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Imaginative Geographies of Mars: the Science and Significance of the Red Planet, 1877 - 1910
Copyright by Kristina Maria Doyle Lane 2006 The Dissertation Committee for Kristina Maria Doyle Lane Certifies that this is the approved version of the following dissertation: IMAGINATIVE GEOGRAPHIES OF MARS: THE SCIENCE AND SIGNIFICANCE OF THE RED PLANET, 1877 - 1910 Committee: Ian R. Manners, Supervisor Kelley A. Crews-Meyer Diana K. Davis Roger Hart Steven D. Hoelscher Imaginative Geographies of Mars: The Science and Significance of the Red Planet, 1877 - 1910 by Kristina Maria Doyle Lane, B.A.; M.S.C.R.P. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2006 Dedication This dissertation is dedicated to Magdalena Maria Kost, who probably never would have understood why it had to be written and certainly would not have wanted to read it, but who would have been very proud nonetheless. Acknowledgments This dissertation would have been impossible without the assistance of many extremely capable and accommodating professionals. For patiently guiding me in the early research phases and then responding to countless followup email messages, I would like to thank Antoinette Beiser and Marty Hecht of the Lowell Observatory Library and Archives at Flagstaff. For introducing me to the many treasures held deep underground in our nation’s capital, I would like to thank Pam VanEe and Ed Redmond of the Geography and Map Division of the Library of Congress in Washington, D.C. For welcoming me during two brief but productive visits to the most beautiful library I have seen, I thank Brenda Corbin and Gregory Shelton of the U.S. -
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. -
Elias Acevedo Travis Adams Trevor Adams Storme Adkins Ricky Amador Linda Allen Dylan Allison Isaac Allison Nathaniel Aguirre Allison
Elias Acevedo Travis Adams Trevor Adams Storme Adkins Ricky Amador Linda Allen Dylan Allison Isaac Allison Nathaniel Aguirre Allison Steven Allison Morgan Amerto Candela Arturo Arriaga Efrain Arriaga Jessica Aten Chase Baird Andrew Baldwin Sarah Ballard Anderson Rojas Benjamin Ballew Christian Banks Matthew Bartlett Regina Bartlett Andrew Beasley Dawson Beck Kieran Becker Brandon Bennett Payton Berryhill Hienzelleman Alyson Adrian Blackwell Caylie Aubrey Boeke Jeremy Bonner Charity Boylen Kyle Bradley Rodney Bradley Beverly Blackwelder Blankenship Hunter Bray Lorene Bristol Rachel Brooks David Brown Parker Brown Kristopher Aaron Buchanan Jacob Buchanan Magnolia Bryant Buchanan Taylor Buchanan Kimberly Kasey Burnette Mariya Burnette Seth Burnette Kynieshra Burns Crislyn Buzbee Ysabela Cable Ashley Cadwell Burleson Abby Calhoun Eduardo Dylan Campbell Ivy Carroll Katelyn Carroll Shawn Carroll Taven Carson Julie Carver Rebecca Caudill Campanur Sarah Causby Kyle Chapman Josie Chilcote Hailey Clark Lesley Clark Mackenzie Clark Coby Conley Hannah Conley Lea Conner Kelsey Kathleen Marco Jarrett Cothron Joshua Cox Makayla Cox Sierra Cox Cameron Crater Daniel Creson Charles Dale Cooper Cornejo-Martinez Carmen Daniels Addison Davis Ashton Davis Brian Davis Caden Davis Joseph Davis Conner Deese Dante Dejesus Katryna Devroude Samantha Krystal Dugan Loretta Edwards Cameron Effler Bailey Elliott Maalik Elliott Matthew Cole England Cheyenne Esque Dominguez Emerson Charles Faurote Callie Fender Damon Fender Kenneth Kayleigh Floyd McKenna Foster Sadie -
Football State Championship Single Game Record Book 11 Man.Xlsx
OSAA State Championship Football Games, 11-Man Single-Game Records see separate record book for 8-man records INDIVIDUAL TEAM OFFENSE OFFENSE MOST YARDS RUSHING MOST POINTS SCORED 357, Andy Taylor, McNary vs. Sheldon, 2001 62, West Linn vs. Central Catholic, 2016 MOST RUSHING ATTEMPTS MOST POINTS, HALF 43, 2 tied 48 (1st), Marist vs. Baker, 2009 MOST RUSHING TOUCHDOWNS MOST POINTS, QUARTER 6, Keanon Lowe, Jesuit vs. Sheldon, 2009 28 (2nd), 2 tied LONGEST RUN HIGHEST COMBINED SCORE 91 (TD), Trevor Tinney, Santiam vs. Kennedy, 2018 99, McNary 51, Beaverton 48, 1997 MOST PASS ATTEMPTS LOWEST COMBINED SCORE 55, Sam Vidlak, Hidden Valley vs Santiam Christian, 2019 0, 3 tied MOST PASS COMPLETIONS MOST TOUCHDOWNS 39, Sam Vidlak, Hidden Valley vs Santiam Christian, 2019 9, 2 tied BEST COMPLETION PERCENTAGE (MIN. 15 ATT) MOST RUSHING ATTEMPTS 86.1 (31-for-36), Cade Knighton, Central Catholic vs Lake Oswego, 2019 70, Dayton vs. Neah-Kah-Nie, 1985 MOST YARDS PASSING MOST RUSHING YARDS 479, Sam Vidlak, Hidden Valley vs Santiam Christian, 2019 489, Vale vs. Harrisburg, 2014 LONGEST PASS MOST RUSHING TOUCHDOWNS 98 (TD), Dalton Reimers to Kody Nelson, Grant Union vs. Regis, 2013 7, 3 tied MOST PASSING TOUCHDOWNS MOST PASS ATTEMPTS 6, Taylor Barton, Beaverton vs. McNary, 1997 55, Hidden Valley vs Santiam Christian, 2019 MOST INTERCEPTIONS THROWN MOST PASS COMPLETIONS 7 (on 18 att.), Lee, Churchill vs. Corvallis, 1979 39, Hidden Valley vs Santiam Christian, 2019 MOST RECEPTIONS MOST PASSING YARDS 18, Jeremiah Noga, Hidden Valley vs Santiam Christian, 2019 479, Hidden Valley vs Santiam Christian, 2019 MOST RECEIVING YARDS MOST PASSING TOUCHDOWNS 270, Jeremiah Noga, Hidden Valley vs Santiam Christian, 2019 7, Beaverton vs. -
Family Group Sheets Surname Index
PASSAIC COUNTY HISTORICAL SOCIETY FAMILY GROUP SHEETS SURNAME INDEX This collection of 660 folders contains over 50,000 family group sheets of families that resided in Passaic and Bergen Counties. These sheets were prepared by volunteers using the Societies various collections of church, ceme tery and bible records as well as city directo ries, county history books, newspaper abstracts and the Mattie Bowman manuscript collection. Example of a typical Family Group Sheet from the collection. PASSAIC COUNTY HISTORICAL SOCIETY FAMILY GROUP SHEETS — SURNAME INDEX A Aldous Anderson Arndt Aartse Aldrich Anderton Arnot Abbott Alenson Andolina Aronsohn Abeel Alesbrook Andreasen Arquhart Abel Alesso Andrews Arrayo Aber Alexander Andriesse (see Anderson) Arrowsmith Abers Alexandra Andruss Arthur Abildgaard Alfano Angell Arthurs Abraham Alje (see Alyea) Anger Aruesman Abrams Aljea (see Alyea) Angland Asbell Abrash Alji (see Alyea) Angle Ash Ack Allabough Anglehart Ashbee Acker Allee Anglin Ashbey Ackerman Allen Angotti Ashe Ackerson Allenan Angus Ashfield Ackert Aller Annan Ashley Acton Allerman Anners Ashman Adair Allibone Anness Ashton Adams Alliegro Annin Ashworth Adamson Allington Anson Asper Adcroft Alliot Anthony Aspinwall Addy Allison Anton Astin Adelman Allman Antoniou Astley Adolf Allmen Apel Astwood Adrian Allyton Appel Atchison Aesben Almgren Apple Ateroft Agar Almond Applebee Atha Ager Alois Applegate Atherly Agnew Alpart Appleton Atherson Ahnert Alper Apsley Atherton Aiken Alsheimer Arbuthnot Atkins Aikman Alterman Archbold Atkinson Aimone -
In T Er Na Sj O Nale O Per a Sj O
Internasjonale operasjoner rapport første halvår 2013 INTERNASJONALE OPERASJONER 02 forsvaret — internasjonale operasjoner innholD Forsvarets operative hovedkvarter Forsvarets operative hovedkvarter i Bodø er ansvarlig for den daglige oppfølgingen av Forsvarets operasjoner både i Norge og i utlandet. Gjennom rapportering og jevnlig besøk i de internasjonale operasjonene, får hovedkvarteret en god situasjonsforståelse. s. 48 ∫ europa miNerydderstyrkeN Norske mineryddere deltar aktivt i jakten på sjøminer, torpedoer og luftbomber som ligger igjen etter verdenskrigene. s. 42 ∫ aFrika deN demokratiske repuBLikkeNkoNGo Forsvaret er til stede med én offiser i bidraget som skal beskytte sivilbefolk- ningen i den demokratiske republikkenkongo.dette er FNs største fredsbeva- rende styrke. Deltakelse i internasjonale Forsvaret i kroner 2013 operasjoner styrker forsvarets evne til å operere sammen meD våre allierte, noe som er en forutsetning for et i miLLioNer kroNer: effektivt forsvar av norge. driFtnorge ForsvarssjeF Harald sunde 73 % 24 % driFtnorge investering 25 055 investering 8382 operasjoner 3 % i utlandet operasjoner i utlandet 1096 tallene viser de midlene som det er budsjettert med for hele 2013 til de internasjonale operasjonene i adenbukta, afghanistan, Bosnia-Hercegovina, kongo, kosovo, midtøsten og sør-sudan. Forsvaret 2013 INTERNASJONALE OPERASJONER 03 s. 52 ∫ europa luFtovervåkiNg med hovedkvarter i tyskland bidrar 24 nord- menn for å sikre luftrom- Innsats ute, met over europa og sørge s. 54 ∫ s. 50 ∫ for varsling. europa sikkerhet hjemme europa traNsportFly iNato Forsvarets viktigste oppgave er å forsvare Norge. Norge har sammen med For å løse denne oppgaven må Forsvaret først BosNia-HercegoviNa elleve andre land gått til og fremst drive realistisk trening og øving, alene den unge nasjonen skal innkjøp av tre enorme og med våre allierte, under norske forhold. -
Psychology of Space Exploration Psychology of About the Book Douglas A
About the Editor Contemporary Research in Historical Perspective Psychology of Space Exploration Psychology of About the Book Douglas A. Vakoch is a professor in the Department As we stand poised on the verge of a new era of of Clinical Psychology at the California Institute of spaceflight, we must rethink every element, including Integral Studies, as well as the director of Interstellar Space Exploration the human dimension. This book explores some of the Message Composition at the SETI Institute. Dr. Vakoch Contemporary Research in Historical Perspective contributions of psychology to yesterday’s great space is a licensed psychologist in the state of California, and Edited by Douglas A. Vakoch race, today’s orbiter and International Space Station mis- his psychological research, clinical, and teaching interests sions, and tomorrow’s journeys beyond Earth’s orbit. include topics in psychotherapy, ecopsychology, and meth- Early missions into space were typically brief, and crews odologies of psychological research. As a corresponding were small, often drawn from a single nation. As an member of the International Academy of Astronautics, intensely competitive space race has given way to inter- Dr. Vakoch chairs that organization’s Study Groups on national cooperation over the decades, the challenges of Interstellar Message Construction and Active SETI. communicating across cultural boundaries and dealing Through his membership in the International Institute with interpersonal conflicts have become increasingly of Space Law, he examines -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
Glossary of Lunar Terminology
Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Characterization of Lunar Crater Ejecta Deposits Using Radar Data from the Mini-Rf Instrument on Lro
44th Lunar and Planetary Science Conference (2013) 2380.pdf CHARACTERIZATION OF LUNAR CRATER EJECTA DEPOSITS USING RADAR DATA FROM THE MINI-RF INSTRUMENT ON LRO. G.W. Patterson, J.T.S. Cahill, and D.B.J. Bussey. Johns Hopkins University Applied Physics Laboratory, Laurel, MD ([email protected]). Introduction: Impact cratering is the dominant formulation the key inputs are the degree of weathering process on the surface of the Moon and a polarization, m, 2 2 2 1/2 primary means of distributing material on the lunar m = (S2 +S3 +S4 ) /S1 surface [1]. Radar data provide unique information on and the degree of circularity, χ, both the horizontal and vertical distribution of impact sin2χ = − S4/mS1. deposits [2]. The Miniature Radio Frequency (Mini- The m−chi decomposition is expressed through a RF) instrument flown on NASAs Lunar Reconnais- color-coded image with, sance Orbiter (LRO) is a Synthetic Aperture Radar R = [m S1 (1 + sin2χ)/2] (SAR) with an innovative hybrid dual-polarimetric G = [S1 (1 – m)] architecture that transmits a circularly polarized signal, B = [mS1 (1 – sin2χ)/2] and receives orthogonal linear polarizations and their where R represents the double-bounce component, G relative phase [3]. The four Stokes parameters that represents the random-polarized (volume scattering) characterize the observed backscattered EM field are component, and the B represents the single-bounce calculated from the received data. These parameters component of backscatter in an observed scene. can be used to produce a variety of derived products Analysis (Byrgius A): Byrgius A is a 19 km di- that provide unique information on the radar scattering ameter Copernican crater located in the lunar highlands properties of a surface. -
Powell Bill Streets Listing FY2012
Powell Bill Streets Listing FY2012 This report is a listing of all streets and street segments that the City of Charlotte, North Carolina had under municipal maintenance for fiscal year 2012 (July 1, 2011 to June 30, 2012). TOTAL MILES OF CITY MAINTAINED STREETS FOR FY2012: 2,434.64 Contact information is as follows: David Snider, PLS City Survey Manager City of Charlotte Engineering Property Management Real Estate Division Survey/Mapping/GIS Section 600 East 4th Street Charlotte, NC 28202 704-336-3875 [email protected] Monday - Friday 7am to 4pm City of Charlotte Powell Bill Report FY2012 Street Name Miles Street Name Miles W 10TH ST 0.41 E 28TH ST 0.13 E 10TH ST 0.18 W 28TH ST 0.69 E 10TH ST 0.47 E 28TH ST 0.17 E 10TH ST 0.08 W 29TH ST 0.11 W 11TH ST 0.08 W 2ND ST 0.21 E 11TH ST 0.67 W 30TH ST 0.28 W 11TH ST 0.09 W 31ST ST 0.17 E 12TH ST 0.75 W 32ND ST 0.42 W 12TH ST 0.10 E 32ND ST 0.11 W 12TH ST 0.34 E 33RD ST 0.11 W 12th St 0.05 E 34TH ST 0.21 E 13TH ST 0.14 E 34TH ST 0.23 E 13TH ST 0.06 E 34TH ST 0.05 E 15TH ST 0.21 E 35TH ST 1.10 W 15TH ST 0.07 E 36TH ST 1.05 E 15TH ST 0.32 E 37TH ST 0.29 E 16TH ST 0.30 E 3RD ST 0.65 E 16TH ST 0.20 W 3RD ST 0.39 E 16TH ST 0.27 W 4TH ST 0.50 E 17TH ST 0.39 E 4TH ST 0.70 E 17TH ST 0.15 E 4TH ST 0.60 E 18TH ST 0.62 W 4TH ST 0.07 E 19TH ST 0.09 W 4TH ST 0.21 E 19TH ST 0.35 W 4TH EXTENSION 0.86 W 1ST ST 0.25 W 5TH ST 0.60 E 1ST ST 0.04 W 5TH ST 0.40 W 1ST ST 0.12 E 5TH ST 0.66 E 20TH ST 0.30 W 5TH ST 0.32 E 20TH ST 0.04 E 5TH ST 0.08 E 21ST ST 0.17 E 5TH ST 1.07 E 22ND ST 0.18 W 6TH ST 0.06 E