The Casella Sensitive Anemometer Micrometeorological Measurements
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A Possible Albian Impact Crater at Murshid, Southern Oman
GeoArabia, Vol. 7, No. 4, 2002 Gulf PetroLink, Bahrain A possible Albian impact crater at Murshid, southern Oman Bruce Levell1, Pascal Richard2 and Folco Hoogendijk2, Petroleum Development Oman ABSTRACT During interpretation of a 3-D seismic survey in southern Oman a solitary, 2.5-km-wide circular basin with a central peak and raised rim was identified in the subsurface 35 km west of the Marmul oil field. The feature is the only one of its kind in the area. The basinal structure is probably of Late Cretaceous (Albian) age and the regional geology strongly suggests that it is neither a volcanic crater nor related to salt-dome tectonics or salt dissolution. It possibly represents a crater formed by a terrestrial impact event and has been named the Murshid crater. This report does not constitute a detailed investigation of the possible impact crater but rather records the 3-D seismic observations and the drilling that has taken place near the structure so far. INTRODUCTION During interpretation of a newly acquired 3-D seismic survey for oil exploration in southern Oman, a solitary 2.5-km-diameter circular basinal feature was identified as a possible impact structure and was named the Murshid crater. It lies 35 km west of the Marmul oil field in the South Oman Salt Basin (Figure 1). The center of the structure is at latitude 18º10’59"N, longitude 54º55’08”E, and it is buried at a depth of approximately 380 m below mean sea level (680 m below the ground surface). The authors are petroleum geologists who felt that the Murshid basinal structure needed reporting to the wider scientific community. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Naval Juniorreserve ()Hiders
DOCUMENT RESUME ED 219 280 SE 038 787 e $ . AUTHOR ' Omans, S. E.; And Others TITLE Workbook for Naval Science 3: An Illustrated Workbook for the NJROTC Sjudent. Focus. on the Trained Person. Technical Report 124. INSTITUTION University of Central Florida, Orlando.. -, SPONS AGENCY Naval %Training Analysis and Evaluation Group, Orlando, Fla. PUB DATE May f2 GRANT N61339-79-D-0105 4 NOTE if 348p.- 4 ,EDRS PRICE MF01/PC14 Plus Postage. DESCRIPTORS Astronomy; Electricity; High Schools; Instructional -Materials; *Leadership; Meteotiology; Military Science; *Military Training; *Physical Sciences; ( *Remedial Reading; *Secondary School Science; Workbooks' _ IDENTIFIERS Navaleistory; *Naval JuniorReserve ()Hiders . ,-..\ Traiffing torps , '-'--..... ..,. ABSTRACT This workbook (first in a series of three) - supplements the textbook of the third year Naval Junior Reserve Officers Training Corps (NJROTC),program and is designed for NJROTC students who do not have the reading skillsOlecessary to fully benefit from the regular curriculum materidls. The workbook is written at the eighth-grade readability level as detprmined by a Computer Readability Editing System'analysis. In addition to its use in the NJROTC program, the wdrkbook may be useful in 'several remedial programs such as Academic Remedial Training(ART) and;the Verbal' Skills Curriculum,\Jzoth of which are offered at each 'of the three . RecruitTraining Com?nands to recruits deficient in reading or oral English skills.' Topics' in the workbook include naval history (1920-1945), leadership.characteristiCs, meteorology, astronomy, sand introductory electricity.'Exercises-include'vocabulary development, matching, concept application, and -extending Yearning actrties. (Author/JN) V 1' ****************************.0***,*************************************** * * Reproductions suppled'bi EDRS are the best that can be made. from- the oryiginal% document. -
A Study About the Temporal Constraints on the Martian Yardangs’ Development in Medusae Fossae Formation
remote sensing Article A Study about the Temporal Constraints on the Martian Yardangs’ Development in Medusae Fossae Formation Jia Liu 1,2 , Zongyu Yue 1,3,*, Kaichang Di 1,3 , Sheng Gou 1,4 and Shengli Niu 4 1 State Key Laboratory of Remote Sensing Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100101, China; [email protected] (J.L.); [email protected] (K.D.); [email protected] (S.G.) 2 University of Chinese Academy of Sciences, Beijing 100049, China 3 CAS Center for Excellence in Comparative Planetology, Hefei 230026, China 4 State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau 999078, China; [email protected] * Correspondence: [email protected]; Tel.: +86-10-64889553 Abstract: The age of Mars yardangs is significant in studying their development and the evolution of paleoclimate conditions. For planetary surface or landforms, a common method for dating is based on the frequency and size distribution of all the superposed craters after they are formed. However, there is usually a long duration for the yardangs’ formation, and they will alter the superposed craters, making it impossible to give a reliable dating result with the method. An indirect method by analyzing the ages of the superposed layered ejecta was devised in the research. First, the layered ejecta that are superposed on and not altered by the yardangs are identified and mapped. Then, the ages of the layered ejecta are derived according to the crater frequency and size distribution on them. These ages indicate that the yardangs ceased development by these times, and the ages are valuable for studying the evolution of the yardangs. -
Pre-Mission Insights on the Interior of Mars Suzanne E
Pre-mission InSights on the Interior of Mars Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, Ulrich Christensen, Véronique Dehant, Mélanie Drilleau, William Folkner, Nobuaki Fuji, et al. To cite this version: Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, et al.. Pre-mission InSights on the Interior of Mars. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.1-72. 10.1007/s11214-018-0563-9. hal-01990798 HAL Id: hal-01990798 https://hal.archives-ouvertes.fr/hal-01990798 Submitted on 23 Jan 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is an author's version published in: https://oatao.univ-toulouse.fr/21690 Official URL : https://doi.org/10.1007/s11214-018-0563-9 To cite this version : Smrekar, Suzanne E. and Lognonné, Philippe and Spohn, Tilman ,... [et al.]. Pre-mission InSights on the Interior of Mars. (2019) Space Science Reviews, 215 (1). -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
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 -
Carnegie Institution of Washington Monograph Series
BTILL UMI Carnegie Institution of Washington Monograph Series BT ILL UMI 1 The Carnegie Institution of Washington, D. C. 1902. Octavo, 16 pp. 2 The Carnegie Institution of Washington, D. C. Articles of Incorporation, Deed of Trust, etc. 1902. Octavo, 15 pp. 3 The Carnegie Institution of Washington, D. C. Proceedings of the Board of Trustees, January, 1902. 1902. Octavo, 15 pp. 4 CONARD, HENRY S. The Waterlilies: A Monograph of the Genus Nymphaea. 1905. Quarto, [1] + xiii + 279 pp., 30 pls., 82 figs. 5 BURNHAM, S. W. A General Catalogue of Double Stars within 121° of the North Pole. 1906. Quarto. Part I. The Catalogue. pp. [2] + lv + 1–256r. Part II. Notes to the Catalogue. pp. viii + 257–1086. 6 COVILLE, FREDERICK VERNON, and DANIEL TREMBLY MACDOUGAL. Desert Botani- cal Laboratory of the Carnegie Institution. 1903. Octavo, vi + 58 pp., 29 pls., 4 figs. 7 RICHARDS, THEODORE WILLIAM, and WILFRED NEWSOME STULL. New Method for Determining Compressibility. 1903. Octavo, 45 pp., 5 figs. 8 FARLOW, WILLIAM G. Bibliographical Index of North American Fungi. Vol. 1, Part 1. Abrothallus to Badhamia. 1905. Octavo, xxxv + 312 pp. 9 HILL, GEORGE WILLIAM, The Collected Mathematical Works of. Quarto. Vol. I. With introduction by H. POINCARÉ. 1905. xix + 363 pp. +errata, frontispiece. Vol. II. 1906. vii + 339 pp. + errata. Vol. III. 1906. iv + 577 pp. Vol. IV. 1907. vi + 460 pp. 10 NEWCOMB, SIMON. On the Position of the Galactic and Other Principal Planes toward Which the Stars Tend to Crowd. (Contributions to Stellar Statistics, First Paper.) 1904. Quarto, ii + 32 pp. -
5648 Village of Warsaw Vlge SWIS Code - 564801
NYS - Real Property System Cross Reference Report - 2021 - Current Year File RPS345/V04/L001 County of Wyoming Parcel Address Sequence Town of Warsaw - 5648 Village of Warsaw Vlge SWIS Code - 564801 Location School Res Pr O R T Parcel Id Name Nbr Name Dist Land Av Total Av Pct Cl C S S C 648.1-9999-131.600/1004 NYS Electric & Gas Corp 564801 0309831 0 882 6 648.1-9999-131.600/1014 NYS Electric & Gas Corp 564801 062572 0 882 6 85.16-1-8 Town Of Warsaw Allen St 564801 61006100 0 653 8 A 85.12-1-30.1 Buzz & Val Properties Inc Allen St 564801 2560028100 0 449 1 A 85.12-1-37 Gott, Donald James Estate. Allen St 564801 1440014400 0 340 1 A 85.12-1-27 Williams, Richard A. 6 Allen St 564801 960034000 0 210 1 A 85.12-2-50 Purdy, Larry L. 21 Allen St 564801 870075000 0 210 1 A 85.12-2-49 Mayer, Cory 25 Allen St 564801 1240055300 0 210 1 A 85.12-2-48 Schneider, Daryl A. 29 Allen St 564801 1710051700 0 210 1 A 85.12-2-47 Skidmore, Benjamine J. 37 Allen St 564801 1320055600 0 210 1 A 85.12-2-46 Vickers, II, Kevin M. 41 Allen St 564801 1240060700 0 220 1 A 85.12-2-45 Hampton, Charlotte 45 Allen St 564801 1240060600 0 210 1 A 85.12-2-44 Bernard, Marjorie A. 49 Allen St 564801 1160049500 50 210 1 A 85.12-3-20 Berkemeier, Jeremy B. -
Luther College Catalog 2010–11 Decorah, Iowa Record 2009–10, Announcements 2010–11
Luther College Catalog 2010–11 Decorah, Iowa Record 2009–10, Announcements 2010–11 The college published its first catalog in 1872—Katalog for det norske Luther - college i Decorah, Iowa, 1861- 1872. It was prepared by [President Laur.] Larsen and ran to 48 pages. It contained a list of officials and faculty members, a history of the college, an outline and a defense of the plan and courses of instruction, a section on discipline and school regulations, and a detailed listing of students at the college from the time of its founding. Larsen’s precise scholarship is apparent on every page. Not until 1883 was a second catalog published, this time in English. —from Luther College 1861–1961, pp. 113-114, by David T. Nelson EQUAL OPPORTUNITY: It is the policy of Luther College to provide equal educational opportunities and equal access to facilities for all qualified persons.The college does not discriminate in employment, educational programs, and activities on the basis of age, color, creed, disability, gender identity, genetic information, national origin, race, religion, sex, sexual orientation, veteran status, or any other basis protected by federal or state law. The provisions of this catalog do not constitute an irrevocable contract between the student and the college. The college reserves the right to change any provision or requirement at any time during the student’s term of residence. Contents Introducing Luther ........................................................ 5 An Overview of Luther College ....................................................6 -
Donald Langmead
FRANK LLOYD WRIGHT: A Bio-Bibliography Donald Langmead PRAEGER FRANK LLOYD WRIGHT Recent Titles in Bio-Bibliographies in Art and Architecture Paul Gauguin: A Bio-Bibliography Russell T. Clement Henri Matisse: A Bio-Bibliography Russell T. Clement Georges Braque: A Bio-Bibliography Russell T. Clement Willem Marinus Dudok, A Dutch Modernist: A Bio-Bibliography Donald Langmead J.J.P Oud and the International Style: A Bio-Bibliography Donald Langmead FRANK LLOYD WRIGHT A Bio-Bibliography Donald Langmead Bio-Bibliographies in Art and Architecture, Number 6 Westport, Connecticut London Library of Congress Cataloging-in-Publication Data Langmead, Donald. Frank Lloyd Wright : a bio-bibliography / Donald Langmead. p. cm.—(Bio-bibliographies in art and architecture, ISSN 1055-6826 ; no. 6) Includes bibliographical references and indexes. ISBN 0–313–31993–6 (alk. paper) 1. Wright, Frank Lloyd, 1867–1959—Bibliography. I. Title. II. Series. Z8986.3.L36 2003 [NA737.W7] 016.72'092—dc21 2003052890 British Library Cataloguing in Publication Data is available. Copyright © 2003 by Donald Langmead All rights reserved. No portion of this book may be reproduced, by any process or technique, without the express written consent of the publisher. Library of Congress Catalog Card Number: 2003052890 ISBN: 0–313–31993–6 ISSN: 1055–6826 First published in 2003 Praeger Publishers, 88 Post Road West, Westport, CT 06881 An imprint of Greenwood Publishing Group, Inc. www.praeger.com Printed in the United States of America The paper used in this book complies with the -
NASA Goddard Space Flight Center, Greenbelt, MD Contact: [email protected]
Updated Catalogs of Peak-Ring Basins and Protobasins on Mars David M.H. Baker; NASA Goddard Space Flight Center, Greenbelt, MD Contact: [email protected] A catalog of craters ≥1 km on Mars from Robbins et al. [2] was used to survey all craters >50 km on the planet (N=2,070) in a manner similar to [5,6] for the Moon and Mercury. Motivation: II. Basin Images Datasets used included MOLA gridded topography and a global THEMIS daytime IR mosaic [7]. During the survey, each crater was identified as having a rim crest in addition to a single interior ring of peaks (peak-ring basin), an interior ring of peaks plus a central peak (protobasin), a central peak only (complex crater), or no interior structure (unclassified). • The morphology of peak-ring basins (exhibiting a rim crest and interior peak Schiaparelli; 446 km Schroeter; 292 km Galle; 223 km Kepler; 222 km Secchi; 217 km Kaiser; 202 km Lowell; 199 km Phillips; 185 km ring) in the complex crater to basin transition on the Moon and Mercury have been well characterized based on data from recent missions to these planetary bodies [e.g., 1]. • Although global crater catalogs have recently been produced for Mars [e.g., 2], the detailed characteristics of the crater to basin transition on Mars has not been fully re-examined since basin ring catalogs and measurements were produced over two decades ago by Pike and Spudis [3], among others. • Here, previous basin catalogs [3] and the global crater catalog of Robbins Unnamed; 180 km Molesworth; 175 km Proctor; 167 km Becquerel; 165 km Ptolemaeus; 165 km Dejnev 152 km Unnamed; 103 km Mie; 101 km et al.