Jökull


Jökull - 01.01.2020, Side 41

Jökull - 01.01.2020, Side 41
Vestergaard et al. arinsson, 1967; Larsen et al., 2013; Pedersen et al., 2018b). In Holocene times, Hekla has mainly pro- duced mixed eruptions which encompasses both ex- plosive and effusive activity (Thordarson and Larsen, 2007; Thordarson and Höskuldsson, 2008; Pedersen et al., 2018b). The eruptions in 1947–48, 1845–46 and 1766–68 were no exceptions (Figure 1). All three be- haved rather similarly, exhibiting a highly explosive subplinian to plinian initial phase (VEI 4) with sig- nificant tephra fallout (Houghton et al., 2013; Janebo et al., 2016a; Gudnason et al., 2018). The follow- ing phases were: fire fountaining, strombolian activity ending with an effusive phase generating large lava- flow fields (Thórarinsson, 1967, 1976; Larsen et al., 1999; Thordarson and Larsen, 2007; Thordarson and Höskuldsson, 2008; Pedersen et al., 2018b). The 1947–48 and 1766–68 eruptions also showed exam- ples of renewed, violent explosivity during the effu- sive phase, but these events never increased to the same force as the initial phase (Thórarinsson, 1967, 1976). Lava-flow morphology Lava is a common and persistent threat to settle- ments and understanding its properties and emplace- ment mechanisms is key for hazard assessment and for predicting lava-flow behaviour and development (Soule et al., 2004; Takagi and Huppert, 2010; Mon- talvo, 2013). This includes the estimation of lava-flow thickness, volume and emplacement style and history (e.g. Wadge et al., 1975; Stevens et al., 1999; Har- ris et al., 2000; Poland, 2014; Albino et al., 2015; Kubanek et al., 2017; Pedersen et al., 2018a). The development and emplacement of lava-flows hinge on parameters such as rheology, effusion rate and erup- tion duration, temperature, topography and surface slopes and also total volume of lava extruded (Walker, 1973; Pinkerton and Wilson, 1994; Parfitt and Wil- son, 2008). Furthermore, the rheology of the lava evolves during emplacement, because of changes in melt composition, oxygen fugacity and temperature of the magma resulting from gas loss, cooling and crys- tallisation (Hulme, 1974; Fink, 1980; Gregg and Fink, 2000; Kilburn, 2004; Kolzenburg et al., 2018). Hekla typically generates ‘a‘ā lavas (Thórarinsson and Sig- valdason, 1972; Grönvold et al., 1983; Höskuldsson et al., 2007; Thordarson and Höskuldsson, 2008) which are flows with autobrecciated exteriors and a coher- ent liquid interior during emplacement, referred to as the core. The autobreccia comprises irregular clink- ers that have rough, sharp surfaces, and are derived from the flow core (Macdonald, 1953). Common mor- phologies that are mentioned in this study, are sheet- flows which formed in a single surge of lava that is not bounded by levées (banks of solidified lava), and channelised flows of lava bounded between lev- ées (Hulme, 1974; Peterson and Tilling, 1980; Row- land and Walker, 1988; Hon et al., 1994; Harris et al., 2009; Harris and Rowland, 2015). Morphologies related to lava inflation include flat-surfaced plateaus (formed like tumuli) called lava rise, collapsed de- pressions called lava-rise pits, and marginal fractures called lava-inflation clefts (Walker, 1991). They form by the injection of lava beneath the surface layer which leads to simple uplift of the surface without any horizontal compression (Walker, 1991). The lava-rise pits and lava-inflation clefts describe, respectively, lava surfaces that failed to be uplifted, and actively in- flating interior of the lava-flow that detaches from the stagnated margin (Walker, 1991; Hon et al., 1994). Inflation structures are commonly found in pāhoehoe flows (e.g. Macdonald, 1953; Walker, 1991, Hon et al., 1994), but inflation structures and lava tubes also occur in ‘a‘ā flows (e.g. Calvari and Pinkerton, 1998, 1999; Pedersen et al., 2017). Lava tubes are insu- lated conduits of still-molten lava beneath a cooler (ultimately solidified) surface layer (Peterson et al., 1994). The boundary of the inflated lava-flow may breach, thus allowing lava breakouts and thereby new lava lobes. Breakouts do not only occur due to rupture of the cooled skin at weak points, but can also oc- cur due to effusion rate fluctuations (Thordarson and Self, 1998; Rowland and Harris, 2015; Pedersen et al., 2017). The emplacement of breakouts may vary depending on viscosity and effusion rate. DATA AND METHODS Remote sensing data and bulk volume estimates The remote sensing data consists of orthophotos and digital elevation models (DEMs) from 1945–46, 1960 and 2015 (Table 1). The remotely-sensed images 38 JÖKULL No. 70, 2020
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