General Volcanology
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Plate Tectonics, Volcanoes, and Earthquakes / Edited by John P
ISBN 978-1-61530-106-5 Published in 2011 by Britannica Educational Publishing (a trademark of Encyclopædia Britannica, Inc.) in association with Rosen Educational Services, LLC 29 East 21st Street, New York, NY 10010. Copyright © 2011 Encyclopædia Britannica, Inc. Britannica, Encyclopædia Britannica, and the Thistle logo are registered trademarks of Encyclopædia Britannica, Inc. All rights reserved. Rosen Educational Services materials copyright © 2011 Rosen Educational Services, LLC. All rights reserved. Distributed exclusively by Rosen Educational Services. For a listing of additional Britannica Educational Publishing titles, call toll free (800) 237-9932. First Edition Britannica Educational Publishing Michael I. Levy: Executive Editor J. E. Luebering: Senior Manager Marilyn L. Barton: Senior Coordinator, Production Control Steven Bosco: Director, Editorial Technologies Lisa S. Braucher: Senior Producer and Data Editor Yvette Charboneau: Senior Copy Editor Kathy Nakamura: Manager, Media Acquisition John P. Rafferty: Associate Editor, Earth Sciences Rosen Educational Services Alexandra Hanson-Harding: Editor Nelson Sá: Art Director Cindy Reiman: Photography Manager Nicole Russo: Designer Matthew Cauli: Cover Design Introduction by Therese Shea Library of Congress Cataloging-in-Publication Data Plate tectonics, volcanoes, and earthquakes / edited by John P. Rafferty. p. cm.—(Dynamic Earth) “In association with Britannica Educational Publishing, Rosen Educational Services.” Includes index. ISBN 978-1-61530-187-4 ( eBook) 1. Plate tectonics. -
Cross-References ASTEROID IMPACT Definition and Introduction History of Impact Cratering Studies
18 ASTEROID IMPACT Tedesco, E. F., Noah, P. V., Noah, M., and Price, S. D., 2002. The identification and confirmation of impact structures on supplemental IRAS minor planet survey. The Astronomical Earth were developed: (a) crater morphology, (b) geo- 123 – Journal, , 1056 1085. physical anomalies, (c) evidence for shock metamor- Tholen, D. J., and Barucci, M. A., 1989. Asteroid taxonomy. In Binzel, R. P., Gehrels, T., and Matthews, M. S. (eds.), phism, and (d) the presence of meteorites or geochemical Asteroids II. Tucson: University of Arizona Press, pp. 298–315. evidence for traces of the meteoritic projectile – of which Yeomans, D., and Baalke, R., 2009. Near Earth Object Program. only (c) and (d) can provide confirming evidence. Remote Available from World Wide Web: http://neo.jpl.nasa.gov/ sensing, including morphological observations, as well programs. as geophysical studies, cannot provide confirming evi- dence – which requires the study of actual rock samples. Cross-references Impacts influenced the geological and biological evolu- tion of our own planet; the best known example is the link Albedo between the 200-km-diameter Chicxulub impact structure Asteroid Impact Asteroid Impact Mitigation in Mexico and the Cretaceous-Tertiary boundary. Under- Asteroid Impact Prediction standing impact structures, their formation processes, Torino Scale and their consequences should be of interest not only to Earth and planetary scientists, but also to society in general. ASTEROID IMPACT History of impact cratering studies In the geological sciences, it has only recently been recog- Christian Koeberl nized how important the process of impact cratering is on Natural History Museum, Vienna, Austria a planetary scale. -
1350-5 Geologist
POSITION DESCRIPTION 1. Position Number 2. Explanation (show any positions replaced) 3. Reason for Submission New Redescription Reestablishment Standardized PD Other 4. Service 5. Subject to Identical Addition (IA) Action HQ Field Yes (multiple use) No (single incumbent) 6. Position Specifications 7. Financial Statement Required 10. Position Sensitivity and Risk Designation Subject to Random Drug Testing Yes No Executive Personnel-OGE-278 Non-Sensitive Employment and Financial Interest-OGE-450 Non-Sensitive: Low-Risk Subject to Medical Standards/Surveillance Yes No None required Public Trust Telework Suitable Yes No 8. Miscellaneous 9. Full Performance Level Non-Sensitive: Moderate-Risk Fire Position Yes No Functional Code: -- Pay Plan: Non-Sensitive: High-Risk Law Enforcement Position Yes No BUS: - - Grade: National Security 11. Position is 12. Position Status Noncritical-Sensitive: Moderate-Risk Competitive SES Noncritical-Sensitive: High-Risk 2-Supervisory Excepted (specify in remarks) SL/ST Critical-Sensitive: High-Risk 4-Supervisor (CSRA) 13. Duty Station Special Sensitive: High-Risk 5-Management Official 6-Leader: Type I 14. Employing Office Location 15. Fair Labor Standards Act Exempt Nonexempt 7-Leader: Type II 16. Cybersecurity Code 17. Competitive Area Code: 8-Non-Supervisory #1: #2: - - #3: - - Competitive Level Code: 18. Classified/Graded by Official Title of Position Pay Plan Occupational Code Grade Initial Date a. Department, Bureau, or Office b. Second Level Review -- -- 19. Organizational Title of Position (if different from, or in addition to, official title) 20. Name of Employee (if vacant, specify) 21. Department, Agency, or Establishment c. Third Subdivision U.S. Department of the Interior a. Bureau/First Subdivision d. -
Hawaii Volcanoes National Park Geologic Resources Inventory Report
National Park Service U.S. Department of the Interior Natural Resource Program Center Hawai‘i Volcanoes National Park Geologic Resources Inventory Report Natural Resource Report NPS/NRPC/GRD/NRR—2009/163 THIS PAGE: Geologists have lloongng been monimonittoorriing the volcanoes of Hawai‘i Volcanoes National Park. Here lalava cascades durduriingng the 1969-1971 Mauna Ulu eruption of Kīlauea VolVolcano. NotNotee the Mauna Ulu fountountaiain in the background. U.S. Geologiogicalcal SurSurvveyey PhotPhotoo by J. B. Judd (12/30/1969). ON THE COVER: ContContiinuouslnuouslyy eruptuptiingng since 1983, Kīllaueaauea Volcano contcontiinues to shapshapee Hawai‘Hawai‘i VoVollccanoes NatiNationalonal ParkPark.. Photo courtesy Lisa Venture/UniversiUniversitty of Cincinnati. Hawai‘i Volcanoes National Park Geologic Resources Inventory Report Natural Resource Report NPS/NRPC/GRD/NRR—2009/163 Geologic Resources Division Natural Resource Program Center P.O. Box 25287 Denver, Colorado 80225 December 2009 U.S. Department of the Interior National Park Service Natural Resource Program Center Denver, Colorado The National Park Service, Natural Resource Program Center publishes a range of reports that address natural resource topics of interest and applicability to a broad audience in the National Park Service and others in natural resource management, including scientists, conservation and environmental constituencies, and the public. The Natural Resource Report Series is used to disseminate high-priority, current natural resource management information with managerial application. The series targets a general, diverse audience, and may contain NPS policy considerations or address sensitive issues of management applicability. All manuscripts in the series receive the appropriate level of peer review to ensure that the information is scientifically credible, technically accurate, appropriately written for the intended audience, and designed and published in a professional manner. -
Poroelastic Responses of Confined Aquifers to Subsurface Strain And
Solid Earth, 6, 1207–1229, 2015 www.solid-earth.net/6/1207/2015/ doi:10.5194/se-6-1207-2015 © Author(s) 2015. CC Attribution 3.0 License. Poroelastic responses of confined aquifers to subsurface strain and their use for volcano monitoring K. Strehlow, J. H. Gottsmann, and A. C. Rust School of Earth Sciences, University of Bristol, Wills Memorial Building, Bristol BS8 1RJ, UK Correspondence to: K. Strehlow ([email protected]) Received: 11 May 2015 – Published in Solid Earth Discuss.: 9 June 2015 Revised: 18 September 2015 – Accepted: 21 October 2015 – Published: 10 November 2015 Abstract. Well water level changes associated with mag- aquifer and are commonly neglected in analytical models. matic unrest can be interpreted as a result of pore pressure These findings highlight the need for numerical models for changes in the aquifer due to crustal deformation, and so the interpretation of observed well level signals. However, could provide constraints on the subsurface processes caus- simulated water table changes do indeed mirror volumetric ing this strain. We use finite element analysis to demonstrate strain, and wells are therefore a valuable addition to monitor- the response of aquifers to volumetric strain induced by pres- ing systems that could provide important insights into pre- surized magma reservoirs. Two different aquifers are invoked eruptive dynamics. – an unconsolidated pyroclastic deposit and a vesicular lava flow – and embedded in an impermeable crust, overlying a magma chamber. The time-dependent, fully coupled models simulate crustal deformation accompanying chamber pres- 1 Introduction surization and the resulting hydraulic head changes as well as flow through the porous aquifer, i.e. -
GEOLOGY What Can I Do with This Major?
GEOLOGY What can I do with this major? AREAS EMPLOYERS STRATEGIES Some employment areas follow. Many geolo- gists specialize at the graduate level. ENERGY (Oil, Coal, Gas, Other Energy Sources) Stratigraphy Petroleum industry including oil and gas explora- Geologists working in the area of energy use vari- Sedimentology tion, production, storage and waste disposal ous methods to determine where energy sources are Structural Geology facilities accumulated. They may pursue work tasks including Geophysics Coal industry including mining exploration, grade exploration, well site operations and mudlogging. Geochemistry assessment and waste disposal Seek knowledge in engineering to aid communication, Economic Geology Federal government agencies: as geologists often work closely with engineers. Geomorphology National Labs Coursework in geophysics is also advantageous Paleontology Department of Energy for this field. Fossil Energy Bureau of Land Management Gain experience with computer modeling and Global Hydrogeology Geologic Survey Positioning System (GPS). Both are used to State government locate deposits. Consulting firms Many geologists in this area of expertise work with oil Well services and drilling companies and gas and may work in the geographic areas Oil field machinery and supply companies where deposits are found including offshore sites and in overseas oil-producing countries. This industry is subject to fluctuations, so be prepared to work on a contract basis. Develop excellent writing skills to publish reports and to solicit grants from government, industry and private foundations. Obtain leadership experience through campus organi- zations and work experiences for project man- agement positions. (Geology, Page 2) AREAS EMPLOYERS STRATEGIES ENVIRONMENTAL GEOLOGY Sedimentology Federal government agencies: Geologists in this category may focus on studying, Hydrogeology National Labs protecting and reclaiming the environment. -
A Ballistics Analysis of the Deep Impact Ejecta Plume: Determining Comet Tempel 1’S Gravity, Mass, and Density
Icarus 190 (2007) 357–390 www.elsevier.com/locate/icarus A ballistics analysis of the Deep Impact ejecta plume: Determining Comet Tempel 1’s gravity, mass, and density James E. Richardson a,∗,H.JayMeloshb, Carey M. Lisse c, Brian Carcich d a Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA b Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721-0092, USA c Planetary Exploration Group, Space Department, Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA d Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA Received 31 March 2006; revised 8 August 2007 Available online 15 August 2007 Abstract − In July of 2005, the Deep Impact mission collided a 366 kg impactor with the nucleus of Comet 9P/Tempel 1, at a closing speed of 10.2 km s 1. In this work, we develop a first-order, three-dimensional, forward model of the ejecta plume behavior resulting from this cratering event, and then adjust the model parameters to match the flyby-spacecraft observations of the actual ejecta plume, image by image. This modeling exercise indicates Deep Impact to have been a reasonably “well-behaved” oblique impact, in which the impactor–spacecraft apparently struck a small, westward-facing slope of roughly 1/3–1/2 the size of the final crater produced (determined from initial ejecta plume geometry), and possessing an effective strength of not more than Y¯ = 1–10 kPa. The resulting ejecta plume followed well-established scaling relationships for cratering in a medium-to-high porosity target, consistent with a transient crater of not more than 85–140 m diameter, formed in not more than 250–550 s, for the case of Y¯ = 0 Pa (gravity-dominated cratering); and not less than 22–26 m diameter, formed in not less than 1–3 s, for the case of Y¯ = 10 kPa (strength-dominated cratering). -
Sulphur Works Is Believed to Have Been the Main Vent for Mount Tehama, a Stratovolcano That Started Erupting About 600,000 Years Ago
Junior Park Explorer Lassen Volcanic National Park Mystery of Mount Tehama Imagine you are standing almost a mile deep inside a stratovolcano. Well, 400,000 years ago you would have been! The area around Sulphur Works is believed to have been the main vent for Mount Tehama, a stratovolcano that started erupting about 600,000 years ago. By 400,000 years ago, it had reached its full height of 11,500 feet. Look around you in a full circle. Can you spot the mountains pictured below? They are all remnants (left over bits) of Mount Tehama. Remnant 1 – Brokeoff Mountain Remnant 2 – Mount Diller Remnant 3 – Pilot Pinnacle Remnant – Mount Conard Activity 1 - See if you can find these remnants on your park map. Trace a circle from one mountain to the next to outline the footprint of Mount Tehama. Be sure to include Little Hot Springs Valley inside the footprint. Activity 2 - Use the diagram on the next page to reconstruct Mount Tehama. Connect point A to point B, A to C, A to D, A to E, & A to F, individually. Can you see Mount Tehama in your imagination? Color in the mountain if you wish. Activity 3 - Another way to reconstruct Mount Tehama is as a view from down in the Sacramento Valley. On the next page, check out how the skyline of Lassen Volcanic National Park looks today, looking east from near Redding. Can you draw what the skyline might have looked like when Mount Tehama was at its full height of 11,500 feet, 400,000 years ago? Use the graph on the next page. -
Impact Cratering
6 Impact cratering The dominant surface features of the Moon are approximately circular depressions, which may be designated by the general term craters … Solution of the origin of the lunar craters is fundamental to the unravel- ing of the history of the Moon and may shed much light on the history of the terrestrial planets as well. E. M. Shoemaker (1962) Impact craters are the dominant landform on the surface of the Moon, Mercury, and many satellites of the giant planets in the outer Solar System. The southern hemisphere of Mars is heavily affected by impact cratering. From a planetary perspective, the rarity or absence of impact craters on a planet’s surface is the exceptional state, one that needs further explanation, such as on the Earth, Io, or Europa. The process of impact cratering has touched every aspect of planetary evolution, from planetary accretion out of dust or planetesimals, to the course of biological evolution. The importance of impact cratering has been recognized only recently. E. M. Shoemaker (1928–1997), a geologist, was one of the irst to recognize the importance of this process and a major contributor to its elucidation. A few older geologists still resist the notion that important changes in the Earth’s structure and history are the consequences of extraterres- trial impact events. The decades of lunar and planetary exploration since 1970 have, how- ever, brought a new perspective into view, one in which it is clear that high-velocity impacts have, at one time or another, affected nearly every atom that is part of our planetary system. -
East-African Rift System Geological Settings of Geothermal Resources and Their Prospects
Presented at Short Course III on Exploration for Geothermal Resources, organized by UNU-GTP and KenGen, at Lake Naivasha, Kenya, October 24 - November 17, 2008. GEOTHERMAL TRAINING PROGRAMME Kenya Electricity Generating Co., Ltd. EAST-AFRICAN RIFT SYSTEM GEOLOGICAL SETTINGS OF GEOTHERMAL RESOURCES AND THEIR PROSPECTS Kristján Saemundsson ISOR – Iceland GeoSurvey Grensásvegur 9 108 Reykjavík ICELAND [email protected] 1. INTRODUCTION The geothermal areas of the East-African Rift System are not all of the same type. Even though related to the Rift the geological settings are different. Some are volcanic, others are not. Parts of the rift zones are highly volcanic but large segments of them are sediment or lake filled grabens. Extreme cases are also found where rift-related fractures produce permeability in basement rocks. In retrospect it may be useful to point out the differences and likely resource characteristics. Below seven types are described, and in which countries they occur as the dominant type. Three of those types are genuine high-temperature geothermal resources. Two may be accessible only in the off flow zone of high-temperature geothermal fields. One is of the sedimentary basin type resource of low to medium temperature, and one other of the low-temperature type is related to fractured basement rock. 2. OFF RIFT VOLCANOES Eritrea (Alid), Yemen (Al Lisi): Volcanic HT-systems suitable for back pressure turbines Main resource at rather high ground (Eritrea) Off flow probably present, perhaps suitable for binary In case of off flow temperature inversion likely Research methods: Geology/volcanology, hydrology, geochemistry, TEM/MT, airborne magnetics, seismicity, gravity 3. -
Journal of Volcanology and Geothermal Research
JOURNAL OF VOLCANOLOGY AND GEOTHERMAL RESEARCH An International Journal on the Geophysical, Geochemical, Petrological, Economic and Environmental Aspects of Volcanology and Geothermal Research AUTHOR INFORMATION PACK TABLE OF CONTENTS XXX . • Description p.1 • Audience p.1 • Impact Factor p.1 • Abstracting and Indexing p.2 • Editorial Board p.2 • Guide for Authors p.4 ISSN: 0377-0273 DESCRIPTION . An international research journal with focus on volcanic and geothermal processes and their impact on the environment and society. Submission of papers covering the following aspects of volcanology and geothermal research are encouraged: (1) Geological aspects of volcanic systems: volcano stratigraphy, structure and tectonic influence; eruptive history; evolution of volcanic landforms; eruption style and progress; dispersal patterns of lava and ash; analysis of real-time eruption observations. (2) Geochemical and petrological aspects of volcanic rocks: magma genesis and evolution; crystallization; volatile compositions, solubility, and degassing; volcanic petrography and textural analysis. (3) Hydrology, geochemistry and measurement of volcanic and hydrothermal fluids: volcanic gas emissions; fumaroles and springs; crater lakes; hydrothermal mineralization. (4) Geophysical aspects of volcanic systems: physical properties of volcanic rocks and magmas; heat flow studies; volcano seismology, geodesy and remote sensing. (5) Computational modeling and experimental simulation of magmatic and hydrothermal processes: eruption dynamics; magma transport and storage; plume dynamics and ash dispersal; lava flow dynamics; hydrothermal fluid flow; thermodynamics of aqueous fluids and melts. (6) Volcano hazard and risk research: hazard zonation methodology, development of forecasting tools; assessment techniques for vulnerability and impact. The journal does not accept geothermal research papers not related to volcanism. AUDIENCE . Volcanologists, petrologists, geochemists, geothermics. -
Depth of Magma Chamber Determined by Experimental Petrologic Methods
DEPTH OF MAGMA CHAMBER DETERMINED BY EXPERIMENTAL PETROLOGIC METHODS Akihiko Tomiya Geological Survey of Japan, 1-1-3, Higashi, Tsukuba, Ibaraki, Japan Keywords: magma chamber, experimental petrology, Usu magma and, therefore, the composition of the residual melt, volcano, deep-seated geothermal resource that is, the evolved magma. ABSTRACT Thermodynamic conditions of a magma chamber can be estimated using petrographic information (e.g., compositions Depth of magma chamber (or young intrusive body) is one of and modal fractions of phenocrysts and groundmass) from a the most important parameters that determine the thermal representative rock erupted from the chamber. In order to structure and the circulation pattern of fluid around a estimate the pressure of magma chamber, the following geothermal area. The depth is also important when we methods are generally used; (1) geobarometer, (2) water recognize the magma chamber as a deep-seated geothermal content, and (3) melting experiment. One of the examples of resource itself. Here, we introduce an experimental petrologic the first method is an amphibole geobarometer (e.g., method for determining the depth of magma chamber. There Hammarstrom and Zen, 1986) where pressure is estimated are several methods in order to determine the depth (pressure) from the aluminum content of the amphibole crystallized from of a magma chamber. Among them, a melting experiment for the magma. This method, however, is difficult to apply to the rock erupted from the magma chamber is the most reliable natural magma because the geobarometer should be applied method. The method consists of the following procedure: (1) only when the mineral assemblage of the magma is the same as Select a sample (volcanic rock) which is representative of that of experimental products for which the geobarometer was magma in the chamber; (2) Give a petrographic description of calibrated.