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Fifth World Forestry Congress
Proceedings of the Fifth World Forestry Congress VOLUME 1 RE University of Washington, Seattle, Washington United States of America August 29September 10, 1960 The President of the United States of America DWIGHT D. EISENHOWER Patron Fifth World Forestry Congress III Contents VOLUME 1 Page Chapter1.Summary and Recommendations of the Congress 1 Chapter 2.Planning for the Congress 8 Chapter3.Local Arrangements for the Congress 11 Chapter 4.The Congress and its Program 15 Chapter 5.Opening Ceremonies 19 Chapter6. Plenary Sessions 27 Chapter 7.Special Congress Events 35 Chapitre 1.Sommaire et recommandations du Congrès 40 Chapitre 2.Preparation des plans en vue du Congrès 48 Chapitre 3.Arrangements locaux en vue du Congrès 50 Chapitre 4.Le Congrès et son programme 51 Chapitre 5.Cérémonies d'ouverture 52 Chapitre 6.Seances plénières 59 Chapitre 7.Activités spéciales du Congrès 67 CapItullo1. Sumario y Recomendaciones del Congreso 70 CapItulo 2.Planes para el Congreso 78 CapItulo 3.Actividades Locales del Congreso 80 CapItulo 4.El Congreso y su Programa 81 CapItulo 5.Ceremonia de Apertura 81 CapItulo 6.Sesiones Plenarias 88 CapItulo 7.Actos Especiales del Congreso 96 Chapter8. Congress Tours 99 Chapter9.Appendices 118 Appendix A.Committee Memberships 118 Appendix B.Rules of Procedure 124 Appendix C.Congress Secretariat 127 Appendix D.Machinery Exhibitors Directory 128 Appendix E.List of Financial Contributors 130 Appendix F.List of Participants 131 First General Session 141 Multiple Use of Forest Lands Utilisation multiple des superficies boisées Aprovechamiento Multiple de Terrenos Forestales Second General Session 171 Multiple Use of Forest Lands Utilisation multiple des superficies boisées Aprovechamiento Multiple de Terrenos Forestales Iv Contents Page Third General Session 189 Progress in World Forestry Progrés accomplis dans le monde en sylviculture Adelantos en la Silvicultura Mundial Section I.Silviculture and Management 241 Sessions A and B. -
Research Natural Areas on National Forest System Lands in Idaho, Montana, Nevada, Utah, and Western Wyoming: a Guidebook for Scientists, Managers, and Educators
USDA United States Department of Agriculture Research Natural Areas on Forest Service National Forest System Lands Rocky Mountain Research Station in Idaho, Montana, Nevada, General Technical Report RMRS-CTR-69 Utah, and Western Wyoming: February 2001 A Guidebook for Scientists, Managers, and E'ducators Angela G. Evenden Melinda Moeur J. Stephen Shelly Shannon F. Kimball Charles A. Wellner Abstract Evenden, Angela G.; Moeur, Melinda; Shelly, J. Stephen; Kimball, Shannon F.; Wellner, Charles A. 2001. Research Natural Areas on National Forest System Lands in Idaho, Montana, Nevada, Utah, and Western Wyoming: A Guidebook for Scientists, Managers, and Educators. Gen. Tech. Rep. RMRS-GTR-69. Ogden, UT: U.S. Departmentof Agriculture, Forest Service, Rocky Mountain Research Station. 84 p. This guidebook is intended to familiarize land resource managers, scientists, educators, and others with Research Natural Areas (RNAs) managed by the USDA Forest Service in the Northern Rocky Mountains and lntermountain West. This guidebook facilitates broader recognitionand use of these valuable natural areas by describing the RNA network, past and current research and monitoring, management, and how to use RNAs. About The Authors Angela G. Evenden is biological inventory and monitoring project leader with the National Park Service -NorthernColorado Plateau Network in Moab, UT. She was formerly the Natural Areas Program Manager for the Rocky Mountain Research Station, Northern Region and lntermountain Region of the USDA Forest Service. Melinda Moeur is Research Forester with the USDA Forest Service, Rocky Mountain ResearchStation in Moscow, ID, and one of four Research Natural Areas Coordinators from the Rocky Mountain Research Station. J. Stephen Shelly is Regional Botanist and Research Natural Areas Coordinator with the USDA Forest Service, Northern Region Headquarters Office in Missoula, MT. -
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. -
Magnetite Biomineralization and Ancient Life on Mars Richard B Frankel* and Peter R Buseckt
Magnetite biomineralization and ancient life on Mars Richard B Frankel* and Peter R Buseckt Certain chemical and mineral features of the Martian meteorite with a mass distribution unlike terrestrial PAHs or those from ALH84001 were reported in 1996 to be probable evidence of other meteorites; thirdly, bacterium-shaped objects (BSOs) ancient life on Mars. In spite of new observations and up to several hundred nanometers long that resemble fos interpretations, the question of ancient life on Mars remains silized terrestrial microorganisms; and lastly, 10-100 nm unresolved. Putative biogenic, nanometer magnetite has now magnetite (Fe304), pyrrhotite (Fel_xS), and greigite (Fe3S4) become a leading focus in the debate. crystals. These minerals were cited as evidence because of their similarity to biogenic magnetic minerals in terrestrial Addresses magnetotactic bacteria. *Department of Physics, California Polytechnic State University, San Luis Obispo, California 93407, USA; e-mail: [email protected] The ancient life on Mars hypothesis has been extensively tDepartments of Geology and Chemistry/Biochemistry, Arizona State challenged, and alternative non-biological processes have University, Tempe, Arizona 85287-1404, USA; e-mail: [email protected] been proposed for each of the four features cited by McKay et al. [4]. In this paper we review the current situa tion regarding their proposed evidence, focusing on the Abbreviations putative biogenic magnetite crystals. BCM biologically controlled mineralization BIM biologically induced mineralization BSO bacterium-shaped object Evidence for and against ancient Martian life PAH polycyclic aromatic hydrocarbon PAHs and BSOs Reports of contamination by terrestrial organic materials [5°,6°] and the similarity of ALH84001 PAHs to non-bio genic PAHs in carbonaceous chondrites [7,8] make it Introduction difficult to positively identify PAHs of non-terrestrial, bio A 2 kg carbonaceous stony meteorite, designated genic origin. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Holocene Glacier Fluctuations
Quaternary Science Reviews 111 (2015) 9e34 Contents lists available at ScienceDirect Quaternary Science Reviews journal homepage: www.elsevier.com/locate/quascirev Invited review Holocene glacier fluctuations * Olga N. Solomina a, b, , Raymond S. Bradley c, Dominic A. Hodgson d, Susan Ivy-Ochs e, f, Vincent Jomelli g, Andrew N. Mackintosh h, Atle Nesje i, j, Lewis A. Owen k, Heinz Wanner l, Gregory C. Wiles m, Nicolas E. Young n a Institute of Geography RAS, Staromonetny-29, 119017, Staromonetny, Moscow, Russia b Tomsk State University, Tomsk, Russia c Department of Geosciences, University of Massachusetts, Amherst, MA 012003, USA d British Antarctic Survey, High Cross, Madingley Road, Cambridge CB3 0ET, UK e Institute of Particle Physics, ETH Zurich, 8093 Zurich, Switzerland f Institute of Geography, University of Zurich, 8057 Zurich, Switzerland g Universite Paris 1 Pantheon-Sorbonne, CNRS Laboratoire de Geographie Physique, 92195 Meudon, France h Antarctic Research Centre, Victoria University Wellington, New Zealand i Department of Earth Science, University of Bergen, N-5020 Bergen, Norway j Uni Research Klima, Bjerknes Centre for Climate Research, N-5020 Bergen Norway k Department of Geology, University of Cincinnati, Cincinnati, OH 45225, USA l Institute of Geography and Oeschger Centre for Climate Change Research, University of Bern, Switzerland m Department of Geology, The College of Wooster, Wooster, OH 44691, USA n Lamont-Doherty Earth Observatory, Columbia University, Palisades, NY, USA article info abstract Article history: A global overview of glacier advances and retreats (grouped by regions and by millennia) for the Received 15 July 2014 Holocene is compiled from previous studies. The reconstructions of glacier fluctuations are based on Received in revised form 1) mapping and dating moraines defined by 14C, TCN, OSL, lichenometry and tree rings (discontinuous 22 November 2014 records/time series), and 2) sediments from proglacial lakes and speleothems (continuous records/ Accepted 27 November 2014 time series). -
From Meteorites to Evolution and Habitability of Planets
Planetary and Space Science 72 (2012) 3–17 Contents lists available at SciVerse ScienceDirect Planetary and Space Science journal homepage: www.elsevier.com/locate/pss From meteorites to evolution and habitability of planets Dehant Ve´ronique a,n, Breuer Doris b, Claeys Philippe c, Debaille Vinciane d, De Keyser Johan e, Javaux Emmanuelle f, Goderis Steven c, Karatekin O¨ zgur a, Spohn Tilman b, Vandaele Ann Carine e, Vanhaecke Frank g, Van Hoolst Tim a, Wilquet Vale´rie e a Royal Observatory of Belgium, 3 avenue Circulaire, Brussels, B-1180, Belgium b Deutsche Zentrum fur¨ Luft- und Raumfahrt, Berlin, Germany c Vrije Universiteit Brussel, Brussels, Belgium d Universite´ Libre de Bruxelles, Brussels, Belgium e Belgian Institute for Space Aeronomy, Brussels, Belgium f Universite´ de Liege, 4000 Liege 1, Belgique g Universiteit Gent, Brussels, Belgium article info abstract Article history: The evolution of planets is driven by the composition, structure, and thermal state of their internal core, Received 31 March 2012 mantle, lithosphere, and crust, and by interactions with a possible ocean and/or atmosphere. A planet’s Accepted 29 May 2012 history is a long chronology of events with possibly a sequence of apocalyptic events in which asteroids, Available online 23 June 2012 comets and their meteorite offspring play an important role. Large meteorite impacts on the young Keywords: Earth could have contributed to the conditions for life to appear, and similarly large meteorite impacts Terrestrial planets could also create the conditions to erase life or drastically decrease biodiversity on the surface of the Habitability planet. Meteorites also contain valuable information to understand the evolution of a planet through Meteorites their gas inclusion, their composition, and their cosmogenic isotopes. -
Local Controls on Sediment Accumulation and Distribution in a Fjord in the West Antarctic Peninsula: Implications for Palaeoenvironmental Interpretations Yuribia P
RESEARCH/REVIEW ARTICLE Local controls on sediment accumulation and distribution in a fjord in the West Antarctic Peninsula: implications for palaeoenvironmental interpretations Yuribia P. Munoz & Julia S. Wellner Department of Earth and Atmospheric Sciences, University of Houston, 4800 Calhoun Road, Houston, TX 77204, USA Keywords Abstract Flandres Bay; Antarctic Peninsula; sediment We analyse surface sediment and its distribution in Flandres Bay, West Antarctic distribution; grain size. Peninsula, in order to understand modern day sediment dispersal patterns in Correspondence a fjord with retreating, tidewater glaciers. The surface sediment descriptions Yuribia P. Munoz, Department of Earth and of 41 cores are included in this study. The sediment facies described include Atmospheric Sciences, University of muddy diatomaceous ooze, diatomaceous mud, pebbly mud, sandy mud and Houston, 4800 Calhoun Road, Houston, mud, with scattered pebbles present in most samples. In contrast to a traditional TX 77204, USA. E-mail: [email protected] conceptual model of glacial sediment distribution in fjords, grain size in Flandres Bay generally coarsens from the inner to outer bay. The smallest grain size sediments were found in the bay head and are interpreted as fine-grained deposits resulting from meltwater plumes and sediment gravity flows occurring close to the glacier front. The middle of the bay is characterized by a high silt percentage, which correlates to diatom-rich sediments. Sediments in the outer bay have a high component of coarse material, which is interpreted as being the result of winnowing from currents moving from the Bellingshausen Sea into the Gerlache Strait. Palaeoenvironmental reconstructions of glacial environ- ments often use grain size as an indicator of proximity to the ice margin. -
Aqueous Alteration in Martian Meteorites: Comparing Mineral Relations in Igneous-Rock Weathering of Martian Meteorites and in the Sedimentary Cycle of Mars
AQUEOUS ALTERATION IN MARTIAN METEORITES: COMPARING MINERAL RELATIONS IN IGNEOUS-ROCK WEATHERING OF MARTIAN METEORITES AND IN THE SEDIMENTARY CYCLE OF MARS MICHAEL A. VELBEL Department of Geological Sciences, 206 Natural Science Building, Michigan State University, East Lansing, Michigan 48824-1115 USA e-mail: [email protected] ABSTRACT: Many of the minerals observed or inferred to occur in the sediments and sedimentary rocks of Mars, from a variety of Mars-mission spacecraft data, also occur in Martian meteorites. Even Martian meteorites recovered after some exposure to terrestrial weathering can preserve preterrestrial evaporite minerals and useful information about aqueous alteration on Mars, but the textures and textural contexts of such minerals must be examined carefully to distinguish preterrestrial evaporite minerals from occurrences of similar minerals redistributed or formed by terrestrial processes. Textural analysis using terrestrial microscopy provides strong and compelling evidence for preterrestrial aqueous alteration products in a numberof Martian meteorites. Occurrences of corroded primary rock-forming minerals and alteration products in meteorites from Mars cover a range of ages of mineral–water interaction, from ca. 3.9 Ga (approximately mid-Noachian), through one or more episodes after ca. 1.3 Ga (approximately mid–late Amazonian), through the last half billion years (late Amazonian alteration in young shergottites), to quite recent. These occurrences record broadly similar aqueous corrosion processes and formation of soluble weathering products over a broad range of times in the paleoenvironmental history of the surface of Mars. Many of the same minerals (smectite-group clay minerals, Ca-sulfates, Mg-sulfates, and the K-Fe–sulfate jarosite) have been identified both in the Martian meteorites and from remote sensing of the Martian surface. -
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MacArtney, Adrienne (2018) Atmosphere crust coupling and carbon sequestration on early Mars. PhD thesis. http://theses.gla.ac.uk/9006/ Copyright and moral rights for this work are retained by the author A copy can be downloaded for personal non-commercial research or study, without prior permission or charge This work cannot be reproduced or quoted extensively from without first obtaining permission in writing from the author The content must not be changed in any way or sold commercially in any format or medium without the formal permission of the author When referring to this work, full bibliographic details including the author, title, awarding institution and date of the thesis must be given Enlighten:Theses http://theses.gla.ac.uk/ [email protected] ATMOSPHERE - CRUST COUPLING AND CARBON SEQUESTRATION ON EARLY MARS By Adrienne MacArtney B.Sc. (Honours) Geosciences, Open University, 2013. Submitted in partial fulfilment of the requirements for the degree of Doctor of Philosophy at the UNIVERSITY OF GLASGOW 2018 © Adrienne MacArtney All rights reserved. The author herby grants to the University of Glasgow permission to reproduce and redistribute publicly paper and electronic copies of this thesis document in whole or in any part in any medium now known or hereafter created. Signature of Author: 16th January 2018 Abstract Evidence exists for great volumes of water on early Mars. Liquid surface water requires a much denser atmosphere than modern Mars possesses, probably predominantly composed of CO2. Such significant volumes of CO2 and water in the presence of basalt should have produced vast concentrations of carbonate minerals, yet little carbonate has been discovered thus far. -
Ancient Martian Life in Allan Hills 84001? Status of Some Current Controversies
Workshop on the Issue of Martian Meteorites 7043.pdf ANCIENT MARTIAN LIFE IN ALLAN HILLS 84001? STATUS OF SOME CURRENT CONTROVERSIES. A. H. Treiman, Lunar and Planetary Institute, 3600 Bay Area Boulevard, Houston TX 77058, USA ([email protected]). Four lines of evidence were taken to suggest that ALH Also, it is possible that the elongate magnetites formed at 84001 contained traces of ancient martian life preserved in high T, but after the carbonates formed [5]. Magnetites are its carbonate mineral masses [1]: abundance of organic also present in void spaces in the carbonate, either as the compounds (PAHs), disequilibrium mineral assemblages, product of decarbonation at high T [21] or as entrapped from morphology of sub-micron magnetite crystals, and presence the aqueous fluid that deposited the carbonates [22]. of objects comparable in size and shape to bacteria. This Summary. There is no consensus on the formation T or evidence is predicated on the carbonate globules having mechanism of carbonate masses. The bulk of evidence, in formed at temperatures conducive to life. Here, I review my opinion, is not consistent with T>400°C [4,6,7]. At pres- evidence on carbonate formation temperature, martian ori- ent, there seems no way to tell whether the carbonates gin of organic compounds, and bacteria-shaped objects. formed at moderate or low T: hotter or colder than ~150°C. Formation Temperature: A precondition for signs of Organic Matter: McKay et al. [1] presented evidence life associated with the carbonate masses [1] is that the that the carbonate pancakes in ALH 84001 are enriched in masses formed at T amenable to life (as we know it) [2], polycyclic aromatic hydrocarbons, PAHs, which are organic <~150°C. -
Mars Pathfinder Landing Site Workshop Ii: Characteristics of the Ares Vallis Region and Field Trips in the Channeled Scabland, Washington
/, NASA-CR-200508 L / MARS PATHFINDER LANDING SITE WORKSHOP II: CHARACTERISTICS OF THE ARES VALLIS REGION AND FIELD TRIPS IN THE CHANNELED SCABLAND, WASHINGTON LPI Technical Report Number 95-01, Part 1 Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI/TR--95-01, Part 1 "lp MARS PATHFINDER LANDING SITE WORKSHOP II: CHARACTERISTICS OF THE ARES VALLIS REGION AND FIELD TRIPS IN THE CHANNELED SCABLAND, WASHINGTON Edited by M. P. Golombek, K. S. Edgett, and J. W. Rice Jr. Held at Spokane, Washington September 24-30, 1995 Sponsored by Arizona State University Jet Propulsion Laboratory Lunar and Planetary Institute National Aeronautics and Space Administration Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Technical Report Number 95-01, Part 1 LPI/TR--95-01, Part 1 Compiled in 1995 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the University Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may he copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This report may he cited as Golomhek M. P., Edger K. S., and Rice J. W. Jr., eds. ( 1992)Mars Pathfinder Landing Site Workshop 11: Characteristics of the Ares Vallis Region and Field Trips to the Channeled Scabland, Washington. LPI Tech. Rpt. 95-01, Part 1, Lunar and Planetary Institute, Houston. 63 pp.