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Multi-stage volcanic island flank collapses with coeval explosive caldera-forming eruptions

  • Scientific Reportsvolume 8, Article number: 1146 (2018)
  • doi:10.1038/s41598-018-19285-2
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Volcanic flank collapses and explosive eruptions are among the largest and most destructive processes on Earth. Events at Mount St. Helens in May 1980 demonstrated how a relatively small (<5 km3) flank collapse on a terrestrial volcano could immediately precede a devastating eruption. The lateral collapse of volcanic island flanks, such as in the Canary Islands, can be far larger (>300 km3), but can also occur in complex multiple stages. Here, we show that multistage retrogressive landslides on Tenerife triggered explosive caldera-forming eruptions, including the Diego Hernandez, Guajara and Ucanca caldera eruptions. Geochemical analyses were performed on volcanic glasses recovered from marine sedimentary deposits, called turbidites, associated with each individual stage of each multistage landslide. These analyses indicate only the lattermost stages of subaerial flank failure contain materials originating from respective coeval explosive eruption, suggesting that initial more voluminous submarine stages of multi-stage flank collapse induce these aforementioned explosive eruption. Furthermore, there are extended time lags identified between the individual stages of multi-stage collapse, and thus an extended time lag between the initial submarine stages of failure and the onset of subsequent explosive eruption. This time lag succeeding landslide-generated static decompression has implications for the response of magmatic systems to un-roofing and poses a significant implication for ocean island volcanism and civil emergency planning.


Volcanic island landslides, their associated tsunamis, and volcanic eruptions pose significant natural hazards to both life and infrastructure. Lateral flank collapse of shield volcanoes can yield prodigious landslides with volumes in excess of 300 km3, such as those in the Hawaiian, Canarian, Cape Verdean and Reunion archipelagos1,2,3,4,5,6,7,8. These are among the largest mass movements on Earth, whose size is far larger than any subaerial landslide9. Such voluminous landslides are especially hazardous because they may cause high-amplitude tsunamis on entering the ocean and also be directly associated with major volcanic eruptions10,11,12,13,14.

Direct observations of volcano flank collapse on land have shown that they can be immediately succeeded by major explosive eruptions. For instance, events at Mount St Helens in 1980 showed how ascent of magma and emplacement of a crytodome caused the edifice to inflate, oversteepen and become unstable15,16. On May 18 1980 at 08:22:11 local time, a 5.1 Mw earthquake related to magma intrusion occurred and triggered a single-stage flank failure ten seconds later comprising two slide blocks17,18. The resulting landslide was followed after thirty seconds by a devastating series of explosive eruptions including a lateral blast that took fifty-eight lives, cost over a billion US$ in damages, and resulted in unquantified potential respiratory health risks to local residents involved15,16,18,19. In addition to the immediately post-collapse lateral blast at Mount St Helens, intense explosive activity continued for nine hours after the initial failure; this was followed by further explosive activity on 25 May, 12 June, 22 July, 7 August and 16–18 October 1980. The later episodes of activity in this sequence punctuated lava dome growth accompanied by frequent minor explosions17.

Mount St Helens is not an isolated example. Well constrained chronologies of the Harimkotan 1933 Bezymianny 1956 and Shiveluch 1964 demonstrate that initial flank collapses were followed by explosive eruptions20. Indeed, the 1964 event at Shiveluch demonstrates that an initial collapse was followed first by a phreatic explosion and then an explosive Plinian eruption20. Analysis of older debris avalanches at Shiveluch indicates this scenario may have been common in the past21,22,23. However, many stratovolcano lateral collapses do not show evidence of coincidental lateral blasts or other types of explosive eruption24,25. Thus, terrestrial volcanoes do not show a consistent coincidence of flank collapse and eruptions, and so there are issues with invoking a cause-and-effect relationship. However, past events on Tenerife, in the Canary Islands, may elucidate the range of relationships between flank collapses and large explosive eruptions.

The Canary Islands is among the most active volcanic archipelagos. Indeed, Tenerife is one of the world’s largest active volcanoes having experienced numerous Plinian eruptions and caldera-collapses, many of which have ejected volumes up to fifty times greater than the 1980 Mount St Helens eruption26,27,28. Furthermore, the Canary Islands, and in particular Tenerife, have incurred numerous large landslides over the last seven million years (roughly every 150 to 250 kyr) with volumes often over 300 km3 (Fig. 1)6,7,8. There is growing evidence that suggests explosive eruptions and mass wasting processes have a cause-and-effect relationship in ocean island settings7,12,29,30,31,32,33,34; whereas some other terrestrial volcanoes show no such relationship9,24,25. During the development of the Canadas Upper Group (1.56 Ma to 0.17 Ma) on Tenerife, in the Western Canary Islands, the Canadas volcano underwent three distinctive phases of growth and destruction, each ending with both a caldera eruption and a coeval lateral flank collapse (Fig. 2)7,8,29,30,31,32,33,34,35. Thus Tenerife presents an excellent opportunity to examine the relationships between these two destructive processes.

Figure 1
Figure 1

Map of the Canary Islands and the Moroccan Turbidite System. Canary Islands debris avalanche deposits shown in black, while Icod deposit is in dark green, the Orotava deposit in dark blue, Roques de Garcia in red, and Cumbre Neuva in yellow. Pale overlay signifies the spatial distribution of the sediment gravity flow deposits associated with the Icod landslide from Northern Tenerife. Sediment core locations are shown as red circles, while cores referenced in this contribution are in yellow and labelled (including ODP Sites 950, 951 and 952). Abbreviations are: AC = Agadir Canyon, AB = Agadir Basin, MAP = Madeira Abyssal Plain, SAP = Seine Abyssal Plain, MDCS = Madeira Distributary Channels, and CBR = Casablanca Ridge. Canary Islands landslides Icod (brown), Orotava (purple) and Rogues de Garcia (red) from Tenerife and Cumbre Nueva (grey). May also shows the area extent of the turbidites associated with the Icod landslide. Map was generated using ArcGIS 10.1 software based upon bathymetric and digital elevation data from GEBCO.

Figure 2
Figure 2

Timing of flank collapses from Northern Tenerife and caldera-forming eruptions. Volcaniclastic turbidites from the Madeira Abyssal Plain recorded at site D11814 (location on Fig. 1). Biostratigraphic and photospectral data from Hunt et al.7. Timing of caldera-forming eruptions from Marti et al.35. Further information regarding the timing of landslides and caldera eruptions and the nature of the deposits are documented in supplement 1.

Previous studies postulate that caldera-forming and similar explosive eruptions may cause ground accelerations that trigger flank collapse33,34. For example, the 2002 explosive eruption of Stromboli Volcano caused a sequence of subsequent tsunamigenic landslides36. The involvement of caldera-forming eruptions on ocean islands influencing flank collapse is postulated with the specific reference to the formation of the Icod and Orotava Valleys on Tenerife31,32,33,34. However, preliminary evidence from distal marine deposits of the Icod landslide (165 ka) on Northern Tenerife and terrestrial deposits from the resulting landslide-tsunamis suggest that initial stages of multistage submarine flank failure were succeeded by the Abrigo caldera-forming eruption12,37. Here, we investigate this relationship between volcanic island landslides and large explosive, often caldera-forming, Plinian eruptions. We wish to understand whether landslides and eruptions are linked, and if so, which comes first. Past work has shown that large-volume volcanic island collapse can occur in multiple distinct stages or sub-units12,38. Therefore we also wish to understand whether particular stages of failure are associated with the eruptions and test previous hypotheses regarding the influence of ocean island flank collapses towards changing magma chamber pressure regimes at depth39.

Our study examines distal marine deposits, called turbidites, from the multistage Icod, Orotava and Roques de Garcia flank collapses on Northern Tenerife. The ages of these deposits coincide with the timing of Abrigo and Granadilla eruptions that generated the Diego Hernandez and Guajara calderas, respectively, and ignimbrite eruptions that created the Ucanca caldera (Fig. 2; Supplementary 1)7,12,27,29,30,31,40,41,42,43,44. We compare chemical compositions of volcanic glass from multiple turbidite layers (sub-units) of these individual slides deposited in the basins adjacent to the Western Canary Islands. These data represent newly analysed volcanic glasses and those collated from past studies12,38. We also analyse volcanic glasses from the coeval Abrigo and Granadilla eruptions recovered from terrestrial exposures near the town of Tajao, Southern Tenerife. We also collate previous analyses of volcanic glasses from a tephra recovered in ODP Core 953 dated to ~1.0 Ma synonymous with the caldera-eruptions at the end of the Ucanca Formation45,46. Comparison of compositions of volcanic glasses from the landslides and eruptions provides a uniquely detailed investigation of the landslide dynamics and their relationships with island volcanism (Supplementary 1, 2)6,7,38.

Tenerife’s flank collapses and their relationship to caldera eruptions

The Las Cañadas volcanic edifice on Tenerife has a history punctuated by both effusive lava flows and explosive eruptions of phonolitic ignimbrites31,47. Indeed, recent volcanism has occurred within three cycles, each culminating in a caldera-forming eruption, these include the most recent Abrigo (160–185 ka) at the end of the Diego Hernandez Cycle, Granadilla (560–600 ka) ignimbrites at the end of the Guajara Cycle, and a series of ignimbrites (1.0–1.2 Ma) at the end of the Ucanca Cycle (Supplementary 12)31,40,41,42,47. The northern flank of Tenerife is sculpted by the voluminous multistage Icod (165 ± 5 ka), Orotava (535 ± 5 ka) and Roques de Garcia (1.15 ± 0.01 Ma) landslides, which broadly coincide with the age of the Abrigo, Granadilla and terminal Ucanca caldera-forming eruptions (Fig. 2; Supplementary 1)6,7,12,39, suggesting that the collapses and eruptions are likely linked7,12,29,30,37; although the nature of that link remained unresolved with certainty.

Turbidites were deposited beneath dilute turbulent sediment flows formed as the slide mass moved downslope under gravity and disaggregated7,8,12,38. Canary Island landslide deposits in adjacent deep sea basins, such as those of the Icod, Oratava and Roques de Garcia landslides, are unusual as they comprise a series of stacked graded turbidite sand and mud intervals, called sub-units (Fig. 3)12,38,48,49. These sub-units are compositionally distinct and record landslide emplacement into the ocean in a series of retrogressive stages12,38,49. In these distal deep-sea environments over 500 km from the islands, each turbidite sub-unit is often separated by a 5–75 cm layer of clay and fine silt. These fine-grained intervening sediments settled relatively slowly from the waning turbidity current, potentially reflecting substantial time lags (representing at least tens to hundreds of hours) between individual successive sub-unit failures (Fig. 3)12. The initial sub-unit(s) within the distal landslide deposits are thicker and contain marine bioclastic sediment and altered volcaniclastics in contrast to later sub-units12,38,49. This suggests that the initial stage(s) of each landslide comprised most of the failure volume, and were sourced from submerged parts of the volcanic island12,38. Later sub-units are smaller-volume and are composed almost entirely of unaltered volcanic glass from the flanks of the active subaerial edifice12,38,49, implicating progressive sub-unit failures migrated retrogressively from the submerged to the entirely subaerial flanks of the volcano12,38,49.

Figure 3
Figure 3

Deposits from the Icod, Orotava and Roques de Garcia landslides from Tenerife recovered from the Agadir Basin and Madeira Abyssal Plain. Deposits show the presence of subunits, with multiple fining-upwards sands that are amalgamated proximally but form discrete sand-mud couplets distally. Distally from source these individual turbidite sub-units are separated by 5–75 cm of turbidite mud representing fine suspension fallout that has settled and consolidated between the flows of each failure stage. SBU stands for sub-unit.

We compared the major element composition of volcanic glasses in the sub-units of the Icod and Oratava landslide-turbidites with the volcanic glass compositions of terrestrial ignimbrite deposits of the Abrigo and Granadilla caldera-forming eruptions. These two caldera-related ignimbrites have distinct glass chemical compositions (Fig. 4). Our work confirmed that only the uppermost sub-unit of the Icod deposit (sub-unit 7), the last stage of multi-stage flank collapse, contains volcanic glasses of the same composition as the Abrigo ignimbrite (Fig. 4). A similar relationship is seen for the Orotava deposit, where only the uppermost sub-units (sub-units 4 and 5) contain volcanic glasses that are consistent with the Granadilla ignimbrite (Fig. 4). Importantly, glasses of compositions representing these ignimbrites are not found in initial sub-units of either Icod or Orotava failure (Fig. 4). This implies that the lattermost stages of landsliding during each multi-stage landslide took place following the deposition of the respective ignimbrites; so the caldera-related eruptions preceded these last subaerial landslide stages in a temporal sequence, but succeeded an initial series of submarine flank landslides.

Figure 4
Figure 4

Compositions of volcanic glasses recovered from sub-units of the Icod, Orotava and Roques de Garcia deposits from Tenerife plotted on Total Alkali-Silica (TAS) diagrams. The Icod deposit represents a collation of data from sub-units from core sites from Agadir Basin and the Madeira Abyssal Plain (data from Hunt et al.7,12,49 and Supplementary 2 inc. 283 new analyses from core D11813 in the Madeira Abyssal Plain), while Orotava and Roques de Garcia subunits are only sampled in the Madeira Abyssal Plain (data from Hunt et al.38 and Supplementary 2 inc. 150 new analyses from core D11813 and 42 new analyses from D11814 in the Madeira Abyssal Plain respectively). Compositions of Abrigo, Granadilla, and Ucanca ignimbrite glasses and whole rock samples were collated from published work (tephra deposit 1.00–1.12 Ma in ODP 953, Rodehurst et al. 1998) and new glasses analyses of the Abrigo (41 new analyses) and Granadilla (47 new analyses) ignimbrites from this study are also plotted for comparison (data from Supplementary 3). Additional composition data of ignimbrite glasses collated from literature44,45,52,66,67,68. Figure show that volcanic glasses explosive volcanic eruptions, including caldera collapse, proposed as being coeval with landslide are only present in the later sub-units, and not present in the initial submarine stages. SBU stands for sub-unit.

The Abrigo and Granadilla eruptions had volumes of 10 and 20 km3, respectively28, and likely rapidly covered the subaerial part of the island with erupted material within a matter of hours. Tephra fallout from the eruption columns and co-genetic pyroclastic density currents would emplace erupted material across the island’s submerged slopes most likely within hours to days from the start of the eruption50,51. Thus should the eruptions have occurred prior to commencement of flank collapse, there should have been both the volume and spatial distribution for that material to be present in the initial stages of the Icod and Orotava flank collapses. Our results imply that the initial failure(s) occurred prior to and thus potentially triggered the final most explosive eruptions in each respective eruption cycle, which in these cases were caldera-forming eruptions. Whilst the landslides do not specifically cause caldera-collapse eruptions, as the magmatic system would have independently developed conditions towards such an eruption, the landslide occurrence may instead escalade the final eruption or induce its occurrence earlier than expected.

A question remains what ultimately triggered the initial submarine stages of each multi-stage landslide leading to the subsequent caldera-collapse eruption and further subsequent subaerial mass wasting? Indeed, could earlier pre-eruptive seismic activity or smaller escalating eruptions trigger the multi-stage flank collapse and commence the aforementioned scenario? Each of the Abrigo and Granadilla terrestrial volcanic successions show a series of pumaceous lapilli fall deposits before the final ignimbrites and tephras representing the caldera collapse eruptions28,42,52. Thus eruptive activity prior to and escalating towards the final caldera-forming eruption may be responsible for triggering the initial submarine stages of flank collapse and inducing the aforementioned scenario.

The Roques de Garcia landslide from Northern Tenerife occurred at 1.15 ± 0.01 Ma, dated from an event bed in the offshore Madeira Abyssal Plain7,8, supports evidence from the Icod and Orotava landslides. This slide is also represented in the deep sea by a series of stacked turbidites representing multistage collapse, similar to the Icod and Orotava deposits (Fig. 3)38. This flank collapse occurs coincidentally with a tephra recovered in ODP Cores 953, 954 and 956 (~1.00–1.15 Ma) that represents an ignimbrite eruption at the end of the Ucanca Formation (1.05 Ma)45,46. Volcanic glasses of terminal Ucanca ignimbrite eruptions have compositions only present in the uppermost subunit (sub-unit 4) (Fig. 4). This supports evidence from the Icod and Orotava landslides, whereby the initial submarine stage(s) of flank collapse likely triggered by volcanic activity or related seismicity are followed by a major explosive eruption, in this case caldera-collapse, and finally the last stage(s) of subaerial flank collapse that contain material from the preceding eruption.

Discussion of landsliding influence on explosive volcanism

Our study importantly demonstrates that whilst early eruptive activity may trigger initial large-volume submarine stages of flank collapse on Tenerife, these initial submarine stages of flank collapse occurred before caldera collapse and potentially induce the eventual explosive eruption. This is demonstrated by only the last stage(s) of the Icod, Orotava and Roques de Garcia failures containing glasses of the respective coeval eruption, thus occurring post-eruption, whilst initial stages are devoid of volcanic glasses of such compositions and are pre-eruption (Figs 34). This data supports models that suggest the significant pressure changes involved with large-scale removal of surface material during flank collapse may be responsible for inducing caldera-collapse eruptions39,43,44,45. This is through means of forced decompression on the magma chamber by removal of overburden by landsliding.

One suggestion is the volcanic island flank collapse leads to decompression of relatively shallow magma chambers likely present during the Ucanca, Granadilla and Abrigo caldera-forming eruptions. Although whilst the landslides induced the final eruptions, the style and explosivity of those eruptions were likely constrained by the properties of the magma chamber that had developed. However, the scenario may be more complicated, at least for the 165 ka phonolitic Abrigo eruption. The Abrigo magma was generated at a pressure of 130 ± 50 MPa at a relatively shallow depth of 4–5 km, but was originally water and volatile undersaturated during magma storage53. It is suggested that an input of volatile-rich mafic magma from depth was likely needed to trigger the caldera-collapse eruption. Numerical modelling demonstrates that landslide-induced unloading of about 3% of an island mass can cause a pressure reduction of several MPa at shallow depths below ocean islands39. This pressure reduction deteriorates exponentially with depth but is still significant at 18–26 km depths beneath Tenerife where primitive basaltic magmas likely accumulate and differentiate39,53,54,55,56. The landslide decompression may have had the effect of instigating the basaltic magma to rise. Despite landslide-induced decompression the shallow Abrigo magma was water and volatile undersaturated (~3 wt% H2O), and may not have erupted explosively53,55. Mixing with the deeper ascending volatile-rich basaltic magma may have instigated such an explosive eruption represented by the Abrigo caldera-collapse53,54,55,56. Effusion of less evolved lavas with high volatile contents follow large flank collapses and ignimbrite eruptions on Tenerife, supporting the notion of deep magma ascent following induced decompression29,39,53,54,57.

For the Icod, Orotava and Roques de Garcia landslides on Tenerife we suggest the following scenario. Firstly, early volcanic activity may initially trigger lateral volcanic island collapse of the submarine flank. Static depressurisation effect caused resulting from flank collapse decompress a shallow magma chamber and induces eruption, and in these cases caldera-forming eruptions. However, where magma compositions were too volatile-undersaturated for such eruptions to commence, static decompression may have caused liberation of mafic, volatile-rich magmas at great depths that ascended and mixed with the shallower volatile under-saturated magma, and finally triggered an explosive eruption29,39,54. The static decompression affects of landslides on ocean island magmatic systems is not restricted to the Canary Islands, with similar effects evidenced from multistage collapses on Montserrat, in the Lesser Antilles57,58.

Multistage collapse, explosive eruptions and tsunamis

Here, we present evidence that triggering eruptions by multistage flank failure is not always instantaneous as observed at the lateral blast of the 1980 Mount St. Helens eruption (Fig. 5). Analysis of stacked turbidites of these landslides recovered in sediment cores from the Madeira Abyssal Plain identified between 5 and 75 cm of 2–4 μm clay is deposited between individual sub-units. It has been suggested that to first deposit and then consolidate these fine-grained intervening sediments to resist erosion by successive sub-unit flows would require time lags on an order of hundreds of hours12. These time lags have a geodynamic and associated geohazard implication, whereby several days to weeks may pass between successive stages of flank collapse and that similar prolonged time may pass before a triggered explosive caldera eruption may occur (Fig. 5).

Figure 5
Figure 5

Idealised model for the relationship between the multistage Icod, Orotava and Roques de Garcia landslides and the Abrigo, Granadilla and terminal Ucanca Formation caldera-forming eruptions. (A) Minor vent related volcanism and shallow magma chamber activity precondition the submarine slopes to fail. (B) Minor eruptions and related seismicity trigger initial submarine stages of multi-stage landslides. (C) Submarine landslides unroof both shallow and deep magma chambers, this either (i) caused static decompression in the shallow magma chamber causing immediate explosive eruption, or (ii) static decompression at depth causing ascension of volatile-rich basalt magma that mixes with otherwise volatile undersaturated shallow magma to trigger explosive eruption. (D) Explosive or caldera-formning eruptions weaken edifice flanks resulting in subaerial stages of multi-stage failure, containing volcanic debris from explosive eruptions.

Volcanic island flank collapses can also produce destructive tsunamis7,13,37,56,57,59. This and other Canary Island flank collapses were multistage, dividing the landslide mass among numerous staggered failures, resulting in reduced tsunami wave amplitudes compared to equivalent single-block subaerial failures, because the volume is the primary control on tsunami amplitude12,13,38,58. Modelling of landslide-tsunamis suggest that time lags of at least greater than 20–50 seconds between successive stages of collapse removes effects of wave inference that would otherwise cause increased tsunami wave amplitudes12,13,60,61,62,63,64. Our study suggests that time lags on the order of days likely exist between the individual stages of last three significant failures from the northern flank of Tenerife, and as a result the tsunami waves were likely discrete without interference and thus had lower comparative amplitudes60,61,62,63,64.

Methods and Data

The sediment piston cores of this study form a component of previous published research and an established basin stratigraphy7,8,65. Examples of the biostratigraphy and hemipelagite lithostratigraphy of these are included in supplement 1. Coccolith biostratigraphy provided a series of datum horizons7. Species were counted using a Hitachi TM1000 SEM at the British Ocean Sediment Core Research Facility (BOSCORF) and the methodology of Hunt et al.7. Counts were completed at five centimetre intervals and above and below turbidites or changes in hemipelagite lithology.

Volcanic glasses from the individual sub-units of the event beds was completed using the SwiftEd EDS as part of the Hitachi TM1000 SEM at BOSCORF and the methodology of Hunt et al.38 (Supplementary 2). Samples from each sub-unit were sieved at 63 μm and subjected to acetic acid (0.1 M) leaching to remove carbonate. For the Icod slide sub-units were sampled from core D11813 and included 283 new analyses across all sub-units. The Orotava slide sub-units were sampled from core D18813 with 150 new analyses, the Roques de Garcia slide sub-units were sampled from core D11814 with 42 new analyses, and the Cumbre Nueva slide sub-units were sampled from core D11818 with 28 new analyses. Grains were mounted on semi-conductor pads and 30–50 volcanic glasses 90–125 μm and >45 μm thick were analysed for 120 s at 15 kV. Samples were recovered from the El Abrigo and Granadilla ignimbrites on Tenerife and analysed using the SwiftEd EDS as part of the Hitachi TM1000 SEM at BOSCORF and the methodology of Hunt et al.38 (Supplementary 3). These data were validated for accuracy and precision using a series of international standard reference materials (SRMs) as analytical glasses, produced using methodology of Hunt et al.38 (Supplementary 4). Concentrations between 1 and 2 wt% had precisions of 5.0–10.2% of the value, concentrations between 2 and 10 wt% had precisions of 1.0–7.5%, while those values >10 wt% had precisions within <1.5% of the value. Accuracies of SEM EDS results compared to certificated data were generally within 0.3–10.0% of the SRM certified value for values >1 wt%. Specifically, SiO2 that ranged from 45.35 to 53.41 wt% among SRMs had accuracies to within 0.3–3.7% of the certified value. For Na2O that ranged from 1.13 to 3.64 wt% among SRMs had accuracies to within 5.8% of the certified value. Values of K2O among the SRMs only ranged from 0.25 to 2.60 wt%, including three SRMs <0.35 wt%, and had precisions on average within 7.2% of the certified value. Generally, values of Na2O and K2O within volcanic glasses analysed were >2.5 wt% and >4.0 wt%, respectively and thus yielded both improved precision and accuracy.

Data availability statement

All geochemical data pertaining to the compositions of volcanic glasses from each of the landslide sub-units and their associated caldera-forming eruptions is supplied within the supplementary data. Any addition data can be made available upon request of the lead author.

Additional information

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The authors would like to acknowledge the support of the NERC British Ocean Sediment Core Research Facility (BOSCORF) during the collection of data from sediment cores collected during previous NERC-funded research cruises. The lead author would like to acknowledge support from the EU FP7 ASTARTE project and NERC NC funding. The authors would also like to acknowledge the input from reviewer Joan Marti and an anonymous reviewer; their comments and suggestions have made this a much stronger article and their comprehensive reviews were very much appreciated.

Author information


  1. National Oceanography Centre, Southampton, European Way, Southampton, SO143ZH, UK

    • James E. Hunt
  2. Department of Earth Sciences, University of Oxford, South Parks Road, Oxford, OX13AN, UK

    • Michael Cassidy
  3. Departments of Earth Sciences and Geography, Durham University, Durham, DH1 3LE, UK

    • Peter J. Talling


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James Hunt – lead author developed the science concepts, wrote and edited the manuscript, collected all sedimentological data and collected and processed all geochemical data. Michael Cassidy – co-author assisted in editing the manuscript, gathered the ignimbrite samples from Tenerife and assisted editing the manuscript. Peter Talling – co-author assisted in development of science concepts and editing of the manuscript.

Competing Interests

The authors declare that they have no competing interests.

Corresponding author

Correspondence to James E. Hunt.

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