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Joint International Conference on Long-term Experiments ...

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the maximum of CO2 have the tendency to be larger than that for O2. We introduce the<br />

following questi<strong>on</strong> at which we must give a resp<strong>on</strong>se: which are the relative<br />

c<strong>on</strong>tributi<strong>on</strong>s of the biological and physical processes to this distributi<strong>on</strong> of gases.<br />

From the measurements it can be seen that the N2O distributi<strong>on</strong> is near to the<br />

atmospheric equilibrium <strong>on</strong> the most latitudes, with the excepti<strong>on</strong> of those closed to the<br />

equator, where N2O is in a big quantity that would imply the existence of an oceanic<br />

source. We need to see which this source is. To answer such questi<strong>on</strong>s we need to know<br />

the gases solubilities, that tell us at which c<strong>on</strong>centrati<strong>on</strong>s are the gases. We must also<br />

discuss about the gases exchange rates that de<strong>term</strong>ines how rapidly a corps immersed in<br />

water will be in equilibrium with the atmosphere at the ocean surface. In a future paper<br />

we will discuss also about the biological processes that take place inside the ocean,<br />

processes that together with the physical <strong>on</strong>es force the gases to go out from the<br />

equilibrium state with atmospheric air.<br />

2. THE GASES SOLUBILITIES<br />

We need to estimate the gas c<strong>on</strong>centrati<strong>on</strong> in mmol ⁄ m 3 in sea water, which is not in<br />

equilibrium with the gas from wet air above of ocean. The gases atmospheric<br />

c<strong>on</strong>centrati<strong>on</strong>s are given as partial pressures in physical atmosphere (atm) defined by<br />

the relati<strong>on</strong>:<br />

pA = χA ⋅P (1)<br />

where the molar fracti<strong>on</strong> χA is the moles number of the comp<strong>on</strong>ent A in the unity of air,<br />

P being the total atmospheric pressure in atm. The most suitable definiti<strong>on</strong> for the gases<br />

solubility is given as:<br />

CA = SA ⋅pA = SA⋅χA⋅P (2)<br />

where CA is the soluti<strong>on</strong> c<strong>on</strong>centrati<strong>on</strong> of the comp<strong>on</strong>ent A in mmol⋅m -3 , equal with 1<br />

μmol⋅l -1 ; SA is the solubility in mmol⋅m -3 ⋅atm -1 . This parameter is related to Bunsen<br />

coefficient β or to the parameter that is functi<strong>on</strong> of solubility, F. These parameters could<br />

be related. In the Table nr.2 the equati<strong>on</strong> and the coefficient for calculati<strong>on</strong> of Bunsen<br />

coefficients and of solubility fracti<strong>on</strong>s F for some gases are given. The solubility decays<br />

with the increasing of the temperature for all gases.<br />

3. THE GAS EXCHANGE<br />

The vertical moti<strong>on</strong>s in the atmosphere and in the ocean are intensively suppressed near<br />

the air-ocean water interface. There were been proposed a variety of models to explain<br />

the effect of this phenomen<strong>on</strong> <strong>on</strong> the gas transfer transverse to the air-water interrface.<br />

We will take into c<strong>on</strong>siderati<strong>on</strong> the stagnant film model. This model supposes that the<br />

turbulence suppressi<strong>on</strong> at the sea-air interface could be represented by molecular<br />

diffusi<strong>on</strong> inside a stable film of finite depth, both in ocean and in the atmosphere. This<br />

model could be easier visualized and gives us the possibility of a direct discussi<strong>on</strong> for<br />

the relative importance of the atmospheric and ocean boundary layers. The model of the<br />

stagnant film represents the transiti<strong>on</strong> from the turbulence inside the free surface fluid to<br />

the molecular diffusi<strong>on</strong> from inside the stable film by a simple structure made from two<br />

layers, illustrated in the Fig.1. If we take into account the fact that doesn’t exist nor<br />

sources nor sinks inside the film, it may be affirmed that fluxes in these films will be<br />

given by the first Fick law:<br />

390

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