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  • Articles  (2)
  • 04. Solid Earth::04.08. Volcanology::04.08.01. Gases  (2)
  • Elsevier  (2)
  • Blackwell Publishing Ltd
  • 2010-2014  (2)
  • 2012  (2)
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  • Articles  (2)
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  • 2010-2014  (2)
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  • 1
    Publication Date: 2017-04-04
    Description: Here we report results from a multidisciplinary field campaign at Villarrica volcano, Chile, in March 2009. A range of direct sampling and remote sensing techniqueswas employed to assess gas and aerosol emissions from the volcano, and extend the time series of measurements that have been made during recent years. Airborne traverses beneath the plume with an ultraviolet spectrometer yielded an average SO2 flux of 3.7 kg s−1. This value is similar to previous measurements made at Villarrica during periods of quiescent activity. The composition of the plume was measured at the crater rim using electrochemical sensors and, for the first time, open-path Fourier transforminfrared spectroscopy, yielding a composition of 90.5 mol% H2O, 5.7% CO2, 2.6%SO2, 0.9% HCl, 0.3% HF and b0.01% H2S. Comparison with previous gas measurements made between 2000 and 2004 shows a correlation between increased SO2/HCl ratios and periods of increased activity. Base-treated filter packs were also employed during our campaign, yielding molar ratios of HBr/SO2=1.1×10−4, HI/SO2=1.4×10−5 and HNO3/SO2=1.1×10−3 in the gas phase. Our data represent the most comprehensive gas inventory at Villarrica to date, and the first evaluation of HBr and HI emissions from a South American volcano. Sun photometry of the plume showed the near-source aerosol size distributions were bimodal with maxima at b0.1 and ~1 μm. These findings are consistent with results from analyses in 2003. Electron microscope analysis of particulatematter collected on filters showed an abundance of sphericalmicron-sized particles that are rich in Si, Mg and Al. Non-spherical, S-rich particles were also observed.
    Description: Antofagasta plc via the University of Cambridge Centre for Latin American Studies, NERC Field Spectroscopy Facility, NERC projectNE/F004222/1, “Volgaspec” projectANR-06-CATT-012-01 and from the NOVAC project. Istituto Nazionale di Geofisica e Vulcanologia and Dipartimento di Protezione Civile-Regione Sicilia. Christ's College, University of Cambridge, NERC IKIMP project, (NE/G001219/1) and NERC grantNE/G01700X/1 for financial support. NERC National Centre for EarthObservation (“Dynamic Earth and geohazards”)
    Description: Published
    Description: 62-75
    Description: 1.2. TTC - Sorveglianza geochimica delle aree vulcaniche attive
    Description: JCR Journal
    Description: reserved
    Keywords: Villarrica ; FTIR ; SO2 flux ; DOAS ; 04. Solid Earth::04.08. Volcanology::04.08.01. Gases
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
    Location Call Number Expected Availability
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  • 2
    Publication Date: 2017-04-04
    Description: Infrared satellite images measured with the MODIS instrument of the volcanic plume produced during the 2006 eruption of Mt. Etna were analysed to produce maps of SO2 amount. We used these maps to reconstruct time series of SO2 fluxes by integrating profiles of SO2 orthogonal to the plume advection direction and multiplying with wind speeds from a meteorological model. These data were then compared with a reconstructed time series of SO2 fluxes measured with the FLAME ground-based network of ultraviolet DOAS systems surrounding the volcano. We found weak agreement on 3rd December when little ash was emitted, but this agreement improved when a 0.3 m s−1 wind speed correction factor was used. FLAME and MODIS results were in good agreement on the 6th December, and improved when a –0.3 m s−1 offset was applied. The corrected data revealed that the only period of time when FLAME and MODIS did not track together was coincident with the presence of ash, which interferes with the IR imagery and retrieval of SO2. We highlight that combining two independent time series of SO2 flux allows a precise determination of wind speed, if there is sufficient time-dependent structure in the SO2 signal. The observed increase in SO2 flux prior to the ash emission is interpreted as a quiescent release of an accumulated gas phase that drive eruptive activity, as previously suggested for the southeast crater system of Etna. In this case the SO2 flux signal therefore acted as a precursor to the eruptive ash events. This work demonstrates that quantitative reconstruction of SO2 flux time series is feasible using MODIS data, opening a new frontier in the use of satellite data to interpret volcanic processes, in particular in poorly monitored remote locations.
    Description: European Space Agency's Earth Observation Envelope Programme (EOEP) – Data User Element (project SAVAA).
    Description: Published
    Description: 80-87
    Description: 1.2. TTC - Sorveglianza geochimica delle aree vulcaniche attive
    Description: JCR Journal
    Description: reserved
    Keywords: SO2 flux ; Modis ; Etna ; 04. Solid Earth::04.08. Volcanology::04.08.01. Gases
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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