Jökull


Jökull - 01.01.2016, Síða 74

Jökull - 01.01.2016, Síða 74
Þorsteinsdóttir et al. Fragmentation in most of the phreatoplinian erup- tions described by Houghton et al. (2000) was brought about by vesiculation and bubble expansion, as well as by quenching by external water. The pumice clasts were vesicular enough to imply that the magma had already formed foam and perhaps begun to fragment or disintegrate before it first encountered external wa- ter. The fragmentation resulting from the magma- water interaction could be the result of thermal con- traction upon quenching, brittle failure caused by high strain rates resulting from expansion of steam or both these mechanisms. Lithics appear to be less com- mon in phreatoplinian eruptions than in the basaltic ones. This could suggest that the fragmentation caused by water takes place at the interface between the magma and ice/water, rather than deeper in the conduit (Dellino et al., 2012). Knowledge about silicic phreatoplinian eruption columns or plumes is limited. It has been suggested that limited amount of water will have little effect on the height and dispersive power but excessive amount will cause column collapse and pyroclastic flows or surges (Houghton et al., 2000). Only two examples of recent subglacial explosive silicic (>63% SiO2) eruptions were found in litera- ture (Guðmundsson et al., 2012; Kratzmann et al., 2009). It is suggested that some phases of the 1991 Hudson eruption were phreatoplinian because of the fine ash produced. However, no phase of the Eyja- fjallajökull eruption was classified as phreatoplinian, although about 94% of the tephra from the first phase (14-16 April) was smaller than 1 mm and up to 50% smaller than 0.063 mm (Gudmundsson et al., 2012). METHODS Tephra samples were collected from soil sections at Framgil on Álftaversafréttur and Einhyrningur west of Markarfljót (Figure 2), 22 and 20 km from cen- tre of caldera, respectively. At each location the tephra layers were cleaned, photographed, measured and macroscopic features described such as bedding, grading, colour, texture, grain size and grain types (for details see Thorsteinsdóttir 2015). Grain analyses Sieving by hand (to avoid breaking/abrading) was used for size fractions larger than 4Φ (0.063 mm) and settling velocity less than 4Φ. A Sedigraph (Mi- cromeritics, 2010) was used for grains smaller than 4Φ. The results from both methods were combined and plotted on a graph, showing the complete grain size distribution of each tephra sample. The elongated grain shape of the SILK tephra may affect the size results because particle size techniques assume that grains are spherical. A comparison between the SILK tephra layers is however considered justified. Grain morphology analysis was carried out on se- lected samples from four eruptions. The parameters ruggedness (ratio of convex perimeter to total perime- ter, CPERIM/PERIM), elongation (ratio of minimum to maximum diameter, DMIN/DMAX) and circularity (4πAREA)/(PERIM)2 were measured using an image analysis program (Eiríksson et al., 1994). Scanning electron microscope (SEM) images on selected tephra samples were obtained using a Hitachi TM3000 electron microscope, in order to demonstrate potential differences between tephra layers which might reflect different eruptive environments. RESULTS Samples from 10 SILK tephra layers were analysed for grain size and 4 samples for grain shape, including the previously analysed SILK-LN layer (Thorsteins- dóttir et al., 2015). The main focus was on possible changes during the period from 2800 to 8100 years ago. The tephra samples were collected at similar dis- tance, 20–22 km, from the center of Katla caldera. The thickness axes are, however, not known for all the layers. Tephra layers SILK-YN, SILK-MN and SILK-A9 were not included in this study. The remain- ing layers (except SILK-A11) were grain size anal- ysed, and SILK-N1, SILK-A8, SILK-A11 and A12 were analysed for grain shape (Table 3). Changes in grain size The younger part of the silicic tephra sequence ap- pears coarse grained while the older part is fine grained (Table 3). The largest grains in the coarser section belong to the grain size categories from -3Φ to 74 JÖKULL No. 66, 2016
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