Extraterrestrialmaterials Processingand Construction
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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. -
COURT of CLAIMS of THE
REPORTS OF Cases Argued and Determined IN THE COURT of CLAIMS OF THE STATE OF ILLINOIS VOLUME 39 Containing cases in which opinions were filed and orders of dismissal entered, without opinion for: Fiscal Year 1987 - July 1, 1986-June 30, 1987 SPRINGFIELD, ILLINOIS 1988 (Printed by authority of the State of Illinois) (65655--300-7/88) PREFACE The opinions of the Court of Claims reported herein are published by authority of the provisions of Section 18 of the Court of Claims Act, Ill. Rev. Stat. 1987, ch. 37, par. 439.1 et seq. The Court of Claims has exclusive jurisdiction to hear and determine the following matters: (a) all claims against the State of Illinois founded upon any law of the State, or upon an regulation thereunder by an executive or administrative ofgcer or agency, other than claims arising under the Workers’ Compensation Act or the Workers’ Occupational Diseases Act, or claims for certain expenses in civil litigation, (b) all claims against the State founded upon any contract entered into with the State, (c) all claims against the State for time unjustly served in prisons of this State where the persons imprisoned shall receive a pardon from the Governor stating that such pardon is issued on the grounds of innocence of the crime for which they were imprisoned, (d) all claims against the State in cases sounding in tort, (e) all claims for recoupment made by the State against any Claimant, (f) certain claims to compel replacement of a lost or destroyed State warrant, (g) certain claims based on torts by escaped inmates of State institutions, (h) certain representation and indemnification cases, (i) all claims pursuant to the Law Enforcement Officers, Civil Defense Workers, Civil Air Patrol Members, Paramedics and Firemen Compensation Act, (j) all claims pursuant to the Illinois National Guardsman’s and Naval Militiaman’s Compensation Act, and (k) all claims pursuant to the Crime Victims Compensation Act. -
Group Ii Xenoliths from Lunar Crater Volcanic Field, Nevada: Implications For
GROUP II XENOLITHS FROM LUNAR CRATER VOLCANIC FIELD, NEVADA: IMPLICATIONS FOR SUBDUCTED PLATE METASOMATISM by JOHN CLARK MOSELY, JR. Under the Direction of MICHAEL F. RODEN ABSTRACT Lunar Crater Volcanic Field (LCVF), a Quaternary volcanic field in central Nevada, is characterized by alkali basalts that host megacrysts of clinopyroxene, amphibole and olivine as well as mafic and ultramafic xenoliths. The Group II xenoliths present at LCVF offer insight in to the complex magmatic processes at play beneath the volcanic field, as well as providing context for Tertiary and Quaternary volcanism in the western United States. Petrologic and geochemical analysis of these xenoliths and the constituent phases are consistent with genesis from a magma enriched in Ti and Al. High modal abundance of amphibole, as well as the presence of anomalously OH and Cl rich apatite within the xenoliths could be attributed to melting of a source rock enriched in water and chlorine. The geochemistry of xenoliths at LCVF is similar to that of subduction driven magmatism observed at island arcs and convergent margins but occurs well inland. Mantle enrichment by the dehydration of the shallowly subducted Farallon plate and subsequent melting of this enriched mantle allows for and is consistent with the hydrous xenoliths and the anomalous apatite hosted within them. GROUP II XENOLITHS FROM LUNAR CRATER VOLCANIC FIELD, NEVADA: IMPLICATIONS FOR SUBDUCTED PLATE METASOMATISM by JOHN CLARK MOSELY, JR. B.S., University of Georgia, 2010 A Thesis Submitted to the Graduate Faculty of The University of Georgia in Partial Fulfillment of the Requirements for the Degree MASTER OF SCIENCE ATHENS, GEORGIA 2015 © 2015 John Clark Mosely, Jr. -
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, -
PROJECT STREET from to MORATORIUM START FY09-Slurry
PROJECT STREET FROM TO MORATORIUM START FY09-Slurry 01ST AV W WALNUT AV UPAS ST 5/7/2010 FY09-Slurry 01ST AV UPAS ST THORN ST 5/7/2010 FY09-Slurry 01ST AV THORN ST SPRUCE ST 5/7/2010 FY10-Overlay 01ST AV PENNSYLVANIA AV BROOKES AV 7/12/2010 FY10-Slurry 01ST AV LEWIS ST W WASHINGTON ST 1/9/2012 FY10-Slurry 01ST AV ARBOR DR MONTECITO WY 1/11/2012 FY10-Slurry 01ST AV MONTECITO WY LEWIS ST 1/11/2012 FY10-Slurry 01ST AV W WASHINGTON ST UNIVERSITY AV 1/11/2012 FY10-Slurry 01ST AV UNIVERSITY AV ROBINSON AV 1/11/2012 FY11-Slurry 01ST AV BEECH ST ASH ST 9/9/2012 FY11-Slurry 01ST AV ASH ST A ST 9/9/2012 FY11-Slurry 01ST AV A ST W B ST 9/9/2012 FY11-Slurry 01ST AV W B ST C ST 9/9/2012 FY11-Slurry 01ST AV ELM ST CEDAR ST 9/9/2012 FY11-Slurry 01ST AV CEDAR ST BEECH ST 9/9/2012 FY11-Overlay 01ST AV ROBINSON AV PENNSYLVANIA AV 10/10/2012 FY08-Overlay 02ND AV ASH ST A ST 4/10/2009 FY09-Overlay 02ND AV C ST BROADWAY 11/3/2009 FY09-Slurry 02ND AV WALNUT AV UPAS ST 5/26/2010 FY09-Slurry 02ND AV UPAS ST THORN ST 5/26/2010 FY09-Slurry 02ND AV THORN ST SPRUCE ST 5/26/2010 FY11-Overlay 02ND AV MARKET ST ISLAND AV 10/16/2012 FY11-Overlay 02ND AV ISLAND AV J ST 10/16/2012 FY09-Slurry 03RD AV LEWIS ST WASHINGTON ST 5/7/2010 FY09-Slurry 03RD AV END ARBOR DR 5/27/2010 FY09-Slurry 03RD AV ARBOR DR MONTECITO WY 5/28/2010 FY09-Slurry 03RD AV MONTECITO WY LEWIS ST 5/28/2010 FY10-Slurry 03RD AV WALNUT AV UPAS ST 1/11/2012 FY11-Slurry 03RD AV UNIVERSITY AV ROBINSON AV 6/5/2012 FY11-Slurry 03RD AV ROBINSON AV PENNSYLVANIA AV 6/5/2012 FY11-Slurry 03RD AV PENNSYLVANIA AV -
Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America
Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America There are approximately 101,135sexual abuse claims filed. Of those claims, the Tort Claimants’ Committee estimates that there are approximately 83,807 unique claims if the amended and superseded and multiple claims filed on account of the same survivor are removed. The summary of sexual abuse claims below uses the set of 83,807 of claim for purposes of claims summary below.1 The Tort Claimants’ Committee has broken down the sexual abuse claims in various categories for the purpose of disclosing where and when the sexual abuse claims arose and the identity of certain of the parties that are implicated in the alleged sexual abuse. Attached hereto as Exhibit 1 is a chart that shows the sexual abuse claims broken down by the year in which they first arose. Please note that there approximately 10,500 claims did not provide a date for when the sexual abuse occurred. As a result, those claims have not been assigned a year in which the abuse first arose. Attached hereto as Exhibit 2 is a chart that shows the claims broken down by the state or jurisdiction in which they arose. Please note there are approximately 7,186 claims that did not provide a location of abuse. Those claims are reflected by YY or ZZ in the codes used to identify the applicable state or jurisdiction. Those claims have not been assigned a state or other jurisdiction. Attached hereto as Exhibit 3 is a chart that shows the claims broken down by the Local Council implicated in the sexual abuse. -
Doc 7281 290 En.Pdf
Department of State Publication 11038 Office of the Secretary of State Office of the Coordinator for Counterterrorism Internet address: http//www.state.gov/s/ct/rls/ Released April 2003 United States Department of State April 2003 © Reuters In a speech at the Jimmy Doolittle Flight Facility in Columbia, South Carolina, on 24 October 2002, President George W. Bush promised to prosecute the war on terror with “patience, focus, and determination.” i* Introduction by Ambassador Cofer Black Coordinator for Counterterrorism The evil of terrorism continued to plague the world throughout 2002, from Bali to Grozny to Mombasa. At the same time, the global war against the terrorist threat was waged intensively in all regions with encouraging results. The year saw the liberation of Afghanistan by Coalition forces, the expulsion of al-Qaida and the oppressive Taliban regime, the destruction of their terrorist training infrastructure, and the installation of a transitional government committed to democracy and economic development. Al-Qaida terrorists are on the run, and thousands of them have been detained. More than one third of al-Qaida’s top leadership has been killed or captured, including some who conspired in the September 11 attacks, the 2000 attack on the USS Cole, and the 1998 bombings of two US Embassies in East Africa. Moreover, the global antiterrorism coalition that was forged in the immediate aftermath of the September 11 attacks in the United States remains united. The world is fighting terrorism on five fronts: diplomatic, intelligence, law enforcement, financial, and military. Diplomatic The progress that has been achieved in the global war on terrorism would not have been possible without intense diplomatic engagement throughout the world. -
Communications of the LUNAR and PLANETARY LABORATORY
Communications of the LUNAR AND PLANETARY LABORATORY Number 70 Volume 5 Part 1 THE UNIVERSITY OF ARIZONA 1966 Communications of the Lunar and Planetary Laboratory These Communications contain the shorter publications and reports by the staff of the Lunar and Planetary Laboratory. They may be either original contributions, reprints of articles published in professional journals, preliminary reports, or announcements. Tabular material too bulky or specialized for regular journals is included if future use of such material appears to warrant it. The Communications are issued as separate numbers, but they are paged and indexed by volumes. The Communications are mailed to observatories and to laboratories known to be engaged in planetary, interplanetary or geophysical research in exchange for their reports and publica- tions. The University of Arizona Press can supply at cost copies to other libraries and interested persons. The University of Arizona GERARD P. KUIPER, Director Tucson, Arizona Lunar and Planetary Laboratory Published with the support of the National Aeronautics and Space Administration Library of Congress Catalog Number 62-63619 NO. 70 THE SYSTEM OF LUNAR CRATERS, QUADRANT IV by D. W. G. ARTHUR, RUTH H. PELLICORI, AND C. A. WOOD May25,1966 , ABSTRACT The designation, diameter, position, central peak information, and state of completeness are listed for each discernible crater with a diameter exceeding 3.5 km in the fourth lunar quadrant. The catalog contains about 8,000 items and is illustrated by a map in 11 sections. hiS Communication is the fourth and final part of listed in the catalog nor shown in the accompanying e System of Lunar Craters, which is a_calalag maps. -
Transportation Development Division
SECTION II TRAFFIC VOLUMES ON STATE HIGHWAYS An asterisk (*) appearing to the left of a count location description indicates an Automatic Traffic Recorder (ATR) Station or Automatic Vehicle Classification (AVC) Station. See Section IV of this book for 2017 monthly traffic volumes, high hour volumes or historical trends at these stations. 29 30 2017 TRAFFIC VOLUMES ON STATE HIGHWAYS 2017 AADT All ATR Milepoint Vehicles AVC Location Description PACIFIC HIGHWAY NO. 1 Milepoint indicates distance from Oregon-California State Line 0.00 16900 Oregon-California State Line 5.02 16800 0.30 mile south of Siskiyou Interchange Neil Creek Automatic Traffic Recorder, Sta. 15-002, 0.86 mile south of Rogue Valley Highway No. 63 11.03 17200 * Interchange (OR99) 13.67 16600 0.50 mile south of Green Springs Highway Interchange (OR66) 18.11 28100 * North Ashland Automatic Traffic Recorder, Sta. 15-021, 0.98 mile south of North Ashland Interchange 19.87 39000 0.77 mile north of North Ashland Interchange 23.90 41500 0.50 mile south of Fern Valley Road Interchange 26.91 43100 0.30 mile south of South Medford Interchange Medford Viaduct Automatic Traffic Recorder, Sta. 15-019, 1.96 miles southeast of the North Medford 28.33 53200 * Interchange 30.59 42700 0.30 mile north of Crater Lake Highway Interchange (OR62) 34.94 38800 0.50 mile south of Seven Oaks Interchange 36.04 41100 0.60 mile north of Seven Oaks Interchange 42.84 40000 * Gold Hill Automatic Traffic Recorder, Sta. 15-001, 2.77 miles south of the Homestead Interchange 44.97 40300 0.50 mile east of Rogue River Highway (OR99), Homestead Interchange 45.61 39300 On Rogue River Bridge 48.32 39100 0.50 mile east of Rogue River Interchange 55.38 37800 0.40 mile south of East Grants Pass Interchange (US199) 57.56 28600 0.50 mile south of Redwood Highway (OR99), North Grants Pass Interchange 61.05 31700 0.40 mile south of Louse Creek Interchange Grave Creek Automatic Traffic Recorder, Sta. -
A Wet Vs Dry Moon: Exploring Volatile Reservoirs and Implications
Program and Abstract Volume LPI Contribution No. 1621 A Wet vs. Dry Moon: Exploring Volatile Reservoirs and Implications for the Evolution of the Moon and Future Exploration June 13–15, 2011 • Houston, Texas Sponsors Curation and Analysis Planning Team for Extraterrestrial Materials (CAPTEM) Lunar Exploration Analysis Group (LEAG) Lunar and Planetary Institute (LPI) NASA Lunar Science Institute (NLSI) NASA Ralph Steckler Program Conveners Chip Shearer (University of New Mexico) Malcolm Rutherford (Brown University) Greg Schmidt (NASA Ames Research Center) Scientific Organizing Committee Don Bogard (Lunar and Planetary Institute-NASA Johnson Space Center) Ben Bussey (John Hopkins University, Advanced Physics Laboratory) Linda Elkins-Tanton (Massachusetts Institute of Technology) Penny King (University of New Mexico Gary Lofgren (NASA Johnson Space Center) Francis McCubbin (University of New Mexico) Carle Pieters (Brown University) Paul Spudis (Lunar and Planetary Institute) Edward Stolper (California Institute of Technology) Richard Vondrak (Goddard Space Flight Center) Diane Wooden (NASA Ames Research Center) Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Contribution No. 1621 Compiled in 2011 by Meeting and Publication Services Lunar and Planetary Institute USRA Houston 3600 Bay Area Boulevard, Houston TX 77058-1113 The Lunar and Planetary Institute is operated by the Universities Space Research Association under a cooperative agreement with the Science Mission Directorate of the National Aeronautics and Space Administration. Any opinions, findings, and conclusions or recommendations expressed in this volume are those of the author(s) and do not necessarily reflect the views of the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. -
Guide to Observing the Moon
Your guide to The Moonby Robert Burnham A supplement to 618128 Astronomy magazine 4 days after New Moon south is up to match the view in a the crescent moon telescope, and east lies to the left. f you look into the western sky a few evenings after New Moon, you’ll spot a bright crescent I glowing in the twilight. The Moon is nearly everyone’s first sight with a telescope, and there’s no better time to start watching it than early in the lunar cycle, which begins every month when the Moon passes between the Sun and Earth. Langrenus Each evening thereafter, as the Moon makes its orbit around Earth, the part of it that’s lit by the Sun grows larger. If you look closely at the crescent Mare Fecunditatis zona I Moon, you can see the unlit part of it glows with a r a ghostly, soft radiance. This is “the old Moon in the L/U. p New Moon’s arms,” and the light comes from sun- /L tlas Messier Messier A a light reflecting off the land, clouds, and oceans of unar Earth. Just as we experience moonlight, the Moon l experiences earthlight. (Earthlight is much brighter, however.) At this point in the lunar cycle, the illuminated Consolidated portion of the Moon is fairly small. Nonetheless, “COMET TAILS” EXTENDING from Messier and Messier A resulted from a two lunar “seas” are visible: Mare Crisium and nearly horizontal impact by a meteorite traveling westward. The big crater Mare Fecunditatis. Both are flat expanses of dark Langrenus (82 miles across) is rich in telescopic features to explore at medium lava whose appearance led early telescopic observ- and high magnification: wall terraces, central peaks, and rays.