Repository logo
  • English
  • Italiano
Log In
New user? Click here to register.Have you forgotten your password?
  1. Home
  2. Affiliation
  3. INGV
  4. Article published / in press
  5. The Ilopango caldera complex, El Salvador: Stratigraphic revision of the complete eruptive sequence and recurrence of large explosive eruptions
 
  • Details

The Ilopango caldera complex, El Salvador: Stratigraphic revision of the complete eruptive sequence and recurrence of large explosive eruptions

Author(s)
Sunye Puchol, Ivan  
Aguirre-Diaz, Gerardo J.  
Pedrazzi, Dario  
Dávila Harris, Pablo  
Miggins, Daniel P.  
Costa, Antonio  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia  
Ortega-Obregón, Carlos  
Lacan, Pierre  
Gutierrez, Eduardo  
Hernández, Walter  
Language
English
Obiettivo Specifico
1V. Storia eruttiva
Status
Published
JCR Journal
JCR Journal
Journal
Journal of Volcanology and Geothermal Research  
Issue/vol(year)
/374 (2019)
ISSN
0377-0273
Pages (printed)
100-119
Date Issued
2019
DOI
10.1016/j.jvolgeores.2019.02.011
URI
https://www.earth-prints.org/handle/2122/13519
Subjects
04.08. Volcanology  
Subjects

Stratigraphy of volca...

Ignimbrite

Central America Volca...

Pull-apart graben

Abstract
Ilopango caldera erupted episodically at least 13 tuff-forming eruptions with a minimum estimate volume of 1–5km3 DRE per eruption, reaching up to 150km3 DRE for the first caldera-forming eruption. All tuffs are of dacitic-rhyolitic composition. The complete pyroclastic sequence spans a range in time from 1.785 to 0.0015 Ma, and based on stratigraphy and geochronology constraints can be divided into three formations: the Comalapa, Altavista and Tierras Blancas formations. In this work, we focus on the members of the newly described Altavista Formation (middle part of Ilopango caldera volcanic sequence), which consist of six con- solidated pyroclastic deposits or tuffs. Each tuff corresponds to a specific eruption followed by a period of quiescence during which soil beds were developed on the deposits. The ages of the Altavista Formation ranges from 918 to 257ka, based on new 40Ar/39Ar, U/Pb-zircon, and U/Th-zircon analyses. The tuffs of this for- mation show similar characteristics in mineralogy and composition. They are calcalkaline, rhyodacitic tuffs, with plagioclase, clinopyroxene, and hornblende. From field mapping and descriptions of the deposits, we have inferred the eruptive styles that include pumice fallouts, pyroclastic density currents and also hydromag- matic explosions. The common vent in all tuffs was the Ilopango caldera and each member of the Altavista Formation could correspond to a caldera collapse event, except for one of the six eruptions. The volume of each member was estimated to be >30km3 DRE, which is the same order of magnitude than that estimated for the Tierra Blanca Joven (TBJ) eruption at about 1500 B. P, and smaller than those of the ignimbrites of the Comalapa Formation, the first three members of the Ilopango caldera reported previously. The tuffs of the Altavista Formation are visible up to 15–20 km away from the caldera's topographic margin. The recurrence interval of large explosive events at the Ilopango caldera was established by integrating the stratigraphic and geochronologic data of all 13 ignimbrites and pumice fallouts erupted from Ilopango caldera since the first one at 1.78 Ma to the last explosive event (TBJ).
Type
article
File(s)
Loading...
Thumbnail Image
Name

sunagu2019b.pdf

Size

16.61 MB

Format

Adobe PDF

Checksum (MD5)

04254cc06c2f6a71dd73502878cfdb22

rome library|catania library|milano library|napoli library|pisa library|palermo library
Explore By
  • Research Outputs
  • Researchers
  • Organizations
Info
  • Earth-Prints Open Archive Brochure
  • Earth-Prints Archive Policy
  • Why should you use Earth-prints?
Earth-prints working group
⚬Anna Grazia Chiodetti (Project Leader)
⚬Gabriele Ferrara (Technical and Editorial Assistant)
⚬Massimiliano Cascone
⚬Francesca Leone
⚬Salvatore Barba
⚬Emmanuel Baroux
⚬Roberto Basili
⚬Paolo Marco De Martini

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback