期刊
JOURNAL OF VOLCANOLOGY AND GEOTHERMAL RESEARCH
卷 118, 期 1-2, 页码 173-203出版社
ELSEVIER
DOI: 10.1016/S0377-0273(02)00256-1
关键词
volcanology; stratigraphy; ignimbrite facies; emplacement processes; Colli Albani (Alban Hills) volcano; Italy
The Villa Senni Eruption Unit (VSEU) represents the last large explosive event of the Tuscolano-Artemisio phase of volcanic activity in the Colli Albani (C.A.) (Alban Hills) Volcanic District, situated about 25 km south east of Rome, Italy. The VSEU succession consists of pyroelastic fallout, density current deposits, covering an area of 1500 km(2), reaching a distance of 35 km or more from vent, and having a volume of 30 km(3) DRE. The VSEU is unusual in that its juvenile products are K-foiditic and phono-tephritic in composition, with less than 50% SiO2 content. The most important products of the VSEU eruption are two pyroelastic density current depositional units the Tufo Lionato (TL) and Pozzolanelle (TP), with each deposit containing several recognisable internal facies types. A short time gap (hours to days) between the deposition of these two,ignimbrites is inferred due to the lack of a palaeosoil or evidence of fluvial reworking at the contact between the two units. A new stratigraphic framework for the VSEU is presented based on field observations, component analyses and detailed lateral correlations, with several new stratigraphic subdivisions proposed. The eruptive sequence is subdivided into depositional facies types, each related to a discrete phase of eruption, and a reconstruction of the three-dimensional geometry and the internal facies association within the VSEU is presented. This reconstruction is used to assess the pyroelastic density current emplacement processes resulting from this ignimbrite forming explosive mafic eruption. The morphology of and internal structures preserved within the mafic VSEU are comparable to those seen in more silicic ignimbrite sequences, suggesting that similar processes of emplacement by pyroelastic density currents can be applied over the entire compositional spectrum. We interpret lateral and vertical facies changes in the VSEU ignimbrite deposits to be caused by changes in the palaeotopographic surface over which the depositing pyroelastic density currents were travelling, as well as spatial and temporal changes in the dynamics of the pyroelastic density currents responsible for their deposition. In particular, interaction between the emplacing pyroelastic density current and the underlying palaeotopography caused local changes in current dynamics, leading to a wide range of localised flow structures and internal facies complexity. These interpretations are made possible because the long axes of valleys into which the VSEU was emplaced, which occur as part of the drainage network surrounding the C.A. volcano, are aligned from 0 to 90degrees to the radial pyroclastic current direction. The erosive power of pyroelastic density currents is recorded by an erosive contact between the TL and TP ignimbrites in proximal exposures (< 12 km) to the north west of the C.A. volcano. (C) 2002 Elsevier Science B.V. All rights reserved.
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