DOCSLIB.ORG

NEWSLETTER Seismic Design of New Low- Cost Housing for El

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
NEWSLETTER Seismic Design of New Low- Cost Housing for El ISSN 0967-859X THE SOCIETY FOR EARTHQUAKE AND S CIVIL ENGINEERING DYNAMICS E SECED E NEWSLETTER Volume 26 No 1 D February 2015 In this issue Seismic Design of New Low- Seismic Design Cost Housing for El Salvador 1 Notable Earthquakes July 2013 – February 2014 9 of New Low- Forthcoming Events 12 Cost Housing for El Salvador Sebastian Kaminski Katherine Coates Arup, London Arup, London Andrew Lawrence Arup, London l Salvador has one of the largest divides between Natural hazards including earthquakes, volcanoes, the rich and the poor in the world with hundreds of flooding and hurricanes, contribute significantly towards thousands living in poverty on only a few dollars per this housing deficit. As the worst effects of hurricanes tend Eday. This poverty, coupled with the frequent earthquakes to be confined to the Caribbean and the Eastern seaboard and other natural disasters, has left many living in sub- of North and Central America, one of Central America’s standard unhygienic and unsafe housing. This problem is greatest natural hazard is arguably earthquakes, as the not isolated to El Salvador, and indeed recent estimates of Pacific Ring of Fire runs down the west coast. Many areas the housing deficit in Latin America as a whole are between are considered to have high seismic hazard (with a Peak 42–51 million dwellings (this is the number of new houses Ground Acceleration greater than 0.4g for a 10% probabil- required to house all those in sub-standard, precariously ity of exceedance in 50 years). In the last 500 years, Central located or overcrowded housing) (UN-Habitat, 2011). America has experienced many earthquakes that caused SECED Newsletter Vol. 26 No. 1 February 2015 | For updates on forthcoming events go to www.seced.org.uk 1 significant damage and loss of life, both in the subduction a copy of a more modern design, often masonry. The de- zone which forms part of the Pacific Ring of Fire and in the sign of engineered houses is normally determined by the local faults along the volcanic chain. government, donors or Non-Governmental Organisations New permanent low-cost housing in Latin America (NGOs). The most common permanent housing options consists of a mixture of engineered and non-engineered currently being constructed in Central America are ado- housing. The design of non-engineered houses often rests be, bahareque (a derivative of wattle-and-daub), confined entirely with the beneficiaries or local skilled workers, and masonry and reinforced hollow blockwork. Unfortunately, will often consist of a vernacular design, or alternatively each of these has a number of drawbacks: adobe has very Table 1: Selection of advantages, disadvantages and relative costs of the main permanent housing options constructed in El Salvador Housing Relative Type Advantages Disadvantages cost Adobe • Very cheap when the correct soil • Typically performs very poorly in an earth- Low type is available locally. quake. • Widely-known construction system. • Requires considerable maintenance. • Good thermal mass hence very cool • Harbours disease-carrying insects. inside. • Very unpopular with locals. • Negligible environmental impact. • Traditionally combined with a heavy tiled roof, increasing the seismic loads and the risk of injury if it falls. Bahareque • Relatively low-cost. • Harbours disease-carrying insects. Medium • Can have good seismic resistance • Susceptible to insect attack and water when in good condition. ingress. • Good thermal mass hence very cool • Requires considerable maintenance. inside. • Relatively unpopular with locals. • Low environmental impact. • Traditionally combined with a heavy tiled roof, increasing the seismic loads and the risk of injury if it falls. Confined • Good seismic resistance when well- • Commonly constructed poorly – detailing Medium- masonry constructed. more complex than reinforced blockwork. high • Challenging to construct (difficult • Higher cost. to place rebar and concrete in small • High environmental impact (fired clay confining elements). bricks and concrete). • Good thermal mass hence very cool • Seismic design rules generally mean inside. houses often have smaller and/or fewer • Popular with locals. windows. • Typically combined with a heavy tiled roof, increasing the seismic loads and the risk of injury if it falls. Reinforced • Very good seismic resistance when • Higher cost. Medium- blockwork well-constructed. • High environmental impact (concrete). high • Very durable. • Good thermal mass hence very cool inside. • Very popular with locals. • Relatively simple to construct. • Normally combined with lightweight zinc-aluminium roof sheeting, reduc- ing the seismic loads and risk of injury if it falls. 2 For updates on forthcoming events go to www.seced.org uk | SECED Newsletter Vol. 26 No. 1 February 2015 low seismic resistance, can harbour disease-carrying in- The design that is being developed is a single-storey sects and is poorly regarded by local communities; baha- four roomed building, approximately 6 m × 6 m, with two reque often deteriorates after approximately a decade due bedrooms, one lounge and one kitchen. The foundations to insect attack and water ingress (López et al., 2004); of the house are a thin reinforced concrete slab sitting on confined masonry is very workmanship dependent and reinforced concrete ground beams under the walls. The relatively expensive (see Table 1). The existing best option walls sit on two courses of hollow reinforced blockwork, for permanent low-cost housing in El Salvador is widely protecting the frame above from water and insect attack. considered to be reinforced hollow blockwork, which is The wall and roof structural frame sits on the blockwork very durable and has good seismic resistance when well- and consists of a simple 2” × 4” structurally graded and constructed; however it is moderately expensive and not pressure-treated pine frame, nailed together with steel very sustainable. straps at key locations to resist wind and seismic loads. The Arup (a UK-based design consultancy), Engage for walls are wrapped in a thin galvanised chicken mesh on Development (a UK-based charity) and the Imperial both sides, and vara de castilla (also known as caña brava – College El Salvador Project (a UK-based charitable or- a local type of cane approximately 25 mm in diameter and ganisation) have been working with REDES (a small El up to 6 m long (Chan, 2014)) is nailed to the frame. The Salvadorean NGO) for the past four years, with the aim of vara de castilla is sourced from local farmers and is treated developing an alternative, low-cost, sustainable, seismical- on site against insects with boron. Cement mortar is then ly-resistant and appropriate low-cost house design suitable plastered on both sides of the walls to form the 60 mm for El Salvador. The design should also be easy to construct thick shear walls. The bases of the walls are painted with and maintain by the local communities themselves, and waterproof paint to protect against driving rain. The roof ideally use local materials such that more money goes back consists of lightweight cement fibreboard sheeting screwed into the local economy. down onto the timber purlins and rafters. The design life of the house is 30 years with minimal maintenance. Overview of Design After conducting research into existing low-cost housing Prototype houses in the Latin American region, in particular using bamboo Two prototype houses were successfully built in El Salvador structurally (Kaminski, 2013), the team developed a solu- in 2012, and have allowed the house design and construc- tion which takes the vernacular bahareque design and “en- tion method to be optimised (El Salvador Project 2012, gineers” it by essentially: treating the timber and wall ma- 2012). They were evaluated again in 2013 and the benefici- trix against insect attack, replacing the mud render with a aries were very happy with them, with no reported struc- more durable and stronger cement mortar and engineering tural problems (see Figures 1 and 2). the connection details. Figure 1: Prototype cane and mortar house under construction (El Salvador Project, 2012). © Sebastian Kaminski SECED Newsletter Vol. 26 No. 1 February 2015 | For updates on forthcoming events go to www.seced.org.uk 3 Figure 2: Prototype cane and mortar house, completed in 2012 (El Salvador Project, 2012). © Sebastian Kaminski Seismic Design Approach of the materials available in El Salvador are imported from The lateral stability system of the structure relies upon per- the US. pendicular shear walls in both directions, roughly evenly A comparative study of different seismic hazard assess- spaced. With a light roof, most of the seismic load is gener- ments for El Salvador was conducted in order to determine ated by the self-weight of the walls themselves. the most appropriate design parameters. Table 2 presents As El Salvador is in a region of high seismic hazard, the the maximum seismic hazard determined for any area seismic demands govern the design of the lateral system; within El Salvador from a number of different published hurricane winds do not tend to affect El Salvador as it is on sources. the West coast of Central America. The El Salvadorean seis- A design PGA of 0.5g (10% probability of exceedance in mic code (MOP, 1994) is based on the Mexico City code and 50 years) has been selected for the design because Benito loosely in turn on an old version of the Uniform Building et al. (2012) was considered to best reflect the most up-to- Code (UBC). In addition, the other El Salvadorean materi- date understanding of seismic hazard in the region, and al design codes are also limited in their scope or refer back one which involved a collaborative effort between different to US or Mexican codes (López et al., 2004). Therefore, in specialists in the region. It also reflects the design criteria order to be able to use an up-to-date, comprehensive and according to which the house may be built anywhere with- consistent set of design codes, the most recent US design in the country.
Load more

Recommended publications
  • Variability in the Location. of the Antarctic Polar Front (90 °
    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 102, NO. C13, PAGES 27,825-27,833, DECEMBER 15, !997 Variability in the location.of the Antarctic Polar Front (90ø- 20øW) from satellite sea surface temperature data J. Keith Moore, Mark R. Abbott, and James G. Richman Collegeof Oceanicand AtmosphericSciences, Oregon State University, Corvallis Abstract. The path of the AntarcticPolar Front (PF) is mappedusing satellite sea surfacetemperature data from the NOAA/NASA Pathfinderprogram. The mean path and variabilityof the PF are stronglyinfluenced by bathymetry.Meandering intensity is weaker where the bathymetryis steeplysloped and increasesin areaswhere the bottom is relativelyflat. There is an inverserelationship between meandering intensity and both the width of the front and the changein temperatureacross it. There is a persistent,large separationbetween the surfaceand subsurfaceexpressions of the PF at Ewing Bank on the Falkland Plateau. 1. Introduction of meanderingjets and fronts hasbeen done previouslyfor the PF [Legeckis,1977] and other strongfrontal systems[Hansen TheAntarctic Polar Front (PF) is a strongjet within t•e and Maul, 1970; Olsonet al., 1983; Cornilion, 1986]. Antarctic CircumpolarCurrent (ACG), which flowseastward Satellite altimeter data has shown that there is little zonal continuouslyaround Antarctica [Nowlin and Klinck, 1986].The coherencein the variabilityof the ACC [Fu and Chelton,1984; PF, also known as the Antarctic Convergence,is the location Sandwelland Zhang, 1989; Chelton et al., 1990; Gille, 1994; where Antarctic surfacewaters movingto the north sink rap- Gille and Kelly,1996]. These studies emphasize the importance idly belowSubantarctic waters [Deacon, 1933, 1937].Thus the of local and regionalinstabilities [Chelton et al., 1990;Gille and PF is a regionof elevatedcurrent speeds and stronghorizontal Kelly,1996].
    [Show full text]
  • Modification and Pathways of Southern Ocean Deep Waters in the Scotia
    Deep-Sea Research I 49 (2002) 681–705 Modification and pathways of Southern Ocean Deep Waters in the Scotia Sea Alberto C. Naveira Garabatoa,*, Karen J. Heywooda, David P. Stevensb a School of Environmental Sciences, University of East Anglia, Norwich NR4 7TJ, UK b School of Mathematics, University of East Anglia, Norwich NR4 7TJ, UK Received 11 September 2000; received in revised form 11 June 2001; accepted 23 October 2001 Abstract An unprecedented high-quality, quasi-synoptic hydrographic data set collected during the ALBATROSS cruise along the rim of the Scotia Sea is examined to describe the pathways of the deep water masses flowing through the region, and to quantify changes in their properties as they cross the sea. Owing to sparse sampling of the northern and southern boundaries of the basin, the modification and pathways of deep water masses in the Scotia Sea had remained poorly documented despite their global significance. Weddell Sea Deep Water (WSDW) of two distinct types is observed spilling over the South Scotia Ridge to the west and east of the western edge of the Orkney Passage. The colder and fresher type in the west, recently ventilated in the northern Antarctic Peninsula, flows westward to Drake Passage along the southern margin of the Scotia Sea while mixing intensely with eastward-flowing Circumpolar Deep Water (CDW) of the antarctic circumpolar current (ACC). Although a small fraction of the other WSDW type also spreads westward to Drake Passage, the greater part escapes the Scotia Sea eastward through the Georgia Passage and flows into the Malvinas Chasm via a deep gap northeast of South Georgia.
    [Show full text]
  • Chapter 4 Tectonic Reconstructions of the Southernmost Andes and the Scotia Sea During the Opening of the Drake Passage
    123 Chapter 4 Tectonic reconstructions of the Southernmost Andes and the Scotia Sea during the opening of the Drake Passage Graeme Eagles Alfred Wegener Institute, Helmholtz Centre for Marine and Polar Research, Bre- merhaven, Germany e-mail: [email protected] Abstract Study of the tectonic development of the Scotia Sea region started with basic lithological and structural studies of outcrop geology in Tierra del Fuego and the Antarctic Peninsula. To 19th and early 20th cen- tury geologists, the results of these studies suggested the presence of a submerged orocline running around the margins of the Scotia Sea. Subse- quent increases in detailed knowledge about the fragmentary outcrop ge- ology from islands distributed around the margins of the Scotia Sea, and later their interpretation in light of the plate tectonic paradigm, led to large modifications in the hypothesis such that by the present day the concept of oroclinal bending in the region persists only in vestigial form. Of the early comparative lithostratigraphic work in the region, only the likenesses be- tween Jurassic—Cretaceous basin floor and fill sequences in South Geor- gia and Tierra del Fuego are regarded as strong enough to be useful in plate kinematic reconstruction by permitting the interpretation of those re- gions’ contiguity in mid-Mesozoic times. Marine and satellite geophysical data sets reveal features of the remaining, submerged, 98% of the Scotia 124 Sea region between the outcrops. These data enable a more detailed and quantitative approach to the region’s plate kinematics. In contrast to long- used interpretations of the outcrop geology, these data do not prescribe the proximity of South Georgia to Tierra del Fuego in any past period.
    [Show full text]
  • Article Size, 12 Nm Pore Size; YMC Collision Energy 15, 22.5, and 30; Isolation Window 1.0 M/Z)
    Biogeosciences, 18, 3485–3504, 2021 https://doi.org/10.5194/bg-18-3485-2021 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Archaeal intact polar lipids in polar waters: a comparison between the Amundsen and Scotia seas Charlotte L. Spencer-Jones1, Erin L. McClymont1, Nicole J. Bale2, Ellen C. Hopmans2, Stefan Schouten2,3, Juliane Müller4, E. Povl Abrahamsen5, Claire Allen5, Torsten Bickert6, Claus-Dieter Hillenbrand5, Elaine Mawbey5, Victoria Peck5, Aleksandra Svalova7, and James A. Smith5 1Department of Geography, Durham University, Lower Mountjoy, South Road, Durham, DH1 3LE, UK 2NIOZ Royal Netherlands Institute for Sea Research, Department of Marine Microbiology and Biogeochemistry, P.O. Box 59, 1790 AB Den Burg, Texel, the Netherlands 3Department of Earth Sciences, Utrecht University, Utrecht, the Netherlands 4Alfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, 27568 Bremerhaven, Germany 5British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET, UK 6MARUM – Center for Marine Environmental Sciences, University of Bremen, Leobener Str. 8, 28359, Bremen, Germany 7School of Natural and Environmental Sciences, Newcastle University, Newcastle-upon-Tyne, NE1 7RU, UK Correspondence: Charlotte L. Spencer-Jones ([email protected]) Received: 7 September 2020 – Discussion started: 5 November 2020 Revised: 3 March 2021 – Accepted: 23 March 2021 – Published: 11 June 2021 Abstract. The West Antarctic Ice Sheet (WAIS) is one of compassing the sub-Antarctic front through to the southern the largest potential sources of future sea-level rise, with boundary of the Antarctic Circumpolar Current. IPL-GDGTs glaciers draining the WAIS thinning at an accelerating rate with low cyclic diversity were detected throughout the water over the past 40 years.
    [Show full text]
  • In Shackleton's Footsteps
    In Shackleton’s Footsteps 20 March – 06 April 2019 | Polar Pioneer About Us Aurora Expeditions embodies the spirit of adventure, travelling to some of the most wild and adventure and discovery. Our highly experienced expedition team of naturalists, historians and remote places on our planet. With over 27 years’ experience, our small group voyages allow for destination specialists are passionate and knowledgeable – they are the secret to a fulfilling a truly intimate experience with nature. and successful voyage. Our expeditions push the boundaries with flexible and innovative itineraries, exciting wildlife Whilst we are dedicated to providing a ‘trip of a lifetime’, we are also deeply committed to experiences and fascinating lectures. You’ll share your adventure with a group of like-minded education and preservation of the environment. Our aim is to travel respectfully, creating souls in a relaxed, casual atmosphere while making the most of every opportunity for lifelong ambassadors for the protection of our destinations. DAY 1 | Wednesday 20 March 2019 Ushuaia, Beagle Channel Position: 21:50 hours Course: 84° Wind Speed: 5 knots Barometer: 1007.9 hPa & falling Latitude: 54°55’ S Speed: 9.4 knots Wind Direction: E Air Temp: 11°C Longitude: 67°26’ W Sea Temp: 9°C Finally, we were here, in Ushuaia aboard a sturdy ice-strengthened vessel. At the wharf Gary Our Argentinian pilot climbed aboard and at 1900 we cast off lines and eased away from the and Robyn ticked off names, nabbed our passports and sent us off to Kathrine and Scott for a wharf. What a feeling! The thriving city of Ushuaia receded as we motored eastward down the quick photo before boarding Polar Pioneer.
    [Show full text]
  • Physical Drivers of Phytoplankton Bloom Initiation in the Southern Ocean's Scotia Sea
    UC San Diego UC San Diego Previously Published Works Title Physical Drivers of Phytoplankton Bloom Initiation in the Southern Ocean's Scotia Sea Permalink https://escholarship.org/uc/item/9tz4q3pc Journal JOURNAL OF GEOPHYSICAL RESEARCH-OCEANS, 124(8) ISSN 2169-9275 Authors Prend, Channing J Gille, Sarah T Talley, Lynne D et al. Publication Date 2019-08-01 DOI 10.1029/2019JC015162 Peer reviewed eScholarship.org Powered by the California Digital Library University of California RESEARCH ARTICLE Physical Drivers of Phytoplankton Bloom Initiation 10.1029/2019JC015162 in the Southern Ocean's Scotia Sea Key Points: Channing J. Prend1 , Sarah T. Gille1 , Lynne D. Talley1 , B. Greg Mitchell1 , • Shallow mixed layers in the Scotia 1 1 Sea support the earliest and largest Isabella Rosso , and Matthew R. Mazloff offshore spring phytoplankton 1 bloom in the Southern Ocean Scripps Institution of Oceanography, La Jolla, CA, USA • About 10% of the water in the bloom region is advected from the Weddell Sea, which helps set the unique Abstract The Scotia Sea is the site of one of the largest spring phytoplankton blooms in the Southern fi strati cation Ocean. Past studies suggest that shelf‐iron inputs are responsible for the high productivity in this region, • Vertical transport associated with a stratified Taylor column may but the physical mechanisms that initiate and sustain the bloom are not well understood. Analysis of enhance productivity by supplying profiling float data from 2002 to 2017 shows that the Scotia Sea has an unusually shallow mixed‐layer depth subsurface iron to the euphotic zone during the transition from winter to spring, allowing the region to support a bloom earlier in the season than elsewhere in the Antarctic Circumpolar Current.
    [Show full text]
  • Chapter 6 Antarctic Oceanography the Region of the World Ocean Bordering on Antarctica Is Unique in Many Respects. First of All
    Chapter 6 Antarctic oceanography The region of the world ocean bordering on Antarctica is unique in many respects. First of all, it is the only region where the flow of water can continue all around the globe nearly unhindered and the circulation therefore comes closest to the situation in the atmosphere. Secondly, the permanent thermocline (the interface z = H(x,y) of Figure 3.1) reaches the surface in the Subtropical Convergence (Figure 5.5) and does not extend into the polar regions; temperature differences between the sea surface and the ocean floor close to the continent are below 1°C and generally do not exceed 5°C, i.e. 20% of the difference found in 1 the tropics (Figure 6.1). What this means is that our 1 /2 layer ocean model cannot be applied to the seas around Antarctica. Fig. 6.1. Temperature profiles for different climatic regions near 150°W (Pacific Ocean). (a) tropical (5°S), (b) subtropical (35°S), (c) subpolar (50°S), (d) polar (55°S). The temperature scale is correct for the polar profile; other profiles are shifted successively by 1°C. Note the shallowness of the warm surface layer and the absence of the permanent thermocline in the polar region. Data from Osborne et al. (1991). It may seem strange that having spent five chapters on a discussion of temperate and tropical ocean dynamics, we now begin our regional discussion with a region that does not fit the earlier picture. However, our earlier discussion is not entirely irrelevant; it taught us how to get an idea of a region's dynamics by identifying the important forces and looking at their balance.
    [Show full text]
  • The Age and Origin of the Central Scotia Sea
    Geophysical Journal International Geophys. J. Int. (2010) 183, 587–600 doi: 10.1111/j.1365-246X.2010.04781.x The age and origin of the central Scotia Sea Graeme Eagles Department of Earth Sciences, Royal Holloway University of London, Egham, Surrey TW20 0EX, UK. E-mail: [email protected] Accepted 2010 August 18. Received 2010 July 6; in original form 2010 May 7 SUMMARY Opening of the Drake Passage gateway between the Pacific and Atlantic oceans has been linked in various ways to Cenozoic climate changes. From the oceanic floor of Drake Passage, the largest of the remaining uncertainties in understanding this opening is in the timing and process of the opening of the central Scotia Sea. All but one of the available constraints on the age of the central Scotia Sea is diagnostic of, or consistent with, a Mesozoic age. Comparison of tectonic and magnetic features on the seafloor with plate kinematic models shows that it is likely to have accreted to a mid-ocean ridge between the South American and Antarctic plates following their separation in Jurassic times. Subsequent regional shallowing may be related GJI Geodynamics and tectonics to subduction-related processes that preceded backarc extension in the East Scotia Sea. The presence of a fragment of Jurassic–Cretaceous ocean floor in the gateway implies that deep water connections through the Scotia Sea basin complex may have been possible since Eocene times when the continental tips of South America and the Antarctic Peninsula first passed each other. Key words: Tectonics and climate interactions; Kinematics of crustal and mantle deforma- tion; Antarctica; South America.
    [Show full text]
  • Origin, Signature and Palaeoclimatic Influence of the Antarctic Circumpolar Current
    Earth-Science Reviews 66 (2004) 143–162 www.elsevier.com/locate/earscirev Origin, signature and palaeoclimatic influence of the Antarctic Circumpolar Current P.F. Barkera,*, E. Thomasb,c a 25 Church St., Great Gransden, Sandy, Beds SG19 3AF, UK b Department of Earth and Environmental Sciences, Wesleyan University, Middletown, CT 06457, USA c Center for the Study of Global Change, Department of Geology and Geophysics, Yale University, New Haven, CT 06520-1809, USA Accepted 27 October 2003 Abstract The Antarctic Circumpolar Current (ACC) is today the strongest current in the world’s ocean, with a significant influence on global climate. Its assumed history and influence on palaeoclimate, while almost certainly equally profound, are here called into question. In this paper, we review 30 years of accumulated data, interpretation and speculation about the ACC, deriving mainly from DSDP and ODP drilling in the Southern Ocean. For most of this time, a conventional view of ACC development, signature and influence has held sway among palaeoceanographers and marine geologists. In this view, the ACC began at about 34 Ma, close to the Eocene–Oligocene boundary, the time of onset of significant Antarctic glaciation and the time of creation of a deep-water gap (Tasmanian Seaway) between Australia and Antarctica as the South Tasman Rise separated from North Victoria Land. This is the ‘‘smoking gun’’ of synchroneity. The Southern Ocean sediment record shows a latest Eocene development and subsequent geographic expansion of a siliceous biofacies, its northern limit taken to indicate the palaeo- position of the ACC axis. In addition, the ACC was considered to have caused Antarctic glaciation by isolating the continent within a cold-water annulus, reducing north–south heat transport.
    [Show full text]
  • The Indian Ocean and the Himalayas : a Geological Interpretation
    The Indian Ocean and the Himalayas : a geological interpretation Autor(en): Gansser, Augusto Objekttyp: Article Zeitschrift: Eclogae Geologicae Helvetiae Band (Jahr): 59 (1966) Heft 2 PDF erstellt am: 11.10.2021 Persistenter Link: http://doi.org/10.5169/seals-163396 Nutzungsbedingungen Die ETH-Bibliothek ist Anbieterin der digitalisierten Zeitschriften. Sie besitzt keine Urheberrechte an den Inhalten der Zeitschriften. Die Rechte liegen in der Regel bei den Herausgebern. Die auf der Plattform e-periodica veröffentlichten Dokumente stehen für nicht-kommerzielle Zwecke in Lehre und Forschung sowie für die private Nutzung frei zur Verfügung. Einzelne Dateien oder Ausdrucke aus diesem Angebot können zusammen mit diesen Nutzungsbedingungen und den korrekten Herkunftsbezeichnungen weitergegeben werden. Das Veröffentlichen von Bildern in Print- und Online-Publikationen ist nur mit vorheriger Genehmigung der Rechteinhaber erlaubt. Die systematische Speicherung von Teilen des elektronischen Angebots auf anderen Servern bedarf ebenfalls des schriftlichen Einverständnisses der Rechteinhaber. Haftungsausschluss Alle Angaben erfolgen ohne Gewähr für Vollständigkeit oder Richtigkeit. Es wird keine Haftung übernommen für Schäden durch die Verwendung von Informationen aus diesem Online-Angebot oder durch das Fehlen von Informationen. Dies gilt auch für Inhalte Dritter, die über dieses Angebot zugänglich sind. Ein Dienst der ETH-Bibliothek ETH Zürich, Rämistrasse 101, 8092 Zürich, Schweiz, www.library.ethz.ch http://www.e-periodica.ch The Indian Ocean and the Himalayas A Geological Interpretation by Augusto Gansser (Zürich)1) with 4 figures in the text and 2 plates (I and II) ABSTRACT The recently discovered lineaments of the Indian Ocean indicate a northwards shift of the Indian Shield which is directly responsible for the Himalayan Orogeny.
    [Show full text]
  • Multi-Modal Survey of Adélie Penguin Mega-Colonies Reveals the Danger
    www.nature.com/scientificreports OPEN Multi-modal survey of Adélie penguin mega-colonies reveals the Danger Islands as a seabird hotspot Received: 30 August 2017 Alex Borowicz 1, Philip McDowall1, Casey Youngfesh 1, Thomas Sayre-McCord2,3, Accepted: 20 February 2018 Gemma Clucas 4,5, Rachael Herman1,7, Steven Forrest6, Melissa Rider6, Mathew Schwaller1, Published: xx xx xxxx Tom Hart4, Stéphanie Jenouvrier 8,9, Michael J. Polito7,8, Hanumant Singh2 & Heather J. Lynch1 Despite concerted international efort to track and interpret shifts in the abundance and distribution of Adélie penguins, large populations continue to be identifed. Here we report on a major hotspot of Adélie penguin abundance identifed in the Danger Islands of the northern tip of the Antarctic Peninsula (AP). We present the frst complete census of Pygoscelis spp. penguins in the Danger Islands, estimated from a multi-modal survey consisting of direct ground counts and computer-automated counts of unmanned aerial vehicle (UAV) imagery. Our survey reveals that the Danger Islands host 751,527 pairs of Adélie penguins, more than the rest of AP region combined, and include the third and fourth largest Adélie penguin colonies in the world. Our results validate the use of Landsat medium- resolution satellite imagery for the detection of new or unknown penguin colonies and highlight the utility of combining satellite imagery with ground and UAV surveys. The Danger Islands appear to have avoided recent declines documented on the Western AP and, because they are large and likely to remain an important hotspot for avian abundance under projected climate change, deserve special consideration in the negotiation and design of Marine Protected Areas in the region.
    [Show full text]
  • Western Scotia Sea Margins: Improved Constraints on The
    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 111, B06101, doi:10.1029/2006JB004361, 2006 Click Here for Full Article Western Scotia Sea margins: Improved constraints on the opening of the Drake Passage Emanuele Lodolo,1 Federica Donda,1 and Alejandro Tassone2 Received 23 February 2006; accepted 7March 2006; published13June 2006. [ 1 ] We present arevised tectonic interpretation (from 28 Ma to 3.2 Ma) of the western sector of the Scotia Sea, incorporating new multichannel seismic reflection profiles and magnetic anomaly identifications for the continental margin offthe Tierra del Fuego Island, and available complementary data for the conjugate margin of the northwestern flank of the South Scotia Ridge. Seismic profiles show aremarkable diversity of the pair of conjugate passive margins of the western Scotia Sea in both their morphology and structural framework. The Tierra del Fuego continental margin can be related to aclassic rifted passive margin, while the southwestern margin of the Scotia Sea is characterized by steep slopes mostly generated by subvertical faults that abruptly separate the continental crust of the South Scotia Ridge from the oceanic crust of the western Scotia Sea. This structural difference was caused by intense strike-slip tectonism, mostly concentrated along the modern South Scotia Ridge since the early development of the western Scotia Sea. We find evidence for apreviously unrecognized magnetic anomaly 10 ( 28 Ma) at the foot of the Tierra del Fuego continental margin; the same anomaly is present at the conjugate northern flank of the South Scotia Ridge. The timing of events leading to the earliest development of the western Scotia Sea, which determined the opening of the Drake Passage is important because this gateway opening had aprofound effect on global circulation and climate.
    [Show full text]