Mount Etna Europe’S Biggest Volcano Gnuckx
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Volcanic Gases and Aerosols Guidelines Introduction
IVHHN Gas Guidelines www.ivhhn.org/gas/guidelines.html Volcanic Gases and Aerosols Guidelines The following pages contain information relating to the health hazards of gases and aerosols typically emitted during volcanic activity. Each section outlines the properties of the emission; its impacts on health; international guidelines for concentrations; and examples of concentrations and effects in volcanic contexts, including casualties. Before looking at the emissions data, we recommend that you read the general introduction to volcanic gases and aerosols first. A glossary to some of the terms used in the explanations and guidelines is also provided at the end of this document. Introduction An introduction to the aims and purpose of the Gas and Aerosol Guidelines is given here, as well as further information on international guideline levels and the units used in the website. A brief review of safety procedures currently implemented by volcanologists and volcano observatories is also provided. General Introduction Gas and aerosol hazards are associated with all volcanic activity, from diffuse soil gas emissions to 2- plinian eruptions. The volcanic emissions of most concern are SO2, HF, sulphate (SO4 ), CO2, HCl and H2S, although, there are other volcanic volatile species that may have human health implications, including mercury and other metals. Since 1900, there have been at least 62 serious volcanic-gas related incidents. Of these, the gas-outburst at Lake Nyos in 1986 was the most disastrous, causing 1746 deaths, >845 injuries and the evacuation of 4430 people. Other volcanic-gas related incidents have been responsible for more than 280 deaths and 1120 injuries, and contributed to the evacuation or ill health of >53,700 people (Witham, in review). -
Characterization of Volcanic Deposits with Ground-Penetrating Radar
Bull Volcanol (1997) 58:515–527 Q Springer-Verlag 1997 ORIGINAL PAPER J. K. Russell 7 M. V. Stasiuk Characterization of volcanic deposits with ground-penetrating radar Received: 10 May 1996 / Accepted: 27 December 1996 Abstract Field-based studies of surficial volcanic de- Key words Ground-penetrating radar 7 Volcanic posits are commonly complicated by a combination of deposits 7 Stratigraphy 7 Dielectric constant 7 Radar poor exposure and rapid lateral variations controlled velocity 7 Pyroclastic flow 7 Airfall 7 Lava by unknown paleotopography. The potential of ground-penetrating radar (GPR) as an aid to volcano- logical studies is shown using data collected from trav- erses over four well-exposed, Recent volcanic deposits Introduction in western Canada. The deposits comprise a pumice airfall deposit (3–4 m thick), a basalt lava flow (3–6 m Studies of surficial volcanic deposits are commonly lim- thick), a pyroclastic flow deposit (15 m thick), and an ited by incomplete exposure. Estimates of the physical internally stratified pumice talus deposit (60 m thick). properties, distributions, thicknesses, and internal Results show that GPR is effective in delineating major structures of the deposits are usually derived from stud- stratigraphic contacts and hence can be used to map ies on a few well-dissected outcrops. Ground-penetrat- unexposed deposits. Different volcanic deposits also ing radar (GPR) is a portable geophysical technique exhibit different radar stratigraphic character, suggest- which can provide ancillary information on the unex- ing that deposit type may be determined from radar posed parts of deposits, thereby facilitating many volca- images. In addition, large blocks within the pyroclastic nological studies. -
The Real Spirit of Eastern Sicily
Drive & Hike, Walk & Discover The Real Spirit of Eastern Sicily Exploring a mythical island: Mount Etna, ancient civilizations, Greek, Roman and Baroque treasures TRIP NOTES 2021 © Genius Loci Travel. All rights reserved. booking@genius -loci.it | www.genius -loci.it *** GENIUS LOCI TRAVEL - The Real Spirit Of Italy *** Drive & Hike, Walk & Discover INTRODUCTION Everybody knows Sicily. And most of us could even name a few famous places such as Taormina, Mt. Etna, and Syracuse. All places which definitely deserve a visit! But this tour will also show you life in Sicily as the real Sicilians live it. You’ll fully explore the south-eastern part of Sicily, home to the eight baroque towns, listed by UNESCO as ‘world heritage sites’. Both Noto and Ragusa are a must! Of course you will visit Syracuse, once the most powerful Greek city in the world, where 3000 years of history are still alive. Visit its amazing Greek ‘Neapolis’ - and perhaps attend a show - and explore this intriguing city carefully. You will of course make a few nice walks, to explore the amazing landscape of the Iblei Mountains. Discover the inland villages, yet to be discovered by mass tourism. Sit in the shade of the orange trees and have a nice country lunch with local specialties. Have a delicious almond or strawberry ‘granita’ for breakfast, swim in the little pools of the wonderful Pantalica Gorge and handpick some fresh oranges. You will be part of the different civilizations that have chosen Sicily as their base: you’ll walk past prehistoric caves, Byzantine churches and baroque buildings. -
VOLCANO-TECTONIC HISTORY of CRATER FLAT, SOUTHWESTERN NEVADA, AS SUGGESTED by NEW EVIDENCE from DRILL HOLE USW-VH-1 and VICINITY By
5)zt.-t"o En-, 6-.-5 f %. _rc . i%: .- 1 - . ~~Open-File Report 82-457 n-File Report 82-457 (.8X/1<~~/I I W II ~~~~~~~~~~~~~~i UNITED STATES V DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY VOLCANO-TECTONIC HISTORY OF CRATER FLAT. SOUTHWESTERN NEVADA, AS SUGGESTED BY NEW EVIDENCE FROM DRILL HOLE USW-VH-1 AND VICINITY Open-File Report 82-457 1982 This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey editorial standards. X 0 X 0 0- 0 Prepared by the U.S. Geological Survey C- for the 3 z Nevada Operations Office -4i U.S. Department of Energy z (Memorandum of Understanding DE-AI08-78ET44802) U, I.- -4 Copies of this Open-file Report may be purchased from Open-File Services Section Branch of Distribution U.S. Geological Survey Box 25425, Federal Center Denver, Colorado 80225 PREPAYMENT IS REQUIRED Price information will be published in the monthly listing RNew Publications of the Geological Surveys FOR ADDITIONAL IXNFORAATION CALL: Commercial: (303)234-5888 FTS: 234-5888 Open-File Report 82-457 Open-File Report 82-457 UNITED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY VOLCANO-TECTONIC HISTORY OF CRATER FLAT, SOUTHWESTERN NEVADA, AS SUGGESTED BY NEW EVIDENCE FROM DRILL HOLE USW-VH-1 AND VICINITY By W. J. Carr CONTENTS Page Abstract... ....... .......... ............................... .........................a.. ............1 Introduction,............................................................ 1 Acknowledgments............................................... ...... ........ 3 Drill-hole location and history..................................... 3 Geologic framework of Crater Flat ...................................6 Aeromagnetic anomalies........................ oo..... ... .......... ..................7 Volcano-tectonic history of Crater Flat ....o........o .................. 9 Lithology of drill hole.'.. ............................. o..................... 12 Structural properties of the core.. -
Chapter 2 Alaska’S Igneous Rocks
Chapter 2 Alaska’s Igneous Rocks Resources • Alaska Department of Natural Resources, 2010, Division of Geological and Geophysical Surveys, Alaska Geologic Materials Center website, accessed May 27, 2010, at http://www.dggs.dnr.state.ak.us/?link=gmc_overview&menu_link=gmc. • Alaska Resource Education: Alaska Resource Education website, accessed February 22, 2011, at http://www.akresource.org/. • Barton, K.E., Howell, D.G., and Vigil, J.F., 2003, The North America tapestry of time and terrain: U.S. Geological Survey Geologic Investigations Series I-2781, 1 sheet. (Also available at http://pubs.usgs.gov/imap/i2781/.) • Danaher, Hugh, 2006, Mineral identification project website, accessed May 27, 2010, at http://www.fremontica.com/minerals/. • Digital Library for Earth System Education, [n.d.], Find a resource—Bowens reaction series: Digital Library for Earth System Education website, accessed June 10, 2010, at http://www.dlese.org/library/query.do?q=Bowens%20reaction%20series&s=0. • Edwards, L.E., and Pojeta, J., Jr., 1997, Fossils, rocks, and time: U.S. Geological Survey website. (Available at http://pubs.usgs.gov/gip/fossils/contents.html.) • Garden Buildings Direct, 2010, Rocks and minerals: Garden Buildings Direct website, accessed June 4, 2010, at http://www.gardenbuildingsdirect.co.uk/Article/rocks-and- minerals. • Illinois State Museum, 2003, Geology online–GeoGallery: Illinois State Museum Society database, accessed May 27, 2010 at http://geologyonline.museum.state.il.us/geogallery/. • Knecht, Elizebeth, designer, Pearson, R.W., and Hermans, Majorie, eds., 1998, Alaska in maps—A thematic atlas: Alaska Geographic Society, 100 p. Lillie, R.J., 2005, Parks and plates—The geology of our National parks, monuments, and seashores: New York, W.W. -
Anatomy of a Volcanic Eruption: Case Study: Mt. St. Helens
Anatomy of a Volcanic Eruption: Case Study: Mt. St. Helens Materials Included in this Box: • Teacher Background Information • 3-D models of Mt. St. Helens (before and after eruption) • Examples of stratovolcano rock products: Tuff (pyroclastic flow), pumice, rhyolite/dacite, ash • Sandbox crater formation exercise • Laminated photos/diagrams Teacher Background There are several shapes and types of volcanoes around the world. Some volcanoes occur on the edges of tectonic plates, such as those along the ‘ring of fire’. But there are also volcanoes that occur in the middle of tectonic plates like the Yellowstone volcano and Kilauea volcano in Hawaii. When asked to draw a volcano most people will draw a steeply sided, conical mountain that has a depression (crater) at the top. This image of a 'typical' volcano is called a stratovolcano (a.k.a. composite volcano). While this is the often visualized image of a volcano, there are actually many different shapes volcanoes can be. A volcano's shape is mostly determined by the type of magma/lava that is created underneath it. Stratovolcanoes get their shape because of the thick, sticky (viscous) magma that forms at subduction zones. This magma/lava is layered between ash, pumice, and rock fragments. These layers of ash and magma will build into high elevation, steeply sided, conical shaped mountains and form a 'typical' volcano shape. Stratovolcanoes are also known for their explosive and destructive eruptions. Eruptions can cause clouds of gas, ash, dust, and rock fragments to eject into the atmosphere. These clouds of ash can become so dense and heavy that they quickly fall down the side of the volcanoes as a pyroclastic flow. -
Properties of Volcanic Ash and Pumice Concrete
Properties of volcanic ash and pumice concrete Autor(en): Hossain, Khandaker M.A. Objekttyp: Article Zeitschrift: IABSE reports = Rapports AIPC = IVBH Berichte Band (Jahr): 81 (1999) PDF erstellt am: 27.09.2021 Persistenter Link: http://doi.org/10.5169/seals-61426 Nutzungsbedingungen Die ETH-Bibliothek ist Anbieterin der digitalisierten Zeitschriften. Sie besitzt keine Urheberrechte an den Inhalten der Zeitschriften. Die Rechte liegen in der Regel bei den Herausgebern. Die auf der Plattform e-periodica veröffentlichten Dokumente stehen für nicht-kommerzielle Zwecke in Lehre und Forschung sowie für die private Nutzung frei zur Verfügung. Einzelne Dateien oder Ausdrucke aus diesem Angebot können zusammen mit diesen Nutzungsbedingungen und den korrekten Herkunftsbezeichnungen weitergegeben werden. Das Veröffentlichen von Bildern in Print- und Online-Publikationen ist nur mit vorheriger Genehmigung der Rechteinhaber erlaubt. Die systematische Speicherung von Teilen des elektronischen Angebots auf anderen Servern bedarf ebenfalls des schriftlichen Einverständnisses der Rechteinhaber. Haftungsausschluss Alle Angaben erfolgen ohne Gewähr für Vollständigkeit oder Richtigkeit. Es wird keine Haftung übernommen für Schäden durch die Verwendung von Informationen aus diesem Online-Angebot oder durch das Fehlen von Informationen. Dies gilt auch für Inhalte Dritter, die über dieses Angebot zugänglich sind. Ein Dienst der ETH-Bibliothek ETH Zürich, Rämistrasse 101, 8092 Zürich, Schweiz, www.library.ethz.ch http://www.e-periodica.ch 145 IABSE COLLOQUIUM PHUKET 1999 \ Properties of Volcanic Ash and Pumice Concrete Khandaker M. A. HOSSAIN Khandaker M. A. Hossain, born in 1963, Lecturer in Civil Engineering received BSc and MSc in civil engineering from Bangladesh University of Engineering The PNG University of Technology & Technology, Dhaka and PhD from Lae, Papua New Guinea Strathclyde University, Glasgow, UK. -
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. -
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. -
Sicily: a Cultural Journey 11 DAYS September 2–12, 2019
Join Friendship Force on Sicily: A Cultural Journey 11 DAYS September 2–12, 2019 Speak to a travel expert today 1-800-438-7672 © 2018 EF Education First Sicily: A Cultural Journey 11 DAYS The Sicilian sun shines light on a different side YOUR TOUR PACKAGE INCLUDES of Italy. 9 nights in handpicked hotels 9 breakfasts In the midst of the Mediterranean, discover an island with personality all its own—full 6 dinners with beer or wine of flavor and teeming with one-of-a-kind art and architecture. From multicultural 1 cooking class Guided sightseeing tours Palermo to breathtaking Taormina, each and every stop on this tour of Sicily reveals Expert Tour Director & local guides unexpected treasures. Private deluxe motor coach INCLUDED HIGHLIGHTS Palermo Cathedral, home-hosted dinner in Palermo, Agrigento's Greek ruins, Piazza Amerina, Syracuse Cathedral, Sicilian cooking class, views of Mount Etna, Taormina's Greek theater TOUR PACE On this guided tour, you'll walk for about 1.5 hours daily across uneven terrain, including cobblestone streets and unpaved roads, at high altitudes. Speak to a travel expert today 1-800-438-7672 © 2018 EF Education First Itinerary Overnight flight | 1 NIGHT Taormina Region | 2 NIGHTS Day 1: Travel day Day 9: Transfer to Taormina & sightseeing tour Board your overnight flight to Palermo today. Included meals: breakfast Transfer to Taormina, where a local guide introduces you to this scenic town perched high above the sea. Palermo | 3 NIGHTS • Enjoy views of Mount Etna, Taormina Cathedral, and the Palazzo Corvaia, seat of the first Sicilian parliament Day 2: Arrival in Palermo • Visit the town’s 2nd-century Greek theater Included meals: welcome dinner Welcome to Italy! Gather with your fellow travelers at tonight’s welcome dinner. -
Volcanism on Mars
Author's personal copy Chapter 41 Volcanism on Mars James R. Zimbelman Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA William Brent Garry and Jacob Elvin Bleacher Sciences and Exploration Directorate, Code 600, NASA Goddard Space Flight Center, Greenbelt, MD, USA David A. Crown Planetary Science Institute, Tucson, AZ, USA Chapter Outline 1. Introduction 717 7. Volcanic Plains 724 2. Background 718 8. Medusae Fossae Formation 725 3. Large Central Volcanoes 720 9. Compositional Constraints 726 4. Paterae and Tholi 721 10. Volcanic History of Mars 727 5. Hellas Highland Volcanoes 722 11. Future Studies 728 6. Small Constructs 723 Further Reading 728 GLOSSARY shield volcano A broad volcanic construct consisting of a multitude of individual lava flows. Flank slopes are typically w5, or less AMAZONIAN The youngest geologic time period on Mars identi- than half as steep as the flanks on a typical composite volcano. fied through geologic mapping of superposition relations and the SNC meteorites A group of igneous meteorites that originated on areal density of impact craters. Mars, as indicated by a relatively young age for most of these caldera An irregular collapse feature formed over the evacuated meteorites, but most importantly because gases trapped within magma chamber within a volcano, which includes the potential glassy parts of the meteorite are identical to the atmosphere of for a significant role for explosive volcanism. Mars. The abbreviation is derived from the names of the three central volcano Edifice created by the emplacement of volcanic meteorites that define major subdivisions identified within the materials from a centralized source vent rather than from along a group: S, Shergotty; N, Nakhla; C, Chassigny. -
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.