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Grosvenor Prints CATALOGUE for the ABA FAIR 2008
Grosvenor Prints 19 Shelton Street Covent Garden London WC2H 9JN Tel: 020 7836 1979 Fax: 020 7379 6695 E-mail: [email protected] www.grosvenorprints.com Dealers in Antique Prints & Books CATALOGUE FOR THE ABA FAIR 2008 Arts 1 – 5 Books & Ephemera 6 – 119 Decorative 120 – 155 Dogs 156 – 161 Historical, Social & Political 162 – 166 London 167 – 209 Modern Etchings 210 – 226 Natural History 227 – 233 Naval & Military 234 – 269 Portraits 270 – 448 Satire 449 – 602 Science, Trades & Industry 603 – 640 Sports & Pastimes 641 – 660 Foreign Topography 661 – 814 UK Topography 805 - 846 Registered in England No. 1305630 Registered Office: 2, Castle Business Village, Station Road, Hampton, Middlesex. TW12 2BX. Rainbrook Ltd. Directors: N.C. Talbot. T.D.M. Rayment. C.E. Ellis. E&OE VAT No. 217 6907 49 GROSVENOR PRINTS Catalogue of new stock released in conjunction with the ABA Fair 2008. In shop from noon 3rd June, 2008 and at Olympia opening 5th June. Established by Nigel Talbot in 1976, we have built up the United Kingdom’s largest stock of prints from the 17th to early 20th centuries. Well known for our topographical views, portraits, sporting and decorative subjects, we pride ourselves on being able to cater for almost every taste, no matter how obscure. We hope you enjoy this catalogue put together for this years’ Antiquarian Book Fair. Our largest ever catalogue contains over 800 items, many rare, interesting and unique images. We have also been lucky to purchase a very large stock of theatrical prints from the Estate of Alec Clunes, a well known actor, dealer and collector from the 1950’s and 60’s. -
General Vertical Files Anderson Reading Room Center for Southwest Research Zimmerman Library
“A” – biographical Abiquiu, NM GUIDE TO THE GENERAL VERTICAL FILES ANDERSON READING ROOM CENTER FOR SOUTHWEST RESEARCH ZIMMERMAN LIBRARY (See UNM Archives Vertical Files http://rmoa.unm.edu/docviewer.php?docId=nmuunmverticalfiles.xml) FOLDER HEADINGS “A” – biographical Alpha folders contain clippings about various misc. individuals, artists, writers, etc, whose names begin with “A.” Alpha folders exist for most letters of the alphabet. Abbey, Edward – author Abeita, Jim – artist – Navajo Abell, Bertha M. – first Anglo born near Albuquerque Abeyta / Abeita – biographical information of people with this surname Abeyta, Tony – painter - Navajo Abiquiu, NM – General – Catholic – Christ in the Desert Monastery – Dam and Reservoir Abo Pass - history. See also Salinas National Monument Abousleman – biographical information of people with this surname Afghanistan War – NM – See also Iraq War Abousleman – biographical information of people with this surname Abrams, Jonathan – art collector Abreu, Margaret Silva – author: Hispanic, folklore, foods Abruzzo, Ben – balloonist. See also Ballooning, Albuquerque Balloon Fiesta Acequias – ditches (canoas, ground wáter, surface wáter, puming, water rights (See also Land Grants; Rio Grande Valley; Water; and Santa Fe - Acequia Madre) Acequias – Albuquerque, map 2005-2006 – ditch system in city Acequias – Colorado (San Luis) Ackerman, Mae N. – Masonic leader Acoma Pueblo - Sky City. See also Indian gaming. See also Pueblos – General; and Onate, Juan de Acuff, Mark – newspaper editor – NM Independent and -
Evidence for Thermal-Stress-Induced Rockfalls on Mars Impact Crater Slopes
Icarus 342 (2020) 113503 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Evidence for thermal-stress-induced rockfalls on Mars impact crater slopes P.-A. Tesson a,b,*, S.J. Conway b, N. Mangold b, J. Ciazela a, S.R. Lewis c, D. M�ege a a Space Research Centre, Polish Academy of Science, Wrocław, Poland b Laboratoire de Plan�etologie et G�eodynamique UMR 6112, CNRS, Nantes, France c School of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK ARTICLE INFO ABSTRACT Keywords: Here we study rocks falling from exposed outcrops of bedrock, which have left tracks on the slope over which Mars, surface they have bounced and/or rolled, in fresh impact craters (1–10 km in diameter) on Mars. The presence of these Thermal stress tracks shows that these rocks have fallen relatively recently because aeolian processes are known to infill Ices topographic lows over time. Mapping of rockfall tracks indicate trends in frequency with orientation, which in Solar radiation � � turn depend on the latitudinal position of the crater. Craters in the equatorial belt (between 15 N and 15 S) Weathering exhibit higher frequencies of rockfall on their north-south oriented slopes compared to their east-west ones. � Craters >15 N/S have notably higher frequencies on their equator-facing slopes as opposed to the other ori entations. We computed solar radiation on the surface of crater slopes to compare insolation patterns with the spatial distribution of rockfalls, and found statistically significant correlations between maximum diurnal inso lation and rockfall frequency. -
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. -
11 Fall Unamagazine
FALL 2011 • VOLUME 19 • No. 3 FOR ALUMNI AND FRIENDS OF THE UNIVERSITY OF NORTH ALABAMA Cover Story 10 ..... Thanks a Million, Harvey Robbins Features 3 ..... The Transition 14 ..... From Zero to Infinity 16 ..... Something Special 20 ..... The Sounds of the Pride 28 ..... Southern Laughs 30 ..... Academic Affairs Awards 33 ..... Excellence in Teaching Award 34 ..... China 38 ..... Words on the Breeze Departments 2 ..... President’s Message 6 ..... Around the Campus 45 ..... Class Notes 47 ..... In Memory FALL 2011 • VOLUME 19 • No. 3 for alumni and friends of the University of North Alabama president’s message ADMINISTRATION William G. Cale, Jr. President William G. Cale, Jr. The annual everyone to attend one of these. You may Vice President for Academic Affairs/Provost Handy festival contact Dr. Alan Medders (Vice President John Thornell is drawing large for Advancement, [email protected]) Vice President for Business and Financial Affairs crowds to the many or Mr. Mark Linder (Director of Athletics, Steve Smith venues where music [email protected]) for information or to Vice President for Student Affairs is being played. At arrange a meeting for your group. David Shields this time of year Sometimes we measure success by Vice President for University Advancement William G. Cale, Jr. it is impossible the things we can see, like a new building. Alan Medders to go anywhere More often, though, success happens one Vice Provost for International Affairs in town and not hear music. The festival student at a time as we provide more and Chunsheng Zhang is also a reminder that we are less than better educational opportunities. -
Numerical Modeling of Magnetic Capture of Martian Atmospheric Dust ______
____________________________________________________________________________ Numerical Modeling of Magnetic Capture of Martian Atmospheric Dust __________________________________________________________________________ Kjartan Kinch Mars Simulation Laboratory Institute of Physics and Astronomy Aarhus University, Denmark Ph.D. Thesis Revised Edition March 2005 III Table of Contents Table of Contents .................................................................................. III List of Publications...............................................................................VII Preface.................................................................................................... IX 1. Introduction.........................................................................................1 1.1. The Mars Exploration Rover mission .................................................................1 1.2. Dust in the Martian Atmosphere .........................................................................2 1.3. Magnetic Properties Experiments .......................................................................3 1.4. The Present Work................................................................................................5 1.4.1. Motivation and Method......................................................................................5 1.4.2. Structure of the Thesis .......................................................................................5 2. The Planet Mars..................................................................................7 -
Widespread Crater-Related Pitted Materials on Mars: Further Evidence for the Role of Target Volatiles During the Impact Process ⇑ Livio L
Icarus 220 (2012) 348–368 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process ⇑ Livio L. Tornabene a, , Gordon R. Osinski a, Alfred S. McEwen b, Joseph M. Boyce c, Veronica J. Bray b, Christy M. Caudill b, John A. Grant d, Christopher W. Hamilton e, Sarah Mattson b, Peter J. Mouginis-Mark c a University of Western Ontario, Centre for Planetary Science and Exploration, Earth Sciences, London, ON, Canada N6A 5B7 b University of Arizona, Lunar and Planetary Lab, Tucson, AZ 85721-0092, USA c University of Hawai’i, Hawai’i Institute of Geophysics and Planetology, Ma¯noa, HI 96822, USA d Smithsonian Institution, Center for Earth and Planetary Studies, Washington, DC 20013-7012, USA e NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA article info abstract Article history: Recently acquired high-resolution images of martian impact craters provide further evidence for the Received 28 August 2011 interaction between subsurface volatiles and the impact cratering process. A densely pitted crater-related Revised 29 April 2012 unit has been identified in images of 204 craters from the Mars Reconnaissance Orbiter. This sample of Accepted 9 May 2012 craters are nearly equally distributed between the two hemispheres, spanning from 53°Sto62°N latitude. Available online 24 May 2012 They range in diameter from 1 to 150 km, and are found at elevations between À5.5 to +5.2 km relative to the martian datum. The pits are polygonal to quasi-circular depressions that often occur in dense clus- Keywords: ters and range in size from 10 m to as large as 3 km. -
Omaha Beach out of Derby with Entrapped Epiglottis
THURSDAY, MAY 2, 2019 WEDNESDAY’S TRACKSIDE DERBY REPORT OMAHA BEACH OUT OF by Steve Sherack DERBY WITH ENTRAPPED LOUISVILLE, KY - With the rising sun making its way through partly cloudy skies, well before the stunning late scratch of likely EPIGLOTTIS favorite Omaha Beach (War Front) rocked the racing world, the backstretch at Churchill Downs was buzzing on a warm and breezy Wednesday morning ahead of this weekend’s 145th GI Kentucky Derby. Two of Bob Baffert’s three Derby-bound ‘TDN Rising Stars’ Roadster (Quality Road) and Improbable (City Zip) were among the first to step foot on the freshly manicured surface during the special 15-minute training window reserved for Derby/Oaks horses at 7:30 a.m. Champion and fellow ‘Rising Star’ Game Winner (Candy Ride {Arg}) galloped during a later Baffert set at 9 a.m. Cont. p3 IN TDN EUROPE TODAY Omaha Beach & exercise rider Taylor Cambra Wednesday morning. | Sherackatthetrack CALYX SENSATIONAL IN ROYAL WARM-UP Calyx (GB) (Kingman {GB}) was scintillating in Ascot’s Fox Hill Farms’s Omaha Beach (War Front), the 4-1 favorite for G3 Pavilion S. on Wednesday. Saturday’s GI Kentucky Derby Presented by Woodford Reserve, Click or tap here to go straight to TDN Europe. will be forced to miss the race after it was discovered that he has an entrapped epiglottis. “After training this morning we noticed him cough a few times,” Hall of Fame trainer Richard Mandella said. “It caused us to scope him and we found an entrapped epiglottis. We can’t fix it this week, so we’ll have to have a procedure done in a few days and probably be out of training for three weeks. -
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, -
Martian Subsurface Properties and Crater Formation Processes Inferred from Fresh Impact Crater Geometries
Martian Subsurface Properties and Crater Formation Processes Inferred From Fresh Impact Crater Geometries The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Stewart, Sarah T., and Gregory J. Valiant. 2006. Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries. Meteoritics and Planetary Sciences 41: 1509-1537. Published Version http://meteoritics.org/ Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:4727301 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA Meteoritics & Planetary Science 41, Nr 10, 1509–1537 (2006) Abstract available online at http://meteoritics.org Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries Sarah T. STEWART* and Gregory J. VALIANT Department of Earth and Planetary Sciences, Harvard University, 20 Oxford Street, Cambridge, Massachusetts 02138, USA *Corresponding author. E-mail: [email protected] (Received 22 October 2005; revision accepted 30 June 2006) Abstract–The geometry of simple impact craters reflects the properties of the target materials, and the diverse range of fluidized morphologies observed in Martian ejecta blankets are controlled by the near-surface composition and the climate at the time of impact. Using the Mars Orbiter Laser Altimeter (MOLA) data set, quantitative information about the strength of the upper crust and the dynamics of Martian ejecta blankets may be derived from crater geometry measurements. -
Santa Fe National Historic Trail: Special History Study
Santa Fe National Historic Trail: Special History Study SANTE FE Special History Study COMERCIANTES, ARRIEROS, Y PEONES: THE HISPANOS AND THE SANTA FE TRADE (Merchants, Muleteers, and Peons) Special History Study Santa Fe National Historic Trail by Susan Calafate Boyle Southwest Cultural Resources Center Professional Papers No. 54 Division of History Southwest Region National Park Service 1994 TABLE OF CONTENTS safe/shs/index.htm Last Updated: 30-Sep-2005 http://www.nps.gov/history/history/online_books/safe/index.htm[7/2/2012 3:03:56 PM] Santa Fe National Historic Trail: Special History Study (Table of Contents) SANTA FE Special History Study TABLE OF CONTENTS COVER LIST OF FIGURES INTRODUCTION CHAPTER I - Isolation and Dependency CHAPTER II - Poverty and Neglect CHAPTER III - Going Down the Royal Road CHAPTER IV - Contraband and the Law CHAPTER V - New Mexican Merchants and Mercantile Capitalism CHAPTER VI - Felipe Chavez CHAPTER VII - Other Leading Merchant Families CONCLUSION RECOMMENDATIONS FOR FURTHER STUDY BIBLIOGRAPHY GLOSSARY APPENDIX I APPENDIX II APPENDIX III APPENDIX IV LIST OF ILLUSTRATIONS Figure 1. "Loading Up." J. Gregg marveled at the dexterity and skill with which hispanos harnessed and adjusted packs of merchandise Figure 2. The Santa Fe Trade: An International Trade Network Figure 3. The Santa Fe Trail: Part of an International Trade Network http://www.nps.gov/history/history/online_books/safe/shst.htm[7/2/2012 3:04:00 PM] Santa Fe National Historic Trail: Special History Study (Table of Contents) Figure 4. Pedro Vial pioneered a route that closely resembled the one Santa Fe Traders would follow in the next century Figure 5. -
First Year of Coordinated Science Observations by Mars Express and Exomars 2016 Trace Gas Orbiter
MANUSCRIPT PRE-PRINT Icarus Special Issue “From Mars Express to ExoMars” https://doi.org/10.1016/j.icarus.2020.113707 First year of coordinated science observations by Mars Express and ExoMars 2016 Trace Gas Orbiter A. Cardesín-Moinelo1, B. Geiger1, G. Lacombe2, B. Ristic3, M. Costa1, D. Titov4, H. Svedhem4, J. Marín-Yaseli1, D. Merritt1, P. Martin1, M.A. López-Valverde5, P. Wolkenberg6, B. Gondet7 and Mars Express and ExoMars 2016 Science Ground Segment teams 1 European Space Astronomy Centre, Madrid, Spain 2 Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France 3 Royal Belgian Institute for Space Aeronomy, Brussels, Belgium 4 European Space Research and Technology Centre, Noordwijk, The Netherlands 5 Instituto de Astrofísica de Andalucía, Granada, Spain 6 Istituto Nazionale Astrofisica, Roma, Italy 7 Institut d'Astrophysique Spatiale, Orsay, Paris, France Abstract Two spacecraft launched and operated by the European Space Agency are currently performing observations in Mars orbit. For more than 15 years Mars Express has been conducting global surveys of the surface, the atmosphere and the plasma environment of the Red Planet. The Trace Gas Orbiter, the first element of the ExoMars programme, began its science phase in 2018 focusing on investigations of the atmospheric composition with unprecedented sensitivity as well as surface and subsurface studies. The coordination of observation programmes of both spacecraft aims at cross calibration of the instruments and exploitation of new opportunities provided by the presence of two spacecraft whose science operations are performed by two closely collaborating teams at the European Space Astronomy Centre (ESAC). In this paper we describe the first combined observations executed by the Mars Express and Trace Gas Orbiter missions since the start of the TGO operational phase in April 2018 until June 2019.