MODELLING VERTICAL STRUCTURE OF PHYSICAL FIELDS IN GULF OF RIGA
Juris Seņņikovs, Uldis Bethers, Laboratory for mathematical modeling of environmental and technological processes, University of Latvia, 8 Zeļļu, LV 1002, Rīga, ph. 7615711, e-mail
bethers@latnet.lvKEYWORDS: Upper mixed layer, stratification, atmosphere – ocean interface, mathematical modelling
ABSTRACT
The mathematical model for description of the time development of the vertical structure of temperature and salinity is developed. Model is based on the heat, mass and turbulent kinetic energy balance of the upper mixed layer; it includes description of the ice formation dynamics. Model accounts for the exchange with atmosphere, Baltic Proper, and for river run – off. The model is applied for simulation of the Gulf of Riga (1992 to 1995) comparing modelling results with observations.
INTRODUCTION
The model of the time-development of the vertical structure of the physical fields, i.e. temperature and salinity in the Gulf of Riga was developed by (Seņņikovs and Bethers, 1995). It is enhanced in the present paper adding the new features:
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Fig.1. Scheme of the processes included in the model used to describe the dynamics of vertical structure of temperature and salinity. |
The ice model inclusion modifies both the principal scheme of the physical model and its mathematical formulation as described in the following Chapters. The principal scheme of the accounted fluxes is given in Fig. 1. A numerical solution is performed by means of modified method (Реснянский, 1989).
PHYSICAL MODEL
Observations (Bērziņ, 1995) indicate presence of a distinct layer with a sharp gradient of the physical parameters in the Gulf of Riga from April till August. The depth profiles of the temperature and salinity include a mixed (quasi-homogenous) upper layer, a thin layer of the change of parameters (thermocline, halocline, pycnocline) and a lower stratified layer. The vertical differences in the physical fields are higher than horizontal, except for the hydrological fronts near rivers’ mouths. Contrary, from November till March the Gulf of Riga is almost vertically homogeneous. This, as well as presence of the ice cover almost every year characterises the difference between the shallow and brackish Gulf and the neighbouring Baltic Proper. The minor horizontal gradients in the main water mass of the Gulf allow a principal description of the seasonal cycle of the physical parameters by a one-dimensional model with the vertical resolution. The integral model of the upper layer similar to (Stigebrandt, 1985; Niiler and Kraus, 1977) is used in the present paper assuming the homogeneity of the physical parameters in this well-mixed layer. The turbulent heat and mass transfer equations are used to describe the physical fields below it.
The upper quasi-homogenous layer is intensively turbulent. Its presence and dynamics relate with the balance of the turbulent kinetic energy (TKE), which is generated mechanically, mainly by the wind and breaking wind waves. TKE is consumed for the mixing the incoming buoyancy flux (fresh water inflow, heat flux through the air-sea interface, ice melting of the ice, etc.), and for the entrainment of the denser and less turbulent water of the lower layer, if the upper layer deepens. The dynamic of the upper layer is affected also by the thermohaline convection in the case of a negative buoyancy flux (cooling above and heating below the minimum density temperature, ice freezing).
The balance of the water mass, heat and salt contents of the upper layer is constructed accounting for the fluxes that are either almost independent on the physical parameters of the Gulf or determined by these parameters. First group includes solar radiation, river run-off, outflow to the Baltic Proper. Inflow from the Baltic Proper has to be prescribed, too; however, its depth distribution is essentially dependent on the stratification of the Gulf. The heat and mass fluxes on the water-air and ice-air surfaces (evaporation/condensation, back radiation, sensible heat flux) depends not only on the external forcing parameters (humidity, wind, cloudiness, air temperature) but also on the temperature of the upper layer and the ice surface temperature. The ice usually covers some part of the Gulf during winters. The physical model under consideration assumes a constant temperature of the upper layer during the ice periods and different parameterisation of the heat fluxes for the ice-free and ice-covered parts of the Gulf. Mechanical generation of the TKE is considered only through the ice-free surface.
MATHEMATICAL MODEL
Conservation equations for upper layer
The balance equations are derived from the basic conservation laws. Mass balance of the upper layer neglecting precipitation/evaporation due their approximate equality is
(1)
here h is the depth of the upper mixed layer; we is the velocity of the entrainment of the water below the mixed layer into the latter; w(z) is the velocity of the vertical advection.
Heat balance for the upper layer
(2)
here r 0 is the reference density (1000 kg·m-3); cp is the isobaric heat capacity of water (4200 J× m-1K-1); V(z) is the volume of the water above the depth z; A(z) is the cross section area at the depth z; TS, TF, Tin(z) are the temperatures of the upper layer, river water and the Baltic Proper water, respectively; D T is the difference between the temperature of the upper layer and the water just below it; F, Qout are the mass fluxes of the rivers and flow to the Baltic Proper; qin(z) is the depth distribution of the inflowing mass flux from the Baltic Proper. The terms on the right hand side of (2) denote, respectively (see also Fig. 1) (i) heat flux through the atmosphere-sea interface Qws including the insolation absorbed in the upper layer; (ii) heat flux through the ice-sea interface (if any) Qiw; (iii) change of the heat content due to the mass fluxes inside the system; (iv) diffusive heat flux to the lower layer; (v) advective heat fluxes from the rivers and from /to the Baltic Proper. The temperature of the upper layer remains at the freezing temperature Tf (assumed constant Tf=-0.3°C) during the ice freezing and melting periods.
Salt balance for the upper layer
(3)
here Qif is the heat flux for the melting of ice; M is the latent heat of the sea ice freezing, (M=3.32× 105 J× kg-1); SS, Sice, SF, Sin are the salinities of the upper layer, sea ice, river and Baltic Proper water, respectively; D S is the difference between SS and the salinity just below the upper layer;
is the density of the diffusive salt flux to the lower layer.
The heat balance for the ice neglects the heat content of the ice cover
(4)
here Qis is the heat flux on the atmosphere - ice interface, positive for the incoming flux.
Balance of the turbulent kinetic energy (TKE)
The equation for the TKE balance stands as
(5)
here the left hand side is the energy that is necessary for the increasing of TKE
(e 2 = 1× 10-4 m2s-2 ) and potential energy of the entraining water. This energy equals to zero during the retreat of pycnocline. D r is the difference between water density in upper layer and just below it. The terms on the right hand side of (5) describe, respectively:
(6)
here r a is the air density (1.26 kg·m-3); Cw=1.1× 10-3 is the wind drag coefficient; W is the wind velocity.
(7)
here the coefficients of, respectively, thermal and haline expansion are defined as
(8)
S(T,S) given by equation of the state of seawater (UNESCO, 1981), g = 9.81 m/s2 is the acceleration due to the gravity.
(9)
here r S=r (TS,SS), r in=r (TB, SB) are the densities of the upper layer and the inflow.
(10)
where n0=0.05 is an empirical constant (Stigebrandt, 1985), characterising the efficiency of the penetration of the thermohaline convection.
Turbulent energy generation by the shear stress on the interface between upper and lower layers is neglected as well as the radiation of the turbulent energy to the lower layer. The penetration of the mechanically generated turbulence is limited due to the Earth rotation by the thickness of the Ekman boundary layer hEk given (Stigebrandt, 1985) as
(11)
here Hk» 0.6 is an empirical constant (Seņņikovs and Bethers, 1995); f=1.22× 10-4s-1 is the Coriolis parameter at latitude 57° N. This limitation does not concern the turbulence generated by the convective motion.
The model of the lower layer
The turbulent heat and mass transfer equations are used for calculating T(z) and S(z) for the lower layer z>h
(12)
here k T, k S are the turbulent heat and mass exchange coefficients, k T» k S » 10-6..10-5 m2s-1.
The boundary conditions for (12) in the absence of the exchange with the bottom are
(13)
here ' denotes ¶ /¶ z.
The heat and mass fluxes are supposed to be proportional to D T and D S, respectively
(14)
here empirical parameters are estimated as lT» lS» 1..100 m.
Parameterisation of the heat fluxes
The heat fluxes Qws and Qis through the sea-atmosphere and ice-atmosphere interfaces are formulated similarly
(15)
here Iw and Ii are the densities of the insolation flux absorbed in the water and ice, respectively. They are calculated using tables of insolation (Гидрометеоиздат, 1975). The solar radiation is assumed being absorbed in the upper mixed layer or the ice cover.
The back radiation from both surfaces is written as (Gill, 1982)
(16)
here s is Stephan-Boltzmann constant (5.67× 10-8 W·m-2K-4); ea is the partial pressure of the water vapour in the air (mbar); nc is cloudiness; e w=0.985, e i=0.96 are emissivities of the water and ice, respectively; T stands either for the water or ice surface temperatures TS or Tice.
The latent heat fluxes (l =2.5× 106 J× kg-1 is the specific latent heat of vaporisation of the water, L=l +M=2.82× 106 J× kg-1 is the specific latent heat of ice sublimation) are calculated assuming evaporation parameterisation (Gill, 1982; Kraus, 1972)
(17)
here CEw» CEi» 1.1× 10-3 are empirical water vapour exchange coefficients over the sea and ice, respectively; qa is the absolute air humidity, qaw, qai are the absolute humidities of the air-sea and air-ice interfaces. They are assumed to be equal to the saturation values of the water vapour at temperatures TS or Tice, respectively.
The sensible heat fluxes are written as (Gill, 1982; Kraus, 1972)
(18)
here cpa = 1000 J× kg-1K-1 is isobaric heat capacity of air; CHw» CHi» 1.1× 10-3 are empirical heat exchange coefficients over the sea and ice, respectively; Ta is the air temperature.
The dependence of the absolute humidity on the water vapour pressure must be added to (15-18)
(19)
here m » 0.62 is the ratio of the molar weights of water and air, pa is the air pressure (assumed pa=1000 mbar). The saturation pressure dependencies on the temperature are necessary for calculating the saturation values of the humidity. They are given for the water vapour above, respectively, the sea and ice surfaces as (Gill, 1982; Kraus, 1972)
(20)
here T is a expressed in ° C.
Model of inflow of the Baltic Proper water
Assumption of the time-independent water level of the Gulf leads to a simple volume balance equation
(21)
The time-dependence of fluxes Qin and Qout can be found by an external model, (Bērziņ et. al, 2000). The outflow to the Baltic Proper is assumed from the upper layer, but an appropriate model is needed for qin(z), the distribution of Qin over the depth. Then the expression for w(z) follows from the continuity and incompressibility:
(22)
Let us assume (i) the depth independent temperature and salinity of the inflowing water Tin(z)=TB, Sin(z)=SB; (ii) the regular distribution by volume of the inflowing water between the sill depth hsill and the equilibrium depth heq which can be found from
(23)
The density of the inflow then stands as
(24)
while the dependence of the vertical advection on z is
(25)
Accounting the additional turbulent energy consumed for the mixing of the inflowing water, (9) can be rewritten as
(26)
Ice model
The ice conditions are described in the simple way, neglecting the variety of the ice forms and the snow cover over the ice. Then the ice conditions can be characterised by the area of the Gulf covered by the ice Aice and the ice volume Vice. Introducing the coefficient ci of the ice coverage and the effective ice thickness
as
(27)
one can derive the equation for the dynamics of the ice amount
(28)
Two additional hypotheses concerning the relationships between ci,
and the observed ice thickness hice are necessary for the closure of (28). The relationship
![]()
(29)
describes the ice volume distribution between the continuous ice cover and the drifting ice. The simplified assumption of no drifting ice
(30)
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Fig.2. Ice thickness vs. Gulf coverage by ice. Observations are 10-day mean values for the years 1976 to 1987. Lines indicate model behaviour of the freezing/melting cycle. Freezing/melting implies an increase/decrease of the ice thickness. |
is adopted in this paper. The temperature of the ice surface, necessary for calculating mass and heat fluxes can be found assuming the linear temperature distribution across the ice cover. Obviously, this temperature cannot be greater than the freezing temperature
(31)
here k ice» 2.1 J× K-1m-1s-1 is the heat conductivity of the ice.
Another hypothesis concerns the dynamics of the ice-covered area of the Gulf. It can be found from the long-term observations of the ice thickness and coverage (Fig. 2). It can be deduced that for the most cases both freezing and melting of the ice proceeds with a linear relation between hice and ci, however, the respective coefficients of the linear relationship are either constant (during freezing) or dependent on the ice distribution at the beginning of the melting period. The above considerations may be formalised as
![]()
(32)
where hcov» 10 cm is the mean of the minimum value of the ice thickness for that the full coverage of Gulf is observed, see model behaviour of (32) in Fig. 2.
RESULTS AND DISCUSSSIONS
The developed model was applied for the real – time simulation of the vertical TS structure of the Gulf of Riga for time period May/92 to Oct/95. The following data were used for the forcing of the model of the dynamics of the vertical structure of the temperature and salinity:
Data was linearly interpolated for their hourly values. The insolation was calculated from the astronomic considerations.
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Fig.3. Calculated time development of the vertical temperature distribution of the Gulf of Riga. |
The calculated time development of the temperature depth distribution is shown in Fig. 3, whilst the time dependence of the surface and bottom temperature including comparison with the observations at station 121 is given in Fig. 4. The calculated development of fluxes on the atmosphere-sea interface is also shown in Fig. 4. Analysing calculations one can conclude that
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Fig.4. Time-dependence of calculated and observed surface (Ts) and bottom (Tb) temperatures (upper graph). Calculated daily means of heat flux (Q) components: insolation (I0), back radiation (Qbr), sensible (Qs) and latent (Ql) heat fluxes (lower graph). |
Model indicates a presence of two ice periods. First (winter 1992/93) is caused by the continuous increased cooling of the water masses during autumn-92, especially Oct-92 (see Fig. 4 for respective heat fluxes) but the second (winter 93/94) by the intensive cooling during Nov-93 and cold Feb-94. Relatively mild winter winds of 1994 were favourable for ice conditions due to the establishment of reverse stratification (see Fig. 3).
ACKNOWLEDGEMENT
This work has been supported by grant No. 96.0326 of Latvian Science Council. Authors owe V.Bērziņ (Latvian Fisheries Research Institute) for the useful discussions concerning the ice conditions over th
e Gulf of Riga, and access to the hydrometeorological and hydrological data series at LatFRI.
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