2016
DOI: 10.1038/srep21220
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Reconstructing the plinian and co-ignimbrite sources of large volcanic eruptions: A novel approach for the Campanian Ignimbrite

Abstract: The 39 ka Campanian Ignimbrite (CI) super-eruption was the largest volcanic eruption of the past 200 ka in Europe. Tephra deposits indicate two distinct plume forming phases, Plinian and co-ignimbrite, characteristic of many caldera-forming eruptions. Previous numerical studies have characterized the eruption as a single-phase event, potentially leading to inaccurate assessment of eruption dynamics. To reconstruct the volume, intensity, and duration of the tephra dispersal, we applied a computational inversion… Show more

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Cited by 61 publications
(89 citation statements)
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References 58 publications
(122 reference statements)
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“…The CI eruption began with the onset of a sustained plinian plume, up to 39 km high, producing a stratified pumice lapilli fall deposit (5.3 km 3 of tephra) dispersed toward the East (Martì et al, 2016;. The plinian phase was followed by a collapsing column phase (Scarpati et al, 2014) during which an impressive pyroclastic density current was generated, spreading over an area of N30,000 km 2 and managing to surmount mountain ridges up to 1000 m high (Fisher et al, 1993).…”
Section: The Campanian Ignimbrite Eruptionmentioning
confidence: 99%
“…The CI eruption began with the onset of a sustained plinian plume, up to 39 km high, producing a stratified pumice lapilli fall deposit (5.3 km 3 of tephra) dispersed toward the East (Martì et al, 2016;. The plinian phase was followed by a collapsing column phase (Scarpati et al, 2014) during which an impressive pyroclastic density current was generated, spreading over an area of N30,000 km 2 and managing to surmount mountain ridges up to 1000 m high (Fisher et al, 1993).…”
Section: The Campanian Ignimbrite Eruptionmentioning
confidence: 99%
“…Estimations of Mass Eruption Rates (MERs) obtained with different independent methods (Wilson and Walker, 1981;Hildreth and Mahood, 1986;Wilson and Hildreth, 1997;Baines and Sparks, 2005;Costa et al, 2014;Martí et al, 2016;Roche et al, 2016) indicate MERs of the orders 10 9 -10 11 kg/s (e.g., Bishop Tuff, Campanian Ignimbrite, Oruanui eruption, Taupo eruption, Peach Spring Tuff, Young Toba Tuff), implying durations of few to several hours only to evacuate even thousands of km 3 of magma.…”
Section: Introductionmentioning
confidence: 99%
“…Because of this strong dependence, uncertainties within 20 % in the determination of column height can translate into uncertainties up to 70 % for the MER (e.g., Biass and Bonadonna, 2011). Averaged column heights of eruptions that have not been directly observed are typically derived from characteristics of tephra deposits (e.g., Bonadonna and Costa, 2013;Carey and Sparks, 1986;Pyle, 1989) or are derived from model inversion (e.g., Connor and Connor, 2006;Marti et al, 2016;Pfeiffer et al, 2005). The empirical correlations to estimate MER in the model are described in Table 2 and are based either on fitting observations (e.g., Mastin et al, 2009) or more sophisticated fits accounting for wind bent-over effects (e.g., Degruyter …”
Section: Mass Eruption Ratementioning
confidence: 99%