Chapter 8 the Dynamics of Hawaiian
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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). -
Age Progressive Volcanism in the New England Seamounts and the Opening of the Central Atlantic Ocean
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 89, NO. B12, PAGES 9980-9990, NOVEMBER 10, 1984 AGEPROGRESSIVE VOLCANISM IN THENEW ENGLAND SEAMOUNTS AND THE OPENING OF THE CENTRAL ATLANTIC OCEAN R. A. Duncan College of Oceanography, Oregon State University, Corvallis Abstract. Radiometric ages (K-Ar and •øAr- transient featur e•s that allow calculations of 39Ar methods) have been determined on dredged relative motions only. volcanic rocks from seven of the New England The possibility that plate motions may be Seamounts, a prominent northwest-southeast trend- recorded by lines of islands and seamounts in the ing volcanic lineament in the northwestern ocean basins is attractive in this regard. If, Atlantic Ocean. The •øAr-39Ar total fusion and as the Carey-Wilson-Morgan model [Carey, 1958; incren•ental heating ages show an increase in Wilson, 1963; Morgan, 19•1] proposes, sublitho- seamount construction age from southeast to spheric, thermal anomalies called hot spots are northwest that is consistent with northwestward active and fixed with respect to one another in motion of the North American plate over a New the earth's upper mantle, they would then consti- England hot spot between 103 and 82 Ma. A linear tute a reference frame for directly and precisely volcano migration rate of 4.7 cm/yr fits the measuring plate motions. Ancient longitudes as seamount age distribution. These ages fall well as latitudes would be determined from vol- Within a longer age progression from the Corner cano construction ages along the tracks left by Seamounts (70 to 75 Ma), at the eastern end of hot spots and, providing relative plate motions the New England Seamounts, to the youngest phase are also known, quantitative estimates of conver- of volcanism in the White Mountain Igneous gent plate motions can be calculated [Engebretson Province, New England (100 to 124 Ma). -
Chapter 2 Alaska’S Igneous Rocks
Chapter 2 Alaska’s Igneous Rocks Resources • Alaska Department of Natural Resources, 2010, Division of Geological and Geophysical Surveys, Alaska Geologic Materials Center website, accessed May 27, 2010, at http://www.dggs.dnr.state.ak.us/?link=gmc_overview&menu_link=gmc. • Alaska Resource Education: Alaska Resource Education website, accessed February 22, 2011, at http://www.akresource.org/. • Barton, K.E., Howell, D.G., and Vigil, J.F., 2003, The North America tapestry of time and terrain: U.S. Geological Survey Geologic Investigations Series I-2781, 1 sheet. (Also available at http://pubs.usgs.gov/imap/i2781/.) • Danaher, Hugh, 2006, Mineral identification project website, accessed May 27, 2010, at http://www.fremontica.com/minerals/. • Digital Library for Earth System Education, [n.d.], Find a resource—Bowens reaction series: Digital Library for Earth System Education website, accessed June 10, 2010, at http://www.dlese.org/library/query.do?q=Bowens%20reaction%20series&s=0. • Edwards, L.E., and Pojeta, J., Jr., 1997, Fossils, rocks, and time: U.S. Geological Survey website. (Available at http://pubs.usgs.gov/gip/fossils/contents.html.) • Garden Buildings Direct, 2010, Rocks and minerals: Garden Buildings Direct website, accessed June 4, 2010, at http://www.gardenbuildingsdirect.co.uk/Article/rocks-and- minerals. • Illinois State Museum, 2003, Geology online–GeoGallery: Illinois State Museum Society database, accessed May 27, 2010 at http://geologyonline.museum.state.il.us/geogallery/. • Knecht, Elizebeth, designer, Pearson, R.W., and Hermans, Majorie, eds., 1998, Alaska in maps—A thematic atlas: Alaska Geographic Society, 100 p. Lillie, R.J., 2005, Parks and plates—The geology of our National parks, monuments, and seashores: New York, W.W. -
Volcanism in a Plate Tectonics Perspective
Appendix I Volcanism in a Plate Tectonics Perspective 1 APPENDIX I VOLCANISM IN A PLATE TECTONICS PERSPECTIVE Contributed by Tom Sisson Volcanoes and Earth’s Interior Structure (See Surrounded by Volcanoes and Magma Mash for relevant illustrations and activities.) To understand how volcanoes form, it is necessary to know something about the inner structure and dynamics of the Earth. The speed at which earthquake waves travel indicates that Earth contains a dense core composed chiefly of iron. The inner part of the core is solid metal, but the outer part is melted and can flow. Circulation (movement) of the liquid outer core probably creates Earth’s magnetic field that causes compass needles to point north and helps some animals migrate. The outer core is surrounded by hot, dense rock known as the mantle. Although the mantle is nearly everywhere completely solid, the rock is hot enough that it is soft and pliable. It flows very slowly, at speeds of inches-to-feet each year, in much the same way as solid ice flows in a glacier. Earth’s interior is hot both because of heat left over from its formation 4.56 billion years ago by meteorites crashing together (accreting due to gravity), and because of traces of natural radioactivity in rocks. As radioactive elements break down into other elements, they release heat, which warms the inside of the Earth. The outermost part of the solid Earth is the crust, which is colder and about ten percent less dense than the mantle, both because it has a different chemical composition and because of lower pressures that favor low-density minerals. -
Volcanic Eruption Impacts Student Worksheet
Volcanic Eruption Impacts Student Worksheet Explosive and Effusive Volcanoes The type of volcanic eruption is largely determined by magma composition. Flux-mediated melting at subduction zones creates a felsic magma with high levels of carbon dioxide and water. These dissolved gases explode during eruption. Effusive volcanoes have a hotter, more mafic magma with lower levels of dissolved gas, allowing them to erupt more calmly (effusive eruption). Sinabung (Indonesia) Mount Sinabung is a stratovolcano located 40 km from the Lake Toba supervolcano in North Sumatra. It lies along the Sunda Arc, where the Indo-Australian plate subducts beneath the Sunda and Burma plates. After 1200 years of dormancy, Sinabung began erupting intermittently in 2010. Major eruptions have occurred regularly since November 2013. In November and December 2015, ash plumes reached 6 – 11 km in height on multiple occasions. Pyroclastic flows and ashfall blanketed the region in January 2014 and lava flows travelled down the south flank, advancing 2.5 km by April 2014. Pyroclastic flows in February 2014 killed 17 people in a town 3 km from the vent. In June 2015, ash falls affected areas 10 – 15 km from the summit on many occasions. A lahar in May 2016, caused fatalities in a village 20 km from Sinabung. Pyroclastic flows occurred frequently throughout 2016 and 2017 Eruption of Sinabung 6 October 2016 Major eruptions occurred in 2018 and 2019. In (Y Ginsu, public domain) February 2018, an eruption destroyed a lava dome of 1.6 million cubic metres. At least 10 pyroclastic flows extended up to 4.9 km and an ash plume rose more than 16 km in altitude. -
Lunar Volcanism Notes (Adapted From
Lunar Volcanism Notes (adapted from http://www.asi.org/adb/m/04/02/volcanic-activity.html) The volcanic rocks produced on the moon are basalts. Basalts are common products of mantle partial melting on the terrestrial planets. This is mainly due to broad similarity of their mantle compositions. For partial melting to occur on the moon, temperatures greater than 1100°C at depths of about 200 km are required. The bulk eruption styles appear to be in the form of lava flows. There is also widespread evidence of fire-fountaining forming pyroclastic deposits (typically glass beads). Sinuous Rilles These are meandering channels which commonly begin at craters. They end by fading into the mare surface, or into chains of elongated pits. Sizes range from a few tens of meters to 3km in width. Lengths range up to 300km in length. Channels are U-shaped or V-shaped, but fallen debris (from the walls, or crater ejecta) have generally modified their cross-sections. Most sinuous rilles are near the mare basin edges, although they are found in most mare deposits. Apollo 15 confirmed the theory that sinuous rilles were analogous to lava channels and collapsed lava tubes. Lunar rilles are much larger than their terrestrial equivalents. This is thought to be due to a combination of reduced gravity, high melt temperature, low viscosity, and high extrusion rates. Domes (Shield Volcanoes) Domes are defined as broad, shallow landforms. These are convex, circular to oval in shape, and occur on the mare basins. Eighty low domes (2-3 degree slopes) have been mapped (Guest & Murray, 1976). -
Analysis of Spattering Activity at Halema'uma'u In
ANALYSIS OF SPATTERING ACTIVITY AT HALEMA‘UMA‘U IN 2015 A THESIS SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I AT MĀNOA IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN GEOLOGY AND GEOPHYSICS May 2017 By Bianca G. Mintz Thesis Committee: Bruce F. Houghton, Chairperson Tim Orr Robert Wright Keywords: spattering, lava lake, outgassing, Kīlauea, Hawaiian, Strombolian i Acknowledgments First, I must thank the faculty and staff at the Department of Geology & Geophysics at the University of Hawai‘i at Mānoa. From when I first entered the department as a freshman in August, 2012, to now as I complete up my masters’ degree the entire department has provided overwhelming amounts of guidance, encouragement, and inspiration. I was truly touched to see so many of my professors attend my oral defense in February, 2017. The professors in this department have created an environment for students to learn the skills for becoming successful scientists. Their encouragement and guidance molded me into the geologist I am today and for that I am very grateful. I would like to thank my advisor Bruce Houghton. When I first met Bruce I was interviewing for an undergraduate position in his lab (as a “lab rat”), and he told me that his goal was to have me love volcanoes. Bruce supported me both during my undergraduate degree and throughout my graduate degree as an advisor, mentor, leader, and role model. He continuously inspired me to push myself harder, to produce a higher level of quality results, and to accomplish my tasks efficiently. -
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. -
“Poseidic” Explosive Eruptions at Loihi Seamount, Hawaii
Downloaded from geology.gsapubs.org on October 5, 2010 “Poseidic” explosive eruptions at Loihi Seamount, Hawaii C. Ian Schipper*1, James D.L. White1, Bruce F. Houghton2, Nobumichi Shimizu3, and Robert B. Stewart4 1Geology Department, University of Otago, PO Box 56, Leith Street, Dunedin 9016, New Zealand 2School of Ocean and Earth Science and Technology (SOEST), University of Hawai’ i at Ma¯noa, 1680 East-West Road, Honolulu, Hawaii 98622, USA 3Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, Massachusetts 02543, USA 4Soil and Earth Sciences, Institute of Natural Resources (INR), Massey University, PB 11-222, Palmerston North 4474, New Zealand ABSTRACT (A.D. 1996) of Loihi’s ~400 ka history (Moore Much remains unknown about submarine explosive eruptions. Their deposits are found et al. 1982; Garcia et al. 2006). to great depths in all the world’s oceans, but eruptions are typically described by analogy Here we describe the southern cone on the to a subaerial nomenclature that ignores the substantial and inevitable infl uences of hydro- southeast summit plateau of Loihi (18°54′N, static pressure and magma-water interaction at submerged edifi ces. Here we explore mag- 155°15′W), examined in October 2006 with matic volatile exsolution and magma-water interaction for a pyroclastic cone-forming erup- the Hawaiian Undersea Research Laboratory’s tion at ~1 km depth on Loihi Seamount, Hawaii. We examine vesicle textures in lapilli—the Pisces IV submersible. The cone is ~60 m high, physical manifestation of degassing; dissolved volatiles in matrix glasses and olivine-hosted 4 × 106 m3 in volume, with a faintly discernable glass inclusions—the geochemical record of ascent and volatile exsolution; and fi ne ash summit rim we interpret as the edge of a partly morphology—the evidence for if and how external water assisted in fragmentation. -
Basaltic Explosive Volcanism: Constraints from Deposits and Models B.F
ARTICLE IN PRESS Chemie der Erde 68 (2008) 117–140 www.elsevier.de/chemer INVITED REVIEW Basaltic explosive volcanism: Constraints from deposits and models B.F. HoughtonÃ, H.M. Gonnermann Department of Geology and Geophysics, University of Hawai’i at Manoa, Honolulu, HI 96822, USA Received 13 March 2008; accepted 10 April 2008 Abstract Basaltic pyroclastic volcanism takes place over a range of scales and styles, from weak discrete Strombolian 2 3 1 7 8 1 explosions ( 10 –10 kg sÀ ) to Plinian eruptions of moderate intensity (10 –10 kg sÀ ). Recent well-documented historical eruptions from Etna, Kı¯lauea and Stromboli typify this diversity. Etna is Europe’s largest and most voluminously productive volcano with an extraordinary level and diversity of Strombolian to subplinian activity since 1990. Kı¯lauea, the reference volcano for Hawaiian fountaining, has four recent eruptions with high fountaining (4400 m) activity in 1959, 1960, 1969 (–1974) and 1983–1986 (–2008); other summit (1971, 1974, 1982) and flank eruptions have been characterized by low fountaining activity. Stromboli is the type location for mildly explosive Strombolian eruptions, and from 1999 to 2008 these persisted at a rate of ca. 9 per hour, briefly interrupted in 2003 and 2007 by vigorous paroxysmal eruptions. Several properties of basaltic pyroclastic deposits described here, such as bed geometry, grain size, clast morphology and vesicularity, and crystal content are keys to understand the dynamics of the parent eruptions. The lack of clear correlations between eruption rate and style, as well as observed rapid fluctuations in eruptive behavior, point to the likelihood of eruption style being moderated by differences in the fluid dynamics of magma and gas ascent and the mechanism by which the erupting magma fragments. -
Week 1 - Terrestrial Volcanism Overview
8/30/2011 Week 1 - Terrestrial Volcanism Overview • Some definitions • Eruption products • Eruption triggers • Eruption styles • The role of water • Where do volcanoes occur • Monogenetic vs polygenetic • Some volcano and eruption examples GG711, Fall 2011 1 8/30/2011 Volcanoes: Places where molten Mid-ocean ridge schematic rock and gasses exit Earth’s (or another planet’s) surface Volcanic construction materials Magma molten or partially molten rock beneath the Earth's surface. When magma erupts onto the surface, it is called lava, or Magma chamber cinders, ash, tephra or other pyroclasts Sketch by B. Myers http://volcanoes.usgs.gov/Products/Pglossary/magma.html GG711, Fall 2011 2 8/30/2011 Eruption Products The relative proportion of these materials occur as a function of magma type, tectonic setting and local variables. Source: USGS Eruption Triggering Some important factors • Tectonic triggers (changes in stress field) • Tectonic setting (compressive or extensional) • Vent opening (pressure increase from new magma input and/or gas exsolution) • Vent plugging/clogging may promote flank eruptions • Closed-system magma differentiation (pressure increase) GG711, Fall 2011 3 8/30/2011 Eruption Styles Important Magmatic factors These work together to affect eruption style • Viscosity • Magma composition • crystallinity • gas content • temperature • pressure Hot runnier Mafic (Magnesium and iron rich) cold stickier silicic (Silicon-dioxide rich) Temperature vs. Magmatic water Crystallinity vs. viscosity vs. viscosity viscosity silicic (Silicon-dioxide -
~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.