DATA CATALOG ERIE for PACE CIENCE and APPLICATIO FIGHT MI ION Volume La De Criptio of Planetary and Heliocentric Pacecraft and Inve Tigation
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Railway Employee Records for Colorado Volume Iii
RAILWAY EMPLOYEE RECORDS FOR COLORADO VOLUME III By Gerald E. Sherard (2005) When Denver’s Union Station opened in 1881, it saw 88 trains a day during its gold-rush peak. When passenger trains were a popular way to travel, Union Station regularly saw sixty to eighty daily arrivals and departures and as many as a million passengers a year. Many freight trains also passed through the area. In the early 1900s, there were 2.25 million railroad workers in America. After World War II the popularity and frequency of train travel began to wane. The first railroad line to be completed in Colorado was in 1871 and was the Denver and Rio Grande Railroad line between Denver and Colorado Springs. A question we often hear is: “My father used to work for the railroad. How can I get information on Him?” Most railroad historical societies have no records on employees. Most employment records are owned today by the surviving railroad companies and the Railroad Retirement Board. For example, most such records for the Union Pacific Railroad are in storage in Hutchinson, Kansas salt mines, off limits to all but the lawyers. The Union Pacific currently declines to help with former employee genealogy requests. However, if you are looking for railroad employee records for early Colorado railroads, you may have some success. The Colorado Railroad Museum Library currently has 11,368 employee personnel records. These Colorado employee records are primarily for the following railroads which are not longer operating. Atchison, Topeka & Santa Fe Railroad (AT&SF) Atchison, Topeka and Santa Fe Railroad employee records of employment are recorded in a bound ledger book (record number 736) and box numbers 766 and 1287 for the years 1883 through 1939 for the joint line from Denver to Pueblo. -
Recurring Slope Lineae: Evidence of Liquid Water on Mars Today?
Recurring Slope Lineae: Evidence of liquid water on Mars today? The High Resolution Imaging Science Experiment (HiRISE) on Mars Reconnaissance Orbiter (MRO) has monitored surface feature changes over several Mars years. One of the more intriguing observations has been of the seasonal occurrence of numerous (multi-thousand) dark streak features advancing down equator-facing slopes in several mid-latitude and equatorial regions of the southern hemisphere. Termed Recurring Slope Lineae (RSL), the streak behavior resembles that of a fluid mobilized by increasing surface temperatures – initiating in spring, incrementally extending downslope through summer, and then fading in the fall and winter seasons. The phenomenon is then seen to repeat the following spring. RSLs are narrow in width (meter-scale), requiring our best resolution imaging to see them, but may extend down-slope for hundreds of meters before terminating. Science teams involved in the discovery of RSL have been cautious in concluding a water-based origin since most of the RSL locations are found in environments well outside the pressure-temperature stability field for liquid water. However, the presence of salts such as perchlorate can depress freezing points by tens of degrees. MRO Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) observations of multiple RSL locations show hydrated mineral absorption signals most consistent with magnesium perchlorate, magnesium chlorate and sodium perchlorate. That raises the possibility of a Mg-, Na-, Cl-rich brine that would also leave these minerals as a kind of evaporite deposit. However, the amount of water, if present, has been constrained at one location by independent Thermal Emission Imaging System (THEMIS; Mars Odyssey) data analysis and a numerical heat transfer model to 0 wt.%, and up to 3 wt.% given observational uncertainties, unlikely to support a sustained flow. -
Appendix 1: Venus Missions
Appendix 1: Venus Missions Sputnik 7 (USSR) Launch 02/04/1961 First attempted Venus atmosphere craft; upper stage failed to leave Earth orbit Venera 1 (USSR) Launch 02/12/1961 First attempted flyby; contact lost en route Mariner 1 (US) Launch 07/22/1961 Attempted flyby; launch failure Sputnik 19 (USSR) Launch 08/25/1962 Attempted flyby, stranded in Earth orbit Mariner 2 (US) Launch 08/27/1962 First successful Venus flyby Sputnik 20 (USSR) Launch 09/01/1962 Attempted flyby, upper stage failure Sputnik 21 (USSR) Launch 09/12/1962 Attempted flyby, upper stage failure Cosmos 21 (USSR) Launch 11/11/1963 Possible Venera engineering test flight or attempted flyby Venera 1964A (USSR) Launch 02/19/1964 Attempted flyby, launch failure Venera 1964B (USSR) Launch 03/01/1964 Attempted flyby, launch failure Cosmos 27 (USSR) Launch 03/27/1964 Attempted flyby, upper stage failure Zond 1 (USSR) Launch 04/02/1964 Venus flyby, contact lost May 14; flyby July 14 Venera 2 (USSR) Launch 11/12/1965 Venus flyby, contact lost en route Venera 3 (USSR) Launch 11/16/1965 Venus lander, contact lost en route, first Venus impact March 1, 1966 Cosmos 96 (USSR) Launch 11/23/1965 Possible attempted landing, craft fragmented in Earth orbit Venera 1965A (USSR) Launch 11/23/1965 Flyby attempt (launch failure) Venera 4 (USSR) Launch 06/12/1967 Successful atmospheric probe, arrived at Venus 10/18/1967 Mariner 5 (US) Launch 06/14/1967 Successful flyby 10/19/1967 Cosmos 167 (USSR) Launch 06/17/1967 Attempted atmospheric probe, stranded in Earth orbit Venera 5 (USSR) Launch 01/05/1969 Returned atmospheric data for 53 min on 05/16/1969 M. -
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. -
Non-Collider Searches for Stable Massive Particles
Non-collider searches for stable massive particles S. Burdina, M. Fairbairnb, P. Mermodc,, D. Milsteadd, J. Pinfolde, T. Sloanf, W. Taylorg aDepartment of Physics, University of Liverpool, Liverpool L69 7ZE, UK bDepartment of Physics, King's College London, London WC2R 2LS, UK cParticle Physics department, University of Geneva, 1211 Geneva 4, Switzerland dDepartment of Physics, Stockholm University, 106 91 Stockholm, Sweden ePhysics Department, University of Alberta, Edmonton, Alberta, Canada T6G 0V1 fDepartment of Physics, Lancaster University, Lancaster LA1 4YB, UK gDepartment of Physics and Astronomy, York University, Toronto, ON, Canada M3J 1P3 Abstract The theoretical motivation for exotic stable massive particles (SMPs) and the results of SMP searches at non-collider facilities are reviewed. SMPs are defined such that they would be suffi- ciently long-lived so as to still exist in the cosmos either as Big Bang relics or secondary collision products, and sufficiently massive such that they are typically beyond the reach of any conceiv- able accelerator-based experiment. The discovery of SMPs would address a number of important questions in modern physics, such as the origin and composition of dark matter and the unifi- cation of the fundamental forces. This review outlines the scenarios predicting SMPs and the techniques used at non-collider experiments to look for SMPs in cosmic rays and bound in mat- ter. The limits so far obtained on the fluxes and matter densities of SMPs which possess various detection-relevant properties such as electric and magnetic charge are given. Contents 1 Introduction 4 2 Theory and cosmology of various kinds of SMPs 4 2.1 New particle states (elementary or composite) . -
Obituary 1967
OBITUARY INDEX 1967 You can search by clicking on the binoculars on the adobe toolbar or by Pressing Shift-Control-F Request Form LAST NAME FIRST NAME DATE PAGE # Abbate Barbara F. 6/6/1967 p.1 Abbott William W. 9/22/1967 p.30 Abel Dean 11/27/1967 p.24 Abel Francis E. 9/25/1967 p.24 Abel Francis E. 9/27/1967 p.10 Abel Frederick B. 11/11/1967 p.26 Abel John Hawk 12/7/1967 p.42 Abel John Hawk 12/11/1967 p.26 Abel William E. 7/10/1967 p.28 Abel William E. 7/12/1967 p.12 Aber George W. 3/14/1967 p.24 Abert Esther F. 7/26/1967 p.14 Abrams Laura R. Hoffman 8/14/1967 p.28 Abrams Laura R. Hoffman 8/17/1967 p.28 Abrams Pearl E. 10/19/1967 p.28 Abrams Pearl E. 10/20/1967 p.10 Achenbach Helen S. 11/6/1967 p.36 Achenbach Helen S. 11/8/1967 p.15 Ackerman Calvin 5/22/1967 p.34 Ackerman Calvin 5/25/1967 p.38 Ackerman Fritz 11/27/1967 p.24 Ackerman Harold 10/27/1967 p.26 Ackerman Harold 10/28/1967 p.26 Ackerman Hattie Mann 4/14/1967 p.21 Ackerman Hattie Mann 4/19/1967 p.14 Adamczyk Bennie 5/3/1967 p.14 Adamo Margaret M. 3/15/1967 p.15 Adamo Margaret M. 3/20/1967 p.28 Adams Anna 6/17/1967 p.22 Adams Anna 6/20/1967 p.17 Adams Harriet C. -
Philadelphia, Pennsylvania (2)” of the Sheila Weidenfeld Files at the Gerald R
The original documents are located in Box 14, folder “5/12/75 - Philadelphia, Pennsylvania (2)” of the Sheila Weidenfeld Files at the Gerald R. Ford Presidential Library. Copyright Notice The copyright law of the United States (Title 17, United States Code) governs the making of photocopies or other reproductions of copyrighted material. Gerald Ford donated to the United States of America his copyrights in all of his unpublished writings in National Archives collections. Works prepared by U.S. Government employees as part of their official duties are in the public domain. The copyrights to materials written by other individuals or organizations are presumed to remain with them. If you think any of the information displayed in the PDF is subject to a valid copyright claim, please contact the Gerald R. Ford Presidential Library. Some items in this folder were not digitized because it contains copyrighted materials. Please contact the Gerald R. Ford Presidential Library for access to these materials. Digitized from Box 14 of the Sheila Weidenfeld Files at the Gerald R. Ford Presidential Library Vol. 21 Feb.-March 1975 PUBLISHED BI-MONTHLY BY PARC, THE PHILADELPHIA ASSOCIATION FOR RETARDED CITIZENS FIRST LADY TO BE HONORED Mrs. Gerald R. Ford will be citizens are invited to attend the "guest of honor at PARC's Silver dinner. The cost of attending is Anniversary Dinner to be held at $25 per person. More details the Bellevue Stratford Hotel, about making reservations may be Monday, May 12. She will be the obtained by calling Mrs. Eleanor recipient of " The PARC Marritz at PARC's office, LO. -
Cover No Spine
2006 VOL 44, NO. 4 Special Issue: The Hans Christian Andersen Awards 2006 The Journal of IBBY,the International Board on Books for Young People Editors: Valerie Coghlan and Siobhán Parkinson Address for submissions and other editorial correspondence: [email protected] and [email protected] Bookbird’s editorial office is supported by the Church of Ireland College of Education, Dublin, Ireland. Editorial Review Board: Sandra Beckett (Canada), Nina Christensen (Denmark), Penni Cotton (UK), Hans-Heino Ewers (Germany), Jeffrey Garrett (USA), Elwyn Jenkins (South Africa),Ariko Kawabata (Japan), Kerry Mallan (Australia), Maria Nikolajeva (Sweden), Jean Perrot (France), Kimberley Reynolds (UK), Mary Shine Thompson (Ireland), Victor Watson (UK), Jochen Weber (Germany) Board of Bookbird, Inc.: Joan Glazer (USA), President; Ellis Vance (USA),Treasurer;Alida Cutts (USA), Secretary;Ann Lazim (UK); Elda Nogueira (Brazil) Cover image:The cover illustration is from Frau Meier, Die Amsel by Wolf Erlbruch, published by Peter Hammer Verlag,Wuppertal 1995 (see page 11) Production: Design and layout by Oldtown Design, Dublin ([email protected]) Proofread by Antoinette Walker Printed in Canada by Transcontinental Bookbird:A Journal of International Children’s Literature (ISSN 0006-7377) is a refereed journal published quarterly by IBBY,the International Board on Books for Young People, Nonnenweg 12 Postfach, CH-4003 Basel, Switzerland tel. +4161 272 29 17 fax: +4161 272 27 57 email: [email protected] <www.ibby.org>. Copyright © 2006 by Bookbird, Inc., an Indiana not-for-profit corporation. Reproduction of articles in Bookbird requires permission in writing from the editor. Items from Focus IBBY may be reprinted freely to disseminate the work of IBBY. -
Jjmonl 1710.Pmd
alactic Observer John J. McCarthy Observatory G Volume 10, No. 10 October 2017 The Last Waltz Cassini’s final mission and dance of death with Saturn more on page 4 and 20 The John J. McCarthy Observatory Galactic Observer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky Technical Support It is through their efforts that the McCarthy Observatory Bob Lambert has established itself as a significant educational and recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Route Mike Chiarella Roger Moore Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Doug Delisle Marc Polansky Cecilia Detrich Joe Privitera Dirk Feather Monty Robson Randy Fender Don Ross Louise Gagnon Gene Schilling John Gebauer Katie Shusdock Elaine Green Paul Woodell Tina Hartzell Amy Ziffer In This Issue INTERNATIONAL OBSERVE THE MOON NIGHT ...................... 4 SOLAR ACTIVITY ........................................................... 19 MONTE APENNINES AND APOLLO 15 .................................. 5 COMMONLY USED TERMS ............................................... 19 FAREWELL TO RING WORLD ............................................ 5 FRONT PAGE ............................................................... -
RSL), Described in the 5 August 2011 Science Report “Seasonal Flows on Warm Martian Slopes”
Animated GIFs to illustrate activity of Recurring Slope Lineae (RSL), described in the 5 August 2011 Science report “Seasonal Flows on Warm Martian Slopes”. All of these animated GIF files consist of a series of orthorectified HiRISE images over locations with RSL activity. Orthorectification corrects oblique images to show how the scene would appear from directly overhead. We perform this using HiRISE Digital Terrain Models (DTMs) at a scale of 1 m/posting. The orthorectified images are all at 0.25 m/pixel scale (or 0.5 m/pixel in cases noted below), so features smaller than 1-2 m diameter cannot be correctly rectified; the result is that small-scale features like boulders appear to wag back and forth. Each GIF is timed to dwell 2 seconds on the first and last frames and 1 second on intermediate frames, but network or computer performance may cause this to vary. The legend on each image gives the exact HiRISE image identifier; see http://uahirise.org/{image identified} for more information about each image. The legend also marks the year and seasonal identifier (Ls) for each image. The Mars years begin with the first years of Mars exploration by robot spacecraft. Ls stands for areocentric longitude of the sun, dividing the year into 360 degrees to mark the seasons. Ls = 180 is the beginning of southern spring, Ls = 270 is the beginning of southern summer, and Ls = 360 (or 0) is the beginning of southern autumn. Well-preserved crater on floor of Newton Crater Each of the gifs below are enhanced color sequences from different section of this crater slope, starting with faded RSL in MY29 (except one in which the color data was largely missing), then showing a sequence of RSL forming and fading in MY30. -
Impact Melt Emplacement on Mercury
Western University Scholarship@Western Electronic Thesis and Dissertation Repository 7-24-2018 2:00 PM Impact Melt Emplacement on Mercury Jeffrey Daniels The University of Western Ontario Supervisor Neish, Catherine D. The University of Western Ontario Graduate Program in Geology A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Jeffrey Daniels 2018 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Geology Commons, Physical Processes Commons, and the The Sun and the Solar System Commons Recommended Citation Daniels, Jeffrey, "Impact Melt Emplacement on Mercury" (2018). Electronic Thesis and Dissertation Repository. 5657. https://ir.lib.uwo.ca/etd/5657 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. Abstract Impact cratering is an abrupt, spectacular process that occurs on any world with a solid surface. On Earth, these craters are easily eroded or destroyed through endogenic processes. The Moon and Mercury, however, lack a significant atmosphere, meaning craters on these worlds remain intact longer, geologically. In this thesis, remote-sensing techniques were used to investigate impact melt emplacement about Mercury’s fresh, complex craters. For complex lunar craters, impact melt is preferentially ejected from the lowest rim elevation, implying topographic control. On Venus, impact melt is preferentially ejected downrange from the impact site, implying impactor-direction control. Mercury, despite its heavily-cratered surface, trends more like Venus than like the Moon. -
SM a R T M U S E U M O F a R T U N Iv E R S It Y O F C H IC a G O B U L L E T in 2 0 0 6 – 20
http://smartmuseum.uchicago.edu Chicago, Illinois 60637 5550 South Greenwood Avenue SMART SMART M U S EUM OF A RT UN I VER SI TY OFCH ICAG O RT RT A OF EUM S U M SMART 2008 – 2006 N I ET BULL O ICAG H C OF TY SI VER I N U SMART MUSEUM OF ART UNIVERSITY OF CHICAGO BULLETIN 2006– 2008 SMART MUSEUM OF ART UNIVERSITY OF CHICAGO BULLETIN 2006–2008 MissiON STATEMENT / 1 SMART MUSEUM BOARD OF GOVERNORS / 3 REPORTS FROM THE CHAIRMAN AND DiRECTOR / 4 ACQUisiTIOns / 10 LOANS / 34 EXHIBITIOns / 44 EDUCATION PROGRAMS / 68 SOURCES OF SUPPORT / 88 SMART STAFF / 108 STATEMENT OF OPERATIOns / 112 MissiON STATEMENT As the ar t museum of the Universit y of Chicago, the David and Alfred Smar t Museum of Ar t promotes the understanding of the visual arts and their importance to cultural and intellectual history through direct experiences with original works of art and through an interdisciplinary approach to its collections, exhibitions, publications, and programs. These activities support life-long learning among a range of audiences including the University and the broader community. SMART MUSEUM BOARD OF GOVERNORS Robert Feitler, Chair Lorna C. Ferguson, Vice Chair Elizabeth Helsinger, Vice Chair Richard Gray, Chairman Emeritus Marilynn B. Alsdorf Isaac Goldman Larry Norman* Mrs. Edwin A. Bergman Jack Halpern Brien O’Brien Russell Bowman Neil Harris Brenda Shapiro* Gay-Young Cho Mary J. Harvey* Raymond Smart Susan O’Connor Davis Anthony Hirschel* Joel M. Snyder Robert G. Donnelley Randy L. Holgate John N. Stern Richard Elden William M. Landes Isabel C.