The 2019 Eruption Dynamics and Morphology at Ebeko Volcano Monitored by Unoccupied Aircraft Systems (UAS) and Field Stations
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Dynamic Petrology and Rheology of Ascending Magma During Lava Dome Eruptions: Effusive–Explosive Activity
Dynamic petrology and rheology of ascending magma during lava dome eruptions: Effusive–explosive activity Thesis submitted in accordance with the requirements of the University of Liverpool for the degree of Doctor of Philosophy by Paul Anthony Wallace May 2019 Declaration of authorship I, Paul Anthony Wallace, declare that this thesis entitled “Dynamic petrology and rheology of ascending magma during lava dome eruptions: Effusive–explosive activity” and the work presented in it is my own. I confirm that: This thesis was completed as part of a research degree at the University of Liverpool; The material contained in this thesis has not been presented, nor is currently being presented, either wholly or in parts, for any other degree or qualifications; Where I have consulted published studies, this have been clearly referenced; Where the work was part of a collaborative effort, I have made clear what others have done and what I have contributed myself; Parts of this thesis have been published or in preparation for publication as: o Wallace, P.A., Kendrick, J.E., Ashworth, J.D., Miwa, T., Coats, R., De Angelis, S.H., Mariani, E., Utley, J.E.P., Biggin, A., Kendrick, R., Nakada, S., Matsushima, T., and Lavallée, Y. (published in Journal of Petrology). Petrological architecture of a magmatic shear zone: A multidisciplinary investigation of strain localisation during magma ascent at Unzen Volcano, Japan. o Wallace, P.A., De Angelis, S.H., Hornby, A.J., Kendrick, J.E., von Aulock, F.W., Clesham, S., Hughes, A., Utley, J.E.P., Hirose, T., Dingwell, D.B., and Lavallée, Y. (published in Geochimica et Cosmochimica Acta). -
Preliminary Volcano-Hazard Assessment for Augustine Volcano, Alaska
DEPARTMENT OF THE INTERIOR U.S. GEOLOGICAL SURVEY Preliminary Volcano-Hazard Assessment for Augustine Volcano, Alaska by Christopher F. Waythomas and Richard B. Waitt Open-File Report 98-106 This report is preliminary and subject to revision as new data become available. Any use of trade, product or firm names is for descriptive purposes only and does not imply endorsement by the U.S. Geological Survey Alaska Volcano Observatory Anchorage, Alaska 1998 U.S. DEPARTMENT OF THE INTERIOR BRUCE BABBITT, Secretary U.S. GEOLOGICAL SURVEY Thomas J. Casadevall, Acting Director For additional information: Copies of this report may be purchased from: U.S. Geological Survey U.S. Geological Survey Alaska Volcano Observatory Branch of Information Services 4200 University Drive Box 25286 Anchorage, AK 99508 Denver, CO 80225-0286 CONTENTS Summary of hazards at Augustine Volcano....................................... 1 Introduction ............................................................... 3 Purposeandscope ...................................................... 3 Physical setting of Augustine Volcano ...................................... 4 Relation to previous studies on Augustine hazards ............................. 5 Prehistoric eruptive history ................................................... 5 Historical eruptions ......................................................... 8 Hazardous phenomena at Augustine Volcano ..................................... 8 Volcanic hazards ....................................................... 12 Volcanicashclouds -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Conduit and Eruption Dynamics of the 1912 Vulcanian Explosions at Novarupta, Alaska
CONDUIT AND ERUPTION DYNAMICS OF THE 1912 VULCANIAN EXPLOSIONS AT NOVARUPTA, ALASKA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I AT MĀNOA IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS December 2017 By Samantha Jo Isgett Dissertation Committee: Bruce F. Houghton, Chairperson Helge M. Gonnermann Christina Neal Thomas Shea John Allen © 2017, Samantha Jo Isgett ii Acknowledgements I probably would not be “standing here today” if my advisor Bruce Houghton had not introduced me to the wonderful world of volcanology. I entered his 300 level volcanology class as a naïve sophomore who had no ambitions of going to graduate school and left knowing that I wanted to be volcanologist and the steps that I needed to take to get there. Bruce has a passion not only for solving the big science question, but also in passing on his knowledge and skill-sets to his students. I cannot thank Bruce enough for seeing in me the potential makings of a scientist and guiding me there. It was, and always will be, a privilege to work with you. I would like to thank my committee — Helge Gonnermann, Thomas Shea, Christina Neal, and John Allen — for pushing me to take every problem and interpretation just a little (or a lot) further. I am especially grateful to Tom and John for stepping in at the last hour. Thank you all for your time and patience. Alain Burgisser, Laurent Arbaret, and Sarah Fagents also brought outside perspectives and skill-sets that were crucial for this project. -
The Mode of Eruptions and Their Tephra Deposits
29 The Mode of Eruptions and Their Tephra Deposits 1 2 Tetsuo KOBAYASHI and Mitsuru OKUNO 1 Earth and Environmental Sciences, Faculty of Science, Kagoshima University 1-21-35 Korimoto, Kagoshima, 890-0065 Japan E-mail: [email protected] 2 Department of Earth System Science, Faculty of Science, Fukuoka University 8-19-1 Nanakuma, Jonan-ku, Fukuoka, 814-0180 Japan Abstract In accordance with the physical properties of the magma and the scale of eruption, the types of explosive eruptions are classified as follows: hawaiian, strombolian, vulcanian, sub-plinian, and plinian eruptions for magmatic eruptions; and surtseyan and phreatoplinian for phreatomagmatic eruptions. The mode of transportation of tephra is divided into the three categories of fall, flow, and surge. Each tephra layer has a characteristic depositional structure, produced not only by the mode of eruption but also by the transportation mode. As tephra layers are deposited during active periods, while loam layers accumulate during quiescent periods, a thick tephra sequence consisting of alternating tephra and loam layers will form around an active volcano. The preservation or erosion of tephra depends on not only the thickness of the deposits but also the cohesion of the tephra and the environment of deposition. Where thin tephra layers are deposited, they can become difficult to identify as individual tephra layers, due to bioturbation of the soil. In such cases, we have to use different techniques to correlate the tephra not only by the morphological feature of the pumice grains, but also by the petrological properties of the pumice, glass shards and phenocrysts. -
Nature of Bright C-Complex Asteroids
Publ. Astron. Soc. Japan (2014) 00(0), 1–20 1 doi: 10.1093/pasj/xxx000 Nature of bright C-complex asteroids Sunao HASEGAWA,1,* Toshihiro KASUGA,2 Fumihiko USUI,3 and Daisuke KURODA4 1Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara 252-5210, Japan 2Public Relations Center, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka-shi, Tokyo 181-8588, Japan 3Center for Planetary Science, Graduate School of Science, Kobe University, 7-1-48, Minatojima-minamimachi, Chuo-Ku, Kobe 650-0047, Japan 4Okayama Astronomical Observatory, Graduate School of Science, Kyoto University, 3037-5 Honjo, Kamogata-cho, Asakuchi, Okayama 719-0232, Japan ∗E-mail: [email protected] Received ; Accepted Abstract Most C-complex asteroids have albedo values less than 0.1, but there are some high-albedo (bright) C-complex asteroids with albedo values exceeding 0.1. To reveal the nature and origin of bright C-complex asteroids, we conducted spectroscopic observations of the asteroids in visible and near-infrared wavelength regions. As a result, the bright B-, C-, and Ch-type (Bus) asteroids, which are subclasses of the Bus C-complex, are classified as DeMeo C-type aster- oids with concave curvature, B-, Xn-, and K-type asteroids. Analogue meteorites and material (CV/CK chondrites, enstatite chondrites/achondrites, and salts) associated with these spec- tral types of asteroids are thought to be composed of minerals and material exposed to high temperatures. A comparison of the results obtained in this study with the SDSS photometric data suggests that salts may have occurred in the parent bodies of 24 Themis and 10 Hygiea, as well as 2 Pallas. -
~Xplosive Volcanism
STUDIES IN GEOPHYSICS ~xplosive4' Volcanism: - Inception, Evolution, and Hazards Geophysics Study Committee Geophysics Research Forum Commission on Physical Sciences, Mathematics, and Resources National Research Council NATIONAL ACADEMY PRESS Washington, D.C. 1984 Experimental Studies of Hydromagmatic Volcanism KESSETH H. WOHLETZ and ROBERT C. MCQL'EES Los Alamos Xational Laboratory ABSTRACT Hydromagmatic volcanism was modeled in experiments in which thermite melt fFe + AtOj explosively interacted with water. Several designs were explored using different contact geometries, water-melt ratios. and confinement pressures. The explosions featured ejection of steam and fragmented melt. The modeled volcanic phenomena includes melt fountains IStrombolian!, dq and wet b.apor explosions (Surtseyan!, and passive chilling of flour (submarine pillow formation!. The pertinent experimental parameters are: (1) ejection velocities of 20 to 100 dsec. (2) confining pressures of 10 to 40 MPa. :3! melt ejecta sizes of microns to centimeters in diameter, (4) steam production at temperatures of 10(PC to high levels of superheating (300 to WC!. and:{5)ejection.modes that are both ballistic and surging flow in a turbulent expanding cbud of . - vapor &id fragments. l'he.resultsindicate that explosive efficiency is strongly controlled by water-melt mass ratio and confining pressure. Optimum thermodynamic eBciency measured as the ratio of mechanical to thermal energy occurs at water-melt ratios between 0.3 and 1.0. Fragmentation increases with explosive energy and degree of water superheating. the magma by rapid decompression. These h~oprocesses may INTRODUCTION operate simultaneously during an eruption if thd magma corn- The understanding of explosive volcanism has been limited by position and environmental factors permit. -
The Youngest Volcanic Eruptions in East‐
FEATURE Feature The youngest volcanic eruptions in East- Central Europe—new findings from the Ciomadul lava dome complex, East Carpathians, Romania D. Karátson1, D. Veres2, S. Wulf3,4, 5 Violent explosive eruptions occurred between c. 51 and 29 thousand years R. Gertisser , E. ago—during the Last Glacial Maximum in East-Central Europe—at the Magyari6 & M. picturesque volcano of Ciomadul, located at the southernmost tip of the Inner Bormann7 Carpathian Volcanic Range in Romania. Field volcanology, glass geochemistry 1Eötvös University, Department of Physical of tephra, radiocarbon and optically stimulated luminescene dating, along Geography, Pázmány s. with coring the lacustrine infill of the two explosive craters of Ciomadul (St 1/C, H-1117 Budapest, Ana and Mohos), constrain the last volcanic activity to three subsequent Hungary eruptive stages. The explosivity was due to the silicic composition of the [email protected] 2 magma producing Plinian-style eruptions, and the interaction of magma Institute of Speleology, Romanian Academy, with the underlying, water-rich rocks resulting in violent phreatomagmatic Clinicilor 5, 400006 Cluj- outbursts. Tephra (volcanic ash) from these eruptions are interbedded with Napoca, Romania; 3GFZ contemporaneous loess deposits, which form thick sequences in the vicinity German Research Centre of the volcano. Moreover, tephra layers are also preserved in the older for Geosciences, Section Mohos crater infill, providing an important archive for palaeoclimate studies. 5.2 – Climate Dynamics and Landscape Evolution, Identifying the final phreatomagmatic eruption of Ciomadul at c. 29.6 ka, Telegrafenberg, D-14473 which shaped the present-day landform of the 1600-m-wide St Ana explosion Potsdam, Germany; crater, we were able to correlate related tephra deposits as far as 350 km 4Heidelberg University, from the source within a thick loess-palaeosol sequence at the Dniester Institute of Earth Sciences, Im Neuenheimer Feld Delta in Roxolany, Ukraine. -
2005 Volcanic Activity in Alaska, Kamchatka, and the Kurile Islands: Summary of Events and Response of the Alaska Volcano Observatory
The Alaska Volcano Observatory is a cooperative program of the U.S. Geological Survey, University of Alaska Fairbanks Geophysical Institute, and the Alaska Division of Geological and Geophysical Surveys . The Alaska Volcano Observtory is funded by the U.S. Geological Survey Volcano Hazards Program and the State of Alaska. 2005 Volcanic Activity in Alaska, Kamchatka, and the Kurile Islands: Summary of Events and Response of the Alaska Volcano Observatory Scientific Investigations Report 2007–5269 U.S. Department of the Interior U.S. Geological Survey Cover: Southeast flank of Augustine Volcano showing summit steaming, superheated fumarole jet, and ash dusting on snow. View is toward the northwest with Iniskin Bay in the distance. Photograph taken by Chris Waythomas, AVO/USGS, December 20, 2005. 2005 Volcanic Activity in Alaska, Kamchatka, and the Kurile Islands: Summary of Events and Response of the Alaska Volcano Observatory By R.G. McGimsey, C.A. Neal, J.P. Dixon, U.S. Geological Survey, and Sergey Ushakov, Institute of Volcanology and Seismology The Alaska Volcano Observatory is a cooperative program of the U.S. Geological Survey, University of Alaska Fairbanks Geophysical Institute, and the Alaska Division of Geological and Geophuysical Surveys. The Alaska Volcano Observatory is funded by the U.S. Geological Survey Volcano Hazards Program and the State of Alaska. Scientific Investigations Report 2007–5269 U.S. Department of the Interior U.S. Geological Survey U.S. Department of the Interior DIRK KEMPTHORNE, Secretary U.S. Geological Survey Mark D. Myers, Director U.S. Geological Survey, Reston, Virginia: 2008 For product and ordering information: World Wide Web: http://www.usgs.gov/pubprod Telephone: 1-888-ASK-USGS For more information on the USGS—the Federal source for science about the Earth, its natural and living resources, natural hazards, and the environment: World Wide Web: http://www.usgs.gov Telephone: 1-888-ASK-USGS Any use of trade, product, or firm names is for descriptive purposes only and does not imply endorsement by the U.S. -
Planetary Defense Final Report I
Team Project - Planetary Defense Final Report i Team Project - Planetary Defense Final Report ii Team Project - Planetary Defense Cover designed by: Tihomir Dimitrov Images courtesy of: Earth Image - NASA US Geological Survey Detection Image - ESA's Optical Ground Station Laser Tags ISS Deflection Image - IEEE Space Based Lasers Collaboration Image - United Nations General Assembly Building Outreach Image - Dreamstime teacher with students in classroom Evacuation Image - Libyan City of Syrte destroyed in 2011 Shield Image - Silver metal shield PNG image The cover page was designed to include a visual representation of the roadmap for a robust Planetary Defense Program that includes five elements: detection, deflection, global collaboration, outreach, and evacuation. The shield represents the idea of defending our planet, giving confidence to the general public that the Planetary Defense elements are reliable. The orbit represents the comet threat and how it is handled by the shield, which represents the READI Project. The curved lines used in the background give a sense of flow representing the continuation and further development for Planetary Defense programs after this team project, as we would like for everyone to be involved and take action in this noble task of protecting Earth. The 2015 Space Studies Program of the International Space University was hosted by the Ohio University, Athens, Ohio, USA. While all care has been taken in the preparation of this report, ISU does not take any responsibility for the accuracy of its content. -
Margaritifer Sinus, MC-19
315°E 320°E 325°E 330°E 335°E 340°E 345°E 350°E 355°E 360°E Hydraotes 0° Iamuna Colles 0° . Chaos HYDRAOTES CHAOS Dia-Cau Vallis vi Ra . Camiling Aromatum Chaos Rypin . Uzer Chimbote Mega MERIDIANI PLANUM . IANI MER Opportunity + . v Wicklow Landing Site .Victoria Windfall . Zulanka . Endeavour .Pebas . Tuskegee . Iazu Pinglo . XANTHE Oglala . Miyamoto Bopolu .Ada . Bamba .Locana CHAOS . Bahn . Zarand . .Spry Manti . Tarata Balboa . ARABIA Huancayo . Vaals AUREUM . Groves . Conches _ Sitka . Berseba . Kaid . Chinju Lachute .Manah Rakke CHAOS Airy-0 . Stobs . Byske . -5° . Butte Airy . -5° Kong . Andapa Azusa Timbuktu . Quorn TERRA . Creel . Wink . Innsbruck TERRA A .Kholm M . Daet S A . Ganges .Sfax .Paks H Batoka Chasma C . Rincon I Glide R P AURORAE CHAOS A Arsinoes Chaos C I S R M R N E A E I R F R G A R I T I -10° ColumbiaValles A -10° M Pyrrhae Chaos C H A O S . S Ubud E L L Tigre A Daga V Vallis Valles . MARGARITIFER Eos Mensa EOS CHASMA Beer -15° Morava Valles -15° . Alnif L o i r e Osuga Valles Eos TERRA Chaos Luba Valles Jones . Noord . Cardona Vinogradov Lorica . -20° Polotsk -20° . Kimry Sigli . Lebu S . Kansk . Shambe . Longa . Gagra a Gringauz ma Arda Valles Glazov ra Paraná Valles L a . V Peta d Nitro . a . o Aspen Grójec n . l Guir l e . Campos Roddy s Dollfus V . Loto Erythraeum . a .Echt Golden - Himera Valles . Galu l . Manzi Chaos l Circle . e . Kirsanov . Bentong s .Bend Yegros . Chapais . Singa Honda . -
The 2018 Fieldworks at Alaid Volcano, Atlasov Island, the Kuriles
BULLETIN OF KAMCHATKA REGIONAL ASSOCIATION «EDUCATIONAL-SCIENTIFIC CENTER». EARTH SCIENCES. ISSUE 39. No. 3. 2018 Original Russian Text © Rashidov V.A., Anikin L.P., 2018, published in Vestnik KRAUNTs. Nauki o Zemle, Vol. 39, No 3 (2018), pp. 105−113. Original text is available at http://www.kscnet.ru/journal/kraesc/article/view/220. THE 2018 FIELDWORKS AT ALAID VOLCANO, ATLASOV ISLAND, THE KURILES In August 2018, we carried out comprehensive employee A.N. Bichenko allowed us to conclude that geological and geophysical investigation of the in August and September, 2018 Alaid Volcano was in northwestern part of island type Alaid Volcano located the stage of fumarolic activity. in the Kuril Island arc on Atlasov Island (fig. a1). These In 2018, the research area was located within the research study is a part of a continuous investigation coastal zone from the Nochnoi Cape to the Plecho resulted from field works performed on Alaid Volcano Cape, and the base camp, as in 2014, was located at in 2007, 2008, 2013−2016. (Rashidov, 2013; Rashidov, the mouth of Alaidsky Brook (fig. 1b, 1c). Anikin, 2014, 2015, 2016, 2017; Rashidov et al., Unlike the Baklan, Alaid and Severny bays 2013). Personal observations, Internet data analysis, (fig. 1b), landing on this part of Atlasov Island is information received from the Vityaz-Aero company’s difficult because of the large amount of seaweed. helicopter plane commander D.A. Zaderey and photos, Quite comfortable conditions for successful field work courtesy of the Volcanoes of Kamchatka natural park’s this year resulted from many streams and large amount Fig.