First Results of the Piton De La Fournaise STRAP 2015 Experiment: Multidisciplinary Tracking of a Volcanic Gas and Aerosol Plume
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"THE POSSIBLES WE DARE": ART AND IDENTITY IN THE POETRY OF THEODORE ROETHKE Item Type text; Dissertation-Reproduction (electronic) Authors Maselli, Sharon Ann Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 04/10/2021 14:20:34 Link to Item http://hdl.handle.net/10150/290470 INFORMATION TO USERS This material was produced from a microfilm copy of the original document. While the most advanced technological means to photograph and reproduce this document have been used, the quality is heavily dependent upon the quality of the original submitted. The following explanation of techniques is provided to help you understand markings or patterns which may appear on this reproduction. 1.The sign or "target" for pages apparently lacking from the document photographed is "Missing Page(s)". If it was possible to obtain the missing page(s) or section, they are spliced into the film along with adjacent pages. This may have necessitated cutting thru an image and duplicating adjacent pages to insure you complete continuity. 2. When an image on the film is obliterated with a large round black mark, it is an indication that the photographer suspected that the copy may have moved during exposure and thus cause a blurred image. You will find a good image of the page in the adjacent frame. 3. When a map, drawing or chart, etc., was part of the material being photographed the photographer followed a definite method in "sectioning" the material. -
The Fumarolic CO Output from Pico Do Fogo Volcano
Ital. J. Geosci., Vol. 139, No. 3 (2020), pp. 325-340, 9 figs., 3 tabs. (https://doi.org/10.3301/IJG.2020.03) © Società Geologica Italiana, Roma 2020 The fumarolic CO2 output from Pico do Fogo Volcano (Cape Verde) ALESSANDRO AIUPPA (1), MARCELLO BITETTO (1), ANDREA L. RIZZO (2), FATIMA VIVEIROS (3), PATRICK ALLARD (4), MARIA LUCE FREZZOTTI (5), VIRGINIA VALENTI (5) & VITTORIO ZANON (3, 4) ABSTRACT output started early back in the 1990s (e.g., GERLACH, 1991), The Pico do Fogo volcano, in the Cape Verde Archipelago off substantial budget refinements have only recently arisen the western coasts of Africa, has been the most active volcano in the from the 8-years (2011-2019) DECADE (Deep Earth Carbon Macaronesia region in the Central Atlantic, with at least 27 eruptions Degassing; https://deepcarboncycle.org/about-decade) during the last 500 years. Between eruptions fumarolic activity has research program of the Deep Carbon Observatory (https:// been persisting in its summit crater, but limited information exists for the chemistry and output of these gas emissions. Here, we use the deepcarbon.net/project/decade#Overview) (FISCHER, 2013; results acquired during a field survey in February 2019 to quantify FISCHER et alii, 2019). the quiescent summit fumaroles’ volatile output for the first time. By One key result of DECADE-funded research has been combining measurements of the fumarole compositions (using both a the recognition that the global CO2 output from subaerial portable Multi-GAS and direct sampling of the hottest fumarole) and volcanism is predominantly sourced from a relatively of the SO2 flux (using near-vent UV Camera recording), we quantify small number of strongly degassing volcanoes. -
ASAR Interferometry at Piton De La Fournaise, Preliminary Results
ASAR Interferometry at Piton de la Fournaise, preliminary results FROGER Jean-Luc1, FUKUSHIMA Yo2, BRIOLE Pierre3, STAUDACHER Thomas4, SOURIOT Thierry2, VILLENEUVE Nicolas5, CHEMINEE Jean-Louis3 1 : Institut de Recherche pour le Développement (IRD) UR31 "Processus et Aléas Volcaniques", LMV, UBP - UMR 6524. 5, rue Kessler, 63 038 Clermont-Ferrand, FRANCE 2 : Laboratoire Magmas et Volcans, Université Blaise Pascal - UMR 6524. 5, rue Kessler, 63 038 Clermont- Ferrand, FRANCE 3: CNRS-UMR 7580, Institut de Physique du Globe de Paris, 4 Place Jussieu, Paris 75005, FRANCE 4: Observatoire Volcanologique du Piton de la Fournaise, Institut de Physique du Globe de Paris, 14 RN3, le 27ème, 97418 La Plaine des Cafres, LA REUNION 5: Université de la Réunion, 15, avenue René Cassin, BP 7151 97715 Saint-Denis, messag cedex 9, LA REUNION Since the detection of surface deformation at Mount Etna, several geodetic studies have been performed on volcanoes with radar interferometric data acquired by the European ERS-1 and ERS-2 satellites, the Japanese JERS-1 satellite and the Canadian RADARSAT-1 satellite. Here we present the preliminary results of an interferometric study of Piton de la Fournaise volcano, Réunion Island, with Synthetic Aperture Radar images acquired by the ASAR- ENVISAT satellite. Launched in March 2002 by the European Space Agency, ENVISAT is an Earth observation dedicated satellite and its payload consists of a set of instruments for measuring the atmosphere and the surface through the atmosphere. One of these instruments is the ASAR radar designed to provide for continuity of the observations started with the SAR on board of the ERS satellites. -
Magma Fragmentation and Particle Size Distributions in Low Intensity Mafc Explosions: the July/August 2015 Piton De La Fournaise Eruption Matthew J
www.nature.com/scientificreports OPEN Magma fragmentation and particle size distributions in low intensity mafc explosions: the July/August 2015 Piton de la Fournaise eruption Matthew J. Edwards1*, Laura Pioli2*, Andrew J. L. Harris3, Lucia Gurioli3 & Simon Thivet3 Understanding magma fragmentation mechanisms in explosive eruptions is a key requirement for volcanic hazard assessment, eruption management and risk mitigation. This paper focuses on a type case small explosivity eruption (July–August 2015 eruption of Piton de la Fournaise). These eruptions, despite being often overlooked, are exceedingly frequent on local-to-global scales and constitute a signifcant hazard in vent-proximal areas, which are often populated by guides, tourists and, indeed, volcanologists due to their accessibility. The explosions presented here are ideal cases for the study of the dynamics of magma fragmentation and how it relates to the size distribution of scoria generated at the vent. We documented these events visually and thermally, and characterised the products through sample-return. This allowed us to describe small-scale gas bursts sending ejecta up to 30 m during intermittent lava fountains. Surface tension instabilities and inertial forces played a major role in fragmentation processes and generated particles with coarse-skewed distributions and median diameters ranging from − 8 to − 10 . However, with time distributions of particles in the most energetic fountains shifted towards more symmetricalϕ shapes as median grains sizes became fner. Analyses of sequences of images demonstrate that the evolution of particle size distributions with time is due to instability of magma droplets and (in-fight) fragmentation. Mafc explosive volcanism is traditionally overlooked with respect to more energetic, higher intensity and destructive silicic volcanism. -
Picturing France
Picturing France Classroom Guide VISUAL ARTS PHOTOGRAPHY ORIENTATION ART APPRECIATION STUDIO Traveling around France SOCIAL STUDIES Seeing Time and Pl ace Introduction to Color CULTURE / HISTORY PARIS GEOGRAPHY PaintingStyles GOVERNMENT / CIVICS Paris by Night Private Inve stigation LITERATURELANGUAGE / CRITICISM ARTS Casual and Formal Composition Modernizing Paris SPEAKING / WRITING Department Stores FRENCH LANGUAGE Haute Couture FONTAINEBLEAU Focus and Mo vement Painters, Politics, an d Parks MUSIC / DANCENATURAL / DRAMA SCIENCE I y Fontainebleau MATH Into the Forest ATreebyAnyOther Nam e Photograph or Painting, M. Pa scal? ÎLE-DE-FRANCE A Fore st Outing Think L ike a Salon Juror Form Your Own Ava nt-Garde The Flo ating Studio AUVERGNE/ On the River FRANCHE-COMTÉ Stream of Con sciousness Cheese! Mountains of Fra nce Volcanoes in France? NORMANDY “I Cannot Pain tan Angel” Writing en Plein Air Culture Clash Do-It-Yourself Pointillist Painting BRITTANY Comparing Two Studie s Wish You W ere Here Synthétisme Creating a Moo d Celtic Culture PROVENCE Dressing the Part Regional Still Life Color and Emo tion Expressive Marks Color Collectio n Japanese Prin ts Legend o f the Château Noir The Mistral REVIEW Winds Worldwide Poster Puzzle Travelby Clue Picturing France Classroom Guide NATIONAL GALLERY OF ART, WASHINGTON page ii This Classroom Guide is a component of the Picturing France teaching packet. © 2008 Board of Trustees of the National Gallery of Art, Washington Prepared by the Division of Education, with contributions by Robyn Asleson, Elsa Bénard, Carla Brenner, Sarah Diallo, Rachel Goldberg, Leo Kasun, Amy Lewis, Donna Mann, Marjorie McMahon, Lisa Meyerowitz, Barbara Moore, Rachel Richards, Jennifer Riddell, and Paige Simpson. -
Pitons, Cirques and Remparts of Reunion Island
EUROPE / NORTH AMERICA PITONS, CIRQUES AND REMPARTS OF REUNION ISLAND FRANCE WORLD HERITAGE NOMINATION - IUCN TECHNICAL EVALUATION PITONS, CIRQUES AND REMPARTS OF REUNION ISLAND (FRANCE) - ID Nº 1317 Background note: This nomination was submitted in 2008 for consideration by the World Heritage Committee at its 33rd Session in 2009. Accordingly, IUCN initiated the evaluation of this nomination in 2008/9 and this included the evaluation mission to La Réunion. In March 2009, the decision was taken by the government of France to postpone the assessment of the nomination by UNESCO’s World Heritage Committee until its 34th Session in 2010. This decision was required due to the fact that three nominations from France were proposed for consideration by the 33rd Session of the World Heritage Committee. The State Party of France had been requested by the UNESCO World Heritage Centre to identify two nominations in line with the limits on annual numbers of nominations set in the Operational Guidelines. As the evaluation process was already initiated by IUCN, a dialogue was maintained with the State Party to clarify a number of issues and address recommendations resulting from the evaluation mission, and discussions from the 2008 session of the IUCN/World Heritage Panel. This evaluation report is therefore based on the original nomination plus the additional information provided by the State Party. 1. DOCUMENTATION i) Date nomination received by IUCN: 31st January 2008 ii) Additional information offi cially requested from and provided by the State Party: additional information was requested by IUCN in December 2008. Additional information from the State Party was provided in February 2009 and November 2009. -
GREAT Day 2007 Program
Welcome to SUNY Geneseo’s First Annual G.R.E.A.T. Day! Geneseo Recognizing Excellence, Achievement & Talent Day is a college-wide symposium celebrating the creative and scholarly endeavors of our students. In addition to recognizing the achievements of our students, the purpose of G.R.E.A.T. Day is to help foster academic excellence, encourage professional development, and build connections within the community. The G.R.E.A.T. Day Planning Committee: Doug Anderson, School of the Arts Anne Baldwin, Sponsored Research Joan Ballard, Department of Psychology Anne Eisenberg, Department of Sociology Charlie Freeman, Department of Physics & Astronomy Tom Greenfield, Department of English Anthony Gu, School of Business Koomi Kim, School of Education Andrea Klein, Scheduling and Special Events The Planning Committee would like to thank: Stacie Anekstein, Ed Antkoviak, Brian Bennett, Cassie Brown, Michael Caputo, Sue Chichester, Betsy Colon, Laura Cook, Ann Crandall, Joe Dolce, Tammy Farrell, Carlo Filice, Richard Finkelstein, Karie Frisiras, Ginny Geer-Mentry, Becky Glass, Dave Gordon, Corey Ha, John Haley, Doug Harke, Gregg Hartvigsen, Tony Hoppa, Paul Jackson, Ellen Kintz, Nancy Johncox, Enrico Johnson, Ken Kallio, Jo Kirk, Sue Mallaber, Mary McCrank, Nancy Newcomb, Elizabeth Otero, Tracy Paradis, Jennifer Perry, Jewel Reardon, Ed Rivenburgh, Linda Shepard, Bonnie Swoger, Helen Thomas, Pam Thomas, and Taryn Thompson. Thank you to President Christopher Dahl and Provost Katherine Conway-Turner for their support of G.R.E.A.T. Day. Thank you to Lynn Weber for delivering our inaugural keynote address. The G.R.E.A.T. Day name was suggested by Elizabeth Otero, a senior Philosophy major. -
The Tennessee Meteorite Impact Sites and Changing Perspectives on Impact Cratering
UNIVERSITY OF SOUTHERN QUEENSLAND THE TENNESSEE METEORITE IMPACT SITES AND CHANGING PERSPECTIVES ON IMPACT CRATERING A dissertation submitted by Janaruth Harling Ford B.A. Cum Laude (Vanderbilt University), M. Astron. (University of Western Sydney) For the award of Doctor of Philosophy 2015 ABSTRACT Terrestrial impact structures offer astronomers and geologists opportunities to study the impact cratering process. Tennessee has four structures of interest. Information gained over the last century and a half concerning these sites is scattered throughout astronomical, geological and other specialized scientific journals, books, and literature, some of which are elusive. Gathering and compiling this widely- spread information into one historical document benefits the scientific community in general. The Wells Creek Structure is a proven impact site, and has been referred to as the ‘syntype’ cryptoexplosion structure for the United State. It was the first impact structure in the United States in which shatter cones were identified and was probably the subject of the first detailed geological report on a cryptoexplosive structure in the United States. The Wells Creek Structure displays bilateral symmetry, and three smaller ‘craters’ lie to the north of the main Wells Creek structure along its axis of symmetry. The question remains as to whether or not these structures have a common origin with the Wells Creek structure. The Flynn Creek Structure, another proven impact site, was first mentioned as a site of disturbance in Safford’s 1869 report on the geology of Tennessee. It has been noted as the terrestrial feature that bears the closest resemblance to a typical lunar crater, even though it is the probable result of a shallow marine impact. -
Large Impact Basins on Mercury: Global Distribution, Characteristics, and Modification History from MESSENGER Orbital Data Caleb I
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, E00L08, doi:10.1029/2012JE004154, 2012 Large impact basins on Mercury: Global distribution, characteristics, and modification history from MESSENGER orbital data Caleb I. Fassett,1 James W. Head,2 David M. H. Baker,2 Maria T. Zuber,3 David E. Smith,3,4 Gregory A. Neumann,4 Sean C. Solomon,5,6 Christian Klimczak,5 Robert G. Strom,7 Clark R. Chapman,8 Louise M. Prockter,9 Roger J. Phillips,8 Jürgen Oberst,10 and Frank Preusker10 Received 6 June 2012; revised 31 August 2012; accepted 5 September 2012; published 27 October 2012. [1] The formation of large impact basins (diameter D ≥ 300 km) was an important process in the early geological evolution of Mercury and influenced the planet’s topography, stratigraphy, and crustal structure. We catalog and characterize this basin population on Mercury from global observations by the MESSENGER spacecraft, and we use the new data to evaluate basins suggested on the basis of the Mariner 10 flybys. Forty-six certain or probable impact basins are recognized; a few additional basins that may have been degraded to the point of ambiguity are plausible on the basis of new data but are classified as uncertain. The spatial density of large basins (D ≥ 500 km) on Mercury is lower than that on the Moon. Morphological characteristics of basins on Mercury suggest that on average they are more degraded than lunar basins. These observations are consistent with more efficient modification, degradation, and obliteration of the largest basins on Mercury than on the Moon. This distinction may be a result of differences in the basin formation process (producing fewer rings), relaxation of topography after basin formation (subduing relief), or rates of volcanism (burying basin rings and interiors) during the period of heavy bombardment on Mercury from those on the Moon. -
Complex Structure of Piton De La Fournaise and Its Underlying
1 Complex structure of Piton de la Fournaise and its underlying 2 lithosphere revealed by MT 3D inversion. 3 4 Lydie-Sarah Gailler1, Anna Marti2, Jean-François Lénat1 5 1 Université Clermont Auvergne, Laboratoire Magmas et Volcans - CNRS, UMR 6524, IRD, R 163, 6 6 Avenue Blaise Pascal TSA 60026 – CS 60026, 63178 AUBIERE Cedex, FRANCE 7 2 Departament de Geodinàmica i Geofísica, Universitat de Barcelona, Spain 8 9 Corresponding author: [email protected] 10 Abstract 11 La Réunion is a large volcanic construction resting on Paleocene oceanic crust. Through the 12 3D inversion of a large set of magnetotelluric (MT) soundings, our results reveal the general 13 resistivity structure of the western part of Piton de la Fournaise volcano down to its base and 14 the first ten kilometers or so of the underlying lithosphere. The upper resistive layer is 15 associated to a superimposition of unsaturated and probably water-saturated lava flows with 16 an averaged thickness of 1.5 km overlying more or less continuous highly conductive patches 17 which imply the presence of highly conductive fluids and/or minerals. In the summit area and 18 Enclos, this conductor is unambiguously attributed to the presently active hydrothermal 19 system. In the Plaine des Sables, it is tentatively associated with the hydrothermal alteration 20 beneath the ancient volcanic center. A third widespread conductive patch is observed below 21 the NW flank of Piton de la Fournaise resulting more likely from volcanic activity since it 22 coincides with part of the N120 rift zone. In the area beneath the Plaine des Sables where a 23 dense intrusive complex has been inferred from gravity models, the resistivity is not 24 significantly higher. -
The 2007 Caldera Collapse of Piton De La Fournaise Volcano: Source Process from Very-Long-Period Seismic Signals Zacharie Duputel, Luis Rivera
The 2007 caldera collapse of Piton de la Fournaise volcano: Source process from very-long-period seismic signals Zacharie Duputel, Luis Rivera To cite this version: Zacharie Duputel, Luis Rivera. The 2007 caldera collapse of Piton de la Fournaise volcano: Source process from very-long-period seismic signals. Earth and Planetary Science Letters, Elsevier, 2019, 527 (10), pp.115786. 10.1016/j.epsl.2019.115786. hal-02324812 HAL Id: hal-02324812 https://hal.archives-ouvertes.fr/hal-02324812 Submitted on 28 Aug 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution| 4.0 International License Earth and Planetary Science Letters 527 (2019) 115786 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl The 2007 caldera collapse of Piton de la Fournaise volcano: Source process from very-long-period seismic signals ∗ Zacharie Duputel , Luis Rivera Institut de Physique du Globe de Strasbourg, UMR7516, Université de Strasbourg/EOST, CNRS, Strasbourg, France a r t i c l e i n f o a b s t r a c t Article history: In April 2007, Piton de la Fournaise volcano experienced its largest caldera collapse in at least 300 yr. -
Mercury Emissions from Soils and Fumaroles of Nea Kameni Volcanic Centre, Santorini (Greece)
Geochemical Journal, Vol. 47, pp. 437 to 450, 2013 Mercury emissions from soils and fumaroles of Nea Kameni volcanic centre, Santorini (Greece) EMANUELA BAGNATO,1* GIANCARLO TAMBURELLO,1 ALESSANDRO AIUPPA,1,2 MARIO SPROVIERI,3 GEORGE E. VOUGIOUKALAKIS4 and MICHELLE PARKS5 1DiSTeM, University of Palermo, Via Archirafi 36, Palermo, Italy 2Istituto di Geofisica e Vulcanologia, Via U. La Malfa 153, Palermo, Italy 3IAMC-CNR, Via del Mare 3, Torretta Granitola, Fraz. Campobello di Mazzara (TP), Italy 4Institute for Geology and Mineral Exploration, 3rd exit Olympic village, 13677, Aharne, Athene, Greece 5Department of Earth Sciences, University of Oxford, South Parks Road, Oxford OX1 3AN, U.K. (Received August 21, 2012; Accepted May 13, 2013) There have been limited studies to date targeting mercury emissions from volcanic fumarolic systems, and no mercury flux data exist for soil or fumarolic emissions at Santorini volcanic complex, Greece. We present results from the first geochemical survey of Hg and major volatile (CO2, H2S, H2O and H2) concentrations and fluxes in the fumarolic gases released by the volcanic/hydrothermal system of Nea Kameni islet; the active volcanic center of Santorini. These data were obtained using a portable mercury spectrometer (Lumex 915+) for gaseous elemental mercury (GEM) determina- tion, and a Multi-component Gas Analyzer System (Multi-GAS) for major volatiles. Gaseous Elemental Mercury (GEM) concentrations in the fumarole atmospheric plumes were systematically above background levels (~4 ng GEM m–3), rang- ing from ~4.5 to 121 ng GEM m–3. Variability in the measured mercury concentrations may result from changes in atmos- pheric conditions and/or unsteady gas release from the fumaroles.