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DACIAN BASIN - GeoEcoMar

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1.2. Stratigraphy<br />

poral limits of these “brackish stages” are different from one area to another. The<br />

ecological facies pertaining to a brackish stage may occur in different space units<br />

or time intervals. The best example is that of the “Pontian type” fauna or “Sarmatian<br />

type” fauna from the Mediterranean area, faunas which have nothing in common<br />

with the Paratethian Pontian or Sarmatian faunal assemblages. These aspects could<br />

also create difficulties for the construction of the magnetostratigraphic scales.<br />

1.2.2. Toward a reliable chronostratigraphic and geochronologic framework<br />

of the Dacian Basin 1<br />

Many contributions of Romanian and/or foreign researchers refer to the ages of the<br />

Dacian Basin sedimentary deposits. Still, an unique (and unanimously accepted)<br />

chronostratigraphic and geochronologic framework has not yet been achieved<br />

(Fig.1.5). To reach a high-resolution dating of the Miocene and Pliocene (sub)stage<br />

boundaries, various new techniques have been integrated with the traditional biostratigraphy,<br />

principally magnetostratigraphy, astrochronology and cyclostratigraphy.<br />

Reliable sampling techniques, sophisticated paleomagnetic laboratories, along<br />

with an increasing number of data analysis methods and more refined criteria<br />

were developed worldwide to retrieve the paleogeomagnetic fossile, i.e. the primary<br />

Natural Remanent Magnetisation (NRM) component (Characteristic Remanent<br />

Magnetisation/ChRM, isolated in laboratory). This magnetic signal, commonly<br />

weak in the sedimentary deposits in which it is printed/”frozen”, may be affected by<br />

noise from a number of perturbation processes or may be obscured subsequently<br />

to rock formation, along their geological and geochemical history.<br />

A breakthrough in age determination has been the astronomical dating (Hilgen,<br />

1991, 1994, Hilgen et. al., 1995, Berggren et al., 1995, Krijgsman, 1996). An Astronomically<br />

calibrated (Polarity) Time Scale [A(P)TS] has been constructed (first, for the<br />

Pliocene – Pleistocene time interval; Lourens et al., 1996), and even incorporated in<br />

the existing (very usable) standard Geomagnetic Polarity Time Scale (GPTS) of Cande<br />

and Kent (1995; CK95). Since 2004, the Astronomical Tuned Neogene Time Scale<br />

(ATNTS2004; Lourens et al., 2004), characterised by an unprecedented resolution<br />

and accuracy, is in use.<br />

In this shortly defined context, the geological time scales (GTS) in figure 1.5,<br />

particularly the ages assigned to the chronostratigraphic boundaries, should be<br />

carefully considered before adopting one of them. To compare and evaluate these<br />

GTS’s (models A, B, C, D) with the intention of assuming a (reliable) version for<br />

the Dacian Basin (possibly, a composite GTS), at least the following major aspects<br />

should be taken into consideration:<br />

1 Author: Sorin-Corneliu Rădan<br />

23

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