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STATION 6<br />

i—r<br />

3400 3000<br />

1600<br />

31-03-78<br />

FIGURE 14. Infra-red spectrometry of the resins.<br />

by Tissot et al ; they were calculated for the earliest samples only<br />

2(C29 + C31)<br />

R 29-31 = C28 + 2C30 + C32<br />

The relationship shows that in this case, the n-C29 and n-C31<br />

predominate. Where the value is over 1, the odd-numbered carbons predominate.<br />

In Table 2, a <strong>com</strong>pilation of these values for all the<br />

stations, it is seen that R is much higher than 1 at Stations 6 and 8.<br />

Even in March 1978, this presence of natural <strong>com</strong>pounds modified<br />

the distribution of hydrocarbons by family :<br />

- saturated hydrocarbon contents were low ,-<br />

- polar-<strong>com</strong>pound contents (resins and asphaltenes) high.<br />

While the ratio of SAT/ARO decreased slightly, as at Stations 5<br />

and 6 (Fig. 17), degradation of n-alkanes and isoprenoids (pristane<br />

and phytane) was observed throughout the period, showing clearly which<br />

polycyclic alkanes are most resistant to degradation.<br />

The chroma tograms of the aromatic hydrocarbons have very marked<br />

profiles under photometric detection (FPD) , and a persistence in the<br />

unresolved <strong>com</strong>plex mixture (FID) (Fig. 16). Comparison of the results<br />

of the GPC with those of the high resolution MS undertaken on the reference<br />

samples of March 23, 1981 at Portsall, and the sampling taken<br />

126

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