Jökull


Jökull - 01.12.1984, Side 91

Jökull - 01.12.1984, Side 91
Fig. 12. The upper end of four dykes. All the dykes end in lava flows. The red inter- beds and scoria between the lava flows are hatched, the dykes are black. The sections are steep or vertical. The illustrations are schematic but are approximately to scale. (?) means that this part of the dyke is not well ex- posed. Dyke (a) is in vertical cliffs. It is of tholeiite basalt and contains many vesicles, which are up to 0.5 cm in diameter. The dyke does not occupy a dip-slip fault, and no fracture is apparent ahead of its upper end. The host rock is tholeiite basalt. Dyke (b) is in vertical cliffs. It is of tholeiite basalt, and small vesicles (1 mm in diameter) are common. It does not occupy a dip-slip fault. The dyke is divided into two parts in this section. C is a joint. The host rock is porphyritic basalt. Dyke (c) ends in vert- ical cliffs. It is of tholeiite ba- salt, but contains hardly any vesicles. It has chilled selvage on its edges. The host rock is scoria in the lower part of the section and tholeiite lava in the upper part. Dyke (d) is of tholeiite basalt with inconspicuous vesicles. The host rock is scoria in the lower part of the section, but tholeiite lava in the upper part. No evidence was found that dykes (c) and (d) occupied dip-slip faults. Mynd 12. Myndin sýnir hvernig fjórir gangar enda upp á við í hraunlögum í svo til lóðréttu sniði. Teikningarnar eru í réttum hlutföllum. east, and the remainder to the south, west, or are vertical. Because many of the faults dip in a direction opposite to the dip direction of the lavas, then if they formed before the tilting of the lava pile their initial dip must have been steeper. Taking the tilting of the lava pile into account would, however, not much change the average dip of the faults because the dip of the lava pile is, on the average, only a few degrees. Also, it is likely that the tilting of the lava pile was a con- tinuous process, accompained by faulting and dyke intrusion, so many of the faults probably formed after a part or all the tilting of the lava pile had occurred. The initial dip of most of the faults, therefore, was presumably similar to that observed today. The throw of the faults is from 0.5 to 25.0 m, with an average of 5.3 m (Fig. 16). In the cliffs, I followed some of the faults upwards to see if any noticeable change in the throw occurred. For the few faults which could be followed upwards, the throw was essentially the same 80-100 m higher JÖKULL 34. ÁR 89
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