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A Preliminary Report of the Battle of the Crater, 30 July 1864
Holding the Line A Preliminary Report of The Battle of the Crater 30 July 1864 Adrian Mandzy, Ph. D. Michelle Sivilich, Ph. D. Benjamin Lewis Fitzpatrick, Ph. D. Dan Sivilich Floyd Patrick Davis Kelsey P. Becraft Dakota Leigh Goedel Jeffrey A. McFadden Jessey C. Reed Jaron A. Rucker A PRELIMINARY REPORT ON THE SURVEY OF THE BATTLE OF THE CRATER, 30 JULY 1864 By Adrian Mandzy, Ph.D., Michelle Sivilich, Ph. D., Floyd Patrick Davis, Kelsey P. Becraft, Dakota Leigh Goedel, Jeffrey A. McFadden, Jessey C. Reed, and Jaron A. Rucker With a Contributions by Daniel Sivilich and Dr. Benjamin Lewis Fitzpatrick Report prepared for the Northeast Region Archeology Program National Park Service 115 John Street, 4th Floor Lowell, Massachusetts 01852-1195 _______________________________ Adrian Mandzy Principal Investigator ARPA Permit 2014.PETE.01 2 Abstract In March 2015, faculty and students from Morehead State University’s History program, along with members of the Battlefield Restoration and Archeological Volunteer Organization (BRAVO) conducted a survey of The Crater Battlefield. Fought on 30 July 1864, during the Siege of Petersburg, the Battle of the Crater, according to the National Park Service, is one of the most important events of the Civil War. The participation of African-American troops in the battle and the subsequent execution of black prisoners highlights the racial animosities that were the underpinning causes of this conflict. The goal of this project is to document the level of integrity of any archaeological resources connected with this field of conflict and to examine how far the Union troops advance beyond the mouth of the Crater. -
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GEOLOGIC MAPPING OF THE LUNAR SOUTH POLE QUADRANGLE (LQ-30). S.C. Mest1,2, D.C. Ber- man1, and N.E. Petro2, 1Planetary Science Institute, 1700 E. Ft. Lowell, Suite 106, Tucson, AZ 85719-2395 ([email protected]); 2Planetary Geodynamics Laboratory, Code 698, NASA GSFC, Greenbelt, MD 20771. Introduction: In this study we use recent image, the surface [7]. Impact craters display morphologies spectral and topographic data to map the geology of the ranging from simple to complex [7-9,24] and most lunar South Pole quadrangle (LQ-30) at 1:2.5M scale contain floor deposits distinct from surrounding mate- [1-7]. The overall objective of this research is to con- rials. Most of these deposits likely consist of impact strain the geologic evolution of LQ-30 (60°-90°S, 0°- melt; however, some deposits, especially on the floors ±180°) with specific emphasis on evaluation of a) the of the larger craters and basins (e.g., Antoniadi), ex- regional effects of impact basin formation, and b) the hibit low albedo and smooth surfaces and may contain spatial distribution of ejecta, in particular resulting mare. Higher albedo deposits tend to contain a higher from formation of the South Pole-Aitken (SPA) basin density of superposed impact craters. and other large basins. Key scientific objectives in- Antoniadi Crater. Antoniadi crater (D=150 km; clude: 1) Determining the geologic history of LQ-30 69.5°S, 172°W) is unique for several reasons. First, and examining the spatial and temporal variability of Antoniadi is the only lunar crater that contains both a geologic processes within the map area. -
Of Vertebrate Fossils from the Middle Eocene Oil Shale of Messel, Germany: Implications for Their Taphonomy and Palaeoenvironment
Palaeogeography, Palaeoclimatology, Palaeoecology 416 (2014) 92–109 Contents lists available at ScienceDirect Palaeogeography, Palaeoclimatology, Palaeoecology journal homepage: www.elsevier.com/locate/palaeo Isotope compositions (C, O, Sr, Nd) of vertebrate fossils from the Middle Eocene oil shale of Messel, Germany: Implications for their taphonomy and palaeoenvironment Thomas Tütken ⁎ Steinmann-Institut für Geologie, Mineralogie und Paläontologie, Universität Bonn, Poppelsdorfer Schloss, 53115 Bonn, Germany article info abstract Article history: The Middle Eocene oil shale deposits of Messel are famous for their exceptionally well-preserved, articulated 47- Received 15 April 2014 Myr-old vertebrate fossils that often still display soft tissue preservation. The isotopic compositions (O, C, Sr, Nd) Received in revised form 30 July 2014 were analysed from skeletal remains of Messel's terrestrial and aquatic vertebrates to determine the condition of Accepted 5 August 2014 geochemical preservation. Authigenic phosphate minerals and siderite were also analysed to characterise the iso- Available online 17 August 2014 tope compositions of diagenetic phases. In Messel, diagenetic end member values of the volcanically-influenced 12 Keywords: and (due to methanogenesis) C-depleted anoxic bottom water of the meromictic Eocene maar lake are isoto- Strontium isotopes pically very distinct from in vivo bioapatite values of terrestrial vertebrates. This unique taphonomic setting al- Oxygen isotopes lows the assessment of the geochemical preservation of the vertebrate fossils. A combined multi-isotope Diagenesis approach demonstrates that enamel of fossil vertebrates from Messel is geochemically exceptionally well- Enamel preserved and still contains near-in vivo C, O, Sr and possibly even Nd isotope compositions while bone and den- Messel tine are diagenetically altered. -
Geoscience and a Lunar Base
" t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history. -
Confronting Antisemitism in Modern Media, the Legal and Political Worlds an End to Antisemitism!
Confronting Antisemitism in Modern Media, the Legal and Political Worlds An End to Antisemitism! Edited by Armin Lange, Kerstin Mayerhofer, Dina Porat, and Lawrence H. Schiffman Volume 5 Confronting Antisemitism in Modern Media, the Legal and Political Worlds Edited by Armin Lange, Kerstin Mayerhofer, Dina Porat, and Lawrence H. Schiffman ISBN 978-3-11-058243-7 e-ISBN (PDF) 978-3-11-067196-4 e-ISBN (EPUB) 978-3-11-067203-9 DOI https://10.1515/9783110671964 This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. For details go to https://creativecommons.org/licenses/by-nc-nd/4.0/ Library of Congress Control Number: 2021931477 Bibliographic information published by the Deutsche Nationalbibliothek The Deutsche Nationalbibliothek lists this publication in the Deutsche Nationalbibliografie; detailed bibliographic data are available on the Internet at http://dnb.dnb.de. © 2021 Armin Lange, Kerstin Mayerhofer, Dina Porat, Lawrence H. Schiffman, published by Walter de Gruyter GmbH, Berlin/Boston The book is published with open access at www.degruyter.com Cover image: Illustration by Tayler Culligan (https://dribbble.com/taylerculligan). With friendly permission of Chicago Booth Review. Printing and binding: CPI books GmbH, Leck www.degruyter.com TableofContents Preface and Acknowledgements IX LisaJacobs, Armin Lange, and Kerstin Mayerhofer Confronting Antisemitism in Modern Media, the Legal and Political Worlds: Introduction 1 Confronting Antisemitism through Critical Reflection/Approaches -
Muslim Scientists and Thinkers
MUSLIM SCIENTISTS AND THINKERS Syed Aslam Second edition 2010 Copyright 2010 by Syed Aslam Publisher The Muslim Observer 29004 W. Eight Mile Road Farmington, MI 48336 Cover Statue of Ibn Rushd Cordoba, Spain ISBN 978-1-61584-980-2 Printed in India Lok-Hit Offset Shah-e-Alam Ahmedabad Gujarat ii Dedicated to Ibn Rushd and other Scientists and Thinkers of the Islamic Golden Age iii CONTENTS Acknowledgments ................................................VI Foreword .............................................................VII Introduction ..........................................................1 1 Concept of Knowledge in Islam ............................8 2 Abu Musa Jabir Ibn Hayyan..................................25 3 Al-Jahiz abu Uthman Ibn Bahar ...........................31 4 Muhammad Ibn Musa al-Khwarizmi....................35 5 Abu Yaqoub Ibn Ishaq al-Kindi ............................40 6 Muhammad bin Zakaria Razi ...............................45 7 Jabir ibn Sinan al-Batani.......................................51 8 Abu Nasar Mohammad ibn al-Farabi....................55 9 Abu Wafa ibn Ismail al-Buzjani ...........................61 10 Abu Ali al-Hasan ibn al-Haytham .......................66 11 Abu Rayhan ibn al-Biruni ....................................71 12 Ali al-Hussain ibn Sina ........................................77 13 Abu Qasim ibn al-Zahrawi ..................................83 iv 14 Omar Khayyam ...................................................88 15 Abu Hamid al-Ghazali .........................................93 -
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 -
Diamond Craters Oregon's Geologic
Text by Ellen M. Benedict, 1985 Features at stops correspond to points on a clock ago, a huge mass of hot gases, volcanic ashes, bits face. Imagine that you are standing in the middle of a of pumice and other pyroclastics (fire-broken rock) Travel And Hiking Hints clock face. Twelve o’clock is the road in front of you violently erupted. The blast – greater than the May and 6 o’clock the road behind. If you always align the 18, 1980, eruption of Mt. St. Helens – deposited a Diamond Craters is located in the high desert country clock face with the road, you should be able to locate layer of pyroclastics 30 to 130 feet thick over an area about 55 miles southeast of Burns, Oregon. It’s an the features. almost 7,000 square miles! isolated place and some precautions should be taken . when traveling in the area. Start Tour. Mileage begins halfway Pyroclastics are between milepost 40 and 41 on State normal behavior Diamond Craters has no tourist facilities. The nearest Highway 205 at the junction to Diamond. for magmas place where gasoline is sold is at Frenchglen. Turn left. (subsurface That’s the opinion held by scores of molten rocks) Keep your scientists and educators who have visited Diamond, Oregon, a small ranching community, was of rhyolitic (a vehicle on named in 1874 for Mace McCoy’s Diamond brand. volcanic material and studied the area. It has the “best and hard-packed The nearby craters soon became known as Diamond related to granite) most diverse basaltic volcanic features in the road surfaces Craters. -
Discoveries of Mass Independent Isotope Effects in the Solar System: Past, Present and Future Mark H
Reviews in Mineralogy & Geochemistry Vol. 86 pp. 35–95, 2021 2 Copyright © Mineralogical Society of America Discoveries of Mass Independent Isotope Effects in the Solar System: Past, Present and Future Mark H. Thiemens Department of Chemistry and Biochemistry University of California San Diego La Jolla, California 92093 USA [email protected] Mang Lin State Key Laboratory of Isotope Geochemistry Guangzhou Institute of Geochemistry, Chinese Academy of Sciences Guangzhou, Guangdong 510640 China University of Chinese Academy of Sciences Beijing 100049 China [email protected] THE BEGINNING OF ISOTOPES Discovery and chemical physics The history of the discovery of stable isotopes and later, their influence of chemical and physical phenomena originates in the 19th century with discovery of radioactivity by Becquerel in 1896 (Becquerel 1896a–g). The discovery catalyzed a range of studies in physics to develop an understanding of the nucleus and the properties influencing its stability and instability that give rise to various decay modes and associated energies. Rutherford and Soddy (1903) later suggested that radioactive change from different types of decay are linked to chemical change. Soddy later found that this is a general phenomenon and radioactive decay of different energies and types are linked to the same element. Soddy (1913) in his paper on intra-atomic charge pinpointed the observations as requiring the observations of the simultaneous character of chemical change from the same position in the periodic chart with radiative emissions required it to be of the same element (same proton number) but differing atomic weight. This is only energetically accommodated by a change in neutrons and it was this paper that the name “isotope” emerges. -
1 2.6 Physical Chemistry and Thermal Evolution of Ices at Ganymede 1 C
1 1 2.6 Physical Chemistry and Thermal Evolution of Ices at Ganymede 2 C. Ahrens, NASA Goddard Space Flight Center, Greenbelt, MD; [email protected] 3 A. Solomonidou, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA; & LEISA 4 – Observatoire de Paris, CNRS, UPMC Univ., Paris 06, Univ. Paris-Diderot, Meudon, France; 5 [email protected] 6 K. Stephan, Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany; 7 [email protected] 8 K. Kalousova, Charles University, Faculty of Mathematics and Physics, Department of Geophysics, 9 Prague, Czech Republic; [email protected] 10 N. Ligier, Institut d’Astrophysique Spatiale, Université Paris-Saclay, Orsay, France; 11 [email protected] 12 T. McCord, Bear Fight Institute, Winthrop, WA; [email protected] 13 C. Hibbitts, Applied Physics Laboratory, Johns Hopkins University, Laurel, MD; 14 [email protected] 15 16 Abstract 17 18 Ganymede’s surface is composed mostly of water ice and other icy materials in addition to minor non-ice 19 components. The formation and evolution of Ganymede’s landforms highly depend on the nature of the 20 icy materials as they present various thermal and rheological behaviors. This chapter reviews the 21 currently known thermodynamic parameters of the ice phases and hydrates reported on Ganymede, which 22 seem to affect the evolution of the surface, using mainly results from the Voyager and Galileo missions. 23 24 Keywords: Ganymede; Ices; Ices, Mechanical Properties; Experimental techniques; Geological 25 processes 26 27 1 Introduction 28 29 Icy bodies of the outer solar system, including satellites of the gas giants, harbor surface ices made of 30 volatile molecules, clathrates, and complex molecules like hydrocarbons. -
Board Certified Fellows
AMERICAN BOARD OF MEDICOLEGAL DEATH INVESTIGATORS Certificant Directory As of September 30, 2021 BOARD CERTIFIED FELLOWS Addison, Krysten Leigh (Inactive) BC2286 Allmon, James L. BC855 Travis County Medical Examiner's Office Sangamon County Coroner's Office 1213 Sabine Street 200 South 9th, Room 203 PO Box 1748 Springfield, IL 62701 Austin, TX 78767 Amini, Navid BC2281 Appleberry, Sherronda BC1721 Olmsted Medical Examiner's Office Adams and Broomfield County Office of the Coroner 200 1st Street Southwest 330 North 19th Avenue Rochester, MN 55905 Brighton, CO 80601 Applegate, MD, David T. BC1829 Archer, Meredith D. BC1036 Union County Coroner's Office Mohave County Medical Examiner 128 South Main Street 1145 Aviation Drive Unit A Marysville, OH 43040 Lake Havasu, AZ 86404 Bailey, Ted E. (Inactive) BC229 Bailey, Sanisha Renee BC1754 Gwinnett County Medical Examiner's Office Virginia Office of the Chief Medical Examiner 320 Hurricane Shoals Road, NE Central District Lawrenceville, GA 30046 400 East Jackson Street Richmond, VA 23219 Balacki, Alexander J BC1513 Banks, Elsie-Kay BC3039 Montgomery County Coroner's Office Maine Office of the Chief Medical Examiner 1430 Dekalb Street 30 Hospital Street PO Box 311 Augusta, ME 04333 Norristown, PA 19404 Bautista, Ian BC2185 Bayer, Lindsey A. BC875 New York City Office of Chief Medical Examiner District 5 and 24 Medical Examiner Office 421 East 26th Street 809 Pine Street New York, NY 10016 Leesburg, FL 34756 Beck, Shari L BC327 Beckham, Phinon Phillips BC2305 Sedgwick Co Reg. Forensic Science Center Virginia Office of the Chief Medical Examiner 1109 N. Minneapolis Northern District Wichita, KS 67214 10850 Pyramid Place, Suite 121 Manassas, VA 20110 Bednar Keefe, Gale M. -
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.