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a) Profiles computed for the north cliff

Polynomial regression curves have been computed to

illustrate the variation in element concentrations in the 100 m

thick sequence of mudstones, shales and cherts which is exposed in

the north cliff at Hartfell. The analysis of variance for the

computed curves is given in Table 3-7. Out of a total of 17

elements considered, only Cu, Mn, Mg and Sr yield profiles which

are significant at the 99 per cent confidence level. The profiles

for Al, K and Pb are significant at the 95 per cent level.

All those profiles which are significant at the 95 per

cent level have been superimposed upon the scatter plots (Figs

59a - 76a). The curves for K and Pb are similar in that both

display trends which increase for the first 15 m from the base of

the cliff and then decrease for the next 10 m. Values then

increase once more and both elements have their greatest

concentrations in the P,linearis Zone, 87 m from the base of the

cliff.

The profiles for Al and Cu are essentially the same as

for K and Pb for the first 85 m up the cliff. Thereafter, values

increase more rapidly. This observation is also true for the

trends computed for Mn and Mg. These, although not varying much

for the first 85 m, begin to change rapidly around the 85 m mark.

The profile for Sr also exhibits inflexions at around 15 m and

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b) Restoration profiles

The true stratigraphic position of the samples before

faulting and folding have been calculated (Chapter I, 3d) and the

results are given in Table 1-2. Polynomial regression curves were

then computed to illustrate the variation of element concentration

through the structurally restored succession. The analysis of

variance for the restored curves is given in Table 3-8.

Out of a total of 17 elements considered, only Al, Cu and

C yield restoration profiles which are significant at the 99 per

cent confidence level. The profiles for Fe and Na are significant

at the 95 per cent level. The six profiles which are significant

at the 95 per cent level have been superimposed upon scatter plots

of the data (Figs 6'lb, 62b, 65b, 68b, 69b, 76b). These profiles

exhibit the same trends, although with greater detail, as the

lower parts of the profiles which have been computed for the total

suite of the samples (cf. Figs 49, 51, 52, 53 and 57).

The significance levels of the vertical profiles for the

sequence as exposed, and for the sequence of samples after

structural restoration are compared in Table 3-9. It is found

that the profiles for Mn, Mg, Sr, K and Pb are more significant

when computed in the in-situ position, whereas structural

restoration improves the fit of the profiles computed for Al, Fe,

Na and C. Although both profiles for Ca lie outside the chosen

confidence limits it is noteworthy that the F-value is greater for

the in-situ profile. This may mean that the in-situ profile of

Ca is more significant than the restoration profile. These results

stratigraphic variations whereas the profiles for Mn, Mg, Ca, Sr,

K and Pb represent variations attributable to effects associated

with faulting.

c) Interpretation

The element assemblage involved with the effects associated

with faulting indicates that a carbonate phase may have been

introduced into the sediments at Hartfell. This phase was not

detected in the mineralogical examination of the samples but as the

mean values of Ca, Mn and Mg at this locality are only 0.02, 0.01

and 0.48 per cent respectively, only small quantities of a carbonate

mineral could possibly be present. Two possibilities can be

considered for the introduction of a carbonate into the sediments:

firstly, metasomatism related to an igneous source, and secondly,

diagenesis related to carbonate-bearing groundwaters. In the first

connexion, Weir (1974) has related the presence of carbonate

minerals in the Silurian rocks of Gatehouse to granitic emanations.

In the Gatehouse area there is ample evidence for surface and sub­

surface igneous activity. However, there is little evidence for

such activity in the vicinity of Hartfell. The nearest proven

igneous body lies below the surface at Leadhills about 25 km to the

north-west of Hartfell. A recent geophysical survey has outlined

the presence of a strong magnetic anomaly in the vicinity of Moffat

(Powell, pers comm.). This anomaly follows the Caledonoid trend

and may indicate the presence of a concealed igneous body.

Carbonate metasomatism may therefore be related to this body.

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replacement is a widespread feature of the Lower Palaeozoic

greywackes (Weir 1974). Such replacement has been observed in

inliers in S.W.Ireland which are well removed from any exposed centre

of igneous activity (Weir 1962). In these instances the outcrops

occur in Carboniferous Limestone terrain and it is likely that the

sediments have been exposed for a considerable period of time to the

circulation of carbonate-rich groundwaters. Calcite is observed to

replace quartz at outcrop in sandstones exposed to semi-desert

conditions (Dapples 1967). As the Hartfell Shale sequence is

predominantly quartz rich it is possible that calcite replacement

could be related to circulating carbonate-saturated groundwater

following the Carboniferous episode of limestone deposition. However,

in contrast to Ireland, carbonate rocks are not prevalent components

of the Scottish Carboniferous. Moreover, deposition of Carboniferous

rocks in the Southern Uplands was almost certainly confined

largely to the basins in which they now occur.

On balance therefore, it would appear that the small

amount of carbonate introduced into the sequence at Hartfell is

metasomatic in origin.

Other than the visual similarity between the profiles for

K and Pb, there is no evidence to support an inter-relationship

between these two elements. Indeed, as will be shown later, K is

considered to be associated with the clay factor and Pb with the

metal factor. Lead is known to be a common substitute for potassium,

especially in igneous rocks (Fairbridge 1972). This substitution is

most frequently observed in potassium feldspars and micas both of