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Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Les Pires Menaces Sont Étudiées En Secret À Spiez
SALAIRES De la peine à suivre la hausse des prix HOCKEY Il devra faire trembler les filets Les rares augmentations n’égalent pas toujours Charles Bertrand a débarqué à Gottéron. le renchérissement bien que l’économie cartonne. L 7 Mais le Français ne jouera pas ce soir. L 19 QUOTIDIEN ROMAND ÉDITÉ À FRIBOURG MARDI 4 DÉCEMBRE 2018 N° 55 • 148 e année / Semaine Fr. 2.70 / Samedi Fr. 3.70 JA 1701 Fribourg Le bâtiment Les pires menaces sont de Yendi revit BULLE L’ancien centre logistique de l’enseigne bulloise de prêt-à-porter Yendi, tombée en faillite depuis, a trouvé preneur. étudiées en secret à Spiez PowerData, une entreprise vaudoise basée à Tolochenaz, près de Morges, espère prendre possession des lieux à partir du milieu de l’an prochain. Spécialisée dans la distribution de produits électroniques, la société compte y créer une douzaine d’emplois dans un premier temps. L 11 Dans la forêt du Burgerwald. Charly Rappo Des sapins locaux à bon prix NOËL Guidées par des traditions locales, de nombreuses communes fribourgeoises proposent des sapins à leurs citoyens pour un prix inférieur à celui du marché. Ces conifères, de qualité malgré la sécheresse de l’été dernier, viennent des forêts du canton. L 13 La loi sur le CO2 se concrétise CLIMAT Le National a empoigné hier la révision totale de la loi sur le CO2 qui Le laboratoire de Spiez est à la pointe de la recherche contre les menaces chimiques ou biologiques. Keystone-archives l’occupera plusieurs jours. L’UDC a tenté de bloquer le dossier, en vain: l’entrée en Situé au pied des majes- taine au total, y analysent les pires me- s’est retrouvé depuis septembre sous les matière a été largement acceptée. -
Relative Ages
CONTENTS Page Introduction ...................................................... 123 Stratigraphic nomenclature ........................................ 123 Superpositions ................................................... 125 Mare-crater relations .......................................... 125 Crater-crater relations .......................................... 127 Basin-crater relations .......................................... 127 Mapping conventions .......................................... 127 Crater dating .................................................... 129 General principles ............................................. 129 Size-frequency relations ........................................ 129 Morphology of large craters .................................... 129 Morphology of small craters, by Newell J. Fask .................. 131 D, method .................................................... 133 Summary ........................................................ 133 table 7.1). The first three of these sequences, which are older than INTRODUCTION the visible mare materials, are also dominated internally by the The goals of both terrestrial and lunar stratigraphy are to inte- deposits of basins. The fourth (youngest) sequence consists of mare grate geologic units into a stratigraphic column applicable over the and crater materials. This chapter explains the general methods of whole planet and to calibrate this column with absolute ages. The stratigraphic analysis that are employed in the next six chapters first step in reconstructing -
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. -
Do Detetor De Hertz Ao Coesor
Do detetor de Hertz ao coesor Em 1886, em Karlsruhe, Alemanha, Heinrich Hertz usava frequentemente as bobinas espirais acopladas de Peter Riess em demonstrações na lecionação das suas aulas de Física. Estas bobinas eram dois anéis metálicos abertos, com igual diâmetro, terminados em pequenas esferas metálicas, cuja distância (spark gap) podia ser ajustada por um parafuso micrométrico. Hertz verificou que era relativamente fácil gerar uma faísca num anel (primário) à custa de uma bobina de indução e observar uma réplica no outro anel (secundário), supostamente por efeito de indução eletromagnética. Hertz concluiu rapidamente que não se tratava de um efeito de indução, uma vez que o afastamento progressivo dos dois anéis não seguia a lei de decréscimo da indução eletromagnética. Hertz usou este dispositivo como detetor de ondas de rádio nos seus trabalhos sobre ondas eletromagnéticas (ver aqui). O anel de Hertz é, assim, o primeiro detetor de sinais de rádio. Este detetor tem uma sensibilidade muito baixa e a pequena faísca nunca pode ser vista por muitas pessoas. Vários investigadores sugeriram alterações para ampliar a visibilidade e estas foram desde a colocação do spark gap num frasco com uma mistura de oxigénio e hidrogénio, que explodiria assim que houvesse uma pequena faísca, e até à inclusão do spark gap dentro de um tubo de descarga de gás de Geissler para a faísca iniciar a descarga dentro do gás e iluminá-lo. Outros investigadores associaram galvanómetros às extremidades do anel de Hertz, para verem o deslocamento do ponteiro, ou até usaram auscultadores de alta impedância ligados às esferas do detetor para ouvir o sinal recebido. -
History of Nonlinear Oscillations Theory in France (1880–1940)
Archimedes 49 New Studies in the History and Philosophy of Science and Technology Jean-Marc Ginoux History of Nonlinear Oscillations Theory in France (1880–1940) History of Nonlinear Oscillations Theory in France (1880–1940) Archimedes NEW STUDIES IN THE HISTORY AND PHILOSOPHY OF SCIENCE AND TECHNOLOGY VOLUME 49 EDITOR JED Z. BUCHWALD, Dreyfuss Professor of History, California Institute of Technology, Pasadena, USA. ASSOCIATE EDITORS FOR MATHEMATICS AND PHYSICAL SCIENCES JEREMY GRAY, The Faculty of Mathematics and Computing, The Open University, UK. TILMAN SAUER, Johannes Gutenberg University Mainz, Germany ASSOCIATE EDITORS FOR BIOLOGICAL SCIENCES SHARON KINGSLAND, Department of History of Science and Technology, Johns Hopkins University, Baltimore, USA. MANFRED LAUBICHLER, Arizona State University, USA ADVISORY BOARD FOR MATHEMATICS, PHYSICAL SCIENCES AND TECHNOLOGY HENK BOS, University of Utrecht, The Netherlands MORDECHAI FEINGOLD, California Institute of Technology, USA ALLAN D. FRANKLIN, University of Colorado at Boulder, USA KOSTAS GAVROGLU, National Technical University of Athens, Greece PAUL HOYNINGEN-HUENE, Leibniz University in Hannover, Germany TREVOR LEVERE, University of Toronto, Canada JESPER LÜTZEN, Copenhagen University, Denmark WILLIAM NEWMAN, Indiana University, Bloomington, USA LAWRENCE PRINCIPE, The Johns Hopkins University, USA JÜRGEN RENN, Max Planck Institute for the History of Science, Germany ALEX ROLAND, Duke University, USA ALAN SHAPIRO, University of Minnesota, USA NOEL SWERDLOW, California Institute of Technology, -
Apollo 17 Index: 70 Mm, 35 Mm, and 16 Mm Photographs
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) Preparation, Scanning, Editing, and Conversion to Adobe Portable Document Format (PDF) by: Ronald A. Wells University of California Berkeley, CA 94720 May 2000 A P O L L O 1 7 I N D E X 7 0 m m, 3 5 m m, A N D 1 6 m m P H O T O G R A P H S M a p p i n g S c i e n c e s B r a n c h N a t i o n a l A e r o n a u t i c s a n d S p a c e A d m i n i s t r a t i o n J o h n s o n S p a c e C e n t e r H o u s t o n, T e x a s APPROVED: Michael C . -
Odd Year Nur-Rn-Lic-30550 G
LicenseNumber FirstName MiddleName LastName RenewalGroup NUR-LPN-LIC-6174 DOLORES ROSE AABERG 2019 - ODD YEAR NUR-RN-LIC-30550 GRETCHEN ELLEN AAGAARD-SHIVELY 2019 - ODD YEAR NUR-RN-LIC-128118 CAMBRIA LAUREN AANERUD 2019 - ODD YEAR NUR-RN-LIC-25862 SOPHIA SABINA AANSTAD 2018 - EVEN YEAR NUR-APRN-LIC-124944 ERIN EDWARD AAS 2018 - EVEN YEAR NUR-RN-LIC-105371 ERIN EDWARD AAS 2018 - EVEN YEAR NUR-RN-LIC-34536 BRYON AAS 2019 - ODD YEAR NUR-RN-LIC-39208 JULIA LYNN AASEN 2018 - EVEN YEAR NUR-APRN-LIC-130522 LORI ANN AASEN 2019 - ODD YEAR NUR-RN-LIC-130520 LORI ANN AASEN 2019 - ODD YEAR NUR-RN-LIC-21015 DEBBIE ABAR 2018 - EVEN YEAR NUR-APRN-LIC-130757 LUKE G ABAR 2018 - EVEN YEAR NUR-RN-LIC-130756 LUKE GORDON ABAR 2019 - ODD YEAR NUR-RN-LIC-31911 AIMEE KRISTINE ABBOTT 2018 - EVEN YEAR NUR-RN-LIC-29448 DENISE M ABBOTT 2018 - EVEN YEAR NUR-RN-LIC-131150 SARAH FRANCES ABBOTT 2018 - EVEN YEAR NUR-LPN-LIC-31701 ANGIE ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-33325 HEIDI ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-4920 LORI ANN ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-97426 DAYMON ABBOTT Expired - 2018 - EVEN YEAR NUR-RN-LIC-13260 ROBERT C ABBOTT Expired - 2018 - EVEN YEAR NUR-RN-LIC-17858 MONICA MAY ABDALLAH 2018 - EVEN YEAR NUR-RN-LIC-48890 STEVEN P ABDALLAH 2019 - ODD YEAR NUR-APRN-LIC-101391 LANEICE LORRAINE ABDEL-SHAKUR Expired - 2018 - EVEN YEAR NUR-RN-LIC-101333 LANEICE LORRAINE ABDEL-SHAKUR Expired - 2018 - EVEN YEAR NUR-RN-LIC-96606 RENDI L ABEL 2018 - EVEN YEAR NUR-RN-LIC-97338 LAURA ANN ABEL 2019 - ODD YEAR NUR-RN-LIC-69876 LACEY ANN ABELL 2019 - ODD YEAR NUR-RN-LIC-131932 -
Experimentally Demonstrated the Intrinsic Instability of the Fluorite-Type Zr Cation Network
0246110 Rta(i) 1 1,2 l,4 1,6 1,l 2 22 Rta(i) Figure 2. Temperature dependence of Zr-FTfor pure orthorhombic zirconia Figure 3 Temperature dependence of Zr-0 shell in tetragonal zirconia solid solution Our study has experimentally demonstrated the intrinsic instability of the fluorite-type Zr cation network. Coherent scattering beween Conclusions central Zr ion and distant cations is weaker and vibration modes of the Zr-cation network are It is found that, for all of zirconia solid softer in tetragonal zirconia than in monoclmic, solutions studied, the dopant-oxygen distances are orthorhombic, or stabilized cubic zirconia. In si@icantly ddferent from the Zr-0 distances. addition, the outer foux oxygens in the 8-fold The dopant-cation distances, on the other hand, coordinated Zr-0 polyhedron are only loosely are usually very close to the Zr-Zr distance, solutions. A bonded and are subject to very large static and confirming the formation of solid dynamic distortions. This effect is illustrated by general structural picture for zirconia solid the expanded portion of the Fourier transform solutions is one that places the dopant cations shown in Figure 3. randomly on tbe Zr sites in the cation network, but with distorted and sometimes very different Dopant Structure dopant-oxygen polyhedra surrounding these dopants. In the case of Ge4+ doping and Y-Nb We have also successfully performed co-doping, short-rangecation ordering has been EXAFS experiments at the dopant absorption suggested from our EXAFS results. edges for doped zirconia solid solutions. Dopants Based on the above structural information studied include the Ce-,Nb-, and Y-K edges as and other EXAFS results obtained from NSLS, well as Ce-LIn edge. -
The Lateral Growth and Coalesence of Magma Systems Royalsocietypublishing.Org/Journal/Rsta Juliet Biggs1 and Catherine Annen1,2
The lateral growth and coalesence of magma systems royalsocietypublishing.org/journal/rsta Juliet Biggs1 and Catherine Annen1,2 1School of Earth Sciences, University of Bristol, Queen’s Road, Bristol, BS8 1RJ, UK Research 2Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, IFSTTAR, Cite this article: Biggs J, Annen C. 2019 The ISTerre, 38000 Grenoble, France lateral growth and coalesence of magma JB, 0000-0002-4855-039X systems . Phil.Trans.R.Soc.A377: 20180005. http://dx.doi.org/10.1098/rsta.2018.0005 Thermal and mechanical models of magma reservoir growth need to be reconciled with deformation patterns and structural relationships observed at Accepted: 16 October 2018 active magma systems. Geophysical observations provide a series of short time-scale snap-shots (100– One contribution of 15 to a Theo Murphy 102 years) of the long-term growth of magmatic 3 6 meeting issue ‘Magma reservoir architecture bodies (10 –10 years). In this paper, we first review evidence for the growth of magmatic systems along and dynamics’. structural features and the associated deformation patterns. We then define three distinct growth stages, Subject Areas: (1) aligned melt pockets, (2) coalesced reservoirs, (3) volcanology, geophysics highly evolved systems, which can be distinguished using short-term surface observations. We use Keywords: two-dimensional thermal models to provide first- thermal models, surface deformation, order constraints on the time scales and conditions transcrustal magmatic systems associated with coalescence of individual magma bodies into large-scale reservoirs. We find that closely spaced intrusions (less than 1 km apart) can develop Author for correspondence: combined viscoelastic shells over time scales of 10s kyr Juliet Biggs and form laterally extensive mush systems over time e-mail: [email protected] scales of 10–100 kyr. -
The Case for Rainfall on a Warm, Wet Early Mars Robert A
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. E11, 5111, doi:10.1029/2001JE001505, 2002 The case for rainfall on a warm, wet early Mars Robert A. Craddock Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, District of Columbia, USA Alan D. Howard Department of Environmental Sciences, University of Virginia, Charlottesville, Virginia, USA Received 11 April 2001; revised 10 April 2002; accepted 10 June 2002; published 23 November 2002. [1] Valley networks provide compelling evidence that past geologic processes on Mars were different than those seen today. The generally accepted paradigm is that these features formed from groundwater circulation, which may have been driven by differential heating induced by magmatic intrusions, impact melt, or a higher primordial heat flux. Although such mechanisms may not require climatic conditions any different than today’s, they fail to explain the large amount of recharge necessary for maintaining valley network systems, the spatial patterns of erosion, or how water became initially situated in the Martian regolith. In addition, there are no clear surface manifestations of any geothermal systems (e.g., mineral deposits or phreatic explosion craters). Finally, these models do not explain the style and amount of crater degradation. To the contrary, analyses of degraded crater morphometry indicate modification occurred from creep induced by rain splash combined with surface runoff and erosion; the former process appears to have continued late into Martian history. A critical analysis of the morphology and drainage density of valley networks based on Mars Global Surveyor data shows that these features are, in fact, entirely consistent with rainfall and surface runoff. -
White Paper Secured Time Synchronization
WHITE PAPER SECURED TIME SYNCHRONIZATION SHARED TALENTS OF FRENCH EXPERTS IN TIME/FREQUENCY SUMMARY 2 EVOLUTION OF TIME PRODUCTION 10 EVOLUTION OF TIME SYNCHRONIZATION 16 EVOLUTION OF TIME BROADCASTING 26 THE SCPTime® PROJECT 53 PARTNERS Text: Maurice GORGY, Nicolas GORGY, Alexandre D’HERBOMEZ, with the participation of Patrick ROYET (Tyléos). Design: Emmanuel ANDRILLON 2 PREFACE Dear readers, Since the XVIIIth century, clockmakers have contributed to the growth in commercial exchanges and then, physicists started to master time measurement precise enough for scientific use. Today, the explosion of the digital economy that produces more than half of trade transactions is bringing a new revolution. Fortunately, French Observatories produce time scales precise to 10-15 seconds which means an error of only 1 second in a 300 million years period of time. France is the technological birthplace of the world’s Time/Frequency industry. Especially as the SYRTE (Paris Observatory, CNRS, UPMC, and LNE) delivers a legal time built on the UTC international time scale (Coordinated Universal Time). Within new digital organizations, time synchronization allows not only to distribute time to clocks but also to synchronized devices (the Internet of Things) and machines with no concern about distance with a precision that can reach a few nanoseconds, depending on the applications. Although high precision time production is perfectly mastered by the Observatories of Paris and Besançon, the actual technological challenge is to master the security and traceability of the date and time from their source to the final user. This is key to fighting cyberattacks that interfere with the time message. Time cybersecurity… a new challenge.