Tilt Signals at Mount Melbourne, Antarctica: Evidence of a Shallow Volcanic Source Salvatore Gambino, Marco Aloisi, Giuseppe Falzone & Angelo Ferro
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Region 19 Antarctica Pg.781
Appendix B – Region 19 Country and regional profiles of volcanic hazard and risk: Antarctica S.K. Brown1, R.S.J. Sparks1, K. Mee2, C. Vye-Brown2, E.Ilyinskaya2, S.F. Jenkins1, S.C. Loughlin2* 1University of Bristol, UK; 2British Geological Survey, UK, * Full contributor list available in Appendix B Full Download This download comprises the profiles for Region 19: Antarctica only. For the full report and all regions see Appendix B Full Download. Page numbers reflect position in the full report. The following countries are profiled here: Region 19 Antarctica Pg.781 Brown, S.K., Sparks, R.S.J., Mee, K., Vye-Brown, C., Ilyinskaya, E., Jenkins, S.F., and Loughlin, S.C. (2015) Country and regional profiles of volcanic hazard and risk. In: S.C. Loughlin, R.S.J. Sparks, S.K. Brown, S.F. Jenkins & C. Vye-Brown (eds) Global Volcanic Hazards and Risk, Cambridge: Cambridge University Press. This profile and the data therein should not be used in place of focussed assessments and information provided by local monitoring and research institutions. Region 19: Antarctica Description Figure 19.1 The distribution of Holocene volcanoes through the Antarctica region. A zone extending 200 km beyond the region’s borders shows other volcanoes whose eruptions may directly affect Antarctica. Thirty-two Holocene volcanoes are located in Antarctica. Half of these volcanoes have no confirmed eruptions recorded during the Holocene, and therefore the activity state is uncertain. A further volcano, Mount Rittmann, is not included in this count as the most recent activity here was dated in the Pleistocene, however this is geothermally active as discussed in Herbold et al. -
Volcanic Activity of Mount Melbourne, Northern Victoria Land
Volcanic activity of Mount Melbourne, Present-day geothermal activity is restricted to the summit area and consists of warm ground, fumarole ice towers and northern Victoria Land pinnacles, and cave systems in snow and firn. Warm ground temperatures were measured using mercury thermometers, and ice-structure dimensions and positions were noted. The J. R. KEYS table compares maximum ground temperatures and shows that those in January 1983 were virtually identical to those in De- Antarctic Consultant cember 1972. As in 1972, the warmest temperatures in 1983 Wellington, New Zealand were associated with patches of yellow to green moss whose presence is consistent with stable heat flow (Nathan and W. C. MCINTOSH, and P. R. KYLE Schulte 1967). A constant degree of geothermal activity appears to have Department of Geoscience persisted for at least the last. 20 years. Vertical aerial pho- New Mexico Institute of Mining and Technology tographs taken in 1963 show a distribution of ice structures and Socorro, New Mexico 87801 bare ground similar to that of both 1972 and 1983. Comparison of observations made in January 1983 and December 1972 indi- cates that the numbers of ice pinnacles and towers in areas I and Mount Melbourne (2,733 meters, 74° 21 S 164° 42 E) is a 3 are unchanged, but in 1983 area 2 had three or four fewer ice mildly active alkaline volcano 12 kilometers from the coast of structures. In 1983 area 1 had about 100 square meters of snow Wood Bay in northern Victoria Land. It is a predominantly and ice-free ground compared to only 40 square meters in 1972, snow- and ice-covered, low-angled strato volcano composed of whereas area 2 had less bare ground than in 1972. -
Discovery of a Tertiary Granite Pluton, Northern Victoria Land
Discovery of a Tertiary granite pluton, percent orthoclase, 10 percent albite (0rq iAbi0), that the albite is Ab98 and that the chlorite is iron-rich. Rims of the magnetite are northern Victoria Land 95 percent megnetite, 5 percent ulvospinel (MtqUvsp), but their cores are Mt70Uvsp30, perhaps indicating primary and sec- ondary phases of this mineral. EDMUND STUMP, The original assemblage appears to have contained two feld- JOHN R. HOLLOWAY, spars, plus quartz. The chlorite presumably was biotite. The and allanite apparently has been undisturbed by secondary effects. SCOTT C. BORG The granite has a minimum melt bulk composition with 75 weight percent silica (Si02) and very low magnesium oxide Department of Geology (MgO) and calcium oxide (CaO). It is slightly peraluminous Arizona State University with 0.9 weight percent normative corundum. Tempe, Arizona 85281 The data from the rubidium/strontium (Rb/Sr) analyses are summarized in the table (X = 1.42 x 10 11 for Rb). Although the RICHARD LEE ARMSTRONG Department of Geological Sciences University of British Columbia Vancouver, British Columbia V6T 1W5 Canada Analytical data Initial 87 Rb 87 Sr Sample Sra Rb Age 87S During the 1980-1981 field season our party undertook sys- 86S 86S 865r tematic collection of early-middle Paleozoic granitoids throughout northern Victoria Land (Stump et al. 1982). In the course of a subsequent strontium isotope study, we discovered ETTC 16.2 218 39.1 0.7195 that one intrusion is Tertiary. whole rock This unique pluton is exposed for about 5 kilometers along 9 ± 1 0.7148 the southwestern side of Mariner Glacier, immediately to the ETT 43.4 179 11.93 0.7162 east of the confluence of Meander Glacier (figure), where it chlorite intrudes Bowers Supergroup at a steep angle, showing very little contact effects. -
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. -
ASAR Interferometry at Piton De La Fournaise, Preliminary Results
ASAR Interferometry at Piton de la Fournaise, preliminary results FROGER Jean-Luc1, FUKUSHIMA Yo2, BRIOLE Pierre3, STAUDACHER Thomas4, SOURIOT Thierry2, VILLENEUVE Nicolas5, CHEMINEE Jean-Louis3 1 : Institut de Recherche pour le Développement (IRD) UR31 "Processus et Aléas Volcaniques", LMV, UBP - UMR 6524. 5, rue Kessler, 63 038 Clermont-Ferrand, FRANCE 2 : Laboratoire Magmas et Volcans, Université Blaise Pascal - UMR 6524. 5, rue Kessler, 63 038 Clermont- Ferrand, FRANCE 3: CNRS-UMR 7580, Institut de Physique du Globe de Paris, 4 Place Jussieu, Paris 75005, FRANCE 4: Observatoire Volcanologique du Piton de la Fournaise, Institut de Physique du Globe de Paris, 14 RN3, le 27ème, 97418 La Plaine des Cafres, LA REUNION 5: Université de la Réunion, 15, avenue René Cassin, BP 7151 97715 Saint-Denis, messag cedex 9, LA REUNION Since the detection of surface deformation at Mount Etna, several geodetic studies have been performed on volcanoes with radar interferometric data acquired by the European ERS-1 and ERS-2 satellites, the Japanese JERS-1 satellite and the Canadian RADARSAT-1 satellite. Here we present the preliminary results of an interferometric study of Piton de la Fournaise volcano, Réunion Island, with Synthetic Aperture Radar images acquired by the ASAR- ENVISAT satellite. Launched in March 2002 by the European Space Agency, ENVISAT is an Earth observation dedicated satellite and its payload consists of a set of instruments for measuring the atmosphere and the surface through the atmosphere. One of these instruments is the ASAR radar designed to provide for continuity of the observations started with the SAR on board of the ERS satellites. -
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. -
Magma Fragmentation and Particle Size Distributions in Low Intensity Mafc Explosions: the July/August 2015 Piton De La Fournaise Eruption Matthew J
www.nature.com/scientificreports OPEN Magma fragmentation and particle size distributions in low intensity mafc explosions: the July/August 2015 Piton de la Fournaise eruption Matthew J. Edwards1*, Laura Pioli2*, Andrew J. L. Harris3, Lucia Gurioli3 & Simon Thivet3 Understanding magma fragmentation mechanisms in explosive eruptions is a key requirement for volcanic hazard assessment, eruption management and risk mitigation. This paper focuses on a type case small explosivity eruption (July–August 2015 eruption of Piton de la Fournaise). These eruptions, despite being often overlooked, are exceedingly frequent on local-to-global scales and constitute a signifcant hazard in vent-proximal areas, which are often populated by guides, tourists and, indeed, volcanologists due to their accessibility. The explosions presented here are ideal cases for the study of the dynamics of magma fragmentation and how it relates to the size distribution of scoria generated at the vent. We documented these events visually and thermally, and characterised the products through sample-return. This allowed us to describe small-scale gas bursts sending ejecta up to 30 m during intermittent lava fountains. Surface tension instabilities and inertial forces played a major role in fragmentation processes and generated particles with coarse-skewed distributions and median diameters ranging from − 8 to − 10 . However, with time distributions of particles in the most energetic fountains shifted towards more symmetricalϕ shapes as median grains sizes became fner. Analyses of sequences of images demonstrate that the evolution of particle size distributions with time is due to instability of magma droplets and (in-fight) fragmentation. Mafc explosive volcanism is traditionally overlooked with respect to more energetic, higher intensity and destructive silicic volcanism. -
Advisory Committee on Reactor Safeguards (ACRS)
Federal Register / Vol. 77, No. 95 / Wednesday, May 16, 2012 / Notices 28903 FOR FURTHER INFORMATION CONTACT: Dates Detailed meeting agendas and meeting Polly A. Penhale at the above address or October 1, 2012 to December 30, 2012. transcripts are available on the NRC (703) 292–7420. Web site at http://www.nrc.gov/reading- Nadene G. Kennedy, rm/doc-collections/acrs. Information SUPPLEMENTARY INFORMATION: The Permit Officer, Office of Polar Programs. regarding topics to be discussed, National Science Foundation, as [FR Doc. 2012–11840 Filed 5–15–12; 8:45 am] changes to the agenda, whether the directed by the Antarctic Conservation BILLING CODE 7555–01–P meeting has been canceled or Act of 1978 (Pub. L. 95–541), as rescheduled, and the time allotted to amended by the Antarctic Science, present oral statements can be obtained Tourism and Conservation Act of 1996, from the Web site cited above or by has developed regulations for the NUCLEAR REGULATORY contacting the identified DFO. establishment of a permit system for COMMISSION Moreover, in view of the possibility that various activities in Antarctica and the schedule for ACRS meetings may be designation of certain animals and Advisory Committee on Reactor adjusted by the Chairman as necessary certain geographic areas requiring Safeguards (ACRS) Meeting of the to facilitate the conduct of the meeting, special protection. The regulations ACRS Subcommittee on Fukushima; persons planning to attend should check establish such a permit system to Notice of Meeting with these references if such designate Antarctic Specially Protected The ACRS Subcommittee on rescheduling would result in a major Areas. -
Federal Register/Vol. 84, No. 78/Tuesday, April 23, 2019/Rules
Federal Register / Vol. 84, No. 78 / Tuesday, April 23, 2019 / Rules and Regulations 16791 U.S.C. 3501 et seq., nor does it require Agricultural commodities, Pesticides SUPPLEMENTARY INFORMATION: The any special considerations under and pests, Reporting and recordkeeping Antarctic Conservation Act of 1978, as Executive Order 12898, entitled requirements. amended (‘‘ACA’’) (16 U.S.C. 2401, et ‘‘Federal Actions to Address Dated: April 12, 2019. seq.) implements the Protocol on Environmental Justice in Minority Environmental Protection to the Richard P. Keigwin, Jr., Populations and Low-Income Antarctic Treaty (‘‘the Protocol’’). Populations’’ (59 FR 7629, February 16, Director, Office of Pesticide Programs. Annex V contains provisions for the 1994). Therefore, 40 CFR chapter I is protection of specially designated areas Since tolerances and exemptions that amended as follows: specially managed areas and historic are established on the basis of a petition sites and monuments. Section 2405 of under FFDCA section 408(d), such as PART 180—[AMENDED] title 16 of the ACA directs the Director the tolerance exemption in this action, of the National Science Foundation to ■ do not require the issuance of a 1. The authority citation for part 180 issue such regulations as are necessary proposed rule, the requirements of the continues to read as follows: and appropriate to implement Annex V Regulatory Flexibility Act (5 U.S.C. 601 Authority: 21 U.S.C. 321(q), 346a and 371. to the Protocol. et seq.) do not apply. ■ 2. Add § 180.1365 to subpart D to read The Antarctic Treaty Parties, which This action directly regulates growers, as follows: includes the United States, periodically food processors, food handlers, and food adopt measures to establish, consolidate retailers, not States or tribes. -
Moult of the Emperor Penguin: Travel, Location, and Habitat Selection
MARINE ECOLOGY PROGRESS SERIES Vol. 204: 269–277, 2000 Published October 5 Mar Ecol Prog Ser Moult of the emperor penguin: travel, location, and habitat selection G. L. Kooyman1,*, E. C. Hunke2, S. F. Ackley3, R. P. van Dam1, G. Robertson4 1Scholander Hall, 0204, Scripps Institution of Oceanography, La Jolla, California 92093, USA 2MS-B216, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA 3Cold Regions Research and Engineering Laboratory 72 Lyme Rd., Hanover, New Hampshire 03755, USA 4Australian Antarctic Division, Channel Highway, Kingston 7050, Tasmania, Australia ABSTRACT: All penguins except emperors Aptenodytes forsteri and Adelies Pygoscelis adeliae moult on land, usually near the breeding colonies. These 2 Antarctic species typically moult some- where in the pack-ice. Emperor penguins begin their moult in early summer when the pack-ice cover of the Antarctic Ocean is receding. The origin of the few moulting birds seen by observers on pass- ing ships is unknown, and the locations are often far from any known colonies. We attached satellite transmitters to 12 breeding adult A. forsteri from western Ross Sea colonies before they departed the colony for the last time before moulting. In addition, we surveyed some remote areas of the Weddell Sea north and east of some large colonies that are located along the southern and western borders of this sea. The tracked birds moved at a rate of nearly 50 km d–1 for more than 1000 km over 30 d to reach areas of perennially consistent pack-ice. Almost all birds traveled to the eastern Ross Sea and western Amundsen Sea. -
Pitons, Cirques and Remparts of Reunion Island
EUROPE / NORTH AMERICA PITONS, CIRQUES AND REMPARTS OF REUNION ISLAND FRANCE WORLD HERITAGE NOMINATION - IUCN TECHNICAL EVALUATION PITONS, CIRQUES AND REMPARTS OF REUNION ISLAND (FRANCE) - ID Nº 1317 Background note: This nomination was submitted in 2008 for consideration by the World Heritage Committee at its 33rd Session in 2009. Accordingly, IUCN initiated the evaluation of this nomination in 2008/9 and this included the evaluation mission to La Réunion. In March 2009, the decision was taken by the government of France to postpone the assessment of the nomination by UNESCO’s World Heritage Committee until its 34th Session in 2010. This decision was required due to the fact that three nominations from France were proposed for consideration by the 33rd Session of the World Heritage Committee. The State Party of France had been requested by the UNESCO World Heritage Centre to identify two nominations in line with the limits on annual numbers of nominations set in the Operational Guidelines. As the evaluation process was already initiated by IUCN, a dialogue was maintained with the State Party to clarify a number of issues and address recommendations resulting from the evaluation mission, and discussions from the 2008 session of the IUCN/World Heritage Panel. This evaluation report is therefore based on the original nomination plus the additional information provided by the State Party. 1. DOCUMENTATION i) Date nomination received by IUCN: 31st January 2008 ii) Additional information offi cially requested from and provided by the State Party: additional information was requested by IUCN in December 2008. Additional information from the State Party was provided in February 2009 and November 2009. -
The Antarctic Treaty
Miscellaneous No. 7 (2007) The Antarctic Treaty Measures adopted at the Twenty-ninth Consultative Meeting held at Edinburgh 12 – 23 June 2006 Presented to Parliament by the Secretary of State for Foreign and Commonwealth Affairs by Command of Her Majesty July 2007 Cm 7167 £17.00 Miscellaneous No. 7 (2007) The Antarctic Treaty Measures adopted at the Twenty-ninth Consultative Meeting held at Edinburgh 12 – 23 June 2006 Presented to Parliament by the Secretary of State for Foreign and Commonwealth Affairs by Command of Her Majesty July 2007 Cm 7167 £17.00 © Crown copyright 2007 The text in this document (excluding the Royal Arms and departmental logos) may be reproduced free of charge in any format or medium providing it is reproduced accurately and not used in a misleading context. The material must be acknowledged as Crown copyright and the title of the document specified. Any enquiries relating to the copyright in this document should be addressed to the Licensing Division, HMSO, St Clements House, 2-16 Colegate, Norwich NR3 1BQ. Fax 01603 723000 or e-mail: [email protected] MEASURES ADOPTED AT THE TWENTY-NINTH CONSULTATIVE MEETING HELD AT EDINBURGH 12 - 23 JUNE 2006 The Measures1 adopted at the Twenty-ninth Antarctic Treaty Consultative Meeting are reproduced below from the Final Report of the Meeting. In accordance with Article IX, paragraph 4, of the Antarctic Treaty, the Measures adopted at Consultative Meetings become effective upon approval by all Contracting Parties whose representatives were entitled to participate in the meeting at which they were adopted (i.e.