Effusion Rate Trends at Etna and Krafla and Their Implications for Eruptive

Total Page:16

File Type:pdf, Size:1020Kb

Effusion Rate Trends at Etna and Krafla and Their Implications for Eruptive Journal of Volcanology and Geothermal Research 102 (2000) 237–270 www.elsevier.nl/locate/jvolgeores Effusion rate trends at Etna and Krafla and their implications for eruptive mechanisms A.J.L. Harrisa,b,*, J.B. Murraya, S.E. Ariesa, M.A. Daviesa, L.P. Flynnb, M.J. Woosterc, R. Wrighta, D.A. Rotherya aDepartment of Earth Sciences, The Open University, Milton Keynes, MK7 6AA, UK bHawaii Institute of Geophysics & Planetology (HIGP)/School of Ocean & Earth Science Technology (SOEST), University of Hawaii, 2525 Correa Road, Honolulu, HI 96822, USA cDepartment of Geography, King’s College London, Strand, London, WC2R 2LS, UK Received 23 July 1999; received in revised form 23 February 2000; accepted 23 February 2000 Abstract Using effusion rates obtained from ground- and satellite-based data we build a data set of 381 effusion rate measurements during effusive activity at Etna and Krafla between 1980 and 1999. This allows us to construct detailed effusion rate curves for six fissure-fed eruptions at Etna and Krafla and four summit-fed eruptions at Etna. These define two trends: Type I and II. Type I trends have effusion rates that rise rapidly to an initial peak, before declining more slowly, resulting in an exponential decrease in eruption rate and declining growth in cumulative volume. Type II trends are characterised by steady effusion and eruption rates, and hence a linear increase in cumulative volume. The former is typical of fissure eruptions and can be explained by tapping of an enclosed, pressurised system. The latter are typical of persistent Etnean summit eruptions, plus one persistent effusive eruption at Stromboli (1985–1986) examined here, and can be explained by overflow of the time-averaged magma supply. We use our effusion rate data to assess the magma balance at Etna (1980–1995) and Krafla (1975–1984). Between 1980 and Ϫ 1995, Etna was supplied at a time-averaged rate of 6:8 ^ 2:3m3 s 1 of which 13% was erupted. At Krafla 817 ^ 30 × 106 m3 was erupted and intruded during 1975–1984, and the ratio of erupted to intruded volume was 0.3. At Etna there is evidence for intrusion of the unerupted magma within and beneath the edifice, as well as storage in the central magma column. At Krafla unerupted magma was intruded into a rift zone, but an increasing proportion of the supply was erupted from 1980 onwards, a result of the rift zone capacity being reached. Magma intruded prior to an eruptive event may also be entrained and/or pushed out during eruption to contribute to the initial high effusion rate phases of Type I events. The detail in our effusion rate curves was only possible using a thermal approach which estimates effusion rates using satellite data. We look forward to analysing satellite-derived effusion rate trends in real-time using data from current and soon-to-be- launched sensors. ᭧ 2000 Elsevier Science B.V. All rights reserved. Keywords: effusion rate; Etna; Krafla 1. Introduction Detailed time series of lava effusion rates can serve * Corresponding author. Tel.: ϩ1-808-956-3157; fax: ϩ1-808- 956-6322. three main purposes. First, they help constrain E-mail address: [email protected] (A.J.L. Harris). relationships between effusion rate and dimensional 0377-0273/00/$ - see front matter ᭧ 2000 Elsevier Science B.V. All rights reserved. PII: S0377-0273(00)00190-6 238 A.J.L. Harris et al. / Journal of Volcanology and Geothermal Research 102 (2000) 237–270 or morphological characteristics, such as flow length removes the effects of decompression and exsolving and area (e.g. Walker, 1973; Malin, 1980; Pieri and gases from bulk effusion rate estimates (Thordarson Baloga, 1986; Pinkerton and Wilson, 1994), and Self, 1993). By providing regular measurements 0 0 pahoehoe– a a transitions (Rowland and Walker, that consider flow activity over the entire flow field, 1990), and tube formation and size (Hallworth et al., including all branches of a bifurcating channel or flow 1987; Peterson et al., 1994; Calvari and Pinkerton, fed by multiple vents, satellite-based measurements 1998). Second, the shape of an effusion rate curve also provide a means of constraining time-varying can be used to infer eruptive mechanisms during effu- effusion and eruption rates. This is especially valuable sive activity (Wadge, 1981). Third, by quantifying the in morphologically complex cases where it may be amount, rate and variation of the erupted magma flux, difficult to measure discharge at all channels/vents effusion rate data contribute to the definition of the simultaneously. mass balance between supplied, intruded and erupted Relationships between effusion rate, flow dimen- magma (e.g. Dzurisin et al., 1984; Dvorak and sions and morphological characteristics have Dzurisin, 1993; Denlinger, 1997). This in turn contri- previously been thoroughly analysed and debated butes to an improved understanding of the rate at (e.g. Malin, 1980; Guest et al., 1987; Pinkerton and which magma is balanced by recycling or is supplied Wilson, 1994; Calvari and Pinkerton, 1998). Here we to conduits and shallow reservoirs, eruption sites, and focus on building detailed effusion rate time-series to intrusions (e.g. Francis et al., 1993; Allard, 1997; deduce eruption mechanisms and mass balances. Harris and Stevenson, 1997; Oppenheimer and Specifically we use a combination of satellite-derived Francis, 1998). However, to date there have been and ground-collected data to produce effusion rate few eruptions for which there have been a sufficient time-series to: (1) define any common and character- number of effusion rate measurements to allow effu- istic effusion rate trends; (2) infer eruptive mechan- sion rate curves to be defined (Wadge, 1981). Here we isms that can explain observed trends; and (3) use ground-based and satellite-data-derived effusion quantify erupted mass fluxes and magma supply rate measurements to produce effusion rate curves rates, and hence examine the relative importance of for as many eruptions as possible at Etna (Sicily) extrusion, intrusion and recycling. and Krafla (Iceland) volcanoes between 1980 and 1999. Between 1980 and 1999, there were 24 and 6 major 2. Effusive activity at Etna and Krafla effusive eruptions at Etna and Krafla, respectively. These resulted in the emplacement of 450 ^ 79 × Etna has been the site of frequent effusive eruptions 106 and ϳ 198 × 106 m3 of lava over a total of 1190 of basaltic (typically hawaiite) lava throughout the and 39 days, at the two volcanoes respectively. 30,000–40,000 year evolution of the currently active Although ground-based estimates made during these Mongibello edifice (Chester et al., 1985; Calvari et al., eruptions are too sparse to allow effusion rate curves 1994; Coltelli et al., 1994). As of 1994 the edifice was to be constructed, a notable exception being Frazzetta 3321 m high. Geophysical and geochemical studies and Romano (1984), use of frequently collected satel- indicate that magma is supplied from a sub-crustal lite thermal data has allowed effusion rate curves to be reservoir at a depth of 16–24 km (Sharp et al., constructed for a number of these eruptions (e.g. 1980; Tanguy et al., 1997), where SO2 emissions Harris et al., 1997a,b). We distinguish between effu- between 1975 and 1995 indicate supply to the upper sion rates and eruption rates. Effusion rate is the plumbing system at a rate of 4.5–8.0 m3 sϪ1 (Allard, instantaneous volume flux of erupted lava that is feed- 1997). In historic times effusive eruptions have ing flow at any particular point in time. Eruption rate typically occurred from the summit craters or from is the time-averaged volume flux obtained by dividing fissures on the volcano flanks (Guest and Murray, the volume of erupted lava at any particular point in 1979; Romano and Sturiale, 1982), producing flow 0 0 an eruption by the time since the eruption began. By fields dominated by a a surfaces (Chester et al., using dense rock equivalent volumes in the calcu- 1985). Data for effusive eruptions between 1868 and lation of eruption rate, consideration of eruption rate 1995 (J.B. Murray, unpublished data) indicate average A.J.L. Harris et al. / Journal of Volcanology and Geothermal Research 102 (2000) 237–270 239 flow-field lengths, areas and bulk volumes of 3.4 km, ning of the rifting episode and to events for which, 1.5 km2 and 16 × 106 m3; respectively. These data although we have no effusion rate data, volumes can show that between 1868 and 1949 an effusive event be obtained from published sources. occurred on average about once every three and a half years, with a time-averaged bulk eruption flux of Ϫ 0.15 m3 s 1. The period from 1950 onwards, however, 3. Effusion rate calculation: data, methods and saw an increase in effusive activity (Murray, 1990). results Between 1950 and 1995, an effusive event occurred about once every 9 months, and a flank eruption every To build effusion rate time series of sufficient 3.3 years. The time-averaged bulk eruption flux temporal detail to define variations in effusion during Ϫ during 1950–1995 was 0.86 m3 s 1, increasing a persistent eruption (i.e. trends occurring over a time throughout the period. Details of the main effusive scale of days to weeks), we have used two sources: (1) eruptions at Etna between 1980 and 1999 are given satellite thermal data; and (2) ground-based measure- in Table 1. ments. Our satellite-based data consist of thermal data The Krafla volcanic system is one of five fissure from three satellite-borne radiometers: the Advanced swarm-central-volcano complexes within the axial Very High Resolution Radiometer (AVHRR), Along- rift zone of N.E.
Recommended publications
  • Iceland Can Be Considered Volcanologist “Heaven”
    Iceland can be considered volcanologist “heaven” 1) Sub-aerial continuation of the Mid-Atlantic Ridge 2) Intersection of a mantle plume with a spreading ocean ridge 3) Volcanism associated with tectonic rifting 4) Sub-glacial volcanism 5) Tertiary flood (plateau) basalts 6) Bi-modal volcanism 7) Submarine volcanism 8) 18 historically active volcanoes 9) Eruptions roughly every 5 years 1. The North Atlantic opened about 54 Ma separating Greenland from Europe. 2. Spreading was initially along the now extinct Agir ridge (AER). 3. The Icelandic plume was under Greenland at that time. 4. The Greenland – Faeroe ridge represents the plume track during the history of the NE Atlantic. Kolbeinsey ridge (KR) 5. During the last 20 Ma the Reykjanes Ridge (RR) Icelandic rift zones have migrated eastward, stepwise, maintaining their position near the plume 6. The plume center is thought to be beneath Vatnajökull 1 North Rift Zone – currently active East Rift Zone – currently active West Rift Zone – last erupted about 1000-1300 AD [Also eastern (Oræfajökull) and western (Snæfellsnese) flank zones] Rift zones comprise en-echelon basaltic fissure swarms 5-15 km wide and up to 200 km long. Over time these fissures swarms develop a volcanic center, eventually maturing into a central volcano with a caldera and silicic Tertiary volcanics > 3.1 Ma volcanism Late Tertiary to Early Quaternary 3.1 – 0.7 Ma Neo-volcanic zone <0.7 - present Schematic representation of Iceland’s mantle plume. The crust is about 35 – 40 km thick Iceland’s mantle plume has been tomographically imaged down to 400 km. Some claim even deeper, through the transition zone, and down to the core – mantle boundary.
    [Show full text]
  • 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.
    [Show full text]
  • 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
    [Show full text]
  • 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
    [Show full text]
  • NE Iceland) Owing to Drone-Based Structure-From-Motion Photogrammetry
    applied sciences Article Reconstruction of Late Pleistocene-Holocene Deformation through Massive Data Collection at Krafla Rift (NE Iceland) Owing to Drone-Based Structure-from-Motion Photogrammetry Fabio Luca Bonali 1,2,*, Alessandro Tibaldi 1,2, Noemi Corti 1 , Luca Fallati 1 and Elena Russo 1,2 1 Department of Earth and Environmental Sciences, University of Milan-Bicocca, I-20126 Milan, Italy; [email protected] (A.T.); [email protected] (N.C.); [email protected] (L.F.); [email protected] (E.R.) 2 CRUST-Interuniversity Center for 3D Seismotectonics with Territorial Applications, I-66100 Chieti Scalo, Italy * Correspondence: [email protected]; Tel.: +39-0264482015 Received: 25 August 2020; Accepted: 24 September 2020; Published: 27 September 2020 Abstract: In the present work, we demonstrate how drone surveys coupled with structure-from-motion (SfM) photogrammetry can help to collect huge amounts of very detailed data even in rough terrains where logistics can affect classical field surveys. The area of study is located in the NW part of the Krafla Fissure Swarm (NE Iceland), a volcanotectonic rift composed of eruptive centres, extension fractures, and normal faults. The surveyed sector is characterized by the presence of a hyaloclastite ridge composed of deposits dated, on a stratigraphic basis, to the Weichselian High Glacial (29.1–12.1 ka BP), and a series of lava flows mostly dating back to 11–12 ka BP. The integration of remotely sensed surveys and field inspections enabled us to recognize that this segment of the Krafla rift is made of grabens arranged en-échelon with a left-stepping geometry.
    [Show full text]
  • Producing MIDS NAC Dems from MESSENGER Images
    Producing MESSENGER DEMs from MDIS NAC Images MANHEIM1, HENRIKSEN, ROBINSON, AND THE MESSENGER TEAM 1ARIZONA STATE UNIVERSITY, TEMPE AZ—[email protected] Launched: August 2004 MESSENGER Mercury Orbit: March 2011 Completed: April 2015 Mercury Dual Imaging System (MDIS) 2 framing cameras: a monochrome NAC and a multispectral WAC NAC wasn’t a stereo camera, but off-nadir observations enable the creation of DEMs NACs have 5 m pixel scale at closest approach Mercury Laser Altimeter (MLA) Radial accuracy of < 20 m Only available between 90° N and 18° S Highly Elliptical Orbit Periapsis: 200 – 500 km (near North Pole) Apoapsis: 10,000 – 15,000 km Methodology: Overview Site Selection & Image Selection Illumination Conditions Imaging Geometry DEM Production Using the USGS Integrated Software for Imagers and Spectrometers (ISIS) and SOCET SET 5.6 Error analysis Creating data products for PDS release Image Selection Selecting stereo images requires compromise between finding optimal images and building up desired coverage. These parameters will dictate the precision of the final product. Strength of stereo: parallax between the two images / unit height Illumination compatibility: distance between the tips of shadows in two images / unit height *Guidelines adapted from Becker, et al. 2015. Images Selected for Our DEMs n=49 Selecting Images to Build Mosaics Sander Crater mosaic: 21 images Selecting Images to Build Mosaics Sander Crater mosaic: 21 images 36 stereo pairs (areas of overlap producing ‘good’ stereo) Selecting Images to Build Mosaics Sander Crater mosaic: 21 images 36 stereo pairs (areas of overlap producing ‘good’ stereo) Resulting DEMs can be mosaicked together (using ISIS) to create one large-area DEM Processing in SOCET SET: Overview Import into SOCET SET 5.6 Relative Triangulation Registration to MLA tracks DEM Extraction Orthophoto Generation Creating Additional Data Products PDS Release *This process is quite similar to that described for LROC NAC DEMs in Henriksen, et al.
    [Show full text]
  • Disaster Aid After the 1783 Laki Eruption
    Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 25 June 2020 doi:10.20944/preprints202001.0070.v2 Haze, Hunger, Hesitation: Disaster aid after the 1783 Laki eruption Claudia E. Wieners ∗ aInstitute of Economics, Scuola Superiore Sant’Anna, Pisa, Italy bCentre for Complex Systems Studies, Utrecht University, Netherlands Abstract The 1783-1784 Laki eruption was one of the most severe natural catastrophes to occur in Iceland in historical times (since 1140 years). Vegetation damage by sulphate aerosol and fluorine poisoning caused a massive decimation of live- stock. The impact of fluorine poisoning and sulphate aerosol on human mortal- ity is uncertain, but the loss of animals caused a famine which took many lives. The vulnerability of the Icelandic society to famine is discussed. 18th Century Iceland was a Danish dependency and, despite the abundance of fish in the surrounding waters, a subsistence farming community and thus highly depen- dent on livestock. On the other hand, the farming community possessed coping strategies which mitigated the impact of livestock loss. During the famine, the Danish government was in principle willing to provide relief. However, local authorities in Iceland were slow to ask for help, and did not dare to exploit the means at their disposal (e.g. the right to ban the export of Icelandic foodstuff) without consent from Copenhagen. The Danish officials in turn were unwill- ing to act decisively upon incomplete information. These two factors prevented timely measures. While 4:4 × 105kg of grain were provided for famine relief in summer 1784, the merchants exported 1:2 × 106kg of fish, which greatly aggra- vated the hunger in the second winter.
    [Show full text]
  • March 21–25, 2016
    FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk,
    [Show full text]
  • Picturing France
    Picturing France Classroom Guide VISUAL ARTS PHOTOGRAPHY ORIENTATION ART APPRECIATION STUDIO Traveling around France SOCIAL STUDIES Seeing Time and Pl ace Introduction to Color CULTURE / HISTORY PARIS GEOGRAPHY PaintingStyles GOVERNMENT / CIVICS Paris by Night Private Inve stigation LITERATURELANGUAGE / CRITICISM ARTS Casual and Formal Composition Modernizing Paris SPEAKING / WRITING Department Stores FRENCH LANGUAGE Haute Couture FONTAINEBLEAU Focus and Mo vement Painters, Politics, an d Parks MUSIC / DANCENATURAL / DRAMA SCIENCE I y Fontainebleau MATH Into the Forest ATreebyAnyOther Nam e Photograph or Painting, M. Pa scal? ÎLE-DE-FRANCE A Fore st Outing Think L ike a Salon Juror Form Your Own Ava nt-Garde The Flo ating Studio AUVERGNE/ On the River FRANCHE-COMTÉ Stream of Con sciousness Cheese! Mountains of Fra nce Volcanoes in France? NORMANDY “I Cannot Pain tan Angel” Writing en Plein Air Culture Clash Do-It-Yourself Pointillist Painting BRITTANY Comparing Two Studie s Wish You W ere Here Synthétisme Creating a Moo d Celtic Culture PROVENCE Dressing the Part Regional Still Life Color and Emo tion Expressive Marks Color Collectio n Japanese Prin ts Legend o f the Château Noir The Mistral REVIEW Winds Worldwide Poster Puzzle Travelby Clue Picturing France Classroom Guide NATIONAL GALLERY OF ART, WASHINGTON page ii This Classroom Guide is a component of the Picturing France teaching packet. © 2008 Board of Trustees of the National Gallery of Art, Washington Prepared by the Division of Education, with contributions by Robyn Asleson, Elsa Bénard, Carla Brenner, Sarah Diallo, Rachel Goldberg, Leo Kasun, Amy Lewis, Donna Mann, Marjorie McMahon, Lisa Meyerowitz, Barbara Moore, Rachel Richards, Jennifer Riddell, and Paige Simpson.
    [Show full text]
  • Impact Melt Emplacement on Mercury
    Western University Scholarship@Western Electronic Thesis and Dissertation Repository 7-24-2018 2:00 PM Impact Melt Emplacement on Mercury Jeffrey Daniels The University of Western Ontario Supervisor Neish, Catherine D. The University of Western Ontario Graduate Program in Geology A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Jeffrey Daniels 2018 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Geology Commons, Physical Processes Commons, and the The Sun and the Solar System Commons Recommended Citation Daniels, Jeffrey, "Impact Melt Emplacement on Mercury" (2018). Electronic Thesis and Dissertation Repository. 5657. https://ir.lib.uwo.ca/etd/5657 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. Abstract Impact cratering is an abrupt, spectacular process that occurs on any world with a solid surface. On Earth, these craters are easily eroded or destroyed through endogenic processes. The Moon and Mercury, however, lack a significant atmosphere, meaning craters on these worlds remain intact longer, geologically. In this thesis, remote-sensing techniques were used to investigate impact melt emplacement about Mercury’s fresh, complex craters. For complex lunar craters, impact melt is preferentially ejected from the lowest rim elevation, implying topographic control. On Venus, impact melt is preferentially ejected downrange from the impact site, implying impactor-direction control. Mercury, despite its heavily-cratered surface, trends more like Venus than like the Moon.
    [Show full text]
  • 1783-84 Laki Eruption, Iceland
    1783-84 Laki eruption, Iceland Eruption History and Atmospheric Effects Thor Thordarson Faculty of Earth sciences, University of Iceland 12/8/2017 1 Atmospheric Effects of the 1783-84 Laki Eruption in Iceland Outline . Volcano-Climate interactions - background Laki eruption . Eruption history . Sulfur release and aerosol loading . Plume transport and aerosol dispersal . Environmental and climatic effects 12/8/2017. Concluding Remarks 2 Santorini, 1628 BC Tambora, 1815 Etna, 44 BC Lakagígar, 1783 Toba, 71,000 BP Famous Volcanic Eruptions Krakatau, 1883 Pinatubo, 1991 El Chichón, 1982 Agung, 1963 St. Helens, 1980 Major volcanic eruptions of the past 250 years Volcano Year VEI d.v.i/Emax IVI Lakagígar [Laki craters], Iceland 1783 4 2300 0.19 Unknown (El Chichón?) 1809 0.20 Tambora, Sumbawa, Indonesia 1815 7 3000 0.50 Cosiguina, Nicaragua 1835 5 4000 0.11 Askja, Iceland 1875 5 1000 0.01* Krakatau, Indonesia 1883 6 1000 0.12 Okataina [Tarawera], North Island, NZ 1886 5 800 0.04 Santa Maria, Guatemala 1902 6 600 0.05 Ksudach, Kamchatka, Russia 1907 5 500 0.02 Novarupta [Katmai], Alaska, US 1912 6 500 0.15 Agung, Bali, Indonesia 1963 4 800 0.06 Mt. St. Helens, Washington, US 1980 5 500 0.00 El Chichón, Chiapas, Mexico 1982 5 800 0.06 Mt. Pinatubo, Luzon, Philippines 1991 6 1000 — Volcano – Climate Interactions Key to Volcanic Forcing is: SO2 mass loading, eruption duration plume height replenishment aerosol production, residence time 12/8/2017 5 Volcanic Forcing: sulfur dioxide sulfate aerosols SO2 75%H2SO4+ 25%H2O clear sky 1991 Pinatubo aerosols
    [Show full text]
  • Lava Shields and Fissure Eruptions of the Western
    Journal of Volcanology and Geothermal Research 186 (2009) 331–348 Contents lists available at ScienceDirect Journal of Volcanology and Geothermal Research journal homepage: www.elsevier.com/locate/jvolgeores Lava shields and fissure eruptions of the Western Volcanic Zone, Iceland: Evidence for magma chambers and crustal interaction Deborah E. Eason ⁎, John M. Sinton Department of Geology and Geophysics, School of Ocean and Earth Science and Technology, 1680 East–West Road, University of Hawaii, Honolulu, HI 96822, United States article info abstract Article history: Volcanic eruptions in Iceland occur either from fissures or central vents (lava shields). Within the post-glacial Received 19 December 2008 Western Volcanic Zone, the Thjófahraun fissure-fed lava field and Lambahraun lava shield were both erupted Accepted 30 June 2009 ~4000 yrs B.P. with eruptive centers separated by only ~25 km. Thjófahraun erupted ~1 km3 of pāhoehoe and Available online 5 July 2009 'a'ā lava from a 9-km long fissure, whereas the Lambahraun lava shield erupted N7km3 of low effusion-rate pāhoehoe. Thjófahraun lavas contain higher K, Rb, Y and Zr, and lower CaO than Lambahraun lavas at the same Keywords: MgO, with variations broadly consistent with evolution by low-pressure crystal fractionation. Lambahraun Iceland mid-ocean ridge spans a larger range of MgO, which generally decreases over time during the eruption. Lambahraun samples fl magma chambers with high Al2O3 and low TiO2 and FeO likely re ect up to 15% plagioclase accumulation. In addition, all samples crustal interaction from Lambahraun exhibit increasing CaO and Nb/Zr with decreasing MgO and overall incompatible-element MORB enrichments greater than predicted by crystal fractionation alone.
    [Show full text]