Ithaca Classified Business Directory 1935
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Imagining Outer Space Also by Alexander C
Imagining Outer Space Also by Alexander C. T. Geppert FLEETING CITIES Imperial Expositions in Fin-de-Siècle Europe Co-Edited EUROPEAN EGO-HISTORIES Historiography and the Self, 1970–2000 ORTE DES OKKULTEN ESPOSIZIONI IN EUROPA TRA OTTO E NOVECENTO Spazi, organizzazione, rappresentazioni ORTSGESPRÄCHE Raum und Kommunikation im 19. und 20. Jahrhundert NEW DANGEROUS LIAISONS Discourses on Europe and Love in the Twentieth Century WUNDER Poetik und Politik des Staunens im 20. Jahrhundert Imagining Outer Space European Astroculture in the Twentieth Century Edited by Alexander C. T. Geppert Emmy Noether Research Group Director Freie Universität Berlin Editorial matter, selection and introduction © Alexander C. T. Geppert 2012 Chapter 6 (by Michael J. Neufeld) © the Smithsonian Institution 2012 All remaining chapters © their respective authors 2012 All rights reserved. No reproduction, copy or transmission of this publication may be made without written permission. No portion of this publication may be reproduced, copied or transmitted save with written permission or in accordance with the provisions of the Copyright, Designs and Patents Act 1988, or under the terms of any licence permitting limited copying issued by the Copyright Licensing Agency, Saffron House, 6–10 Kirby Street, London EC1N 8TS. Any person who does any unauthorized act in relation to this publication may be liable to criminal prosecution and civil claims for damages. The authors have asserted their rights to be identified as the authors of this work in accordance with the Copyright, Designs and Patents Act 1988. First published 2012 by PALGRAVE MACMILLAN Palgrave Macmillan in the UK is an imprint of Macmillan Publishers Limited, registered in England, company number 785998, of Houndmills, Basingstoke, Hampshire RG21 6XS. -
The History of Valentine Camp by Mary Farrell
History of Valentine Camp Mary M. Farrell Trans-Sierran Archaeological Research P.O. Box 840 Lone Pine, CA 93545 November 7, 2015 Prepared for Valentine Eastern Sierra Reserve University of California, Santa Barbara, Natural Reserve System Sierra Nevada Aquatic Research Laboratory 1016 Mt. Morrison Road Mammoth Lakes, CA 93546 Abstract Located in Mammoth Lakes, California, Valentine Camp and the nearby Sierra Nevada Aquatic Research Laboratory form the Valentine Eastern Sierra Reserve, a field research station in the University of California's Natural Reserve System. The University’s tenure at Valentine Camp began over 40 years ago, but the area’s history goes back thousands of years. Before the arrival of Euroamericans in the nineteenth century, the region was home to Paiutes and other Native American tribes. Land just east of Valentine Camp was surveyed under contract with the United States government in 1856, and mineral deposits in the mountains just west of Valentine Camp brought hundreds of miners to the vicinity in the last decades of the nineteenth century. Even as mining in the region waned, grazing increased. The land that became Valentine Camp was patented in 1897 by Thomas Williams, a rancher and capitalist who lived in Owens Valley. It was Williams’s son, also Thomas, who sold the 160 acres to Valentine Camp’s founders. Those founders were very wealthy, very influential men in southern California who could have, and did, vacation wherever they wanted. Anyone familiar with the natural beauty of Mammoth Lakes would not be surprised that they chose to spend time at Valentine Camp. Valentine Camp was donated to the University of California Natural Land and Water Reserve System (now the Natural Reserve System) in 1972 to ensure the land’s continued protection. -
Go for Lunar Landing Conference Report
CONFERENCE REPORT Sponsored by: REPORT OF THE GO FOR LUNAR LANDING: FROM TERMINAL DESCENT TO TOUCHDOWN CONFERENCE March 4-5, 2008 Fiesta Inn, Tempe, AZ Sponsors: Arizona State University Lunar and Planetary Institute University of Arizona Report Editors: William Gregory Wayne Ottinger Mark Robinson Harrison Schmitt Samuel J. Lawrence, Executive Editor Organizing Committee: William Gregory, Co-Chair, Honeywell International Wayne Ottinger, Co-Chair, NASA and Bell Aerosystems, retired Roberto Fufaro, University of Arizona Kip Hodges, Arizona State University Samuel J. Lawrence, Arizona State University Wendell Mendell, NASA Lyndon B. Johnson Space Center Clive Neal, University of Notre Dame Charles Oman, Massachusetts Institute of Technology James Rice, Arizona State University Mark Robinson, Arizona State University Cindy Ryan, Arizona State University Harrison H. Schmitt, NASA, retired Rick Shangraw, Arizona State University Camelia Skiba, Arizona State University Nicolé A. Staab, Arizona State University i Table of Contents EXECUTIVE SUMMARY..................................................................................................1 INTRODUCTION...............................................................................................................2 Notes...............................................................................................................................3 THE APOLLO EXPERIENCE............................................................................................4 Panelists...........................................................................................................................4 -
Historical Painting Techniques, Materials, and Studio Practice
Historical Painting Techniques, Materials, and Studio Practice PUBLICATIONS COORDINATION: Dinah Berland EDITING & PRODUCTION COORDINATION: Corinne Lightweaver EDITORIAL CONSULTATION: Jo Hill COVER DESIGN: Jackie Gallagher-Lange PRODUCTION & PRINTING: Allen Press, Inc., Lawrence, Kansas SYMPOSIUM ORGANIZERS: Erma Hermens, Art History Institute of the University of Leiden Marja Peek, Central Research Laboratory for Objects of Art and Science, Amsterdam © 1995 by The J. Paul Getty Trust All rights reserved Printed in the United States of America ISBN 0-89236-322-3 The Getty Conservation Institute is committed to the preservation of cultural heritage worldwide. The Institute seeks to advance scientiRc knowledge and professional practice and to raise public awareness of conservation. Through research, training, documentation, exchange of information, and ReId projects, the Institute addresses issues related to the conservation of museum objects and archival collections, archaeological monuments and sites, and historic bUildings and cities. The Institute is an operating program of the J. Paul Getty Trust. COVER ILLUSTRATION Gherardo Cibo, "Colchico," folio 17r of Herbarium, ca. 1570. Courtesy of the British Library. FRONTISPIECE Detail from Jan Baptiste Collaert, Color Olivi, 1566-1628. After Johannes Stradanus. Courtesy of the Rijksmuseum-Stichting, Amsterdam. Library of Congress Cataloguing-in-Publication Data Historical painting techniques, materials, and studio practice : preprints of a symposium [held at] University of Leiden, the Netherlands, 26-29 June 1995/ edited by Arie Wallert, Erma Hermens, and Marja Peek. p. cm. Includes bibliographical references. ISBN 0-89236-322-3 (pbk.) 1. Painting-Techniques-Congresses. 2. Artists' materials- -Congresses. 3. Polychromy-Congresses. I. Wallert, Arie, 1950- II. Hermens, Erma, 1958- . III. Peek, Marja, 1961- ND1500.H57 1995 751' .09-dc20 95-9805 CIP Second printing 1996 iv Contents vii Foreword viii Preface 1 Leslie A. -
The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile. -
(Owen Willans) Richardson
O. W. (Owen Willans) Richardson: An Inventory of His Papers at the Harry Ransom Center Descriptive Summary Creator: Richardson, O. W. (Owen Willans), 1879-1959 Title: O. W. (Owen Willans) Richardson Papers Dates: 1898-1958 (bulk 1920-1940) Extent: 112 document boxes, 2 oversize boxes (49.04 linear feet), 1 oversize folder (osf), 5 galley folders (gf) Abstract: The papers of Sir O. W. (Owen Willans) Richardson, the Nobel Prize-winning British physicist who pioneered the field of thermionics, contain research materials and drafts of his writings, correspondence, as well as letters and writings from numerous distinguished fellow scientists. Call Number: MS-3522 Language: Primarily English; some works and correspondence written in French, German, or Italian . Note: The Ransom Center gratefully acknowledges the assistance of the Center for History of Physics, American Institute of Physics, which provided funds to support the processing and cataloging of this collection. Access: Open for research Administrative Information Additional The Richardson Papers were microfilmed and are available on 76 Physical Format reels. Each item has a unique identifying number (W-xxxx, L-xxxx, Available: R-xxxx, or M-xxxx) that corresponds to the microfilm. This number was recorded on the file folders housing the papers and can also be found on catalog slips present with each item. Acquisition: Purchase, 1961 (R43, R44) and Gift, 2005 Processed by: Tessa Klink and Joan Sibley, 2014 Repository: The University of Texas at Austin, Harry Ransom Center Richardson, O. W. (Owen Willans), 1879-1959 MS-3522 2 Richardson, O. W. (Owen Willans), 1879-1959 MS-3522 Biographical Sketch The English physicist Owen Willans Richardson, who pioneered the field of thermionics, was also known for his work on photoelectricity, spectroscopy, ultraviolet and X-ray radiation, the electron theory, and quantum theory. -
NASA Ames to Establish Nationwide Lunar Science Institute
November 2007 Worden gives upbeat message about future work for Ames BY JOHN BLUCK "We have switched material to In an upbeat talk to a crowd that phenolic impregnated carbon abla- filled the Ames main auditorium, tor (PICA), a (heat shield) material Ames Center Director S. Pete Worden developed here," Worden noted. His outlined an exciting future at Ames projected slide also listed Ames as that includes new work in exploration, leading PICA development and test- science and aeronautics -- each about a ing both for the Crew Exploration Ve- third of the center's efforts, he said. "I hicle, now called Orion, and the Mars have a gazillion charts to go through," Science Laboratory (MSL), which has photo by Eric James NASA he said. a planned launch date in fall 2009. His wide-ranging presentation Worden said that Ames' arc jets about Ames touched on moon explo- facility "a unique facility in the world." ration, a lunar institute, moon dust re- He added, "We want to upgrade search, heat shield work for spacecraft them." destined for the moon and Mars, a Mars sample "cache box" assignment, Life Sciences rising supercomputer capability, small "We are getting additional life Ames Center Director S. Pete Worden responds satellite work with a potential for support tasks assigned by Johnson to a question during the recent upbeat talk he many missions, increased astrobiology (and Marshall)," Worden said. "This is gave to the center about the future of Ames. work, growing cooperation among significant." continued on page 5 academia, and commercial partners and Ames and much more. -
South Pole-Aitken Basin
Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole. -
Appendix a Recovery of Ejecta Material from Confirmed, Probable
Appendix A Recovery of Ejecta Material from Confirmed, Probable, or Possible Distal Ejecta Layers A.1 Introduction In this appendix we discuss the methods that we have used to recover and study ejecta found in various types of sediment and rock. The processes used to recover ejecta material vary with the degree of lithification. We thus discuss sample processing for unconsolidated, semiconsolidated, and consolidated material separately. The type of sediment or rock is also important as, for example, carbonate sediment or rock is processed differently from siliciclastic sediment or rock. The methods used to take and process samples will also vary according to the objectives of the study and the background of the investigator. We summarize below the methods that we have found useful in our studies of distal impact ejecta layers for those who are just beginning such studies. One of the authors (BPG) was trained as a marine geologist and the other (BMS) as a hard rock geologist. Our approaches to processing and studying impact ejecta differ accordingly. The methods used to recover ejecta from unconsolidated sediments have been successfully employed by BPG for more than 40 years. A.2 Taking and Handling Samples A.2.1 Introduction The size, number, and type of samples will depend on the objective of the study and nature of the sediment/rock, but there a few guidelines that should be followed regardless of the objective or rock type. All outcrops, especially those near industrialized areas or transportation routes (e.g., highways, train tracks) need to be cleaned off (i.e., the surface layer removed) prior to sampling. -
Odd Year Nur-Rn-Lic-30550 G
LicenseNumber FirstName MiddleName LastName RenewalGroup NUR-LPN-LIC-6174 DOLORES ROSE AABERG 2019 - ODD YEAR NUR-RN-LIC-30550 GRETCHEN ELLEN AAGAARD-SHIVELY 2019 - ODD YEAR NUR-RN-LIC-128118 CAMBRIA LAUREN AANERUD 2019 - ODD YEAR NUR-RN-LIC-25862 SOPHIA SABINA AANSTAD 2018 - EVEN YEAR NUR-APRN-LIC-124944 ERIN EDWARD AAS 2018 - EVEN YEAR NUR-RN-LIC-105371 ERIN EDWARD AAS 2018 - EVEN YEAR NUR-RN-LIC-34536 BRYON AAS 2019 - ODD YEAR NUR-RN-LIC-39208 JULIA LYNN AASEN 2018 - EVEN YEAR NUR-APRN-LIC-130522 LORI ANN AASEN 2019 - ODD YEAR NUR-RN-LIC-130520 LORI ANN AASEN 2019 - ODD YEAR NUR-RN-LIC-21015 DEBBIE ABAR 2018 - EVEN YEAR NUR-APRN-LIC-130757 LUKE G ABAR 2018 - EVEN YEAR NUR-RN-LIC-130756 LUKE GORDON ABAR 2019 - ODD YEAR NUR-RN-LIC-31911 AIMEE KRISTINE ABBOTT 2018 - EVEN YEAR NUR-RN-LIC-29448 DENISE M ABBOTT 2018 - EVEN YEAR NUR-RN-LIC-131150 SARAH FRANCES ABBOTT 2018 - EVEN YEAR NUR-LPN-LIC-31701 ANGIE ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-33325 HEIDI ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-4920 LORI ANN ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-97426 DAYMON ABBOTT Expired - 2018 - EVEN YEAR NUR-RN-LIC-13260 ROBERT C ABBOTT Expired - 2018 - EVEN YEAR NUR-RN-LIC-17858 MONICA MAY ABDALLAH 2018 - EVEN YEAR NUR-RN-LIC-48890 STEVEN P ABDALLAH 2019 - ODD YEAR NUR-APRN-LIC-101391 LANEICE LORRAINE ABDEL-SHAKUR Expired - 2018 - EVEN YEAR NUR-RN-LIC-101333 LANEICE LORRAINE ABDEL-SHAKUR Expired - 2018 - EVEN YEAR NUR-RN-LIC-96606 RENDI L ABEL 2018 - EVEN YEAR NUR-RN-LIC-97338 LAURA ANN ABEL 2019 - ODD YEAR NUR-RN-LIC-69876 LACEY ANN ABELL 2019 - ODD YEAR NUR-RN-LIC-131932 -
Experimentally Demonstrated the Intrinsic Instability of the Fluorite-Type Zr Cation Network
0246110 Rta(i) 1 1,2 l,4 1,6 1,l 2 22 Rta(i) Figure 2. Temperature dependence of Zr-FTfor pure orthorhombic zirconia Figure 3 Temperature dependence of Zr-0 shell in tetragonal zirconia solid solution Our study has experimentally demonstrated the intrinsic instability of the fluorite-type Zr cation network. Coherent scattering beween Conclusions central Zr ion and distant cations is weaker and vibration modes of the Zr-cation network are It is found that, for all of zirconia solid softer in tetragonal zirconia than in monoclmic, solutions studied, the dopant-oxygen distances are orthorhombic, or stabilized cubic zirconia. In si@icantly ddferent from the Zr-0 distances. addition, the outer foux oxygens in the 8-fold The dopant-cation distances, on the other hand, coordinated Zr-0 polyhedron are only loosely are usually very close to the Zr-Zr distance, solutions. A bonded and are subject to very large static and confirming the formation of solid dynamic distortions. This effect is illustrated by general structural picture for zirconia solid the expanded portion of the Fourier transform solutions is one that places the dopant cations shown in Figure 3. randomly on tbe Zr sites in the cation network, but with distorted and sometimes very different Dopant Structure dopant-oxygen polyhedra surrounding these dopants. In the case of Ge4+ doping and Y-Nb We have also successfully performed co-doping, short-rangecation ordering has been EXAFS experiments at the dopant absorption suggested from our EXAFS results. edges for doped zirconia solid solutions. Dopants Based on the above structural information studied include the Ce-,Nb-, and Y-K edges as and other EXAFS results obtained from NSLS, well as Ce-LIn edge. -
R-700 MIT's ROLE in PROJECT APOLLO VOLUME I PROJECT
R-700 MIT’s ROLE IN PROJECT APOLLO FINAL REPORT ON CONTRACTS NAS 9-153 AND NAS 9-4065 VOLUME I PROJECT MANAGEMENT SYSTEMS DEVELOPMENT ABSTRACTS AND BIBLIOGRAPHY edited by James A. Hand OCTOBER 1971 CAMBRIDGE, MASSACHUSETTS, 02139 ACKNOWLEDGMENTS This report was prepared under DSR Project 55-23890, sponsored by the Manned Spacecraft Center of the National Aeronautics and Space Administration. The description of project management was prepared by James A. Hand and is based, in large part, upon discussions with Dr. C. Stark Draper, Ralph R. Ragan, David G. Hoag and Lewis E. Larson. Robert C. Millard and William A. Stameris also contributed to this volume. The publication of this document does not constitute approval by the National Aeronautics and Space Administration of the findings or conclusions contained herein. It is published for the exchange and stimulation of ideas. @ Copyright by the Massachusetts Institute of Technology Published by the Charles Stark Draper Laboratory of the Massachusetts Institute of Technology Printed in Cambridge, Massachusetts, U. S. A., 1972 ii The title of these volumes, “;LJI’I”s Role in Project Apollo”, provides but a mcdest hint of the enormous range of accomplishments by the staff of this Laboratory on behalf of the Apollo program. Rlanss rush into spaceflight during the 1060s demanded fertile imagination, bold pragmatism, and creative extensions of existing tecnnologies in a myriad of fields, The achievements in guidance and control for space navigation, however, are second to none for their critical importance in the success of this nation’s manned lunar-landing program, for while powerful space vehiclesand rockets provide the environment and thrust necessary for space flight, they are intrinsicaily incapable of controlling or guiding themselves on a mission as complicated and sophisticated as Apollo.