The Antarctic Sun, December 26, 1999
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Species Status Assessment Emperor Penguin (Aptenodytes Fosteri)
SPECIES STATUS ASSESSMENT EMPEROR PENGUIN (APTENODYTES FOSTERI) Emperor penguin chicks being socialized by male parents at Auster Rookery, 2008. Photo Credit: Gary Miller, Australian Antarctic Program. Version 1.0 December 2020 U.S. Fish and Wildlife Service, Ecological Services Program Branch of Delisting and Foreign Species Falls Church, Virginia Acknowledgements: EXECUTIVE SUMMARY Penguins are flightless birds that are highly adapted for the marine environment. The emperor penguin (Aptenodytes forsteri) is the tallest and heaviest of all living penguin species. Emperors are near the top of the Southern Ocean’s food chain and primarily consume Antarctic silverfish, Antarctic krill, and squid. They are excellent swimmers and can dive to great depths. The average life span of emperor penguin in the wild is 15 to 20 years. Emperor penguins currently breed at 61 colonies located around Antarctica, with the largest colonies in the Ross Sea and Weddell Sea. The total population size is estimated at approximately 270,000–280,000 breeding pairs or 625,000–650,000 total birds. Emperor penguin depends upon stable fast ice throughout their 8–9 month breeding season to complete the rearing of its single chick. They are the only warm-blooded Antarctic species that breeds during the austral winter and therefore uniquely adapted to its environment. Breeding colonies mainly occur on fast ice, close to the coast or closely offshore, and amongst closely packed grounded icebergs that prevent ice breaking out during the breeding season and provide shelter from the wind. Sea ice extent in the Southern Ocean has undergone considerable inter-annual variability over the last 40 years, although with much greater inter-annual variability in the five sectors than for the Southern Ocean as a whole. -
A Case Study of Sea Ice Concentration Retrieval Near Dibble Glacier, East Antarctica
European MSc in Marine Environment MER and Resources UPV/EHU–SOTON–UB-ULg REF: 2013-0237 MASTER THESIS PROJECT A case study of sea ice concentration retrieval near Dibble Glacier, East Antarctica: Contradicting observations between passive microwave remote sensing and optical satellites BY LAM Hoi Ming August 2016 Bremen, Germany PLENTZIA (UPV/EHU), SEPTEMBER 2016 European MSc in Marine Environment MER and Resources UPV/EHU–SOTON–UB-ULg REF: 2013-0237 Dr Manu Soto as teaching staff of the MER Master of the University of the Basque Country CERTIFIES: That the research work entitled “A case study of sea ice concentration retrieval near Dibble Glacier, East Antarctica: Contradiction between passive microwave remote sensing and optical satellite observations” has been carried out by LAM Hoi Ming in the Institute of Environmental Physics, University of Bremen under the supervision of Dr Gunnar Spreen from the of the University of Bremen in order to achieve 30 ECTS as a part of the MER Master program. In September 2016 Signed: Supervisor PLENTZIA (UPV/EHU), SEPTEMBER 2016 Abstract In East Antarctica, around 136°E 66°S, spurious appearance of polynya (open water area within an ice pack) is observed on ice concentration maps derived from the ASI (ARTIST Sea Ice) algorithm during the period of February to April 2014, using satellite data from the Advanced Microwave Scanning Radiometer 2 (AMSR-2). This contradicts with the visual images obtained by the Moderate Resolution Imaging Spectroradiometer (MODIS), which show the area to be ice covered during the period. In this study, data of ice concentration, brightness temperature, air temperature, snowfall, bathymetry, and wind in the area were analysed to identify possible explanations for the occurrence of such phenomenon, hereafter referred to as the artefact. -
ENVIRONMENTAL IMPACT ASSESSMENT – AUSTRALIAN ANTARCTIC PROGRAM AVIATION OPERATIONS 2020-2025 Draft Released for Public Comment
ENVIRONMENTAL IMPACT ASSESSMENT – AUSTRALIAN ANTARCTIC PROGRAM AVIATION OPERATIONS 2020-2025 draft released for public comment This document should be cited as: Commonwealth of Australia (2020). Environmental Impact Assessment – Australian Antarctic Program Aviation Operations 2020-2025 – draft released for public comment. Australian Antarctic Division, Kingston. © Commonwealth of Australia 2020 This work is copyright. You may download, display, print and reproduce this material in unaltered form only (retaining this notice) for your personal, non-commercial use or use within your organisation. Apart from any use as permitted under the Copyright Act 1968, all other rights are reserved. Requests and enquiries concerning reproduction and rights should be addressed to. Disclaimer The contents of this document have been compiled using a range of source materials and were valid as at the time of its preparation. The Australian Government is not liable for any loss or damage that may be occasioned directly or indirectly through the use of or reliance on the contents of the document. Cover photos from L to R: groomed runway surface, Globemaster C17 at Wilkins Aerodrome, fuel drum stockpile at Davis, Airbus landing at Wilkins Aerodrome Prepared by: Dr Sandra Potter on behalf of: Mr Robb Clifton Operations Manager Australian Antarctic Division Kingston 7050 Australia 2 Contents Overview 7 1. Background 9 1.1 Australian Antarctic Program aviation 9 1.2 Previous assessments of aviation activities 10 1.3 Scope of this environmental impact assessment 11 1.4 Consultation and decision outcomes 12 2. Details of the proposed activity and its need 13 2.1 Introduction 13 2.2 Inter-continental flights 13 2.3 Air-drop operations 14 2.4 Air-to-air refuelling operations 14 2.5 Operation of Wilkins Aerodrome 15 2.6 Intra-continental fixed-wing operations 17 2.7 Operation of ski landing areas 18 2.8 Helicopter operations 18 2.9 Fuel storage and use 19 2.10 Aviation activities at other sites 20 2.11 Unmanned aerial systems 20 2.12 Facility decommissioning 21 3. -
146268 Li, Binghui Full.Pdf (8.266Mb)
Department of Imaging and Applied Physics Centre for Marine Science and Technology Acoustic observation of ice rifting and breaking events on the Antarctic ice shelf using remote hydroacoustic listening stations Binghui Li This thesis is presented for the Degree of Doctor of Philosophy of Curtin University of Technology February 2010 DECLARATION To the best of my knowledge and belief this thesis contains no material previously published by any other person except where due acknowledgement has been made. This thesis contains no material which has been accepted for the award of any other degree or diploma in any university. Signature: _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ Date: _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ ABSTRACT Long-term continuous monitoring of ice break-up on ice shelves and icebergs in Antarctica is essential for a global observation system of climate change and its consequences. While calving of massive pieces of ice from the Antarctic ice shelf is well observed from satellites, numerous ice breaks of smaller volume cannot be systematically monitored and statistically analysed by the existing means of remote sensing and local in-situ observations. This study aimed to investigate the feasibility of an alternative monitoring approach based on remote acoustic observations of ice rifting and breaking events on Antarctic ice shelves and icebergs using distant underwater acoustic listening stations in the ocean. This investigation was carried out using long-term continuous sea noise recordings made from 2002 to 2007 at two hydroacoustic stations deployed in the Indian Ocean as part of the International Monitoring System of the Comprehensive Nuclear-Test-Ban Treaty: off Cape Leeuwin in Western Australia (HA01) and off Chagos Archipelago (HA08). -
Australian Antarctic Program Aviation Operations 2020-2025
ENVIRONMENTAL IMPACT ASSESSMENT – AUSTRALIAN ANTARCTIC PROGRAM AVIATION OPERATIONS 2020-2025 This document should be cited as: Commonwealth of Australia (2020). Environmental Impact Assessment – Australian Antarctic Program Aviation Operations 2020-2025. Australian Antarctic Division, Kingston. © Commonwealth of Australia 2020 This work is copyright. You may download, display, print and reproduce this material in unaltered form only (retaining this notice) for your personal, non-commercial use or use within your organisation. Apart from any use as permitted under the Copyright Act 1968, all other rights are reserved. Requests and enquiries concerning reproduction and rights should be addressed to. Disclaimer The contents of this document have been compiled using a range of source materials and were valid as at the time of its preparation. The Australian Government is not liable for any loss or damage that may be occasioned directly or indirectly through the use of or reliance on the contents of the document. Cover photos from L to R: groomed runway surface, Globemaster C17 at Wilkins Aerodrome, fuel drum stockpile at Davis, Airbus landing at Wilkins Aerodrome Prepared by: Dr Sandra Potter on behalf of: Charlton Clark General Manager Operations and Safety Australian Antarctic Division Kingston 7050 Australia 2 Contents Overview 7 1. Background 9 1.1 Australian Antarctic Program aviation 9 1.2 Previous assessments of aviation activities 10 1.3 Scope of this environmental impact assessment 11 1.4 Consultation 13 2. Details of the proposed activity and its need 14 2.1 Introduction 14 2.2 Inter-continental flights 14 2.3 Air-drop operations 15 2.4 Air-to-air refuelling operations 15 2.5 Operation of Wilkins Aerodrome 16 2.6 Intra-continental fixed-wing operations 18 2.7 Operation of ski landing areas 19 2.8 Helicopter operations 20 2.9 Fuel storage and use 20 2.10 Aviation activities at other sites 21 2.11 Unmanned aerial systems 22 2.12 Facility decommissioning 22 3. -
CURRICULUM VITAE Frank-Oliver Nitsche Lamont-Doherty Earth Observatory of Columbia University E-Mail: [email protected] 61 Rt
CURRICULUM VITAE Frank-Oliver Nitsche Lamont-Doherty Earth Observatory of Columbia University E-mail: [email protected] 61 Rt. 9W, Palisades, NY 10964, U.S.A. WWW: http://www.ldeo.columbia.edu/~fnitsche Phone: +1 845 365 8746 EDUCATION Ph.D. Geology and Geophysics (magna cum laude) 1997 University of Bremen, Germany. Thesis: “Development of a sedimentation model for the Bellingshausen and Amundsen Seas”. Diplom in Geophysics 1994 Institute of Geophysics, University of Kiel, Germany. Thesis: “Investigations of magnetic anomalies in archaeology using three-dimensional models and cross-correlation”. Additional training in Marine Geotechnics 1991/92 Marine Geotechnics M.Sc. Program, School of Ocean Sciences, University of Northwest Wales, Bangor, UK RESEARCH INTERESTS Glacial and glacial-marine sediment processes; Sealoor and benthic habitat mapping; Estuarine and coastal sediment dynamic and transport; Continental margins; Sub-surface imaging; GIS; Data integration and Visualization PROFESSIONAL EXPERIENCE Research Scientist 2011 - present Lamont-Doherty Earth Observatory of Columbia University, U.S.A. Adjunct Professor 2011 - 2017 Barnard College, NYC, U.S.A. Associate Research Scientist 2010 - 2011 Lamont-Doherty Earth Observatory of Columbia University, U.S.A. Doherty Associate Research Scientist 2004 – 2010 Lamont-Doherty Earth Observatory of Columbia University, U.S.A. Postdoctoral Scientist 2001 - 2004 Lamont-Doherty Earth Observatory of Columbia University, U.S.A. Postdoctoral Scientist 1997 - 2001 Institute of Geophysics, -
UCLA Electronic Theses and Dissertations
UCLA UCLA Electronic Theses and Dissertations Title Multi-Temporal Variability Within Antarctic Coastal Polynyas and Their Relationships To Large-Scale Atmospheric Phenomena Permalink https://escholarship.org/uc/item/0tj68195 Author Ward, Jason Michael Publication Date 2018 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California UNIVERSITY OF CALIFORNIA Los Angeles Multi-Temporal Variability Within Antarctic Coastal Polynyas and Their Relationships To Large-Scale Atmospheric Phenomena A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Geography by Jason Michael Ward 2018 ABSTRACT OF THE DISSERTATION Multi-Temporal Variability Within Antarctic Coastal Polynyas and Their Relationships To Large-Scale Atmospheric Phenomena by Jason Michael Ward Doctor of Philosophy in Geography University of California, Los Angeles, 2018 Professor Marilyn N Raphael, Chair Open water and thin ice areas, known as coastal polynyas, form along the Antarctic coastline and allow continued interaction between the ocean and atmosphere throughout the sea ice advance season. Coastal polynyas are the most productive locations of sea ice formation, Antarctic bottom water formation, and biological activity in the Southern Ocean. Changes in these elements are greatly controlled by polynya area variability. To carry out an in-depth study of polynya area variability, a 26-year 25-polynya daily area dataset was created and analyzed. The long term trend and the daily, monthly, seasonal, and annual variations are separated to analyze the multi- temporal variability of the polynyas and investigate their individual and regional responses to prominent large-scale atmospheric circulation patterns. Results indicate that most polynya variability occurs at the daily scale, followed by monthly and seasonal variations. -
Influence of Dispersal Processes on the Global Dynamics of Emperor
Appendices: Influence of dispersal processes on the global dynamics of Emperor penguin, a species threatened by climate change. Contents A Information about the known colonies of the emperor penguin in Antarctica. 2 B Description of the metapopulation model 5 B.1 Construction of the reproduction matrix F .......................5 B.2 The dispersal model . .9 C Global sensitivity analysis 13 D Baby models 15 D.1 Case 1 and 2: dispersion to the good patch is not always optimal . 15 D.1.1 Description of local and global dynamics . 15 D.1.2 Close to the equilibrium: analytical results. 16 D.1.3 Far away from the equilibrium: numerical results. 18 D.2 Case 3: Random dispersion between poor quality habitats . 20 D.3 Implications of theoretical results for the emperor penguin . 21 E Local and regional population dynamics 23 E.1 Population size of each colony . 23 E.2 Regional population size . 26 F Isolating the colonies on the Ross Sea 31 G Random departure and random search dispersal 34 1 A Information about the known colonies of the emperor penguin in Antarctica. Table 1: Information about the known colonies of the emperor penguin in Antarctica, modified from Fretwell et al. (2012) { see the figure A.1 for a spatial repartition of the known colonies in Antarctica. # is the index of the colony used in our figures; BE is the best estimate of the observed number of breeding pairs in 2009 used in our model simulations. # name longitude latitude BE 2009 1 Snowhill -57.44 -64.52 2164 2 Dolleman -60.43 -70.61 1620 3 Smith -60.83 -74.37 4018 4 Gould -47.68 -
The Emperor Penguin - Vulnerable to Projected Rates of Warming and Sea Ice Loss ⁎ Philip N
Biological Conservation xxx (xxxx) xxxx Contents lists available at ScienceDirect Biological Conservation journal homepage: www.elsevier.com/locate/biocon Review The emperor penguin - Vulnerable to projected rates of warming and sea ice loss ⁎ Philip N. Trathana, , Barbara Wieneckeb, Christophe Barbraudc, Stéphanie Jenouvrierc,d, Gerald Kooymane, Céline Le Bohecf,g, David G. Ainleyh, André Anceli,j, Daniel P. Zitterbartk,l, Steven L. Chownm, Michelle LaRuen, Robin Cristofario, Jane Youngerp, Gemma Clucasq, Charles-André Bostc, Jennifer A. Brownr, Harriet J. Gilletta, Peter T. Fretwella a British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge CB30ET, UK b Australian Antarctic Division, 203 Channel Highway, Tasmania 7050, Australia c Centre d'Etudes Biologiques de Chizé, UMR 7372, Centre National de la Recherche Scientifique, 79360 Villiers en Bois, France d Biology Department, MS-50, Woods Hole Oceanographic Institution, Woods Hole, MA, USA e Scholander Hall, Scripps Institution of Oceanography, 9500 Gilman Drive 0204, La Jolla, CA 92093-0204, USA f Département d'Écologie, Physiologie, et Éthologie, Institut Pluridisciplinaire Hubert Curien (IPHC), Centre National de la Recherche Scientifique, Unite Mixte de Recherche 7178, 23 rue Becquerel, 67087 Strasbourg Cedex 02, France g Scientific Centre of Monaco, Polar Biology Department, 8 Quai Antoine 1er, 98000, Monaco h H.T. Harvey and Associates Ecological Consultants, Los Gatos, California, CA 95032, USA i Université de Strasbourg, IPHC, 23 rue Becquerel, 67087 Strasbourg, France j CNRS, UMR7178, 67087 Strasbourg, France k Applied Ocean Physics and Engineering, Woods Hole Oceanographic Institution, Woods Hole, MA, USA l Department of Physics, University of Erlangen-Nuremberg, Henkestrasse 91, 91052 Erlangen, Germany m School of Biological Sciences, Monash University, VIC 3800, Australia n University of Minnesota, Minneapolis and St. -
Morphological Characteristics of the Ice Margins of Antarctic Ice Shelf and Outlet Glacier Extracted from Icesat Laser Altimetry Along-Track Profiles
Terr. Atmos. Ocean. Sci., Vol. 27, No. 4, 451-462, August 2016 doi: 10.3319/TAO.2015.12.24.01(ISRS) Morphological Characteristics of the Ice Margins of Antarctic Ice Shelf and Outlet Glacier Extracted from ICESat Laser Altimetry Along-Track Profiles Jieun Kim1, Jaehyung Yu2, *, Lei Wang 3, Hongxing Liu 4, and Haein Shin1 1 Department of Astronomy, Space Science and Geology, Chungnam National University, Daejeon, Korea 2 Department of Geology & Earth Environmental Sciences, Chungnam National University, Daejeon, Korea 3 Department of Geography & Anthropology, Louisiana State University, Louisiana, U.S.A. 4 Department of Geography, University of Cincinnati, Ohio, U.S.A. Received 2 June 2015, revised 14 December 2015, accepted 24 December 2015 ABSTRACT The Antarctic ice sheet topography including elevation and slope is a key parameter for understanding ice sheet dynam- ics because the surface slope is a major controller of the ice flow gravitational driving stress magnitude. This study used Ice, Cloud, and land Elevation Satellite (ICESat) laser altimetry data to analyze the ice margin morphological parameters for 20 ice shelves and 12 outlet glaciers distributed over Antarctica. The bottom-up segmentation algorithm application effectively extracted the morphological parameters from the laser altimetry profiles. The ice shelves had an average boundary elevation of 29.5 m and a slope of 7.8°, with a decreasing surface slope pattern from the boundary to the inner side. The average number of segments and the length of the coastal margin for ice shelves extracted from the bottom-up segmentation algorithm is 3.2 and is 18.4 km, respectively. -
Discovery of New Colonies by Sentinel2 Reveals Good and Bad News for Emperor Penguins Peter T
ORIGINAL RESEARCH Discovery of new colonies by Sentinel2 reveals good and bad news for emperor penguins Peter T. Fretwell & Philip N. Trathan British Antarctic Survey, Madingley Road, Cambridge, United Kingdom Keywords Abstract Breeding colonies, climate change, penguins, Satellite remote sensing, Sentinel2 The distribution of emperor penguins is circumpolar, with 54 colony locations currently reported of which 50 are currently extant as of 2019. Here we report Correspondence on eight newly discovered colonies and confirm the rediscovery of three breed- Peter Fretwell, British Antarctic Survey, ing sites, only previously reported in the era before Very High Resolution satel- Madingley Road, Cambridge, United lite imagery was available, making a total of 61 breeding locations. This Kingdom. Tel: +44(0) 1223 221425; Fax: +44 represents an increase of ~20% in the number of breeding sites, but, as most of (0)1223 362616; E-mail: [email protected] the colonies appear to be small, they may only increase the total population by – Editor: Kylie Scales around 5 10%. The discoveries have been facilitated by the use of Sentinel2 Associate Editor: Phil Bouchet satellite imagery, which has a higher resolution and more efficient search mech- anism than the Landsat data previously used to search for colonies. The small Received: 28 January 2020; Revised: 10 June size of these new colonies indicates that considerations of reproductive output 2020; Accepted: 10 July 2020 in relation to metabolic rate during huddling is likely to be of interest. Some of the colonies exist in offshore habitats, something not previously reported for emperor penguins. Comparison with recent modelling results show that the doi: 10.1002/rse2.176 geographic locations of all the newly found colonies are in areas likely to be highly vulnerable under business-as-usual greenhouse gas emissions scenarios, suggesting that population decreases for the species will be greater than previ- ously thought. -
Hydroacoustic Signals Generated by Parked and Drifting Icebergs in the Southern Indian and Pacific Oceans
Geophys. J. Int. (2006) 165, 817–834 doi: 10.1111/j.1365-246X.2006.02911.x Hydroacoustic signals generated by parked and drifting icebergs in the Southern Indian and Pacific Oceans Jacques Talandier,1 Olivier Hyvernaud,2 Dominique Reymond2 and Emile A. Okal3 1D´epartement Analyse et Surveillance de l’Environnement, Commissariata ` l’Energie Atomique, Boıteˆ Postale 12, F-91680 Bruy´eres-le-Chˆatel, France 2Laboratoire de D´etection et G´eophysique, Commissariatal’Energie ` Atomique, Boıteˆ Postale 640, F-98713 Papeete, Tahiti, French Polynesia 3Department of Geological Sciences, Northwestern University, Evanston, IL 60201, USA. E-mail: [email protected] Accepted 2005 December 21. Received 2005 December 17; in original form 2005 March 27 SUMMARY Wereport the detection, principally by the French Polynesian seismic network, of hydroacoustic signals generated inside large icebergs, either ‘parked’ along the Wilkes coast of Antarctica in the Indian Ocean, or drifting in the Southern Pacific Ocean between latitudes of 55◦ and 65◦S, during the years 2002–2004. The signals can be classified into two very broad families, based on the nature of their spectra. A first group features prominently monochromatic signals, whose frequency can, however, fluctuate with time during a single sequence of emission (typically lasting a few to a few tens of minutes). Such signals are generally reminiscent of those detected in 2000 in the Ross Sea and are generated principally in the Indian Ocean ‘iceberg parking lot’, between longitudes 144◦E and 156◦E. A new family of signals features a much broader spectrum, superimposed on a number of preferential frequencies suggesting the background activation of a number of resonators; these signals occur both in the parking lot and in the Southern Pacific.