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Chronicle 2004
The Annual Magazine of King Edward's School, Birmingham CHRONICLE 2004 CONTENTS Hellos 5 Goodbyes 16 Features 22 Dram a 38 Trips 43 Words and Pictures 62 Music 76 Houses 80 Societies 86 Sport 90 K€S Chronicle 2004 The Editorial Team Hellos & Goodbyes Matthew Gammie Features Matthew Hosty Trips Euan Stirling & Oliver Carter Drama Peter Wozniak Music Tom Cadigan Words Charles Butler Houses Amit Sinha Societies Jamie Sunderland Sport Philip Satterthwaite, Amer Shafi, & Vidu Shanmugarajah Cover Elliot Weaver Banners Tarsem Madhar Staff Tom Hosty Editorial Chronicle is the work of a large number of people. Most immediately we have to thank Sandra Bürden at the Resources Centre, who assembles the pages on her computer and who is to thank for much of the fine detail of the magazine's final appearance: I am hugely indebted to her for her energy, initiative and attention to detail. Earlier in the chain stand the section editors, whose job is to round up copy and pictures for their sections and devise the running order and general page layouts for that section. They also have to go in for a good deal of rewriting: prolixity must be trimmed, irrelevance eliminated, errors put right and facetiousness filtered out. To be a good editor requires not only a good ear for language and a high level of compétence in written English: it also calls for patience and good humour in the actual pursuit of material. Mirabile dictu, it sometimes happens that contributors to the magazine are strong on promises but weak on performance. This year's editors have been terrifie. -
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. -
No. 40. the System of Lunar Craters, Quadrant Ii Alice P
NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates. -
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. -
University Microfilms International T U T T L E , V Ir G in Ia G R a C E
INFORMATION TO USERS This was produced from a copy of a document sent to us for microfilming. While the most advanced technological means to photograph and reproduce this document have been used, the quality is heavily dependent upon the quality of the material subm itted. The following explanation of techniques is provided to help you understand markings or notations which may appear on this reproduction. 1. The sign or “target” for pages apparently lacking from the document photographed is “Missing Page(s)”. If it was possible to obtain the missing page(s) or section, they are spliced into the film along with adjacent pages. This may have necessitated cutting through an image and duplicating adjacent pages to assure you of complete continuity. 2. When an image on the film is obliterated with a round black mark it is an indication that the film inspector noticed either blurred copy because of movement during exposure, or duplicate copy. Unless we meant to delete copyrighted materials that should not have been filmed, you will find a good image of the page in the adjacent frame. 3. When a map, drawing or chart, etc., is part of the material being photo graphed the photographer has followed a definite method in “sectioning” the material. It is customary to begin filming at the upper left hand corner of a large sheet and to continue from left to right in equal sections with small overlaps. If necessary, sectioning is continued again-beginning below the first row and continuing on until complete. 4. For any illustrations that cannot be reproduced satisfactorily by xerography, photographic prints can be purchased at additional cost and tipped into your xerographic copy. -
General Disclaimer One Or More of the Following Statements May Affect
https://ntrs.nasa.gov/search.jsp?R=19710025504 2020-03-11T22:36:49+00:00Z View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NASA Technical Reports Server General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) 6 X t B ICC"m date: July 16, 1971 955 L'Enfant Plaza North, S. W Washington, D. C. 20024 to Distribution B71 07023 from. J. W. Head suhiecf Derivation of Topographic Feature Names in the Apollo 15 Landing Region - Case 340 ABSTRACT The topographic features in the region of the Apollo 15 landing site (Figure 1) are named for a number of philosophers, explorers and scientists (astronomers in particular) representing periods throughout recorded history. It is of particular interest that several of the individuals were responsible for specific discoveries, observations, or inventions which considerably advanced the study and under- standing of the moon (for instance, Hadley designed the first large reflecting telescope; Beer published classic maps and explanations of the moon's surface). -
Table of Exposures
Table of Exposures Dole UT Focal Emulsion Exposure Moon's age Plate Nos. ralio sec. days 08.11.65 2132· f/29 Kodak 0.250 Plole 0.4 15.3 7e/2 08.01.66 2228 f/24 Kodak 0.250 Plate 0.31 17.0 3b, 15e 31.01.66 1947 1/24 Kodak 0.250 Plale 0.3 10.1 5b 02.02.66 1944 f/24 Kodak 0.250 Plote 0.25 12.1 7b, 8b 06.02.66 2326 1/24 Kodak 0.250 Plole 0.2 16.3 14c,16b 05.03.66 2259 1/41 IIford Zenith Plole 0.1 13 .5 lOe/l 27.04.66 2152 1/24 lIford G.30 Plate 0.5 6.9 150 28.04.66 2046 f/30 lIford G.30 Pia Ie 0.8 7.9 10,130 23.05.66 2033 f/24 Kodak 0.250 Plole 0.7 3.4 15e/2 23.05,66 2034 f/24 Kodak 0.250 Plate 0.7 3.4 3e/2,4b 23.05.66 2036 1/24 Kodak 0.250 Plate 0.7 3.4 16e 28.05.66 2122 1/30 IIford G.30 Plole 0.8 8.4 140 29.05.66 2103 1/30 IIford G.30 Plate 0.8 9.4 2e 23.06.66 2109 f/24 lIford G.30 Pia Ie 1.0 5.0 160 06.08.66 0211 f/30 Illord G.30 Pia Ie 0.7 18.9 2b 06.08.66 0215 1/30 IIford G.30 Plale 0.7 18.9 lb, 13b 09.08.66 0315 1/30 IIlord G.30 Plate 1.1 23.8 50,60 09.08.66 03 17 1/30 Ilford G.30 Plate 1.1 23.8 90, 91/2, 11 b, 12e/l 06. -
Planetary Science : a Lunar Perspective
APPENDICES APPENDIX I Reference Abbreviations AJS: American Journal of Science Ancient Sun: The Ancient Sun: Fossil Record in the Earth, Moon and Meteorites (Eds. R. 0.Pepin, et al.), Pergamon Press (1980) Geochim. Cosmochim. Acta Suppl. 13 Ap. J.: Astrophysical Journal Apollo 15: The Apollo 1.5 Lunar Samples, Lunar Science Insti- tute, Houston, Texas (1972) Apollo 16 Workshop: Workshop on Apollo 16, LPI Technical Report 81- 01, Lunar and Planetary Institute, Houston (1981) Basaltic Volcanism: Basaltic Volcanism on the Terrestrial Planets, Per- gamon Press (1981) Bull. GSA: Bulletin of the Geological Society of America EOS: EOS, Transactions of the American Geophysical Union EPSL: Earth and Planetary Science Letters GCA: Geochimica et Cosmochimica Acta GRL: Geophysical Research Letters Impact Cratering: Impact and Explosion Cratering (Eds. D. J. Roddy, et al.), 1301 pp., Pergamon Press (1977) JGR: Journal of Geophysical Research LS 111: Lunar Science III (Lunar Science Institute) see extended abstract of Lunar Science Conferences Appendix I1 LS IV: Lunar Science IV (Lunar Science Institute) LS V: Lunar Science V (Lunar Science Institute) LS VI: Lunar Science VI (Lunar Science Institute) LS VII: Lunar Science VII (Lunar Science Institute) LS VIII: Lunar Science VIII (Lunar Science Institute LPS IX: Lunar and Planetary Science IX (Lunar and Plane- tary Institute LPS X: Lunar and Planetary Science X (Lunar and Plane- tary Institute) LPS XI: Lunar and Planetary Science XI (Lunar and Plane- tary Institute) LPS XII: Lunar and Planetary Science XII (Lunar and Planetary Institute) 444 Appendix I Lunar Highlands Crust: Proceedings of the Conference in the Lunar High- lands Crust, 505 pp., Pergamon Press (1980) Geo- chim. -
0 Lunar and Planetary Institute Provided by the NASA Astrophysics Data System LAVA FLOODING of EARLY PLANETARY CRUSTS
LAVA FLOODING OF EARLY PLANETARY CRUSTS: GEOMETRY, THICKNESS, AND VOLUMES CF FLOODED LUNAR HIGHLAND TERRA IN. James W. Head, Dept. of Geol og ica I Sciences, Brown Univ., Providence, RI 02912. Recognition of the volcanic origin of surface deposits on ancient cra- tered planetary surfaces provides important information on the presence and significance of melting in the interior. Establishment of the composition, age, and volume of such deposits provides additional clues concerning the characteristics of the thermal history of the planet.' In addition, the Thickness, geometry, and volumes of volcanic deposits provide important data for understanding tectonics and I i thospheric deformation. Once deposits have been recognized as of volcanic origin, it has often been difficult to estab- , . , I sh thicknesses and volumes because in the processes of emp lacement, l avas cover the initial crustal surface, obscuring the geometry of the pre-volcanic terrain. In addition to geophysical analyses, attempts to establish thick- nesses and volumes have concentrated on four approaches: I ) measuring diam- eters and sxposed rim heights of impact craters protruding through the depos- i TS; ' 2 l @cati ng craters in vo l can ic deposits that have excavated sub-vo l- can i c material ;" 3) using stratigraphic techniques; 7 and 4) using the geom- etry of co~parableunflooded regions as models for the initial topography. 2 P<lihouyh these approaches have provided significant advances in the under- stand ing of the emp lacement of the l unar maria,' there are sti l l basic uncer- ta inties concerning thicknesses and vol umes in many areas. -
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, -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base.