Technology Today Spring 2013

Total Page:16

File Type:pdf, Size:1020Kb

Technology Today Spring 2013 Spring 2013 TECHNOLOGY® today Southwest Research Institute® San Antonio, Texas Spring 2013 • Volume 34, No.2 TECHNOLOGY today COVER Director of Communications Craig Witherow Editor Joe Fohn TECHNOLOGY Assistant Editor today Deborah Deffenbaugh Editorial Assistant Kasey Chenault Design Scott Funk Photography Larry Walther Illustrations Andrew Blanchard Southwest Research Institute San Antonio, Texas D019022 About the cover Exposed rock strata can reveal folds, faults and other Technology Today (ISSN 1528-431X) is published three times deformation features that also exist deep underground in the each year and distributed free of charge. The publication same formation and may have significance for the performance discusses some of the more than 1,000 research and develop- of oil and gas reservoirs. ment projects under way at Southwest Research Institute. The materials in Technology Today may be used for educational and informational purposes by the public and the media. Credit to Southwest Research Institute should be given. This authorization does not extend to property rights such as patents. Commercial and promotional use of the contents in Technology Today without the express written consent of Southwest Research Institute is prohibited. The information published in Technology Today does not necessarily reflect the position or policy of Southwest Research Institute or its clients, and no endorsements should be made or inferred. Address correspondence to the editor, Department of Communications, Southwest Research Institute, P.O. Drawer 28510, San Antonio, Texas 78228-0510, or e-mail [email protected]. To be placed on the mailing list or to make address changes, call (210) 522-2257 or fax (210) 522-3547, or visit update.swri.org. © 2013 Southwest Research Institute. All rights reserved. Technology Today, Southwest Research Institute and SwRI are registered marks in the U.S. Patent and Trademark Office. About the Institute Since its founding in 1947, Southwest Research Institute (SwRI) has contributed to the advancement of science and technology by working with clients in industry and government. Per forming research for the benefit of humankind is a long-held tradition. The Institute comprises 11 divisions engaged in contract research spanning a wide range of technologies. Southwest Research Institute on the Internet: swri.org CONTENTS ARTICLES 2 Stress Management Structural geology and geomechanics are applied to energy exploration and production. 6 A Good Scout An SwRI-developed tool enables signal analysts to scan an area’s radio spectrum and locate signal sources. 10 A Dazzling Development in Security An SwRI-developed technology fends off intruders using an eye-safe laser. 14 A Moon-shot in the Dark An SwRI-developed instrument observes mercury, other chemicals in the plumes of intentional lunar impacts by two spacecraft. Departments Technics….15 Technical Staff Activities….17 Recent Features….25 Stress Management Structural geology and geomechanics are applied to energy exploration and production D019018 Rock strata often are non-uniform and may contain folds, faults and other deformation. Faults too small to observe using traditional seismic technology, such as those marked in red in the bottom inset photo, nevertheless may be important to the formation and performance of oil and gas reservoirs. A significant percentage of total faulting may be below the detection limit, as shown in the graph in the top inset. By David A. Ferrill, Ph.D., Alan P. Morris, Ph.D., Kevin J. Smart, Ph.D. and Ronald N. McGinnis fter more than 150 years of oil deformation. To be and gas production following successful in these the first successful oil well in increasingly challenging D019015 Pennsylvania in 1859, most of exploration and produc- Athe easy-to-produce oil and gas reser- tion environments, voirs have already been found. New petroleum geologists hydrocarbon discoveries tend to be more need higher resolution structurally complex and located in tools, but perhaps more tighter rock, at greater depths or in important, they need deeper water. Finding these harder-to- sophisticated training reach resources, and then producing from to aid interpreters as them, calls for ever-increasing expertise they analyze the data in characterizing and understanding the generated by the improved hardware predicting stress changes resulting from influences of geologic structures on the and software tools. A team of geologists production activities such as hydraulic deposition and deformation of reservoir, from Southwest Research Institute fracturing and pressure declines; and seal, and source strata. (SwRI) has developed approaches to performing geomechanical analyses using Over the years, new and more sensi- aid oil and gas exploration and improve physical analog and numerical modeling tive seismic technologies have been the prospects for successful production techniques. developed to reveal formerly unrecog- from unconventional reservoirs. Stress and geomechanical analyses nized subsurface geologic structures. In The process involves collecting allow geologists to leverage limited many cases, however, the products of data to characterize the natural defor- static data and thus track dynamic stress geologic deformation which occur as mation, rock mechanical properties and deformation over time. The time faults, folds and fractures are still below and stress environments; studying scales range from geologically instan- the detection limits of 3-D seismic outcrops to characterize reservoir taneous seismic deformation caused reflection data, thus requiring a geolo- rocks or their analogs; analyzing stress by earthquakes or induced hydraulic gist to predict or infer subseismic-scale fields, both past and present, and fracturing, to longer-term production 2 Technology Today • Spring 2013 Dr. David A. Ferrill is director of the Earth, Material and Planetary Sciences Department. He is a structural geologist with international research experience in various tectonic regimes and oil and gas exploration. Dr. Alan P. Morris, a staff scientist, is a structural geologist with expertise in quantitative analysis of rock deformation. Dr. Kevin J. Smart, a principal scientist, is a structural geologist with cross-training in computational solid mechanics. Ronald N. McGinnis, a senior research scientist, is a structural geologist with expertise in characterizing mechanical stratigraphy and the control it has on deformation. All are with the Earth, Material and Planetary Sciences Department of the Geosciences and Engineering Division at Southwest Research Institute. (field lifetime) scales, and ultimately to reservoirs takes advantage of in situ stress buried beneath the earth’s surface, direct geologic time scales. and fluid pressure conditions to reactivate analogs of the rock types and structural natural fractures and induce new fractures features (folds, faults and fractures) can The basics of reservoir analysis to create or enhance fracture permeability. be observed first-hand somewhere at the In contrast, declining fluid pressures over earth’s surface. In the spirit of H.H. Read’s Geologic structure, stress and fluid a reservoir’s productive lifetime can cause observation that the best geologists are pressure conditions, and geomechanical naturally permeable faults and fractures the ones who have seen the most rocks, behavior of rock are key elements in to close or lose their permeability, thus it is essential to develop an understand- determining trap, reservoir and charge reducing overall reservoir permeability or ing of reservoir behavior by observing in hydrocarbon systems. Conventional compartmentalizing the reservoir. and analyzing rocks in the field. To this hydrocarbon traps are commonly formed In many cases, hydrocarbon genera- end, geologists inform their models by by geologic structures such as domes, tion and migration into a reservoir studying the closest field analogs to the anticlines, and sealing faults. Fracture depends on stress conditions, geomecha- reservoir rocks they wish to understand. and fault systems can also compromise nical properties of rock, deformation trap integrity and may be difficult or processes, and geologic structure. These Modeling applications impossible to detect. So-called uncon- conditions commonly combine to provide ventional resource plays, where the pathways for migration of hydrocarbons Geomechanics is the application of source and reservoir rock are the same, from the site of source rock matura- mechanical (or rock mechanical) princi- are becoming increasingly important in tion, sometimes called the “kitchen.” In ples to geologic problems. Although hydrocarbon exploration and production. unconventional reservoirs, the kitchen is geomechanical modeling often invokes These unconventional plays are typically also the reservoir, and conditions that are the idea of computer-based analysis, dependent on induced fracturing favorable for migration are detrimental to the structural geology community has a (“fracking”) for their economic viability, the richness of the reservoir because they well-established record of using physical and therefore the presence or absence of allow some hydrocarbons to escape. analog as well as numerical modeling natural faults and fractures, the ambient Although, with virtually no significant techniques to understand structural stress state, and the mechanical charac- exceptions, oil and gas reservoirs are geology and geomechanics problems. teristics of the reservoir rocks are critical factors
Recommended publications
  • NOAO Newsletter #104
    NOAO Newsletter NATIONAL OPTICAL ASTRONOMY OBSERVATORY ISSUE 104 — SEPTEMBER 2011 Science Highlights Finding Hidden Supermassive Black Holes in Distant Galaxies ........ 2 Gemini, MMT, and Hale ............................................................ 22 Star Formation Rises with Time in UV-Bright Galaxies CTIO Instruments Available for 2012A ......................................... 24 over the First Two Billion Years.................................................... 4 Gemini Instruments Available for 2012A* ................................... 25 Gemini/GMOS—Spectroscopy of a Large Sample KPNO Instruments Available for 2012A........................................ 26 of Strong Lensing Selected Galaxy Clusters ................................. 5 MMT Instruments Available for 2012A ......................................... 27 Late-Time Light Curves of Type II Supernovae: Hale Instruments Available for 2012A ......................................... 27 Physical Properties of SNe and Their Environment ....................... 7 CHARA Instruments Available for 2012 ........................................ 27 Changes Made to the ORP ........................................................... 27 System Science Capabilities Participating in the SMARTS Consortium ..................................... 28 NOAO at the Science Frontiers of the 2010 Decadal Survey ........... 10 After Twelve Years of Mosaic II… ................................................ 28 Dr. Timothy Beers to Become Associate Director for KPNO ............ 11 Phoenix Returning
    [Show full text]
  • 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
    [Show full text]
  • Geologic Studies of Planetary Surfaces Using Radar Polarimetric Imaging 2
    Geologic studies of planetary surfaces using radar polarimetric imaging 2 4 Lynn M. Carter NASA Goddard Space Flight Center 8 Donald B. Campbell 9 Cornell University 10 11 Bruce A. Campbell 12 Smithsonian Institution 13 14 14 Abstract: Radar is a useful remote sensing tool for studying planetary geology because it is 15 sensitive to the composition, structure, and roughness of the surface and can penetrate some 16 materials to reveal buried terrain. The Arecibo Observatory radar system transmits a single 17 sense of circular polarization, and both senses of circular polarization are received, which allows 18 for the construction of the Stokes polarization vector. From the Stokes vector, daughter products 19 such as the circular polarization ratio, the degree of linear polarization, and linear polarization 20 angle are obtained. Recent polarimetric imaging using Arecibo has included Venus and the 21 Moon. These observations can be compared to radar data for terrestrial surfaces to better 22 understand surface physical properties and regional geologic evolution. For example, 23 polarimetric radar studies of volcanic settings on Venus, the Moon and Earth display some 24 similarities, but also illustrate a variety of different emplacement and erosion mechanisms. 25 Polarimetric radar data provides important information about surface properties beyond what can 26 be obtained from single-polarization radar. Future observations using polarimetric synthetic 27 aperture radar will provide information on roughness, composition and stratigraphy that will 28 support a broader interpretation of surface evolution. 29 2 29 1.0 Introduction 30 31 Radar polarimetry has the potential to provide more information about surface physical 32 properties than single-polarization backscatter measurements, and has often been used in remote 33 sensing observations of Solar System objects.
    [Show full text]
  • Technology Today Spring 2016
    Spring 2016 HIDDEN STRUCTURES REVEALED THE METHANE SwRI WINS CYGNSS DETECTORS R&D 100 CONSTELLATION 10 CHALLENGE 18AWARDS 22TECHNOLOGYCOMPLETE TODAY 13 AVIATION FUEL TESTING To meet the needs of the Department of Defense, the Energy Institute, and the aviation industry, SwRI maintains facilities to qualify fuel filters, develop new test methods, and enhance aviation fuel technology. The coalescer-separator shown removes dirt and water contaminants from fuel in both commercial and military fuel handling systems. SwRI works with industry organizations to develop and improve quality standards. The Institute also helps industry develop advanced sensing technologies and fuel handling equipment. AVIATION FUEL FILTRATION AVIATION FUEL MONITORS AVIATION FUEL COALESCERS AVIATION FUEL ADDITIVES WATER MAPPING TEST JET FUEL ELECTRONIC SENSOR MIL PRF 52308J ELECTRONIC SENSORS aviationturbinefuels.swri.org DM018200_6585 12 SPRING 2016 • VOLUME 37, NO. 1 Executive Director of Communications ON THE COVER Tim Martin, Ph.D. Editor 2 Hidden Structures Revealed Deb Schmid Flight control surfaces include the flaps, tabs, Assistant Editor and spoilers that allow a pilot to adjust and Rob Leibold control an aircraft’s flight attitude. Using the Contributors Institute’s recently aquired powerful CT Barbara Bowen scanner, SwRI engineers imaged the aluminum Robert Crowe honeycomb control surface to visualize its Deborah Deffenbaugh D021911 internal structure. This 3-D visualization shows Maria Stothoff a bonding layer running through the structure. Design 8 New Horizons News Jessica Vidal Photography 10 The Methane Detectors Challenge Larry Walther Ian McKinney 14 Consortia News Circulation Stephanie Paredes 16 Pluto-Jupiter Infographic 18 SwRI Wins R&D 100 Awards Technology Today (ISSN 1528-431X) is published 19 TechBytes three times each year and distributed free of charge.
    [Show full text]
  • NOAO Newsletter #101
    NOAO/NSO Newsletter NATIONAL OPTICAL ASTRONOMY OBSERVATORY/NATIONAL SOLAR OBSERVATORY Issue 101 — March 2010 Science Highlights CTIO Instruments Available for 2010B ......................................... 22 Kitt Peak Observations Provide Solid Ground for Kepler ................. 2 Gemini Instruments Expected to be Available for 2010B .............. 23 Early Results from the NEWFIRM Medium-Band Survey ................. 3 Keck Instruments Available for 2010B ......................................... 24 The NOAO Outer Limits Survey: Stellar Populations in the MMT Instruments Available for 2010B ......................................... 24 Extremities of the Magellanic Clouds ......................................... 4 Magellan Instruments Available for 2010B .................................. 24 Evidence that Temporal Changes in Solar Subsurface Hale Instruments Available for 2010B ......................................... 24 Helicity Precede Active Region Flaring ....................................... 6 New NOAO Survey Programs Selected ......................................... 25 McMath-Pierce Observations of the Lunar Impact Third Quarter 2010 NSO Proposal Deadline .................................. 25 Plume from the LCROSS Mission ................................................. 8 NOAO Operations & Staff System Science Capabilities Director’s News .......................................................................... 26 Creating a Roadmap for the Ground-Based O/IR System............... 10 Ongoing Celebrations of Our 50th Anniversary
    [Show full text]
  • Fungos Presentes Em Sedimentos Marinhos E Lacustres Da Antártica: Taxonomia, Diversidade E Bioprospecção De Metabólitos Bioativos
    Universidade Federal de Minas Gerais Programa de Pós-Graduação em Microbiologia Fungos presentes em sedimentos marinhos e lacustres da Antártica: taxonomia, diversidade e bioprospecção de metabólitos bioativos Mayara Baptistucci Ogaki Belo Horizonte, MG 2019 Universidade Federal de Minas Gerais Programa de Pós-Graduação em Microbiologia Fungos presentes em sedimentos marinhos e lacustres da Antártica: taxonomia, diversidade e bioprospecção de metabólitos bioativos Tese apresentada ao programa de Pós-Graduação em Microbiologia do Instituto de Ciências Biológicas da Universidade Federal de Minas Gerais. Orientador: Dr. Luiz Henrique Rosa Departamento de Microbiologia/ICB, UFMG Belo Horizonte, MG 2019 Colaboradores: Dr. Carlos Augusto Rosa Departamento de Microbiologia/ICB, UFMG Dr. Carlos Leomar Zani Dra. Tânia Maria de Almeida Alves Centro de Pesquisas René Rachou, FIOCRUZ/MG Dra. Rosemary Vieira Dr. Arthur Ayres Universidade Federal Fluminense, RJ Dr. Juan Manoel Lírio Instituto Antartico Argentino, Buenos Aires, Argentina 043 Ogaki, Mayara Baptistucci. Fungos presentes em sedimentos marinhos e lacustres da Antártica: taxonomia, diversidade e bioprospecção de metabólitos bioativos [manuscrito] / Mayara Baptistucci Ogaki. – 2019. 212 f. : il. ; 29,5 cm. Orientador: Dr. Luiz Henrique Rosa. Tese (doutorado) – Universidade Federal de Minas Gerais, Instituto de Ciências Biológicas. Programa de Pós-Graduação em Microbiologia. 1. Microbiologia. 2. Regiões Antárticas. 3. Fungos. 4. Bioprospecção. 5. Biodiversidade. I. Rosa, Luiz Henrique. II. Universidade Federal de Minas Gerais. Instituto de Ciências Biológicas. III. Título. CDU: 579 Ficha Catalográfica elaborada por Fabiane C. M. Reis – CRB6/ 2680 Dedicatória Aos meus maiores apoios, “minha família e amigos”. Agradecimentos Agradeço a todo corpo docente e funcionários do programa de pós-graduação em Microbiologia e ao apoio financeiro do CNPq e CAPES pela concessão de minha bolsa de estudos e pelos subsídios que permitiram a concretização desta tese.
    [Show full text]
  • Swri Internal Research and Development 2017
    Internal Research and Development 2017 The SwRI IR&D Program exists to broaden the Institute's technology base and to encourage staff professional growth. Internal funding of research enables the Institute to advance knowledge, increase its technical capabilities, and expand its reputation as a leader in science and technology. The program also allows Institute engineers and scientists to continually grow in their technical fields by providing freedom to explore innovative and unproven concepts without contractual restrictions and expectations. Space Science Materials Research & Structural Mechanics Intelligent Systems, Advanced Computer & Electronic Technology, & Automation Measurement & Nondestructive Evaluation of Materials & Structures Engines, Fuels, Lubricants, & Vehicle Systems Geology & Nuclear Waste Management Fluid & Machinery Dynamics Electronic Systems & Instrumentation Chemistry & Chemical Engineering Copyright© 2017 by Southwest Research Institute. All rights reserved under U.S. Copyright Law and International Conventions. No part of this publication may be reproduced in any form or by any means, electronic or mechanical, including photocopying, without permission in writing from the publisher. All inquiries should be addressed to Communications Department, Southwest Research Institute, P.O. Drawer 28510, San Antonio, Texas 78228-0510, [email protected], fax (210) 522-3547. 2017 IR&D | IR&D Home SwRI IR&D 2017 – Space Science Augmenting a Novel Magnetohydrodynamics Code for Studying Astrophysical Plasmas and Space Weather,
    [Show full text]
  • Swri IR&D Program 2013
    Internal Research and Development 2013 The SwRI IR&D Program exists to broaden the Institute's technology base and to encourage staff professional growth. Internal funding of research enables the Institute to advance knowledge, increase its technical capabilities, and expand its reputation as a leader in science and technology. The program also allows Institute engineers and scientists to continually grow in their technical fields by providing freedom to explore innovative and unproven concepts without contractual restrictions and expectations. Space Science Materials Research & Structural Mechanics Intelligent Systems, Advanced Computer & Electronic Technology, & Automation Measurement & Nondestructive Evaluation of Materials & Structures Engines, Fuels, Lubricants, & Vehicle Systems Geology & Nuclear Waste Management Fluid & Machinery Dynamics Electronic Systems & Instrumentation Chemistry & Chemical Engineering Copyright© 2014 by Southwest Research Institute. All rights reserved under U.S. Copyright Law and International Conventions. No part of this publication may be reproduced in any form or by any means, electronic or mechanical, including photocopying, without permission in writing from the publisher. All inquiries should be addressed to Communications Department, Southwest Research Institute, P.O. Drawer 28510, San Antonio, Texas 78228-0510, [email protected], fax (210) 522 -3547. 2013 IR&D | IR&D Home SwRI IR&D 2013 – Space Science Capability Development and Demonstration for Next-Generation Suborbital Research, 15-R8115 Development
    [Show full text]
  • 19680012850.Pdf
    Research in Space Science SA0 Special Report No. 268 AN ANALYSIS OF THE MARINER 4 PHOTOGRAPHY OF MARS Clark R. Chapman, James €3. Pollack, and Carl Sagan February 14, 1968 % Smithsonian Institution A s tr o phy s ica1 Ob s e rvat ory Cambridge, Massachusetts 02138 708-1 1 TABLE OF CONTENTS Section Page ABSTRACT...... ........................... vi INTRODUCTION ............................. 1 A NEW REDUCTION OF THE CRATERING STATISTICS. 3 CRATER EROSION AND OBLITERATION . 17 SOURCES OF IMPACT CRATERS. 23 5 MAJOR TOPOGRAPHICAL FEATURES AS POSSIBLE CRATERS.................................. 33 6 EROSION MECHANISMS . 35 7 CRATERS AS SOURCES OF DUS-T . 51 8 CRATERAGES .............................. 53 9 VARIATION OF CRATER DENSITIES WITH POSITION ONMARS.. ................................ 55 10 RECOMMENDATIONS FOR FUTURE WORK. 59 11 ACKNOWLEDGMENTS . 61 REFERENCES ............................... 62 APPENDIXA ............................... ~-1 APPENDIXB ............................... B-1 BIOGRAPHICAL NOTES . LIST OF ILLUSTRATIONS Figure Page 1 Low-quality reproduction of Picture 4 of the Mariner 4 photographic sequence. 5 2 Sketch of the position of cataloged craters (Appendices A and B), Picture 4 of the Mariner 4 photographic sequence. 6 3 Low-quality reproduction of Picture 7 of the Mariner 4 photographic sequence. 7 4 Sketch of the position of cataloged craters (Appendices A and B), Picture 7 of the Mariner 4 photographic sequence. 8 5 Low-quality reproduction of Picture 11 of the Mariner 4 photographic sequence. 9 6 Sketch of the position of cataloged craters (Appendices A and B), Picture 11 of the Mariner 4 photographic sequence. 10 7 Diameter-frequency plot for Pictures 7 through 14, Qualities A and B (left); Pictures 7 to 11, Qualities A and B (center); and Pictures 7 and 11, Qualities A and B (right) .
    [Show full text]
  • Appendix:. Maps of the Terrestrial Planets
    APPENDIX Maps of the Terrestrial Planets Mercury SOUTH POLAR REGION SCALE 1 8388000 AT 56' LATITUDE POLAR STEREOGRAPHIC PROJECTION i \ \ \ \ .. \. 200 KILOMETERS 400 600 800 1000 NORTH POLAR REGION Mercury North 0 ZW KILOMETERS 400 600 800 1000 2W0 257. I 550. , 140. / / f30. r20. * / - - I +I". 1 1 / / / I North -GO'7 South SCALE 1 50000MO llmm 50 kml AT 0 LlT4TUDE MERCATOR PROlECTlON CONTOUR PLANET ELEVATION RADIUS l~~lornererrl IU~lometerrl 6063 Earth North Pole 278 South Pole 279 Earth Moon ' 1 "'rnl",,, , 'f 4 .I-.%, + I/>, ,,, /!v~00xu3 \\' 345 ! , , , 15 (15WI 0 NORTH POLAR REGION Moon Mars NORTH POLAR REGION Polar cap 81 11apparld on August 4. 1972 SOUTH POLAR REGION Polar cap as 11 sSWrd on February 28 1972 287 Mars 4u-t-t PLAt$ITIA F South SCALE 1 25.0m.0m A7 0' LATITUDE 1 12.549 CCO IT M' LATITUDE MERCITOR PROJLCTON m lorn ern CONTOUR lNTERYltL I KlLOMETRE 288 REFERENCES CHAPTER 1 Burns, J. A., 1976. Consequences of tidal slowing of Mercury: Icarus, v. 28, pp. 453-458. Beatty, J. K., B. O'Leary, and A. Chaikin, 1981. The New Solar Carr, M. H., L. S. Crumpler, J. A. Cutts, R. Greeley, J. E. System: Sky Publishing Corp., Cambridge, Mass. Guest, and H. Masursky, 1977. Martian impact craters and Shoemaker, E. M., 1962. Interpretation of lunar craters: Physics emplacement of ejecta by surface flow: J. Geophys. Res., v. 82, and Astronomy of the Moon (Kopal, Z., ed.), Academic Press, p. 4055. N.Y., pp. 283-359. Chapman, C. R., 1976. Chronology of terrestrial planet evolu- Shoemaker, E.
    [Show full text]
  • Thedatabook.Pdf
    THE DATA BOOK OF ASTRONOMY Also available from Institute of Physics Publishing The Wandering Astronomer Patrick Moore The Photographic Atlas of the Stars H. J. P. Arnold, Paul Doherty and Patrick Moore THE DATA BOOK OF ASTRONOMY P ATRICK M OORE I NSTITUTE O F P HYSICS P UBLISHING B RISTOL A ND P HILADELPHIA c IOP Publishing Ltd 2000 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior permission of the publisher. Multiple copying is permitted in accordance with the terms of licences issued by the Copyright Licensing Agency under the terms of its agreement with the Committee of Vice-Chancellors and Principals. British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library. ISBN 0 7503 0620 3 Library of Congress Cataloging-in-Publication Data are available Publisher: Nicki Dennis Production Editor: Simon Laurenson Production Control: Sarah Plenty Cover Design: Kevin Lowry Marketing Executive: Colin Fenton Published by Institute of Physics Publishing, wholly owned by The Institute of Physics, London Institute of Physics Publishing, Dirac House, Temple Back, Bristol BS1 6BE, UK US Office: Institute of Physics Publishing, The Public Ledger Building, Suite 1035, 150 South Independence Mall West, Philadelphia, PA 19106, USA Printed in the UK by Bookcraft, Midsomer Norton, Somerset CONTENTS FOREWORD vii 1 THE SOLAR SYSTEM 1
    [Show full text]
  • National Aeronautics and Space Administration) 111 P HC AO,6/MF A01 Unclas CSCL 03B G3/91 49797
    https://ntrs.nasa.gov/search.jsp?R=19780004017 2020-03-22T06:42:54+00:00Z NASA TECHNICAL MEMORANDUM NASA TM-75035 THE LUNAR NOMENCLATURE: THE REVERSE SIDE OF THE MOON (1961-1973) (NASA-TM-75035) THE LUNAR NOMENCLATURE: N78-11960 THE REVERSE SIDE OF TEE MOON (1961-1973) (National Aeronautics and Space Administration) 111 p HC AO,6/MF A01 Unclas CSCL 03B G3/91 49797 K. Shingareva, G. Burba Translation of "Lunnaya Nomenklatura; Obratnaya storona luny 1961-1973", Academy of Sciences USSR, Institute of Space Research, Moscow, "Nauka" Press, 1977, pp. 1-56 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION M19-rz" WASHINGTON, D. C. 20546 AUGUST 1977 A % STANDARD TITLE PAGE -A R.,ott No0... r 2. Government Accession No. 31 Recipient's Caafog No. NASA TIM-75O35 4.-"irl. and Subtitie 5. Repo;t Dote THE LUNAR NOMENCLATURE: THE REVERSE SIDE OF THE August 1977 MOON (1961-1973) 6. Performing Organization Code 7. Author(s) 8. Performing Organizotion Report No. K,.Shingareva, G'. .Burba o 10. Coit Un t No. 9. Perlform:ng Organization Nome and Address ]I. Contract or Grant .SCITRAN NASw-92791 No. Box 5456 13. T yp of Report end Period Coered Santa Barbara, CA 93108 Translation 12. Sponsoring Agiicy Noms ond Address' Natidnal Aeronautics and Space Administration 34. Sponsoring Agency Code Washington,'.D.C. 20546 15. Supplamortary No9 Translation of "Lunnaya Nomenklatura; Obratnaya storona luny 1961-1973"; Academy of Sciences USSR, Institute of Space Research, Moscow, "Nauka" Press, 1977, pp. Pp- 1-56 16. Abstroct The history of naming the details' of the relief on.the near and reverse sides 6f .
    [Show full text]