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T Antarctic Ce Sheet Itiative
race Publication 3115, Vol. 1 t Antarctic ce Sheet itiative :_,.me.-1: Science and ;mentation Plan iv-_J_ E -- --__o • E _-- rz " _ • _ _v_-- . "2-. .... E _ ____ __ _k - -- - ...... --rr r_--_.-- .... m-- _ £3._= --- - • ,r- ..... _ k • -- ..... __= ---- = ............ --_ m -- -- ..... Z Im .... r .... _,... ___ "--. 11 1"1 I' I i ¸ NASA Conference Publication 3115, Vol. 1 West Antarctic Ice Sheet Initiative Volume 1: Science and Implementation Plan Edited by Robert A. Bindschadler NASA Goddard Space Flight Center Greenbelt, Maryland Proceedings of a workshop cosponsored by the National Aeronautics and Space Administration, Washington, D.C., and the National Science Foundation, Washington, D.C., and held at Goddard Space Flight Center Greenbelt, Maryland October 16-18, 1990 IXl/_/X National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1991 CONTENTS Page Preface v Workshop Participants vi Acknowledgements vii Map viii 1. Executive Summary 1 2. Climatic Importance of Ice Sheets 4 3. Marine Ice Sheet Instability 5 4. The West Antarctic Ice Sheet Initiative 6 4.1 Goal and Objectives 6 4.2 A Multidisciplinary Project 7 4.3 Scientific Focus: A Single Goal 7 4.4 Geographic Focus: West Antarctica 7 4.5 Duration: A Phased Approach 8 5. Science Plan 10 5.1 Glaciology 10 5.1.1 Ice Dynamics 10 5.1.2 Ice Cores 16 5.2 Meteorology 19 5.3 Oceanography 23 5.4 Geology and Geophysics 27 5.4.1 Terrestrial Geology 27 5.4.2 Marine Geology and Geophysics 28 5.4.3 Subglacial Geology and Geophysics 30 6. -
Lecture 21: Glaciers and Paleoclimate Read: Chapter 15 Homework Due Thursday Nov
Learning Objectives (LO) Lecture 21: Glaciers and Paleoclimate Read: Chapter 15 Homework due Thursday Nov. 12 What we’ll learn today:! 1. 1. Glaciers and where they occur! 2. 2. Compare depositional and erosional features of glaciers! 3. 3. Earth-Sun orbital parameters, relevance to interglacial periods ! A glacier is a river of ice. Glaciers can range in size from: 100s of m (mountain glaciers) to 100s of km (continental ice sheets) Most glaciers are 1000s to 100,000s of years old! The Snowline is the lowest elevation of a perennial (2 yrs) snow field. Glaciers can only form above the snowline, where snow does not completely melt in the summer. Requirements: Cold temperatures Polar latitudes or high elevations Sufficient snow Flat area for snow to accumulate Permafrost is permanently frozen soil beneath a seasonal active layer that supports plant life Glaciers are made of compressed, recrystallized snow. Snow buildup in the zone of accumulation flows downhill into the zone of wastage. Glacier-Covered Areas Glacier Coverage (km2) No glaciers in Australia! 160,000 glaciers total 47 countries have glaciers 94% of Earth’s ice is in Greenland and Antarctica Mountain Glaciers are Retreating Worldwide The Antarctic Ice Sheet The Greenland Ice Sheet Glaciers flow downhill through ductile (plastic) deformation & by basal sliding. Brittle deformation near the surface makes cracks, or crevasses. Antarctic ice sheet: ductile flow extends into the ocean to form an ice shelf. Wilkins Ice shelf Breakup http://www.youtube.com/watch?v=XUltAHerfpk The Greenland Ice Sheet has fewer and smaller ice shelves. Erosional Features Unique erosional landforms remain after glaciers melt. -
Rapid Cenozoic Glaciation of Antarctica Induced by Declining
letters to nature 17. Huang, Y. et al. Logic gates and computation from assembled nanowire building blocks. Science 294, Early Cretaceous6, yet is thought to have remained mostly ice-free, 1313–1317 (2001). 18. Chen, C.-L. Elements of Optoelectronics and Fiber Optics (Irwin, Chicago, 1996). vegetated, and with mean annual temperatures well above freezing 4,7 19. Wang, J., Gudiksen, M. S., Duan, X., Cui, Y. & Lieber, C. M. Highly polarized photoluminescence and until the Eocene/Oligocene boundary . Evidence for cooling and polarization sensitive photodetectors from single indium phosphide nanowires. Science 293, the sudden growth of an East Antarctic Ice Sheet (EAIS) comes 1455–1457 (2001). from marine records (refs 1–3), in which the gradual cooling from 20. Bagnall, D. M., Ullrich, B., Sakai, H. & Segawa, Y. Micro-cavity lasing of optically excited CdS thin films at room temperature. J. Cryst. Growth. 214/215, 1015–1018 (2000). the presumably ice-free warmth of the Early Tertiary to the cold 21. Bagnell, D. M., Ullrich, B., Qiu, X. G., Segawa, Y. & Sakai, H. Microcavity lasing of optically excited ‘icehouse’ of the Late Cenozoic is punctuated by a sudden .1.0‰ cadmium sulphide thin films at room temperature. Opt. Lett. 24, 1278–1280 (1999). rise in benthic d18O values at ,34 million years (Myr). More direct 22. Huang, Y., Duan, X., Cui, Y. & Lieber, C. M. GaN nanowire nanodevices. Nano Lett. 2, 101–104 (2002). evidence of cooling and glaciation near the Eocene/Oligocene 8 23. Gudiksen, G. S., Lauhon, L. J., Wang, J., Smith, D. & Lieber, C. M. Growth of nanowire superlattice boundary is provided by drilling on the East Antarctic margin , structures for nanoscale photonics and electronics. -
Asynchronous Antarctic and Greenland Ice-Volume Contributions to the Last Interglacial Sea-Level Highstand
ARTICLE https://doi.org/10.1038/s41467-019-12874-3 OPEN Asynchronous Antarctic and Greenland ice-volume contributions to the last interglacial sea-level highstand Eelco J. Rohling 1,2,7*, Fiona D. Hibbert 1,7*, Katharine M. Grant1, Eirik V. Galaasen 3, Nil Irvalı 3, Helga F. Kleiven 3, Gianluca Marino1,4, Ulysses Ninnemann3, Andrew P. Roberts1, Yair Rosenthal5, Hartmut Schulz6, Felicity H. Williams 1 & Jimin Yu 1 1234567890():,; The last interglacial (LIG; ~130 to ~118 thousand years ago, ka) was the last time global sea level rose well above the present level. Greenland Ice Sheet (GrIS) contributions were insufficient to explain the highstand, so that substantial Antarctic Ice Sheet (AIS) reduction is implied. However, the nature and drivers of GrIS and AIS reductions remain enigmatic, even though they may be critical for understanding future sea-level rise. Here we complement existing records with new data, and reveal that the LIG contained an AIS-derived highstand from ~129.5 to ~125 ka, a lowstand centred on 125–124 ka, and joint AIS + GrIS contributions from ~123.5 to ~118 ka. Moreover, a dual substructure within the first highstand suggests temporal variability in the AIS contributions. Implied rates of sea-level rise are high (up to several meters per century; m c−1), and lend credibility to high rates inferred by ice modelling under certain ice-shelf instability parameterisations. 1 Research School of Earth Sciences, The Australian National University, Canberra, ACT 2601, Australia. 2 Ocean and Earth Science, University of Southampton, National Oceanography Centre, Southampton SO14 3ZH, UK. 3 Department of Earth Science and Bjerknes Centre for Climate Research, University of Bergen, Allegaten 41, 5007 Bergen, Norway. -
West Antarctic Ice Sheet Divide Ice Core Climate, Ice Sheet History, Cryobiology
QUARTERLY UPDATE August 2009 West Antarctic Ice Sheet Divide Ice Core Climate, Ice Sheet History, Cryobiology 2009/2010 Field Operations Our main objectives for the coming field season are: 1) To ship ice from 680 to ~2,100 m to NICL 2) Recover core to a depth of 2,600 to 2,900 m The U.S. Antarctic Program will be establishing a multi year field camp at Byrd this season to support field operations around Pine Island Bay and elsewhere in West Antarctica. The camp at Byrd will complicate our logistics because the heavy equipment that will prepare the Byrd skiway will be flown to WAIS Divide and driven to Byrd, and a camp at Byrd will make for more competition for flights. But this is a much better plan than supporting those operations out of WAIS Divide, which would have increased the WAIS Divide population to 100 people. Other science activities at WAIS Divide this season include the following: CReSIS ground traverse to Pine Island Bay Flow dynamics of two Amundsen Sea glaciers: Thwaites and Pine Island. PI: Anandakrishnan Ocean-Ice Interaction in the Amundsen Sea sector of West Antarctica. PI: Joughin Space physics magnetometer. PI: Zesta Antarctic Automatic Weather Station Program. PI: Weidner Polar Experiment Network for Geospace Upper atmosphere Investigations. PI: Lessard Artist, paintings of ice and glacial features. PI: McKee IDDO is making several modifications to the drill that should increase the amount of core that can be recovered each time the drill is lowered into the hole, which will increase the amount of ice we can recover this season. -
Mount Harding, Grove Mountains, East Antarctica
MEASURE 2 - ANNEX Management Plan for Antarctic Specially Protected Area No 168 MOUNT HARDING, GROVE MOUNTAINS, EAST ANTARCTICA 1. Introduction The Grove Mountains (72o20’-73o10’S, 73o50’-75o40’E) are located approximately 400km inland (south) of the Larsemann Hills in Princess Elizabeth Land, East Antarctica, on the eastern bank of the Lambert Rift(Map A). Mount Harding (72°512 -72°572 S, 74°532 -75°122 E) is the largest mount around Grove Mountains region, and located in the core area of the Grove Mountains that presents a ridge-valley physiognomies consisting of nunataks, trending NNE-SSW and is 200m above the surface of blue ice (Map B). The primary reason for designation of the Area as an Antarctic Specially Protected Area is to protect the unique geomorphological features of the area for scientific research on the evolutionary history of East Antarctic Ice Sheet (EAIS), while widening the category in the Antarctic protected areas system. Research on the evolutionary history of EAIS plays an important role in reconstructing the past climatic evolution in global scale. Up to now, a key constraint on the understanding of the EAIS behaviour remains the lack of direct evidence of ice sheet surface levels for constraining ice sheet models during known glacial maxima and minima in the post-14 Ma period. The remains of the fluctuation of ice sheet surface preserved around Mount Harding, will most probably provide the precious direct evidences for reconstructing the EAIS behaviour. There are glacial erosion and wind-erosion physiognomies which are rare in nature and extremely vulnerable, such as the ice-core pyramid, the ventifact, etc. -
36. Comparison of Winter and Summer Growth Stages of the Diatom Eucampia Antarctica from the Kerguelen Plateau and South of the Antarctic Convergence Zone1
Barron, J., Larsen, B., et al., 1991 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 119 36. COMPARISON OF WINTER AND SUMMER GROWTH STAGES OF THE DIATOM EUCAMPIA ANTARCTICA FROM THE KERGUELEN PLATEAU AND SOUTH OF THE ANTARCTIC CONVERGENCE ZONE1 Greta A. Fryxell2 ABSTRACT On ODP Leg 119, specimens collected of Eucampia antarctica (Castracane) Mangin var. antarctica exhibited mor- phological and distribution patterns that contrasted with those of Eucampia antarctica var. recta (Mangin) G. Fryxell et Prasad. E. antarctica var. antarctica was found over the northern Kerguelen Plateau, north of the summer Antarctic Convergence Zone, in the subpolar plankton and in the sediments. E. antarctica var. recta was found close to the conti- nent in Prydz Bay. It was also collected near and under the ice in the northern Weddell Sea on a National Science Foun- dation Division of Polar Programs project (1983-1988). A key feature for distinguishing the two varieties in the field is the growth habit, with curvature in broad girdle view of the nominate, subpolar variety in both the winter stage and the more lightly silicified summer stage. A low ratio of terminal to intercalary valves results from the repeated division of the original doublets into chains of considerable length of the winter stage. Small spines around the elevations of one valve serve to clasp the sibling valve and maintain the chain formation. Cells of E. antarctica var. recta tend to be somewhat larger than E. antarctica var. antarctica, and they form chains that are straight in broad girdle view but slightly curved in narrow girdle view. -
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. -
The Antarctic Contribution to Holocene Global Sea Level Rise
The Antarctic contribution to Holocene global sea level rise Olafur Ing6lfsson & Christian Hjort The Holocene glacial and climatic development in Antarctica differed considerably from that in the Northern Hemisphere. Initial deglaciation of inner shelf and adjacent land areas in Antarctica dates back to between 10-8 Kya, when most Northern Hemisphere ice sheets had already disappeared or diminished considerably. The continued deglaciation of currently ice-free land in Antarctica occurred gradually between ca. 8-5 Kya. A large southern portion of the marine-based Ross Ice Sheet disintegrated during this late deglaciation phase. Some currently ice-free areas were deglaciated as late as 3 Kya. Between 8-5 Kya, global glacio-eustatically driven sea level rose by 10-17 m, with 4-8 m of this increase occurring after 7 Kya. Since the Northern Hemisphere ice sheets had practically disappeared by 8-7 Kya, we suggest that Antarctic deglaciation caused a considerable part of the global sea level rise between 8-7 Kya, and most of it between 7-5 Kya. The global mid-Holocene sea level high stand, broadly dated to between 84Kya, and the Littorina-Tapes transgressions in Scandinavia and simultaneous transgressions recorded from sites e.g. in Svalbard and Greenland, dated to 7-5 Kya, probably reflect input of meltwater from the Antarctic deglaciation. 0. Ingcilfsson, Gotlienburg Universiw, Earth Sciences Centre. Box 460, SE-405 30 Goteborg, Sweden; C. Hjort, Dept. of Quaternary Geology, Lund University, Sdvegatan 13, SE-223 62 Lund, Sweden. Introduction dated to 20-17 Kya (thousands of years before present) in the western Ross Sea area (Stuiver et al. -
Glacier (And Ice Sheet) Mass Balance
Glacier (and ice sheet) Mass Balance The long-term average position of the highest (late summer) firn line ! is termed the Equilibrium Line Altitude (ELA) Firn is old snow How an ice sheet works (roughly): Accumulation zone ablation zone ice land ocean • Net accumulation creates surface slope Why is the NH insolation important for global ice• sheetSurface advance slope causes (Milankovitch ice to flow towards theory)? edges • Accumulation (and mass flow) is balanced by ablation and/or calving Why focus on summertime? Ice sheets are very sensitive to Normal summertime temperatures! • Ice sheet has parabolic shape. • line represents melt zone • small warming increases melt zone (horizontal area) a lot because of shape! Slightly warmer Influence of shape Warmer climate freezing line Normal freezing line ground Furthermore temperature has a powerful influence on melting rate Temperature and Ice Mass Balance Summer Temperature main factor determining ice growth e.g., a warming will Expand ablation area, lengthen melt season, increase the melt rate, and increase proportion of precip falling as rain It may also bring more precip to the region Since ablation rate increases rapidly with increasing temperature – Summer melting controls ice sheet fate* – Orbital timescales - Summer insolation must control ice sheet growth *Not true for Antarctica in near term though, where it ʼs too cold to melt much at surface Temperature and Ice Mass Balance Rule of thumb is that 1C warming causes an additional 1m of melt (see slope of ablation curve at right) -
Open-File Report 2007-1047, Extended Abstracts
U.S. Geological Survey Open-File Report 2007-1047 Antarctica: A Keystone in a Changing World—Online Proceedings for the 10th International Symposium on Antarctic Earth Sciences Santa Barbara, California, U.S.A.—August 26 to September 1, 2007 Edited by Alan Cooper, Carol Raymond, and the 10th ISAES Editorial Team 2007 Extended Abstracts Extended Abstract 001 http://pubs.usgs.gov/of/2007/1047/ea/of2007-1047ea001.pdf Ross Aged Ductile Shearing in the Granitic Rocks of the Wilson Terrane, Deep Freeze Range area, north Victoria Land (Antarctica) by Federico Rossetti, Gianluca Vignaroli, Fabrizio Balsamo, and Thomas Theye Extended Abstract 002 http://pubs.usgs.gov/of/2007/1047/ea/of2007-1047ea002.pdf Postcollisional Magmatism of the Ross Orogeny (Victoria Land, Antarctica): a Granite- Lamprophyre Genetic Link S. Rocchi, G. Di Vincenzo, C. Ghezzo, and I. Nardini Extended Abstract 003 http://pubs.usgs.gov/of/2007/1047/ea/of2007-1047ea003.pdf Age of Boron- and Phosphorus-Rich Paragneisses and Associated Orthogneisses, Larsemann Hills: New Constraints from SHRIMP U-Pb Zircon Geochronology by C. J. Carson, E.S. Grew, S.D. Boger, C.M. Fanning and A.G. Christy Extended Abstract 004 http://pubs.usgs.gov/of/2007/1047/ea/of2007-1047ea004.pdf Terrane Correlation between Antarctica, Mozambique and Sri Lanka: Comparisons of Geochronology, Lithology, Structure And Metamorphism G.H. Grantham, P.H. Macey, B.A. Ingram, M.P. Roberts, R.A. Armstrong, T. Hokada, K. by Shiraishi, A. Bisnath, and V. Manhica Extended Abstract 005 http://pubs.usgs.gov/of/2007/1047/ea/of2007-1047ea005.pdf New Approaches and Progress in the Use of Polar Marine Diatoms in Reconstructing Sea Ice Distribution by A. -
Climate Change and Southern Ocean Resilience
No.No. 52 5 l l JuneMay 20202021 POLARKENNAN PERSPECTIVES CABLE Adélie penguins on top of an ice flow near the Antarctic Peninsula. © Jo Crebbin/Shutterstock Climate Change and Southern Ocean Resilience REPORT FROM AN INTERDISCIPLINARY SCIENTIFIC WORKSHOP, MARCH 30, 2021 Andrea Capurroi, Florence Colleoniii, Rachel Downeyiii, Evgeny Pakhomoviv, Ricardo Rourav, Anne Christiansonvi i. Boston University Frederick S. Pardee Center for the Study of the Longer-Range Future ii. Istituto Nazionale di Oceanografia e di Geofisica Sperimentale Antarctic and Southern Ocean Coalition iii. Australian National University iv. University of British Columbia v. Antarctic and Southern Ocean Coalition vi. The Pew Charitable Trusts CONTENTS I. INTRODUCTION BY EVAN T. BLOOM 3 II. EXECUTIVE SUMMARY 5 III. CLIMATE CHANGE AND SOUTHERN OCEAN RESILIENCE 7 A. CLIMATE CHANGE AND THE SOUTHERN OCEAN 7 B. CONNECTION OF REGIONAL SOUTHERN OCEAN PROCESS TO GLOBAL SYSTEMS 9 C. UNDERSTANDING PROCESS CHANGES IN THE SOUTHERN OCEAN 10 D. ANTARCTIC GOVERNANCE AND DECISION MAKING 15 E. CONCLUSION 18 F. REFERENCES 19 POLAR PERSPECTIVES 2 No. 5 l June 2021 I. INTRODUCTION BY EVAN T. BLOOM vii Fig 1: Southern Ocean regions proposed for protection A network of MPAs could allow for conservation of distinct areas, each representing unique ecosystems As the world prepares for the Glasgow Climate Change Conference in November 2021, there is considerable focus on the Southern Ocean. The international community has come to realize that the polar regions hold many of the keys to unlocking our understanding of climate-related phenomena - and thus polar science will influence policy decisions on which our collective futures depend.