PALEOINTENSITY RESULTS FROM THE PERMO-CARBONIFEROUS (KIAMAN) REVERSEDSUPERCHRON - THE GREAT-WHIN AND MIDLAND-VALLEY SILLS OF THE NORTHERN UNITED-KINGDOM
Dn. Thomas et al., PALEOINTENSITY RESULTS FROM THE PERMO-CARBONIFEROUS (KIAMAN) REVERSEDSUPERCHRON - THE GREAT-WHIN AND MIDLAND-VALLEY SILLS OF THE NORTHERN UNITED-KINGDOM, Geophysical journal international, 123(3), 1995, pp. 798-816
Fifty Thellier palaeointensity determinations were made from the Great
Whin Sill (GWS) of northern England and the Midland Valley Sill (MVS)
of central Scotland, which form the major part of a late Carboniferou
s quartz-dolerite complex. Palaeodirectional analysis confirms that th
e reversed polarity characteristic remanence carried by samples from b
oth sills is consistent with the Permo-Carboniferous reversed superchr
on. Palaeomagnetic results suggest that the two sills may not be exact
ly contemporaneous. The MVS was intruded rapidly some time during the
emplacement of the GWS, which was itself emplaced over a considerable
time period. The MVS may well represent the northernmost expression of
the instrusive activity. A mean palaeointensity of 22.9+/-2.6 mu T wa
s calculated for the Great Whin Sill, with a corresponding VDM value o
f 5.9 x 10(22) A m(2). The palaeointensity value calculated from the M
idland Valley Sill was much lower, 13.0+/-0.5 mu T, with a correspondi
ng VDM value of 3.3 x 10(22) A m(2). Detailed rock magnetic analyses a
nd stepwise thermal demagnetization studies reveal that the remanence
carrier in both sills is magnetite of mixed domain state. Multidomain
grains are less important in the Midland Valley Sill and thus greater
confidence is attached to palaeointensity results from this sill. VDM
values from this and other studies of the Permo-Carboniferous reversed
superchron (P-CRS) indicate that the dipole strength showed similar v
ariations to that witnessed for the past 5 Ma. There is no conclusive
support in favour of either the weak or strong held models that have b
een suggested for superchrons. More palaeointensity results are needed
from the termination of the P-CRS and the late Permian/early Triassic
in order to understand how the dipole field evolved during the P-CRS
and its relationship to the so-called Mesozoic dipole low.