Water and the Generation of Volcanic Electricity
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Iceland Can Be Considered Volcanologist “Heaven”
Iceland can be considered volcanologist “heaven” 1) Sub-aerial continuation of the Mid-Atlantic Ridge 2) Intersection of a mantle plume with a spreading ocean ridge 3) Volcanism associated with tectonic rifting 4) Sub-glacial volcanism 5) Tertiary flood (plateau) basalts 6) Bi-modal volcanism 7) Submarine volcanism 8) 18 historically active volcanoes 9) Eruptions roughly every 5 years 1. The North Atlantic opened about 54 Ma separating Greenland from Europe. 2. Spreading was initially along the now extinct Agir ridge (AER). 3. The Icelandic plume was under Greenland at that time. 4. The Greenland – Faeroe ridge represents the plume track during the history of the NE Atlantic. Kolbeinsey ridge (KR) 5. During the last 20 Ma the Reykjanes Ridge (RR) Icelandic rift zones have migrated eastward, stepwise, maintaining their position near the plume 6. The plume center is thought to be beneath Vatnajökull 1 North Rift Zone – currently active East Rift Zone – currently active West Rift Zone – last erupted about 1000-1300 AD [Also eastern (Oræfajökull) and western (Snæfellsnese) flank zones] Rift zones comprise en-echelon basaltic fissure swarms 5-15 km wide and up to 200 km long. Over time these fissures swarms develop a volcanic center, eventually maturing into a central volcano with a caldera and silicic Tertiary volcanics > 3.1 Ma volcanism Late Tertiary to Early Quaternary 3.1 – 0.7 Ma Neo-volcanic zone <0.7 - present Schematic representation of Iceland’s mantle plume. The crust is about 35 – 40 km thick Iceland’s mantle plume has been tomographically imaged down to 400 km. Some claim even deeper, through the transition zone, and down to the core – mantle boundary. -
Geoscience and a Lunar Base
" t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history. -
Supplementary Material
Supplementary material S1 Eruptions considered Askja 1875 Askja, within Iceland’s Northern Volcanic Zone (NVZ), erupted in six phases of varying intensity, lasting 17 hours on 28–29 March 1875. The main eruption included a Subplinian phase (Unit B) followed by hydromagmatic fall and with some proximal pyroclastic flow (Unit C) and a magmatic Plinian phase (Unit D). Units C and D consisted of 4.5 x 108 m3 and 1.37 x 109 m3 of rhyolitic tephra, respectively [1–3]. Eyjafjallajökull 2010 Eyjafjallajökull is situated in the Eastern Volcanic Zone (EVZ) in southern Iceland. The Subplinian 2010 eruption lasted from 14 April to 21 May, resulting in significant disruption to European airspace. Plume heights ranged from 3 to 10 km and dispersing 2.7 x 105 m3 of trachytic tephra [4]. Hverfjall 2000 BP Hverfjall Fires occurred from a 50 km long fissure in the Krafla Volcanic System in Iceland’s NVZ. Magma interaction with an aquifer resulted in an initial basaltic hydromagmatic fall deposit from the Hverfjall vent with a total volume of 8 x 107 m3 [5]. Eldgja 10th century The flood lava eruption in the first half of the 10th century occurred from the Eldgja fissure within the Katla Volcanic System in Iceland’s EVZ. The mainly effusive basaltic eruption is estimated to have lasted between 6 months and 6 years, and included approximately 16 explosive episodes, both magmatic and hydromagmatic. A subaerial eruption produced magmatic Unit 7 (2.4 x 107 m3 of tephra) and a subglacial eruption produced hydromagmatic Unit 8 (2.8 x 107 m3 of tephra). -
Warren and Taylor-2014-In Tog-The Moon-'Author's Personal Copy'.Pdf
This article was originally published in Treatise on Geochemistry, Second Edition published by Elsevier, and the attached copy is provided by Elsevier for the author's benefit and for the benefit of the author's institution, for non- commercial research and educational use including without limitation use in instruction at your institution, sending it to specific colleagues who you know, and providing a copy to your institution’s administrator. All other uses, reproduction and distribution, including without limitation commercial reprints, selling or licensing copies or access, or posting on open internet sites, your personal or institution’s website or repository, are prohibited. For exceptions, permission may be sought for such use through Elsevier's permissions site at: http://www.elsevier.com/locate/permissionusematerial Warren P.H., and Taylor G.J. (2014) The Moon. In: Holland H.D. and Turekian K.K. (eds.) Treatise on Geochemistry, Second Edition, vol. 2, pp. 213-250. Oxford: Elsevier. © 2014 Elsevier Ltd. All rights reserved. Author's personal copy 2.9 The Moon PH Warren, University of California, Los Angeles, CA, USA GJ Taylor, University of Hawai‘i, Honolulu, HI, USA ã 2014 Elsevier Ltd. All rights reserved. This article is a revision of the previous edition article by P. H. Warren, volume 1, pp. 559–599, © 2003, Elsevier Ltd. 2.9.1 Introduction: The Lunar Context 213 2.9.2 The Lunar Geochemical Database 214 2.9.2.1 Artificially Acquired Samples 214 2.9.2.2 Lunar Meteorites 214 2.9.2.3 Remote-Sensing Data 215 2.9.3 Mare Volcanism -
The Surtsey 1963 Eruption Plume, Characteristics and Tephra Dispersal
Geophysical Research Abstracts Vol. 21, EGU2019-17144, 2019 EGU General Assembly 2019 © Author(s) 2019. CC Attribution 4.0 license. The Surtsey 1963 eruption plume, characteristics and tephra dispersal Einar Sindri Ólafsson (1), Magnus T Guðmundsson (2), and Esther R. Guðmundsdóttir (3) (1) Institute of Earth Sciences, University of Iceland, Reykjavik, Iceland ([email protected]), (2) Institute of Earth Sciences, University of Iceland, Reykjavik, Iceland ([email protected]), (3) Institute of Earth Sciences, University of Iceland, Reykjavik, Iceland ([email protected]) Surtsey is a basaltic island in the south-western end of Vestmannaeyjar archipelago off the south coast of Iceland and is a part of the Vestmannaeyjar volcanic system. It is built from the ocean floor at about 130 m depth in a series of eruptions during 1963-1967, one of the longest eruption in Iceland in historical times. The eruptions can be split into four phases. The first phase of the eruptions was explosive and phreatomagmatic in character. The aim of this study is to put constraints on the mass of tephra transported with the plume. This is done in two ways: (1) Study soil profiles on Heimaey and on the mainland to look for tephra deposits from Surtsey as well as note contemporary descriptions of tephra fallout; and (2) by compiling existing contemporary records of plume height and use plume height – mass transport systematics to estimate the transport. Finally, we compare the outcomes of (1) and (2). Eruption started on 14 November 1963. It was explosive and fed an eruption plume rising typically to 5-9 km in November and December 1963. -
Antimicrobial Activity of Tooth Powder Containing Hekla Lava and Calendula
Swathi.A et al /J. Pharm. Sci. & Res. Vol. 7(10), 2015, 882-884 Antimicrobial Activity of Tooth Powder Containing Hekla Lava and Calendula Swathi.A, Muralidharan.N.P Bachelor of Dental Surgery,Saveetha Dental College and Hospital,Chennai Aim And Objective To study anti microbial activity of tooth powder containing Hekla lava and calendula. Background Homeopathy medicine is always a cheaper alternate and called as poor mans medicine. Hekla lava with calendula is available as a tooth powder in the market. It is a homeopathy remedy used in treating gingivitis and loose sockets which are the major problems in old age patients. It's properties can be explored as a intracanal medicament in root canal treatment as well. Materials And Methods Hekla lava with calendula powder, chlorhexidine gel and calcium hydroxide are obtained. The antibacterial activity of Hekla lava with calendula was tested against the odontogenic bacteria such as Streptococcus mutans and Enterococcus. They were subjected for the anti microbial activity by agar well diffusion method. Results In our study, we have found that the tooth powder containing hekla lava and calendula have considerable antimicobial effects ,which are compared with chlorhexidine and calcium hydroxide ,which are already in practice. Conclusion The study reveals that the tooth powder hekla lava with calendula has a good anti microbial effect against mutans and enterococcus ,which can be used in treating various dental problems. INTRODUCTION sesquiterpenes, flavonoid glycosides, triterpene saponins, The most common forms of human periodontal disease are triterpene alcohols, flavonoids, carotenoids, xanthophylls, gingivitis and periodontitis. Gingivitis is defined as an phenolic acids, steroids, mucilage, tocopherol, and inflammation of the gingiva. -
Subglacial and Submarine Volcanism in Iceland
Mars Polar Science 2000 4078.pdf SUBGLACIAL AND SUBMARINE VOLCANISM IN ICELAND. S. P. Jakobsson, Icelandic Inst. of Natural His- tory, P. O. Box 5320, 125 Reykjavik, Iceland Introduction: Iceland is the largest landmass ex- mounds, ridges and tuyas [5]. The thickness of basal posed along the Mid-Ocean Ridge System. It has been basaltic pillow lava piles often exceeds 60-80 meters constructed over the past 16 Ma by basaltic to silicic and a 300 m thick section has been reported. Pillow volcanic activity occurring at the Mid-Atlantic Ridge, lavas may also form lenses or pods at a higher level in and is topographically elevated because of the abundant the volcanoes. igneous material produced in association with the Ice- It has been suggested that at a water depth less than land hot spot, the center of which is thought to be lo- approximately 100-150 m, basaltic phreatic explosions cated beneath Vatnajokull glacier [1]. The axial rift produce hydroclastites. It appears feasible to subdivide zones which run through Iceland from southwest to the hyaloclastites of the Icelandic ridges and tuyas, ge- northeast are in direct continuation of the crestal zones netically into two main types. A substantial part of the of the Mid Atlantic Ridge and are among the most ac- base of the submarine Surtsey tuya is poorly bedded, tive volcanic zones on Earth. unsorted, hydroclastite, which probably was quenched Subglacial Volcanism: Volcanic accumulations of and rapidly accumulated below the seawater level with- hyaloclastites which are deposits formed by the intru- out penetrating the surface [6]. Only 1-2 % of the vol- sion of lava beneath water or ice and the consequent ume of extruded material in the 1996 Gjalp eruption fell shattering into small angular vitric particles, combined as air-fall tephra, the bulk piled up below the ice [4]. -
Using GIS to Study Potential Lahar Hazards from Hekla and Grímsvötn, Southern Iceland
Using GIS to Study Potential Lahar Hazards from Hekla and Grímsvötn, Southern Iceland The University of Texas at Austin Jackson School of Geosciences Ian Yeats 12/04/2014 Introduction Iceland is an island nation far in the northern hemisphere, with a portion of the country included in the Arctic Circle. Its position over a magmatic hotspot and the Atlantic mid-ocean ridge cause it to have a very active volcanic setting. Some of these eruptions, like that of Eyjafjallajökull in 2010, make worldwide news due to large ash clouds disrupting global air traffic, but many of them go unnoticed to the world. Hence, Icelandic people are very accustomed to responding to volcanic hazards, and it is essential to understand the possible risks involved with living near these active volcanoes. One major hazard associated with volcanism is lahars, or jökulhlaups in Icelandic. In Iceland, these form from the rapid melting of glaciers and snow and the addition of large quantities of volcanic material. These are very large, and sometimes hot, mudslides that even occur without a present eruption. This project used ArcMap to predict potential flow paths of lahars from two major volcanoes in southern Iceland: Hekla and Grímsvötn. Both of these have very active histories, with their last eruptions occurring in 2000 and 2011, respectively. The end goal is to produce maps that highlight these hazards, as well as towns and roads that may stand in their way. Data and Analysis This project required detailed national elevation data, a country boundary, roads, towns, rivers, and the locations of Icelandic volcanoes. -
GEOLOGY THEME STUDY Page 1
NATIONAL HISTORIC LANDMARKS Dr. Harry A. Butowsky GEOLOGY THEME STUDY Page 1 Geology National Historic Landmark Theme Study (Draft 1990) Introduction by Dr. Harry A. Butowsky Historian, History Division National Park Service, Washington, DC The Geology National Historic Landmark Theme Study represents the second phase of the National Park Service's thematic study of the history of American science. Phase one of this study, Astronomy and Astrophysics: A National Historic Landmark Theme Study was completed in l989. Subsequent phases of the science theme study will include the disciplines of biology, chemistry, mathematics, physics and other related sciences. The Science Theme Study is being completed by the National Historic Landmarks Survey of the National Park Service in compliance with the requirements of the Historic Sites Act of l935. The Historic Sites Act established "a national policy to preserve for public use historic sites, buildings and objects of national significance for the inspiration and benefit of the American people." Under the terms of the Act, the service is required to survey, study, protect, preserve, maintain, or operate nationally significant historic buildings, sites & objects. The National Historic Landmarks Survey of the National Park Service is charged with the responsibility of identifying America's nationally significant historic property. The survey meets this obligation through a comprehensive process involving thematic study of the facets of American History. In recent years, the survey has completed National Historic Landmark theme studies on topics as diverse as the American space program, World War II in the Pacific, the US Constitution, recreation in the United States and architecture in the National Parks. -
The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile. -
A) Precipitation of Minerals from Evaporating Seawater B
1. Which process could lead directly to the formation of pumice rock? A) precipitation of minerals from evaporating seawater B) metamorphism of unmelted rock material C) deposition of quartz sand D) explosive eruption of lava from a volcano Base your answers to questions 2 through 4 on the map below. The black triangle represents Mt. Hekla, a volcano in Iceland. The isolines represent the thickness of ash, in centimeters, that settled on Earth's surface after a volcanic eruption of Mt. Hekla on March 29, 1947. Point X is a location on the surface of the ash. 2. At the time of the eruption, the wind direction was primarily from the A) east B) west C) north D) south 3. How many centimeters thick was the ash beneath point X? A) 0 B) 15 C) 20 D) 25 4. In addition to the ash, solid rock formed on Mt. Hekla from the lava extruded during this eruption. This rock is most likely A) light-colored metamorphic B) dark-colored metamorphic C) fine-grained igneous D) coarse-grained igneous 5. Base your answer to the following question on the map below, which shows an area of the northwestern United States affected by a major volcanic eruption at Crater Lake during the Holocene Epoch. The pattern of distribution of the ash from the volcano was most likely caused by the direction of the A) magnetic field B) force of the volcanic eruption C) flow of surface water D) atmospheric air movements 6. Base your answer to the following question on the cross section and map of a portion of Earth's crust shown below. -
1876-09-09.Pdf
KVOL. VI. DOVER, MORRIS COUNTY, NEW JERSJEY, SATURDAY, SEPTEMBER U, 1870. NO. 39 Curds. POKTIC. 1 E'IVIK'II l»:n I. i THE IRON ERA A few mouths ago two gen'lcmen wenl A family on Pine strciit oo a jiup o Perhaps the uwat ftimilinr of inybtori- IS VAIX. xcerr THAT ^OUE WORE IIUDI; OIIS'A A fumily named Smith ban recently (niflHfuirids nro tlirm protlnciul liv Uiu fCDUauiffi Busy SATCIDAT I t K. A. BENNETT, Af. D , .HIVIJI] toOenminlowiJ, uml Mr, Brown s"[iut to fiKbt a duel upropus of an nclrcss, the KcnTouQdliitid brand—ono of U.HSI Ah, paldoti nith tliu Iruntlng njljn, AND OT1IEI13 WEIIB TATTOOI'D. add 11)13 ia Iiotr inntturs p:mai!tl: 51.libyful creatures with misehkvaitH even, Yi'Dtrifaqniat; fitniiliar, 1JUC.IIIHB ulfiioat .J.V, <m Saturday, leaned ovor tbo fence every country fair ia vitritcid liy one ur BENJ.II.VOGT. HOMCEOPATHIC Tlii.ii; ii. M luiili:Lire sivain! nmt Riive to our rejinricir nia im|»reHsiooH Fcuillit-rndo and OHiviur, tbe flnt "*w- Vhv. family are very niucj ultachuil to it. Yon may wait till the cnm',03 Hrlligbl diou, y nn tb b tinted" by MM. Peilcller and Gitillurd. Iu tbetio hard tiuiiu tu become uttncli n dUit'r of tha-e exbibitorii, niyhterifius, EDITOR i«o pr.oniF.Tor,. nf Mr. Hinitb'abuy, a li'd ubuutfmirtocu bcL-aiiMo tlio r«nl Knurco of suUnd d<ip« PHYSICIAN & SUKGKOX, Till Ilia fliry stjin tlnHli nut hi tbo ekk-a, 187C, iirnviuE ul H*tug KOUK yeiii-H old: tbcRPCond by MM.