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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. -
Paul Scherrer Institute Scientific Report 1998. Volume V
ETOf-C//—^ fo / PAUL S CHER HER INSTITUT ISSN 1423-7342 March 1999 i J i I i i i i PSI • Scientific Report 1998 / Volume V General Energy Photo Cover View along the tubing system of a prototype Condensation Interface which was developed for the on-line measurement of heavy metal concentrations in hot gases. See article by Ch. Ludwig, S. Stuck! and A.J. Schuler Photo: Armin Muller, RSI PAULSCHERRER INSTITUT ISSN 1423-7342 March 1999 Scientific Report 1998 Volume V General Energy ed. by: Christina Daum and Jakob Leuenberger CH-5232 Villigen PSI Switzerland Phone: 056/310 21 11 Telefax: 056/310 21 99 http://www1.psi.ch/www_f5_hn/f5_home.html DISCLAIMER Portions of this document may be illegible in electronic image products. Images are produced from the best available original document. TABLE OF CONTENTS Introduction 1 A. Wokaun Renewable Energies and Materials Cycles 3 The Influence of Chlorine on the Fate and Activity of Alkali Metals during the Gasification of 4 Wood R. Struis, C. von Scala, A. Schuler, S. Stuck! On-Board Conversion of Methanol to Dimethyl Ether as an Alternative Diesel Fuel 6 H. Armbruster, G. Heinzelmann, R. Struis, S. Stuck! Solar Thermal Production of Zinc: Program Strategy 8 A. Steinfeld, A. Weidenkaff, S. Moeller, R. Palumbo Economic Evaluation of the Solar Thermal Co-Production of Zinc, Synthesis Gas, and 10 Hydrogen A. Steinfeld, I. Spiewak (EC Joint Research Centre, Spain) Solar Production of Catalytic Filamentous Carbon by Thermal Decomposition of Hydro- 12 carbons and Carbon Monoxide V.A. Kirillov, G.G. Kuvshinov, Yu.l. -
Lunar Distances Final
A (NOT SO) BRIEF HISTORY OF LUNAR DISTANCES: LUNAR LONGITUDE DETERMINATION AT SEA BEFORE THE CHRONOMETER Richard de Grijs Department of Physics and Astronomy, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia Email: [email protected] Abstract: Longitude determination at sea gained increasing commercial importance in the late Middle Ages, spawned by a commensurate increase in long-distance merchant shipping activity. Prior to the successful development of an accurate marine timepiece in the late-eighteenth century, marine navigators relied predominantly on the Moon for their time and longitude determinations. Lunar eclipses had been used for relative position determinations since Antiquity, but their rare occurrences precludes their routine use as reliable way markers. Measuring lunar distances, using the projected positions on the sky of the Moon and bright reference objects—the Sun or one or more bright stars—became the method of choice. It gained in profile and importance through the British Board of Longitude’s endorsement in 1765 of the establishment of a Nautical Almanac. Numerous ‘projectors’ jumped onto the bandwagon, leading to a proliferation of lunar ephemeris tables. Chronometers became both more affordable and more commonplace by the mid-nineteenth century, signaling the beginning of the end for the lunar distance method as a means to determine one’s longitude at sea. Keywords: lunar eclipses, lunar distance method, longitude determination, almanacs, ephemeris tables 1 THE MOON AS A RELIABLE GUIDE FOR NAVIGATION As European nations increasingly ventured beyond their home waters from the late Middle Ages onwards, developing the means to determine one’s position at sea, out of view of familiar shorelines, became an increasingly pressing problem. -
Graphical Evidence for the Solar Coronal Structure During the Maunder Minimum: Comparative Study of the Total Eclipse Drawings in 1706 and 1715
J. Space Weather Space Clim. 2021, 11,1 Ó H. Hayakawa et al., Published by EDP Sciences 2021 https://doi.org/10.1051/swsc/2020035 Available online at: www.swsc-journal.org Topical Issue - Space climate: The past and future of solar activity RESEARCH ARTICLE OPEN ACCESS Graphical evidence for the solar coronal structure during the Maunder minimum: comparative study of the total eclipse drawings in 1706 and 1715 Hisashi Hayakawa1,2,3,4,*, Mike Lockwood5,*, Matthew J. Owens5, Mitsuru Sôma6, Bruno P. Besser7, and Lidia van Driel – Gesztelyi8,9,10 1 Institute for Space-Earth Environmental Research, Nagoya University, 4648601 Nagoya, Japan 2 Institute for Advanced Researches, Nagoya University, 4648601 Nagoya, Japan 3 Science and Technology Facilities Council, RAL Space, Rutherford Appleton Laboratory, Harwell Campus, OX11 0QX Didcot, UK 4 Nishina Centre, Riken, 3510198 Wako, Japan 5 Department of Meteorology, University of Reading, RG6 6BB Reading, UK 6 National Astronomical Observatory of Japan, 1818588 Mitaka, Japan 7 Space Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria 8 Mullard Space Science Laboratory, University College London, RH5 6NT Dorking, UK 9 LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, 92195 Meudon, France 10 Konkoly Observatory, Hungarian Academy of Sciences, 1121 Budapest, Hungary Received 18 October 2019 / Accepted 29 June 2020 Abstract – We discuss the significant implications of three eye-witness drawings of the total solar eclipse on 1706 May 12 in comparison with two on 1715 May 3, for our understanding of space climate change. These events took place just after what has been termed the “deep Maunder Minimum” but fall within the “extended Maunder Minimum” being in an interval when the sunspot numbers start to recover. -
Journal of Space Law Volume 40 Number 1-2 2015-2016
Journal of Space Law Volume 40 Number 1-2 2015-2016 Articles The Exploitation of Asteroids and The Non-Appropriation Principle: Reflections on the nature of property rights in light of the US Space Resource Act of 2015 ............................................................................................Philip de Man Green for Liftoff: Structural Changes for Environmental and Economic Sustainability in Space Launching ............................................................................Justin Fisch Asteroid Mining and its Legal Implications.................................Devanshu Ganatra, Neil Modi Regulating the Void: In-orbit Collisions and Space Debris...........................Timothy G. Nelson Global Cap and Trade System for Space Debris: Putting a Price on Space Hazards ......................................................Anja Nakarada Pecujlic, Sarah Katharina Germann Effective Exercise of ‘In-space Jurisdiction’: The US Approach and the Problems it is Facing ....................................................................................Frans von der Dunk Commentaries The Legality of Mining Celestial Bodies New..................................................Thomas Gangale New Space Activities Expose a Potential Legal Vacuum............................Susan J. Trepczynski Book Reviews & Space Law Bibliography 61 1 to 40 -2 2 Vol. , No. 1 Journal of Space Law Pages 2013 JOURNAL OF SPACE LAW VOLUME 40, NUMBER 1&2 2015-2016 JOURNAL OF SPACE LAW UNIVERSITY OF MISSISSIPPI SCHOOL OF LAW A JOURNAL DEVOTED TO SPACE -
Smithsonian Contributions to Astrophysics
Smithsonian Contributions to Astrophysics VOLUME 5, NUMBER 8 AN ANNOTATED BIBLIOGRAPHY ON INTERPLANETARY DUST by PAUL W. HODGE, FRANCES W. WRIGHT, AND DORRIT HOFFLEIT SMITHSONIAN INSTITUTION Washington, D.C. 1961 Publications of the Astrophysical Observatory This series, Smithsonian Contributions to Astrophysics, was inaugurated in 1956 to provide a proper communication for the results of research con- ducted at the Astrophysical Observatory of the Smithsonian Institution. Its purpose is the "increase and diffusion of knowledge" in the field of astrophysics, with particular emphasis on problems of the sun, the earth and the solar system. Its pages are open to a limited number of papers by other investigators with whom we have common interests. Another series is Annals of the Astrophysical Observatory. It was started in 1900 by the Observatory's first director, Samuel P. Langley, and has been published about every 10 years since that date. These quarto volumes, some of which are still available, record the history of the Observatory's researches and activities. Many technical papers and volumes emanating from the Astrophysical Observatory have appeared in the Smithsonian Miscellaneous Collections. Among these are Smithsonian Physical Tables, Smithsonian Meteorological Tables, and World Weather Records. Additional information concerning these publications may be secured from the Editorial and Publications Division, Smithsonian Institution, Wash- ington, D.C. FBED L. WHIPPLE, Director, Astrophysical Observatory, Cambridge, Mass. Smithsonian Institution. For sale by the Superintendent of Documents, U.S. Government Printing Office Washington 25, D.C. - Price 25 cents An Annotated Bibliography on Interplanetary Dust BY PAUL W. HODGE,1 FRANCES W. WRIGHT,1 AND DORRIT HOFFLEIT3 This annotated bibliography presents a AHNERT, E. -
Special Regions’’: Findings of the Second MEPAG Special Regions Science Analysis Group (SR-SAG2)
ASTROBIOLOGY Volume 14, Number 11, 2014 News & Views ª Mary Ann Liebert, Inc. DOI: 10.1089/ast.2014.1227 A New Analysis of Mars ‘‘Special Regions’’: Findings of the Second MEPAG Special Regions Science Analysis Group (SR-SAG2) John D. Rummel,1 David W. Beaty,2 Melissa A. Jones,2 Corien Bakermans,3 Nadine G. Barlow,4 Penelope J. Boston,5 Vincent F. Chevrier,6 Benton C. Clark,7 Jean-Pierre P. de Vera,8 Raina V. Gough,9 John E. Hallsworth,10 James W. Head,11 Victoria J. Hipkin,12 Thomas L. Kieft,5 Alfred S. McEwen,13 Michael T. Mellon,14 Jill A. Mikucki,15 Wayne L. Nicholson,16 Christopher R. Omelon,17 Ronald Peterson,18 Eric E. Roden,19 Barbara Sherwood Lollar,20 Kenneth L. Tanaka,21 Donna Viola,13 and James J. Wray22 Abstract A committee of the Mars Exploration Program Analysis Group (MEPAG) has reviewed and updated the description of Special Regions on Mars as places where terrestrial organisms might replicate (per the COSPAR Planetary Protection Policy). This review and update was conducted by an international team (SR-SAG2) drawn from both the biological science and Mars exploration communities, focused on understanding when and where Special Regions could occur. The study applied recently available data about martian environments and about terrestrial organisms, building on a previous analysis of Mars Special Regions (2006) undertaken by a similar team. Since then, a new body of highly relevant information has been generated from the Mars Reconnaissance Orbiter (launched in 2005) and Phoenix (2007) and data from Mars Express and the twin Mars Exploration Rovers (all 2003). -
E.G., Young Et Al. 2017
Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 203 (2017) 235–264 www.elsevier.com/locate/gca l2 13 The relative abundances of resolved CH2D2 and CH3D and mechanisms controlling isotopic bond ordering in abiotic and biotic methane gases E.D. Young a,⇑, I.E. Kohl a, B. Sherwood Lollar b, G. Etiope c,d, D. Rumble III e, S. Li (李姝宁) a, M.A. Haghnegahdar a, E.A. Schauble a, K.A. McCain a, D.I. Foustoukos e, C. Sutclife b, O. Warr b, C.J. Ballentine f, T.C. Onstott g, H. Hosgormez h, A. Neubeck i, J.M. Marques j,I.Pe´rez-Rodrı´guez k, A.R. Rowe k, D.E. LaRowe k, C. Magnabosco l, L.Y. Yeung m, J.L. Ash a, L.T. Bryndzia n a University of California Los Angeles, United States b University of Toronto, Canada c Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma 2, Italy d Faculty of Environmental Science and Engineering, Babes-Bolyai University, Cluj-Napoca, Romania e Carnegie Institution of Washington, United States f University of Oxford, United Kingdom g Princeton University, United States h Istanbul University, Republic of Turkey i Stockholm University, Sweden j Universidade de Lisboa, Portugal k University of Southern California, United States l Simons Foundation, United States m Rice University, United States n Shell International Exploration and Production Inc., United States Received 11 August 2016; accepted in revised form 31 December 2016; Available online 11 January 2017 Abstract 12 13 We report measurements of resolved CH2D2 and CH3D at natural abundances in a variety of methane gases produced 12 13 naturally and in the laboratory. -
Characterization of Impactite Clay Minerals with Implications for Mars Geologic Context and Mars Sample Return
Western University Scholarship@Western Electronic Thesis and Dissertation Repository 4-9-2020 10:00 AM Characterization of Impactite Clay Minerals with Implications for Mars Geologic Context and Mars Sample Return Christy M. Caudill The University of Western Ontario Supervisor Dr. Gordon Osinski The University of Western Ontario Co-Supervisor Dr. Livio Tornabene The University of Western Ontario Graduate Program in Geology A thesis submitted in partial fulfillment of the equirr ements for the degree in Doctor of Philosophy © Christy M. Caudill 2020 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Geology Commons, and the Other Earth Sciences Commons Recommended Citation Caudill, Christy M., "Characterization of Impactite Clay Minerals with Implications for Mars Geologic Context and Mars Sample Return" (2020). Electronic Thesis and Dissertation Repository. 6935. https://ir.lib.uwo.ca/etd/6935 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. Abstract Geological processes, including impact cratering, are fundamental throughout rocky bodies in the solar system. Studies of terrestrial impact structures, like the Ries impact structure, Germany, have informed on impact cratering processes – e.g., early hot, hydrous degassing, autometamorphism, and recrystallization/devitrification of impact glass – and products – e.g., impact melt rocks and breccias comprised of clay minerals. Yet, clay minerals of authigenic impact origin remain understudied and their formation processes poorly-understood. This thesis details the characterization of impact-generated clay minerals at Ries, showing that compositionally diverse, abundant Al/Fe/Mg smectite clays formed through these processes in thin melt-bearing breccia deposits of the ejecta, as well as at depth. -
The Relative Abundances of Resolved L2ch2d2 and 13CH3D And
Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 203 (2017) 235–264 www.elsevier.com/locate/gca l2 13 The relative abundances of resolved CH2D2 and CH3D and mechanisms controlling isotopic bond ordering in abiotic and biotic methane gases E.D. Young a,⇑, I.E. Kohl a, B. Sherwood Lollar b, G. Etiope c,d, D. Rumble III e, S. Li (李姝宁) a, M.A. Haghnegahdar a, E.A. Schauble a, K.A. McCain a, D.I. Foustoukos e, C. Sutclife b, O. Warr b, C.J. Ballentine f, T.C. Onstott g, H. Hosgormez h, A. Neubeck i, J.M. Marques j,I.Pe´rez-Rodrı´guez k, A.R. Rowe k, D.E. LaRowe k, C. Magnabosco l, L.Y. Yeung m, J.L. Ash a, L.T. Bryndzia n a University of California Los Angeles, United States b University of Toronto, Canada c Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma 2, Italy d Faculty of Environmental Science and Engineering, Babes-Bolyai University, Cluj-Napoca, Romania e Carnegie Institution of Washington, United States f University of Oxford, United Kingdom g Princeton University, United States h Istanbul University, Republic of Turkey i Stockholm University, Sweden j Universidade de Lisboa, Portugal k University of Southern California, United States l Simons Foundation, United States m Rice University, United States n Shell International Exploration and Production Inc., United States Received 11 August 2016; accepted in revised form 31 December 2016; Available online 11 January 2017 Abstract 12 13 We report measurements of resolved CH2D2 and CH3D at natural abundances in a variety of methane gases produced 12 13 naturally and in the laboratory. -
Bulk Mineralogy of Lunar Crater Central Peaks Via Thermal Infrared Spectra from the Diviner Lunar Radiometer - a Study of the Moon’S Crustal Composition at Depth
Bulk mineralogy of Lunar crater central peaks via thermal infrared spectra from the Diviner Lunar Radiometer - A study of the Moon’s crustal composition at depth Eugenie Song A thesis submitted in partial fulfillment of the requirements for the degree of Master of Sciences University of Washington 2012 Committee: Joshua Bandfield Alan Gillespie Bruce Nelson Program Authorized to Offer Degree: Earth and Space Sciences 1 Table of Contents List of Figures ............................................................................................................................................... 3 List of Tables ................................................................................................................................................ 3 Abstract ......................................................................................................................................................... 4 1 Introduction .......................................................................................................................................... 5 1.1 Formation of the Lunar Crust ................................................................................................... 5 1.2 Crater Morphology ................................................................................................................... 7 1.3 Spectral Features of Rock-Forming Silicates in the Lunar Environment ................................ 8 1.4 Compositional Studies of Lunar Crater Central Peaks ........................................................... -
User Guide To
USER GUIDE TO 1 2 5 0 , 000 S CA L E L U NA R MA P S DANNY C. KINSLER Lunar Science Institute 3303 NASA Road #1 Houston, TX 77058 Telephone: 713/488-5200 Cable Address: LUNSI The Lunar Science Institute is operated by the Universities Space Research Association under Contract No. NSR 09-051-001 with the National Aeronautics and Space Administration. This document constitutes LSI Contribution No. 206 March 1975 USER GUIDE TO 1 : 250 , 000 SCALE LUNAR MAPS GENERAL In 1 972 the NASA Lunar Programs Office initiated the Apoll o Photographic Data Analysis Program. The principal point of this program was a detail ed 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 useabl e 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 desi gned to present in outline form the neces- sary background information for 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. The base is compiled from vertical Metric photography from Apollo missions 15, 16, and 17.