The Summer Season June 1-July 31, 1993
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Planetary Geologic Mappers Annual Meeting
Program Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Planetary Geologic Mappers Annual Meeting June 12–14, 2018 • Knoxville, Tennessee Institutional Support Lunar and Planetary Institute Universities Space Research Association Convener Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Science Organizing Committee David Williams, Chair Arizona State University Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Robert Jacobsen Earth and Planetary Sciences Department, University of Tennessee Knoxville Bradley Thomson Earth and Planetary Sciences Department, University of Tennessee Knoxville Abstracts for this meeting are available via the meeting website at https://www.hou.usra.edu/meetings/pgm2018/ Abstracts can be cited as Author A. B. and Author C. D. (2018) Title of abstract. In Planetary Geologic Mappers Annual Meeting, Abstract #XXXX. LPI Contribution No. 2066, Lunar and Planetary Institute, Houston. Guide to Sessions Tuesday, June 12, 2018 9:00 a.m. Strong Hall Meeting Room Introduction and Mercury and Venus Maps 1:00 p.m. Strong Hall Meeting Room Mars Maps 5:30 p.m. Strong Hall Poster Area Poster Session: 2018 Planetary Geologic Mappers Meeting Wednesday, June 13, 2018 8:30 a.m. Strong Hall Meeting Room GIS and Planetary Mapping Techniques and Lunar Maps 1:15 p.m. Strong Hall Meeting Room Asteroid, Dwarf Planet, and Outer Planet Satellite Maps Thursday, June 14, 2018 8:30 a.m. Strong Hall Optional Field Trip to Appalachian Mountains Program Tuesday, June 12, 2018 INTRODUCTION AND MERCURY AND VENUS MAPS 9:00 a.m. Strong Hall Meeting Room Chairs: David Williams Devon Burr 9:00 a.m. -
Abridged Final Report with Resolutions
Brussels 18–24 September Regional Association VI (Europe) 2009 Fifteenth session Nassau, 18–24 September 2009 XV-RA VI XV-RA WMO-No. 1046 www.wmo.int WMO-No. 1046 Regional Association VI (Europe) Fifteenth session Brussels 18–24 September 2009 Abridged final report with resolutions WMO-No. 1046 WMO-No. 1046 © World Meteorological Organization, 2009 The right of publication in print, electronic and any other form and in any language is reserved by WMO. Short extracts from WMO publications may be reproduced without authorization, provided that the complete source is clearly indicated. Editorial correspondence and requests to publish, reproduce or translate this publication in part or in whole should be addressed to: Chairperson, Publications Board World Meteorological Organization (WMO) 7 bis, avenue de la Paix Tel.: +41 (0) 22 730 84 03 P.O. Box 2300 Fax: +41 (0) 22 730 80 40 CH-1211 Geneva 2, Switzerland E-mail: [email protected] ISBN 978-92-63-11046-6 NOTE The designations employed in WMO publications and the presentation of material in this publication do not imply the expression of any opinion whatsoever on the part of the Secretariat of WMO concerning the legal status of any country, territory, city or area, or of its authorities, or concerning the delimitation of its frontiers or boundaries. Opinions expressed in WMO publications are those of the authors and do not necessarily reflect those of WMO. The mention of specific companies or products does not imply that they are endorsed or recommended by WMO in preference to others of a similar nature which are not mentioned or advertised. -
MARS an Overview of the 1985–2006 Mars Orbiter Camera Science
MARS MARS INFORMATICS The International Journal of Mars Science and Exploration Open Access Journals Science An overview of the 1985–2006 Mars Orbiter Camera science investigation Michael C. Malin1, Kenneth S. Edgett1, Bruce A. Cantor1, Michael A. Caplinger1, G. Edward Danielson2, Elsa H. Jensen1, Michael A. Ravine1, Jennifer L. Sandoval1, and Kimberley D. Supulver1 1Malin Space Science Systems, P.O. Box 910148, San Diego, CA, 92191-0148, USA; 2Deceased, 10 December 2005 Citation: Mars 5, 1-60, 2010; doi:10.1555/mars.2010.0001 History: Submitted: August 5, 2009; Reviewed: October 18, 2009; Accepted: November 15, 2009; Published: January 6, 2010 Editor: Jeffrey B. Plescia, Applied Physics Laboratory, Johns Hopkins University Reviewers: Jeffrey B. Plescia, Applied Physics Laboratory, Johns Hopkins University; R. Aileen Yingst, University of Wisconsin Green Bay Open Access: Copyright 2010 Malin Space Science Systems. This is an open-access paper distributed under the terms of a Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Abstract Background: NASA selected the Mars Orbiter Camera (MOC) investigation in 1986 for the Mars Observer mission. The MOC consisted of three elements which shared a common package: a narrow angle camera designed to obtain images with a spatial resolution as high as 1.4 m per pixel from orbit, and two wide angle cameras (one with a red filter, the other blue) for daily global imaging to observe meteorological events, geodesy, and provide context for the narrow angle images. Following the loss of Mars Observer in August 1993, a second MOC was built from flight spare hardware and launched aboard Mars Global Surveyor (MGS) in November 1996. -
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 -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Catalogo Giornate Del Cinema Muto 2011
Clara Bow in Mantrap, Victor Fleming, 1926. (Library of Congress) Merna Kennedy, Charles Chaplin in The Circus, 1928. (Roy Export S.A.S) Sommario / Contents 3 Presentazione / Introduction 31 Shostakovich & FEKS 6 Premio Jean Mitry / The Jean Mitry Award 94 Cinema italiano: rarità e ritrovamenti Italy: Retrospect and Discovery 7 In ricordo di Jonathan Dennis The Jonathan Dennis Memorial Lecture 71 Cinema georgiano / Georgian Cinema 9 The 2011 Pordenone Masterclasses 83 Kertész prima di Curtiz / Kertész before Curtiz 0 1 Collegium 2011 99 National Film Preservation Foundation Tesori western / Treasures of the West 12 La collezione Davide Turconi The Davide Turconi Collection 109 La corsa al Polo / The Race to the Pole 7 1 Eventi musicali / Musical Events 119 Il canone rivisitato / The Canon Revisited Novyi Vavilon A colpi di note / Striking a New Note 513 Cinema delle origini / Early Cinema SpilimBrass play Chaplin Le voyage dans la lune; The Soldier’s Courtship El Dorado The Corrick Collection; Thanhouser Shinel 155 Pionieri del cinema d’animazione giapponese An Audience with Jean Darling The Birth of Anime: Pioneers of Japanese Animation The Circus The Wind 165 Disney’s Laugh-O-grams 179 Riscoperte e restauri / Rediscoveries and Restorations The White Shadow; The Divine Woman The Canadian; Diepte; The Indian Woman’s Pluck The Little Minister; Das Rätsel von Bangalor Rosalie fait du sabotage; Spreewaldmädel Tonaufnahmen Berglund Italianamerican: Santa Lucia Luntana, Movie Actor I pericoli del cinema / Perils of the Pictures 195 Ritratti / Portraits 201 Muti del XXI secolo / 21st Century Silents 620 Indice dei titoli / Film Title Index Introduzioni e note di / Introductions and programme notes by Peter Bagrov Otto Kylmälä Aldo Bernardini Leslie Anne Lewis Ivo Blom Antonello Mazzucco Lenny Borger Patrick McCarthy Neil Brand Annette Melville Geoff Brown Russell Merritt Kevin Brownlow Maud Nelissen Günter A. -
Hip # 987-1088
Hip No. Consigned by Tate Farms Hip No. 987 Jess Sizzlin SI 92 987 1997 Sorrel Mare Streakin La Jolla SI 99 {Streakin Six SI 104 Mr Jess Perry SI 113 { Bottom’s Up SI 82 Scoopie Fein SI 99 {Sinn Fein SI 98 Jess Sizzlin SI 92 Legs La Scoop SI 95 3654393 Easy Jet SI 100 {Jet Deck SI 100 Sizzlin Kim SI 86 Lena’s Bar TB SI 95 (1987) { Sun Spots {Double Bid SI 100 Winsum Miss SI 95 By MR JESS PERRY SI 113 (1992). Champion 2-year-old, $687,184 [G1]. Sire of 799 ROM, 107 stakes winners, $39,619,142, incl. champions APOL- LITICAL JESS SI 107 (world champion, $1,399,831, Los Alamitos Derby [G1]), ONE FAMOUS EAGLE SI 101 ($1,387,453 [G1]). Sire of the dams of 46 stakes winners, incl. BODACIOUS DASH SI 101 ($756,495 [G1]), JES A GAME SI 111 ($323,978 [G2]), TERRIFIC SYNERGY SI 92 ($288,066 [RG2]). 1st dam SIZZLIN KIM SI 86, by Easy Jet. Placed to 3. Dam of 7 foals, 6 to race, 3 winners, including– Jess Sizzlin SI 92 (f. by Mr Jess Perry). Stakes placed winner, below. Streakin Kim (f. by Streakin La Jolla). Unplaced. Dam of– Kims Corona SI 97 (g. by Corona Cocktail). 3 wins to 4, $38,666. 2nd dam SUN SPOTS, by Double Bid. Unraced. Dam of 13 starters, 7 ROM, incl.– SUN KISSES SI 102 (f. by Game Plan). 7 wins to 3, $68,935, Shebester Derby, Mystery Derby. Dam of Exquisite Expense SI 99 ($42,264 [G3]). -
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. -
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. -
VIRVĖ SAVO KARTUVĖMS Kapitalistų Sandėriai Su Komunistais Vytautas Meškauskas
T e oc. oi' 5 □ TL i r. s t r c ba š' 7243 So» Albanv fk., ' yi Chiccęp, III, ‘ 304.29 ; I0TEKA Į -----THE LITHUANIAN NATIONAL NEVVSPAPER -------- P.O. BOX 03206 > 6116 ST. CLAIR AVENUE > CLEVELAND, OHIO 44103 Vol.LXIV Balandis - April 19, 1979 Nr.16 *< TAUTINES MINTIES LIETUVIŲ LAIKRAŠTIS VIRVĖ SAVO KARTUVĖMS Kapitalistų sandėriai su komunistais Vytautas Meškauskas Turiu pasakyti, kad Leninas išpranašavo visą proce Konkrečiai kalbant, pereitų są. Leninas, kuris didesnę savo gyvenimo dalį praleido metų prekybos su sovietais Vakaruose, bet ne Rusijoje, kuris geriau pažinojo Vaka apyvarta siekė tik 2.8 biijonus rus kaip Rusiją, visados rašė ir sakė, jog Vakarų kapi dolerių, t.y. tik trečdalį pre talistai padarys viską, kad sustiprintų SSSR ekonomiją. kybos su ... Taiwanu. Biznie Jie konkuruos savo tarpe, kad mums parduoti gerybes rius tačiau vilioja ne tiek da pigiau ir greičiau, tik tam, kad sovietai jas pirktų ne iš bartinės, kiek ateities galimy bės. Šiaip ar taip, Sovietiją vieno, bet iš kito. Jis sakė: jie taip darys negalvodami sudaro rinką su 250 milijonų apie savo pačių ateitį. Vienu sunkiu momentu partijos gyventojų. posėdyje Maskvoje jis drąsino: "Draugai, nepasiduokit Nepaisant to, kad bolševi panikai, jei mums pasidarys labai sunku, mes duosime kai konfiskavo visus užsienie virvę buržuazijai, ir buržuazija pati pasikars." čių kapitalus, buvusius caro Tada, Kari Radek,... kuris buvo labai sąmojingas, Rusijoje - vien Singerio kom paklausė: Vladimire Iličiau, bet iš kur mes paimsime tiek panija prieš karą ten turėjo daug virvės buržuazijos pasikorimui?” Leninas nerūpes 27,000 tarnautojų. Vakarų tingai atsakė: "Jie mus ja aprūpins." kapitalistai padėjo sovietų (Iš Aleksandro Solženicyno 1975 m. -
A Concept for the Deployment of a Large
i-SAIRAS2020-Papers (2020) 5072.pdf A CONCEPT FOR THE DEPLOYMENT OF A LARGE LUNAR CRATER RADIO TELESCOPE USING TEAMS OF TETHERED ROBOTS Virtual Conference 19–23 October 2020 Patrick McGarey1*, Saptarshi Bandyopadhyay1†, Ramin Rafizadeh1, Ashish Goel1, Manan Arya1, Issa Nesnas1, Joe Lazio1, Paul Goldsmith1, Adrian Stoica1, Marco Quadrelli1, Gregg Hallinan2 1 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA, USA 91109 *[email protected], †[email protected] 2Astronomy Department, California Institute of Technology, 1200 East California Blvd, Pasadena, CA, USA 91125 ABSTRACT 1 INTRODUCTION Kilometer-scale craters on the far side of the Moon have unique potential as future locations for large ra- dio telescopes, which can observe the universe at wavelengths and frequencies (>10 m, < 30 MHz) not possible with conventional Earth or orbital-based ap- proaches. Distinct advantages of building a Lunar Crater Radio Telescope (LCRT) on the far side include i) isolation from radio noise due to the Earth’s iono- sphere, orbiting satellites, and the Sun, ii) days of un- interrupted dark/cold sky viewing during lunar night, and iii) terrain geometry naturally suited for con- structing the largest mesh antenna structure in the So- lar System. A key challenge to constructing LCRT on the Moon is related to the complexity of deploying a Figure 1: Illustration of the Lunar Crater Radio Tele- 1-km diameter antenna and hanging receiver within a scope (LCRT) concept. The green antenna reflector is lunar crater whose diameter, depth, and slope are 3-5 shown suspended by lift wires just below a suspended km, 1 km, and ~30 degrees respectively. -
PERO Proposal
_ i b '’ V '•• •• , .1 ’ ^ V ' ' ■■• ; ■■ FRIDAY, JANUARY #1, 1»64 «® SEOTSEN V jStanrlt^Btfr lEwning li^rald Aierafg Dally Net Pteas Kne Far tlw WMk DaM servloes o f the UJB. C on fer Auraaiy 95^ 1964 The VTW Poet will sponsor Course to Stop FORRBNT Rally Set Sunday ence of Mayors and to urge Rahi aadiag aatiiy seafood night from 6 to 12:80 Curtis Wants them to jedn. 8 and M mm. Marla. Piojaa- l ^ u t Town ajn. for membera and guests Manchester’s board of direc Smoking Plan tors—sound or sOnk Moo 13,881 85 «a‘ 46i.- eaaiair'L ^ By Youth Council $ 5 iwm. sUda projeoton, to n ig h t tors, earlier this month voted vuCUm AiMtt b r e ^ , aaU . M lgli 66 4a 9)1^1^ . 3fr. and Mrs. Gordon lUxdc- To Negotiate the town’s partlcipatian In the A ICMohester agency Is «• WELDON DRUG CO. I ad CXraiilattMi win ot 58 Marion Dr. will be John B. Cumer- HI, an en- TIm Manoheater Christian conference, at an annual ooat Maneh0$tmr^A Cky of Vlttagf Charm gineman third class ip the Unit peoted to ^Mosor a ‘Tlve-Oajr 901 Main SWVeL 948-5991 boat and hoetesa Sunday from Y outh OourcB wlH present its o f 8100. Plan to atop Smoking,” the » - 8 to 6 pjn. at the LuU Junior ed States Coast Guard and son Bus Contract Youth Week RaBy Service from Mayor Mahoney attended last ■ult of a meeting last idght at (CliaaWlad AdverUsfaig oa Paga 16) PRICE SEVEN CENTS Kuaeum.