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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. -
General Index
General Index Italicized page numbers indicate figures and tables. Color plates are in- cussed; full listings of authors’ works as cited in this volume may be dicated as “pl.” Color plates 1– 40 are in part 1 and plates 41–80 are found in the bibliographical index. in part 2. Authors are listed only when their ideas or works are dis- Aa, Pieter van der (1659–1733), 1338 of military cartography, 971 934 –39; Genoa, 864 –65; Low Coun- Aa River, pl.61, 1523 of nautical charts, 1069, 1424 tries, 1257 Aachen, 1241 printing’s impact on, 607–8 of Dutch hamlets, 1264 Abate, Agostino, 857–58, 864 –65 role of sources in, 66 –67 ecclesiastical subdivisions in, 1090, 1091 Abbeys. See also Cartularies; Monasteries of Russian maps, 1873 of forests, 50 maps: property, 50–51; water system, 43 standards of, 7 German maps in context of, 1224, 1225 plans: juridical uses of, pl.61, 1523–24, studies of, 505–8, 1258 n.53 map consciousness in, 636, 661–62 1525; Wildmore Fen (in psalter), 43– 44 of surveys, 505–8, 708, 1435–36 maps in: cadastral (See Cadastral maps); Abbreviations, 1897, 1899 of town models, 489 central Italy, 909–15; characteristics of, Abreu, Lisuarte de, 1019 Acequia Imperial de Aragón, 507 874 –75, 880 –82; coloring of, 1499, Abruzzi River, 547, 570 Acerra, 951 1588; East-Central Europe, 1806, 1808; Absolutism, 831, 833, 835–36 Ackerman, James S., 427 n.2 England, 50 –51, 1595, 1599, 1603, See also Sovereigns and monarchs Aconcio, Jacopo (d. 1566), 1611 1615, 1629, 1720; France, 1497–1500, Abstraction Acosta, José de (1539–1600), 1235 1501; humanism linked to, 909–10; in- in bird’s-eye views, 688 Acquaviva, Andrea Matteo (d. -
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. -
User Guide to 1:250,000 Scale Lunar Maps
CORE https://ntrs.nasa.gov/search.jsp?R=19750010068Metadata, citation 2020-03-22T22:26:24+00:00Z and similar papers at core.ac.uk Provided by NASA Technical Reports Server USER GUIDE TO 1:250,000 SCALE LUNAR MAPS (NASA-CF-136753) USE? GJIDE TO l:i>,, :LC h75- lu1+3 SCALE LUNAR YAPS (Lumoalcs Feseclrch Ltu., Ottewa (Ontario) .) 24 p KC 53.25 CSCL ,33 'JIACA~S G3/31 11111 DANNY C, KINSLER Lunar Science Instltute 3303 NASA Road $1 Houston, TX 77058 Telephone: 7131488-5200 Cable Address: LUtiSI USER GUIDE TO 1: 250,000 SCALE LUNAR MAPS GENERAL In 1972 the NASA Lunar Programs Office initiated the Apollo Photographic Data Analysis Program. The principal point of this program was a detailed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17. One of the requirements of this program was the production of detailed photo base maps at a useable scale. NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas. This paper is designed to present in outline form the neces- sary background informatiox or users to become familiar with the program. MAP FORMAT * The scale chosen for the project was 1:250,000 . The re- search being done required a scale that Principal Investigators (PI'S) using orbital photography could use, but would also serve PI'S doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west. -
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. -
Adams Adkinson Aeschlimann Aisslinger Akkermann
BUSCAPRONTA www.buscapronta.com ARQUIVO 27 DE PESQUISAS GENEALÓGICAS 189 PÁGINAS – MÉDIA DE 60.800 SOBRENOMES/OCORRÊNCIA Para pesquisar, utilize a ferramenta EDITAR/LOCALIZAR do WORD. A cada vez que você clicar ENTER e aparecer o sobrenome pesquisado GRIFADO (FUNDO PRETO) corresponderá um endereço Internet correspondente que foi pesquisado por nossa equipe. Ao solicitar seus endereços de acesso Internet, informe o SOBRENOME PESQUISADO, o número do ARQUIVO BUSCAPRONTA DIV ou BUSCAPRONTA GEN correspondente e o número de vezes em que encontrou o SOBRENOME PESQUISADO. Número eventualmente existente à direita do sobrenome (e na mesma linha) indica número de pessoas com aquele sobrenome cujas informações genealógicas são apresentadas. O valor de cada endereço Internet solicitado está em nosso site www.buscapronta.com . Para dados especificamente de registros gerais pesquise nos arquivos BUSCAPRONTA DIV. ATENÇÃO: Quando pesquisar em nossos arquivos, ao digitar o sobrenome procurado, faça- o, sempre que julgar necessário, COM E SEM os acentos agudo, grave, circunflexo, crase, til e trema. Sobrenomes com (ç) cedilha, digite também somente com (c) ou com dois esses (ss). Sobrenomes com dois esses (ss), digite com somente um esse (s) e com (ç). (ZZ) digite, também (Z) e vice-versa. (LL) digite, também (L) e vice-versa. Van Wolfgang – pesquise Wolfgang (faça o mesmo com outros complementos: Van der, De la etc) Sobrenomes compostos ( Mendes Caldeira) pesquise separadamente: MENDES e depois CALDEIRA. Tendo dificuldade com caracter Ø HAMMERSHØY – pesquise HAMMERSH HØJBJERG – pesquise JBJERG BUSCAPRONTA não reproduz dados genealógicos das pessoas, sendo necessário acessar os documentos Internet correspondentes para obter tais dados e informações. DESEJAMOS PLENO SUCESSO EM SUA PESQUISA. -
The W.A.S.P the Warren Astronomical Society Paper
Vol. 49, no. 11 November, 2018 The W.A.S.P The Warren Astronomical Society Paper President Jeff MacLeod [email protected] The Warren Astronomical Society First Vice President Jonathan Kade [email protected] Second Vice President Joe Tocco [email protected] Founded: 1961 Treasurer Ruth Huellmantel [email protected] P.O. Box 1505 Secretary Jerry Voorheis [email protected] Outreach Diane Hall [email protected] Warren, Michigan 48090-1505 Publications Brian Thieme [email protected] www.warrenastro.org Entire board [email protected] Photo credit: Joe Tocco 1 Society Meeting Times Astronomy presentations and lectures twice each month at 7:30 PM: First Monday at Cranbrook Institute of November Discussion Science. Group Meeting Third Thursday at Macomb Community College - South Campus Building E (Library) Come on over, and talk astronomy, space Note: for the rest of 2018, we are meeting in news, and whatnot! room E308, in building E. The Discussion Group meeting for November will be at Jon Blum’s home on Tuesday, November 20, at 7:00 PM. Jon has been Snack Volunteer hosting this every November for several years, Schedule so come and be part of the annual photo. Jon will provide lots of snacks, so please don’t Nov 5 Cranbrook Jim Shedlowsky bring any food or drinks. Jon’s home is in Nov 15 Macomb Riyad Matti Farmington Hills. Dec 3 Cranbrook Joe Tocco If you do not receive the address and directions If you are unable to bring the snacks on your in your email a week before this event, please scheduled day, or if you need to reschedule, email [email protected] for this information. -
01 Edmunson Simulant
SECTION 1: LUNAR HISTORY Dr. Jennifer Edmunson 1.1 Introduction Why understanding events in lunar history is important for engineers and simulant users: • It explains the motivation for exploration of the Moon. o To understand the evolution of our own planet. • It explains the origin of the operating environment for spacecraft, and ultimately influences the spacecraft design. • It describes human and spacecraft hazards. o Morphology of the landing site. o Micrometeorite bombardment. o Lunar regolith (boulders, dust). • It influences landing site locations. o Areas in permanent sunlight and shadow. o Regions of interest to scientists. • It provides the basis for predicting the chemical composition and physical properties of the lunar surface at specific sites. • It explains the impact history of the moon, which has changed the surface into its present form (creating the regolith). • It describes the processes that created the size distribution of regolith components, as well as their chemistry. 1.2 Initial Impact The Earth and Moon have similar chemistries and share the same oxygen isotope signature. This oxygen isotope signature is different from other planets and asteroids. Because of this, the Earth and Moon must have formed at the same distance from the Sun, or from a single chemical reservoir. The “Giant Impact” theory of lunar origin involves the proto-Earth being struck by a Mars-sized impactor (called Theia). Scientists favor this theory because it explains not only the similarities in composition (and the identical oxygen isotope signature) and the known mass of both the Earth and Moon, but the angular momentum of the Earth-Moon system. -
Upper Darby High School, 601 N Lansdowne Ave, Drexel Hill, PA
Basalt Thickness of Mare Tranquillitatis using Two Methods Upper Darby High School, 601 N Lansdowne Ave, Drexel Hill, PA Gutama Biru, Chris DeMott, Galen Farmer, Daniel Gordon, Isabel Hunt, Kenneth Lin, Thomas Nguyen, Zach Thornton, Vince Tran, Most Yeasmin PROBLEM ISOPACH MAPS The purpose of this experiment is to evaluate two methods of calculating basalt thickness in Mare Tranquillitatis. Figure 1 is the original isopach map used for reference. Figures 2 and 3 are isopach maps made using 3DField software. INTRODUCTION Lunar maria are large impact craters or basins that have been filled with basalt. While the Moon was still cooling, lava seeped into these basins through cracks, cooling to form the maria. This study compares two methods of determining the thickness of basalt in Mare Tranquillitatis: the Pre-Mare Crater Method and the Post- Figure 2. Pre-Mare Crater Isopach Mare Crater Method. The first method uses craters from before the mare was formed and the latter uses craters from after the mare was formed, as the names imply. Previous work ( De HONs map reference) has been conducted using these methods to Figure 1. Reference Map (DeHon 1974) calculate mare thickness; however the tools used to collect that data are outdated. The current study, conducted using data from the Lunar Reconnaissance Orbiter and Clementine camera, compares the two methods for determining mare thickness. The Pre-Mare Crater Method used craters that were formed inside the large impact basins before they filled with lava. By measuring the diameter of these craters, the original rim height can be estimated using a relationship defined by Pike (1974, 1977). -
Lita Ford and Doro Interviewed Inside Explores the Brightest Void and the Shadow Self
COMES WITH 78 FREE SONGS AND BONUS INTERVIEWS! Issue 75 £5.99 SUMMER Jul-Sep 2016 9 771754 958015 75> EXPLORES THE BRIGHTEST VOID AND THE SHADOW SELF LITA FORD AND DORO INTERVIEWED INSIDE Plus: Blues Pills, Scorpion Child, Witness PAUL GILBERT F DARE F FROST* F JOE LYNN TURNER THE MUSIC IS OUT THERE... FIREWORKS MAGAZINE PRESENTS 78 FREE SONGS WITH ISSUE #75! GROUP ONE: MELODIC HARD 22. Maessorr Structorr - Lonely Mariner 42. Axon-Neuron - Erasure 61. Zark - Lord Rat ROCK/AOR From the album: Rise At Fall From the album: Metamorphosis From the album: Tales of the Expected www.maessorrstructorr.com www.axonneuron.com www.facebook.com/zarkbanduk 1. Lotta Lené - Souls From the single: Souls 23. 21st Century Fugitives - Losing Time 43. Dimh Project - Wolves In The 62. Dejanira - Birth of the www.lottalene.com From the album: Losing Time Streets Unconquerable Sun www.facebook. From the album: Victim & Maker From the album: Behind The Scenes 2. Tarja - No Bitter End com/21stCenturyFugitives www.facebook.com/dimhproject www.dejanira.org From the album: The Brightest Void www.tarjaturunen.com 24. Darkness Light - Long Ago 44. Mercutio - Shed Your Skin 63. Sfyrokalymnon - Son of Sin From the album: Living With The Danger From the album: Back To Nowhere From the album: The Sign Of Concrete 3. Grandhour - All In Or Nothing http://darknesslight.de Mercutio.me Creation From the album: Bombs & Bullets www.sfyrokalymnon.com www.grandhourband.com GROUP TWO: 70s RETRO ROCK/ 45. Medusa - Queima PSYCHEDELIC/BLUES/SOUTHERN From the album: Monstrologia (Lado A) 64. Chaosmic - Forever Feast 4.