Sa. Elming et al., THE DRIFT OF THE FENNOSCANDIAN AND UKRAINIAN SHIELDS DURING THE PRECAMBRIAN - A PALEOMAGNETIC ANALYSIS, Tectonophysics, 223(3-4), 1993, pp. 177-198
A revised Precambrian (2.85-0.6 Ga) Apparent Polar Wander Path (APWP)
for the Fennoscandian Shield, based on a new compilation and analysis
of data, is presented. In fitting the APW path to successive Grand Mea
n Palaeomagnetic poles (GMPs), we applied the spherical spline techniq
ue originally developed by Jupp and Kent in 1987. The position and ori
entation of the Fennoscandian Shield during 2.85-0.6 Ga was determined
from the GMPs. Major palaeoclimatological findings are used to constr
ain the palaeomagnetic interpretation of palaeolatitudes. The general
drift of Fennoscandia, from relatively high latitudes in the late Arch
aean-Early Proterozoic to nearly equatorial latitudes in the Middle Pr
oterozoic, correlates with palaeoclimatological indications that a per
iod of cold climate was followed by one of warm climate during this ti
me interval. From the continuous APWP the APW velocities and latitudin
al drift velocities of the shield were calculated. An accumulated APW
curve was also calculated. The palaeomagnetic data are irregularly dis
tributed and some periods are rather poorly represented. This means th
at the calculated velocities can sometimes be artifacts of sampling. L
ate Archaean and Early Proterozoic (2.85-1.90 Ga) data are too sparse
to make these calculations meaningful and velocity calculations are th
erefore restricted to data of 1.90 Ga and younger ages. The accumulate
d APW curve shows a number of linear segments with varying slopes, ind
icating sudden changes in drift rate. During the Middle Proterozoic (1
.90-1.35 Ga) there was a period when the rate of APW was constant and
low and that of latitudinal drift also was low. This pattern changed a
t ca. 1.35 Ga, and the following Middle-Late Proterozoic period can be
described by rapid APW and strongly fluctuating drift velocities. Jot
nian rifting and the intrusion of numerous dyke swarms (at ca. 1.25 Ga
) correlate with this shift in rate. These changes are attributed to c
hanges in plate configuration. A new database for the Ukrainian Shield
is also presented, and GMPs in the 2.32-1.20 Ga range are defined. Th
e database is still inadequate and the comparison of the Ukrainian and
Fennoscandian drift histories is therefore tentative. Similarities in
position, latitudinal drift and rotation during the Early-Middle Prot
erozoic are, nevertheless, evident. A close relationship between the s
hields in this period is consistent with the low APW rate of Fennoscan
dia, indicating that Fennoscandia may have been part of a larger conti
nent, including the Ukraine, at that time. At ca. 1.2 Ga, the latitudi
nal position of Ukraine differed significantly from that of Fennoscand
ia, suggesting that the large shield split up between ca. 1.35 and 1.2
Ga. This would explain the change in APW rate at 1.35 Ga. The subsequ
ent increase in rate was due to a reduction in the size of the shield.
The discrepancy in palaeopositions of Fennoscandia and Ukraine at 1.2
Ga led Mikhailova and Kravchenko to suggest a late Precambrian time (
1.07-0.57 Ga) for the accreation of Fennoscandia to the East European
Platform (EEP). This may be correct as the rate of APW for Fennoscandi
a decreased in the late Precambrian, reflecting such a consolidation.