Planetary Cartography and Mapping: Where We Are Today, and Where We Are Heading For?
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Extensional Tectonics in Tempe Terra 8 May 2006
Extensional tectonics in Tempe Terra 8 May 2006 Tectonic processes (extensional stresses, in this case) have led to the development of these grabens. After the tectonic activity, other processes reshaped the landscape. In the scene, the results of weathering and mass transport can be seen. Due to erosion, the surface has been smoothed, giving formerly sharp edges a rounded appearance. Such terrain is called "fretted terrain" and is characteristic for the transition of highland to lowland. The valleys and grabens are 5 to 10 kilometres wide and up to 1500 metres deep. Along the graben flanks, the layering of the bedrock is exposed. The lineations on the valley floors are attributed to a slow viscous movement of material, Extensional tectonics in Tempe Terra. presumably in connection with ice. These lineations and indications of possible ice underneath the surface lead scientists to assume that the structures are rock glaciers or similar phenomena These images, taken by the High Resolution known from alpine regions on Earth. Stereo Camera (HRSC) on board ESA's Mars Express spacecraft, show the tectonic 'grabens' in The stereo and colour capabilities, and the high- Tempe Terra, a geologically complex region that is resolution coverage of extended areas, provided by part of the old Martian highlands. the HRSC camera allow for improved study of the complex geologic evolution of the Red Planet. The The HRSC obtained these images during orbit Mars Express HRSC camera gives scientists the 1180 on 19 December 2004 with a ground opportunity to better understand the tectonics of resolution of approximately 16.5 metres per pixel. -
Digital Mapping & Spatial Analysis
Digital Mapping & Spatial Analysis Zach Silvia Graduate Community of Learning Rachel Starry April 17, 2018 Andrew Tharler Workshop Agenda 1. Visualizing Spatial Data (Andrew) 2. Storytelling with Maps (Rachel) 3. Archaeological Application of GIS (Zach) CARTO ● Map, Interact, Analyze ● Example 1: Bryn Mawr dining options ● Example 2: Carpenter Carrel Project ● Example 3: Terracotta Altars from Morgantina Leaflet: A JavaScript Library http://leafletjs.com Storytelling with maps #1: OdysseyJS (CartoDB) Platform Germany’s way through the World Cup 2014 Tutorial Storytelling with maps #2: Story Maps (ArcGIS) Platform Indiana Limestone (example 1) Ancient Wonders (example 2) Mapping Spatial Data with ArcGIS - Mapping in GIS Basics - Archaeological Applications - Topographic Applications Mapping Spatial Data with ArcGIS What is GIS - Geographic Information System? A geographic information system (GIS) is a framework for gathering, managing, and analyzing data. Rooted in the science of geography, GIS integrates many types of data. It analyzes spatial location and organizes layers of information into visualizations using maps and 3D scenes. With this unique capability, GIS reveals deeper insights into spatial data, such as patterns, relationships, and situations - helping users make smarter decisions. - ESRI GIS dictionary. - ArcGIS by ESRI - industry standard, expensive, intuitive functionality, PC - Q-GIS - open source, industry standard, less than intuitive, Mac and PC - GRASS - developed by the US military, open source - AutoDESK - counterpart to AutoCAD for topography Types of Spatial Data in ArcGIS: Basics Every feature on the planet has its own unique latitude and longitude coordinates: Houses, trees, streets, archaeological finds, you! How do we collect this information? - Remote Sensing: Aerial photography, satellite imaging, LIDAR - On-site Observation: total station data, ground penetrating radar, GPS Types of Spatial Data in ArcGIS: Basics Raster vs. -
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. -
Direct-To-Digital Mapping Methodology: a Hands-On Guidebook for Applying Google Earth
Steven DeRoy / The Firelight Group / January 2016 Direct-To-Digital Mapping Methodology: A Hands-on Guidebook for Applying Google Earth Copyright © Steven DeRoy and the Firelight Group (www.thefirelightgroup.com) 1 | Page Table of Contents ACKNOWLEDGEMENTS 4 PURPOSE OF THIS GUIDE 4 PREPARE TO MAP 5 DOWNLOAD AND INSTALL GOOGLE EARTH 5 SET UP YOUR FILE FOLDERS ON YOUR COMPUTER 5 INTERVIEW ROOM SETTING 5 START THE INTERVIEW 5 INTERVIEW CHECK LIST 6 INTERVIEW KIT 6 SET UP GOOGLE EARTH 6 CHECK YOUR EQUIPMENT 6 INFORM THE PARTICIPANT AND MAKE THEM COMFORTABLE 6 BEFORE STARTING THE INTERVIEW 7 REMINDERS DURING THE INTERVIEW 7 INTERVIEW OVERVIEW 8 INTRODUCTIONS 8 MAPPING 8 INTERVIEW 8 STORAGE OF RESULTS 8 MAPPING NOTES 9 OVERVIEW OF GOOGLE EARTH 10 WHAT IS GOOGLE EARTH? 10 WHY USE GOOGLE EARTH? 10 HOW ARE GOOGLE EARTH AND MAPS DIFFERENT? 10 INTRODUCTION TO THE GOOGLE EARTH INTERFACE 11 NAVIGATING IN GOOGLE EARTH 11 SET UP YOUR ENVIRONMENT 12 THE “PLACES” PANEL 13 SET UP FOLDERS TO STORE YOUR DATA 13 ORGANIZE YOUR FOLDERS 14 UNDERSTANDING SCALE 14 Copyright © Steven DeRoy and the Firelight Group (www.thefirelightgroup.com) 2 | Page HOW TO MAP IN GOOGLE EARTH 16 WHAT TO RECORD FOR EACH SITE 16 ADDING POINTS (PLACEMARKS) 16 ADDING LINES (PATHS) 18 ADDING AREAS (POLYGONS) 19 EDITING MAPPED DATA 20 INTERVIEWS CONDUCTED WITH NO MAPPING DATA 20 OVERLAYING DATA FROM PAST STUDIES 21 CLOSING OFF THE INTERVIEW 22 SAVING KMZ FILES 22 COPY AND SAVE ALL DIGITAL AUDIO AND VIDEO FILES TO YOUR LAPTOP/COMPUTER 23 BACKUP YOUR FILES 23 USEFUL RESOURCES 24 Copyright © Steven DeRoy and the Firelight Group (www.thefirelightgroup.com) 3 | Page Acknowledgements Steven DeRoy, Director of the Firelight Group, produced this comprehensive guidebook. -
Glossary of Lunar Terminology
Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites. -
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 -
Digital Mapping Techniques ‘02— Workshop Proceedings
cov02 5/20/03 3:19 PM Page 1 So Digital Mapping Techniques ‘02— Workshop Proceedings May 19-22, 2002 Salt Lake City, Utah Convened by the Association of American State Geologists and the United States Geological Survey Hosted by the Utah Geological Survey U.S. GEOLOGICAL SURVEY OPEN-FILE REPORT 02-370 Printed on recycled paper CONTENTS I U.S. Department of the Interior U.S. Geological Survey Digital Mapping Techniques ʻ02— Workshop Proceedings Edited by David R. Soller May 19-22, 2002 Salt Lake City, Utah Convened by the Association of American State Geologists and the United States Geological Survey Hosted by the Utah Geological Survey U.S. GEOLOGICAL SURVEY OPEN-FILE REPORT 02-370 2002 II CONTENTS CONTENTS III This report is preliminary and has not been reviewed for conformity with the U.S. Geological Survey editorial standards. Any use of trade, product, or firm names in this publication is for descriptive purposes only and does not imply endorsement by the U.S. Government or State governments II CONTENTS CONTENTS III CONTENTS Introduction By David R. Soller (U.S. Geological Survey). 1 Oral Presentations The Value of Geologic Maps and the Need for Digitally Vectorized Data By James C. Cobb (Kentucky Geological Survey) . 3 Compilation of a 1:24,000-Scale Geologic Map Database, Phoenix Metropoli- tan Area By Stephen M. Richard and Tim R. Orr (Arizona Geological Survey). 7 Distributed Spatial Databases—The MIDCARB Carbon Sequestration Project By Gerald A. Weisenfluh (Kentucky Geological Survey), Nathan K. Eaton (Indiana Geological Survey), and Ken Nelson (Kansas Geological Survey) . -
Digital Geologic Mapping Methods
INTERNATIONAL JOURNAL OF GEOLOGY Issue 3, Volume 2, 2008 Digital geologic mapping methods: from field to 3D model M. De Donatis, S. Susini and G. Delmonaco Abstract—Classical geologic mapping is one of the main techniques software 2DMove and 3DMove by Midland Valley Exploration Ltd. used in geology where pencils, paper base map and field book are the This paper reports a case study of digital mapping carried out in traditional tools of field geologists. In this paper, we describe a new the Southern Apennines. This work is part of an ENEA project, method of digital mapping from field work to buiding three funded by the Italian Ministry of University and Research, devoted to dimensional geologic maps, including GIS maps and geologic cross- heritage sites prone to landslide risk where local-scale geologic and sections. The project consisted of detailed geologic mapping of the geomorphic mapping is fundamental in the preliminary stage of the are of Craco village (Matera - Italy). The work started in the lab by project. implementing themes for defining a cartographic base (aerial photos, topographic and geologic maps) and for field work (developing II. Study area symbols for outcrops, dip data, boundaries, faults, and landslide The study area (Fig. 1) is located in the Southern Apennines, types). Special prompts were created ad hoc for data collection. All around Craco, a small village in the Matera Province along a ridge data were located or mapped through GPS. It was possible to easily between the Bruscata and Salandrella stream. store any types of documents (digital pictures, notes, and sketches), linked to an object or a geo-referenced point. -
Origin of the Anomalously Rocky Appearance of Tsiolkovskiy Crater
Icarus 273 (2016) 237–247 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Origin of the anomalously rocky appearance of Tsiolkovskiy crater ∗ Benjamin T. Greenhagen a, , Catherine D. Neish b, Jean-Pierre Williams c, Joshua T.S. Cahill a, Rebecca R. Ghent d,e,PaulO. Hayne f, Samuel J. Lawrence g,NoahE. Petro h, Joshua L. Bandfield i a Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099, United States b Department of Earth Sciences, Western University Biological & Geological Sciences Building, Room 1026 1151 Richmond St. N. London, ON N6A 5B7 Canada c Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles 595 Charles Young Drive East, Box 951567 Los Angeles, CA 90095-1567, United States d Department of Earth Sciences, Earth Sciences Centre 22 Russell Street Toronto, Ontario, M5S 3B1, Canada e Planetary Science Institute, 1700 East Fort Lowell, Suite 106 Tucson, AZ 85719-2395, United States f Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive Pasadena, CA 91109 ASU, United States g School of Earth and Space Exploration, PO Box 871404 Tempe, AZ 85287-1404, United States h NASA’s Goddard Space Flight Center, 8800 Greenbelt Rd Greenbelt, MD 20771, United States i Space Science Institute, 4750 Walnut Street | Suite 205 Boulder, Colorado 80301, United States a r t i c l e i n f o a b s t r a c t Article history: Rock abundance maps derived from the Diviner Lunar Radiometer instrument on the Lunar Reconnais- Received 3 August 2015 sance Orbiter (LRO) show Tsiolkovskiy crater to have high surface rock abundance and relatively low re- Revised 6 February 2016 golith thickness. -
Adams Adkinson Aeschlimann Aisslinger Akkermann
BUSCAPRONTA www.buscapronta.com ARQUIVO 27 DE PESQUISAS GENEALÓGICAS 189 PÁGINAS – MÉDIA DE 60.800 SOBRENOMES/OCORRÊNCIA Para pesquisar, utilize a ferramenta EDITAR/LOCALIZAR do WORD. A cada vez que você clicar ENTER e aparecer o sobrenome pesquisado GRIFADO (FUNDO PRETO) corresponderá um endereço Internet correspondente que foi pesquisado por nossa equipe. Ao solicitar seus endereços de acesso Internet, informe o SOBRENOME PESQUISADO, o número do ARQUIVO BUSCAPRONTA DIV ou BUSCAPRONTA GEN correspondente e o número de vezes em que encontrou o SOBRENOME PESQUISADO. Número eventualmente existente à direita do sobrenome (e na mesma linha) indica número de pessoas com aquele sobrenome cujas informações genealógicas são apresentadas. O valor de cada endereço Internet solicitado está em nosso site www.buscapronta.com . Para dados especificamente de registros gerais pesquise nos arquivos BUSCAPRONTA DIV. ATENÇÃO: Quando pesquisar em nossos arquivos, ao digitar o sobrenome procurado, faça- o, sempre que julgar necessário, COM E SEM os acentos agudo, grave, circunflexo, crase, til e trema. Sobrenomes com (ç) cedilha, digite também somente com (c) ou com dois esses (ss). Sobrenomes com dois esses (ss), digite com somente um esse (s) e com (ç). (ZZ) digite, também (Z) e vice-versa. (LL) digite, também (L) e vice-versa. Van Wolfgang – pesquise Wolfgang (faça o mesmo com outros complementos: Van der, De la etc) Sobrenomes compostos ( Mendes Caldeira) pesquise separadamente: MENDES e depois CALDEIRA. Tendo dificuldade com caracter Ø HAMMERSHØY – pesquise HAMMERSH HØJBJERG – pesquise JBJERG BUSCAPRONTA não reproduz dados genealógicos das pessoas, sendo necessário acessar os documentos Internet correspondentes para obter tais dados e informações. DESEJAMOS PLENO SUCESSO EM SUA PESQUISA. -
Digital Earth Based on Metadata Electronic Maps Standard
DIGITAL EARTH BASED ON METADATA ELECTRONIC MAPS STANDARD Alexander Martynenko 2 build., 44, Vavilova st., Moscow, 117333, Russia, Institute of Informatics Problems, Russian Academy of Sciences, [email protected] Digital Earth was at the center of attention at 19th International Cartographic Conference (Ottawa) and 1st International Symposium on Digital Earth (Beijing) in 1999 [1, 2]. The discussion raised in the papers on the theory of Metadata Standard Systems that could be used in International and National Spatial Information Infrastructures to establish Digital Earth still continues. We highly appreciate the essential contribution made by Chinese scientists: Zhao Yongping, Huang Fang, Guo Jingjun, Feng Quan, Cui Weihong. Since 1990s the Information Society is being created in Russia. Each member of this Society will be able to obtain complete and actual information, including geoinformation, in any point of geographical space, by means of Internet. Today it is obvious that this problem could be solved in most effective way by using electronic libraries of various intent, including electronic map libraries. Completeness, methods and form of geoinformation, temporal factors of the information supply can be considered as the main criteria for evaluating quality of the electronic geoinformation resources. In the process of creating the electronic geoinformation resources, standardization in the area of geoinformation technologies plays the main role. Today, at the boundary of millennia, the Global Geoinformatic Mapping (GGM) appears as the prior direction of scientific and technical progress. Its goal is the cartographic representation of the real world and creation of the global computer model of the Earth, comprised of millions of space images and electronic maps of various subjects and scales, themes and also reference information [3, 4]. -
Ogdc)—Release 6
State of Oregon Oregon Department of Geology and Mineral Industries Ian P. Madin, Interim State Geologist README FILE FOR OREGON GEOLOGIC DATA COMPILATION (OGDC)—RELEASE 6 by Rachel L. Smith1 and Warren P. Roe1 2015 1 Formerly with Oregon Department of Geology and Mineral Industries, 800 NE Oregon St., Ste. 965, Portland, OR 97015 Oregon Geologic Data Compilation Release 6 DISCLAIMER This product is for informational purposes and may not have been prepared for or be suitable for legal, engineering, or surveying purposes. Users of this information should review or consult the primary data and information sources to ascertain the usability of the information. This publication cannot substitute for site-specific investigations by qualified practitioners. Site-specific data may give results that differ from the results shown in the publication. Spatial inaccuracies exist in this data set, and some functionalities of Oregon Geologic Data Compilation have changed from previous versions due to the transition to an Esri®-formatted geodatabase. Known issues include topology errors, small spatial data gaps, typographical errors, incomplete metadata, and other minor errors. Oregon Department of Geology and Mineral Industries | Oregon Geologic Data Compilation, release 6 Published in conformance with ORS 516.030 For additional information: Administrative Offices 800 NE Oregon Street #28, Suite 965 Portland, OR 97232 Telephone (971) 673-1555 Fax (971) 673-1562 http://www.oregongeology.org http://egov.oregon.gov/DOGAMI/ Oregon Department of Geology