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Joint International Conference on Long-term Experiments ...

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c<strong>on</strong>centrati<strong>on</strong> measurements of the radium how much rad<strong>on</strong>-222 is formed in a unit of<br />

time. The measurements effectuated in the mixed layer present a deficiency relative<br />

to the quantity at which we should expect. The flux to the atmosphere can be estimated<br />

from this deficiency and the gas exchange coefficient is found from the rapport of the<br />

flux to the air–water c<strong>on</strong>centrati<strong>on</strong> gradient. We will present a simple estimati<strong>on</strong>, but we<br />

will firstly c<strong>on</strong>sider the process of a series of decays, which imply radium-226 and<br />

rad<strong>on</strong>-222. Radiu-226 has a half value life time much l<strong>on</strong>ger than rad<strong>on</strong>-222. These two<br />

isotopes are put in isolati<strong>on</strong> until when they reaches equilibrium, where the exchange<br />

rates for which the two isotopes are decayed are equal. It is better to give the<br />

c<strong>on</strong>centrati<strong>on</strong> of these radioisotopes by the activity, noted as A, which is equal with the<br />

product between the decay c<strong>on</strong>stant λ and the atoms number that are present in a<br />

volume unit:<br />

A Rn-222 = λ⋅CRn-222 (13)<br />

where CRn-222 represents the atom c<strong>on</strong>centrati<strong>on</strong> per volume unit. In the case of our<br />

c<strong>on</strong>sidered isotopes the c<strong>on</strong>centrati<strong>on</strong> is given in dpm ⁄100 Kg, where dpm is the<br />

number of decays in a minute. The decay c<strong>on</strong>stant is given as a rapport between ln(2)<br />

and the mean half value life time. The equilibrium activity of Rn-222 is of the form A Rn-<br />

222 Ra-226<br />

= A .<br />

The rad<strong>on</strong> deficiency due to the gas exchange is given by:<br />

Φ = h(A Ra-226 - A Rn-222 ) (14)<br />

where h is the Rad<strong>on</strong>-222 layer depth and the activities are the values <strong>on</strong> this layer. The<br />

flux will be of the form:<br />

Φ = - kapă(CRn-222)aer - (CRn-222)water =<br />

k<br />

= −<br />

water<br />

[ A ) − ( A ) ]<br />

(15)<br />

λ Rn−222<br />

air Rn−222<br />

water<br />

The c<strong>on</strong>centrati<strong>on</strong> of the atmospheric rad<strong>on</strong> Rn-222 is much lower than that from the<br />

ocean. Then we can ignore the activity of Rn-222air and we make equal the last two<br />

equati<strong>on</strong>s, obtaining the following result:<br />

⎛ A ⎞<br />

k = λ h⎜<br />

Ra − 226<br />

− 1⎟<br />

(16)<br />

water ⎜ A ⎟<br />

⎝ Rn − 222 ⎠<br />

From the made measurements it was obtained (in a mixed layer of 40 m in depth) that<br />

the rapport of Ra-226 to Rn-222 is 1,6, giving a pushing velocity kappa of the form:<br />

ln( 2)<br />

−1<br />

k<br />

water<br />

= 40 m(<br />

1,<br />

6 − 1)<br />

= 4,<br />

4 m d = 10 cm / hour (17)<br />

3,<br />

85d<br />

(c) Applicati<strong>on</strong>s<br />

One of the advantages of in situ researches is that they have permitted a better<br />

understanding of the role played by organic films for de<strong>term</strong>inati<strong>on</strong> of the gases<br />

exchanges. After obtaining such results more types of models for this phenomen<strong>on</strong> of<br />

the gas exchange were been given. It is not the aim of this paper to develope models,<br />

which were <strong>on</strong>ly used in the next discussi<strong>on</strong> and could be given in the Table nr.3. We<br />

wish that, <strong>on</strong> these models base to answer at some questi<strong>on</strong>s that were been not<br />

394

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