Computer Science
Scientific paper
Jan 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977e%26psl..33..310k&link_type=abstract
Earth and Planetary Science Letters, Volume 33, Issue 3, p. 310-320.
Computer Science
11
Scientific paper
Most dykes appear to be intruded in a zone less than 50 m wide at spreading ridges, while the lavas they feed flow out 1 km or so to either side (Kidd, 1976, 1977). The resulting oceanic crust consists of a lava layer with few dykes which grades down through a rapid transition of increasing dykes into a sheeted dyke layer which in turn grades down into gabbro. The shape of the source blocks of oceanic magnetic anomalies can be determined from this structure. The boundary between two adjacent blocks is effectively sharp and dips: toward the spreading axis at a shallow to moderate angle in the lavas, then steeply away in the sheeted dykes and finally gently away from the spreading axis in the gabbro. There is no significant mixing of oppositely magnetised rocks across such a reversal boundary. In older oceanic crust (more than a few million years) the lavas are probably only a few times more highly magnetised than the sheeted dykes and gabbro. Consequently the latter may make a significant contribution to observed magnetic anomalies, particularly when the width of the source blocks is large. Source blocks of this shape may explain several enigmatic features of magnetic anomalies and provide better matches of computed with observed anomalies than thin, vertical sided blocks.
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