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Annual Report 2011-2012
____2011 2012 Annual Report Cover Page Imprint Puzzle composed of six images (from the upper left to the lower right): Publisher International Space Science Institute 1. The Three Gorges Dam spans the Yangtze River in Hallerstrasse 6 east-central China, and is the world's largest power CH-3012 Bern station in terms of installed capacity, with its vast Switzerland reservoir stretching for 660 km (NASA, GSFC, METI, Tel.: +41 31 631 48 96 ERSDAC, JAROS, and U.S./Japan ASTER Science Fax.: +41 31 631 48 97 Team). E-mail: [email protected] Internet: www.issibern.ch 2. The High Resolution Stereo Camera on ESA’s Mars Express orbiter has obtained images of Hephaestus Editors Fossae, a region on Mars dotted with craters and Andrea Fischer and Rudolf von Steiger channel systems (ESA, DLR, FU Berlin (G. Neukum)). Concept/Layout 3. This X-ray image shows a comet-like blob of gas Andrea Fischer about 5 million light-years long hurling through a distant galaxy cluster at nearly 1 000 kilometres per Cover Design second (University of Maryland, Baltimore County Andrea Fischer (UMBC)). Printed by 4. Picture of the cosmic microwave background Länggass Druck AG (CMB) radiation which thermal radiation filling the Länggassstr. 65 observable universe almost uniformly (WMAP Sci- 3000 Bern 9 ence Team, NASA). Switzerland 5. The map of the surface of an exoplanet, or a planet beyond our solar system. The map, which shows temperature variations across the cloudy tops of a gas giant called HD 189733b, is made from in- frared data taken by NASA's Spitzer Space Telescope (NASA, JPL Caltech, H. -
A MTAK Kiadványai 47. Budapest, 1966
A MAGYAR TUDOMÁNYOS AKADÉMIA KÖNYVTARÁNAK KÖZLEMÉNYEI PUBLICATIONES BIBLIOTHECAE ACADEMIAE SCIENTIARUM HUNGARICAE 47. INDEX ÀCRONYMORUM SELECTORUM Institute* communicationis BUDAPEST, 1966 VOCABULARIUM ABBREVIATURARUM BIBLIOTHECARII III Index acronymorum selectorum 7. Instituta communicationis A MAGYAR TUDOMÁNYOS AKADÉMIA KÖNYVTARÁNAK KÖZLEMÉNYEI PUBLICATIONES BIBLIOTHECAE ACADEMIAE SCIENTIARUM HUNGARICAE 47. VOCABULARIUM ABBREVIATURARUM BIBLIOTHECARII Index acronymorum selectorum 7. Instituta communicationis BUDAPEST, 196 6 A MAGYAR TUDOMÁNYOS AKADÉMIA KÖNYVTARÁNAK KÖZLEMÉNYEI PUBLICATIONES BIBLIOTHECAE ACADEMIAE SCIENTIARUM HUNGARICAE 47. INDEX ACRONYMORUM SELECTORUM 7 Instituta communications. BUDAPEST, 1966 INDEX ACRONYMORUM SELECTORUM Pars. 7. Instituta communicationis. Adiuvantibus EDIT BODNÁ R-BERN ÁT H et MAGDA TULOK collegit et edidit dr. phil. ENDRE MORAVEK Lectores: Gyula Tárkányi Sámuel Papp © 1966 MTA Köynvtára F. к.: Rózsa György — Kiadja a MTA Könyvtára — Példányszám: 750 Alak A/4. - Terjedelem 47'/* A/5 ív 65395 - M.T.A. KESz sokszorosító v ELŐSZÓ "Vocabularium abbreviaturarum bibliothecarii" cimü munkánk ez ujabb füzete az "Index acronymorum selectorum" kötet részeként, a köz- lekedési és hírközlési intézmények /ilyen jellegű állami szervek, vasu- tak, légiközlekedési vállalatok, távirati irodák, sajtóügynökségek stb/ névröviditéseit tartalmazza. Az idevágó felsőbb fokú állami intézmények /pl. minisztériumok stb./ nevének acronymáit, amelyeket az "Instituta rerum publicarum" c. kötetben közöltünk, technikai okokból nem -
Walter Alvarez,Professor
DEPARTMENT OF EARTH & PLANETARY SCIENCE DEPARTMENT UPDATE 2017 -2018 FROM THE CHAIR WELCOME TO OUR ANNUAL UPDATE write this introduction after returning from our summer geology field camp. What a treat. I met many of the students when they took their first geoscience class, EPS 50. The capstone field course showed how much these new alumni Ihave grown during their time in EPS to develop into creative and talented geoscientists. On page 13 we hear from one of our 66 new graduates, Departmental Citation recipient Theresa Sawi, about her efforts to understand how earthquakes influence volcanic eruptions. Our faculty, students, staff and alumni continue to make our department one of the world’s best. Our newest faculty member, Bethanie Edwards (page 3), broadens the department’s expertise to include marine biogeochemistry. Along with the arrival of Bill Boos and Daniel Stolper two years ago, we continue to expand our efforts to understand all MARINE SCIENCE aspects of Earth’s changing climate. GET TO KNOW OUR FACULTY There have also been some losses. After 36 years, Tim Teague retired. He may be irreplaceable, but we will try. After three years of dedicated service, always with a smile, Richard Allen’s term as chair ended, and he will continue to direct the Seismological Laboratory. Mark Richards moved to Seattle where he is the University of Washington’s provost. Accolades continue to pour in, and I highlight a few. The American Geophysical Union recognized recent Alumnus Leif BETHANIE EDWARDS Karlstrom with the Kuno Award (page 16) and Professor David Romps with the Atmospheric Sciences Ascent award. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Near Surface CO2 Triple Oxygen Isotope Composition
Terr. Atmos. Ocean. Sci., Vol. 27, No. 1, 99-106, February 2016 doi: 10.3319/TAO.2015.09.16.01(A) Near Surface CO2 Triple Oxygen Isotope Composition Sasadhar Mahata1, Chung-Ho Wang 2, Sourendra Kumar Bhattacharya1, and Mao-Chang Liang1, 3, 4, 5, * 1 Research Center for Environmental Changes, Academia Sinica, Taipei, Taiwan, R.O.C. 2 Institute of Earth Sciences, Academia Sinica, Taipei, Taiwan, R.O.C. 3 Graduate Institute of Astronomy, National Central University, Taoyuan, Taiwan, R.O.C. 4 Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan, R.O.C. 5 Department of Physics, University of Houston, Texas, U.S.A. Received 9 March 2015, revised 14 June 2015, accepted 16 September 2015 ABSTRACT The isotopic composition of carbon dioxide in the atmosphere is a powerful tool for constraining its sources and sinks. In particular, the 17O oxygen anomaly [Δ17O = 1000 × ln(1 + δ17O/1000) - 0.516 × 1000 × ln(1 + δ18O/1000)], with a value > 0.5‰ produced in the middle atmosphere, provides an ideal tool for probing the exchange of carbon dioxide between the biosphere/hydrosphere and atmosphere. The biosphere/hydrosphere and anthropogenic emissions give values ≤ 0.3‰. There- fore, any anomaly in near surface CO2 would reflect the balance between stratospheric input and exchange with the aforemen- 17 tioned surface sources. We have analyzed Δ O values of CO2 separated from air samples collected in Taipei, Taiwan, located in the western Pacific region. The obtained mean anomaly is 0.42 ± 0.14‰ (1-σ standard deviation), in good agreement with model prediction and a published decadal record. -
Evaluating the Options for Carbon Sequestration
Evaluating the options for carbon sequestration Clair Gough and Simon Shackley Tyndall Centre (North), UMIST, Manchester Melvin G. R. Cannell Centre for Ecology and Hydrology, Bush Estate, Midlothian November 2002 Tyndall Centre for Climate Change Research Technical Report 2 Evaluating the options for carbon sequestration Tyndall Centre Technical Report No. 2 November 2002 This is the final report from Tyndall research project IT1.22 (Carbon sequestration: a pilot stage multi-criteria evaluation of biological and physio-chemical approaches). The following researchers worked on this project: Dr Simon Shackley and Clair Gough, Tyndall Centre (North) and Manchester School of Management, UMIST Prof Melvin Cannell and Dr Ronnie Milne, Centre for Ecology and Hydrology, Edinburgh Prof John Shepherd, Tyndall Centre (South), Southampton Oceanography Centre, University of Southampton Contents Page Number Introduction 1 Section A. Biological Carbon Sequestration 1. Carbon sequestration 3 2. Biomass Energy Substitution 9 3. Discussion 20 References 24 Section B. Geological Carbon Sequestration 1. Key Options and Issues 29 2. Long-term scenarios for carbon storage 39 3. Multi Criteria Assessment 45 4. Conclusions 66 References 68 Appendix A Glossary of terms and units Appendix B Carbon Storage Scenarios Appendix C Assessment Criteria Appendix D Interview participants Appendix E Multi-criteria Evaluation of Low Carbon Energy Technologies (spreadsheet) Appendix F Working Paper “Burying Carbon under the Sea: An Initial Exploration of Public Opinions” Acknowledgements The authors would like to thank all of those stakeholders whom we have consulted in the process of conducting this study. In particular, we would like to thank Sam Holloway and others at the British Geological Survey. -
Science-Centric Sampling Approaches of Geo-Physical Environments for Realistic Robot Navigation
SCIENCE-CENTRIC SAMPLING APPROACHES OF GEO-PHYSICAL ENVIRONMENTS FOR REALISTIC ROBOT NAVIGATION A Thesis Presented to The Academic Faculty by Lonnie T. Parker, IV In Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the School of Electrical and Computer Engineering Georgia Institute of Technology August 2012 Copyright c 2012 by Lonnie T. Parker, IV SCIENCE-CENTRIC SAMPLING APPROACHES OF GEO-PHYSICAL ENVIRONMENTS FOR REALISTIC ROBOT NAVIGATION Approved by: Professor Ayanna M. Howard, Advisor Professor Jeff Shamma School of Electrical and Computer School of Electrical and Computer Engineering Engineering Georgia Institute of Technology Georgia Institute of Technology Professor Fumin Zhang Professor Mike Stilman School of Electrical and Computer College of Computing Engineering Georgia Institute of Technology Georgia Institute of Technology Professor George Riley Date Approved: June 15, 2012 School of Electrical and Computer Engineering Georgia Institute of Technology DEDICATION Based upon the infallible word of God, I dedicate this work to Him, according to Proverbs 16:3. iii ACKNOWLEDGEMENTS Before anyone else, I want to acknowledge and thank my Lord and Savior, Jesus Christ, whom I am in and who lives within me. This degree and this experience would not be possible without His provision, favor, and grace. Especially in the moments when I did not believe it was possible to finish, my faith in Him pushed me forward. Next, to my wife, Andrea, who has been my constant encourager, supporter, and living reminder that I could complete this journey, thank you. Simply your presence in my life has made this walk all the more bearable. I love you. -
Global 3-D Simulations of the Triple Oxygen Isotope Signature 17O in Atmospheric
RESEARCH ARTICLE Global 3-D Simulations of the Triple Oxygen Isotope 10.1029/2019JD030387 17 Signature Δ O in Atmospheric CO2 Key Points: • This work presents a first view Gerbrand Koren1 , Linda Schneider2,3, Ivar R. van der Velde4,5, Erik van Schaik1, on possible spatial and temporal 6,7 8 8 17 Sergey S. Gromov , Getachew A. Adnew , Dorota J. Mrozek Martino , gradients of Δ OinCO2 across the 8,9 10 11 12 globe Magdalena E. G. Hofmann , Mao-Chang Liang , Sasadhar Mahata , Peter Bergamaschi , • Tropical, boreal, and Southern Ingrid T. van der Laan-Luijkx1, Maarten C. Krol1,8 , Thomas Röckmann8 , 17 Hemisphere observations of Δ Oin and Wouter Peters1,13 CO2 could be of great interest • We implemented spatially and 1Meteorology and Air Quality Group, Wageningen University & Research, Wageningen, The Netherlands, 2Institute of temporally explicit sources and sinks Meteorology and Climate Research (IMK-TRO), Karlsruhe Institute of Technology, Karlsruhe, Germany, 3Now at of Δ17OinCO in a 3-D model 2 4 framework Zentrum für Sonnenenergie- und Wasserstoff-Forschung Baden-Württemberg (ZSW), Stuttgart, Germany, Earth System Research Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, USA, 5Now at Faculty of Science, VU University Amsterdam, Amsterdam, The Netherlands, 6Atmospheric Chemistry Department, Max-Planck Supporting Information: Institute for Chemistry, Mainz, Germany, 7Institute of Global Climate and Ecology of Roshydromet and RAS, Moscow, • Supporting Information S1 Russia, 8Institute of Marine and Atmospheric Research, Utrecht University, Utrecht, The Netherlands, 9Now at Picarro B.V. 's-Hertogenbosch, The Netherlands, 10Institute of Earth Sciences, Academia Sinica, Taipei, Taiwan, 11Institute of Correspondence to: Global Environmental Change, Xian Jiaotong University, Xian, China, 12European Commission Joint Research Centre, G. -
Drawing Down N2 O
www.unep.org United Nations Environment Programme Drawing Down N2O P. O. Box 30552 - 00100 Nairobi, Kenya Tel.: +254 20 762 1234 Fax: +254 20 762 3927 e-mail: [email protected] To Protect Climate and the Ozone Layer www.unep.org A UNEP Synthesis Report Published by the United Nations Environment Programme (UNEP), November 2013 Copyright © UNEP 2013 ISBN: 978-92-807-3358-7 DEW/1748/NA This publication may be reproduced in whole or in part and in any form for educational or non-profit services without special permission from the copyright holder, provided acknowledgement of the source is made. UNEP would appreciate receiving a copy of any publication that uses this publication as a source. No use of this publication may be made for resale or any other commercial purpose whatsoever without prior permission in writing from the United Nations Environment Programme. Applications for such permission, with a statement of the purpose and extent of the reproduction, should be addressed to the Director, DCPI, UNEP, P. O. Box 30552, Nairobi 00100, Kenya. Disclaimers Mention of a commercial company or product in this document does not imply endorsement by UNEP or the authors. The use of information from this document for publicity or advertising is not permitted. Trademark names and symbols are used in an editorial fashion with no intention on infringement of trademark or copyright laws. We regret any errors or omissions that may have been unwittingly made. © Images and illustrations as specified. Cover Images: All images from Shutterstock. Forest fire: Peter J. Wilson; Agriculture collage: Symbiot; Coal fire plant: Gary Whitton; Atmosphere: Andrew Armyagov. -
Exobiology in the Solar System & the Search for Life on Mars
SP-1231 SP-1231 October 1999 Exobiology in the Solar System & The Search for Life on Mars for The Search Exobiology in the Solar System & Exobiology in the Solar System & The Search for Life on Mars Report from the ESA Exobiology Team Study 1997-1998 Contact: ESA Publications Division c/o ESTEC, PO Box 299, 2200 AG Noordwijk, The Netherlands Tel. (31) 71 565 3400 - Fax (31) 71 565 5433 SP-1231 October 1999 EXOBIOLOGY IN THE SOLAR SYSTEM AND THE SEARCH FOR LIFE ON MARS Report from the ESA Exobiology Team Study 1997-1998 Cover Fossil coccoid bacteria, 1 µm in diameter, found in sediment 3.3-3.5 Gyr old from the Early Archean of South Africa. See pages 160-161. Background: a portion of the meandering canyons of the Nanedi Valles system viewed by Mars Global Surveyor. The valley is about 2.5 km wide; the scene covers 9.8 km by 27.9 km centred on 5.1°N/48.26°W. The valley floor at top right exhibits a 200 m-wide channel covered by dunes and debris. This channel suggests that the valley might have been carved by water flowing through the system over a long period, in a manner similar to rivers on Earth. (Malin Space Science Systems/NASA) SP-1231 ‘Exobiology in the Solar System and The Search for Life on Mars’, ISBN 92-9092-520-5 Scientific Coordinators: André Brack, Brian Fitton and François Raulin Edited by: Andrew Wilson ESA Publications Division Published by: ESA Publications Division ESTEC, Noordwijk, The Netherlands Price: 70 Dutch Guilders/ EUR32 Copyright: © 1999 European Space Agency Contents Foreword 7 I An Exobiological View of the -
SITE SELECTION for the FIRST SUSTAINABLE MARS BASE Workshop Abstract #2001
SITE SELECTION FOR THE FIRST SUSTAINABLE MARS BASE Workshop Abstract #2001 D. C. Barker, MAXD, Inc. G. James, NASA JSC G. Chamitoff, Texas A&M University S. Clifford, LPI Exploration Zone Map #1002 1st EZ Workshop for Human Missions to Mars 150 E 180 E 210 E 40 N Utopia Planetia V2 Dorsa Arcadia Planetia Phlegra EZ 39N, 172E 30 N Elysium Mons 1 39N, 172E 2 Exploration Zone Map #1002 All RROIs are SROIs but all SROIs are not necessarily RROIs ! 1st EZ Workshop for Human Missions to Mars Dome Structures Landing Zone SROI 1 & Base (25km x 20km) Tyndall S1 Alt -3960 m Crater S3 SROI 4 S4 S1 Fluidized 2 Craters Plains S1 S3 SROI 3 Units S3 RROI 3 S1 2 EZ S2 2 S1 100 km rad Hydrated Minerals S3 SROI 2 Sheet S1 Silicates Near 1 RROI 2 Surface Ice THEMIS Image RROI 1 EZ wide 39N, 172E 3 Exploration Zone Map #1002 1st EZ Workshop for Human Missions to Mars TES Dust Cover Index (DCI) TES over THEMIS 1 39N, 172E 4 Exploration Zone Map #1002 1st EZ Workshop for Human Missions to Mars TES Rock Abundance TES over THEMIS 1 39N, 172E 5 Landing Zone 1st EZ Workshop for Human Missions to Mars 172 E Elevation Thermal Inertia Slope Albedo Dust Index 25km x 20km (larger than Avg: -3966 Avg: 240.2 Avg: 0.33 Avg: 0.156 Avg: 0.968 expected for precision Max: -3953 Max: 253 Max: 0.99 Max: 0.996 Max: 0.983 human landing) Min: -3985 Min: 233 Min: 0.03 Min: 0.025 Min: 0.949 average annual temperature ~(-73.15 C) 39 N Final Landing Sites and Base infrastructure could be moved widely in this region without altering access to primary resources (i.e., H2O) or areas of scientific interest t. -
1St Eucornea Congress Venice 2010 June 17-19 Programme
1st EuCornea Congress Venice 2010 June 17-19 Programme o r n C e u a E E u a e C o r n European Society of Cornea and Ocular Surface Disease Specialists in Joint Meeting - Società Italiana Cellulle Staminali e Superficie Oculare (S.I.C.S.S.O.) - Società Oftalmologica Universitaria (S.O.U.) - [email protected] Local Organiser: Giancarlo Caprioglio Scientific Co-ordinator: Paolo Vinciguerra REGIONE DEL VENETO 1st EuCornea Congress Buffet Dinner, Magic Show DJ and Dancing Friday 18 June Enjoy a beautiful dinner in the Arsenale de Venezia followed by a Magic Show performed by the famous Silvan Tickets: €55 each (Available at the EuCornea registration desk) ~ ACCESS BY PRIVATE BOAT ONLY ~ Private Boats will depart from the Molino Stucky Hilton at 7.00pm Private Boats will depart from St Mark’s Square at 7.10pm Private Boats will depart from the Arsenale to the Molino Stucky Hilton and St Mark’s Square at 11.30pm and 01.00am in Joint Meeting: Venice June 17-19 - Società Italiana Cellulle Staminali e Superficie Oculare (S.I.C.S.S.O.) - Società Oftalmologi Universitari (S.O.U.) 2010 - [email protected] COntentS EuCornea Board 2 Message from the President 3 General Information 4 Scientific Programme Overview 5 Plan of Congress Centre 6 List of Exhibitors and Exhibition Floorplan 7 Scientific Sessions – Thursday 8 Scientific Sessions – Friday 12 Scientific Sessions – Saturday 16 EuCornea Medal Lectures 16 Courses / Industry Symposia 17 Electronic Posters 19 Keynote Abstracts 25 Invited Speaker Abstracts 29 Free Paper Abstracts 39 Poster Abstracts 65 Vaporetto Map 76 Molino Stucky Hilton Shuttle Boat Timetable 77 Tours 78 Index 79 1 1st EuCornea Congress eUCORnea BOaRd PReSIdent: Vincenzo Sarnicola ITALY PReSIdent EleCt/ VICe PReSIdent: Harminder S.