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A small phreatic eruption through Crater Lake producing vertically and radially directed dark surtseyan jets of Crater Lake water, gas and solid ejecta, and a whitish radial base surge with a diameter of c. 200 m. Note low angle of the jet falling to the left. Image captured in 1971 by P. Otway. 

A small phreatic eruption through Crater Lake producing vertically and radially directed dark surtseyan jets of Crater Lake water, gas and solid ejecta, and a whitish radial base surge with a diameter of c. 200 m. Note low angle of the jet falling to the left. Image captured in 1971 by P. Otway. 

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At 20:26 (NZDT) on 25 September 2007 a moderate gas-driven eruption beneath the summit Crater Lake of Mt. Ruapehu, New Zealand generated a directed ballistic fallout apron and surtseyan jet that impacted an area of c. 2.5 km2 to the north of the vent. Two climbers were caught in the blast at a hut 600 m from the vent. Primary, ice-slurry lahars wer...

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... trend (major and trace element compositions) that spans a wide compositional range shown by eruptives between 1945 and 1996 (Gamble et al., 1999). The dense and vesicle-poor nature of the clasts suggests that they represent the degassed portions of magma from historic eruptions. Densities of the andesite lava and andesite breccia clast types were determined using the technique outlined by Carmichael (1984), and range from 1.7 g/cm 3 (cemented breccia) to 2.7 g/cm 3 (lava), with porosities of 1% (lava) to 41% (cemented breccia) (Table 1). The brecciated clasts tend to disintegrate on immersion in water, in part due to the breakdown of hydrothermal swelling clays. The lava clasts are relatively impermeable and there is little difference between wet and dry densities, while the andesite breccias and cemented lake sediments and/or vent debris are relatively permeable. The volume of ballistic ejecta produced by the 25 September 2007 event was calculated using dispersal data from aerial photographs and GIS, and clast size measurements (contoured point data) taken at various locations on the summit area (Fig. 6). The volume calculation is considered a minimum because a signi fi cant portion of the erupted material probably fell back into Crater Lake, was washed back in by run-off from the collapsing surtseyan jet, did not clear the lake rim, was carried off the summit by the eruption-triggered lahars, or was buried and masked by the jetted deposits. To calculate the volume of the ballistic material, we recorded clast sizes and types along the main dispersal axis and constructed an isopleth map (Fig 6). In order to convert non-uniformly distributed ballistics to isopachs a scaling factor, F , was determined, based on the percentage coverage of ballistic clasts and/or impact craters within a 100 m 2 quadrant at 3 locations on the summit plateau (Fig. 6). The value of F remains near-constant (0.015 to 0.013) despite increasing distance from the vent (i.e. 1.5 to 1.3% of each quadrant was occupied by ballistic clasts). The volume of the ballistic deposit was obtained by multiplying the isopleth by F = 0.013, giving a minimum estimated volume of 1.6 × 10 5 m 3 . Assuming a mean (measured) density of 2.36 g/cm 3 the erupted ballistic mass is thus c. 3.8 × 10 8 kg. In addition to the scattered ballistics emplaced across the summit plateau, an area of 2.5 km 2 was covered by a relatively thin, ash to lapilli-sized, and massively-bedded unit interpreted to be derived from a surtseyan-type event (Fig. 7). On the southern face of Dome Ridge, we excavated a pit into this deposit to determine whether there were changes in both grain size and componentry through the eruption. The deposit has a relatively uniform grain size distribution: the graphic mean ( M z ) ranges from 10 to 20 mm (Fig. 8). The surtseyan deposit consists of variably hydrothermally-altered andesite lava lithics, intensely altered rock fragments, weakly to strongly mineral-cemented lake sediments dominated by fi ne sand and mud, and recycled scoria and glass from previous historic eruptions characterised by alteration rims. Andesite lava lithics are similar in hand specimen to the discrete ballistics, comprising porphyritic andesitic lava fragments, with some lava clasts exhibiting coarsely porphyritic textures, highlighted by the range in plagioclase pheno- cryst abundance. A small proportion ( b 2 vol.%) of the surtseyan deposit probably represents juvenile magma, which appears as fresh and unaltered moderately vesicular and glassy ash and fi ne lapilli. Particle morphol- ogies are indicative of melt quenching during fragmentation and the glass is dacitic in composition (Christenson et al., 2010-this issue). The surtseyan unit is variously distributed among individual ballistic blocks, indicating a complex emplacement chronology. The surtseyan deposit was distributed northwards along a similar azimuth to the ballistic apron, and its thickness appears to be locally controlled by summit topography, implying emplacement from a low-angle directed jet and a component of post-depositional fl ow and modi fi cation. This is seen clearly in the area of North Crater where the crater margins have contained the fl ow, causing minor, yet diffuse run-up (Fig. 7). Although the 25 September 2007 eruption occurred at night, dynamically similar eruptions have occurred during the 1970's, 1980's and 1990's during daylight and fi ne weather, and have been videoed and photographed by many eye-witnesses. These observations yield valuable insights into the nature of gas-driven, phreatic and phreatomagmatic blasts through Ruapehu's Crater Lake. Dark surtseyan jets (e.g. Kokelaar and Durant, 1983) of explosively displaced water droplets, also referred to as ‘ rooster-tails ’ or ‘ cockscomb jets ’ may have risen N 800 m above Crater Lake, while simultaneously ejected ballistic blocks fl ew further and faster due to greater inertia leaving white vapour trails in the atmosphere (Fig. 9). As the jets collapse and fall under the in fl uence of gravity, they impact the snow pack, leaving sharp-edged deposits that closely match their maximum projection range: a northward-directed jet from the 23 September 1995 eruption travelled c. 2 km in ∼ 20 s. Diffuse base surges develop from dilute parts of the collapsing jets and higher white steam column, but do not appear to produce signi fi cant deposits. Due to the different velocities and trajectories of the ballistics and surtseyan jets, they arrive at the ground surface in a variable and complex order: the last deposits to be emplaced are high- fl ying ballistics with launch angles N 45°. The volume of the September 2007 jetted deposit was determined by measuring ash thickness at various locations across and down the main northward-directed dispersal axis (Fig. 7). The variable topography of the summit plateau and syn- and post-depositional fl owage of the jetted deposit under the in fl uence of gravity resulted in a highly variable deposit thickness. At Dome Ridge, the jetted deposit is represented by a b 1 cm thick veneer, while in Central Crater it is ponded to a thickness of 10 – 12 cm. Based on a crude isopach map (Fig. 7), the minimum volume of the jetted deposit is estimated at c. 1 × 10 5 m 3 : giving an erupted mass of c. 2.4 × 10 8 kg assuming a mean density of 2.36 g/cm 3 . Some jetted and ballistic material was lost by run-off to form lahars (see below). Water ejected from Crater Lake in the directed surtseyan jet, together with condensate from the high eruption steam column, fell on the summit area of Mt. Ruapehu, running off and entraining the upper part of the seasonal snowpack to form a number of ice-slurry lahars (Lube et al., 2009). Similar multi-component volcanogenic mass- fl ows have occurred during previous eruptions of Ruapehu (Cronin et al., 1996a), and at other snow-clad volcanoes overseas (Pierson and Janda, 1994; Waitt et al., 1994; Major and Newhall, 1989). Two eruption-triggered lahars are recognised in the eastern Whangaehu catchment; with a third fl ow occurring c. 1.5 h after the initial explosion. The fi rst and largest lahar consisted of two near- simultaneous pulses (W1a and W1b) resulting from run-off of ejected Crater Lake water, ballistics, and entrained snow and ice from the head of the Whangaehu Glacier, the fl anks of Dome, and the southern half of Central Crater (Fig. 1). These fl ows left a 200 – 280 m wide grey deposit of ash-coated mm-diameter ice particles, fragments of ejected lake sediment, and ash, lapilli and blocks as a swath running down the centre of the 17 o Whangaehu Glacier (Figs. 1 and 2), before entering the North Branch of the Whangaehu Gorge (only minor overspill occurred into the South Branch). Evidence for erosion includes shallow gullies and potholes cut in the glacier surface. Pulses W1a and W1b travelled 7.3 km and 8.5 km respectively, giving H/L ratios of 0.162 and 0.168, similar to snow-slurry lahars at other volcanoes (Pierson et al., 1990; Pierson and Janda, 1994; Waitt et al., 1994; Cronin et al., 1996a). The combined area of W1 is 8.14 × 10 m , most of which represents the broad but thin swath on the Whangaehu Glacier; once con fi ned in the gorge the deposits are narrower but thicker. Total deposit volume is estimated at c. 3.5 – 7.0 × 10 5 m 3 . A second lahar (W2) was generated by syn-eruptive water displacement across the lake outlet coupled with a topographically- controlled base surge into the outlet gorge. It fl owed across the toe of a large landslide c. 500 m downstream where it picked up additional lithic material that gave the deposit a distinctive brown colour. W2 fi lled the outlet gorge to a width of c. 60 – 80 m and a depth of 6 – 8 m, giving it a cross-section area similar to the much wider but shallower W1 pulses on the Whangaehu Glacier, and travelled c. 10.7 km from source (H/L ratio = 0.122) to cover an area of 330,000 m 2 with a volume estimated at c. 2.5 – 5.0 × 10 5 m 3 . At the RTMT lahar monitoring site, 7.1 km downstream from Crater Lake, lahar pulses W1a and W1b formed a single grey depositional unit that buried the 80 m-wide valley fl oor beneath 1 – 3 m of frozen ice slurry containing clay to boulder-sized lithic material (Fig. 10). This was partially overlain by the grey-brown deposits of W2. The matrix of both consisted of mm- sized sub-rounded particles of clear ice, representing modi fi ed snow and fi rn, coated with a fi lm of silt and clay. Both units showed coarse- tail normal grading: coarse clasts included ice fragments up to 15 cm in diameter and lithic boulders up to 70 cm across. Lithic clasts were dominated by hydrothermally-altered andesite lava (36 – 50 wt.%) and scoria (18 – 20 wt.%), often veined or crusted with gypsum and alunite, and pieces of pale, laminated lake- fl oor sediment (34 – 43 wt.%). Black mm-sized globules of sulphur were abundant in the matrix. The deposits of W2 contained a slightly higher proportion ...

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Volcanic ballistics are the main hazard to life and infrastructure from Strombolian eruptions, which are a tourist drawcard, exposing people to this hazard. Most research to date has been to understand this style of eruption and how ballistics form and travel. However, little focus has been placed on how ballistics are distributed within ballistic fields or the inclusion of this data into hazard and risk assessments. In this study we used a UAV to image the ballistic field, and cameras to record eruptions at Yasur Volcano, Vanuatu from 28 July – 2 August and 17 – 19 October 2016. We present the mapped distributions from the two trips, how the field changes with distance and direction from the vent, and how eruption dynamics influence these changes. Our evidence for directionality results in considerable variation in summit ballistic hazard and is an important consideration for ballistic hazard and risk assessments.
... We infer this material to be a region of altered rock most likely reflecting the present day and previous hydrothermal systems. Andesite ballistic blocks from beneath Crater Lake, ejected in the 2007 eruption (Kilgour et al., 2010), are moderately to highly altered and have measured susceptibility of <0.002 SI, consistent with the low apparent susceptibility region recovered by our model. We tentatively interpret this to be the upper portion of the plumbing system ("heat pipe") (Christenson & Wood, 1993;Hurst et al., 1991) that supplies heat, gas, liquid, and occasionally magma to Crater Lake. ...
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Combining 3‐D inversion of high‐resolution aeromagnetic data with airborne hyperspectral imaging creates a new method to map buried structure and hydrothermal alteration, applied to Mt. Ruapehu volcano, New Zealand. Hyperspectral imaging is sensitive to surface mineralogy including alteration minerals, while magnetic vector inversion reveals the volumetric distribution of magnetic susceptibility from which we interpret buried geology. Probability assessment from multiple model regularizations provides an important model uncertainty estimate. At Ruapehu, hyperspectral imaging highlights two main regions of surface alteration: the Pinnacle Ridge and the southeast flanks. The magnetic model of Pinnacle Ridge shows that alteration seen at surface continues to depth, but strongly magnetic, unaltered dikes form the core of the ridge. On the southeast flanks, the magnetic model also shows alteration imaged on the surface continues to depth; however, a previously unknown, magnetized sill intrudes part of the flank. Several smaller demagnetized regions are modeled, unlike at neighboring Mt. Tongariro where the hydrothermal system created a large demagnetized core. We propose that these differences relate to spatially focused (Ruapehu) vs distributed (Tongariro) eruption vents, the degree of faulting of the edifice and its glaciation history. Lava‐ice interaction produces fine‐grained lavas with measured magnetic susceptibilities similar to some moderately altered lavas, illustrating that care must be taken in the interpretation of magnetic data in the absence of geological information. The combination of hyperspectral imaging and aeromagnetic data inversion distinguishes shallow surface weathering from deeper‐seated hydrothermally altered rock masses, with implications for the magnitude and probability of collapse events.