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Dynamic Petrology and Rheology of Ascending Magma During Lava Dome Eruptions: Effusive–Explosive Activity
Dynamic petrology and rheology of ascending magma during lava dome eruptions: Effusive–explosive activity Thesis submitted in accordance with the requirements of the University of Liverpool for the degree of Doctor of Philosophy by Paul Anthony Wallace May 2019 Declaration of authorship I, Paul Anthony Wallace, declare that this thesis entitled “Dynamic petrology and rheology of ascending magma during lava dome eruptions: Effusive–explosive activity” and the work presented in it is my own. I confirm that: This thesis was completed as part of a research degree at the University of Liverpool; The material contained in this thesis has not been presented, nor is currently being presented, either wholly or in parts, for any other degree or qualifications; Where I have consulted published studies, this have been clearly referenced; Where the work was part of a collaborative effort, I have made clear what others have done and what I have contributed myself; Parts of this thesis have been published or in preparation for publication as: o Wallace, P.A., Kendrick, J.E., Ashworth, J.D., Miwa, T., Coats, R., De Angelis, S.H., Mariani, E., Utley, J.E.P., Biggin, A., Kendrick, R., Nakada, S., Matsushima, T., and Lavallée, Y. (published in Journal of Petrology). Petrological architecture of a magmatic shear zone: A multidisciplinary investigation of strain localisation during magma ascent at Unzen Volcano, Japan. o Wallace, P.A., De Angelis, S.H., Hornby, A.J., Kendrick, J.E., von Aulock, F.W., Clesham, S., Hughes, A., Utley, J.E.P., Hirose, T., Dingwell, D.B., and Lavallée, Y. (published in Geochimica et Cosmochimica Acta). -
Pyroclastic Flow Hazards
Pyroclastic Flow Hazards Lecture Objectives -definition and characteristics -generation of pyroclastic flows -impacts and hazards What are pyroclastic flows? Pyroclastic flows are high- density mixtures of hot, dry rock fragments and hot gases that move away from the vent that erupted them at high speeds. Generation Mechanisms: -explosive eruption of molten or solid rock fragments, or both. -non-explosive eruption of lava when parts of dome or a thick lava flow collapses down a steep slope. Most pyroclastic flows consist of two parts: a basal flow of coarse fragments that moves along the ground, and a turbulent cloud of ash that rises above the basal flow. Ash may fall from this cloud over a wide area downwind from the pyroclastic flow. Mt. St. Helens Effects of pyroclastic flows A pyroclastic flow will destroy nearly everything in its path. With rock fragments ranging in size from ash to boulders traveling across the ground at speeds typically greater than 80 km per hour, pyroclastic flows knock down, shatter, bury or carry away nearly all objects and structures in their way. The extreme temperatures of rocks and gas inside pyroclastic flows, generally between 200°C and 700°C, can cause combustible material to burn, especially petroleum products, wood, vegetation, and houses. Pyroclastic flows vary considerably in size and speed, but even relatively small flows that move <5 km from a volcano can destroy buildings, forests, and farmland. On the margins of pyroclastic flows, death and serious injury to people and animals may result from burns and inhalation of hot ash and gases. Pyroclastic flows generally follow valleys or other low-lying areas and, depending on the volume of rock debris carried by the flow, they can deposit layers of loose rock fragments to depths ranging from less than one meter to more than 200 m. -
Iv BOLIVIA the Top of the World
iv BOLIVIA The top of the world Bolivia takes the breath away - with its beauty, its geographic and cultural diversity, and its lack of oxygen. From the air, the city of La Paz is first glimpsed between two snowy Andean mountain ranges on either side of a plain; the spread of the joined-up cities of El Alto and La Paz, cradled in a huge canyon, is an unforgettable sight. For passengers landing at the airport, the thinness of the air induces a mixture of dizziness and euphoria. The city's altitude affects newcomers in strange ways, from a mild headache to an inability to get up from bed; everybody, however, finds walking up stairs a serious challenge. The city's airport, in the heart of El Alto (literally 'the high place'), stands at 4000 metres, not far off the height of the highest peak in Europe, Mont Blanc. The peaks towering in the distance are mostly higher than 5000m, and some exceed 6000m in their eternally white glory. Slicing north-south across Bolivia is a series of climatic zones which range from tropical lowlands to tundra and eternal snows. These ecological niches were exploited for thousands of years, until the Spanish invasion in the early sixteenth century, by indigenous communities whose social structure still prevails in a few ethnic groups today: a single community, linked by marriage and customs, might live in two or more separate climes, often several days' journey away from each other on foot, one in the arid high plateau, the other in a temperate valley. -
The Science Behind Volcanoes
The Science Behind Volcanoes A volcano is an opening, or rupture, in a planet's surface or crust, which allows hot magma, volcanic ash and gases to escape from the magma chamber below the surface. Volcanoes are generally found where tectonic plates are diverging or converging. A mid-oceanic ridge, for example the Mid-Atlantic Ridge, has examples of volcanoes caused by divergent tectonic plates pulling apart; the Pacific Ring of Fire has examples of volcanoes caused by convergent tectonic plates coming together. By contrast, volcanoes are usually not created where two tectonic plates slide past one another. Volcanoes can also form where there is stretching and thinning of the Earth's crust in the interiors of plates, e.g., in the East African Rift, the Wells Gray-Clearwater volcanic field and the Rio Grande Rift in North America. This type of volcanism falls under the umbrella of "Plate hypothesis" volcanism. Volcanism away from plate boundaries has also been explained as mantle plumes. These so- called "hotspots", for example Hawaii, are postulated to arise from upwelling diapirs with magma from the core–mantle boundary, 3,000 km deep in the Earth. Erupting volcanoes can pose many hazards, not only in the immediate vicinity of the eruption. Volcanic ash can be a threat to aircraft, in particular those with jet engines where ash particles can be melted by the high operating temperature. Large eruptions can affect temperature as ash and droplets of sulfuric acid obscure the sun and cool the Earth's lower atmosphere or troposphere; however, they also absorb heat radiated up from the Earth, thereby warming the stratosphere. -
Evaluación Del Riesgo Volcánico En El Sur Del Perú
EVALUACIÓN DEL RIESGO VOLCÁNICO EN EL SUR DEL PERÚ, SITUACIÓN DE LA VIGILANCIA ACTUAL Y REQUERIMIENTOS DE MONITOREO EN EL FUTURO. Informe Técnico: Observatorio Vulcanológico del Sur (OVS)- INSTITUTO GEOFÍSICO DEL PERÚ Observatorio Vulcanológico del Ingemmet (OVI) – INGEMMET Observatorio Geofísico de la Univ. Nacional San Agustín (IG-UNSA) AUTORES: Orlando Macedo, Edu Taipe, José Del Carpio, Javier Ticona, Domingo Ramos, Nino Puma, Víctor Aguilar, Roger Machacca, José Torres, Kevin Cueva, John Cruz, Ivonne Lazarte, Riky Centeno, Rafael Miranda, Yovana Álvarez, Pablo Masias, Javier Vilca, Fredy Apaza, Rolando Chijcheapaza, Javier Calderón, Jesús Cáceres, Jesica Vela. Fecha : Mayo de 2016 Arequipa – Perú Contenido Introducción ...................................................................................................................................... 1 Objetivos ............................................................................................................................................ 3 CAPITULO I ........................................................................................................................................ 4 1. Volcanes Activos en el Sur del Perú ........................................................................................ 4 1.1 Volcán Sabancaya ............................................................................................................. 5 1.2 Misti .................................................................................................................................. -
Volcanic Eruptions
Volcanic Eruptions •Distinguish between nonexplosive and explosive volcanic eruptions. • Identify the features of a volcano. • Explain how the composition of magma affects the type of volcanic eruption that will occur. • Describe four types of lava and four types of pyroclastic material. I. Volcanic Eruptions A. A volcano is a vent or fissure in the Earth’s surface through which molten rock and gases are expelled. B. Molten rock is called magma. C. Magma that flows onto the Earth’s surface is called lava. II. Nonexplosive Eruptions A. Nonexplosive eruptions are the most common type of volcanic eruptions. These eruptions produce relatively calm flows of lava in huge amounts. B. Vast areas of the Earth’s surface, including much of the sea floor and the Northwestern United States, are covered with lava form nonexplosive eruptions. Kilauea Volcano in Hawaii Island III. Explosive Eruptions A. While explosive eruptions are much rarer than non-explosive eruptions, the effects can be incredibly destructive. B. During an explosive eruption, clouds of hot debris, ash, and gas rapidly shoot out from a volcano. C. An explosive eruption can also blast millions of tons of lava and rock from a volcano, and can demolish and entire mountainside. Alaska's Mount Redoubt eruption in March 2009 IV. What Is Inside a Volcano? A. The interior of a volcano is made up of two main features. B. The magma chamber is the body of molten rock deep underground that feeds a volcano. C. The vent is an opening at the surface of the Earth through which volcanic material passes. -
Preliminary Volcano-Hazard Assessment for Augustine Volcano, Alaska
DEPARTMENT OF THE INTERIOR U.S. GEOLOGICAL SURVEY Preliminary Volcano-Hazard Assessment for Augustine Volcano, Alaska by Christopher F. Waythomas and Richard B. Waitt Open-File Report 98-106 This report is preliminary and subject to revision as new data become available. Any use of trade, product or firm names is for descriptive purposes only and does not imply endorsement by the U.S. Geological Survey Alaska Volcano Observatory Anchorage, Alaska 1998 U.S. DEPARTMENT OF THE INTERIOR BRUCE BABBITT, Secretary U.S. GEOLOGICAL SURVEY Thomas J. Casadevall, Acting Director For additional information: Copies of this report may be purchased from: U.S. Geological Survey U.S. Geological Survey Alaska Volcano Observatory Branch of Information Services 4200 University Drive Box 25286 Anchorage, AK 99508 Denver, CO 80225-0286 CONTENTS Summary of hazards at Augustine Volcano....................................... 1 Introduction ............................................................... 3 Purposeandscope ...................................................... 3 Physical setting of Augustine Volcano ...................................... 4 Relation to previous studies on Augustine hazards ............................. 5 Prehistoric eruptive history ................................................... 5 Historical eruptions ......................................................... 8 Hazardous phenomena at Augustine Volcano ..................................... 8 Volcanic hazards ....................................................... 12 Volcanicashclouds -
Explosive Eruptions
Explosive Eruptions -What are considered explosive eruptions? Fire Fountains, Splatter, Eruption Columns, Pyroclastic Flows. Tephra – Any fragment of volcanic rock emitted during an eruption. Ash/Dust (Small) – Small particles of volcanic glass. Lapilli/Cinders (Medium) – Medium sized rocks formed from solidified lava. – Basaltic Cinders (Reticulite(rare) + Scoria) – Volcanic Glass that solidified around gas bubbles. – Accretionary Lapilli – Balls of ash – Intermediate/Felsic Cinders (Pumice) – Low density solidified ‘froth’, floats on water. Blocks (large) – Pre-existing rock blown apart by eruption. Bombs (large) – Solidified in air, before hitting ground Fire Fountaining – Gas-rich lava splatters, and then flows down slope. – Produces Cinder Cones + Splatter Cones – Cinder Cone – Often composed of scoria, and horseshoe shaped. – Splatter Cone – Lava less gassy, shape reflects that formed by splatter. Hydrovolcanic – Erupting underwater (Ocean or Ground) near the surface, causes violent eruption. Marr – Depression caused by steam eruption with little magma material. Tuff Ring – Type of Marr with tephra around depression. Intermediate Magmas/Lavas Stratovolcanoes/Composite Cone – 1-3 eruption types (A single eruption may include any or all 3) 1. Eruption Column – Ash cloud rises into the atmosphere. 2. Pyroclastic Flows Direct Blast + Landsides Ash Cloud – Once it reaches neutral buoyancy level, characteristic ‘umbrella cap’ forms, & debris fall. Larger ash is deposited closer to the volcano, fine particles are carried further. Pyroclastic Flow – Mixture of hot gas and ash to dense to rise (moves very quickly). – Dense flows restricted to valley bottoms, less dense flows may rise over ridges. Steam Eruptions – Small (relative) steam eruptions may occur up to a year before major eruption event. . -
Vegetation and Climate Change on the Bolivian Altiplano Between 108,000 and 18,000 Years Ago
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by DigitalCommons@University of Nebraska University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Earth and Atmospheric Sciences, Department Papers in the Earth and Atmospheric Sciences of 1-1-2005 Vegetation and climate change on the Bolivian Altiplano between 108,000 and 18,000 years ago Alex Chepstow-Lusty Florida Institute of Technology, [email protected] Mark B. Bush Florida Institute of Technology Michael R. Frogley Florida Institute of Technology, 150 West University Boulevard, Melbourne, FL Paul A. Baker Duke University, [email protected] Sherilyn C. Fritz University of Nebraska-Lincoln, [email protected] See next page for additional authors Follow this and additional works at: https://digitalcommons.unl.edu/geosciencefacpub Part of the Earth Sciences Commons Chepstow-Lusty, Alex; Bush, Mark B.; Frogley, Michael R.; Baker, Paul A.; Fritz, Sherilyn C.; and Aronson, James, "Vegetation and climate change on the Bolivian Altiplano between 108,000 and 18,000 years ago" (2005). Papers in the Earth and Atmospheric Sciences. 30. https://digitalcommons.unl.edu/geosciencefacpub/30 This Article is brought to you for free and open access by the Earth and Atmospheric Sciences, Department of at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Papers in the Earth and Atmospheric Sciences by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. Authors Alex Chepstow-Lusty, Mark B. Bush, Michael R. Frogley, Paul A. Baker, Sherilyn C. Fritz, and James Aronson This article is available at DigitalCommons@University of Nebraska - Lincoln: https://digitalcommons.unl.edu/ geosciencefacpub/30 Published in Quaternary Research 63:1 (January 2005), pp. -
Seasonal Patterns of Atmospheric Mercury in Tropical South America As Inferred by a Continuous Total Gaseous Mercury Record at Chacaltaya Station (5240 M) in Bolivia
Atmos. Chem. Phys., 21, 3447–3472, 2021 https://doi.org/10.5194/acp-21-3447-2021 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Seasonal patterns of atmospheric mercury in tropical South America as inferred by a continuous total gaseous mercury record at Chacaltaya station (5240 m) in Bolivia Alkuin Maximilian Koenig1, Olivier Magand1, Paolo Laj1, Marcos Andrade2,7, Isabel Moreno2, Fernando Velarde2, Grover Salvatierra2, René Gutierrez2, Luis Blacutt2, Diego Aliaga3, Thomas Reichler4, Karine Sellegri5, Olivier Laurent6, Michel Ramonet6, and Aurélien Dommergue1 1Institut des Géosciences de l’Environnement, Université Grenoble Alpes, CNRS, IRD, Grenoble INP, Grenoble, France 2Laboratorio de Física de la Atmósfera, Instituto de Investigaciones Físicas, Universidad Mayor de San Andrés, La Paz, Bolivia 3Institute for Atmospheric and Earth System Research/Physics, Faculty of Science, University of Helsinki, Helsinki, 00014, Finland 4Department of Atmospheric Sciences, University of Utah, Salt Lake City, UT 84112, USA 5Université Clermont Auvergne, CNRS, Laboratoire de Météorologie Physique, UMR 6016, Clermont-Ferrand, France 6Laboratoire des Sciences du Climat et de l’Environnement, LSCE-IPSL (CEA-CNRS-UVSQ), Université Paris-Saclay, Gif-sur-Yvette, France 7Department of Atmospheric and Oceanic Sciences, University of Maryland, College Park, MD 20742, USA Correspondence: Alkuin Maximilian Koenig ([email protected]) Received: 22 September 2020 – Discussion started: 28 October 2020 Revised: 20 January 2021 – Accepted: 21 January 2021 – Published: 5 March 2021 Abstract. High-quality atmospheric mercury (Hg) data are concentrations were linked to either westerly Altiplanic air rare for South America, especially for its tropical region. As a masses or those originating from the lowlands to the south- consequence, mercury dynamics are still highly uncertain in east of CHC. -
A Submarine Perspective of the Honolulu Volcanics, Oahu
Journal of Volcanology and Geothermal Research 151 (2006) 279–307 www.elsevier.com/locate/jvolgeores A submarine perspective of the Honolulu Volcanics, Oahu David A. Clague a,*, Jennifer B. Paduan a, William C. McIntosh b, Brian L. Cousens c, Alice´ S. Davis a, Jennifer R. Reynolds d a Monterey Bay Aquarium Research Institute, 7700 Sandholdt Road, Moss Landing, CA 95039-9644, USA b New Mexico Geochronology Research Laboratory, N.M. Bureau of Geology, New Mexico Tech, 801 Leroy Place, Socorro, 87801-4796, USA c Ottawa-Carleton Geoscience Centre, Department of Earth Sciences, Carleton University, 1125 Colonel By Drive, Ottawa, Ontario, Canada K1S 5B6 d School of Fisheries and Ocean Sciences, West Coast and Polar Regions Undersea Research Center, University of Alaska Fairbanks, P.O. Box 757220, 213 O’Neill Building, Fairbanks, AK 99775, USA Accepted 15 July 2005 Available online 27 December 2005 Abstract Lavas and volcaniclastic deposits were observed and collected from 4 submarine cones that are part of the Honolulu Volcanics on Oahu, Hawaii. The locations of these and a few additional, but unsampled, vents demonstrate that nearly all the vents are located on or very close to the shoreline of Oahu, with the most distal vent just 12 km offshore. The clastic samples and outcrops range from coarse breccias to cross-bedded ash deposits and show that explosive volcanism at depths between about 350 and 590 m depth played a part in forming these volcanic cones. The eruptive styles appear to be dominantly effusive to strombolian at greater depths, but apparently include violent phreatomagmatic explosive activity at the shallower sites along the submarine southwest extension of the Koko Rift. -
Scale Deformation of Volcanic Centres in the Central Andes
letters to nature 14. Shannon, R. D. Revised effective ionic radii and systematic studies of interatomic distances in halides of 1–1.5 cm yr21 (Fig. 2). An area in southern Peru about 2.5 km and chalcogenides. Acta Crystallogr. A 32, 751–767 (1976). east of the volcano Hualca Hualca and 7 km north of the active 15. Hansen, M. (ed.) Constitution of Binary Alloys (McGraw-Hill, New York, 1958). 21 16. Emsley, J. (ed.) The Elements (Clarendon, Oxford, 1994). volcano Sabancaya is inflating with U LOS of about 2 cm yr . A third 21 17. Tanaka, H., Takahashi, I., Kimura, M. & Sobukawa, H. in Science and Technology in Catalysts 1994 (eds inflationary source (with ULOS ¼ 1cmyr ) is not associated with Izumi, Y., Arai, H. & Iwamoto, M.) 457–460 (Kodansya-Elsevier, Tokyo, 1994). a volcanic edifice. This third source is located 11.5 km south of 18. Tanaka, H., Tan, I., Uenishi, M., Kimura, M. & Dohmae, K. in Topics in Catalysts (eds Kruse, N., Frennet, A. & Bastin, J.-M.) Vols 16/17, 63–70 (Kluwer Academic, New York, 2001). Lastarria and 6.8 km north of Cordon del Azufre on the border between Chile and Argentina, and is hereafter called ‘Lazufre’. Supplementary Information accompanies the paper on Nature’s website Robledo caldera, in northwest Argentina, is subsiding with U (http://www.nature.com/nature). LOS of 2–2.5 cm yr21. Because the inferred sources are more than a few kilometres deep, any complexities in the source region are damped Acknowledgements such that the observed surface deformation pattern is smooth.