and Hagen, 1995; Feistel, 2008a) taken at the in-situ the isothermal compressibility, κT , AW ∂T 0entropy= s and the surface pressure P0 as the reference pressure, ∂vAW ∂P wA,s AW AW AV AV AV W W W ∂hAW v κ =− =w v κ +w v κ (7.17) AVθ AW AV= AV W. W W AV (7.14) T T T w v α∂ +w v α +w 3 [v]3 [s]/D ∂P A s A = AW AW A w ,T = w ,P P0 . (7.19) wAVcAV +wWcW/T +wAV (3 s )2 /D (3 [v])2 P P AW [ ] A +wAV AW , DA Neglecting the liquid contributions to the heat capacity in W W ≈ and the thermal expansion coefficient, αAW, the denominator, i.e., using w cP 0, leads to the approx- imate “pseudoadiabatic” lapse rate (Emanuel, 1994; Jacob- ∂vAW vAWαAW= =wAVvAVαAV+wWvWαW (7.18) son, 2005). In this simplified model the condensate is as- ∂T wA,P sumed to precipitate and disappear immediately from the ris- AV 3AW [v]3AS [s] ing parcel (v. Bezold, 1888; Rogers and Yau, 1989). This +w . model picture fails for sinking air as it cannot explain the DA
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ 35
derived from Eqs. (7.3) and (7.7), as
∂hAV LAW = TΛ [][]s = Λ h ≡ hAV − A − hW . (7.22) P AW AW ∂ A T ,P
Of particular interest is the saturation point of humid air. At the dewpoint, no liquid water is present, wW = 0, so we infer from Eq. (7.3) the relation
A = sat ( ) w AAW T, P at the dewpoint (7.23)
34 between the independent variables of Eq. (7.4). This dewpoint surface in the (wA ,T, P) space bounds the validity of the Gibbs function of wet air. On the surface, the Gibbs functions of wet air and of humid air have the same values, unknown, such as for measured radiosonde profiles. Selected values of Eq. (7.19) computed at a negligible condensate fraction are displayed in Fig. 7. WA ( A )= AV ( sat ) R. Feistel et al.: Thermodynamic properties of sea airg w ,T, P g AAW ,T, P . 107 (7.24)
Adiabatic Lapse Rate of Wet Air Dry-Air Fraction Range of Humid Air and Wet Air 0.425 100
0.4 90 1 101 HUMID AIR 3.2 0.375 5 h Pa 80 5 0.35 00 h hP 70 0.325 a
2 60 0 0 0.3 h P 10 a 50 0.275 0 h P 0.25 a 40
300 hPa Air inFraction % 0.225 30
LapseRate K /(100in m) 400 hPa 500 hPa WET AIR 600 hPa 0.2 20 800 hPa 1000 hPa 0.175 10
0.15 0 0 5 10 15 20 25 30 35 40 45 50 0 10 20 30 40 50 60 70 80 90 100 Temperature t /°C Temperature t /°C
Fig. 7: Adiabatic lapse rate (7.19) of wet air at the dewpoint, i.e. containing a negligible Fig. 8: The saturation curves Asat (T, P) computed from solving Eq. (7.5) at the Fig.amount 7. of liquidAdiabatic water, at lapsedifferent rate temperatures (7.19) a ofnd pressures wet air as atindicated the dewpoint, by the curves.i.e. Fig. 8. The saturation curvesAW Asat (T,P ) computed from solv- containingNote that this lapse a negligible rate is termed amount “moist” in ofsome liquid literature. water, For convenience, at different the rate temper- is pressures 1013.25, 500, 200 and 100 hPa,AW as indicated, between the freezing and the shown per 100 m altitude difference as common in meteorology, rather than per pressure ing Eq.boiling (7.5) temperature at the of pressurespure water separate 1013.25, the phys 500,ically sensible 200 anddry-air 100 fractions, hPa, aturesdifference. and For pressurescomparison, the as lapse indicated rate of humid by the air is curves. shown in NoteFig. 2. that this lapse ≥ sat ( ) as indicated,A AAW T between, P , of the single-phase the freezing state of and humid the air boiling from those temperature of the two-phase of rate is termed “moist” in some literature. For convenience, the rate state of wet air, wA ≤ Asat (T, P). On a particular saturation curve the two systems pure water separate theAW physically sensible dry-air fractions, A ≥ isDuring shown the adiabatic per 100 lifting m process, altitude the differenceliquid fraction asincreases common at the adiabatic in meteorology, condensation Asat (T,P ), of the single-phase state of humid air from those of rate AW rather than per pressure difference. For comparison, the lapse rate A ≤ sat the two-phase state of wet air, w AAW (T,P ). On a particular of humid ∂w airW is shown inδ AW Fig. 2. − = ()1− wW s . (7.20) saturation curve the two systems coincide, Eqs. (7.23), (7.24). The ∂ P A A sat w ,s W = − A liquid fraction of wet air,w 1 w /AAW (T,P ), Eq. (7.3), is shown in Fig. 9. latentThe latent contributions heat for the evaporation in Eq.of liquid (7.19) water follows since from there Eq. (7.16) is then as the no ratio liquid of the latent part of the heat capacity to the isobaric evaporation rate of the liquid fraction (Fig. 9), in the parcel that could evaporate. If in reality precipitation ∂wW wA Λ [s] happens− during = rising,AW , the sinking air must correctly be (7.21)de- ∂ T A A D scribed byw the,P moist-adiabaticA lapse rate (5.25) rather than A = sat Eq. (7.19), which produces the warming “foehn wind” effect w AAW (T,P ) at the dewpoint (7.23) at the lee side of a mountain. In addition to being conve- between the independent variables of Eq. (7.4). This dew- nient simplifications, the definition of such “pseudo” prop- point surface in the wA,T,P space bounds the validity of erties is practically useful for cases in which the condensed the Gibbs function of wet air. On the surface, the Gibbs func- water fraction is unknown, such as for measured radiosonde tions of wet air and of humid air have the same values, profiles. Selected values of Eq. (7.19) computed at a negligi- ble condensate fraction are displayed in Fig. 7. gWA wA,T,P = gAV Asat ,T,P . (7.24) During the adiabatic lifting process, the liquid fraction in- AW creases at the adiabatic condensation rate For an unsaturated humid-air parcel with the in-situ prop- ∂wW δAW erties (A, T , P), the dewpoint temperature T and pressure − = 1−wW S . (7.20) DP ∂P wA,s A PDP are met during adiabatic uplift when the two equations The latent heat for the evaporation of liquid water follows sat AAW (TDP,PDP) = A (7.25) from Eq. (7.16) as the ratio of the latent part of the heat ca- pacity to the isobaric evaporation rate of the liquid fraction (Fig. 9), AV AV s (A,TDP,PDP) = s (A,T,P ) (7.26) ∂wW wA 3 [s] − = AW , (7.21) ∂T wA,P A DA are satisfied. The solution of Eqs. (7.25) and (7.26) defines the adiabatic dewpoint temperature TDP (A,T,P ) and pres- derived from Eqs. (7.3) and (7.7), as sure PDP (A,T,P ) for a given unsaturated sample of humid ∂hAV air. This dewpoint temperature is also regarded as the isen- AW = = ≡ AV − − W LP T 3AW [s] 3AW [h] h A h .(7.22) tropic condensation temperature (ICT), defined as the tem- ∂A T ,P perature at which saturation is reached when unsaturated air Of particular interest is the saturation point of humid air. At is cooled adiabatically at a constant mass mixing ratio of wa- W the dewpoint, no liquid water is present, w = 0, so we infer ter vapour (Rogers and Yau, 1989; Jacobson, 2005). The from Eq. (7.3) the relation dewpoint pressure is regarded as the isentropic condensation www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 108 R. Feistel et al.: Thermodynamic properties of sea air 37
a) Liquid Fraction of Wet Air at 1013.25 hPa entropy, Gibbs energy and therefore also enthalpy cross over 100 continuously between humid air and wet air. Since the mass 10% 90 fraction wW and thus the volume of the native liquid phase 20% 80 are zero at the saturation point, the density changes contin- 30% uously, too, and therefore also the Helmholtz function and 70 40% the internal energy of the parcel. The second derivatives of 60 the potential functions such as the compressibility or the heat 50% 50 capacity change discontinuously across the saturation curve, 60% 40 however. 70% 30 Property changes of wet air subject to adiabatic processes
LiquidMass inFraction % 80% are preferably computed from the enthalpy as the appropri- 20 ate thermodynamic potential. To express the enthalpy hAW, 90% 10 Eq. (7.13), in terms of its natural variables wA, s and P , the 0 Eq. (7.12), 0 10 20 30 40 50 60 70 80 90 100 Temperature t /°C AW A = b) Liquid Fraction of Wet Air at 500 hPa s w ,T,P s (7.29) 100 10% 90 derived from the Gibbs function (7.4) must be inverted nu- 20% A A 80 merically for the temperature, T (w , s, P). At given w 30% and P , this computation is sensible only if s takes values re- 70 stricted to its particular range of validity, s (wA, P) ≤ s ≤ 40% min 60 A smax(w , P), as shown in Fig. 6, bound between freezing 50% 50 and complete evaporation of the liquid part. From the given 60% 40 pressure P , the minimum temperature Tmin is available from 70% the freezing point of liquid water, Eq. (8.1), and from it, in 30 AW A
LiquidMass inFraction % = 80% turn, the minimum entropy of wet air, smin s (w , Tmin, 20 P), Eq. (7.10). The upper end point, the “cloud base”, is de- 90% 10 fined by the saturation of humid air at the given air fraction, A 0 A = w , Eq. (7.27), solving Eq. (7.5) for T = Tmax at the 0 10 20 30 40 50 60 70 80 90 100 Temperature t /°C given pressure P . Since entropy is continuous at the phase-
transition point from humid to wet air, the maximum entropy of wet air is therefore given by s = sAV(wA, T , P), Fig. 9. Liquid mass fraction wW of wet air, the “burden” of con- max max densed water, as a function of temperature at 1013.25 hPa (a) and Eq. (5.16). 500 hPa (b) between the freezing point and the point at which com- plete evaporation of the liquid component occurs for dry-air frac- tions wA of wet air, Eq. (7.3), between 10% and 90% as indicated 8 Properties of sea air below the freezing point by the curves. The complement (1−wW) is the gaseous humid-air fraction of wet air. At temperatures below the freezing point of seawater, the sea-air system forms a third phase, solid ice Ih, which does not contain relevant amounts of sea salt or air. More pre- level (ICL) during adiabatic uplift. As an example, solutions cisely, ice-crystal distortions due to occasionally built-in salt of Eqs. (7.25), (7.26) are shown in Fig. 16. or air particles are considered as negligibly seldom, which Approaching the transition point from the other side (i.e., can safely be expected if the freezing process is sufficiently from below the saturation curve in Fig. 8), this dewpoint slow or the ice is sufficiently aged. This assumption does (“cloud base”) is reached by adiabatic compression of wet not exclude the presence of macroscopic brine pockets or air A air with the in-situ properties w ,T,P if the conditions bubbles within the ice which count as parts of the liquid or the gas phase, respectively. In other words, the equilibrium sat = A AAW (TDP,PDP) w (7.27) properties between humid air, seawater and ice do no depend on the spatial distributions or shapes of the three phases in the system. Any surface-tension effects are neglected in this WA A WA A s w ,TDP,PDP = s w ,T,P (7.28) model. The binary relation “A is at equilibrium with B” is transi- hold, which define the point where the parcel’s liquid frac- tive; if it holds for a pair of systems (A, B), and for another tion wW is completely evaporated but the humid air is still pair (B, C), then it is true for (A, C), too. Thus, for example, saturated (Fig. 9). Thus, passing the dewpoint adiabatically, if we have sea ice forming a barrier between humid air and
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic properties of sea air 109 water and in thermodynamic equilibrium with each of them, lowered by about 2.4 mK if dissolved air is present (Doherty then the air and the water are also in thermodynamic equi- and Kester, 1974; Feistel, 2008a). librium even though they are not in contact; if the ice layer In this section, we generalize the Gibbs function of sea were removed, the remaining humid air and water would be air, gSA, Sect. 6, to the Gibbs function of sea-ice air, gSIA, in equilibrium. Either the seawater or the humid air may also extending the validity of Eq. (6.2) below the freezing tem- be removed without upsetting the equilibrium between the perature of water/seawater, remaining pair. Similarly, if a hole is made in the ice barrier, gSIA wA,wS,T,P = wAVgAV (A,T,P ) (8.2) no adjustment is required to maintain equilibrium. Note that SW SW Ih Ih if ice were added to a system containing air and seawater at +w g (SA,T,P )+w g (T,P ) equilibrium, then establishing equilibrium conditions for the The sample of sea-ice air has the total mass mSIA = mSW + new system may require property adjustments in the air and mAV + mIh, consisting of the liquid phase, seawater, mSW, seawater. However, if a new equilibrium is achieved contain- the gas phase, humid air, mAV, and the solid phase, ice Ih, ing all three elements then any one of them may be removed mIh. The mass fractions of seawater, at constant T and P without upsetting the equilibrium be- SW SW SIA S tween the remaining pair. In this sense, the properties of the w = m /m = w /SA, (8.3) equilibrium between ice and humid air, briefly “ice air”, are humid air, independent of the presence or distribution of seawater; sim- ilarly, the equilibrium state between seawater and ice, “sea wAV = mAV/mSIA = wA/A, (8.4) ice”, does not depend on the continued presence of the am- and ice, wIh = mIh/mSIA, obey the identity bient air components. Thermodynamic equations for sea ice S A Ih were derived from the Gibbs functions of seawater and of ice w /SA +w /A+w = 1. (8.5) by Feistel and Hagen (1998). Quantitative formulas for air- The equilibrium condition (6.4) of equal chemical potentials free sublimation pressure and enthalpy are available down to of water in the different phases takes the generalized form of 50 K from Feistel and Wagner (2007) and IAPWS (2008b). the two separate equations The three-phase system, referred to here as “sea-ice air”, SW ! has the independent variables T and P as well as the mass SW ∂g Ih 3SI [g] ≡ g −SA −g = 0 (8.6) S A ∂SA fractions of salt, w , and of air, w , with respect to the sys- T ,P tem’s total mass. The special cases of sublimation equilibria or of sea ice are available from the formulas considered here ∂gAV S A 3 [g] ≡ gAV −A −gIh = 0. (8.7) in the limits of vanishing sea salt, w =0, or of air, w =0, AI ∂A respectively. The salt-free equilibria are considered in more T ,P detail in Sect. 9. The relative spatial distribution of the three At given T and P , these equations define the equilibrium phases is not relevant here for the thermodynamic properties fractions of air, A(T , P), and salt, SA(T , P), as well as the Ih S A of the parcel as a whole, for instance, the humid air part may ice fraction, w (w , w , T , P), from Eq. (8.5). Between be completely separated from the seawater part by a surface the freezing points of pure water and seawater the stable ex- layer of ice. This is true since the equilibrium between three istence of freshwater (e.g., as fog droplets in the air) and of phases always implies equilibrium conditions for each cho- ice (e.g., as ice fog in the air) is impossible in sea air. The sen pair of phases. humid-air part, i.e. the gas fraction of dry air mixed with Of particular interest is the special case of ice air at zero vapour, of sea air is always subsaturated, Fig. 10, as a re- salinity, wS=0, i.e. the properties of saturated air containing sult of the vapour-pressure lowering due to dissolved salt. In ice as in cirrus clouds or ice fog, air resting over a frozen contrast, below the freezing point of seawater, ice is a sta- lake or precipitating frost. The equations and formulas are ble phase (either within air or seawater) of sea-ice air and similar to those for wet air, Sect. 7, except that the liquid- the humid-air fraction is always saturated since no relevant water properties of that section are substituted by the related amounts of salt are “dissolved” in ice. Note that the freez- ice properties for the application below the freezing point. ing point of liquid water is not a distinguished temperature The freezing point T (P ) of liquid water is computed from for vapour, regardless of whether or not air is present. As a the equilibrium condition of equal chemical potentials of the stable gas phase of water, vapour can exist down to 40–50 K two phases, (Feistel and Wagner, 2007). From the total derivative of Eq. (8.6), i.e. the Clausius- gW (T,P ) = gIh (T,P ). (8.1) Clapeyron differential equation for sea ice, ∂ W d3 [g] = 0 = 3 [g] dS (8.8) Here, g is the Gibbs function of liquid water, Eq. (3.3), and SI ∂S SI A Ih A T ,P g is the Gibbs function of ice, Eq. (F1). At 101 325 Pa, " # " # ∂g ∂g the freezing temperature of pure water is 273.152 519(2) K +3 dT +3 dP SI ∂T SI ∂P (Feistel and Wagner, 2006; IAPWS, 2008b, 2009b), and is SA,P SA,T www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 40
S + A + Ih = w / SA w / A w 1. (8.5)
The equilibrium condition (6.4) of equal chemical potentials of water in the different phases takes the generalized form of the two separate equations
∂g SW Λ []g ≡ g SW − S − g Ih = 0 (8.6) SI A ∂ SA T ,P
∂g AV Λ []g ≡ g AV − A − g Ih = 0 . (8.7) AI ∂ A T ,P
At given T and P, these equations define the equilibrium fractions of air, A(T, P), and salt, Ih SA(T, P), as well as the ice fraction, w (T, P), from Eq. (8.5). Between the freezing points of pure water and seawater the stable existence of freshwater (e.g., as fog droplets in the air) and of ice (e.g., as ice fog in the air) is impossible in sea air. The humid-air part, i.e. the gas fraction of dry air mixed with vapour, of sea air is always subsaturated, Fig. 10, as a result of the vapour-pressure lowering due to dissolved salt. In contrast, below the freezing point of seawater, ice is a stable phase (either within air or seawater) of sea-ice air and the humid-air fraction is always saturated since no relevant amounts of salt are “dissolved” in ice. Note that 110the freezing point of liquid water is not a distinguished temperature for vapour, regardless of R. Feistel et al.: Thermodynamic properties of sea air whether or not air is present. As a stable gas phase of water, vapour can exist down to 40-50 K (Feistel and Wagner, 2007). a) Sea-Air Specific Humidity of ice air from the differential of Eq. (8.7). The related iso- 0.4 baric and isothermal air drying rates are IceIceIce 0.38 sat 35 g/kg AI ∂AAI 3AI [s] 80 g/kg 0.36 δP = − = A , (8.10) 120 g/kg ∂T DA 0.34 P ∂Asat 3 v 0.32 AI AI AI [ ] δT = − = −A , 0.3 ∂P T DA 0.28 in which DA is defined in Eq. (6.8). Crossing the freezing 0.26 point (Tf,Pf) of pure water, the drying rates of humid air change discontinuously from the ones relative to liquid water, Specific Humidity in % 0.24 Eqs. (7.7) and (7.8), to those relative to ice, Eq. (8.10), while 0.22 sat = the saturation value itself is continuous, i.e., AAI (Tf,Pf) 0.2 sat AAW (Tf,Pf) at this point. 0.18 We infer from Eqs. (8.5), (8.9) and (8.10), that upon heat- -8 -7 -6 -5 -4 -3 -2 -1 0 1 Temperature41 t /°C ing the ice fraction shrinks at the isobaric melting rate,
! ∂wIh 3 [s] 3 [s] b) Sea-Air Relative Humidity (WMO) SIA SW SI AV AI εP = − = w +w , (8.11) 100 ∂T DS DA wA,wS,P 10 g/kg 99 20 g/kg or, when compressed, at the isothermal melting rate, 30 g/kg 98 40 g/kg Ih ! ∂w 3SI [v] 3AI [v] 50 g/kg SIA SW AV 97 εT = − = −w −w .(8.12) 60 g/kg ∂P DS DA wA,wS,T 70 g/kg 96 80 g/kg 95 With the help of Eqs. (8.5–8.12) we can now compute the 90 g/kg first and second derivatives of the Gibbs function (8.2) for a 100 g/kg 94 system composed of seawater, ice, and humid air. 110 g/kg 93 SIA
Relative Humidity in % The specific entropy of sea ice air, s , follows as 120 g/kg ! 92 ∂gSIA sSIA = − = wAVsAV +wSWsSW +wIhsIh, (8.13) 91 ∂T wA,wS,P 90 -8 -7 -6 -5 -4 -3 -2 -1 0 1 the enthalpy is Temperature t /°C SIA SIA SIA AV AV SW SW Ih Ih h = g +T s = w h +w h +w h , (8.14) Fig. 10: Specific (panel a) and relative (panel b) humidity of sea air, i.e., humid air in Fig. 10.equilibriumSpecific with seawater,(a) and at sea-level relative pressure,(b) humidityP = 101325 Pa, of as seaa function air, of i.e., and the specific volume humidtemperature air in for equilibrium different absolute with salinities seawater, as indicated at by sea-level the curves. The pressure, equilibrium air fraction A is computed from Eq. (6.4); the resulting specific humidity is q = (1 – A). SIA ! P =101 325 Pa, as a function of temperature for different absolute SIA ∂g AV AV SW SW Ih Ih The relative humidity RH WMO is determined from A by the WMO definition (10.4) v = =w v +w v +w v . (8.15) salinitieswith the as saturated indicated air fraction by the Asat curves. given by Eq. The (8.7). equilibrium The specific humidity air fraction related to ∂P Asat is displayed as the bold curve “Ice” in panel a), indicating the saturation of sea-ice wA,wS,T A is computedair due to ice formation from Eq. below (6.4); the freezing the resultingtemperature at specific the particular humidity salinity. is q =(1−A). The relative humidity RHWMO is determined from A by Thus, the first derivatives of the Gibbs function are strictly sat additive with regard to the phases present. the WMO definition (10.4) with the saturated air fraction A given SIA byFrom Eq. the (8.7).total derivative The specificof Eq. (8.6), humidity i.e. the Clausius-Clapeyron related to A differentialsat is displayed equation for as sea For the second temperature derivative of g , exploiting ice, the bold curve “Ice” a), indicating the saturation of sea-ice air due Eqs. (8.13), (8.3), (8.4) we have to ice formation below∂ the freezing temperature∂ at ∂ the particular ! " Λ [] = = Λ [] + Λ g + Λ g SIA SIA AV d SI g 0 SI g d SA SI dT SI dP (8.8) cp ∂s ∂s salinity. ∂S ∂T ∂P AV A T ,P SA ,P SA ,T = = w (8.16) T ∂T ∂T wA,wS,P A,P we infer the partial derivatives for the change of the brine salinity, SA(T, P), independent of air, # " ! ∂sAV ∂A ∂sSW we infer the partial derivatives for the change of the brine + + SW ∂S Λ [s] ∂S Λ [v] w salinity, SA (T= −,SP)SI, independent, ofA air,= S SI (8.9) ∂A ∂T A S ∂T ∂ A A ∂ A T ,P w ,w ,P T P DS P T DS SA,P SW ! # Ih ! where∂S ADS is defined in Eq.3 (6.9).SI [ s] ∂SA 3SI [v] ∂s ∂SA Ih ∂s = −SA , = SA (8.9) + +w ∂T DS ∂P DS ∂SA ∂T A S ∂T P T T ,P w ,w ,P P where D is defined in Eq. (6.9). wA ∂A wS ∂S S −sAV −sSW A For ice air we get from Eq. (8.7) the saturated value for the 2 2 A ∂T wA,wS,P SA ∂T wA,wS,P air fraction, A = Asat (T,P ), with respect to ice, independent ! AI ∂wIh of the presence of seawater. In the same way as in Eq. (8.8) +sIh ∂T we can derive the Clausius-Clapeyron differential equation wA,wS,P
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic properties of sea air 111 from which we obtain the formula for the isobaric heat ca- 9 Properties of ice air pacity, In the limit of zero salinity, the composite system “sea ice SIA = AV AV + SW SW + Ih Ih cp w cp w cp w cp (8.17) air” described in the previous section turns into “wet ice air”, ( 2 2 ) i.e. the equilibrium of liquid water, ice and vapour in the pres- AV (3AI [s]) SW (3SI [s]) +T w +w . ence of air. When there is no air, wA=0, temperature and DA DS pressure of this system equal the triple-point temperature and In the scientific literature, we are not aware of a pressure of water, while the mutual mass ratios of the three thermodynamically rigorous definition of the latent heat phases are controlled by two additional constraints such as that occurs in conjunction with the exchange of wa- the volume and the total entropy of the sample. When air is ter between seawater, humid air and ice. We define added, the partial vapour pressure P V will remain close to = V AV here the latent-heat part of the heat capacity (8.17), the triple-point pressure but the total pressure, P P /xV , AV 2 SW 2 T w (3AI [s]) /DA +w (3SI [s]) DS , divided by the Eq. (5.6), of such an air parcel will be different, Fig. 11. This isobaric melting rate, i.e. the mass fraction loss of ice, state is controlled by Eqs. (8.5–8.7) at zero salinity, i.e., − ∂wIh/∂T from Eq. (8.11), as the isobaric latent wA,wS,P W Ih SIA 3WI [g] ≡ g −g = 0 (9.1) heat of ice, LP , of this system, wAV (3 [h])2 /D +wSW (3 [h])2 /D LSIA = AI A SI S . P AV SW (8.18) AV w 3AI [h]/DA +w 3SI [h]/DS AV ∂g Ih 3AI [g] ≡ g −A −g = 0. (9.2) This expression includes both the latent heats of melting ∂A T ,P (subscript SI) and of sublimation (AI), and only indirectly This system of equations can be solved for the temperature that of evaporation (AS). Rather than simply being added T (A) and the pressure P (A) as functions of the air fraction up, the transition enthalpies appear averaged, weighted by A. sublimation and melting rates. For freshwater (wS=0), this SIA The three mass fractions of the parcel’s phases, liquid wa- formula for LP reduces to the sublimation enthalpy in air, ter, wW, ice, wIh, and saturated humid air, wAV = wA/A, 3AI [h], are related to temperature and pressure via the mass frac- ∂hAV tion A(T , P) of dry air in humid air, i.e., to the solution of AI = [ ] ≡ AV − − Ih LP 3AI h h A h . (8.19) Eqs. (9.1), (9.2): ∂A T ,P A A w Alternatively, for air-free conditions (w =0), it provides the wW +wIh + = 1. (9.3) melting enthalpy in seawater, 3SI [h] A A SW ! At a given air fraction w and entropy s, Fig. 12, SI SW ∂h Ih LP = 3SI[h] ≡ h −SA −h . (8.20) ∂SA wA T ,P s = wWsW (T,P )+wIhsIh (T,P )+ sAV (A,T,P ) (9.4) A The expressions for the latent heat must be independent of the freely adjustable coefficients. It is easily verified that this system of wet ice air still possesses one degree of free- Eqs. (8.18–8.20) satisfy this necessary condition. In all dom. We term the pressure it takes at complete melting, cases, using the simple difference between the enthalpies wIh=0, the isentropic freezing level (IFL) of wet air, and at of ice and seawater or humid air rather than Eqs. (8.19), complete freezing, wW=0, the isentropic melting level (IML) (8.20), would be essentially wrong for this reason. In other of ice air. For sea air with entropy and air fraction com- words, the numerical values of the additional saline enthalpy puted from Eqs. (6.4) and (6.18), these curves are displayed × SW in Fig. 17. term SA ∂h /∂SA T ,P or the humid-air enthalpy term × AV At pressures below the IML, the liquid phase has disap- A ∂h /∂A T ,P depend on the arbitrary choices made for the adjustable coefficients and must not be neglected. peared and the system reduces to “ice air”. When changes in T or P cause a certain water mass to be transferred between ice and the two fluid phases, there is 10 Relative humidity and fugacity no additional direct transfer of water between those fluids, seawater and humid air, i.e., Eq. (8.18) covers the latent heat Relative humidity is not uniquely defined in the literature. of all three phases below the freezing point. This means that Sometimes it is defined as the ratio of the actual partial pres- Eq. (8.18) can also be expressed in terms of the transition sure of vapour in air to the saturated vapour pressure, and properties of the other two possible phase pairs, sublimation sometimes as the ratio of their corresponding mole fractions (AI) and evaporation (SA), or melting (SI) and evaporation (Van Wylen and Sonntag, 1965; Sonntag, 1982). All defi- (SA), using the relation (6.6), 3SA = 3SI −3AI. nitions give the same results in the ideal-gas limit. Also in www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 112 R. Feistel et al.: Thermodynamic properties of sea air 45 47
a) Wet-Ice-Air Pressure a) Entropy of Ice Air at 1013.25 hPa 2000 200
1000 0
) 90%
-1 80% -200 500 K 70% -1 60% -400 50% 200 -600 / hPa / 40% / (J kg s P P 30% -800 100 20% 20% -1000 10% 50 -1200 Pressure Pressure -1400 20 -1600
10 Specific Entropy -1800 5 -2000 0 10 20 30 40 50 60 70 80 90 100 -100 -90 -80 -70 -60 -50 -40 -30 -20 -10 0 Air Fraction A in % Temperature t /°C
b) Wet-Ice-Air Temperature 0.01 b) Entropy of Ice Air at 500 hPa 90% 200 0.008 80% 0 0.006 )
-1 70% -200
K 60% 0.004 -1 50% -400 / °C /
t t 0.002 40% -600 / (J kg
s 30% 0 30% -800 20% -0.002 10% -1000
Temperature -0.004 -1200
-0.006 -1400 -1600 -0.008 Specific Entropy -1800 0 10 20 30 40 50 60 70 80 90 100 -2000 Air Fraction A in % -100 -90 -80 -70 -60 -50 -40 -30 -20 -10 0 Temperature t /°C
Fig. 11. Equilibrium pressure P , panel (a), and temperature T , Fig. 12. Entropy of ice air as a function of temperature at panel (b), as a function of the mass fraction A of dry air in humid ◦ air of a parcel containing liquid water, ice and humid air. At A=0, 1013.25 hPa (a) and 500 hPa (b) between −100 C and the melt- A the curve ends in the common triple point of water at about 611 Pa ing point of the solid component for dry-air fractions w of ice air and 273.16 K. Note that the dissolution of air in liquid water is not between 10% and 90% as indicated by the curves. considered here which may have comparable additional effects on the freezing temperature (Doherty and Kester, 1974; IAPWS, 2004; mosphere at some observed temperature, to the saturation Feistel, 2008a). vapour pressure of pure water at this temperature (Calvert, 1990; IUPAC, 1997). For a real-gas mixture such as air, this approximation, relative humidity is a property of fluid partial pressures of its components are defined by the total water at given temperature and pressure of the vapour phase, pressure multiplied by the mole fraction of that component independent of the presence of air. (Lehmann et al., 1996; IUPAC, 1997) The CCT10 definition of relative humidity is in terms of a = mole fraction: at given pressure and temperature, the ratio, P xaP. (10.1) expressed as a percent, of the mole fraction of water vapour This definition of the relative humidity takes the form to the vapour mole fraction which the moist gas would have if it were saturated with respect to either water or ice at the AV xV same pressure and temperature. Consistent with CCT, IU- RHCCT = (10.2) xAV,sat PAC11 defines relative humidity as the ratio, often expressed V as a percentage, of the partial pressure of water in the at- AV with regard to the mole fraction of vapour xV (A) from sat 10CCT: Consultative Committee for Thermometry, www.bipm. Eq. (5.6) and the saturated air fraction A (T , P) from org/en/committees/cc/cct/. Eq. (7.5) with respect to liquid water and from Eq. (8.7) with 11IUPAC: International Union of Pure and Applied Chemistry, respect to ice. The pressure derivative provides the rate of www.iupac.org. relative humidification upon adiabatic uplift,
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ 48
Fig. 12: Entropy of ice air as a function of temperature at 1013.25 hPa (Panel a) and 500 hPa (Panel b) between –100 °C and the melting point of the solid component for R. Feisteldry-air etfractions al.: w ThermodynamicA of ice air between 10% propertiesand 90% as indicated of sea by the air curves. 113 50
Dry-Air Fraction Range of Humid Air and Ice Air Dry-Air Fraction of Humid Air at 101325 Pa 100 HUMID AIR 100 99 1013 99.5 10 % 50 98 0 h Pa 97 99 20 % 96 2 0 30 % 0 h 95 P a 98.5 40 % 94 93 98 50 % 92 60 % 1 97.5 91 0 ICE AIR 0 Air inFraction % h Air inFraction % 70 % 90 P a 97 80 % 89 88 90 % 96.5 87 100 % 100 % 86 96 85 -60 -55 -50 -45 -40 -35 -30 -25 -20 -15 -10 -5 0 0 5 10 15 20 25 30 35 40 45 50 55 60 Temperature t /°C Temperature t /°C sat ( ) Fig. 13: Saturation curves AAI T, P computed by solving Eq. (118) at the pressures Fig. 13.1013.25,Saturation 500, 200 and 100 curves hPa, as indicated.Asat (T,P Betwee) ncomputed –60 °C and the by melting solving Fig. 14: Mass fraction A of dry air in humid air as a function of temperature at nomal temperature of ice, these curves separateAI the physically reasonable dry-air fractions, Fig.pressure, 14. 101325Mass Pa, fractionfor differentA relativeof dry humidit airies in (WMO humid definition, air as Eq. a function10.4) as indicated of Eq. (9.2)A ≥ A atsat (T the, P), pressuresof the single-phase 1013.25, state of humid 500, air 200 from and those100 of the hPa, two-phase as in-state by the curves from 10% to 100% (dewpoint). Specific humidity is q = 1 – A. Below the AI ◦ temperature at nomal pressure, 101 325 Pa, for different relative hu- dicated.of ice Betweenair, wA ≤ Asat (−T,60P) . AtC the and saturation the point, melting the two temperature systems coincide of. ice, dewpoint curve (100%), liquid water is present, i.e., the stable state is wet air rather than AI midities (WMO definition, Eq. 10.4) as indicated by the curves from these curves separate the physically reasonable dry-air fractions, humid air. 10% to 100% (dewpoint). Specific humidity is q=1−A. Below the ≥ sat A 10.A RelativeAI (T,P Humidity), of theand single-phaseFugacity state of humid air from those dewpoint curve (100%), liquid water is present, i.e., the stable state A ≤ sat The adiabatic humidification rate, i.e. the rate of increase of relative humidity of an ofRelative the two-phase humidity is not state uniquely of icedefined air, inw the literature.AAI (SometimesT,P ). At it is the defined saturation as the ratio isadiabatically wet air ratherlifted air than parcel humid follows from air. Eqs. (10.4) and (7.9) as point,of the actual the twopartial systems pressure of coincide.vapour in air to the saturated vapour pressure, and sometimes ∂RH r as the ratio of their corresponding mole fractions (Van Wylen and Sonntag, 1965; Sonntag, χ()A,T, P = − WMO = ()δ AW + ΓAV δ AW . (10.5) 1982). All definitions give the same results in the ideal-gas limit. Also in this approximation, ∂ sat 2 T P P A,s ()1− A relative humidity is a property of fluid water at given temperature and pressure of the vapour AW
phase, independent of the presence of air. Sometimes, especially when considering phase or chemical equilibria, it is more convenient to 10 use the fugacity (or activity)∂RH ratherWMO than partial pressure (Lewis, 1908; Glasstone, 1947; The CCT definition of relative∂RH humidityCCT is in terms of mole fraction: At given pressure and = − χMöbius(A,T,P and Dürselen,) = − 1973; Ewing et al., 1994; IUPAC, 1997; Blandamer et al., 2005).(10.5) The χtemperature,(A,T,P the) ratio, expressed as a percent, of the mole fraction of water vapour to(10.3) the ∂P fugacity of vapour in humid air is∂P defined as, Eq. (5.31), vapour mole fraction which the moist gas wouldA,s have if it were saturated with respect to A,s r AV W AW V AV AW 10 x M = µ +(A,T, P) CCT: ConsultativeV Committee for Thermometry,AW www.bipm.org/en/committees/cc/cct/AV AW ()()= 0 δT 0 δP . = + fV A,T, P fV2T exp . (10.6) δT 0 δP . − sat R T A sat2 1 AAW W M 1−A V Sometimes,The chemical potential especially of vapour in when humid air, considering µ , is given in Eq. phase (5.15). orRW is chemical the specific AW gas constant of water. The reference fugacity, Here, the drying rates δ with respect to liquid water and equilibria, it is more convenient to use the fugacity (or ac- AV the lapse rate 0 of humid air are defined in Eqs. (7.7), (7.8) tivity) rather than partial pressure (Lewis, 1908; Glasstone, AW and (5.25). Below the freezing point, δ must be replaced 1947; Mobius¨ and Durselen,¨ 1973; Ewing et al., 1994; IU- AI by δ with respect to ice, Eq. (8.10). PAC, 1997; Blandamer et al., 2005). The fugacity of vapour 12 The WMO definition of the relative humidity is (Rogers in humid air is defined as, Eq. (5.31), and Yau, 1989; Pruppacher and Klett, 1997; Jacobson, 2005), µV (A,T,P ) f (A,T,P ) = f 0 (T )exp . (10.6) V V R T r 1/A−1 W RHWMO = = (10.4) rsat 1/Asat −1 The chemical potential of vapour in humid air, µV, is given in Eq. (5.15). R is the specific gas constant of water. The V A W where r = (1−A)/A = m /m is the humidity ratio. The reference fugacity, relation (10.4) between air fraction, temperature and relative V humidity is shown quantitatively in Fig. 14. 0 µ f (T ) = lim fV (A,T,P )exp − (10.7) AV ≈ A W V → If r is small, we can estimate xV rM /M from P 0 RWT Eq. (5.6) and therefore RH ≈ RH , i.e. approximate ( ) WMO CCT µV,id consistency of Eqs. (10.2) and (10.4). = xVP exp − The adiabatic humidification rate, i.e. the rate of increase RWT of relative humidity of an adiabatically lifted air parcel fol- is chosen such that in the ideal-gas limit of infinite dilution, lows from Eqs. (10.4) and (7.9) as fV converges to the partial pressure of vapour (Glasstone, 1947; Guggenheim, 1967), Eq. (10.1), ( ) µV −µV,id f = xAVP . 12 V V exp (10.8) WMO: World Meteorological Organisation, www.wmo.int. RWT www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 114 R. Feistel et al.: Thermodynamic properties of sea air
The ideal-gas chemical potential µV,id is given in Eq. (H13), In first approximation, derived from a series expansion AV = and the mole fraction of vapour in humid air, xV , is given in with respect to salinity, we obtain from Eq. (10.9), mSW S + 2 SW = + Eqs. (5.6) and (B9). SA/M O(SA), and φ 1 O(SA) the linear relation = 0 The ratio λV fV/fV is the absolute activity of vapour (Ewing et al., 1994; IUPAC, 1997). MW ϕSA ≈ − S AV 1 S A (10.15) The fugacity-pressure ratio fV/ xV P is known as the M fugacity coefficient or enhancement factor in meteorology. The saturation fugacity is defined by the equilibrium from Eq. (10.14), i.e. Raoult’s law for the vapour-pressure between liquid water and vapour in air, µV (A,T,P ) = lowering of seawater (Landau and Lifschitz, 1987; Feistel et µW (0,T,P ), i.e. al., 2008b). In the ideal-gas limit, Eqs. (10.14) and (10.15) are valid, too, for the relative humidity, ϕSA ≈ RH. W sat 0 µ (0,T,P ) Below the freezing temperature of pure water at given fV = fV (T )exp , (10.9) RWT pressure, the saturated vapour is defined by the chemical po- tential of ice rather than liquid water, i.e. by where µW = gW(T , P) = gSW (0, T , P) is the chemical po- ( ) tential of liquid water, i.e. its Gibbs energy (3.3). The relative µIh (T,P ) sat = 0 fugacity ϕ of humid air can thus be defined as fV fV (T )exp , (10.16) RWT f µV (A,T,P )−µW (0,T,P ) = V = ϕ sat exp . (10.10) instead of Eq. (10.9). Then, the relative fugacity of sea air is fV RWT SA ( W Ih ) , f µ (S ,T,P )−µ (T,P ) In the ideal-gas limit, µV = µV id, the relative fugacity ϕ ap- SA = V = A ϕ sat exp (10.17) proaches the relative humidity (10.2) because of Eq. (10.8). fV RWT It follows that the relative fugacity of sea air is When the temperature is lowered further to the freezing point f SA µW (S ,T,P )−µW (0,T,P ) of seawater, the exponent of Eq. (10.17) vanishes and the air ϕSA = V = exp A (10.11) sat is saturated, φSA=1, for sea-ice air at any lower temperature. fV RWT since its vapour is assumed to be in equilibrium (6.4) with V W seawater, µ (A, T , P)=µ (SA, T , P). 11 Isentropic expansion of sea-air The chemical potential difference in the exponent is pro- portional to the osmotic coefficient of seawater, φSW, which In an external gravity field, equilibrium states possess verti- is computed from the saline part of the Gibbs function, cally constant temperature and chemical potentials but are Eq. (6.1), as (Feistel and Marion, 2007; Feistel, 2008a), stratified in entropy and concentrations (Landau and Lifs- chitz, 1987). Adiabatically mixed air columns are better " S ! # SW 1 S ∂g approximations of the real atmosphere, characterized by the φ (SA,T,P ) = − g −SA , (10.12) mSWRT ∂SA conjugate properties of constant entropy and concentrations T ,P with temperature and chemical potentials depending on the and mSW is the molality of seawater (Millero et al., 2008), vertical coordinate (Feistel and Feistel, 2006). It must be emphasised that an adiabatically well-mixed air column in S m = A . (10.13) a gravity field is not in thermodynamic equilibrium since SW − S (1 SA)M the irreversible thermodynamic driving forces are the non- We infer for the relative fugacity of sea air the simple formula zero gradients of in-situ temperature and chemical poten- tials, rather than those of potential temperature or concen- trations (Glansdorff and Prigogine, 1971). Due to the slug- SA W SW ϕ = exp −mSWM φ , (10.14) gish molecular relaxation in comparison to turbulent mixing, equilibrium states are prevented from being approached un- which is also known as the activity aW of water in seawater der ambient conditions. While the air column as a whole (Falkenhagen et al., 1971; Millero and Leung, 1976; Feistel therefore remains far from overall equilibrium, each thin iso- and Marion, 2007). Similar to the ideal gas approximation, baric layer is assumed in the following to be in local thermo- the relative fugacity of sea air is independent of the presence dynamic equilibrium. In particular thermodynamic equilib- or the properties of air. In Eq. (10.14), ϕSA ≤ 1 expresses rium is assumed to hold within a boundary layer extending the fact that the vapour pressure of seawater is lower than the only slightly above and below the sea surface. saturation pressure of liquid pure water, i.e., that humid air In the sea-air atmosphere model of this section we con- in equilibrium with seawater above its freezing temperature sider an air column which is in equilibrium with the sea sur- is always subsaturated. face and “vertically” isentropic. The pressure is used here
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ 54
∂T ∂ 2hSA Γ = = . (11.3) ∂ A S ∂ ∂ P w ,w ,s s P wA ,wS R. Feistel et al.: Thermodynamic properties of sea air 115
as the “vertical” coordinate so that gravity is only implic- Sea-Air Isentropes itly considered. The vertical profile of the real atmosphere 1007 is simulated by isentropic expansion of a parcel with given mass fractions of air and water. All thermodynamic proper- 1008 ICL (liqu ties of the vertical profile of the sea-air atmosphere model id) can be computed from three given independent variables, 1009 / hPa / the in-situ temperature at the surface (sea-surface temper- P 1010 ature, SST), the sea-level pressure (SLP), here assumed as 101 325 Pa, and the sea-surface salinity (SSS), here assumed
II CC 1011
LL
Pressure Pressure as 35.16504 g/kg (Millero et al., 2008). (( icic
ee Depending on pressure and entropy as its natural variables, ))
44 33 33 22 22 11 11 55 00 1012
00 55 00 55 00 55 00
°° °°
CC CC
°° °° °° °° °° °° °° enthalpy h is the most convenient thermodynamic potential CC CC CC CC CC CC CC function for the description of adiabatic processes (Feistel 1013 and Hagen, 1995; Feistel, 2008a). The “vertical” isentropic 1.06 1.08 1.1 1.12 1.14 1.16 1.18 1.2 1.22 1.24 1.26 1.28 1.3 1.32 density profile is computed from Density ρ /(kg m -3 )
−1 Fig. 15: Vertical isentropic sea-air profiles of density overlying seawater at standard- ∂h -1 ρ(P ) = (11.1) Fig. 15.ocean salinityVertical (35.16504 isentropic g kg ) and sea-air sea-level profiles pressure (101325 of density Pa) for different overlying SST values between 0 and 40 °C as indicated. The related isentropic− 1condensation levels ∂P A seawater at standard-ocean salinity (35.16504 g kg ) and sea-level w ,s (ICL) of liquid water and ice (bold lines) are also shown. ◦ pressure (101 325 Pa) for different SST values between 0 and 40 C and the isentropic temperature profile (Fig. 16) from as indicated. The related isentropic condensation levels (ICL) of liquid water and ice (bold lines) are55 also shown. ∂h T (P ) = . (11.2) ∂s wA,P Sea-Air Isentropes 1007 Here, wA is the mass fraction of dry air, h the enthalpy and s the entropy of either humid air or of the composite systems 1008 (liquid) wet air, ice air, or wet ice air. Solving Eqs. (7.25), (7.26), the ICL subsaturated equilibrium humidity of sea air (Fig. 3) results 1009 / hPa /
in an isentropic condensation level (ICL) of 4–5 hPa below P surface pressure (Figs. 15, 16). In Earth’s atmosphere, this 1010 corresponds to an altitude of about 30–40 m above the sea 1011
) ) surface. Pressure ee
cc
ii
((
Below the dewpoint temperature, the sea-air potential LL
CC must be replaced by the wet-air potential (7.1), and be- II 1012 low the frost point it is replaced by the corresponding ice- 1013 air potential. Note that in doing this, we are consider- -5 0 5 10 15 20 25 30 35 40 45 ing condensed/frozen water as a floating, not precipitating Temperature t /°C aerosol/fog/cloud. Recall that any fallout from the sample is neglected by the model approach of an isentropically ex- Fig. 16: Vertical isentropic sea-air profiles (almost vertical thin lines) of temperature Fig. 16.for differentVertical SST values isentropic between 0 sea-air and 40 °C profiles at standard-ocean (almost salinity vertical and sea-level thin panded, gravity-free parcel. lines)pressure of temperature of 101325 Pa, for together different with the SST related values isentropic between condensation 0 and levels 40 (ICL)◦C of liquid water and ice (bold lines). Below the freezing temperature of seawater, sea The adiabatic lapse rate of sea air at the surface is available at standard-oceanair is saturated at the salinity sea surface. and The sea-level slope of the pressure isentropes ofis given 101 by 325 the Pa,adiabatic to- from the formula getherlapse with rate, the Eqs. related (6.25), (6.26). isentropic condensation levels (ICL) of liq-
! uid water and ice (bold lines). Below the freezing temperature of ∂T ∂2hSA 0 = = . (11.3) seawater, sea air is saturated at the sea surface. The slope of the ∂P A S ∂s∂P isentropes is given by the adiabatic lapse rate, Eqs. (6.25), (6.26). w ,w ,s wA,wS
the liquid or solid water phase, neither at the sea surface nor 12 Discussion within clouds (Korolev and Isaac, 2006). Thermodynamics can be used to estimate the distance from equilibrium and the The isentropic expansion of sea air considered in the previ- related irreversible fluxes. ous section represents a rather idealized model of the marine During the oceanographic expedition AMOR-92 of r/v atmosphere. In this section, we consider for illustration pur- “A. v. Humboldt” in the late summer of 1992 in the Atlantic poses some examples taken from observations and compare coastal upwelling region off Morocco (Hagen et al., 1996), them with related properties of the sea-air model. Frequently, regular radiosonde sampling of the atmosphere was carried the ambient atmosphere is not in an equilibrium state with out. To provide comparisons with examples of real maritime www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 116 R. Feistel et al.: Thermodynamic properties of sea air atmospheric profiles, we have selected here two casts as de- Table 1. Two selected radiosonde profiles taken off Morocco in scribed to Table 1 and shown in Fig. 19. In RS #37 we see September 1992 on r/v “A. v. Humboldt”. The sea-surface salinity approximately isentropic conditions consistent with the lo- SSS is given on the 1978 Practical Salinity Scale (PSS-78) which is cal surface conditions at the sight. However, in the night converted to the Absolute Salinity SA=SSS×uPS used in this paper −1 time outside the upwelling filament (RS #14), the conditions by the factor uPS=(35.16504/35) g kg (Millero et al., 2008; IOC, strongly deviate from the idealized local isentropic condi- 2010). tions indicated by the vertical line. The presence of Sahara dust in the local atmosphere at this time indicates that certain Radiosonde RS #14 RS #37 air layers were advected from the continent. Note that the Date 17.09.92 21.09.92 near-surface air is almost saturated, likely due to radiative UTC 04:54 12:28 cooling. Lat ◦ N 31.96 31.00 In Fig. 19, the entropy profiles computed from radiosonde Long ◦ W 11.01 10.17 data are compared with the sea-air entropy computed from Wind vel (m/s) 9.6 2.7 the related measured sea-surface salinity (SSS), sea-surface Wind dir (deg) 27 18 temperature (SST) and sea-surface pressure, Table 1. Clouds Sc, tr, Cu, fra Ci, fib As another example measured over the tropical Atlantic, a Cover 10/10 1/10 radiosonde profile launched at 15:47 UTC on 7 March 2004 P(hPa) 1014.0 1017.8 ◦ ◦ T-dry (◦C) 21.2 16.9 off South America at 9.85797 N, 33.11862 E is selected ◦ from the AEROSE-I cruise (Nalli et al., 2005; Morris et SST ( C) 22.3 17.3 SSS 36.96 36.23 al., 2006) and displayed in Fig. 20. The sea-surface tem- ◦ Remark Sahara dust dust perature registered by the vessel was 26.28 C, the absolute Upwelling no yes salinity 36.22 g/kg (Practical Salinity 36.05). The surface pressure was 1011.33 hPa, the relative humidity was 70.2%, 56 much lower than the related equilibrium sea-air relative hu- midity, Fig. 3. In the near-surface atmosphere between 1000 Sea-Air Isentropic Freezing & Melting Level and 930 hPa, entropy and air fraction form an almost homo- 200 geneous layer which is characteristic for isentropically mix- ing or rising air. Since radiosondes cannot measure the con- densed fraction of wet or ice air above the condensation level, 300 ) L the displayed profiles reflect the gaseous part only. In com- IM ( ) g L) in L / hPa / ti IF l ( parison to equilibrium conditions at the sea surface (indicated e g 400 P P M in zi e re by the vertical lines), the ambient air had lower entropy and F specific humidity. 500 Over most ocean regions, surface relative humidity has rel- Pressure Pressure 600 atively small spatial and inter-annual variations; it is typi- 700 cally within 75%–82% during all seasons (Dai, 2006). In 800 contrast, the global warming signal is observed in the to- 900 tal atmospheric moisture content over the oceans that has 1000 increased by 0.41 kg/m2 per decade since 1988 (Santer et -5 0 5 10 15 20 25 30 35 40 45 Sea-Surface Temperature t /°C al., 2007), while at the same time the upper-ocean salin- ity is rising over large parts of the global ocean (Curry et Fig. 17: Isentropic freezing level (IFL) and melting level (IML) of sea air with Fig. 17. Isentropic freezing level–1 (IFL) and melting level (IML) of al., 2003; Stott et al., 2008). This effect counteracts the in- standard-ocean salinity (35.16504 g kg ) as a function of the sea-surface temperature sea air(SST), with computed standard-ocean from Eqs. (9.3), salinity (9.4) with (35.16504 entropy and g air kg fraction−1) as computed a function from creasing freshwater flux from melting glaciers and polar ice Eqs. (6.4) and (6.18). At pressures higher than IFL, the condensed part is liquid, at of thepressures sea-surface lower than temperature IML, the condensate (SST), is ice. computed Between the two from curves, Eqs. the solid, (9.3), caps, as described by the “osmotic potential” of Cochrane (9.4) withliquid and entropy gas phase and of water air fractioncoexist. Both computed curves begin from at the condensation Eqs. (6.4) level and and Cochrane (2009). Durack and Wijffels (2009) found (ICL), Fig. 16, and do not reach the sea surface. Note that the local temperature (Fig. (6.18).18) At is always pressures very near higher 0 °C in than the mixed-phase IFL, the condensedregion between partIML and is liquid,IFL. at that the surface salinity of the global ocean has generally pressures lower than IML, the condensate is ice. Between the two been increasing in arid (evaporation-dominated) regions and curves, the solid, liquid and gas phase of water coexist. Both curves freshening in humid (precipitation-dominated) regions, with begin at the condensation level (ICL), Fig. 16, and do not reach the a spatial distribution similar to that of the surface salinity sea surface. Note that the local temperature (Fig. 18) is always very ◦ anomalies relative to the spatial mean over the globe. This near 0 C in the mixed-phase region between IML and IFL. has led them to suggest that the global hydrological cycle has accelerated over the past few decades. The explanation for climatological trends in surface salinity in specific regions In non-equilibrium situations that are usually found at the such as the brackish Baltic Sea estuary can be significantly air-sea interface, Figs. 19 and 20, thermodynamic fluxes more complicated (Feistel et al., 2008a). are driven by Onsager forces such as the gradient of
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic57 properties of sea air 117 59
Sea-Air Isentropes Entropy Profile of RS 14 200 200
ICE AIR WET AIR
300 300 / hPa /
400 hPa / P P 400 P P
500 500
Pressure Pressure 600
Pressure Pressure 600 700 700 800 800 900 900 1000 1000 -40 -35 -30 -25 -20 -15 -10 -5 0 5 10 15 20 25 30 35 40 100 120 140 160 180 200 220 240 260 280 300 Temperature t /°C Specific Entropy s / (J kg -1 K -1 )
Fig.Fig. 18: 18. VerticalVertical isentropic isentropic sea-air profiles sea-air of te profilesmperature for of different temperature SST values for between differ- – Entropy Profile of RS 37 ent40 and SST +40 values°C at standard-ocean between salinity−40 and(35.16504 +40 g◦ kgC-1 at) and standard-ocean sea-level pressure (101325 salinity 200 Pa), beyond the related−1 isentropic condensation level shown in Fig. 16. Note that the pressure (35.16504range in Fig. 16 g is kg compressed) and into sea-level a very thin pressure layer at the (101bottom 325 of this Pa), plot.beyond The isentropic the relatedtransition isentropicbetween liquid condensationand solid condensate, level between shown IFL and in IML Fig. in Fig. 16. 17, Note has an that extremely small lapse rate and appears here as a pressure jump, i.e. as an almost isothermal thelayer pressure in which the range solid, liquid inFig. and vapour 16 is phase compressed of water coexist, into Fig. a 11b. very thin layer 300 at the bottom of this plot. The isentropic transition between liquid and12. solid Discussion condensate, between IFL and IML in Fig. 17, has an ex- hPa / 400 tremely small lapse rate and appears here as a pressure jump, i.e. P The isentropic expansion of sea air considered in the previous section represents a rather asidealized an almost model of isothermal the marine atmosphere. layer in Inwhich this section, the we solid, consider liquid for illustration and vapour 500 phasepurposes of some water examples coexist, taken from Fig. observations 11b. and compare them with related properties
of the sea-air model. Frequently, the ambient atmosphere is not in an equilibrium state with Pressure 600 the liquid or solid water phase, neither at the sea surface nor within clouds (Korolev and Isaac, 2006). Thermodynamics can be used to estimate the distance from equilibrium and the 700 related irreversible fluxes. µ/T (Glansdorff and Prigogine, 1971; De Groot and Mazur, 800 1984).During the oceanographic At the sea expedition surface, AMOR-92 assuming of r/v “A.v. the Humboldt” same in temperature the late summer of 900 1992 in the Atlantic coastal upwelling region off Morocco (Hagen et al., 1996), regular 1000 andradiosonde pressure sampling on of the both atmosphere sides was of carried the interface, out. To provide the comparisons dimensionless with 100 120 140 160 180 200 220 240 260 280 300 examples of real maritime atmospheric profiles, we have selected here two casts as described Specific Entropy s / (J kg -1 K -1 ) Onsagerto Table 1 and force shown Xin Fig.SA (19.A,S In RSA ,T,P#37 we see) driving approximately the isentropic transfer conditions of water isconsistent the difference with the local surface between conditions the at chemical the sight. However, potentials in the night of time water outside in the humid air and in seawater, Fig. 19. Entropy of two radiosonde profiles taken on the subtropical Atlantic off Morocco, Table 1, computed from Eq. (5.16), neglect- µ µV (A,T,P ) µW (S ,T,P ) ing any unknown condensed fraction, compared with the related = = AV − A XSA 1 (12.1) sea-air entropy, computed from ocean surface properties by means RWT RWT RWT of the equilibrium Eq. (6.4) and shown here as vertical lines. The cond large difference in the upper panel probably results from strong off- It vanishes at the condensation point, A = A (SA, T , P), Eq. (6.4), rather than at saturation. Equation (12.1) can be shore wind that also carried Sahara dust observed at this time. expressed in terms of fugacities, Eqs. (10.10) and (10.11), in the form 13 Summary ϕ(A) X = = m MWφSW + ϕ(A). SA ln SA SW ln (12.2) ϕ (SA) The broad aims of this paper are twofold. First, to provide Rather than the relative humidity, Eqs. (10.2), (10.4), the a collection of equations for various properties of equilib- ria between seawater, ice and humid air, derived directly sea-air Onsager force XSA, in conjunction with the formula (6.28) for the evaporation enthalpy of seawater, is relevant from the thermodynamic potentials for the elementary com- for the parameterization of non-equilibrium latent heat fluxes ponents. Second, to review information on sea air condi- across the sea surface. In the special case of limnological ap- tions and provide a best estimate of the sea-air potential func- plications, or below the freezing point of seawater, it reduces tion(s), expressed in different forms, based on previously published work. Very accurate and comprehensive formu- to XSA = lnϕ(A), which corresponds to the relative humid- lations of these potentials have recently become available ity, ln(RHCCT), in the ideal-gas approximation. (IAPWS, 2008, 2009a, b; Lemmon et al., 2000; Feistel et al., 2008b) and permit the consistent computation of all their thermodynamic single-phase properties as well as of their www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 118 R. Feistel et al.: Thermodynamic properties of sea air 61
Air Fraction Profile of AEROSE 04030715 namic relations. Consequently, it is a fundamental feature 200 of our approach that the quantitative accuracy of the ther- modynamic potentials used as “inputs” is not relevant to the mathematical correctness of the fundamental thermodynamic 300 relations which are the primary subject of this paper. Because of our focus on general relations that follow from exact ther- / hPa / 400 P P modynamic principles, we do not discuss the correctness of any particular selection taken from the various published em- 500 pirical geophysical correlation equations. In most cases, the
Pressure Pressure 600 verifications of those empirical equations have been achieved 700 through many practical applications as discussed in the liter- 800 ature. Similarly, we do not discuss the mutual consistency 900 of examples for pairwise and higher-order combinations of 1000 97.5 97.75 98 98.25 98.5 98.75 99 99.25 99.5 99.75 100 those correlations in order to, say, demonstrate the higher ac- Air Fraction in % curacy of the potential functions we employ.
The relations considered here constitute the mathemati- Entropy Profile of AEROSE 04030715 cal “processing pipeline” applied to extract from the given 200 “input” the various special properties of interest. If im- proved formulations for any of the chosen potential func- tions become available in the future, these “inputs” may be 300 substituted for our current choices without any fundamental changes of the relations collected and published in this pa- / hPa / 400 P P per. Nevertheless, we note that the potential functions that 500 we recommend here are (or are planned to be) formulated in officially endorsed IAPWS documents and represent interna- Pressure Pressure 600 tionally recognized standards that possess distinctively high 700 reliability and accuracy. 800 Starting from those very few but comprehensive formula- 900 1000 tions, all thermodynamic properties can be derived (within 100 120 140 160 180 200 220 240 260 280 300 the range of validity and the related uncertainty) in a consis- Specific Entropy s / (J kg -1 K -1 ) tent and highly accurate way. Based on this approach, stud- ies of different authors using these properties will be much Fig. 20. Profiles of air fraction and entropy of the radiosonde pro- more directly comparable. We also note that although lim- files AEROSE 04030715 taken on 7 March 2004 15:47 UTC in ◦ ◦ itations of space and time have not permitted it, a virtually the tropical Atlantic at 9.85797 N, 33.11862 E showing an isen- unlimited set of tailored correlation equations can be derived tropic surface layer (Courtesy Nicholas R. Nalli, NOAA). The ver- for special applications from the exact thermodynamic rela- tical lines indicate the values computed for the humid-air part from the sea-air equilibrium at the observed sea-surface temperature of tions and the chosen potential functions, even for properties 26.28 ◦C and salinity of 36.22 g/kg, Eqs. (6.4) and (6.18). The air for which direct measurements are unavailable or show sig- fraction A on the abscissa relates to specific humidity, q=1−A. nificant uncertainties (e.g., sublimation pressures at very low temperatures or freezing points at high pressures). It should be noted that the two parts, i.e., the empirical pri- various combinations in mutual phase equilibria. The for- mary standard and the set of rigorous thermodynamic formu- mulas focus in particular on systems having seawater as one las, can be advanced essentially independently. That is, new component, such as sea ice, sea air or sea-ice air, and also functions based on the fundamental thermodynamic relations cover the traditional meteorological application for the limit- can be introduced into user libraries (e.g., Feistel et al., 2009; ing case of vanishing salinity. Wright et al., 2009) and/or new or extended versions of the In this paper we suggest an approach that is conceptually empirically determined thermodynamic potentials can be in- (and practically) different from the common approach of us- troduced without directly affecting the other part. All that is ing a collection of separate empirical equations for properties required is that a standard interface be established to com- of interest. In particular, we describe how a small number of municate information between the two parts. For example, a previously published potential functions can be consistently mass-based Gibbs function with its first and second deriva- combined with each other and exploited mathematically to tives, inputs of Absolute Salinity, absolute ITS-90 tempera- calculate the wide range of thermodynamic properties of in- ture and absolute pressure can be replaced by a revised or terest in oceanography and meteorology. Most of the equa- completely new function with these same properties without tions that we consider are expressions of exact thermody- requiring any other changes.
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic properties of sea air 119
Table A1. Chemical composition of sea salt (Millero et al., 2008). The Helmholtz function (5.2) of humid air is composed Mole fractions are exact by definition, mass fractions are rounded here of the Helmholtz functions of dry air and of fluid water to seven digits behind the period. Uncertainties of the molar masses with additional second and third cross virial coefficients de- (Wieser, 2006) are given in brackets. scribing the air-water interaction, i.e. non-ideal properties of humid air, Fig. 1. Mole Mass Molar mass The Gibbs function (6.2) of sea-air describes a composite Solute fraction fraction g mol−1 system of seawater and humid air in mutual thermodynamic + equilibrium, controlled by the Clausius-Clapeyron Eq. (6.7). Na 0.418 8071 0.306 5958 22.989 769 28(2) Mg2+ 0.047 1678 0.036 5055 24.3050(6) Subsequently, formulas for several properties of sea air are Ca2+ 0.009 1823 0.011 7186 40.078(4) derived from the Gibbs function, in particular the latent heat K+ 0.009 1159 0.011 3495 39.0983(1) of seawater, Eq. (6.28), Fig. 5. Sr2+ 0.000 0810 0.000 2260 87.62(1) In the limit of vanishing salinity, sea air reduces to wet air, Cl− 0.487 4839 0.550 3396 35.453(2) i.e. saturated humid air in equilibrium with condensed water. 2− SO4 0.025 2152 0.077 1319 96.0626(50) The Gibbs function of wet air, Eqs. (7.1) and (7.4), provides − HCO3 0.001 5340 0.002 9805 61.016 84(96) various properties of central interest in meteorology, in par- Br− 0.000 7520 0.001 9134 79.904(1) ticular the saturation point (7.5), Figs. 8 and 9. The humid-air 2− CO3 0.000 2134 0.000 4078 60.0089(10) part of sea air is subsaturated, Fig. 3. The subsaturation of sea − B(OH)4 0.000 0900 0.000 2259 78.8404(70) air can be quantified by the relative humidity, Eqs. (10.2) and F− 0.000 0610 0.000 0369 18.998 403 2(5) (10.4), in two different standard definitions, or by the relative OH− 0.000 0071 0.000 0038 17.007 33(7) fugacity, Eqs. (10.10) and (10.14). B(OH)3 0.000 2807 0.000 5527 61.8330(70) Below the freezing temperature of seawater, sea air con- CO2 0.000 0086 0.000 0121 44.0095(9) tains ice Ih as a third phase. Its Gibbs function, Eq. (8.2), Sea salt 1.000 0000 1.000 0000 31.404(2) and the two Clausius-Clapeyron equations, Eqs. (8.8) and (6.7), are used to derive equations for related properties. The humid-air part of sea-ice air is always saturated because the equilibrium between ice and humid air is independent of ad- access to sea-air as well as fluid water, ice and seawater prop- ditionally present seawater. A special situation occurs be- erties. tween the freezing points of water and of sea-water where neither ice nor liquid water can form a stable phase. In this temperature interval, the humid-air part of sea air is subsat- Appendix A urated, Fig. 10. The latent heat, Eq. (8.18), of sea-ice air, i.e. of water evaporating at constant pressure from sea ice, Composition of sea salt and dry air is a complex three-phase expression which, beyond the sub- The chemical compositions of sea salt and dry air are given limation enthalpy, includes the melting heat resulting from in Tables A1 and A2, respectively. the temperature change of ice and the salinity change of the brine. At zero salinity, sea-ice air reduces to ice air with only two Appendix B phases, ice and humid air, except for a small temperature- pressure window in which ice, liquid water and water vapour Thermodynamic potential of dry air coexist in the presence of air. This “triple-point” atmosphere is referred to as wet ice air, Fig. 11, and forms an almost The specific Helmholtz energy for dry air is (Lemmon et al., isothermal layer of isentropically lifted air between the melt- 2000), ing and the freezing level, Figs. 17, 18. In the two-phase A A L h id res i region of ice air, saturation is defined with respect to ice, f T ,ρ = RAT α (τ,δ)+α (τ,δ) , (B1) Fig. 13. L = L A, L The properties provided in this paper can be computed where RA R /M is the specific gas constant of air, from the currently available potential functions for humid MA,L=28.9586 g mol−1 and RL=8.31451 J mol−1 K−1 are air, fluid water, ice and seawater and the related equations the molar mass and gas constant used by Lemmon et will not require modification as the potentials are improved. al. (2000). Note that these values differ slightly from the Based on functions available from the literature as repeated most recent ones given in Table A1. The function αid (τ,δ) is in detail in the appendix, a new seawater library (Feistel et the ideal-gas part, al., 2009; Wright et al., 2009) has currently been developed as source code in Fortran and Visual Basic, with later ver- sions planned also in MatLab and C/C++, and will offer easy www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 120 R. Feistel et al.: Thermodynamic properties of sea air
Table A2. Chemical composition of dry air. Mole fractions from Table B1. Coefficients and exponents for the ideal-gas part (B2) Picard et al. (2008) except for N2 which was adjusted by subtracting for dry air (Lemmon et al., 2000). Here, we have adjusted the co- 0 0 all other mole fractions from 1 (Picard et al., 2008). Uncertainties efficients n4 and n5 to the reference state conditions of zero en- of the molar masses (Wieser, 2006) are given in brackets. tropy and zero enthalpy of dry air at the standard ocean surface state, 0 ◦C and 101 325 Pa. The originally published values are 0 = − 0 = Mole Mass Molar mass n4 13.841 928 076 and n5 17.275 266 575. Gas fraction fraction g mol−1 0 0 i ni i ni N2 0.780 847 9 0.755 184 73 28.013 4(3) −7 O2 0.209 390 0 0.231 318 60 31.998 8(4) 1 +0.605 719 400 00×10 8 +0.791 309 509 00 Ar 0.009 332 0 0.012 870 36 39.948 (1) 2 −0.210 274 769 00×10−4 9 +0.212 236 768 00 −3 CO2 0.000 400 0 0.000 607 75 44.009 5(9) 3 −0.158 860 716 00×10 10 −0.197 938 904 00 Ne 0.000 018 2 0.000 012 68 20.179 7(6) 4 +0.974 502 517 439 48×10 11 +0.253 636 500 00×102 He 0.000 005 2 0.000 000 72 4.002 602(2) 5 +0.100 986 147 428 912×102 12 +0.169 074 100 00×102 − × −3 + × 2 CH4 0.000 001 5 0.000 000 83 16.042 46(81) 6 0.195 363 420 00 10 13 0.873 127 900 00 10 Kr 0.000 001 1 0.000 003 18 83.798 (2) 7 +0.249 088 803 20×10 H2 0.000 000 5 0.000 000 03 2.015 88(10) N2O 0.000 000 3 0.000 000 46 44.012 8(4) CO 0.000 000 2 0.000 000 19 28.010 1(9) Xe 0.000 000 1 0.000 000 45 131.293 (6) Appendix C Air 1.000 000 0 0.999 999 98 28.965 46(33) Thermodynamic potential of fluid water
The specific Helmholtz energy for fluid (gaseous and liquid) water is (IAPWS, 2009a; Wagner and Pruß, 2002), f V T ,ρV = f V,id T ,ρV +R95T φres (τ,δ), (C1) 5 W id = +X 0 i−4 + 0 1.5 + 0 α (τ,δ) lnδ ni τ n6τ n7 lnτ (B2) where f V,id T ,ρV is the ideal-gas part, Eq. (C2), = i 1 95 = −1 −1 h i h i RW 461.51805 J kg K is the specific gas constant 0 0 0 0 res +n8 ln 1−exp −n11τ +n9 ln 1−exp −n12τ of H2O used in IAPWS-95, and φ (τ,δ) is the di- h i mensionless residual part consisting of 56 terms, avail- + 0 + 0 n10 ln 2/3 exp n13τ able from Eq. (C5) and the Tables C2–C4. Note that the gas constant used here differs from the most re- and αres (τ,δ) is the residual part, W −1 −1 cent value, RW = R/M =461.52364 J kg K , where MW=18.015268 g mol−1 is the molar mass of water 10 19 res X ik jk X ik jk lk α (τ,δ) = nkδ τ + nkδ τ exp −δ . (B3) (IAPWS, 2005). V,id V k=1 k=11 The ideal-gas part, f T ,ρ , of the specific Helmholtz energy for water vapour is (modified from Here, the reduced variables are τ = 132.6312K/T , δ = IAPWS, 2009a; Wagner and Pruß, 2002) ρA/ 10.4477moldm−3 ×MA,L, and the coefficients are V,id V 95 h 0 ex i given in Tables B1 and B2. Numerical check values are avail- f T ,ρ = RW T φ (τ,δ)+φ (τ) . (C2) able from Table I2, Appendix I. The temperature scale is ITS-90. Equation (B1) describes The function φ0 (τ,δ) was obtained from an equation for reliable experimental data available for 60–873 K and to the specific isobaric heat capacity developed by J.R. Cooper 70 MPa, and predicts air properties even up to 2000 K and (1982) and reads 2000 MPa. Here, we are interested only in the ranges in 8 X − 0 0 0 0 0 0 γi τ which air is in its gas phase, either at T > Tc, or T in the φ (τ,δ) = lnδ +n1 +n2τ +n3 lnτ + ni ln 1−e . (C3) interval Tc > T > TLiq(P ), between the critical temperature i=4 T and the dewpoint temperature T of liquid air. The V c Liq Reduced density δ = ρ /ρc and temperature τ = Tc/T are critical point of air is at Tc=132.5306 K, Pc=3.7860 MPa, specified by ρ = 322kgm−3, T = 647.096K. The coeffi- −3 A,L −3 c c ρc=11.8308 mol dm ×M ≈342.685 kg m . The dew- cients of Eq. (C3) are available from Table C1. The IAPWS- point curve TLiq(P ) is given by Lemmon et al. (2000). 95 reference state conditions define the internal energy and the entropy of liquid water to be zero at the triple point. A highly accurate numerical implementation of these con- ditions gave the values rounded to 16 digits for the ad- ◦ = − ◦ = justable coefficients n1 8.320446483749693 and n2 6.683210527593226 (Feistel et al., 2008b).
Ocean Sci., 6, 91–141, 2010 www.ocean-sci.net/6/91/2010/ R. Feistel et al.: Thermodynamic properties of sea air 121
Table B2. Coefficients and exponents for the fundamental Eq. (B3) for dry air (Lemmon et al., 2000).
k ik jk lk nk k ik jk lk nk 1 1 0 0 +0.118 160 747 229 11 1 1.6 1 −0.101 365 037 912 2 1 0.33 0 +0.713 116 392 079 12 3 0.8 1 −0.173 813 690 970 3 1 1.01 0 −0.161 824 192 067×10 13 5 0.95 1 −0.472 103 183 731×10−1 4 2 0 0 +0.714 140 178 971×10−1 14 6 1.25 1 −0.122 523 554 253×10−1 5 3 0 0 −0.865 421 396 646×10−1 15 1 3.6 2 −0.146 629 609 713 6 3 0.15 0 +0.134 211 176 704 16 3 6 2 −0.316 055 879 821×10−1 7 4 0 0 +0.112 626 704 218×10−1 17 11 3.25 2 +0.233 594 806 142×10−3 8 4 0.2 0 −0.420 533 228 842×10−1 18 1 3.5 3 +0.148 287 891 978×10−1 9 4 0.35 0 +0.349 008 431 982×10−1 19 3 15 3 −0.938 782 884 667×10−2 10 6 1.35 0 +0.164 957 183 186×10−3
Table C1. Coefficients of the ideal part (C3). Note that the orig- The residual part of Eq. (C1) has the form inally published values (Wagner and Pruß, 2002) of the adjustable ◦ ◦ coefficients n1 and n2 are slightly different from those given here. 7 51 res X di ti X di ti ci Those given here are preferred (IAPWS, 2009b; Feistel et al., φ = niδ τ + niδ τ exp −δ (C5) 2008b). i=1 i=8 54 X 0 0 + n δdi τ ti exp −α (δ −ε )2 −β (τ −γ )2 i ni γi i i i i i i=52 1 −8.32044648374969 56 2 +6.68321052759323 X + n 1bi δψ 3 +3.00632 i i=55 4 +0.012436 1.28728967 5 +0.97315 3.53734222 with the abbreviations 6 +1.2795 7.74073708 2 2ai 7 +0.96956 9.24437796 1 = θ +Bi |δ −1| , 8 +0.24873 27.5075105 1 β θ = 1−τ +Ai |δ −1| i , and
2 2 The temperature T is measured on the ITS-90 scale. The ψ = exp −Ci (δ −1) −Di (τ −1) . range of validity is 130–1273 K without the extension (C4), i.e. with φex (τ) ≡ 0. The range can be extended to include Equation (C1) is valid between 50 and 1273 K and for the region 50–130 K with a correction function added in this pressures up to 1000 MPa in the stable single-phase region temperature range, of fluid water. Uncertainty estimates are available from IAPWS (2009a) and Wagner and Pruß (2002). Numerical check values are available from Table I2, Appendix I. φex (τ) (C4) ! 1 3 τ 9 9τ τ 2 = E × − − (τ +ε)ln − + + , 2τ ε2 ε 2ε 2ε2 2ε3 Appendix D at 50 K ≤ T ≤ 130 K, Thermodynamic potential of humid air
AV,id where TE=130 K , E=0.278296458178592, ε = Tc/Te. At The Helmholtz energy F of humid air in the ideal-gas τ=ε, φex (τ) is zero, as well as its first, second, third and approximation (H3) is additive with respect to its compo- A,id V,id fourth temperature derivatives. This correction has been de- nents air, F , and vapour, F (Landau and Lifschitz, termined such that when applied to Cooper’s formula used 1987, §93), in IAPWS-95, it results in a fit to the heat capacity data of AV,id A,id V,id F (NA,NV,T,V ) = F (NA,T,V )+F (NV,T,V ). (D1) Woolley (1980) between 50 and 130 K with an r.m.s. devia- −4 tion of 6×10 in cp/RW. This extension formula has been Here, NA and NV are the numbers of air and vapour parti- developed particularly for implementation in the source-code cles in the volume V . The additivity of the Helmholtz en- library and is not published elsewhere. ergy (D1) is consistent with the entropy of mixing of ideal www.ocean-sci.net/6/91/2010/ Ocean Sci., 6, 91–141, 2010 122 R. Feistel et al.: Thermodynamic properties of sea air
Table C2. Coefficients of the residual part (C5). Table C3. Coefficients of the residual part (C5).
i ci di ti ni i di ti ni αi βi γ i εi 1 0 1 −0.5 +0.012533547935523 52 3 0 −31.306260323435 20 150 1.21 1 2 0 1 0.875 +7.8957634722828 53 3 1 31.546140237781 20 150 1.21 1 3 0 1 1 −8.7803203303561 54 3 4 −2521.3154341695 20 250 1.25 1 4 0 2 0.5 +0.31802509345418 5 0 2 0.75 −0.26145533859358 −3 6 0 3 0.375 −7.8199751687981×10 Table C4. Coefficients of the residual part (C5). 7 0 4 1 +8.8089493102134×10−3 8 1 1 4 −0.66856572307965 i ai bi Bi ni Ci Di Ai βi 9 1 1 6 +0.20433810950965 − − × −5 55 3.5 0.85 0.2 0.14874640856724 28 700 0.32 0.3 10 1 1 12 6.6212605039687 10 56 3.5 0.95 0.2 0.31806110878444 32 800 0.32 0.3 11 1 2 1 −0.19232721156002 12 1 2 5 −0.25709043003438 13 1 3 4 +0.16074868486251 14 1 4 2 −0.040092828925807 15 1 4 13 +3.9343422603254×10−7 gases, Eq. (H9). At higher densities, the corresponding 16 1 5 9 −7.5941377088144×10−6 Helmholtz energy of the real-gas mixture is 17 1 7 3 +5.6250979351888×10−4 F AV (N ,N ,T,V ) = F A (N ,T,V )+F V (N ,T,V ) (D2) 18 1 9 4 −1.5608652257135×10−5 A V A V AV + × −9 Q 19 1 10 11 1.1537996422951 10 −kT ln . 20 1 11 4 +3.6582165144204×10−7 QAQV 21 1 13 13 −1.3251180074668×10−12 A V AV 22 1 15 1 −6.2639586912454×10−10 The configuration integrals Q , Q and Q of the canon- 23 2 1 7 −0.10793600908932 ical partition function are defined in terms of the pair- 24 2 2 1 +0.017611491008752 interaction potentials u between the particles of air at the 25 2 2 9 +0.22132295167546 positions rA and those of vapour at rV, as (β = 1/kT ): 26 2 2 10 −0.40247669763528 27 2 3 10 +0.58083399985759 Z A NA V NV AV dr dr −3 Q = (D3) 28 2 4 3 +4.9969146990806×10 V V 29 2 4 7 −0.031358700712549 V − 30 2 4 10 0.74315929710341 ( NA NV 31 2 5 10 +0.4780732991548 X A A X V V exp −β uAA ri ,rj −β uVV ri ,rj 32 2 6 6 +0.020527940895948 i