Monitoring Recent Glacier Variations in the Southern Patagonia Icefield, Utilizing Remote Sensing Data
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Variations of Patagonian Glaciers, South America, Utilizing RADARSAT Images
Variations of Patagonian Glaciers, South America, utilizing RADARSAT Images Masamu Aniya Institute of Geoscience, University of Tsukuba, Ibaraki, 305-8571 Japan Phone: +81-298-53-4309, Fax: +81-298-53-4746, e-mail: [email protected] Renji Naruse Institute of Low Temperature Sciences, Hokkaido University, Sapporo, 060-0819 Japan, Phone: +81-11-706-5486, Fax: +81-11-706-7142, e-mail: [email protected] Gino Casassa Institute of Patagonia, University of Magallanes, Avenida Bulness 01855, Casilla 113-D, Punta Arenas, Chile, Phone: +56-61-207179, Fax: +56-61-219276, e-mail: [email protected] and Andres Rivera Department of Geography, University of Chile, Marcoleta 250, Casilla 338, Santiago, Chile, Phone: +56-2-6783032, Fax: +56-2-2229522, e-mail: [email protected] Abstract Combining RADARSAT images (1997) with either Landsat MSS (1987 for NPI) or TM (1986 for SPI), variations of major glaciers of the Northern Patagonia Icefield (NPI, 4200 km2) and of the Southern Patagonia Icefield (SPI, 13,000 km2) were studied. Of the five NPI glaciers studied, San Rafael Glacier showed a net advance, while other glaciers, San Quintin, Steffen, Colonia and Nef retreated during the same period. With additional data of JERS-1 images (1994), different patterns of variations for periods of 1986-94 and 1994-97 are recognized. Of the seven SPI glaciers studied, Pio XI Glacier, the largest in South America, showed a net advance, gaining a total area of 5.66 km2. Two RADARSAT images taken in January and April 1997 revealed a surge-like very rapid glacier advance. -
PATAGONIA Located in Argentina and Chile, Patagonia Is a Natural Wonderland That Occupies the Southernmost Reaches of South America
PATAGONIA Located in Argentina and Chile, Patagonia is a natural wonderland that occupies the southernmost reaches of South America. It is an extraordinary landscape of dramatic mountains, gigantic glaciers that calve into icy lakes, cascading waterfalls, crystalline streams and beech forests. It is also an area rich in wildlife such as seals, humpback whales, pumas, condors and guanacos. The best time to visit Patagonia is between October and April. Highlights Spectacular Perito Moreno Glacier; scenic wonders of Los Glaciares National Park; unforgettable landscapes of Torres del Paine; breathtaking scenery of the Lakes District. Climate The weather is at its warmest and the hours of daylight at their longest (18 hours) during the summer months of Nov-Mar. This is also the windiest and busiest time of year. Winter provides clear skies, less windy conditions and fewer tourists; however temperatures can be extremely cold. 62 NATURAL FOCUS – TAILOR-MADE EXPERIENCES Pristine Patagonia Torres Del Paine National Park in Patagonia was incredible! I had never seen anything like it before. This was one of the most awesome trips I have ever been on. Maria-Luisa Scala WWW.NATURALFOCUSSAFARIS.COM.AU | E: [email protected] | T: 1300 363 302 63 ARGENTINIAN PATAGONIA • PERITO MORENO Breathtaking Perito Moreno Glacier © Shutterstock PERITO MORENO GLACIER 4 days/3 nights From $805 per person twin share Departs daily ex El Calafate Price per person from: Twin Single Xelena (Standard Room Lake View) $1063 $1582 El Quijote Hotel (Standard Room) $962 $1423 -
South America Cryonet Meeting, 27-29 October 2014, Santiago De
TECHNICAL REPORT No. 2013- xx Insert title of report ....... WORLD METEOROLOGICAL ORGANIZATION GLOBAL CRYOSPHERE WATCH REPORT No. 8 CryoNet South America Workshop First Session Santiago de Chile, Chile 27-29 October 2014 © World Meteorological Organization, 2014 The right of publication in print, electronic and any other form and in any language is reserved by WMO. Short extracts from WMO publications may be reproduced without authorization, provided that the complete source is clearly indicated. Editorial correspondence and requests to publish, reproduce or translate this publication in part or in whole should be addressed to: Chair, Publications Board World Meteorological Organization (WMO) 7 bis, avenue de la Paix Tel.: +41 (0) 22 730 8403 P.O. Box 2300 Fax: +41 (0) 22 730 8040 CH-1211 Geneva 2, Switzerland E-mail: [email protected] NOTE The designations employed in WMO publications and the presentation of material in this publication do not imply the expression of any opinion whatsoever on the part of WMO concerning the legal status of any country, territory, city or area, or of its authorities, or concerning the delimitation of its frontiers or boundaries. The mention of specific companies or products does not imply that they are endorsed or recommended by WMO in preference to others of a similar nature which are not mentioned or advertised. The findings, interpretations and conclusions expressed in WMO publications with named authors are those of the authors alone and do not necessarily reflect those of WMO or its Members. FINAL -
A Review of the Current State and Recent Changes of the Andean Cryosphere
feart-08-00099 June 20, 2020 Time: 19:44 # 1 REVIEW published: 23 June 2020 doi: 10.3389/feart.2020.00099 A Review of the Current State and Recent Changes of the Andean Cryosphere M. H. Masiokas1*, A. Rabatel2, A. Rivera3,4, L. Ruiz1, P. Pitte1, J. L. Ceballos5, G. Barcaza6, A. Soruco7, F. Bown8, E. Berthier9, I. Dussaillant9 and S. MacDonell10 1 Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales (IANIGLA), CCT CONICET Mendoza, Mendoza, Argentina, 2 Univ. Grenoble Alpes, CNRS, IRD, Grenoble-INP, Institut des Géosciences de l’Environnement, Grenoble, France, 3 Departamento de Geografía, Universidad de Chile, Santiago, Chile, 4 Instituto de Conservación, Biodiversidad y Territorio, Universidad Austral de Chile, Valdivia, Chile, 5 Instituto de Hidrología, Meteorología y Estudios Ambientales (IDEAM), Bogotá, Colombia, 6 Instituto de Geografía, Pontificia Universidad Católica de Chile, Santiago, Chile, 7 Facultad de Ciencias Geológicas, Universidad Mayor de San Andrés, La Paz, Bolivia, 8 Tambo Austral Geoscience Consultants, Valdivia, Chile, 9 LEGOS, Université de Toulouse, CNES, CNRS, IRD, UPS, Toulouse, France, 10 Centro de Estudios Avanzados en Zonas Áridas (CEAZA), La Serena, Chile The Andes Cordillera contains the most diverse cryosphere on Earth, including extensive areas covered by seasonal snow, numerous tropical and extratropical glaciers, and many mountain permafrost landforms. Here, we review some recent advances in the study of the main components of the cryosphere in the Andes, and discuss the Edited by: changes observed in the seasonal snow and permanent ice masses of this region Bryan G. Mark, The Ohio State University, over the past decades. The open access and increasing availability of remote sensing United States products has produced a substantial improvement in our understanding of the current Reviewed by: state and recent changes of the Andean cryosphere, allowing an unprecedented detail Tom Holt, Aberystwyth University, in their identification and monitoring at local and regional scales. -
168 2Nd Issue 2015
ISSN 0019–1043 Ice News Bulletin of the International Glaciological Society Number 168 2nd Issue 2015 Contents 2 From the Editor 25 Annals of Glaciology 56(70) 5 Recent work 25 Annals of Glaciology 57(71) 5 Chile 26 Annals of Glaciology 57(72) 5 National projects 27 Report from the New Zealand Branch 9 Northern Chile Annual Workshop, July 2015 11 Central Chile 29 Report from the Kathmandu Symposium, 13 Lake district (37–41° S) March 2015 14 Patagonia and Tierra del Fuego (41–56° S) 43 News 20 Antarctica International Glaciological Society seeks a 22 Abbreviations new Chief Editor and three new Associate 23 International Glaciological Society Chief Editors 23 Journal of Glaciology 45 Glaciological diary 25 Annals of Glaciology 56(69) 48 New members Cover picture: Khumbu Glacier, Nepal. Photograph by Morgan Gibson. EXCLUSION CLAUSE. While care is taken to provide accurate accounts and information in this Newsletter, neither the editor nor the International Glaciological Society undertakes any liability for omissions or errors. 1 From the Editor Dear IGS member It is now confirmed. The International Glacio be moving from using the EJ Press system to logical Society and Cambridge University a ScholarOne system (which is the one CUP Press (CUP) have joined in a partnership in uses). For a transition period, both online which CUP will take over the production and submission/review systems will run in parallel. publication of our two journals, the Journal Submissions will be twotiered – of Glaciology and the Annals of Glaciology. ‘Papers’ and ‘Letters’. There will no longer This coincides with our journals becoming be a distinction made between ‘General’ fully Gold Open Access on 1 January 2016. -
Glaciar Jorge Montt (Chilean Patagonia) Dynamics Derived from Photos Obtained by Fixed Cameras and Satellite Image Feature Tracking
Annals of Glaciology 53(60) 2012 doi: 10.3189/2012AoG60A152 147 Glaciar Jorge Montt (Chilean Patagonia) dynamics derived from photos obtained by fixed cameras and satellite image feature tracking Andre´s RIVERA,1,2 Javier CORRIPIO,3 Claudio BRAVO,1 Sebastia´n CISTERNAS1 1Centro de Estudios Cientı´ficos (CECS), Valdivia, Chile E-mail: [email protected] 2Departamento de Geografı´a, Universidad de Chile, Santiago, Chile 3meteoexploration.com ABSTRACT. Tidewater calving glaciers can undergo large fluctuations not necessarily in direct response to climate, but rather owing to complex ice–water interactions at the glacier termini. One example of this process in Chilean Patagonia is Glaciar Jorge Montt, where two cameras were installed in February 2010, collecting up to four glacier photographs per day, until they were recovered on 22 January 2011. Ice velocities were derived from feature tracking of the geo-referenced photos, yielding a mean value of 13 Æ 4md–1 for the whole lower part of the glacier. These velocities were compared to satellite- imagery-derived feature tracking obtained in February 2010, resulting in similar values. During the operational period of the cameras, the glacier continued to retreat (1 km), experiencing one of the highest calving fluxes ever recorded in Patagonia (2.4 km3 a–1). Comparison with previous data also revealed ice acceleration in recent years. These very high velocities are clearly a response to enhanced glacier calving activity into a deep water fjord. 1. INTRODUCTION Warren and others, 1995; Rignot and others, 1996a,b). Another SPI glacier with direct ice velocity measurements is The Patagonian icefields have been shrinking at high rates in –1 the last 50 years, compared to the area losses experienced Glaciar Tyndall, where a maximum of 1.9 m d was meas- since the Little Ice Age, contributing significantly to sea- ured in 1985 near the medial moraine (Kadota and others, level rise (Glasser and others, 2011). -
The 21St-Century Fate of the Mocho-Choshuenco Ice Cap in Southern Chile
The Cryosphere, 15, 3637–3654, 2021 https://doi.org/10.5194/tc-15-3637-2021 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. The 21st-century fate of the Mocho-Choshuenco ice cap in southern Chile Matthias Scheiter1,a, Marius Schaefer2, Eduardo Flández3, Deniz Bozkurt4,5, and Ralf Greve6,7 1Research School of Earth Sciences, Australian National University, Canberra, Australia 2Instituto de Ciencias Físicas y Matemáticas, Universidad Austral de Chile, Valdivia, Chile 3Departamento de Física, Facultad de Ciencias, Universidad de Chile, Santiago, Chile 4Departamento de Meteorología, Universidad de Valparaíso, Valparaíso, Chile 5Center for Climate and Resilience Research (CR)2, Santiago, Chile 6Institute of Low Temperature Science, Hokkaido University, Sapporo, Japan 7Arctic Research Center, Hokkaido University, Sapporo, Japan aformerly at: Institut für Geophysik und Geoinformatik, TU Bergakademie Freiberg, Freiberg, Germany Correspondence: Matthias Scheiter ([email protected]) Received: 8 October 2020 – Discussion started: 11 November 2020 Revised: 23 June 2021 – Accepted: 25 June 2021 – Published: 6 August 2021 Abstract. Glaciers and ice caps are thinning and retreat- different global climate models and on the uncertainty asso- ing along the entire Andes ridge, and drivers of this mass ciated with the variation of the equilibrium line altitude with loss vary between the different climate zones. The south- temperature change. Considering our results, we project a ern part of the Andes (Wet Andes) has the highest abun- considerable deglaciation of the Chilean Lake District by the dance of glaciers in number and size, and a proper under- end of the 21st century. standing of ice dynamics is important to assess their evo- lution. -
Glacier Clusters Identification Across Chilean Andes Using Topo-Climatic
119 Glacier Clusters identification across Chilean Andes using Topo-Climatic variables Identificación de clústeres glaciares a lo largo de los Andes chilenos usando variables topoclimáticas Historial del artículo Alexis Caroa; Fernando Gimenob; Antoine Rabatela; Thomas Condoma; Recibido: Jean Carlos Ruizc 15 de octubre de 2020 Revisado a Université Grenoble Alpes, CNRS, IRD, Grenoble-INP, Institut des Géosciences de l’Environnement (UMR 5001), 30 de octubre de 2020 Grenoble, France. Aceptado: b Department of Environmental Science and Renewable Natural Resources, University of Chile, Santiago, Chile. 05 de noviembre de 2020 c Sorbonne Université, Paris, France. Keywords Abstract Chilean Andes, climatology, Using topographic and climatic variables, we present glacier clusters in the Chilean Andes (17.6-55.4°S), where the glacier clusters, topography Partitioning Around Medoids (PAM) unsupervised machine learning algorithm was utilized. The results classified 23,974 glaciers inside thirteen clusters, which show specific conditions in terms of annual and monthly amounts of precipitation, temperature, and solar radiation. In the Dry Andes, the mean annual values of the five glacier clusters (C1-C5) display precipitation and temperature difference until 400 mm (29 and 33°S) and 8°C (33°S), with mean elevation contrast of 1800 m between glaciers in C1 and C5 clusters (18 to 34°S). While in the Wet Andes the highest differences were observed at the Southern Patagonia Icefield latitude (50°S), were the mean annual values for precipitation and temperature show maritime precipitation above 3700 mm/yr (C12), where the wet Western air plays a key role, and below 1000 mm/yr in the east of Southern Patagonia Icefield (C10), with differences temperature near of 4°C and mean elevation contrast of 500 m. -
Response of the Patagonian Glaciers to Present and Future Atmospheric Changes
Response of the Patagonian Glaciers to Present and Future Atmospheric Changes Claudio Andrés Bravo Lechuga Submitted in accordance with the requirements for the degree of Doctor of Philosophy The University of Leeds School of Geography November, 2020 - ii - The candidate confirms that the work submitted is his/her own, except where work which has formed part of jointly-authored publications has been included. The contribution of the candidate and the other authors to this work has been explicitly indicated below. The candidate confirms that appropriate credit has been given within the thesis where reference has been made to the work of others. The work in Chapter three of the thesis has appeared in publication as follows: Bravo C., D. Quincey, A. Ross, A. Rivera, B. Brock, E. Miles and A. Silva (2019). Air temperature characteristics, distribution and impact on modeled ablation for the South Patagonia Icefield. Journal of Geophysical Research: Atmospheres 124(2), 907–925. doi: org/101029/2018JD028857. C. Bravo designed the study, analysed the data and prepared the paper. E. Miles discussed the results and contributed to the writing. D.J. Quincey, A.N. Ross, A. Rivera, B. Brock and E. Miles oversaw the research and reviewed the manuscript. C. Bravo, A. Silva and A. Rivera participated in the field campaigns preparing logistic and installing and configuring the Automatic Weather Stations. All authors discussed the results and reviewed the manuscript. The work in Chapter four of the thesis has appeared in publication as follows: Bravo C., D. Bozkurt, Á. Gonzalez-Reyes, D.J. Quincey, A.N. Ross, D. -
Modern Sedimentary Processes at the Heads of Martínez Channel And
Marine Geology 419 (2020) 106076 Contents lists available at ScienceDirect Marine Geology journal homepage: www.elsevier.com/locate/margo Modern sedimentary processes at the heads of Martínez Channel and Steffen Fjord, Chilean Patagonia T ⁎ Elke Vandekerkhovea, , Sebastien Bertranda, Eleonora Crescenzi Lannaa, Brian Reidb, Silvio Pantojac a Renard Centre of Marine Geology, Department of Geology, Ghent University, Krijgslaan 281 S8, 9000 Gent, Belgium b Centro de Investigación en Ecosistemas de la Patagonia (CIEP), Universidad Austral de Chile, Francisco Bilbao 323, Coyhaique, Chile c Departamento de Oceanografía and Centro de Investigación Oceanográfica COPAS Sur-Austral, Universidad de Concepción, Concepción, Chile ARTICLE INFO ABSTRACT Editor: Michele Rebesco Chilean fjord sediments constitute high-resolution archives of climate and environmental change in the southern Keywords: Andes. To interpret such records accurately, it is crucial to understand how sediment is transported and de- Chilean fjords posited within these basins. This issue is of particular importance in glaciofluvial Martínez Channel and Steffen Multibeam bathymetry Fjord (48°S), due to the increasing occurrence of Glacial Lake Outburst Floods (GLOFs) originating from outlet Submarine channel glaciers of the Northern Patagonian Icefield. Hence, the bathymetry of the head of Martínez Channel and Steffen Turbidity current Fjord was mapped at high resolution and the grain-size and organic carbon content of grab sediment samples Sediment transport were examined. Results show that the subaquatic deltas of Baker and Huemules rivers at the head of Martínez Channel and Steffen Fjord, respectively, are deeply incised (up to 36 m) by sinuous channels. The presence of sediment waves and coarser sediments within these channels imply recent activity and sediment transport by turbidity currents. -
Global Warming Can Alter Shape of the Planet, As Melting Glaciers Erode the Land
News date: October 1, 2015 compiled by Dr. Alvarinho J. Luis Global warming can alter shape of the planet, as melting glaciers erode the land Climate change is causing more than just warmer oceans and erratic weather. According to scientists, it also has the capacity to alter the shape of the planet. In a five-year study published today in Nature, lead author Michele Koppes from the University of British Columbia, compared glaciers in Patagonia and in the Antarctic Peninsula. She and her team found that glaciers in warmer Patagonia moved 100 to 1,000 times faster and caused more erosion than those in Antarctica, as warmer temperatures and melting ice helped lubricate the bed of the glaciers. Antarctica is warming up, and as it moves to temperatures above zero degrees Celsius, the glaciers are all going to start moving faster. We are already seeing that the ice sheets are starting to move faster and should become more erosive, digging deeper valleys and shedding more sediment into the oceans. The repercussions of this erosion add to the already complex effects of climate change in the polar regions. Faster moving glaciers deposit more sediment in downstream basins and on the continental shelves, potentially impacting fisheries, dams and access to clean freshwater in mountain communities. The polar continental margins in particular are hotspots of biodiversity, notes Koppes. If you're pumping out that much more sediment into the water, you're changing the aquatic habitat. The Canadian Arctic, one of the most rapidly warming regions of the world, will feel these effects acutely. -
Abstract Book, ###(###), CECS, Valdivia, Chile
Co-Sponsors Collaborators Edition of 500 copies Compañía Impresora Meza Ltda. Santiago, Chile January 2010 Abstracts should be cited as: Name of authors. 2010. Title. International Glaciological Conferen- ce VICC 2010 “Ice and Climate Change: A View from the South”, Valdivia, Chile, 1-3 February 2010. Abstract Book, ###(###), CECS, Valdivia, Chile. WELCOME OF THE DIRECTOR When one studies a very complicated system, a very pre- cious tool to have at hand is an extreme regime, whe- re key features of the complex problem are exhibited bla- tantly in a simplified context, without cumbersome details. In cosmology, that is, the study of the Universe as a who- le, the black hole provides such a tool, and recent advance- ments have shown it to be, not only a key witness of, but also a key actor in, determining the present state of the Universe. The motivation for starting the research activity in glaciology at CECS about ten years ago followed that approach, with climate pla- ying the role of the Universe and ice playing the role of the black hole. Since then, the field has become somewhat of a band wagon, and the phenomenon of climate change nowadays fascinates mankind. The sociological reasons for this are probably connected with atavistic feelings about eternal persistence of the human species, our planet, and the like. To the theoretical physicist who writes these words, and who has been forced by fact, to become used to the possibility that the Universe as a whole will come to an end, this fascination with climate change is quite remarkable and somewhat worrisome.