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South America 2007-08
1 The Patagonian Adventure – two Tasmanians in South America Dec/Jan 07-08 Keith and Sib Corbett What and where “Patagonia’ is the name given to the southern part of South America, actually shared between Chile and Argentina. It extends roughly from 40° to 56°S latitude, and includes the large island of Tierra del Fuego (the same size as Tasmania) at the bottom. The Andean mountains run down the western side, about 200km wide and up to 4000m high, with two small icecaps, hundreds of glaciers, and thousands of fiords and glacial valleys and lakes. The Andes and west coast are exceptionally wet – 3 to 4 metres of rainfall annually – and are mostly covered by wet forest. But there is an extreme rain shadow effect, and the eastern foothills and the 400-500km wide expanse of semi-flat pampas to the east, in Argentina, are exceptionally dry, with only 200mm of rain or less. This pampas area, which includes the eastern half of Tierra del Fuego, is covered in dry grass and low shrubs, has been developed as grazing land for several centuries, and is divided into numerous large grazing properties called ‘estancias’. It’s extremely boring country to travel through (everyone else on the bus went to sleep), and your eyes are constantly drawn to the snow-covered mountains to the west. Hence the Andes are a great tourist attraction for the local people – somewhere cool and moist and interesting to go. The long glacial history has resulted in huge volumes of rock (hundreds of cubic km) being carved away from the mountains by ice, deposited as moraine boulders around the foothills, and then re-deposited further out by rivers as endless plains of grey pebbly gravel, which is what much of the pampas consists of. -
Download Detailed Itinerary (Pdf)
CHILE T R E K K I N G T H E T O R R E S D E L P A I N E C I R C U I T B Y F O O T 9 - D A Y S This Patagonia adventure, hiking through famous Torres del Paine National Park along the Paine Circuit, is an unmatched Patagonia hiking adventure. During this 9 day trek, we experience one of the world’s last great nature refuges, surrounded every step of the way by raw, unspoiled beauty and nature. At night, we refuel at camps located near the big eco-camp or other refugios, enjoying most of our morning and evening meals within their comforts, the stunning park as our backyard. This Patagonia hike is truly an unparalleled outdoor experience. Day 1 PUNTA ARENAS - TORRES DEL PAINE ARRIVAL All travellers must arrive into the Punta Arenas airport by 11:00am. We'll be there to greet you and transfer you to the famous Torres del Paine National Park, 345 km/216 miles away. The drive is approximately 5 hours, but a very scenic one and in the summer months (December to March) the sun sets around 11pm, so we have plenty of light to admire the landscape en route while entering the park. If we’re lucky we’ll see guanacos, rheas and huge rabbits grazing on the plains. On the way, we will Day 2 stop for lunch in Puerto Natales, a village ECOCAMP TO DICKSON LAKE on the shores of "Seno de Ultima TREKKING Esperanza." The entire journey into Torres del Paine is scenic and invigorating, as we'll The day begins with breakfast at the Eco- quickly start seeing the area's wildlife, camp before we prepare for our hike to including many birds. -
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. -
Remote Sensing Study of Glacial Change in the Northern Patagonian Icefield
Advances in Remote Sensing, 2015, 4, 270-279 Published Online December 2015 in SciRes. http://www.scirp.org/journal/ars http://dx.doi.org/10.4236/ars.2015.44022 Remote Sensing Study of Glacial Change in the Northern Patagonian Icefield Lucy Dixon, Shrinidhi Ambinakudige Department of Geosciences, Mississippi State University, Starkville, MS, USA Received 23 October 2015; accepted 27 November 2015; published 30 November 2015 Copyright © 2015 by authors and Scientific Research Publishing Inc. This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/ Abstract The Patagonian Icefield has the largest temperate ice mass in the southern hemisphere. Using re- mote sensing techniques, this study analyzed multi-decadal glacial retreat and expansion of glaci- er lakes in Northern Patagonia. Glacial boundaries and glacier lake boundaries for 1979, 1985, 2000, and 2013 were delineated from Chilean topographic maps and Landsat satellite images. As- ter stereo images were used to measure mass balance from 2007 to 2012. The highest retreat was observed in San Quintin glacier. The area of glacier lakes increased from 13.49 km2 in 1979 to 65.06 km2 in 2013. Four new glacier lakes formed between 1979 and 2013. Between 2007 and 2012, significant glacial thinning was observed in major glaciers, including HPN1, Pared Norte, Strindberg, Acodado, Nef, San Quintin, Colonia, HPN4, and Benito glaciers. Generally, ablation zones lost more mass than accumulation zones. Keywords Patagonia, Glaciers, South America, ASTER 1. Introduction Glaciers are key indicators for assessing climate change [1]-[3]. Beginning in the nineteenth century, glaciers in many parts of the world retreated significantly, which was a clear indicator of climate warming [3]-[7]. -
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 -
Glacial Lakes of the Central and Patagonian Andes
Aberystwyth University Glacial lakes of the Central and Patagonian Andes Wilson, Ryan; Glasser, Neil; Reynolds, John M.; Harrison, Stephan; Iribarren Anacona, Pablo; Schaefer, Marius; Shannon, Sarah Published in: Global and Planetary Change DOI: 10.1016/j.gloplacha.2018.01.004 Publication date: 2018 Citation for published version (APA): Wilson, R., Glasser, N., Reynolds, J. M., Harrison, S., Iribarren Anacona, P., Schaefer, M., & Shannon, S. (2018). Glacial lakes of the Central and Patagonian Andes. Global and Planetary Change, 162, 275-291. https://doi.org/10.1016/j.gloplacha.2018.01.004 Document License CC BY General rights Copyright and moral rights for the publications made accessible in the Aberystwyth Research Portal (the Institutional Repository) are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. • Users may download and print one copy of any publication from the Aberystwyth Research Portal for the purpose of private study or research. • You may not further distribute the material or use it for any profit-making activity or commercial gain • You may freely distribute the URL identifying the publication in the Aberystwyth Research Portal Take down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. tel: +44 1970 62 2400 email: [email protected] Download date: 09. Jul. 2020 Global and Planetary Change 162 (2018) 275–291 Contents lists available at ScienceDirect Global and Planetary Change journal homepage: www.elsevier.com/locate/gloplacha Glacial lakes of the Central and Patagonian Andes T ⁎ Ryan Wilsona, , Neil F. -
The 2015 Chileno Valley Glacial Lake Outburst Flood, Patagonia
Aberystwyth University The 2015 Chileno Valley glacial lake outburst flood, Patagonia Wilson, R.; Harrison, S.; Reynolds, John M.; Hubbard, Alun; Glasser, Neil; Wündrich, O.; Iribarren Anacona, P.; Mao, L.; Shannon, S. Published in: Geomorphology DOI: 10.1016/j.geomorph.2019.01.015 Publication date: 2019 Citation for published version (APA): Wilson, R., Harrison, S., Reynolds, J. M., Hubbard, A., Glasser, N., Wündrich, O., Iribarren Anacona, P., Mao, L., & Shannon, S. (2019). The 2015 Chileno Valley glacial lake outburst flood, Patagonia. Geomorphology, 332, 51-65. https://doi.org/10.1016/j.geomorph.2019.01.015 Document License CC BY General rights Copyright and moral rights for the publications made accessible in the Aberystwyth Research Portal (the Institutional Repository) are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. • Users may download and print one copy of any publication from the Aberystwyth Research Portal for the purpose of private study or research. • You may not further distribute the material or use it for any profit-making activity or commercial gain • You may freely distribute the URL identifying the publication in the Aberystwyth Research Portal Take down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. tel: +44 1970 62 2400 email: [email protected] Download date: 09. Jul. 2020 Geomorphology 332 (2019) 51–65 Contents lists available at ScienceDirect Geomorphology journal homepage: www.elsevier.com/locate/geomorph The 2015 Chileno Valley glacial lake outburst flood, Patagonia R. -
Area Changes of Glaciers on Active Volcanoes in Latin America Between 1986 and 2015 Observed from Multi-Temporal Satellite Imagery
Journal of Glaciology (2019), Page 1 of 15 doi: 10.1017/jog.2019.30 © The Author(s) 2019. This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons. org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited. Area changes of glaciers on active volcanoes in Latin America between 1986 and 2015 observed from multi-temporal satellite imagery JOHANNES REINTHALER,1,2 FRANK PAUL,1 HUGO DELGADO GRANADOS,3 ANDRÉS RIVERA,2,4 CHRISTIAN HUGGEL1 1Department of Geography, University of Zurich, Zurich, Switzerland 2Centro de Estudios Científicos, Valdivia, Chile 3Instituto de Geofisica, Universidad Nacional Autónoma de México, Mexico City, Mexico 4Departamento de Geografía, Universidad de Chile, Chile Correspondence: Johannes Reinthaler <[email protected]> ABSTRACT. Glaciers on active volcanoes are subject to changes in both climate fluctuations and vol- canic activity. Whereas many studies analysed changes on individual volcanoes, this study presents for the first time a comparison of glacier changes on active volcanoes on a continental scale. Glacier areas were mapped for 59 volcanoes across Latin America around 1986, 1999 and 2015 using a semi- automated band ratio method combined with manual editing using satellite images from Landsat 4/5/ 7/8 and Sentinel-2. Area changes were compared with the Smithsonian volcano database to analyse pos- sible glacier–volcano interactions. Over the full period, the mapped area changed from 1399.3 ± 80 km2 − to 1016.1 ± 34 km2 (−383.2 km2)or−27.4% (−0.92% a 1) in relative terms. -
To Late-Holocene Explosive Rhyolitic Eruptions from Chaitén Volcano, Chile
Andean Geology 40 (2): 216-226. May, 2013 Andean Geology doi: 10.5027/andgeoV40n2-a02 formerly Revista Geológica de Chile www.andeangeology.cl Evidence of mid- to late-Holocene explosive rhyolitic eruptions from Chaitén Volcano, Chile Sebastian F.L. Watt1, 2, David M. Pyle1, Tamsin A. Mather1 1 Department of Earth Sciences, University of Oxford, South Parks Road, Oxford OX1 3AN, U.K. [email protected]; [email protected]; [email protected] 2 National Oceanography Centre, Southampton, University of Southampton Waterfront Campus, European Way, Southampton SO14 3ZH, U.K. ABSTRACT. The 2008 eruption of Chaitén Volcano was widely cited as the first activity at the volcano for over 9000 years. However, we have identified evidence from proximal pyroclastic deposits for three additional explosive eruptions of Chaitén within the past 5000 years. Chaitén has therefore produced at least five explosive eruptions in the Holocene, making it among the most active volcanoes, in terms of explosive output, in the southern part of the Andean Southern Volcanic Zone. All of the five identified Holocene explosive eruptions produced homogeneous high-silica rhyolite, with near identical compositions. Based on our pyroclastic sequence, we suggest that the largest-volume Holocene eruption of Chaitén occurred at ~4.95 ka, and we correlate this with the Mic2 deposit, which was previously thought to originate from the nearby Michinmahuida Volcano. Keywords: Chaitén Volcano, Andean southern volcanic zone, Holocene tephra stratigraphy, Rhyolite, Explosive volcanism. RESUMEN. Evidencia de erupciones riolíticas del Holoceno medio a tardío del volcán Chaitén, Chile. La erupción del volcán Chaitén en el año 2008 ha sido mencionada ampliamente como la primera actividad de este en los últimos 9 mil años. -
Lawrence Berkeley National Laboratory Recent Work
Lawrence Berkeley National Laboratory Recent Work Title Assessment of high enthalpy geothermal resources and promising areas of Chile Permalink https://escholarship.org/uc/item/9s55q609 Authors Aravena, D Muñoz, M Morata, D et al. Publication Date 2016 DOI 10.1016/j.geothermics.2015.09.001 Peer reviewed eScholarship.org Powered by the California Digital Library University of California Assessment of high enthalpy geothermal resources and promising areas of Chile Author links open overlay panel DiegoAravena ab MauricioMuñoz ab DiegoMorata ab AlfredoLahsen ab Miguel ÁngelParada ab PatrickDobson c Show more https://doi.org/10.1016/j.geothermics.2015.09.001 Get rights and content Highlights • We ranked geothermal prospects into measured, Indicated and Inferred resources. • We assess a comparative power potential in high-enthalpy geothermal areas. • Total Indicated and Inferred resource reaches 659 ± 439 MWe divided among 9 areas. • Data from eight additional prospects suggest they are highly favorable targets. • 57 geothermal areas are proposed as likely future development targets. Abstract This work aims to assess geothermal power potential in identified high enthalpy geothermal areas in the Chilean Andes, based on reservoir temperature and volume. In addition, we present a set of highly favorable geothermal areas, but without enough data in order to quantify the resource. Information regarding geothermal systems was gathered and ranked to assess Indicated or Inferred resources, depending on the degree of confidence that a resource may exist as indicated by the geoscientific information available to review. Resources were estimated through the USGS Heat in Place method. A Monte Carlo approach is used to quantify variability in boundary conditions. -
OIB Antarctic Flight 10, Antarctica Peninsula #2 Aircraft DC-8 Flight
OIB Antarctic Flight 10, Antarctica Peninsula #2 Aircraft DC-8 Flight Number DC8-100119 Flt Req # 108002 Flight Hours 9.4 Date 10/31/09 Purpose of Flight ICE Bridge Peninsula-2 Aircraft Status Airworthy Sensor Status All installed sensors operational. Significant Issues None Accomplishments Low level survey over a variety of Peninsula targets. Cloud cover obscured about 400 km of the planned 2300 km lines (~18% loss). Cloud cover affected the regions south of 72 deg. Sensors worked throughout. LVIS collected approximately one hour of sea ice data during the transit. McCords, Snow and Ku Band radars were operational throughout the target areas. Made a low pass over Palmer Station and conducted two passes over Punta Arenas for instrument calibration. Planned events Down day tomorrow Flight Summary Peninsula-2, FLT 11 Saturday, October 31, 2009 Seelye Martin (Mission Principal Investigator): Weather Summary: this is the first potentially clear day on the Peninsula. AMPS forecast shows a major system moving from west, reaching peninsula about 1800 UTC. Peninsula south of about 73 S is under heavy clouds. From their Antarctic forecast network, Fight Services shows that the lower Peninsula has broken cloud decks at 1,500 and 3,000 ft. Quoting John Sonntag, “For any other area, we would not fly, but the peninsula is open so infrequently that we have to try it.” Suspect we will have cloud problems at both north and south end of flight lines. Mission Description: This is a repeat of ATM lines flown by the Chilean/NASA P-3 in October 2008. The lines cover the Fleming Glacier, Mobile Oil Inlet and a pair of ICESat lines, one on the George-V ice shelf and a parallel one over Palmer Land, plus a single pass down the Crane Glacier. -
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