Basaltic-Volcano Systems
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Geologic Storage Formation Classification: Understanding Its Importance and Impacts on CCS Opportunities in the United States
BEST PRACTICES for: Geologic Storage Formation Classification: Understanding Its Importance and Impacts on CCS Opportunities in the United States First Edition Disclaimer This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference therein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed therein do not necessarily state or reflect those of the United States Government or any agency thereof. Cover Photos—Credits for images shown on the cover are noted with the corresponding figures within this document. Geologic Storage Formation Classification: Understanding Its Importance and Impacts on CCS Opportunities in the United States September 2010 National Energy Technology Laboratory www.netl.doe.gov DOE/NETL-2010/1420 Table of Contents Table of Contents 5 Table of Contents Executive Summary ____________________________________________________________________________ 10 1.0 Introduction and Background -
Lunar and Planetary Science XXXII (2001) 1509.Pdf
Lunar and Planetary Science XXXII (2001) 1509.pdf TERRESTRIAL ANALOGS FOR MARTIAN VOLCANIC FEATURES SEEN IN MOC IMAGES. L. Keszthelyi and A. S. McEwen, Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona 85721 Introduction: Many of the Mars Orbital Camera lavas. For example, if basaltic lavas are erupted after images include volcanic features whose initially inter- significant cooling and crystallization, their rheology pretation is best made by examining terrestrial analogs. will mimic more evolved lavas [3]. But relatively Channel-fed aa, rubbly pahoehoe sheets, inflated pa- evolved compositions should be expected to cap the hoehoe, and lava tubes have now been observed and Martian shield volcanoes, just as evolved, alkalic lavas evidence for voluminous and widespread mafic pyro- cap the Hawaiian shield volcanoes [4]. Such lavas are clastics continues to mount. After these initial qualita- the natural products of a cooling mantle magma source tive interpretations are made, more quantitative mod- region or a crystallizing basaltic magma chamber. The eling can be effectively applied in future studies. presence of such lavas is not evidence for arc-type vol- Shield volcanoes: The five major shield volcanoes canism. are the most prominent volcanic features on Mars. While highly speculative at this point, the observa- Examination of ~200 MOC images of the Tharsis vol- tions to date suggest that the Martian shield volcanoes canoes, Olympus Mons, and Elysium Mons showed a may be dominantly basaltic but are capped by a layer terrain largely mantled by various types of cover. This of more evolved lavas. Moderate explosive activity is makes interpretation of the volcanic features challeng- usually associated with the eruption of such evolved ing. -
Temporal Evolution of the Barombi Mbo Maar, a Polygenetic Maar-Diatreme Volcano of the Cameroon Volcanic Line*
International Journal of Geosciences, 2014, 5, 1315-1323 Published Online October 2014 in SciRes. http://www.scirp.org/journal/ijg http://dx.doi.org/10.4236/ijg.2014.511108 Temporal Evolution of the Barombi Mbo Maar, a Polygenetic Maar-Diatreme Volcano of the Cameroon Volcanic Line* Boris Chako Tchamabé1#, Takeshi Ohba1, Issa1, Seigo Ooki1, Dieudonné Youmen2, Sebastien Owona2, Gregory Tanyileke3, Joseph Victor Hell3 1Laboratory of Volcanology and Geochemistry, Department of Chemistry, Tokai University, Tokyo, Japan 2Department of Earth Science, Faculty of Sciences, University of Douala, Douala, Cameroon 3Institute of Mining and Geological Research (IRGM), Yaoundé, Cameroon Email: #[email protected] Received 1 August 2014; revised 25 August 2014; accepted 15 September 2014 Copyright © 2014 by authors and Scientific Research Publishing Inc. This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/ Abstract The Barombi Mbo Maar (BMM), which is the largest maar in Cameroon, possesses about 126 m- thick well-preserved pyroclastic deposits sequence in which two successive paleosoil beds have been identified. The maar was thought to have been active a million years ago. However, layers stratigraphically separated by the identified paleosoils have been dated to shed lights on its age and to reconstruct the chronology of its past activity. The results showed that the BMM formed through three eruptive cycles: the first ~0.51 Ma ago, the second at ~0.2 Ma and the third ~0.08 Ma B.P. The ages indicate that the BMM maar-forming eruptions were younger than a million years. The findings also suggested that the maar is polygenetic. -
Abandonment of the Name Hartford Hill Rhyolitetuff and Adoption of New Formation Names for Middle Tertiary Ash-Flow Tuffs in the Carson City- Silver City Area, Nevada
Abandonment of the Name Hartford Hill RhyoliteTuff and Adoption of New Formation Names for Middle Tertiary Ash-Flow Tuffs in the Carson City- Silver City Area, Nevada GEOLOGICAL SURVEY BULLETIN 1457-D Abandonment of the Name Hartford Hill Rhyolite Tuff and Adoption of New Formation Names for Middle Tertiary Ash-Flow Tuffs in the Carson City- Silver City Area, Nevada By EDWARD C. BINGLER CONTRIBUTIONS TO STRATIGRAPHY GEOLOGICAL SURVEY BULLETIN 1457-D UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1978 UNITED STATES DEPARTMENT OF THE INTERIOR CECIL D. ANDRUS, Secretary GEOLOGICAL SURVEY H. William Menard, Director Dingier, Edward C. Abandonment of the name Hartford Hill rhyolite tuff and adoption of new formation names for middle Tertiary ash-flow tuffs in the Carson City - Silver City area, Nevada (Contributions to stratigraphy) Geological Survey Bulletin 1457-D Supt. of Docs. No.: I 19.3: 1457-D Bibliography: p. D19 I. Geology, Stratigraphic-Tertiary. 2. Volcanic ash, tuff, etc.-Nevada- Carson City region. 3. Geology-Nevada-Carson City region. I. Title. II. Series. HI. Series: United States. Geological Survey. Bulletin 1457-D. QE75.B9 no. 1457-D [QE691] 557.3'08s [551.7'8] 78-606063 For sale by the Superintendent of Documents, U. S. Government Printing Office Washington, D. C. 20402 Stock Number 024-001-03124-8 CONTENTS Page Abstract___________________________________ Dl Introduction ______________________________________ 1 Acknowledgments ________________________________ 5 Ash-flow stratigraphy in the Carson City-Silver City area ___________ 7 Mickey Pass Tuff ________________________________ 7 Lenihan Canyon Tuff _____________________________ 8 Nine Hill Tuff _______________________________ 11 Eureka Canyon Tuff ______________________________ 14 Dacitetuff __________________________________ 16 Rhyolite tuff and augite rhyodacite tuff ___________________ 16 Santiago Canyon Tuff _____________________________ 17 References cited _____________________________^_____ 19 ILLUSTRATIONS Page FIGURE 1. -
Geology of the Nairobi Region, Kenya
% % % % % % % % %% %% %% %% %% %% %% % GEOLOGIC HISTORY % %% %% % % Legend %% %% %% %% %% %% %% % % % % % % HOLOCENE: %% % Pl-mv Pka %%% Sediments Mt Margaret U. Kerichwa Tuffs % % % % %% %% % Longonot (0.2 - 400 ka): trachyte stratovolcano and associated deposits. Materials exposed in this map % %% %% %% %% %% %% % section are comprised of the Longonot Ash Member (3.3 ka) and Lower Trachyte (5.6-3.3 ka). The % Pka' % % % % % % L. Kerichwa Tuff % % % % % % Alluvial fan Pleistocene: Calabrian % % % % % % % Geo% lo% gy of the Nairobi Region, Kenya % trachyte lavas were related to cone building, and the airfall tuffs were produced by summit crater formation % % % % % % % % % % % % % % % % % Pna % % % % %% % (Clarke et al. 1990). % % % % % % Pl-tb % % Narok Agglomerate % % % % % Kedong Lake Sediments Tepesi Basalt % % % % % % % % % % % % % % % % %% % % % 37.0 °E % % % % 36.5 °E % % % % For area to North see: Geology of the Kijabe Area, KGS Report 67 %% % % % Pnt %% % PLEISTOCENE: % % %% % % % Pl-kl %% % % Nairobi Trachyte % %% % -1.0 ° % % % % -1.0 ° Lacustrine Sediments % % % % % % % % Pleistocene: Gelasian % % % % % Kedong Valley Tuff (20-40 ka): trachytic ignimbrites and associated fall deposits created by caldera % 0 % 1800 % % ? % % % 0 0 % % % 0 % % % % % 0 % 0 8 % % % % % 4 % 4 Pkt % formation at Longonot. There are at least 5 ignimbrite units, each with a red-brown weathered top. In 1 % % % % 2 % 2 % % Kiambu Trachyte % Pl-lv % % % % % % % % % % %% % % Limuru Pantellerite % % % % some regions the pyroclastic glass and pumice has been -
Source to Surface Model of Monogenetic Volcanism: a Critical Review
Downloaded from http://sp.lyellcollection.org/ by guest on September 28, 2021 Source to surface model of monogenetic volcanism: a critical review I. E. M. SMITH1 &K.NE´ METH2* 1School of Environment, University of Auckland, Auckland, New Zealand 2Volcanic Risk Solutions, Massey University, Palmerston North 4442, New Zealand *Correspondence: [email protected] Abstract: Small-scale volcanic systems are the most widespread type of volcanism on Earth and occur in all of the main tectonic settings. Most commonly, these systems erupt basaltic magmas within a wide compositional range from strongly silica undersaturated to saturated and oversatu- rated; less commonly, the spectrum includes more siliceous compositions. Small-scale volcanic systems are commonly monogenetic in the sense that they are represented at the Earth’s surface by fields of small volcanoes, each the product of a temporally restricted eruption of a composition- ally distinct batch of magma, and this is in contrast to polygenetic systems characterized by rela- tively large edifices built by multiple eruptions over longer periods of time involving magmas with diverse origins. Eruption styles of small-scale volcanoes range from pyroclastic to effusive, and are strongly controlled by the relative influence of the characteristics of the magmatic system and the surface environment. Gold Open Access: This article is published under the terms of the CC-BY 3.0 license. Small-scale basaltic magmatic systems characteris- hazards associated with eruptions, and this is tically occur at the Earth’s surface as fields of small particularly true where volcanic fields are in close monogenetic volcanoes. These volcanoes are the proximity to population centres. -
Insight Into Subvolcanic Magma Plumbing Systems Wendy A
Insight into subvolcanic magma plumbing systems Wendy A. Bohrson Department of Geological Sciences, Central Washington University, 400 E. University Way, Ellensburg, Washington 98926, USA The Island of Hawaii, which is among the of CO2 inclusions (Bohrson and Clague, 1988; best-studied volcanic islands on Earth, provides Roedder, 1965). Rare gabbro from layer 3 of the lush ground for debates in volcanology that oceanic crust has also been identifi ed (Clague, focus on how magmatic systems evolve in space 1987a). Thus, a likely location for the deeper and time. Hawaiian volcanoes evolve through chamber is at the base of the oceanic crust. The four eruptive stages that are characterized by relatively low magma supply associated with distinct composition, magma supply rate, and the pre-shield and rejuvenated stages appar- Shallow magma plumbing degree of mantle melting (e.g., Clague, 1987a, ently precludes any persistent crustal magma system 1987b, and references therein). The pre-shield plumbing system; spinel lherzolite and garnet (shield stage) stage, fi rst identifi ed on Loihi Seamount (Moore pyroxenite xenoliths originate in the mantle et al., 1982), erupts mostly alkalic basalt and based on geobarometry, compositional charac- Deep basanite that refl ect a small magma supply and teristics, and other constraints (e.g., Frey and magma plumbing derive from relatively small degrees of mantle Roden, 1987; Frey, 1982). system melting. During the shield stage, tholeiitic Although rare on Hawaiian volcanoes, the (shield and post-shield stage) basalt (like that currently erupted at Kilauea more evolved compositions also provide insight and Mauna Loa) dominates, and refl ects com- into plumbing system dynamics. -
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. -
Ignimbrites to Batholiths Ignimbrites to Batholiths: Integrating Perspectives from Geological, Geophysical, and Geochronological Data
Ignimbrites to batholiths Ignimbrites to batholiths: Integrating perspectives from geological, geophysical, and geochronological data Peter W. Lipman1,* and Olivier Bachmann2 1U.S. Geological Survey, Mail Stop 910, Menlo Park, California 94028, USA 2Institute of Geochemistry and Petrology, ETH Zurich, CH-8092 Zürich, Switzerland ABSTRACT related intrusions cooled and solidified soon shorter. Magma-supply estimates (from ages after zircon crystallization, as magma sup- and volcano-plutonic volumes) yield focused Multistage histories of incremental accu- ply waned. Some researchers interpret these intrusion-assembly rates sufficient to gener- mulation, fractionation, and solidification results as recording pluton assembly in small ate ignimbrite-scale volumes of eruptible during construction of large subvolcanic increments that crystallized rapidly, leading magma, based on published thermal models. magma bodies that remained sufficiently to temporal disconnects between ignimbrite Mid-Tertiary processes of batholith assembly liquid to erupt are recorded by Tertiary eruption and intrusion growth. Alternatively, associated with the SRMVF caused drastic ignimbrites, source calderas, and granitoid crystallization ages of the granitic rocks chemical and physical reconstruction of the intrusions associated with large gravity lows are here inferred to record late solidifica- entire lithosphere, probably accompanied by at the Southern Rocky Mountain volcanic tion, after protracted open-system evolution asthenospheric input. field (SRMVF). Geophysical -
MEKE MAAR / Republic of Turkey 1. Name and Adress of the Compiler Of
MEKE MAAR / Republic of Turkey 1. Name and adress of the compiler of this form: Selim ERDOGAN (Hydrogeological Engineer, M.Sc) Ministry of Environment & Forestry., General Directorate of Nature Conservation & National Parks., Wetlands Division Address: Çevre ve Orman Bakanlığı, İstanbul Caddesi No: 98 Phone: 0090 312 3840510 / 3021 Fax: 0090 312 3842476 Email: [email protected] 2. Date this sheet was completed/updated 01.02.2006 3. Country: Republic of Turkey 4. Name of the Ramsar Site Meke Maar 5. Map of Site included A site map of 1:25 000 scale and providing the characteristics indicated in the Annex III of this guideline is included in this package. a) Hard Copy: YES b) Digital (electronic) Format: YES 6. Geographical Coordinates: 33038’28’’ E., 37041’10’’ N 7. General Location: Turkey is separated into 82 administrative districts. As regards area extension, Konya is the largest district of Turkey. It’s also the 4th biggest city with approximately 2 million habitants. Meke Maar is situated in Konya district. The distance of it to the center of the city is approximately 101 km (towards the south of the district). The subdivision in which the Meke Maar is located, is Karapınar and it’s 8 km far from the site. 8. Elevation: 1004 m (minimum – the elevation of the plain on which the maar is situated) 1280 m (maximum – the elevation of the crater of the volcano) 9. Area: 202 hectares 10. Overview: Meke Maar is a volcanic system which contains typically a volcanic rock mass and a crater lake up above. However the system differs from other volcanic systems with its caldera lake surrounding the volcanic mass (See pictures in Annex 2). -
31 a Preliminary Study Of
31 A PRELIMINARY STUDY OF THE: TERTIARY VOLCANIC AND SEDIMENTARY ROCKS, GÜMELE, ESKİŞEHİR Eskişehir, Gümele Çevresindeki Tersiyer Volkanik ve Sedimanter Kayaçlarda Bir Ön Çalışma Taylan Lünel Middle East Technical University, Department of Geological Engineering Ankara ÖZ. — Seyitgazi-Eskişehir antiklinoriumu'nun çok fazla deforme olmuş ve metamorfizmaya uğramış kayaçlarının kuzey-kuzeybatısında bulunan sedimanter ve volkanik kayaçlar incelenmiştir. Karasal ve gölsel fasiyesde meydana gelen Tersi- yer sedimanter kayaçlar Güney Eskişehir küvetinde olunmuşlardır. Karasal fasiye- si meydana getiren kayaç birimlerini kaba kumtaşları, kumtaşları, bitki kalıntıları ihtiva eden kil ve marnlar ve serpantinit blokları taşıyan bazal konglomerası teşkil etmektedir. Gölsel fasiyes ise genellikle killi ve tüflü kalkerler, kalkerler, marnlar, kon- glomeralar ve tüflerden meydana gelmiştir. Küvetteki en eski sedimanlar ve piroklas- tikler Alt Miosen'de oluşmuşlardır. Yataya yakın konumlanmış bazik-intermediyar lav akıntıları Pliosen yaşlı olup Altüst Neojen sedimantasyon kesikliğinde meyda- na gelmiştir. Üst Neojen sedimanter kayaçları intermediyar-basaltik volkaniklerin üzerinde ince bandlar şeklinde bulunurlar. Bu birim marn ve kalkerlerden meyda- na gelmiştir. Alt Miosen’de asid volkanik faaliyetler neticesinde meydana gelen sil- lar (unweldd tuffs) oligomikt konglomeralardan evvel teşekkül etmiştir. Bu volkanik aktitivite muhtemelen kesikli ve kısıtlı olarak devam etmiş ve tüflü kalkerleri mey- dana getirmiştir. Pliosen yaşlı bazik-intermediyar -
Hawaiian Volcanoes: from Source to Surface Site Waikolao, Hawaii 20 - 24 August 2012
AGU Chapman Conference on Hawaiian Volcanoes: From Source to Surface Site Waikolao, Hawaii 20 - 24 August 2012 Conveners Michael Poland, USGS – Hawaiian Volcano Observatory, USA Paul Okubo, USGS – Hawaiian Volcano Observatory, USA Ken Hon, University of Hawai'i at Hilo, USA Program Committee Rebecca Carey, University of California, Berkeley, USA Simon Carn, Michigan Technological University, USA Valerie Cayol, Obs. de Physique du Globe de Clermont-Ferrand Helge Gonnermann, Rice University, USA Scott Rowland, SOEST, University of Hawai'i at M noa, USA Financial Support 2 AGU Chapman Conference on Hawaiian Volcanoes: From Source to Surface Site Meeting At A Glance Sunday, 19 August 2012 1600h – 1700h Welcome Reception 1700h – 1800h Introduction and Highlights of Kilauea’s Recent Eruption Activity Monday, 20 August 2012 0830h – 0900h Welcome and Logistics 0900h – 0945h Introduction – Hawaiian Volcano Observatory: Its First 100 Years of Advancing Volcanism 0945h – 1215h Magma Origin and Ascent I 1030h – 1045h Coffee Break 1215h – 1330h Lunch on Your Own 1330h – 1430h Magma Origin and Ascent II 1430h – 1445h Coffee Break 1445h – 1600h Magma Origin and Ascent Breakout Sessions I, II, III, IV, and V 1600h – 1645h Magma Origin and Ascent III 1645h – 1900h Poster Session Tuesday, 21 August 2012 0900h – 1215h Magma Storage and Island Evolution I 1215h – 1330h Lunch on Your Own 1330h – 1445h Magma Storage and Island Evolution II 1445h – 1600h Magma Storage and Island Evolution Breakout Sessions I, II, III, IV, and V 1600h – 1645h Magma Storage