Causes of complexity in a fallout dominated plinian eruption sequence: 312 ka Fasnia Member, Diego Hernández Formation, Tenerife, Spain
Introduction
Plinian eruption sequences have long been depicted as a progression from an initial, sustained buoyant eruption column phase producing fallout deposits to a column collapse phase producing pyroclastic flows (e.g. Sparks et al., 1973; 0.57 Ma Granadilla Member, Tenerife, Bryan et al., 2000; 184 ka and 172 ka Lower Pumice 1 and 2 eruption sequences, Santorini, Gertisser et al., 2009, Simmons et al., 2016, Simmons et al., 2017a, Simmons et al., 2017b). However, many plinian eruptions are more complex and are characterised by one or more intra-plinian partial collapses of the eruption column, and involving varying degrees of phreatic/phreatomagmatic explosive activity, before a final column collapse. Such sequences are represented by interstratified pumice fallout, intra-plinian ignimbrites, ash layers and, in most cases, a ‘climactic’ ignimbrite which caps the sequence (e.g. 0.28 Ma Poris eruption, Tenerife, Spain, Edgar et al., 2002, Brown and Branney, 2004; 4.5 ka Fogo A, Azores, Pensa et al., 2015; Vesuvius 79 CE, Sigurdsson et al., 1985, Cioni et al., 1992a, Cioni et al., 1999, Gurioli et al., 2005, Shea et al., 2012; 1600 CE Huaynaputina eruption, Peru, Adams et al., 2001, Thouret et al., 2002; the 1912 Novarupta-Katmai eruption, Houghton et al., 2004, Hildreth and Fierstein, 2012; 1991 Pinatubo eruption, Philippines, Rosi et al., 2001). Some plinian sequences are also marked by voluminous lithic clast breccias at the interface of pyroclastic fallout and flow deposits or intercalated within an ignimbrite sequence (e.g., Wright and Walker, 1977, Druitt and Sparks, 1982, Druitt, 1985, Bacon, 1983, Walker, 1985, Allen and Cas, 1998, Rosi et al., 2001, Pittari et al., 2008, Bear et al., 2009, Simmons et al., 2016, Simmons et al., 2017a, Simmons et al., 2017b). Such deposits have been used to infer the onset of caldera collapse (e.g. Bacon, 1983, Edgar et al., 2002, Bear et al., 2009, Simmons et al., 2017a, Simmons et al., 2017b).
The volcanic island of Tenerife preserves many phonolitic plinian eruption sequences, some simple (e.g. Bryan et al., 2000), some complex (e.g. Edgar et al., 2002). In this paper, we focus on the most complex and voluminous, the 312 ka Fasnia Member eruption sequence. We present the detailed stratigraphy based on island-wide mapping and correlation, we estimate the volume for each major depositional unit, assess the timing of ignimbrite formation, and discuss the numerous factors that determined eruption processes. This study will enhance understanding of the hazards of complex plinian eruptions on Tenerife and elsewhere.
Section snippets
Geological background
Tenerife is the largest of the Canary Islands, Spain. It emerged as an alkali basaltic shield volcano system ca.12 Myr ago (Ancochea et al., 1990; Table 1), producing thick, mostly mafic lava sequences that are now exposed in three heavily dissected massifs (the ‘Old Basaltic Series’ of Fuster et al., 1968; Fig. 1a, Table 1). After 3.8 Ma, a central post-shield stratovolcanic complex, the Las Cañadas Edifice, developed in the centre of the island (Fig. 1a). An extended phase of mafic to felsic
Terminology
Although the umbrella term “pyroclastic density current” (PDC) has been in vogue in recent years for gravity driven hot flows of pyroclastic debris, this term is too non-specific when detailed process interpretation is required of particular deposits. It does not adequately distinguish between the different types of pyroclastic density currents, such as the spectrum of high particle concentration pyroclastic flows (pumice and ash, scoria and ash, block and ash and blast flows) and surges (base
Stratigraphy and facies of the Fasnia Member
The 312 ka Fasnia Member is one of the most widespread units on Tenerife, having originally covered > 80% of the island. It has been subdivided into 22 stratigraphic units based on grain size, sorting, componentry, depositional structures, deposit morphology and regional correlations (Fig. 2, Fig. 3). The main lithofacies are first described and their origins interpreted, and then individual stratigraphic units are discussed and interpreted within the newly established stratigraphy of the Fasnia
Complexity of the Fasnia eruption sequence and eruption column instability
The Fasnia eruption sequence, with 7 main magmatic plinian fallout units, interspersed with 7 main ignimbrite units, and 8 main ash horizons, seems to be at least as complex as other examples listed in the introduction. The complexities reflect partial to total eruption column collapse events, and at least some phreatic/phreatomagmatic/hydrothermal influences. Apart from after the major Ravelo and Atogo Ignimbrite-forming events, there is no evidence to suggest that the eruption column
Conclusions
• The Fasnia eruption sequence is one of the most complex plinian eruption sequences yet recorded, with multiple plinian pumice fallout deposits, which themselves are often internally complex, at least 7 ignimbrites, and multiple ash horizons of both surge and fallout origin.
• The complexity in the eruption sequence reflects an unstable eruption column that was susceptible to numerous, partial, eruption column collapse events generating intra-plinian ignimbrites and surges.
• Much of the
Acknowledgements
Much of this research represents part of the PhD research of Campbell Edgar at Monash University. The research was funded by discretionary research funds of Ray Cas, NSF grant EAR-0001013 to John Wolff, and MCyT REN2001-0502/RIES and EC EVG1-CT-2002-00058 grants to Joan Marti. We thank Peter Larson, Jeff Grandy, Inés Galindo, Nemesio Pérez, Jill Middleton, Keith Brunstad and Janet Sumner for assistance in the field and discussion on aspects of Tenerife geology, and Jesus Garrido and the staff
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