Walter Alvarez,Professor
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Program and Abstracts of 2017 Congress / Programme Et Résumés
1 Sponsors | Commanditaires Gold Sponsors | Commanditaires d’or Silver Sponsors | Commanditaires d’argent Other Sponsors | Les autres Commanditaires 2 Contents Sponsors | Commanditaires .......................................................................................................................... 2 Welcome from the Premier of Ontario .......................................................................................................... 5 Bienvenue du premier ministre de l'Ontario .................................................................................................. 6 Welcome from the Mayor of Toronto ............................................................................................................ 7 Mot de bienvenue du maire de Toronto ........................................................................................................ 8 Welcome from the Minister of Fisheries, Oceans and the Canadian Coast Guard ...................................... 9 Mot de bienvenue de ministre des Pêches, des Océans et de la Garde côtière canadienne .................... 10 Welcome from the Minister of Environment and Climate Change .............................................................. 11 Mot de bienvenue du Ministre d’Environnement et Changement climatique Canada ................................ 12 Welcome from the President of the Canadian Meteorological and Oceanographic Society ...................... 13 Mot de bienvenue du président de la Société canadienne de météorologie et d’océanographie ............. -
Global Scale Impacts
Global Scale Impacts Erik Asphaug Arizona State University Gareth Collins Imperial College, London Martin Jutzi University of Bern Global scale impacts modify the physical or thermal state of a substantial fraction of a target asteroid. Specific effects include accretion, family formation, reshaping, mixing and layering, shock and frictional heating, fragmentation, material compaction, dilatation, stripping of mantle and crust, and seismic degradation. Deciphering the complicated record of global scale impacts, in asteroids and meteorites, will lead us to understand the original planet-forming process and its resultant populations, and their evolution in time as collisions became faster and fewer. We provide a brief overview of these ideas, and an introduction to models. 1. Introduction v1 < v2 are the velocities of the target and projectile in the center of mass frame. If the energy is sufficiently intense, The most important parameter governing the global ex- Q > Q , then shattering occurs, breaking the solid bonds tent of an impact is the mass ratio of the projectile to the S∗ of the asteroid into pieces no larger than M =2. If gravita- target, γ = M =M . In the case of a cratering event this 1 2 1 tionally bound (ejected at < v ) then shattering produces ratio is small, and there is a well-defined geometric locus. esc a rubble pile as defined below; otherwise if fragments are Crater scaling then becomes a powerful tool (e.g. Housen escaping, the result is a collection of new asteroids. This et al. 1983) that allows simple analytical approaches to be is the classic example of hitting something so hard that applied to determine whether an impact ‘goes global’ – for you break it. -
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 -
In Pdf Format
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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. -
VOLCANIC ERUPTIONS at PLATE BOUNDARIES Give Your Research the Visibility It Deserves
VOL. 97 NO. 13 1 JUL 2016 Career Paths for African-American Students Did Solar Flares Cook Up Life? High Energy Growth Forecast Through 2040 VOLCANIC ERUPTIONS AT PLATE BOUNDARIES Give Your Research the Visibility it Deserves Abstract Submission Deadline: 3 August Submit by 27 July and Win Big Submit your abstract by 27 July for the chance to win Fall Meeting VIP status, including front row seats for two at all keynote lectures, and more fallmeeting.agu.org Earth & Space Science News Contents 1 JULY 2016 PROJECT UPDATE VOLUME 97, ISSUE 13 9 Creating Career Paths for African-American Students in Geosciences A new initiative at Stony Brook University teaches marketable skills, engages students in research projects, and fosters professional career tracks of underrepresented minorities. NEWS 6 Advisory Panel Calls for Large Increase for Ocean Exploration The recently established Ocean Exploration Advisory Board also urged the National Oceanic and Atmospheric Administration 12 to increase its role in federal coordination of exploration. COVER RESEARCH SPOTLIGHT Understanding Volcanic Eruptions Researchers Attribute Where Plates Meet 31 Human Infl uence on Climate Back to 1930s A new project clarifies the relationships between tectonics and A new study finds that humans likely have volcanic systems and how they influence hazards on Italy’s Mount triggered the past 16 record-breaking hot Etna and Vulcano and Lipari islands. years on Earth, up to 2014. Earth & Space Science News Eos.org // 1 Contents DEPARTMENTS Editor in Chief Barbara T. Richman: AGU, Washington, D. C., USA; eos_ [email protected] Editors Christina M. S. Cohen Wendy S. -
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. -
Experimental Investigations of Photochemically-Generated Organic Aerosols and Applications to Early Earth and Mars
Experimental investigations of photochemically-generated organic aerosols and applications to early Earth and Mars By Emily Faye Chu A dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in Chemistry in the Graduate Division of the University of California, Berkeley Committee in charge: Professor Kristie A. Boering, Chair Professor Stephen R. Leone Professor Imke de Pater Spring 2013 Abstract Experimental investigations of photochemically-generated organic aerosols and applications to early Earth and Mars By Emily Faye Chu Doctor of Philosophy in Chemistry University of California, Berkeley Professor Kristie A. Boering, Chair Aerosols in planetary atmospheres play a critical role in radiative transfer and thus also in determining the penetration depth of UV radiation and atmospheric temperatures. For early Mars and an anoxic early Earth, aerosols may have significantly influenced the stability of liquid water at the surface, as well as climate and habitability, yet the study of aerosol formation remains poorly constrained by models and experiments, making conclusions difficult. Significant progress can be made in reducing these uncertainties by providing additional laboratory constraints and tests for the photochemical and microphysical models used to generate the greatly varying predictions about aerosol formation in terrestrial-like atmospheres. Photochemistry experiments measuring gas- and condensed-phase species were conducted to determine (1) the extent to which a photochemical -
Appendix I Authors and Editors
Appendix I Authors and editors Frances Bagenal (editor) Ofer Cohen Laboratory for Almospheric and Space Harvard-Smithsonian Center for Physics Astrophysics UCB 600 University of Colorado 60 Garden St. 3665 Discovery Drive Cambridge, MA 02138, USA Boulder, CO 80303, USA email: [email protected] email: [email protected] Debra Fischer Mario M. Bisi Department of Astronomy, Science and Technology Facilities Yale University, Council New Haven, CT 06520, USA Rutherford Appleton Laboratory email : [email protected] Harwell, Oxford OX 11 OQX, UK email: Mario.Bisi@<;lfc.ac.uk Marina Galand Department of Physics Stephen W. Boughcr Imperial CoHege London Atmospheric, Oceanic, and Space Prince Consort Road Science Department London SW7 2AZ, UK 2455 Hayward Avenue email: [email protected] University of Michigan Ann Arbor, MT 48109, USA Mihaly Horanyi email: [email protected] Laboratory for Almospheric and Space Physics, and David Brain Department of Physics Laboratory for Atmospheric and Space Un iversiLy of Colorado, Boulder, CO Physics 80303, USA University of Colorado email: Mihaly.Horanyi@Jasp. 3665 Discovery Drive colorado.edu Boulder, CO 80303, USA email: [email protected] 327 328 Appe11dL\ I A11rliors and editors Margaret G. Kivel son Palo Alto, CA 94304- I 191, USA Department of Earth, Planetary, and email: [email protected] Space Sciences University of California, Los Angeles David E. Siskind Los Angeles, CA 90095-1567. USA Space Science Division and Naval Research Laboratory Department of Atmospheric, Oceanic 4555 Overlook Ave. SW and Space Sciences Washington DC, 20375, USA University of Mi chigan email: [email protected] Ann Arbor, MI 48109-2143, USA Jan J. -
MILLER INSTITUTE NEWSLETTER Miller Fellow Focus: Alex Thompson
MILLER INSTITUTE NEWSLETTER Fall 2005 Miller Fellow Focus: Alex Thompson Second year Miller Fellow Alex atmospheric non-methane Thompson is an atmospheric chemist hydrocarbons and halocarbons. She working with Prof. Ronald Amundson applied this analysis to very clean air in the Department of Environmental (from the Arctic and the Southern Science, Policy and Management. Ocean), and polluted air (from Toronto and Auckland) in order to How do human activities impact the understand emission patterns and chemistry of the atmosphere? What atmospheric processing, i.e. mixing are the interactions between the and photochemistry. After her Earth’s surface and the atmosphere? doctorate, Alex recognised that the How do these interactions impact the future of global environmental change climate and vice versa? These research involves understanding earth questions are the motivation behind system interfaces, often requiring a Alex’s research. More specifically, multidisciplinary approach. So she Alex is interested in using isotopes to came to UC Berkeley to work with probe the interface between the lower soil scientist and isotope geochemist atmosphere and the oceans, Prof. Ronald Amundson (ESPM). cryosphere, and biosphere. Isotopes They chose to investigate nitrous address the contribution of each of an element have only very small oxide. production pathway using the total differences in their chemical and 15N/14N and 18O/16O content of nitrous physical properties. Their relative Nitrous oxide lasts in the atmosphere oxide or its precursors as a diagnostic. sensitivity or insensitivity to various for a long time (~120 years) and has The problem is that bulk isotope processes allow isotope ratios to be 300 times the global warming signatures are not sufficiently distinct powerful tracers in many areas of potential of CO making it an 2 or well enough defined to differentiate natural science research, including extremely influential greenhouse gas. -
Director National Center for Atmospheric Research
Boulder, Colorado Director National Center for Atmospheric Research Leadership Profile Prepared by Suzanne M. Teer Robert W. Luke July 2018 This leadership profile is intended to provide information about UCAR and the position of Director, National Center for Atmospheric Research. It is designed to assist qualified individuals in assessing their interest in this position. The National Center for Atmospheric Research is a federally funded research and development center sponsored by the National Science Foundation. Since NCAR's founding in 1960, the University Corporation for Atmospheric Research, a nonprofit consortium of 117 North American academic institutions, has managed NCAR on behalf of NSF. The University Corporation for Atmospheric Research is an equal opportunity/equal access/affirmative action employer that strives to develop and maintain a diverse workforce. UCAR is committed to providing equal opportunity for all employees and applicants for employment and does not discriminate on the basis of race, age, creed, color, religion, national origin or ancestry, sex, gender, disability, veteran status, genetic information, sexual orientation, gender identity or expression, or pregnancy. UCAR is committed to inclusivity and promoting an equitable environment that values and respects the uniqueness of all members of the organization. 1 Table of Contents: The Opportunity: Overview 3 The Role: Director of the National Center for Atmospheric Research 4 Qualifications and Personal Qualities 5 Opportunities and Expectations for Leadership 7 The National Center for Atmospheric Research: An Overview 8 The National Science Foundation Cooperative Agreement 11 The University Corporation for Atmospheric Research: An Overview 12 Boulder, Colorado 17 Procedure for Candidacy 19 Appendix I: Diversity Statement 20 Appendix II: NCAR Director Search Committee 22 2 The Opportunity: Overview The University Corporation for Atmospheric Research invites inquiries, nominations, and expressions of interest for the position of Director of the National Center for Atmospheric Research.