Sherman Island Initial Environmental Evaluation
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The Ross Sea Dipole - Temperature, Snow Accumulation and Sea Ice Variability in the Ross Sea Region, Antarctica, Over the Past 2,700 Years
Clim. Past Discuss., https://doi.org/10.5194/cp-2017-95 Manuscript under review for journal Clim. Past Discussion started: 1 August 2017 c Author(s) 2017. CC BY 4.0 License. The Ross Sea Dipole - Temperature, Snow Accumulation and Sea Ice Variability in the Ross Sea Region, Antarctica, over the Past 2,700 Years 5 RICE Community (Nancy A.N. Bertler1,2, Howard Conway3, Dorthe Dahl-Jensen4, Daniel B. Emanuelsson1,2, Mai Winstrup4, Paul T. Vallelonga4, James E. Lee5, Ed J. Brook5, Jeffrey P. Severinghaus6, Taylor J. Fudge3, Elizabeth D. Keller2, W. Troy Baisden2, Richard C.A. Hindmarsh7, Peter D. Neff8, Thomas Blunier4, Ross Edwards9, Paul A. Mayewski10, Sepp Kipfstuhl11, Christo Buizert5, Silvia Canessa2, Ruzica Dadic1, Helle 10 A. Kjær4, Andrei Kurbatov10, Dongqi Zhang12,13, Ed D. Waddington3, Giovanni Baccolo14, Thomas Beers10, Hannah J. Brightley1,2, Lionel Carter1, David Clemens-Sewall15, Viorela G. Ciobanu4, Barbara Delmonte14, Lukas Eling1,2, Aja A. Ellis16, Shruthi Ganesh17, Nicholas R. Golledge1,2, Skylar Haines10, Michael Handley10, Robert L. Hawley15, Chad M. Hogan18, Katelyn M. Johnson1,2, Elena Korotkikh10, Daniel P. Lowry1, Darcy Mandeno1, Robert M. McKay1, James A. Menking5, Timothy R. Naish1, 15 Caroline Noerling11, Agathe Ollive19, Anaïs Orsi20, Bernadette C. Proemse18, Alexander R. Pyne1, Rebecca L. Pyne2, James Renwick1, Reed P. Scherer21, Stefanie Semper22, M. Simonsen4, Sharon B. Sneed10, Eric J., Steig3, Andrea Tuohy23, Abhijith Ulayottil Venugopal1,2, Fernando Valero-Delgado11, Janani Venkatesh17, Feitang Wang24, Shimeng -
Office of Polar Programs
DEVELOPMENT AND IMPLEMENTATION OF SURFACE TRAVERSE CAPABILITIES IN ANTARCTICA COMPREHENSIVE ENVIRONMENTAL EVALUATION DRAFT (15 January 2004) FINAL (30 August 2004) National Science Foundation 4201 Wilson Boulevard Arlington, Virginia 22230 DEVELOPMENT AND IMPLEMENTATION OF SURFACE TRAVERSE CAPABILITIES IN ANTARCTICA FINAL COMPREHENSIVE ENVIRONMENTAL EVALUATION TABLE OF CONTENTS 1.0 INTRODUCTION....................................................................................................................1-1 1.1 Purpose.......................................................................................................................................1-1 1.2 Comprehensive Environmental Evaluation (CEE) Process .......................................................1-1 1.3 Document Organization .............................................................................................................1-2 2.0 BACKGROUND OF SURFACE TRAVERSES IN ANTARCTICA..................................2-1 2.1 Introduction ................................................................................................................................2-1 2.2 Re-supply Traverses...................................................................................................................2-1 2.3 Scientific Traverses and Surface-Based Surveys .......................................................................2-5 3.0 ALTERNATIVES ....................................................................................................................3-1 -
(Bio)Chemical Complexity in Icy Satellites, with a Focus on Europa
Searching for (bio)chemical complexity in icy satellites, with a focus on Europa Contact Scientist: Olga Prieto-Ballesteros ([email protected]) Centro de Astrobiología (CSIC-INTA) Ctra. De Ajalvir km. 4, 28850 Torrejón de Ardoz. Madrid. Spain VOYAGE 2050. Searching for (bio)chemical complexity in icy satellites, with a focus on Europa TABLE OF CONTENTS TABLE OF CONTENTS 1 1. EXECUTIVE SUMMARY 2 2. THE SCIENCE QUESTION 3 2.1 BASIS OF THE STRATEGY TO SEARCH FOR LIFE IN THE SOLAR SYSTEM 3 2.2 THE SEARCH FOR COMPLEXITY 5 3. THE SPACE MISSION STRATEGY 7 3.1 MISSION DESTINATION: EUROPA 7 3.1.1 Main elements of the mission 8 3.1.2 Exploration of the plumes 10 3.2 THE MISSION IN A WORLDWIDE CONTEXT 11 4. TECHNOLOGICAL CHALLENGES 12 4.1 Europa orbiter 12 4.2 Europa lander 12 4.3 Europa ocean explorer 13 4.4 Europa jumper 14 4.5 Key Instrumentation 14 5. MEMBERS OF THE PROPOSER TEAM 16 6. REFERENCES 18 1 VOYAGE 2050. Searching for (bio)chemical complexity in icy satellites, with a focus on Europa SEARCHING FOR (BIO)CHEMICAL COMPLEXITY IN ICY SATELLITES, WITH A FOCUS ON EUROPA 1. EXECUTIVE SUMMARY Organic chemistry is ubiquitous in the Solar System. A significant repertoire of organic molecules has been detected in bodies outside the Earth (e.g., in meteorites, in cometary nuclei, on Mars or on icy moons), but none of the detected organic mixtures has enough complexity to indicate Life. There are a number of potentially habitable bodies in the solar system where water, chemical gradients and energy coexist, in particular Mars and the icy moons of the giant planets. -
Antarctic Primer
Antarctic Primer By Nigel Sitwell, Tom Ritchie & Gary Miller By Nigel Sitwell, Tom Ritchie & Gary Miller Designed by: Olivia Young, Aurora Expeditions October 2018 Cover image © I.Tortosa Morgan Suite 12, Level 2 35 Buckingham Street Surry Hills, Sydney NSW 2010, Australia To anyone who goes to the Antarctic, there is a tremendous appeal, an unparalleled combination of grandeur, beauty, vastness, loneliness, and malevolence —all of which sound terribly melodramatic — but which truly convey the actual feeling of Antarctica. Where else in the world are all of these descriptions really true? —Captain T.L.M. Sunter, ‘The Antarctic Century Newsletter ANTARCTIC PRIMER 2018 | 3 CONTENTS I. CONSERVING ANTARCTICA Guidance for Visitors to the Antarctic Antarctica’s Historic Heritage South Georgia Biosecurity II. THE PHYSICAL ENVIRONMENT Antarctica The Southern Ocean The Continent Climate Atmospheric Phenomena The Ozone Hole Climate Change Sea Ice The Antarctic Ice Cap Icebergs A Short Glossary of Ice Terms III. THE BIOLOGICAL ENVIRONMENT Life in Antarctica Adapting to the Cold The Kingdom of Krill IV. THE WILDLIFE Antarctic Squids Antarctic Fishes Antarctic Birds Antarctic Seals Antarctic Whales 4 AURORA EXPEDITIONS | Pioneering expedition travel to the heart of nature. CONTENTS V. EXPLORERS AND SCIENTISTS The Exploration of Antarctica The Antarctic Treaty VI. PLACES YOU MAY VISIT South Shetland Islands Antarctic Peninsula Weddell Sea South Orkney Islands South Georgia The Falkland Islands South Sandwich Islands The Historic Ross Sea Sector Commonwealth Bay VII. FURTHER READING VIII. WILDLIFE CHECKLISTS ANTARCTIC PRIMER 2018 | 5 Adélie penguins in the Antarctic Peninsula I. CONSERVING ANTARCTICA Antarctica is the largest wilderness area on earth, a place that must be preserved in its present, virtually pristine state. -
2019 Weddell Sea Expedition
Initial Environmental Evaluation SA Agulhas II in sea ice. Image: Johan Viljoen 1 Submitted to the Polar Regions Department, Foreign and Commonwealth Office, as part of an application for a permit / approval under the UK Antarctic Act 1994. Submitted by: Mr. Oliver Plunket Director Maritime Archaeology Consultants Switzerland AG c/o: Maritime Archaeology Consultants Switzerland AG Baarerstrasse 8, Zug, 6300, Switzerland Final version submitted: September 2018 IEE Prepared by: Dr. Neil Gilbert Director Constantia Consulting Ltd. Christchurch New Zealand 2 Table of contents Table of contents ________________________________________________________________ 3 List of Figures ___________________________________________________________________ 6 List of Tables ___________________________________________________________________ 8 Non-Technical Summary __________________________________________________________ 9 1. Introduction _________________________________________________________________ 18 2. Environmental Impact Assessment Process ________________________________________ 20 2.1 International Requirements ________________________________________________________ 20 2.2 National Requirements ____________________________________________________________ 21 2.3 Applicable ATCM Measures and Resolutions __________________________________________ 22 2.3.1 Non-governmental activities and general operations in Antarctica _______________________________ 22 2.3.2 Scientific research in Antarctica __________________________________________________________ -
S41467-018-05625-3.Pdf
ARTICLE DOI: 10.1038/s41467-018-05625-3 OPEN Holocene reconfiguration and readvance of the East Antarctic Ice Sheet Sarah L. Greenwood 1, Lauren M. Simkins2,3, Anna Ruth W. Halberstadt 2,4, Lindsay O. Prothro2 & John B. Anderson2 How ice sheets respond to changes in their grounding line is important in understanding ice sheet vulnerability to climate and ocean changes. The interplay between regional grounding 1234567890():,; line change and potentially diverse ice flow behaviour of contributing catchments is relevant to an ice sheet’s stability and resilience to change. At the last glacial maximum, marine-based ice streams in the western Ross Sea were fed by numerous catchments draining the East Antarctic Ice Sheet. Here we present geomorphological and acoustic stratigraphic evidence of ice sheet reorganisation in the South Victoria Land (SVL) sector of the western Ross Sea. The opening of a grounding line embayment unzipped ice sheet sub-sectors, enabled an ice flow direction change and triggered enhanced flow from SVL outlet glaciers. These relatively small catchments behaved independently of regional grounding line retreat, instead driving an ice sheet readvance that delivered a significant volume of ice to the ocean and was sustained for centuries. 1 Department of Geological Sciences, Stockholm University, Stockholm 10691, Sweden. 2 Department of Earth, Environmental and Planetary Sciences, Rice University, Houston, TX 77005, USA. 3 Department of Environmental Sciences, University of Virginia, Charlottesville, VA 22904, USA. 4 Department -
Basal Crevasses on the Larsen C Ice Shelf, Antarctica
GEOPHYSICAL RESEARCH LETTERS, VOL. 39, L16504, doi:10.1029/2012GL052413, 2012 Basal crevasses on the Larsen C Ice Shelf, Antarctica: Implications for meltwater ponding and hydrofracture Daniel McGrath,1 Konrad Steffen,1 Harihar Rajaram,2 Ted Scambos,3 Waleed Abdalati,1,4 and Eric Rignot5,6 Received 1 June 2012; revised 20 July 2012; accepted 23 July 2012; published 29 August 2012. [1] A key mechanism for the rapid collapse of both the Lar- thickness (due to the density difference between water and sen A and B Ice Shelves was meltwater-driven crevasse ice), fracturing the ice shelf into numerous elongate icebergs propagation. Basal crevasses, large-scale structural features [van der Veen, 1998, 2007; Scambos et al., 2003, 2009; within ice shelves, may have contributed to this mechanism in Weertman, 1973]. The narrow along-flow width and elon- three important ways: i) the shelf surface deforms due to gated across-flow length of these icebergs distinguishes them modified buoyancy and gravitational forces above the basal from tabular icebergs, and likely facilitates a positive feed- crevasse, creating >10 m deep compressional surface depres- back during the disintegration process, as elongate icebergs sions where meltwater can collect, ii) bending stresses from overturn and initiate further ice shelf calving [MacAyeal the modified shape drive surface crevassing, with crevasses et al., 2003; Guttenberg et al., 2011; Burton et al., 2012]. reaching 40 m in width, on the flanks of the basal-crevasse- [3] Dramatic atmospheric warming over the past five dec- induced trough and iii) the ice thickness is substantially ades has increased surface meltwater production along the reduced, thereby minimizing the propagation distance before a Antarctic Peninsula (AP) [Vaughan et al.,2003;van den full-thickness rift is created. -
Czech Research in Antarctica
Main Facts The Czech Johann Gregor Mendel Polar Station Building the Station CZECH RESEARCH IN ANTARCTICA james ross island precise position of the station the thawing landscape e island is located on the Atlantic side of the northernmost part of 63° 48’ 5.6’’S AND 57° 53’ 5.6’’W e entire island was covered by ice approximately 13,000 years ago. “Thanks to the building of the station we the Antarctic Peninsula, approximately between 63°45’ and 64°30’S, Conceived as a station to be operated in the Antarctic summer, from Since that time the ice covering the island thaws alternately slower and have become members of an elite club of 57°00’ and 58°30’W. the end of December to the beginning of March. At this time up to faster, although the island experienced periods when glaciation was countries doing research and other work in Antarctica. I’m delighted that the Czech Geologically the island is composed of cretaceous sediment (siltstone, fieen individuals can stay at the station. more extensive than today. Today the retreat of the ice has produced scientific programme was approved as sandstone, and conglomerate). On top of this surface appear volcanoes, e crew is quartered in the operational building, which is a wooden so-called “thawed oases”. Simply put, these are parts of the terrain that a high-quality project by the other countries which were active until the earlier Quaternary Period. Everything construction with perfect thermal insulation. e station is heated by seem to have been pulled from an enormous freezer and are gradually of the Antarctic Treaty. -
Thurston Island
RESEARCH ARTICLE Thurston Island (West Antarctica) Between Gondwana 10.1029/2018TC005150 Subduction and Continental Separation: A Multistage Key Points: • First apatite fission track and apatite Evolution Revealed by Apatite Thermochronology ‐ ‐ (U Th Sm)/He data of Thurston Maximilian Zundel1 , Cornelia Spiegel1, André Mehling1, Frank Lisker1 , Island constrain thermal evolution 2 3 3 since the Late Paleozoic Claus‐Dieter Hillenbrand , Patrick Monien , and Andreas Klügel • Basin development occurred on 1 2 Thurston Island during the Jurassic Department of Geosciences, Geodynamics of Polar Regions, University of Bremen, Bremen, Germany, British Antarctic and Early Cretaceous Survey, Cambridge, UK, 3Department of Geosciences, Petrology of the Ocean Crust, University of Bremen, Bremen, • ‐ Early to mid Cretaceous Germany convergence on Thurston Island was replaced at ~95 Ma by extension and continental breakup Abstract The first low‐temperature thermochronological data from Thurston Island, West Antarctica, ‐ fi Supporting Information: provide insights into the poorly constrained thermotectonic evolution of the paleo Paci c margin of • Supporting Information S1 Gondwana since the Late Paleozoic. Here we present the first apatite fission track and apatite (U‐Th‐Sm)/He data from Carboniferous to mid‐Cretaceous (meta‐) igneous rocks from the Thurston Island area. Thermal history modeling of apatite fission track dates of 145–92 Ma and apatite (U‐Th‐Sm)/He dates of 112–71 Correspondence to: Ma, in combination with kinematic indicators, geological -
Historical Behaviour of Dome C and Talos Dome (East Antarctica) As
Available online at www.sciencedirect.com Global and Planetary Change 60 (2008) 576–588 www.elsevier.com/locate/gloplacha Historical behaviour of Dome C and Talos Dome (East Antarctica) as investigated by snow accumulation and ice velocity measurements ⁎ Stefano Urbini a, Massimo Frezzotti b, , Stefano Gandolfi c, Christian Vincent d, Claudio Scarchilli b, Luca Vittuari c, Michel Fily d a Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, 00143 Roma, Italy b Ente per le Nuove Tecnologie, l'Energia e l'Ambiente, Via Anguillarese, 301, 00123 Roma, Italy c Dipartimento di Ingegneria delle Strutture, dei Trasporti, delle Acque, del Rilevamento, del Territorio, V.le Risorgimento 2, 40086 Bologna, Italy d Laboratoire de Glaciologie et Géophysique de l'Environnement, CNRS-UJF, 54 rue Molière, Grenoble, France Received 9 March 2007; accepted 14 August 2007 Available online 29 August 2007 Abstract Ice divide–dome behaviour is used for ice sheet mass balance studies and interpretation of ice core records. In order to characterize the historical behaviour (last 400 yr) of Dome C and Talos Dome (East Antarctica), ice velocities have been measured since 1996 using a GPS system, and the palaeo-spatial variability of snow accumulation has been surveyed using snow radar and firn cores. The snow accumulation distribution of both domes indicates distributions of accumulation that are non-symmetrical in relation to dome morphology. Changes in spatial distributions have been observed over the last few centuries, with a decrease in snow accumulation gradient along the wind direction at Talos Dome and a counter-clockwise rotation of accumulation distribution in the northern part of Dome C. -
Where Is the Best Site on Earth? Domes A, B, C, and F, And
Where is the best site on Earth? Saunders et al. 2009, PASP, 121, 976-992 Where is the best site on Earth? Domes A, B, C and F, and Ridges A and B Will Saunders1;2, Jon S. Lawrence1;2;3, John W.V. Storey1, Michael C.B. Ashley1 1School of Physics, University of New South Wales 2Anglo-Australian Observatory 3Macquarie University, New South Wales [email protected] Seiji Kato, Patrick Minnis, David M. Winker NASA Langley Research Center Guiping Liu Space Sciences Lab, University of California Berkeley Craig Kulesa Department of Astronomy and Steward Observatory, University of Arizona Saunders et al. 2009, PASP, 121 976992 Received 2009 May 26; accepted 2009 July 13; published 2009 August 20 ABSTRACT The Antarctic plateau contains the best sites on earth for many forms of astronomy, but none of the existing bases was selected with astronomy as the primary motivation. In this paper, we try to systematically compare the merits of potential observatory sites. We include South Pole, Domes A, C and F, and also Ridge B (running NE from Dome A), and what we call `Ridge A' (running SW from Dome A). Our analysis combines satellite data, published results and atmospheric models, to compare the boundary layer, weather, aurorae, airglow, precipitable water vapour, thermal sky emission, surface temperature, and the free atmosphere, at each site. We ¯nd that all Antarctic sites are likely to be compromised for optical work by airglow and aurorae. Of the sites with existing bases, Dome A is easily the best overall; but we ¯nd that Ridge A o®ers an even better site. -
Multi-Year Analysis of Distributed Glacier Mass Balance Modelling and Equilibrium Line Altitude on King George Island, Antarctic Peninsula
The Cryosphere, 12, 1211–1232, 2018 https://doi.org/10.5194/tc-12-1211-2018 © Author(s) 2018. This work is distributed under the Creative Commons Attribution 4.0 License. Multi-year analysis of distributed glacier mass balance modelling and equilibrium line altitude on King George Island, Antarctic Peninsula Ulrike Falk1,2, Damián A. López2,3, and Adrián Silva-Busso4,5 1Climate Lab, Institute for Geography, Bremen University, Bremen, Germany 2Center for Remote Sensing of Land Surfaces (ZFL), Bonn University, Bonn, Germany 3Institute of Geology and Mineralogy, University Cologne, Cologne, Germany 4Faculty of Exact and Natural Sciences, University Buenos Aires, Buenos Aires, Argentina 5Instituto Nacional de Agua (INA), Ezeiza, Buenos Aires, Argentina Correspondence: Ulrike Falk ([email protected]) Received: 12 October 2017 – Discussion started: 1 December 2017 Revised: 15 March 2018 – Accepted: 19 March 2018 – Published: 10 April 2018 Abstract. The South Shetland Islands are located at the seen over the course of the 5-year model run period. The win- northern tip of the Antarctic Peninsula (AP). This region ter accumulation does not suffice to compensate for the high was subject to strong warming trends in the atmospheric sur- variability in summer ablation. The results are analysed to as- face layer. Surface air temperature increased about 3K in sess changes in meltwater input to the coastal waters, specific 50 years, concurrent with retreating glacier fronts, an in- glacier mass balance and the equilibrium line altitude (ELA). crease in melt areas, ice surface lowering and rapid break- The Fourcade Glacier catchment drains into Potter cove, has up and disintegration of ice shelves.