Abstract
Summary. Five hundred and sixteen sites in Arran were sampled. After cleaning by heating and/or alternating fields 87 per cent yielded directions with α95 < 10°, comprising 435 dykes, 12 sills and one granite; polarities could be determined for some of the remainder. Directions are thought to be primary and on average are shallower than corresponds to the mean centred axial dipole, with many shallow reversely‐magnetized dykes present. Seventeen per cent of the dykes are normally magnetized, 5 per cent have intermediate directions. Polarity does not correlate with petrography, thickness or trend, but does depend upon location. In particular, on the NE coast up to 70 per cent are normal, and possibly belong to a different swarm. Normal polarities were found for both sites in the Northern Granite, for Holy Island and for some of the sills. In conjunction with the known stratigraphy this shows that the rocks were formed during an R‐N‐R sequence of polarities, or more probably R‐N‐R‐N. Using the radiometric age of 58 Ma for the Northern Granite and the best estimate of the polarity time‐scale the duration of activity was probably in the range 0.5 to 3.4 Ma if three polarity periods were involved, and 3.4 to 4.4 Ma if four were involved. Copyright © 1978, Wiley Blackwell. All rights reserved
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CITATION STYLE
Dagley, P., Mussett, A. E., Wilson, R. L., & Hall, J. M. (1978). The British Tertiary igneous province: palaeomagnetism of the Arran dykes. Geophysical Journal of the Royal Astronomical Society, 54(1), 75–91. https://doi.org/10.1111/j.1365-246X.1978.tb06757.x
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