Dissertation Calibration of the Pierre Auger Observatory Fluorescence
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Monadnock Vol. 45 | June 1971
THE MONADNOCK I - L. .RK UNIVERSITY Vol. XLV )GRAPHICAL SOCIETY June, 1971 THE MQNADNOCK Volume XIN Editor, Edwin T. Wei5e, Jr. Aaooite Editor5 James FOnSeOa Kirsten Haring David Seairøn Photoqzapher, Ernie Wight ypists Ronnie Mason Phyllis sczynski 323812 ii ‘7f THE MONADNOCK CONTENTs . 2 DIRECT0I MESSAGE THE JESUITS IN NORTH AMERICA: A STUDY . IN ENVIRONMENTAL COCEUALIZATI Eenry Aay 4 STRUCTURE IN TRANSACTION SYSTEMS. .Christopher Clayton 9 CULTURE AND AGRICULTURE ON THE ANEPJCAN NTIER Brad Baltensperger 22 THE PROBABILISTIC APPROACH TO SPATIAL THEORY Kang-tsung Chang 30 AROHITECTURE AND GEOGRAPHICAL STUDIES: A REVIEW Stephen Hobart 36 AN ESSAY ON GROWTH POLE THEORY B. David Miller 40 MIND, MEANING, AND MILIEU: PSYCHOLOGICAL NEED AND DESIGRED ENVIRONMENTS Ernest A. Wight Jr 43 SPATIAL DYNAMICS IN CLASSICAL LOCATION THEORY Alfred Hecht 52 THE GRADUATE SCHOOL OF GEOGRAPHY 56 ALUMNI NEWS 65 A N(YTE ON THE QUESTIONNAIRE 80 :1 DIRECTOR’S MESSAGE This academic year is very special for Geography at Clark, marking the fiftieth year of the founding of the Graduate School of Geography by Wallace W. Atwood. Dedication of the new Geography facilities — with special recognition to the memory of John K. Wright, Historical Geographer and Geosophist, an adopted son of Clark — is one appropriate mode of celebration. Another mark of the occasion is the honor accorded to two major figures in American Geography: Clark could not have chosen two more distinguished geographers than Richard Hartshorne and Samuel Van Valkenburg on whom were bestowed .1 . - Honorary Doctorates of Law at the anniversary ceremonies of April .17th. Very different in their contributions and their characters, Richard Hartshorne provided American geography with its philosophic and method ological rationale and Dr. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
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, -
A Study About the Temporal Constraints on the Martian Yardangs’ Development in Medusae Fossae Formation
remote sensing Article A Study about the Temporal Constraints on the Martian Yardangs’ Development in Medusae Fossae Formation Jia Liu 1,2 , Zongyu Yue 1,3,*, Kaichang Di 1,3 , Sheng Gou 1,4 and Shengli Niu 4 1 State Key Laboratory of Remote Sensing Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100101, China; [email protected] (J.L.); [email protected] (K.D.); [email protected] (S.G.) 2 University of Chinese Academy of Sciences, Beijing 100049, China 3 CAS Center for Excellence in Comparative Planetology, Hefei 230026, China 4 State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau 999078, China; [email protected] * Correspondence: [email protected]; Tel.: +86-10-64889553 Abstract: The age of Mars yardangs is significant in studying their development and the evolution of paleoclimate conditions. For planetary surface or landforms, a common method for dating is based on the frequency and size distribution of all the superposed craters after they are formed. However, there is usually a long duration for the yardangs’ formation, and they will alter the superposed craters, making it impossible to give a reliable dating result with the method. An indirect method by analyzing the ages of the superposed layered ejecta was devised in the research. First, the layered ejecta that are superposed on and not altered by the yardangs are identified and mapped. Then, the ages of the layered ejecta are derived according to the crater frequency and size distribution on them. These ages indicate that the yardangs ceased development by these times, and the ages are valuable for studying the evolution of the yardangs. -
The Ship 2014/2015
A more unusual focus in your magazine this College St Anne’s year: architecture and the engineering skills that make our modern buildings possible. The start of our new building made this an obvious choice, but from there we go on to look at engineering as a career and at the failures and University of Oxford follies of megaprojects around the world. Not that we are without the usual literary content, this year even wider in range and more honoured by awards than ever. And, as always, thanks to the generosity and skills of our contributors, St Anne’s College Record a variety of content and experience that we hope will entertain, inspire – and at times maybe shock you. My thanks to the many people who made this issue possible, in particular Kate Davy, without whose support it could not happen. Hope you enjoy it – and keep the ideas coming; we need 2014 – 2015 them! - Number 104 - The Ship Annual Publication of the St Anne’s Society 2014 – 2015 The Ship St Anne’s College 2014 – 2015 Woodstock Road Oxford OX2 6HS UK The Ship +44 (0) 1865 274800 [email protected] 2014 – 2015 www.st-annes.ox.ac.uk St Anne’s College St Anne’s College Alumnae log-in area Development Office Contacts: Lost alumnae Register for the log-in area of our website Over the years the College has lost touch (available at https://www.alumniweb.ox.ac. Jules Foster with some of our alumnae. We would very uk/st-annes) to connect with other alumnae, Director of Development much like to re-establish contact, and receive our latest news and updates, and +44 (0)1865 284536 invite them back to our events and send send in your latest news and updates. -
GEOLOGY THEME STUDY Page 1
NATIONAL HISTORIC LANDMARKS Dr. Harry A. Butowsky GEOLOGY THEME STUDY Page 1 Geology National Historic Landmark Theme Study (Draft 1990) Introduction by Dr. Harry A. Butowsky Historian, History Division National Park Service, Washington, DC The Geology National Historic Landmark Theme Study represents the second phase of the National Park Service's thematic study of the history of American science. Phase one of this study, Astronomy and Astrophysics: A National Historic Landmark Theme Study was completed in l989. Subsequent phases of the science theme study will include the disciplines of biology, chemistry, mathematics, physics and other related sciences. The Science Theme Study is being completed by the National Historic Landmarks Survey of the National Park Service in compliance with the requirements of the Historic Sites Act of l935. The Historic Sites Act established "a national policy to preserve for public use historic sites, buildings and objects of national significance for the inspiration and benefit of the American people." Under the terms of the Act, the service is required to survey, study, protect, preserve, maintain, or operate nationally significant historic buildings, sites & objects. The National Historic Landmarks Survey of the National Park Service is charged with the responsibility of identifying America's nationally significant historic property. The survey meets this obligation through a comprehensive process involving thematic study of the facets of American History. In recent years, the survey has completed National Historic Landmark theme studies on topics as diverse as the American space program, World War II in the Pacific, the US Constitution, recreation in the United States and architecture in the National Parks. -
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 -
Proceedings of the United States National Museum
Proceedings of the United States National Museum SMITHSONIAN INSTITUTION • WASHINGTON, D.C. Volume 123 1967 Number 3604 Revision of the Beetles Of Genus Glyptoscelis (Coleoptera: Chrysomelidae) By Doris H. Blake Honorary Research Associate, Department of Entomology In a paper on the Coleoptera of Fort Tejon, Calif. (Proc. Acad. Nat. Sci. Philadelphia, vol. 9, p. 81, 1859), LeConte briefly de- scribed the genus Glyptoscelis as follows: "The genus Glyptoscelis (Chevrolat) [Dejean Catalogue, 3rd ed., p. 438, nomen nudum, 1837] is distinguished from the other genera allied to Eumolpus by the mouth not being covered beneath by the presternum, by the claws being toothed, and by the tibiae being longitudinally sulcate. The head is not sculptured as in Heteraspis [Graphops]." The first species, pubescens, was described as early as 1777 by Fabri- cius under Eumolpus. Linneaus in 1788 gave this species another name, and he was followed by Olivier in 1808 with still another specific name, and our own early American entomologist, Thomas Say, in 1827 gave a fourth name to this species, which is widespread over the eastern half of the United States. Say also described two other species from the eastern and middle states under Eumolpus. In LeConte's paper of 1859 he described Glyptoscelis albida, the first species from the West Coast. In 1878, nearly 20 years later, he de- scribed G. longior, a second western species. In the meantime, in l 2 PROCEEDINGS OF THE NATIONAL MUSEUM vol. 123 1873, Crotch, adopting LeConte's generic name Glyptoscelis, de- scribed from California three more species of this predominately West Coast genus. -
Lhcb Prepares for RICH Physics
I n t e r n at I o n a l J o u r n a l o f H I g H - e n e r g y P H y s I c s CERN COURIERV o l u m e 47 n u m b e r 6 J u ly/a u g u s t 2 0 07 LHCb prepares for RICH physics NEUTRINOS LHC FOCUS InSIDE STORY Borexino starts On the trail of At the far side to take data p8 heavy flavour p30 of the world p58 CCJulAugCover1.indd 1 11/7/07 13:50:51 Project1 10/7/07 13:56 Page 1 CONTENTS Covering current developments in high- energy physics and related fields worldwide CERN Courier is distributed to member-state governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly, except for January and August. The views expressed are not necessarily those of the CERN management. Editor Christine Sutton CERN CERN, 1211 Geneva 23, Switzerland E-mail [email protected] Fax +41 (0) 22 785 0247 Web cerncourier.com Advisory board James Gillies, Rolf Landua and Maximilian Metzger Laboratory correspondents: COURIERo l u m e u m b e r u ly u g u s t V 47 N 6 J /A 20 07 Argonne National Laboratory (US) Cosmas Zachos Brookhaven National Laboratory (US) P Yamin Cornell University (US) D G Cassel DESY Laboratory (Germany) Ilka Flegel, Ute Wilhelmsen EMFCSC (Italy) Anna Cavallini Enrico Fermi Centre (Italy) Guido Piragino Fermi National Accelerator Laboratory (US) Judy Jackson Forschungszentrum Jülich (Germany) Markus Buescher GSI Darmstadt (Germany) I Peter IHEP, Beijing (China) Tongzhou Xu IHEP, Serpukhov (Russia) Yu Ryabov INFN (Italy) Barbara Gallavotti Jefferson Laboratory (US) Steven Corneliussen JINR -
South Pole-Aitken Basin
Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole. -
Annual Report 2014-2015
2014 2015 Annual Report Table of Contents 2/3 The International Space Science Institute (ISSI) is an Institute of Advanced Studies where scientists from all over the world meet in a multi- and interdisciplinary setting to reach out for new scientific horizons. The main function is to contribute to the achievement of a deeper understanding of the re- sults from different space missions, ground based observations and laboratory experiments, and add- ing value to those results through multidisciplinary research. The program of ISSI covers a widespread spectrum of disciplines from the physics of the solar system and planetary sciences to astrophysics and cosmology, and from Earth sciences to astrobiology. 4 From the Board of Trustees 20 International Teams 5 From the Directors 37 International Teams approved in 2015 6 About the International Space Science Institute 39 Visiting Scientists 7 The Board of Trustees 41 International Space Science Institute Beijing 8 The Science Committee 42 Events and ISSI in the media at a glance (including centerfold) 9 ISSI Staff 44 Staff Activities 10 Facilities 48 Staff Publications 11 Financial Overview 51 Visitor Publications 12 The Association Pro ISSI 61 Space Sciences Series of ISSI (SSSI) 13 Scientific Activities: The 20th Year 66 ISSI Scientific Reports Series (SR) 14 Forum 67 Pro ISSI SPATIUM Series 15 Workshops 68 ISSI Publications in the 20th Business Year ISSI Annual Report 2014 | 2015 From the Board of Trustees One year ago the undersigned was appointed by the President as secretary of the Board, succeeding Kathrin Altwegg who had served in that capacity for six years. -
Laser Beam Profile & Beam Shaping
Copyright by Priti Duggal 2006 An Experimental Study of Rim Formation in Single-Shot Femtosecond Laser Ablation of Borosilicate Glass by Priti Duggal, B.Tech. Thesis Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Master of Science in Engineering The University of Texas at Austin August 2006 An Experimental Study of Rim Formation in Single-Shot Femtosecond Laser Ablation of Borosilicate Glass Approved by Supervising Committee: Adela Ben-Yakar John R. Howell Acknowledgments My sincere thanks to my advisor Dr. Adela Ben-Yakar for showing trust in me and for introducing me to the exciting world of optics and lasers. Through numerous valuable discussions and arguments, she has helped me develop a scientific approach towards my work. I am ready to apply this attitude to my future projects and in other aspects of my life. I would like to express gratitude towards my reader, Dr. Howell, who gave me very helpful feedback at such short notice. My lab-mates have all positively contributed to my thesis in ways more than one. I especially thank Dan and Frederic for spending time to review the initial drafts of my writing. Thanks to Navdeep for giving me a direction in life. I am excited about the future! And, most importantly, I want to thank my parents. I am the person I am, because of you. Thank you. 11 August 2006 iv Abstract An Experimental Study of Rim Formation in Single-Shot Femtosecond Laser Ablation of Borosilicate Glass Priti Duggal, MSE The University of Texas at Austin, 2006 Supervisor: Adela Ben-Yakar Craters made on a dielectric surface by single femtosecond pulses often exhibit an elevated rim surrounding the crater.