Modelling Surtseyan Ejecta
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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. -
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). -
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). -
Explosive Subaqueous Eruptions: the Influence of Volcanic Jets on Eruption Dynamics and Tephra Dispersal in Underwater Eruptions
EXPLOSIVE SUBAQUEOUS ERUPTIONS: THE INFLUENCE OF VOLCANIC JETS ON ERUPTION DYNAMICS AND TEPHRA DISPERSAL IN UNDERWATER ERUPTIONS by RYAN CAIN CAHALAN A DISSERTATION Presented to the Department of Earth ScIences and the Graduate School of the UniversIty of Oregon In partIaL fulfiLLment of the requirements for the degree of Doctor of PhiLosophy December 2020 DISSERTATION APPROVAL PAGE Student: Ryan CaIn CahaLan Title: ExplosIve Subaqueous EruptIons: The Influence of Volcanic Jets on EruptIon DynamIcs and Tephra DIspersaL In Underwater EruptIons This dissertatIon has been accepted and approved in partIaL fulfiLLment of the requirements for the Doctor of PhiLosophy degree in the Department of Earth ScIences by: Dr. Josef Dufek ChaIrperson Dr. Thomas GIachettI Core Member Dr. Paul WaLLace Core Member Dr. KeLLy Sutherland InstItutIonaL RepresentatIve and Kate Mondloch Interim VIce Provost and Dean of the Graduate School OriginaL approvaL sIgnatures are on fiLe wIth the UniversIty of Oregon Graduate School. Degree awarded December 2020 II © 2020 Ryan Cain Cahalan III DISSERTATION ABSTRACT Ryan CaIn CahaLan Doctor of PhiLosophy Department of Earth ScIences December 2020 Title: ExplosIve Subaqueous EruptIons: The Influence of Volcanic Jets on EruptIon DynamIcs and Tephra DIspersaL In Underwater EruptIons Subaqueous eruptIons are often overlooked in hazard consIderatIons though they represent sIgnificant hazards to shipping, coastLInes, and in some cases, aIrcraft. In explosIve subaqueous eruptIons, volcanic jets transport fragmented tephra and exsolved gases from the conduit into the water column. Upon eruptIon the volcanic jet mIxes wIth seawater and rapidly cools. This mIxing and assocIated heat transfer ultImateLy determInes whether steam present in the jet wILL completeLy condense or rise to breach the sea surface and become a subaeriaL hazard. -
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. -
Pyroclastic Deposits I: Pyroclastic Fall Deposits
Pyroclastic Deposits I: Pyroclastic Fall Deposits EAS 458 Volcanology Introduction . We have seen that physics is useful in understanding volcanic processes, but physical models must be constrained by and tested against observation. We have 1925 years of historic observations of Vesuvius (79 AD to present) . Far less for most other volcanoes . In all, a very, very small fraction of eruptions . Most descriptions are of limited use . Observations about volcanic processes must depend primarily on geologic observations . The geologic record of volcanic eruptions consists primarily of the deposits produced by them. 1 Pyroclastic Deposits . Three types of pyroclastic deposits . Fall Deposits . Fallout from an eruptive column . Flow Deposits . Produced by pyroclastic flows . Surge Deposits . Often associated with flow deposits . Associated with explosive events, such as phreatomagmatic explosions Pyroclastic Deposits . Characteristics . Fall Deposits . Mantle topography . Parallel bedding . Well sorted . Often graded . Flow Deposits . Topographically constrained . Poorly sorted . Often graded . Surge Deposits . Partially topographically constrained . Cross bedding characteristic . Intermediate sorting . Often graded 2 Pyroclastic Fall Deposits . General term: tephra . Types . Scoria (mafic , larger size) . Pumice (silicic, larger size) . Ash (fine grained) Fall Deposits: Bedding . Except very near vent, “fall” particles settle vertically. Therefore, extensive deposits (such as those of Plinian eruptions) will be equally thick at any given distance and direction from the vent. Hence, they mantle topography . (Scoria cones produced by Hawaiian and Strobolian eruptions obviously don’t mantle topography) 3 Fall Deposits: Sorting . The distance a particle will travel from the vent depends on: . Ejection velocity . Particle size . For conditions at any particular time and place, particles of a small range of sizes will fall out. -
Mt. Pico, Pico Island, Azores, October 2012 (Photo: Hans Johansson)
Cover photograph: Mt. Pico, Pico Island, Azores, October 2012 (photo: Hans Johansson) Abstract The Azores is situated in the North Atlantic Ocean and is one of the most active volcanic regions in the Northern Hemisphere. The volcanic history of the islands is fairly well known and several explosive trachytic eruptions have been reported but the geo‐ chemical compositions of the glass component of the tephra as well as the dispersal of tephras to distal areas are less well known. The purpose of this study is twofold: (1) to present major element geochemistry of the glass component from several historic as well as prehistoric tephras, including the trachybasaltic Capelinhos AD 1957‐58 eruption on the island of Faial, and the trachytic explosive eruptions of Sete Cidades (c. AD 1440), Fogo A (c. 5000 BP), Fogo AD 1563 and Furnas AD 1630 on the island of São Miguel; (2) to present a refined tephrostratigraphy for the island of Pico. Analyses of major element geochemistry suggest that tephras from the three active stratovolcanoes on São Miguel can be separated in biplots showing e.g. FeOtot vs.TiO2 and FeOtot vs. CaO. The tephrostratigraphy of Caveiro bog on the island of Pico is based on a radiocarbon dated core with eight tephra layers extending back to c. 7000 BP. All tephras are of trachybasaltic/basaltic trachyandesitic composition except the oldest layer, which is of basanitic composition. An attempt was made to correlate the tephra record of Caveiro bog with the previously investigated Lake Caveiro. A tephra‐based correlation between the Caveiro bog and Lake Caveiro is not straightforward and only three tephras in Caveiro bog can possibly be correlated with tephras found in the sediments of Lake Caveiro. -
ETD Template
Syn-eruptive incision of Koko Crater, Oahu, Hawaii by condensed steam and hot cohesive debris flows: a re-interpretation of the type locality of “surge-eroded U-shaped channels” by Jessica Keri Bluth B.S., State University of New York at Binghamton, 2001 Submitted to the Graduate Faculty of Arts and Sciences in partial fulfillment of the requirements for the degree of Master of Science University of Pittsburgh 2004 UNIVERSITY OF PITTSBURGH FACULTY OF ARTS AND SCIENCES This dissertation was presented by Jessica Keri Bluth It was defended on June 25, 2004 and approved by Dr. Michael Ramsey Dr. Charles Jones Dr. Ian Skilling Committee Chairperson ii Syn-eruptive incision of Koko Crater, Oahu by condensed steam and hot cohesive debris flows: a re-interpretation of the type locality of “surge-eroded U-shaped channels” Jessica K. Bluth, M.S. Department of Geology and Planetary Science University of Pittsburgh, 2004 Phreatomagmatic fall, low-concentration PDC deposits and remobilized equivalents dominate the products of craters (tuff cones/rings) of Koko fissure, south-east Oahu. At Koko crater, Fisher (1977) described “U-shaped” channels, which he interpreted as due to erosion by low-concentration PDCs (surges), with minor modification by stream and debris flows. Similar channels on tuff cones and rings elsewhere in the world have been interpreted as “surge-eroded” by subsequent authors. However, no evidence for erosion by PDCs was observed during recent fieldwork, which suggested rather the following model. An important observation is that initial incision is always correlated with the emplacement of vesiculated ash layers (derived from Hanauma Bay), and is only very rarely associated with other facies. -
The Quaternary Plant Fossil Record from the Volcanic Azores Archipelago (Portugal, North Atlantic Ocean): a Review
Historical Biology An International Journal of Paleobiology ISSN: 0891-2963 (Print) 1029-2381 (Online) Journal homepage: http://www.tandfonline.com/loi/ghbi20 The Quaternary plant fossil record from the volcanic Azores Archipelago (Portugal, North Atlantic Ocean): a review Carlos A. Góis-Marques, Lea de Nascimento, Miguel Menezes de Sequeira, José María Fernández-Palacios & José Madeira To cite this article: Carlos A. Góis-Marques, Lea de Nascimento, Miguel Menezes de Sequeira, José María Fernández-Palacios & José Madeira (2018): The Quaternary plant fossil record from the volcanic Azores Archipelago (Portugal, North Atlantic Ocean): a review, Historical Biology, DOI: 10.1080/08912963.2018.1444761 To link to this article: https://doi.org/10.1080/08912963.2018.1444761 Published online: 28 Feb 2018. Submit your article to this journal View related articles View Crossmark data Full Terms & Conditions of access and use can be found at http://www.tandfonline.com/action/journalInformation?journalCode=ghbi20 HISTORICAL BIOLOGY, 2018 https://doi.org/10.1080/08912963.2018.1444761 The Quaternary plant fossil record from the volcanic Azores Archipelago (Portugal, North Atlantic Ocean): a review Carlos A. Góis-Marquesa,b , Lea de Nascimentoc , Miguel Menezes de Sequeirab,d , José María Fernández-Palaciosc and José Madeiraa aLaboratório Associado, Departamento de Geologia, Faculdade de Ciências da Universidade de Lisboa and Instituto Dom Luiz (IDL), Universidade de Lisboa, Lisboa, Portugal; bFaculdade de Ciências da Vida, Madeira Botanical Group (GBM), Universidade da Madeira, Funchal, Portugal; cIsland Ecology and Biogeography Group, Instituto Universitario de Enfermedades Tropicales y Salud Pública de Canarias (IUETSPC), Universidad de La Laguna (ULL), La Laguna, Spain; dCIBIO Centro de Investigação em Biodiversidade e Recursos Genéticos, InBIO Laboratório Associado, Pólo dos Açores, Portugal ABSTRACT ARTICLE HISTORY Plant fossils are known from the Azores Islands, yet poorly studied. -
Prospects and Pitfalls in Integrating Volcanology and Archaeology: Areview
Journal of Volcanology and Geothermal Research 401 (2020) 106977 Contents lists available at ScienceDirect Journal of Volcanology and Geothermal Research journal homepage: www.elsevier.com/locate/jvolgeores Invited review article Prospects and pitfalls in integrating volcanology and archaeology: Areview Felix Riede a,⁎, Gina L. Barnes b, Mark D. Elson c, Gerald A. Oetelaar d, Karen G. Holmberg e, Payson Sheets f a Laboratory for Past Disaster Science, Department of Archaeology and Heritage Studies, Aarhus University, Denmark b Department of Earth Sciences, Durham University, United Kingdom c School of Anthropology, University of Arizona, United States of America d Department of Anthropology and Archaeology, University of Calgary, Canada e Gallatin School of Individualized Study, New York University, United States of America f Department of Anthropology, University of Colorado, Boulder, United States of America article info abstract Article history: Volcanic eruptions and interactions with the landforms and products these yield, are a constant feature of human Received 28 February 2020 life in many parts of the world. Seen over long timespans, human–volcano interactions become stratified in sed- Received in revised form 15 June 2020 imentary archives containing eruptive products and archaeological remains. This review is concerned with Accepted 15 June 2020 charting the overlapping territory of volcanology and archaeology and attempts to plot productive routes for fur- Available online 17 June 2020 ther conjoined research. We define archaeological volcanology as a field of study that brings together incentives, insights, and methods from both volcanology and from archaeology in an effort to better understand both past Keywords: Social volcanology volcanism as well as past cultural change, and to improve risk management practices as well as the contemporary Geoarcheology engagement with volcanism and its products. -
The Role of Substrate Hydrogeology and Surface Hydrology in the Construction of Phreatomagmatic Volcanoes on an Active Monogenetic Field (Auckland, New Zealand)
Copyright is owned by the Author of the thesis. Permission is given for a copy to be downloaded by an individual for the purpose of research and private study only. The thesis may not be reproduced elsewhere without the permission of the Author. The role of substrate hydrogeology and surface hydrology in the construction of phreatomagmatic volcanoes on an active monogenetic field (Auckland, New Zealand) A thesis presented in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Earth Science At Massey University, Palmerston North, New Zealand Javier Agustín Flores 2015 2 Abstract Phreatomagmatic activity is pervasive in the Auckland Volcanic Field (AVF) with more than two thirds of the erupted volcanoes showing this type of activity at different degrees, dominantly at the onset of their eruptive histories. In general, the volcanoes built in the northern AVF rest on Late Miocene Waitemata Group rocks (turbiditic siltstone and sandstone succession), whereas in the southern AVF the Waitemata rocks are overlain by tens of metres of Plio-Pleistocene, water-saturated sediments (Tauranga Group and Kaawa Formation). Identifying the control exerted by the type of substrate in the eruption dynamics of the phreatomagmatic phases of three volcanoes in the AVF is the objective of this study. The stratigraphic, sedimentary, and pyroclast characteristics of the phreatomagmatic sequences of Maungataketake, Motukorea, and North Head volcanoes, together with supplementary information on the geology and hydrogeology of the area, were investigated to solve the problem. Three phreatomagmatic eruptive scenarios were outlined. Scenario 1 (Maungataketake eruption) and Scenario 2 (Motukorea eruption) depict the formation of maar-diatreme volcanoes in the southern and northern AVF, respectively. -
Geomorphic Impacts of the 1257 CE Eruption of Samalas Along the Alas Strait, West Nusa Tenggara, Indonesia Bachtiar Wahyu Mutaqin
Geomorphic impacts of the 1257 CE eruption of Samalas along the Alas strait, West Nusa Tenggara, Indonesia Bachtiar Wahyu Mutaqin To cite this version: Bachtiar Wahyu Mutaqin. Geomorphic impacts of the 1257 CE eruption of Samalas along the Alas strait, West Nusa Tenggara, Indonesia. Geography. Université Panthéon-Sorbonne - Paris I; Univer- sitas Gadjah Mada (Yogyakarta, Indonésie), 2018. English. NNT : 2018PA01H071. tel-02413719v2 HAL Id: tel-02413719 https://tel.archives-ouvertes.fr/tel-02413719v2 Submitted on 16 Dec 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. ECOLE DOCTORALE DE GEOGRAPHIE DE PARIS (ED 4434) Laboratoire de Géographie Physique - UMR 8591 Doctoral Thesis in Geography Bachtiar Wahyu MUTAQIN IMPACTS GÉOMORPHIQUES DE L'ÉRUPTION DU SAMALAS EN 1257 LE LONG DU DÉTROIT D'ALAS, NUSA TENGGARA OUEST, INDONÉSIE Defense on: 11 December 2018 Supervised by : Prof. Franck LAVIGNE (Université Paris 1 – Panthhéon Sorbonne) Prof. HARTONO (Universitas Gadjah Mada) Rapporteurs : Prof. Hervé REGNAULD (Université de Rennes 2) Prof. SUWARDJI (Universitas Mataram) Examiners : Prof. Nathalie CARCAUD (AgroCampus Ouest) Dr. Danang Sri HADMOKO (Universitas Gadjah Mada) 1 Abstract As the most powerful event in Lombok’s recent eruptive history, volcanic materials that were expelled by the Samalas volcano in 1257 CE covered the entire of Lombok Island and are widespread in its eastern part.