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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). -
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.. -
Geochemistry of Sideromelane and Felsic Glass Shards in Pleistocene Ash Layers at Sites 953, 954, and 9561
Weaver, P.P.E., Schmincke, H.-U., Firth, J.V., and Duffield, W. (Eds.), 1998 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 157 25. GEOCHEMISTRY OF SIDEROMELANE AND FELSIC GLASS SHARDS IN PLEISTOCENE ASH LAYERS AT SITES 953, 954, AND 9561 Andrey A. Gurenko2 and Hans-Ulrich Schmincke2 ABSTRACT Sideromelane and felsic glass shards from unconsolidated Pleistocene volcaniclastic sediments drilled at Sites 953, 954, and 956 are thought to have derived from submarine and subaerial volcanic eruptions on Gran Canaria (Sites 953 and 954) and Tenerife (Sites 954 and 956). We analyzed these glasses by electron microprobe for major elements and sulfur, chlorine, and fluorine. Sideromelane glasses represent a spectrum from alkali basalt through basanite, hawaiite, mugearite, and tephrite to nephelinite. Felsic glasses have compositions similar to benmoreite, trachyte, and phonolite. Vesiculated mafic and felsic glass shards, which are characterized by low S and Cl concentrations (0.01−0.06 wt% S and 0.01–0.04 wt% Cl), are interpreted to have formed by pyroclastic activity on land or in shallow water and appeared to have been strongly degassed. Vesicle-free blocky glass shards having 0.05−0.13 wt% S are likely to have resulted from submarine eruptions at moderate water depths and represent undegassed or slightly degassed magmas. Cl concentrations range from 0.01 to 0.33 wt% and increase with increasing MgO, suggesting that Cl behaves as an incompatible element during magma crystallization. Concentrations of fluorine (0.04− 0.34 wt% F) are likely to represent undegassed values, and the variations in F/K ratios between 0.02 and 0.24 are believed to reflect those of parental magmas and of the mantle source. -
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. -
Nonexplosive and Explosive Magma/Wet-Sediment Interaction
Journal of Volcanology and Geothermal Research 181 (2009) 155–172 Contents lists available at ScienceDirect Journal of Volcanology and Geothermal Research journal homepage: www.elsevier.com/locate/jvolgeores Nonexplosive and explosive magma/wet-sediment interaction during emplacement of Eocene intrusions into Cretaceous to Eocene strata, Trans-Pecos igneous province, West Texas Kenneth S. Befus a,⁎, Richard E. Hanson a, Daniel P. Miggins b, John A. Breyer a, Arthur B. Busbey a a Department of Geology, Texas Christian University, Box 298830, Fort Worth, TX 76129, USA b U.S. Geological Survey, Denver Federal Center, Box 25046, Denver, CO 80225, USA article info abstract Article history: Eocene intrusion of alkaline basaltic to trachyandesitic magmas into unlithified, Upper Cretaceous Received 16 June 2008 (Maastrichtian) to Eocene fluvial strata in part of the Trans-Pecos igneous province in West Texas produced Accepted 22 December 2008 an array of features recording both nonexplosive and explosive magma/wet-sediment interaction. Intrusive Available online 13 January 2009 complexes with 40Ar/39Ar dates of ~47–46 Ma consist of coherent basalt, peperite, and disrupted sediment. Two of the complexes cutting Cretaceous strata contain masses of conglomerate derived from Eocene fluvial Keywords: deposits that, at the onset of intrusive activity, would have been N400–500 m above the present level of phreatomagmatism peperite exposure. These intrusive complexes are inferred to be remnants of diatremes that fed maar volcanoes during diatreme an early stage of magmatism in this part of the Trans-Pecos province. Disrupted Cretaceous strata along Trans-Pecos Texas diatreme margins record collapse of conduit walls during and after subsurface phreatomagmatic explosions. -
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. -
Analogues for Radioactive Waste For~1S •
PNL-2776 UC-70 3 3679 00049 3611 ,. NATURALLY OCCURRING GLASSES: ANALOGUES FOR RADIOACTIVE WASTE FOR~1S • Rodney C. Ewing Richard F. Haaker Department of Geology University of New Mexico Albuquerque, ~ew Mexico 87131 April 1979 Prepared for the U.S. Department of Energy under Contract EY-76-C-06-1830 Pacifi c i'lorthwest Laboratory Richland, Washington 99352 TABLE OF CONTENTS List of Tables. i i List of Figures iii Acknowledgements. Introduction. 3 Natural Glasses 5 Volcanic Glasses 9 Physical Properties 10 Compos i ti on . 10 Age Distributions 10 Alteration. 27 Devitrification 29 Hydration 32 Tekti tes. 37 Physical Properties 38 Composition . 38 Age Distributions . 38 Alteration, Hydration 44 and Devitrification Lunar Glasses 44 Summary . 49 Applications to Radioactive Waste Disposal. 51 Recommenda ti ons 59 References 61 Glossary 65 i LIST OF TABLES 1. Petrographic Properties of Natural Glasses 6 2. Average Densities of Natural Glasses 11 3. Density of Crystalline Rock and Corresponding Glass 11 4. Glass and Glassy Rocks: Compressibility 12 5. Glass and Glassy Rocks: Elastic Constants 13 6. Glass: Effect of Temperature on Elastic Constants 13 7. Strength of Hollow Cylinders of Glass Under External 14 Hydrostatic Pressure 8. Shearing Strength Under High Confining Pressure 14 9. Conductivity of Glass 15 10. Viscosity of Miscellaneous Glasses 16 11. Typical Compositions for Volcanic Glasses 18 12. Selected Physical Properties of Tektites 39 13. Elastic Constants 40 14. Average Composition of Tektites 41 15. K-Ar and Fission-Track Ages of Tektite Strewn Fields 42 16. Microprobe Analyses of Various Apollo 11 Glasses 46 17. -
Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility
Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility Hjalti Franzson Gudmundur H. Gudfinnsson Julia Frolova Helga M. Helgadóttir Bruce Pauly Anette K. Mortensen Sveinn P. Jakobsson Prepared for National Energy Authority and Reykjavík Energy ÍSOR-2011/064 ICELAND GEOSURVEY Reykjavík: Orkugardur, Grensásvegur 9, 108 Reykjavík, Iceland - Tel.: 528 1500 - Fax: 528 1699 Akureyri: Rangárvellir, P.O. Box 30, 602 Akureyri, Iceland - Tel.: 528 1500 - Fax: 528 1599 [email protected] - www.isor.is Report Project no.: 540105 Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility Hjalti Franzson Gudmundur H. Gudfinnsson Julia Frolova Helga M. Helgadóttir Bruce Pauly Anette K. Mortensen Sveinn P. Jakobsson Prepared for National Energy Authority and Reykjavík Energy ÍSOR-2011/064 December 2011 Key page Report no. Date Distribution ÍSOR-2011/064 December 2011 Open Closed Report name / Main and subheadings Number of copies Icelandic Hyaloclastite Tuffs. Petrophysical Properties, Alteration 7 and Geochemical Mobility Number of pages 103 Authors Project manager Hjalti Franzson, Gudmundur H. Gudfinnsson, Julia Frolova, Hjalti Franzson Helga M. Helgadóttir, Bruce Pauly, Anette K. Mortensen and Sveinn P. Jakobsson Classification of report Project no. 540105 Prepared for National Energy Authority and Reykjavík Energy Cooperators Moscow University, University of California in Davis, Natural History Museum in Iceland Abstract This study attempts to define the properties of hyaloclastite formations which control their petrophysical characteristics during their progressive alteration. It is based on 140 tuffaceous cores from last glaciation to 2–3 m y. The water content shows a progressive increase with alteration to about 12%, which mainly is bound in the smectite and zeolite alteration minerals. -
Basalt-Trachybasalt Samples in Gale Crater, Mars
Open Research Online The Open University’s repository of research publications and other research outputs Basalt-trachybasalt samples in Gale Crater, Mars Journal Item How to cite: Edwards, Peter H.; Bridges, John C.; Wiens, Roger; Anderson, Ryan; Dyar, Darby; Fisk, Martin; Thompson, Lucy; Gasda, Patrick; Filiberto, Justin; Schwenzer, Susanne P.; Blaney, Diana and Hutchinson, Ian (2017). Basalt- trachybasalt samples in Gale Crater, Mars. Meteoritics & Planetary Science, 52(11) pp. 2391–2410. For guidance on citations see FAQs. c 2017 The Authors Meteoritics Planetary Science https://creativecommons.org/licenses/by-nc-nd/4.0/ Version: Version of Record Link(s) to article on publisher’s website: http://dx.doi.org/doi:10.1111/maps.12953 Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online’s data policy on reuse of materials please consult the policies page. oro.open.ac.uk Meteoritics & Planetary Science 52, Nr 11, 2391–2410 (2017) doi: 10.1111/maps.12953 Basalt–trachybasalt samples in Gale Crater, Mars Peter H. EDWARDS1, John C. BRIDGES 1*, Roger WIENS2, Ryan ANDERSON3, Darby DYAR4, Martin FISK5, Lucy THOMPSON 6, Patrick GASDA2, Justin FILIBERTO7, Susanne P. SCHWENZER8, Diana BLANEY9, and Ian HUTCHINSON1 1Department of Physics and Astronomy, Leicester Institute for Space and Earth Observation, University of Leicester, Leicester LE1 7RH, UK 2Los Alamos National Lab, Los Alamos, New Mexico 87545, USA 3USGS Astrogeology Science -
29. Sulfur Isotope Ratios of Leg 126 Igneous Rocks1
Taylor, B., Fujioka, K., et al., 1992 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 126 29. SULFUR ISOTOPE RATIOS OF LEG 126 IGNEOUS ROCKS1 Peter Torssander2 ABSTRACT Sulfur isotope ratios have been determined in 19 selected igneous rocks from Leg 126. The δ34S of the analyzed rocks ranges from -0.1 o/00 to +19.60 o/oo. The overall variation in sulfur isotope composition of the rocks is caused by varying degrees of seawater alteration. Most of the samples are altered by seawater and only five of them are considered to have maintained their magmatic sulfur isotope composition. These samples are all from the backarc sites and have δ34S values varying from +0.2 o/oo to +1.6 o/oo , of which the high δ34S values suggest that the earliest magmas in the rift are more arc-like in their sulfur isotope composition than the later magmas. The δ34S values from the forearc sites are similar to or heavier than the sulfur isotope composition of the present arc. INTRODUCTION from 0 o/oo to +9 o/00 (Ueda and Sakai, 1984), which could arise from inhomogeneities in the mantle but are more likely a result of contami- Sulfur is a volatile element that can be degassed during the ascent nation from the subducting slab (A. Ueda, pers. comm., 1988). of basaltic magma. Degassing causes sulfur isotope fractionation; the Leg 126 of the Ocean Drilling Program (ODP) drilled seven sites isotopic composition of sulfur in rocks can vary with the concentra- in the backarc and forearc of the Izu-Bonin Arc (Fig. -
Nicaragua's Cerro Negro Stratovolcano
NICARAGUANICARAGUA’S’S CERROCERRO NEGRONEGRO STRASTRATOVTOVOLCANOOLCANO —— HOW DID IT BLOW ITS TOP??? 1) A stratovolcano or composite volcano 6) Large cloud of pyroclastic debris, is built of alternating layers of lava Match the explanations with the numbers on the volcano and find out. steam, and other vapors erupted and pyroclastic (ash or ejected de- from Cerro Negro. The larger, bris) deposits. These deposits accu- heavier fragments fall back on the mulate around the central vent in a cone while the smaller, lighter ash cone-shaped pile. Lava may flow from 6 fragments are carried great dis- fissures (fractures or cracks) radi- tances before they settle. ating from the central vent, whereas the multi-sized pyroclastics are B 7) A smaller cloud of darker material ejected from the main vent. 9 indicates that a localized eruption L has just occurred. 2) Steam and other vapors rising from 10 the large volcanic blocks erupted 8 from the main crater recently. Com- ) Cloud of vapors from the volcano is mostly steam and ash, but also con- pare with the older, cooler volcanic 8 tains chlorine, fluorine, sulfur, and blocks at the ends of the tracks or L 5 their acids. furrows that run down the slope of 5 the main cone. These tracks or fur- 5 9 rows were plowed by the rolling 7 9) Shadow cast by the ash and vapor blocks. Some house-size blocks now 5 cloud from the volcano (6) carried lie loosely at the bottom of the 5 by turbulent hot gasses and winds. slope. 4 When the volcanic ash settles, the 2 pyroclastic deposit that forms is 9 called an ash fall. -
Cretaceous Basaltic Phreatomagmatic Volcanism in West Texas: Maar Complex at Peña Mountain, Big Bend National Park ⁎ K.S
Available online at www.sciencedirect.com Journal of Volcanology and Geothermal Research 173 (2008) 245–264 www.elsevier.com/locate/jvolgeores Cretaceous basaltic phreatomagmatic volcanism in West Texas: Maar complex at Peña Mountain, Big Bend National Park ⁎ K.S. Befus a, , R.E. Hanson a, T.M. Lehman b, W.R. Griffin c a Department of Geology, Texas Christian University, Box 298830, Fort Worth, TX 76129, USA b Department of Geosciences, Texas Tech University, Box 41053, Lubbock, TX 79409, USA c Department of Geosciences, University of Texas at Dallas, Box 830688, Richardson, Texas 75083, USA Received 23 March 2007; accepted 25 January 2008 Available online 10 March 2008 Abstract A structurally complex succession of basaltic pyroclastic deposits produced from overlapping phreatomagmatic volcanoes occurs within Upper Cretaceous floodplain deposits in the Aguja Formation in Big Bend National Park, West Texas. Together with similar basaltic deposits recently documented elsewhere in the Aguja Formation, these rocks provide evidence for an episode of phreatomagmatic volcanism that predates onset of arc magmatism in the region in the Paleogene. At Peña Mountain, the pyroclastic deposits are ≥70 m thick and consist dominantly of tabular beds of lapillistone and lapilli tuff containing angular to fluidal pyroclasts of altered sideromelane intermixed with abundant accidental terrigenous detritus derived from underlying Aguja sediments. Tephra characteristics indicate derivation from phreatomagmatic explosions involving fine- scale interaction between magma and sediment in the shallow subsurface. Deposition occurred by pyroclastic fall and base-surge processes in near-vent settings; most base-surge deposits lack tractional sedimentary structures and are inferred to have formed by suspension sedimentation from rapidly decelerating surges.