Fracture and surface crust development in a Holocene pahoehoe lava flow on the Island of Tenerife,Canaries |
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| Institution: | 1. Instituto de Geofísica, Universidad Nacional Autónoma de México, Circuito exterior, C.U. México D.F. 04510, México;2. Universidad de Ciencias y Artes de Chiapas, Centro de Monitoreo Volcanológico-Sismológico y Subsecretaría de Protección Civil del Gobierno del Estado De Chiapas México;3. Facultad de Química, Unidad Sisal, Universidad Nacional Autónoma de México, Puerto de Abrigo Sisal, Yucatán 97355, México |
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| Abstract: | An almost horizontal pahoehoe surface in a Holocene plagioclase basanite lava on Tenerife displays three scales of fracture within the surface crust. An early-formed set of large-scale fractures divides up the surface into an orthogonal set of rectangular slabs with dimensions of several metres and depths of 10–12 cm. The shortest slab dimension is parallel to the flow emplacement direction, inferred from a strong surface lineation. The slabs are domed with the centre an average of 9.6 cm (with range 4–19.6 cm) above the edges of the slabs. Profiles of the slabs normal and perpendicular to the margins and through the crest indicate that they can be described by a power law in which the deflection of the slab, h, is related to the distance from the crest, x, with an exponent between 2 and 3. Analysis of joints within the slabs indicates two smaller scale networks. An intermediate scale joint network bounds blocks with rectilinear to polygonal shapes in plan-view and has a characteristic mean spacing of 24.2 cm (range 10.5–48 cm). The major fractures in this set are normal and parallel to the slab margins. A smaller-scale joint network bounds polygonal equant blocks in plan-view and has characteristic spacing of 6.4 cm (range 3.7–10.5 cm). A model of cooling from the pahoehoe surface is used to constrain the growth of the crust and timing of fracture development. The large-scale slabs are attributed to localised accumulation of gas beneath the growing crust causing buoyant forces. The tensile stresses caused by uplift are sufficient to form the large-scale fractures after 2 or 3 h of cooling. The intermediate scale fracture network is attributed to the flexure of the slab crust. The smaller scale polygonal joint network is related to the build up of isotropic tensile stresses in the cooling slab crust due to thermal contraction with fracture development being promoted by the flexure of the slabs. An analysis of the slab deformation indicates that lava crust is weak. The weakness is explained by division of the crust into three zones: an outer zone with small scale joints that cause negligible strength, a middle zone of elastic behaviour in which stress can build up, and a lower zone of plastic deformation. The crustal slabs display profiles similar to that expected in a bending elastic plate. The deformation of the 10-cm-thick crust can be explained if the elastic zone was about 2-cm thick. This result agrees with an independent calculation of elastic zone thickness based on the position of the brittle–ductile transition being located at the 600°C isotherm at a depth of about 2 cm when the crustal slabs were rifted apart. |
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