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500-Year-Old Sturgeon Found in Danish Royal Shipwreck
12 Established 1961 Lifestyle Features Sunday, September 6, 2020 An Italian military attache stands as Swiss President Simonetta Sommaruga (right) attends a press conference on the A picture taken in Camorino, southern Switzerland during the inauguration of the Ceneri Base railway tunnel shows a eve of the inauguration of the Ceneri Base railway tunnel. — AFP photos train arriving. witzerland opened its Ceneri tunnel on the border before crossing the landlocked country. between the north and south of the mountainous Friday-completing a mammoth project cut- “This is the final link that gives us a flat line country. Sommaruga cut the ribbon at the northern Sting a new route through the Alps which straight through the Alps,” Swiss Federal Railways end as the first freight train passed through, head- should transform rail links between northern and chief executive Vincent Ducrot told AFP at the tun- ing south. southern Europe. After opening the Lotschberg nel’s media launch on Thursday. “In the future, we “This new train line through the Alps is the Base Tunnel in 2007 and the Gotthard Base Tunnel will be able to have freight trains 750 meters long project of the century for our country,” the presi- in 2016, the Ceneri in Switzerland’s southern Ticino that can carry up to 2,100 tons of goods” per con- dent told AFP. “It is the biggest investment we region is the final stage of the New Railway Link voy, he said, highlighting the environmental bene- have ever made,”, she said, calling it “a strong through the Alps project. The route should ease fits. -
Program and Abstracts of 2017 Congress / Programme Et Résumés
1 Sponsors | Commanditaires Gold Sponsors | Commanditaires d’or Silver Sponsors | Commanditaires d’argent Other Sponsors | Les autres Commanditaires 2 Contents Sponsors | Commanditaires .......................................................................................................................... 2 Welcome from the Premier of Ontario .......................................................................................................... 5 Bienvenue du premier ministre de l'Ontario .................................................................................................. 6 Welcome from the Mayor of Toronto ............................................................................................................ 7 Mot de bienvenue du maire de Toronto ........................................................................................................ 8 Welcome from the Minister of Fisheries, Oceans and the Canadian Coast Guard ...................................... 9 Mot de bienvenue de ministre des Pêches, des Océans et de la Garde côtière canadienne .................... 10 Welcome from the Minister of Environment and Climate Change .............................................................. 11 Mot de bienvenue du Ministre d’Environnement et Changement climatique Canada ................................ 12 Welcome from the President of the Canadian Meteorological and Oceanographic Society ...................... 13 Mot de bienvenue du président de la Société canadienne de météorologie et d’océanographie ............. -
Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography on the Occasion of the 50Th Anniversary of Apollo 11 Moon Landing
Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography On the occasion of the 50th anniversary of Apollo 11 moon landing Please note: A specific item in this catalogue may be sold or is on hold if the provided link to our online inventory (by clicking on the blue-highlighted author name) doesn't work! Milestones of Science Books phone +49 (0) 177 – 2 41 0006 www.milestone-books.de [email protected] Member of ILAB and VDA Catalogue 07-2019 Copyright © 2019 Milestones of Science Books. All rights reserved Page 2 of 71 Authors in Chronological Order Author Year No. Author Year No. BIRT, William 1869 7 SCHEINER, Christoph 1614 72 PROCTOR, Richard 1873 66 WILKINS, John 1640 87 NASMYTH, James 1874 58, 59, 60, 61 SCHYRLEUS DE RHEITA, Anton 1645 77 NEISON, Edmund 1876 62, 63 HEVELIUS, Johannes 1647 29 LOHRMANN, Wilhelm 1878 42, 43, 44 RICCIOLI, Giambattista 1651 67 SCHMIDT, Johann 1878 75 GALILEI, Galileo 1653 22 WEINEK, Ladislaus 1885 84 KIRCHER, Athanasius 1660 31 PRINZ, Wilhelm 1894 65 CHERUBIN D'ORLEANS, Capuchin 1671 8 ELGER, Thomas Gwyn 1895 15 EIMMART, Georg Christoph 1696 14 FAUTH, Philipp 1895 17 KEILL, John 1718 30 KRIEGER, Johann 1898 33 BIANCHINI, Francesco 1728 6 LOEWY, Maurice 1899 39, 40 DOPPELMAYR, Johann Gabriel 1730 11 FRANZ, Julius Heinrich 1901 21 MAUPERTUIS, Pierre Louis 1741 50 PICKERING, William 1904 64 WOLFF, Christian von 1747 88 FAUTH, Philipp 1907 18 CLAIRAUT, Alexis-Claude 1765 9 GOODACRE, Walter 1910 23 MAYER, Johann Tobias 1770 51 KRIEGER, Johann 1912 34 SAVOY, Gaspare 1770 71 LE MORVAN, Charles 1914 37 EULER, Leonhard 1772 16 WEGENER, Alfred 1921 83 MAYER, Johann Tobias 1775 52 GOODACRE, Walter 1931 24 SCHRÖTER, Johann Hieronymus 1791 76 FAUTH, Philipp 1932 19 GRUITHUISEN, Franz von Paula 1825 25 WILKINS, Hugh Percy 1937 86 LOHRMANN, Wilhelm Gotthelf 1824 41 USSR ACADEMY 1959 1 BEER, Wilhelm 1834 4 ARTHUR, David 1960 3 BEER, Wilhelm 1837 5 HACKMAN, Robert 1960 27 MÄDLER, Johann Heinrich 1837 49 KUIPER Gerard P. -
Vraket Efter Gribshunden (C. 1483–1495) – Ett Unikt Exempel På Medeltida Skeppsarkitektur
Vraket efter Gribshunden (c. 1483–1495) – ett unikt exempel på medeltida skeppsarkitektur Niklas Eriksson enom att Östersjöns bräckta vatten saknar skeppsmask kan gamla Gskeppsvrak bevaras i århundraden. Sedan sportdykning blev populärt Rekonstruktion av en av de bärgade kanonerna från Gribshunden (Blekinge på 1960-talet har privatpersoner kontinuerligt påträffat och rapporterat museum). nya fynd. Men ibland kan det ta lite tid innan det uppdagas hur intressant ett vrak verkligen är. Redan 1971 påträffade medlemmar av Dykarklubben Doppingarna ett nedbrutet gammalt skeppsvrak på nio meters vattendjup der medeltiden och kom att fasas ut under 1500-talet till förmån för mer i Ekösund, en naturhamn i Blekinge skärgård utanför Ronneby. kraftfulla och pålitliga mynningsladdade bronskanoner. Genom åren kom vraket att besökas sporadiskt av klubbens medlemmar. Kalmar läns museum genomförde flera arkeologiska undersökningar av Det var först år 2000 som arkeologer gjordes uppmärksamma på just det vraket på uppdrag av länsstyrelsen i Blekinge. En mindre utgrävning ge- här fyndet. Dykaren Jonas Thörngren hade observerat ett slags märkliga nomfördes och ett antal fynd av keramik, matrester, delar av en ringbryn- urholkade stockar på vraket. Han kontaktade arkeologen Lars Einarsson ja och många andra föremål av medeltida karaktär tillvaratogs. Dessutom på Kalmar läns museum som drog slutsatsen att det förmodligen rörde sig bärgades nio lavettstockar som tillsammans med fynden från utgrävningen om lavettstockar till bakladdade smidda järnkanoner. Dessa var vanliga un- finns i Blekinge museums samlingar. Vid fältarbetet togs även träprover för dendrokronologisk analys. En sådan analys utgår från virkets årsringar. Genom att trädet växer till sig olika mycket ved för varje säsong så bildar Fil.Dr. -
Thermal and Crustal Evolution of Mars Steven A
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. E7, 10.1029/2001JE001801, 2002 Thermal and crustal evolution of Mars Steven A. Hauck II1 and Roger J. Phillips McDonnell Center for the Space Sciences and Department of Earth and Planetary Sciences, Washington University, Saint Louis, Missouri, USA Received 11 October 2001; revised 4 February 2002; accepted 11 February 2002; published 16 July 2002. [1] We present a coupled thermal-magmatic model for the evolution of Mars’ mantle and crust that may be consistent with estimates of the average crustal thickness and crustal growth rate. By coupling a simple parameterized model of mantle convection to a batch- melting model for peridotite, we can investigate potential conditions and evolutionary paths of the crust and mantle in a coupled thermal-magmatic system. On the basis of recent geophysical and geochemical studies, we constrain our models to have average crustal thicknesses between 50 and 100 km that were mostly formed by 4 Ga. Our nominal model is an attempt to satisfy these constraints with a relatively simple set of conditions. Key elements of this model are the inclusion of the energetics of melting, a wet (weak) mantle rheology, self-consistent fractionation of heat-producing elements to the crust, and a near- chondritic abundance of those elements. The latent heat of melting mantle material is a small (percent level) contributor to the total planetary energy budget over 4.5 Gyr but is crucial for constraining the thermal and magmatic history of Mars. Our nominal model predicts an average crustal thickness of 62 km that was 73% emplaced by 4 Ga. -
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, -
Testing Hypotheses for the Origin of Steep Slope of Lunar Size-Frequency Distribution for Small Craters
CORE Metadata, citation and similar papers at core.ac.uk Provided by Springer - Publisher Connector Earth Planets Space, 55, 39–51, 2003 Testing hypotheses for the origin of steep slope of lunar size-frequency distribution for small craters Noriyuki Namiki1 and Chikatoshi Honda2 1Department of Earth and Planetary Sciences, Kyushu University, Hakozaki 6-10-1, Higashi-ku, Fukuoka 812-8581, Japan 2The Institute of Space and Astronautical Science, Yoshinodai 3-1-1, Sagamihara 229-8510, Japan (Received June 13, 2001; Revised June 24, 2002; Accepted January 6, 2003) The crater size-frequency distribution of lunar maria is characterized by the change in slope of the population between 0.3 and 4 km in crater diameter. The origin of the steep segment in the distribution is not well understood. Nonetheless, craters smaller than a few km in diameter are widely used to estimate the crater retention age for areas so small that the number of larger craters is statistically insufficient. Future missions to the moon, which will obtain high resolution images, will provide a new, large data set of small craters. Thus it is important to review current hypotheses for their distributions before future missions are launched. We examine previous and new arguments and data bearing on the admixture of endogenic and secondary craters, horizontal heterogeneity of the substratum, and the size-frequency distribution of the primary production function. The endogenic crater and heterogeneous substratum hypotheses are seen to have little evidence in their favor, and can be eliminated. The primary production hypothesis fails to explain a wide variation of the size-frequency distribution of Apollo panoramic photographs. -
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 -
Download New Glass Review 21
NewG lass The Corning Museum of Glass NewGlass Review 21 The Corning Museum of Glass Corning, New York 2000 Objects reproduced in this annual review Objekte, die in dieser jahrlich erscheinenden were chosen with the understanding Zeitschrift veroffentlicht werden, wurden unter that they were designed and made within der Voraussetzung ausgewahlt, dass sie in- the 1999 calendar year. nerhalb des Kalenderjahres 1999 entworfen und gefertigt wurden. For additional copies of New Glass Review, Zusatzliche Exemplare der New Glass please contact: Review konnen angefordert werden bei: The Corning Museum of Glass Buying Office One Corning Glass Center Corning, New York 14830-2253 Telephone: (607) 974-6479 Fax: (607) 974-7365 E-mail: [email protected] All rights reserved, 2000 Alle Rechte vorbehalten, 2000 The Corning Museum of Glass The Corning Museum of Glass Corning, New York 14830-2253 Corning, New York 14830-2253 Printed in Frechen, Germany Gedruckt in Frechen, Bundesrepublik Deutschland Standard Book Number 0-87290-147-5 ISSN: 0275-469X Library of Congress Catalog Card Number Aufgefuhrt im Katalog der Library of Congress 81-641214 unter der Nummer 81-641214 Table of Contents/In halt Page/Seite Jury Statements/Statements der Jury 4 Artists and Objects/Kunstlerlnnen und Objekte 16 1999 in Review/Ruckblick auf 1999 36 Bibliography/Bibliografie 44 A Selective Index of Proper Names and Places/ Ausgewahltes Register von Eigennamen und Orten 73 Jury Statements Here is 2000, and where is art? Hier ist das Jahr 2000, und wo ist die Kunst? Although more people believe they make art than ever before, it is a Obwohl mehr Menschen als je zuvor glauben, sie machen Kunst, "definitionless" word about which a lot of people disagree. -
Documenting, Interpreting, Publishing, Re-Using
Documenting, Interpreting, Publishing, Re-using. Paola DERUDAS, Lund University, Sweden Keywords: 3D documentation, 3D contents, web-based visualization system, interactive reporting system Introduction and aims Data management plays a key role in the archaeological process. The technological advances and the active integration of traditional and innovative 3D practices have increased the accuracy of documentation, enabling richer and more complete recording and allowing the reflexive engagement of the archaeologist in the interpretation process (Berggren et al. 2015). The diffusion of daily 3D documentation of the stratigraphy, which has become quite common in many archaeological excavations, has resulted also in the production of even a huger amount of data than before. This plenty of multimedia data, composed of 3D models, images, videos, texts, tables, and so on, led to new opportunities and issues, connected mainly to the need for handling massive dataset, both in time and space. All data format produced within an excavation hence need a proper archive and management, after being homogenized, georeferenced and catalogued. They also need to be enriched by metadata, to be physically stored, and finally to be published. Thus, it appears that simply storing data can be useful but limited. Archaeologists lack a comprehensive archival system realized keeping in mind the chance of re-using that very same data also for other scientific purposes, interpretation and publication, as well as dissemination. The dissertation project describes some of the methods and procedures employed by the Department of Archeology at Lund University to deal with these matters. The research aims to investigate how the application of targeted technologies could contribute to standardizing and optimizing the archaeological data management and online publication work. -
Wreck Rap Malta
wreck rap Divers on the wreck of the Polynesian in Malta Text by Fatin Iesa Photos courtesy of Dave Gration, University of Malta, Heritage Malta Ranging from calm shore dives for beginner divers to techni- cal diving on elusive, unmarked wreck sites, which can only be found via depth sounder—diving in Malta has it all. Just beyond Malta’s dramatic underwater landscapes of strange rock for- mations, chimneys and caves, visitors can discover Malta’s intriguing and piquant past. To Malta's aid visiting divers, a newly creat- ed Underwater Cultural Heritage Unit (UCHU) has been formed within the Heritage Malta agen- Deep-Water Wrecks cy under the country’s cultural & Newly Created Underwater Heritage Unit ministry to manage the deep historical wreck sites of Malta. The UCHU provides informa- Currently rated as the world’s tenth small- Mediterranean Sea, 93km south of Italy torically had great strategic importance ters for the British Mediterranean Fleet tion regarding the history of the est and fifth most densely populated and 288km north of Africa, surrounded by as a naval base in the power struggles where many ships and warplanes for the wrecks, how to appreciate them country, Malta is the biggest of the three warm clear waters and year-round tem- between Europe, Africa and the Middle Allied powers were stationed. islands of the Maltese Archipelago, which perate climate. East. In the 19th century, Malta was colo- Touched by the sands of time, many and what the proper etiquette is also includes Gozo and Comino islands. Due to its central location in the nised by the British. -
Installers.Pdf
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