Deep Ice-Core Drilling to 800 M at Dome a in East Antarctica
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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 -
China's Expanding Antarctic Interests
CHINA’S EXPANDING ANTARCTIC INTERESTS: IMPLICATIONS FOR NEW ZEALAND Professor Anne-Marie Brady1 | University of Canterbury | [email protected] Policy brief no. 2 | June 3, 2017 Presented at the conference: ‘Small States and the Changing Global Order: New Zealand Faces the Future’ at University of Canterbury, Christchurch, New Zealand, 3-4 June 2017 China is rapidly expanding its activities in Antarctica and some of its behaviour appears to breach the terms of the Antarctic Treaty. New Zealand must rethink its assessment of risk in Antarctica and devise a strategy to protect its interests there. Key findings • Some of China's interests and activities in Antarctica, which include undeclared military activities and mineral exploration, may be at odds with New Zealand strategic interests and they potentially breach international law. • China is rapidly expanding its presence in a triangle-shaped area it calls the "East Antarctic Sector" and has stated in policy documents that it reserves the right to make a claim in Antarctica. • New Zealand must rethink its assessment of risk in Antarctica and devise a strategy to protect its interests there. Executive summary China has rapidly expanded its activities in Antarctica and the Southern Ocean in recent years. The 2016 White Paper on Defence defines China as a "key strategic partner" for New Zealand.2 New Zealand has strong and expanding relations with China; while our top trading partners also have China as their major market. New Zealand benefits hugely from the economic opportunities associated with China's economic growth. At the same time, China's economic growth has funded a dramatic expansion in military capabilities and is challenging the longstanding strategic order in Northeast Asia and the Indo-Asia-Pacific. -
Site Testing Dome A, Antarctica
Site testing Dome A, Antarctica J.S. Lawrencea*, M.C.B. Ashleya, M.G. Burtona, X. Cuib, J.R. Everetta, B.T. Indermuehlea, S.L. Kenyona, D. Luong-Vana, A.M. Moorec, J.W.V. Storeya, A. Tokovinind, T. Travouillonc, C. Pennypackere, L. Wange, D. Yorkf aSchool of Physics, University of New South Wales, Australia bNanjing Institute of Astronomical Optics and Technology, China cCalifornia Institute of Technology, USA dCerro-Tololo Inter-American Observatories, Chile eLawrence Berkeley Lab, University of California/Berkeley, USA fUniversity of Chicago, USA ABSTRACT Recent data have shown that Dome C, on the Antarctic plateau, is an exceptional site for astronomy, with atmospheric conditions superior to those at any existing mid-latitude site. Dome C, however, may not be the best site on the Antarctic plateau for every kind of astronomy. The highest point of the plateau is Dome A, some 800 m higher than Dome C. It should experience colder atmospheric temperatures, lower wind speeds, and a turbulent boundary layer that is confined closer to the ground. The Dome A site was first visited in January 2005 via an overland traverse, conducted by the Polar Research Institute of China. The PRIC plans to return to the site to establish a permanently manned station within the next decade. The University of New South Wales, in collaboration with a number of international institutions, is currently developing a remote automated site testing observatory for deployment to Dome A in the 2007/8 austral summer as part of the International Polar Year. This self-powered observatory will be equipped with a suite of site testing instruments measuring turbulence, optical and infrared sky background, and sub-millimetre transparency. -
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. -
Magazine Issue 32 2017
AUSTRALIAN ANTARCTIC MAGAZINE ISSUE 32 2017 ANTARCTICA valued, protected and understood www.antarctica.gov.au The Australian Antarctic Division, a Division of the Department of the Environment and Energy, leads Australia’s Antarctic program and seeks to advance Australia’s Antarctic interests in pursuit of its vision of having ‘Antarctica valued, protected and understood’. It does this by managing Australian government activity in Antarctica, providing transport and logistic support to Australia’s Antarctic research program, maintaining four permanent Australian research stations, and conducting scientific research programs both on land and in the Southern Ocean. Australia’s Antarctic national interests are to: • Preserve our sovereignty over the Australian Antarctic Territory, including our sovereign rights over the adjacent From the OPERATIONS offshore areas. 5 A taste for shipping • Take advantage of the special opportunities Antarctica offers for scientific research. Director SCIENCE • Protect the Antarctic environment, having regard to its special qualities and effects on our region. 19 ‘Whale cams’ reveal secret • Maintain Antarctica’s freedom from strategic and/or life of ocean giants political confrontation. As this magazine went to press, entries for the “Name our Icebreaker” • Be informed about and able to influence developments in a competition were flooding in from schools around Australia. The region geographically proximate to Australia. competition is a unique and exciting opportunity for Australian • Derive any reasonable economic benefits from living and students in grades 5 to 8 to play a role in Australia’s Antarctic history non-living resources of the Antarctic (excluding deriving such benefits from mining and oil drilling). and to learn more about the Australian Antarctic Program through associated classroom materials aligned with the curriculum. -
Download Factsheet
Antarctic Factsheet Geographical Statistics May 2005 AREA % of total Antarctica - including ice shelves and islands 13,829,430km2 100.00% (Around 58 times the size of the UK, or 1.4 times the size of the USA) Antarctica - excluding ice shelves and islands 12,272,800km2 88.74% Area ice free 44,890km2 0.32% Ross Ice Shelf 510,680km2 3.69% Ronne-Filchner Ice Shelf 439,920km2 3.18% LENGTH Antarctic Peninsula 1,339km Transantarctic Mountains 3,300km Coastline* TOTAL 45,317km 100.00% * Note: coastlines are fractal in nature, so any Ice shelves 18,877km 42.00% measurement of them is dependant upon the scale at which the data is collected. Coastline Rock 5,468km 12.00% lengths here are calculated from the most Ice coastline 20,972km 46.00% detailed information available. HEIGHT Mean height of Antarctica - including ice shelves 1,958m Mean height of Antarctica - excluding ice shelves 2,194m Modal height excluding ice shelves 3,090m Highest Mountains 1. Mt Vinson (Ellsworth Mts.) 4,892m 2. Mt Tyree (Ellsworth Mts.) 4,852m 3. Mt Shinn (Ellsworth Mts.) 4,661m 4. Mt Craddock (Ellsworth Mts.) 4,650m 5. Mt Gardner (Ellsworth Mts.) 4,587m 6. Mt Kirkpatrick (Queen Alexandra Range) 4,528m 7. Mt Elizabeth (Queen Alexandra Range) 4,480m 8. Mt Epperly (Ellsworth Mts) 4,359m 9. Mt Markham (Queen Elizabeth Range) 4,350m 10. Mt Bell (Queen Alexandra Range) 4,303m (In many case these heights are based on survey of variable accuracy) Nunatak on the Antarctic Peninsula 1/4 www.antarctica.ac.uk Antarctic Factsheet Geographical Statistics May 2005 Other Notable Mountains 1. -
Where Is the Best Site on Earth? Domes A, B, C and F, and Ridges a and B
Where is the best site on Earth? Domes A, B, C and F, and Ridges A and B Will Saunders' 2 , Jon S. Lawrence' 2 3 , John W.V. Storey', Michael C.B. Ashley' 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 ABSTRACT The Antarctic plateau contains the best sites on earth for many forms of astronomy, but none of the existing bases were 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, free atmosphere, sky brightness, pecipitable water vapour, and surface temperature at each site. We find that all Antarctic sites are likely compromised for optical work by airglow and aurorae. Of the sites with existing bases, Dome A is the best overall; but we find that Ridge A offers an even better site. We also find that Dome F is a remarkably good site. Dome C is less good as a thermal infrared or terahertz site, but would be able to take advantage of a predicted ‘OH hole’ over Antarctica during Spring. -
Reporting to the Asia Pacific Fire Protection and Fire Service Industry
REPORTING TO THE ASIA PACIFIC FIRE PROTECTION AND FIRE SERVICE INDUSTRY www.apfmag.com Issue 59 • October 2016 NFPA #1964 Compliant Wildland Fire Industrial Fire Water Supply Handheld Nozzles ® TASK FORCE TIPS® FIRE FIGHTING EQUIPMENT Fire Apparatus Equipment Foam Equipment 3701 INNOVATION WAY MADE IN USA VALPARAISO, IN U.S.A. +1.219.548.4000 www.tft.com www.newforce.tft.com REPORTING TO THE ASIA PACIFIC FIRE PROTECTION AND FIRE SERVICE INDUSTRY Contents OCTOBER 2016 REGULARS. 5 Editors Comment 7 Industry Comment www.apfmag.com Issue 59 • October 2016 8 News and Profiles OCTOBER 2016 • ISSUE 59 Cover image: Dual pressure automatic nozzles, such FEATURES. as the MidForce nozzle shown here, provide maximum stream reach and penetration in high pressure mode, and maximum flow when the low pressure mode is 24 Emergency response in Antarctica selected. Image courtesy of S. Haase. Publishers 31 Firefighting foam concentrates Mark Seton [email protected] 24 – the constant evolution: Part 2 David Staddon [email protected] Editor 36 Improving survival for ‘out Neil Bibby ASFM, FAICD, MIFireE [email protected] of hospital’ cardiac arrest Contributing Editors Rhonda Abotomey, Martin Boyle, Penny Burns, 41 Gaseous fire suppression systems Javier Castro, Chris Chiesa, Ed Comeau, Robert Fawcett, David J. Ganz, Jeff Kepert, Thomas Loridan, – understanding safety measures Torbjorn Lundmark, Michelle Murphy, Steve O’Malley, Gary Parkinson, Ange Pestell, Peter Ryan, Brett Shields, Brett Staines, Deb Symons, Melanie Taylor, William Thurston, Kevin Tory, 48 Women and Firefighting Australasia Bronwyn Walker, Joel Ward, Duncan J. White. 2016: Right place. Right time Design Manager Richard Parsons [email protected] 55 Protective clothing and Web and IT Manager equipment for Fire Fighters Neil Spinney [email protected] 59 A hands on approach International Sales 36 Mark Seton TECHNOLOGY IS SECURITY. -
Site Testing for Submillimetre Astronomy at Dome C, Antarctica
A&A 535, A112 (2011) Astronomy DOI: 10.1051/0004-6361/201117345 & c ESO 2011 Astrophysics Site testing for submillimetre astronomy at Dome C, Antarctica P. Tremblin1, V. Minier1, N. Schneider1, G. Al. Durand1,M.C.B.Ashley2,J.S.Lawrence2, D. M. Luong-Van2, J. W. V. Storey2,G.An.Durand3,Y.Reinert3, C. Veyssiere3,C.Walter3,P.Ade4,P.G.Calisse4, Z. Challita5,6, E. Fossat6,L.Sabbatini5,7, A. Pellegrini8, P. Ricaud9, and J. Urban10 1 Laboratoire AIM Paris-Saclay (CEA/Irfu, Univ. Paris Diderot, CNRS/INSU), Centre d’études de Saclay, 91191 Gif-Sur-Yvette, France e-mail: [pascal.tremblin;vincent.minier]@cea.fr 2 University of New South Wales, 2052 Sydney, Australia 3 Service d’ingénierie des systèmes, CEA/Irfu, Centre d’études de Saclay, 91191 Gif-Sur-Yvette, France 4 School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff, CF24 3AA, UK 5 Concordia Station, Dome C, Antarctica 6 Laboratoire Fizeau (Obs. Côte d’Azur, Univ. Nice Sophia Antipolis, CNRS/INSU), Parc Valrose, 06108 Nice, France 7 Departement of Physics, University of Roma Tre, Italy 8 Programma Nazionale Ricerche in Antartide, ENEA, Rome Italy 9 Laboratoire d’Aérologie, UMR 5560 CNRS, Université Paul-Sabatier, 31400 Toulouse, France 10 Chalmers University of Technology, Department of Earth and Space Sciences, 41296 Göteborg, Sweden Received 25 May 2011 / Accepted 17 October 2011 ABSTRACT Aims. Over the past few years a major effort has been put into the exploration of potential sites for the deployment of submillimetre astronomical facilities. Amongst the most important sites are Dome C and Dome A on the Antarctic Plateau, and the Chajnantor area in Chile. -
The Opening of the Transpolar Sea Route: Logistical, Geopolitical, Environmental, and Socioeconomic Impacts
Marine Policy xxx (xxxx) xxx Contents lists available at ScienceDirect Marine Policy journal homepage: http://www.elsevier.com/locate/marpol The opening of the Transpolar Sea Route: Logistical, geopolitical, environmental, and socioeconomic impacts Mia M. Bennett a,*, Scott R. Stephenson b, Kang Yang c,d,e, Michael T. Bravo f, Bert De Jonghe g a Department of Geography and School of Modern Languages & Cultures (China Studies Programme), Room 8.09, Jockey Club Tower, Centennial Campus, The University of Hong Kong, Hong Kong b RAND Corporation, Santa Monica, CA, USA c School of Geography and Ocean Science, Nanjing University, Nanjing, 210023, China d Jiangsu Provincial Key Laboratory of Geographic Information Science and Technology, Nanjing, 210023, China e Collaborative Innovation Center for the South Sea Studies, Nanjing University, Nanjing, 210023, China f Scott Polar Research Institute, University of Cambridge, Cambridge, UK g Graduate School of Design, Harvard University, Cambridge, MA, USA ABSTRACT With current scientifc models forecasting an ice-free Central Arctic Ocean (CAO) in summer by mid-century and potentially earlier, a direct shipping route via the North Pole connecting markets in Asia, North America, and Europe may soon open. The Transpolar Sea Route (TSR) would represent a third Arctic shipping route in addition to the Northern Sea Route and Northwest Passage. In response to the continued decline of sea ice thickness and extent and growing recognition within the Arctic and global governance communities of the need to anticipate -
“O 3 Enhancement Events” (Oees) at Dome A, East Antarctica
Discussions https://doi.org/10.5194/essd-2020-130 Earth System Preprint. Discussion started: 5 August 2020 Science c Author(s) 2020. CC BY 4.0 License. Open Access Open Data Year-round record of near-surface ozone and “O3 enhancement events” (OEEs) at Dome A, East Antarctica Minghu Ding1,2,*, Biao Tian1,*, Michael C. B. Ashley3, Davide Putero4, Zhenxi Zhu5, Lifan Wang5, Shihai Yang6, Chuanjin Li2, Cunde Xiao2, 7 5 1State Key Laboratory of Severe Weather, Chinese Academy of Meteorological Sciences, Beijing 100081, China 2State Key Laboratory of Cryospheric Science, Northwest Institute of Eco-Environment and Resources, Chinese Academy of Sciences, Lanzhou 730000, China 3School of Physics, University of New South Wales, Sydney 2052, Australia 4CNR–ISAC, National Research Council of Italy, Institute of Atmospheric Sciences and Climate, via Gobetti 101, 40129, 10 Bologna, Italy 5Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210034, China 6Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China 7State Key Laboratory of Earth Surface Processes and Resource Ecology, Beijing Normal University, Beijing 100875, China *These authors contributed equally to this work. 15 Correspondence to: Minghu Ding ([email protected]) Abstract. Dome A, the summit of the east Antarctic Ice Sheet, is an area challenging to access and is one of the harshest environments on Earth. Up until recently, long term automated observations from Dome A were only possible with very low power instruments such as a basic meteorological station. To evaluate the characteristics of near-surface O3, continuous observations were carried out in 2016. Together with observations at the Amundsen-Scott Station (South Pole – SP) and 20 Zhongshan Station (ZS, on the southeast coast of Prydz Bay), the seasonal and diurnal O3 variabilities were investigated. -
Astronomy Within Antarctica
Astronomy within Antarctica The past and the present Nianqi Tang (Petra) December 2010 1 Table of contents Abstract 1 Introduction 1.1 General information on Antarctica 1.2 Past and Present Astronomy sites 2 Advantages of carrying out Astronomical activities in Antarctica 2.1 Atmospheric stability 2.2 Temperature 2.3 Air conditions 2.4 Low seismic activity 2.5 Low level of aerosols 2.6 Continuous observing 2.7 Low artificial light pollution 2.8 Financial aspects 2.9 Contributions 3 Disadvantages of carrying out Astronomical activities in Antarctica 3.1 Sky coverage 3.2 Limited access (maintenance) 3.3 Long periods of twilight 3.4 Pollution (Moon light) 3.5 Environmental and instrumental limitation 3.6 Personnel aspects 3.7 Anomolies 4 The future of Antarctic astronomy 2 Abstract Early astronomy activities were not practiced until the 1950s, however today the activities are undergoing at four plateau sites: the Amundsen-Scott South Pole Station, Concordia Station at Dome A, Kunlun Station at Dome A and Fuji Station at Dome F, in addition to the long duration ballooning from the coastal station of McMurdo, at stations run by the USA, France / Italy, China, Japan and the USA respectively (Indermuehle et al. 2004). All these programs are operating with great difficulties due to natural environment and technology limitations; however the temptation of the ideal astronomical laboratory has always been the driving force to astronomers to overcome the difficulties. This review presents a general introduction of Antarctic astronomy, and discusses the advantages and disadvantages of conducting astronomy in Antarctica. At last, the review will summerise the achivements of the past astronomy researches, and looks at the future of astronomy in Antarctica.