John Fowles in Focus
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Lunar Impact Crater Identification and Age Estimation with Chang’E
ARTICLE https://doi.org/10.1038/s41467-020-20215-y OPEN Lunar impact crater identification and age estimation with Chang’E data by deep and transfer learning ✉ Chen Yang 1,2 , Haishi Zhao 3, Lorenzo Bruzzone4, Jon Atli Benediktsson 5, Yanchun Liang3, Bin Liu 2, ✉ ✉ Xingguo Zeng 2, Renchu Guan 3 , Chunlai Li 2 & Ziyuan Ouyang1,2 1234567890():,; Impact craters, which can be considered the lunar equivalent of fossils, are the most dominant lunar surface features and record the history of the Solar System. We address the problem of automatic crater detection and age estimation. From initially small numbers of recognized craters and dated craters, i.e., 7895 and 1411, respectively, we progressively identify new craters and estimate their ages with Chang’E data and stratigraphic information by transfer learning using deep neural networks. This results in the identification of 109,956 new craters, which is more than a dozen times greater than the initial number of recognized craters. The formation systems of 18,996 newly detected craters larger than 8 km are esti- mated. Here, a new lunar crater database for the mid- and low-latitude regions of the Moon is derived and distributed to the planetary community together with the related data analysis. 1 College of Earth Sciences, Jilin University, 130061 Changchun, China. 2 Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China. 3 Key Laboratory of Symbol Computation and Knowledge Engineering of Ministry of Education, College of Computer Science and Technology, Jilin University, 130012 Changchun, China. 4 Department of Information Engineering and Computer ✉ Science, University of Trento, I-38122 Trento, Italy. -
On Celestial Wings / Edgar D
Library of Congress Cataloging-in-Publication Data Whitcomb. Edgar D. On Celestial Wings / Edgar D. Whitcomb. p. cm. Includes bibliographical references. 1. United States. Army Air Forces-History-World War, 1939-1945. 2. Flight navigators- United States-Biography. 3. World War, 1939-1945-Campaigns-Pacific Area. 4. World War, 1939-1945-Personal narratives, American. I. Title. D790.W415 1996 940.54’4973-dc20 95-43048 CIP ISBN 1-58566-003-5 First Printing November 1995 Second Printing June 1998 Third Printing December 1999 Fourth Printing May 2000 Fifth Printing August 2001 Disclaimer This publication was produced in the Department of Defense school environment in the interest of academic freedom and the advancement of national defense-related concepts. The views expressed in this publication are those of the author and do not reflect the official policy or position of the Department of Defense or the United States government. This publication has been reviewed by security and policy review authorities and is cleared for public release. Digitize February 2003 from August 2001 Fifth Printing NOTE: Pagination changed. ii This book is dedicated to Charlie Contents Page Disclaimer........................................................................................................................... ii Foreword............................................................................................................................ vi About the author .............................................................................................................. -
Fiction John Fowles, the Collector, Boston: Little, Brown and Company, 1963
BIBLIOGRAPHY WORKS BY JOHN FOWLES Fiction John Fowles, The Collector, Boston: Little, Brown and Company, 1963. —— Daniel Martin, Boston: Little, Brown and Company, 1977. —— The Ebony Tower, Boston: Little, Brown and Company, 1974. —— The French Lieutenant’s Woman, Boston: Little, Brown and Company, 1969. —— A Maggot, Boston: Little, Brown and Company, 1985. —— The Magus, New York: Dell Publishing, 1978. —— Mantissa, Boston: Little, Brown and Company, 1982. Nonfiction John Fowles, The Aristos, Boston: Little, Brown and Company, 1964. —— The Enigma of Stonehenge, New York: Summit Books, 1980. —— Foreword, in Ourika, by Claire de Duras, trans. John Fowles, New York: MLA, 1994, xxix-xxx. —— Islands, Boston: Little, Brown and Company, 1978. —— Lyme Regis Camera, Boston: Little, Brown and Company, 1990. —— Shipwreck, Boston: Little, Brown and Company, 1975. —— A Short History of Lyme Regis, Boston: Little, Brown and Company, 1982. —— Thomas Hardy’s England, Boston: Little, Brown and Company, 1984. —— The Tree, New York: The Ecco Press, 1979. Translations Claire de Duras, Ourika, trans. John Fowles, New York: MLA, 1994. 238 John Fowles: Visionary and Voyeur Essays John Fowles, “Gather Ye Starlets”, in Wormholes, ed. Jan Relf, New York: Henry Holt and Company, 1998, 89-99. —— “I Write Therefore I Am”, in Wormholes, ed. Jan Relf, New York: Henry Holt and Company, 1998, 5-12. —— “The J.R. Fowles Club”, in Wormholes, ed. Jan Relf, New York: Henry Holt and Company, 1998, 67. —— “John Aubrey and the Genesis of the Monumenta Britannica”, in Wormholes, ed. Jan Relf, New York: Henry Holt and Company, 1998, 175-96. —— “The John Fowles Symposium, Lyme Regis, July 1996”, in Wormholes, ed. -
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. -
Film Film Film Film
Annette Michelson’s contribution to art and film criticism over the last three decades has been un- paralleled. This volume honors Michelson’s unique C AMERA OBSCURA, CAMERA LUCIDA ALLEN AND TURVEY [EDS.] LUCIDA CAMERA OBSCURA, AMERA legacy with original essays by some of the many film FILM FILM scholars influenced by her work. Some continue her efforts to develop historical and theoretical frame- CULTURE CULTURE works for understanding modernist art, while others IN TRANSITION IN TRANSITION practice her form of interdisciplinary scholarship in relation to avant-garde and modernist film. The intro- duction investigates and evaluates Michelson’s work itself. All in some way pay homage to her extraordi- nary contribution and demonstrate its continued cen- trality to the field of art and film criticism. Richard Allen is Associ- ate Professor of Cinema Studies at New York Uni- versity. Malcolm Turvey teaches Film History at Sarah Lawrence College. They recently collaborated in editing Wittgenstein, Theory and the Arts (Lon- don: Routledge, 2001). CAMERA OBSCURA CAMERA LUCIDA ISBN 90-5356-494-2 Essays in Honor of Annette Michelson EDITED BY RICHARD ALLEN 9 789053 564943 MALCOLM TURVEY Amsterdam University Press Amsterdam University Press WWW.AUP.NL Camera Obscura, Camera Lucida Camera Obscura, Camera Lucida: Essays in Honor of Annette Michelson Edited by Richard Allen and Malcolm Turvey Amsterdam University Press Front cover illustration: 2001: A Space Odyssey. Courtesy of Photofest Cover design: Kok Korpershoek, Amsterdam Lay-out: japes, Amsterdam isbn 90 5356 494 2 (paperback) nur 652 © Amsterdam University Press, Amsterdam, 2003 All rights reserved. Without limiting the rights under copyright reserved above, no part of this book may be reproduced, stored in or introduced into a retrieval system, or transmitted, in any form or by any means (electronic, me- chanical, photocopying, recording or otherwise) without the written permis- sion of both the copyright owner and the author of the book. -
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. -
Secondary Craters on Europa and Implications for Cratered Surfaces
Vol 437|20 October 2005|doi:10.1038/nature04069 LETTERS Secondary craters on Europa and implications for cratered surfaces Edward B. Bierhaus1, Clark R. Chapman2 & William J. Merline2 For several decades, most planetary researchers have regarded the craters were typically not spatially random, but instead appeared in impact crater populations on solid-surfaced planets and smaller clumps and clusters16 even at distances far (several hundred kilo- bodies as predominantly reflecting the direct (‘primary’) impacts metres) from the nearest large primary crater. This clustered spatial of asteroids and comets1. Estimates of the relative and absolute distribution contrasts with primary impacts, which are spatially ages of geological units on these objects have been based on this random. The low spatial density and unusual non-random spatial assumption2. Here we present an analysis of the comparatively distribution of Europa’s small craters enabled us to achieve what has sparse crater population on Jupiter’s icy moon Europa and suggest been previously difficult, namely unambiguous identification and that this assumption is incorrect for small craters. We find that quantification of the contribution of distant secondary craters to the ‘secondaries’ (craters formed by material ejected from large total crater SFD. This, in turn, allows us to re-examine the overall primary impact craters) comprise about 95 per cent of the small crater age-dating methodology. We discuss the specifics of the craters (diameters less than 1 km) on Europa. We therefore con- Europa data first. clude that large primary impacts into a solid surface (for example, We measured more than 17,000 craters in 87 low-compression, ice or rock) produce far more secondaries than previously low-sun, high-resolution Europa images (scales ,60 m pixel21), believed, implying that the small crater populations on the which cover nine regions totalling 0.2% of Europa’s surface (a much Moon, Mars and other large bodies must be dominated by larger percentage of Europa has been imaged at lower resolutions), secondaries. -
Annual Report 2008 – 2009
O L D S T U R B R I D G E Summer 2009 Special Annual VILLAGE Report Edition Visitor 2008-2009 2008--2009 Momentum and More The History of Fireworks Farms, Families, and Change Cooking with OSV Summer Events a member magazine that keeps you coming back Old Sturbridge Village, a museum and learning resource of 2008-2009 Building Momentum New England life, invites each visitor to find meaning, pleasure, a letter from President Jim Donahue relevance, and inspiration through the exploration of history. to our newly designed V I S I T O R magazine. We hope that you will learn new things and come to visit t is no secret around the Village that I like to keep my eye on the “dashboard” – a set of key the Village soon. There is always something fun to do at indicators that I am consistently checking to make sure we are steering OSV in the right direction. In fact, Welcome O l d S T u R b ri d g E V I l l a g E . I take a lot of good-natured kidding about how often I peek at the attendance figures each day, eager to see if we beat last year’s number. And I have to admit that I get energized when the daily mail brings in new donations, when the sun is shining, the parking lot is full, when I can hear happy children touring the Village, and the visitor comments are upbeat and favorable. Volume XlIX, No. 2 Summer 2009 Special Annual Report Edition I am happy to report these indicators have been overwhelmingly positive during the past year – solid proof that Old Sturbridge Village is building on last year’s successes and is poised to finish this decade much stronger There is nothing quite like learning about history from than when it started. -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
A Critical Study of the Novels of John Fowles
University of New Hampshire University of New Hampshire Scholars' Repository Doctoral Dissertations Student Scholarship Spring 1986 A CRITICAL STUDY OF THE NOVELS OF JOHN FOWLES KATHERINE M. TARBOX University of New Hampshire, Durham Follow this and additional works at: https://scholars.unh.edu/dissertation Recommended Citation TARBOX, KATHERINE M., "A CRITICAL STUDY OF THE NOVELS OF JOHN FOWLES" (1986). Doctoral Dissertations. 1486. https://scholars.unh.edu/dissertation/1486 This Dissertation is brought to you for free and open access by the Student Scholarship at University of New Hampshire Scholars' Repository. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of University of New Hampshire Scholars' Repository. For more information, please contact [email protected]. A CRITICAL STUDY OF THE NOVELS OF JOHN FOWLES BY KATHERINE M. TARBOX B.A., Bloomfield College, 1972 M.A., State University of New York at Binghamton, 1976 DISSERTATION Submitted to the University of New Hampshire in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in English May, 1986 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. This dissertation has been examined and approved. .a JL. Dissertation director, Carl Dawson Professor of English Michael DePorte, Professor of English Patroclnio Schwelckart, Professor of English Paul Brockelman, Professor of Philosophy Mara Wltzllng, of Art History Dd Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. I ALL RIGHTS RESERVED c. 1986 Katherine M. Tarbox Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. to the memory of my brother, Byron Milliken and to JT, my magus IV Reproduced with permission of the copyright owner.