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Monadnock Vol. 45 | June 1971
THE MONADNOCK I - L. .RK UNIVERSITY Vol. XLV )GRAPHICAL SOCIETY June, 1971 THE MQNADNOCK Volume XIN Editor, Edwin T. Wei5e, Jr. Aaooite Editor5 James FOnSeOa Kirsten Haring David Seairøn Photoqzapher, Ernie Wight ypists Ronnie Mason Phyllis sczynski 323812 ii ‘7f THE MONADNOCK CONTENTs . 2 DIRECT0I MESSAGE THE JESUITS IN NORTH AMERICA: A STUDY . IN ENVIRONMENTAL COCEUALIZATI Eenry Aay 4 STRUCTURE IN TRANSACTION SYSTEMS. .Christopher Clayton 9 CULTURE AND AGRICULTURE ON THE ANEPJCAN NTIER Brad Baltensperger 22 THE PROBABILISTIC APPROACH TO SPATIAL THEORY Kang-tsung Chang 30 AROHITECTURE AND GEOGRAPHICAL STUDIES: A REVIEW Stephen Hobart 36 AN ESSAY ON GROWTH POLE THEORY B. David Miller 40 MIND, MEANING, AND MILIEU: PSYCHOLOGICAL NEED AND DESIGRED ENVIRONMENTS Ernest A. Wight Jr 43 SPATIAL DYNAMICS IN CLASSICAL LOCATION THEORY Alfred Hecht 52 THE GRADUATE SCHOOL OF GEOGRAPHY 56 ALUMNI NEWS 65 A N(YTE ON THE QUESTIONNAIRE 80 :1 DIRECTOR’S MESSAGE This academic year is very special for Geography at Clark, marking the fiftieth year of the founding of the Graduate School of Geography by Wallace W. Atwood. Dedication of the new Geography facilities — with special recognition to the memory of John K. Wright, Historical Geographer and Geosophist, an adopted son of Clark — is one appropriate mode of celebration. Another mark of the occasion is the honor accorded to two major figures in American Geography: Clark could not have chosen two more distinguished geographers than Richard Hartshorne and Samuel Van Valkenburg on whom were bestowed .1 . - Honorary Doctorates of Law at the anniversary ceremonies of April .17th. Very different in their contributions and their characters, Richard Hartshorne provided American geography with its philosophic and method ological rationale and Dr. -
Mars Reconnaissance Orbiter
Chapter 6 Mars Reconnaissance Orbiter Jim Taylor, Dennis K. Lee, and Shervin Shambayati 6.1 Mission Overview The Mars Reconnaissance Orbiter (MRO) [1, 2] has a suite of instruments making observations at Mars, and it provides data-relay services for Mars landers and rovers. MRO was launched on August 12, 2005. The orbiter successfully went into orbit around Mars on March 10, 2006 and began reducing its orbit altitude and circularizing the orbit in preparation for the science mission. The orbit changing was accomplished through a process called aerobraking, in preparation for the “science mission” starting in November 2006, followed by the “relay mission” starting in November 2008. MRO participated in the Mars Science Laboratory touchdown and surface mission that began in August 2012 (Chapter 7). MRO communications has operated in three different frequency bands: 1) Most telecom in both directions has been with the Deep Space Network (DSN) at X-band (~8 GHz), and this band will continue to provide operational commanding, telemetry transmission, and radiometric tracking. 2) During cruise, the functional characteristics of a separate Ka-band (~32 GHz) downlink system were verified in preparation for an operational demonstration during orbit operations. After a Ka-band hardware anomaly in cruise, the project has elected not to initiate the originally planned operational demonstration (with yet-to-be used redundant Ka-band hardware). 201 202 Chapter 6 3) A new-generation ultra-high frequency (UHF) (~400 MHz) system was verified with the Mars Exploration Rovers in preparation for the successful relay communications with the Phoenix lander in 2008 and the later Mars Science Laboratory relay operations. -
Primitive Bodies Panel Planetary Science Decadal Survey Space Studies Board National Research Council
Space Studies Board Mailing Address: 500 Fifth Street, NW Washington, DC 20001 www.nationalacademies.org Primitive Bodies Panel Planetary Science Decadal Survey Space Studies Board National Research Council National Academy of Sciences Building 2101 Constitution Ave. NW, Washington, D.C. (Entrance at 2100 C Street NW) Conference Room 150 FINAL AGENDA1 September 9-11, 2009 Wednesday, September 9, 2009 CLOSED SESSION 7:30 a.m. Room Opens (Breakfast available in the meeting room) 8:30 a.m. Welcome and Agenda Review Joseph Veverka 8:45 a.m. Overview of NRC Study Process Dwayne Day 9:15 a.m. Balance and Composition Discussion Dwayne Day 10:00 a.m. Break OPEN SESSION2 10:15 a.m. Decadal Survey Overview Steven Squyres Cornell University 11:00 a.m. Lessons Learned from the 2003 Decadal Survey Dale Cruikshank NASA Ames Research Center 11:45 a.m. Committee Discussion (Lunch will be served in the meeting room, committee discussion will continue) 12:45 p.m. Charge to the Decadal Survey James Green/Lindley Johnson NASA Headquarters 1 Updated September 8, 2009 2 Webcast at http://nasa-nai.acrobat.com/primitive1/, Audio at 866-606-4717, Access Code 6686308. This meeting is being held to gather information to help the committee conduct its activities. The committee will examine the information and material obtained during open sessions in an effort to inform its work. Although opinions may be stated and lively discussion may ensue, no conclusions are being drawn at this time. Therefore, observers who draw conclusions about the committee's work based on today's discussions will be doing so prematurely. -
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. -
Course Descriptions
COURSE DESCRIPTIONS Architectural Design Technology COURSE DESCRIPTIONS The following course descriptions are intended to briefly describe the nature of each of the courses. For more complete information, AAD 180 Fundamentals of Design I 3 (2,2,0,0) departments or faculty can provide specific course syllabuses. Introduction to the principles and theories of design and design methodology in the “making” of representations of form and space. The numbers in the right side of each description define the credits and average weekly contact hours the student will spend AAD 182 Fundamentals of Design II 3 (2,2,0,0) in formal classes during a 16 week semester. Classes scheduled Continuation of AAD 180, with emphasis on spatial sequence, for other than a 16 week semester will have the contact hours tectonics, and design precedents. adjusted accordingly. Prerequisite: AAD 180. A – defines the number of semester credits B Architecture – average number of lecture hours per week C – average number of laboratory hours per week AAE 100 Introduction to Architecture 3 (3,0,0,0) D – average number of clinical hours per week Survey of architecture. Includes historical examples and the E – average number of other formal instructional hours per week theoretical, social, technical, and environmental forces that shape this profession. Especially for majors and non-majors who wish to explore this field as a career choice. Automotive Technology, Collision and Repair ABDY 101B Collision Repair Fundamentals and Estimating 4 (1,6,0,0) This lecture/lab course includes an overview of the collision industry, instruction in safe shop procedures, measurement, vehicle disassembly, and estimating software and techniques. -
Curriculum Vitae
DANTE S. LAURETTA Lunar and Planetary Laboratory Department of Planetary Sciences University of Arizona Tucson, AZ 85721-0092 Cell: (520) 609-2088 Email: [email protected] CHRONOLOGY OF EDUCATION Washington University, St. Louis, MO Dept. of Earth and Planetary Sciences Ph.D. in Earth and Planetary Sciences, 1997 Thesis: Theoretical and Experimental Studies of Fe-Ni-S, Be, and B Cosmochemistry Advisor: Bruce Fegley, Jr. University of Arizona, Tucson, AZ Depts. of Physics, Mathematics, and East Asian Studies B.S. in Physics and Mathematics, Cum Laude, 1993 B.A. in Oriental Studies (emphasis: Japanese), Cum Laude, 1993 CHRONOLOGY OF EMPLOYMENT Professor, Lunar and Planetary Laboratory, Dept. of Planetary Sciences, University of Arizona, Tucson, AZ; 2012 – present. Principal Investigator, OSIRIS-REx Asteroid Sample Return Mission, NASA New Frontiers Program, 2011 – present. Deputy Principal Investigator, OSIRIS-REx Asteroid Sample Return Mission, NASA New Frontiers Program, 2008 – 2011. Associate Professor, Lunar and Planetary Laboratory, Dept. of Planetary Sciences, University of Arizona, Tucson, AZ; 2006 – 2012. Assistant Professor, Lunar and Planetary Laboratory, Dept. of Planetary Sciences, University of Arizona, Tucson, AZ; 2001 – 2006. Associate Research Scientist, Dept. of Chemistry & Biochemistry, Arizona State University, Tempe, AZ; 1999 – 2001. Postdoctoral Research Associate, Dept. of Geology, Arizona State University, Tempe, AZ Primary project: Transmission electron microscopy of meteoritic minerals. Supervisor: Peter R. Buseck; Dates: 1997 – 1999. Research Assistant, Dept. of Earth and Planetary Sciences, Washington Univ., St. Louis, MO Primary project: Experimental studies of sulfide formation in the solar nebula. Advisor: Bruce Fegley, Jr.; Dates: 1993 – 1997. Research Intern, NASA Undergraduate Research Program, University of Arizona, Tucson, AZ Primary project: Development of a logic-based language for S.E.T.I. -
The Planetary Report
A Publication of THEPLANETA SOCIETY o o o • o -e o o Board of Directors CARL SAGAN NORMAN R. AUGUSTI NE President Chairman and CEO, Director, Martin Marietta Corporation Laboratory for Planetary Studies, Cornelf University JOHN E. BRYSON Chairman and CEO, BRUCE MURRAY Southern California Edison Vice President Professor of Planetary Science, JOSEPH RYAN California Institute of Technology O'Melveny & Myers LOU IS FRIEDMAN STEVEN SPI ELBERG A WARNING FROM YOUR EDITOR Bringing People Together Through Executive Director director and producer You may soon be getting a phone call Planetary Science-Page 13-Education Board of Advisors from me. No, I won't be asking you for has always been close to the hearts of DIANE ACKERMAN JOHN M. LOGSDON donations or nagging you about a missed Planetary Society members, and we have poet and author Director, Space Policy Institute, George Washington University deadline (a common fear among planetary sponsored many programs to promote sci BUZZ ALDRIN Apollo 11 astronaut HANS MARK scientists). Instead, I will be asking for ence education around the world. We've The University of Texas at Austin RICHARD BERENDZEN your opinion about The Planetary Report. gathered together reports on three projects educator and astrophysicist JAMES MICHENER author JACQUES BLAMONT Each month our computer will randomly now completed and one just beginning. Chief Scientist, Centre MARVIN MINSKY Nationa! d'Etudes Spatia/es, Toshiba Professor of Media Arts select several members whom I will call to A Planetary Readers' Service-Page 16- France and Sciences, Massachusetts Institute of Technology discuss the contents of our latest issue-or For most of its history, the science we call RAY BRADBURY poet and author PHILIP MORRISON any other topic related to our publications. -
Mro High Resolution Imaging Science Experiment (Hirise)
Sixth International Conference on Mars (2003) 3287.pdf MROHIGHRESOLUTIONIMAGINGSCIENCEEXPERIMENT(HIRISE): INSTRUMENTDEVELOPMENT.AlanDelamere,IraBecker,JimBergstrom,JonBurkepile,Joe Day,DavidDorn,DennisGallagher,CharlieHamp,JeffreyLasco,BillMeiers,AndrewSievers,Scott StreetmanStevenTarr,MarkTommeraasen,PaulVolmer.BallAerospaceandTechnologyCorp.,PO Box1062,Boulder,CO80306 Focus Introduction:Theprimaryfunctionalre- Mechanism PrimaryMirror quirementoftheHiRISEimager,figure1isto PrimaryMirrorBaffle 2nd Fold allowidentificationofbothpredictedandun- Mirror knownfeaturesonthesurfaceofMarstoa muchfinerresolutionandcontrastthanprevi- ouslypossible[1],[2].Thisresultsinacam- 1st Fold erawithaverywideswathwidth,6kmat Mirror 300kmaltitude,andahighsignaltonoise ratio,>100:1.Generationofterrainmaps,30 Filters cmverticalresolution,fromstereoimages Focal requiresveryaccurategeometriccalibration. Plane Theprojectlimitationsofmass,costand schedulemakethedevelopmentchallenging. FocalPlane SecondaryMirror Inaddition,thespacecraftstability[3]must Electronics TertiaryMirror SecondaryMirrorBaffle notbeamajorlimitationtoimagequality. Thenominalorbitforthesciencephaseofthe missionisa3pmorbitof255by320kmwith Figure1Cameraopticalpathoptimizedforlowmass periapsislockedtothesouthpole.Thetrack Integration(TDI)tocreateveryhigh(100:1)signalnoise velocityisapproximately3,400m/s. ratioimages. HiRISEFeatures:TheHiRISEinstrumentperformance Theimagerdesignisanall-reflectivethreemirrorastig- goalsarelistedinTable1.Thedesignfeaturesa50cm matictelescopewithlight-weightedZeroduropticsanda -
The Space-Based Global Observing System in 2010 (GOS-2010)
WMO Space Programme SP-7 The Space-based Global Observing For more information, please contact: System in 2010 (GOS-2010) World Meteorological Organization 7 bis, avenue de la Paix – P.O. Box 2300 – CH 1211 Geneva 2 – Switzerland www.wmo.int WMO Space Programme Office Tel.: +41 (0) 22 730 85 19 – Fax: +41 (0) 22 730 84 74 E-mail: [email protected] Website: www.wmo.int/pages/prog/sat/ WMO-TD No. 1513 WMO Space Programme SP-7 The Space-based Global Observing System in 2010 (GOS-2010) WMO/TD-No. 1513 2010 © World Meteorological Organization, 2010 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 these 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 No. 2300 Fax: +41 (0)22 730 80 40 CH-1211 Geneva 2, Switzerland E-mail: [email protected] FOREWORD The launching of the world's first artificial satellite on 4 October 1957 ushered a new era of unprecedented scientific and technological achievements. And it was indeed a fortunate coincidence that the ninth session of the WMO Executive Committee – known today as the WMO Executive Council (EC) – was in progress precisely at this moment, for the EC members were very quick to realize that satellite technology held the promise to expand the volume of meteorological data and to fill the notable gaps where land-based observations were not readily available. -
American Mathematical Association of Two-Year Colleges
American Mathematical Association of Two-Year Colleges Photo courtesy of Visit Phoenix/dspaz.com 47th AMATYC Annual Conference Keynote Speakers October 28 – 31, 2021 Lindy Elkins-Tanton Arizona State University The NASA Psyche Mission: Journey to a Metallic World Sheraton Phoenix Downtown 340 North 3rd Street Talithia Williams Harvey Mudd College Phoenix, AZ 85004 Power in Numbers: Reservations (online): Unveiling Hidden Figures https://tinyurl.com/AMATYC2021Sheraton Reservations (phone): 1.866.837.4213 ext. 4 (mention AMATYC Conference) Featured Speakers James Tanton Mathematical Association of America Opening Doors The Astounding Mathematics Through Mathematics of Bicycle Tracks Scott Adamson Chandler-Gilbert CC Fired Up to Take Online Teaching Innovations Back to the Classroom! Hosted by ArizMATYC and the Southwest Region www.amatyc.org Vision Statement To be the leading voice and resource for excellence in mathematics education in the first two years of college Mission Statement To provide high quality professional development, to advocate and collaborate at all levels, and to build communities of learners for all involved in mathematics education in the first two years of college. Adopted by the Board on April 1, 2016 Core Values These are the Core Values that guide AMATYC’s internal and external interactions with each other and our community: Academic Excellence Access Collegiality Innovation Integrity Professional Development Teaching Excellence KEYNOTE SPEAKERS Thursday Keynote Session Lindy Elkins-Tanton The NASA Psyche Mission: Journey to a Metallic World Thursday, October 28 3:00 pm – 4:30 pm “Psyche” is both the name of a metallic asteroid, and the name of the NASA mission to visit that asteroid. -
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, -
ELEMENTAL ABUNDANCES in METEORITIC CHONDRULES Abstract Approved: Redacted for Privacy Roman A
AN ABSTRACT OF THE THESIS OF THOMAS WARD OSBORN III for the Doctor of Philosophy . (Name) (Degree) in Chemistry presented on September 28, 1971 (Major) (Date) Title: ELEMENTAL ABUNDANCES IN METEORITIC CHONDRULES Abstract approved: Redacted for Privacy Roman A. Schmitt High-precision instrumental neutron activation analysis has been used to determine Al, Na, Mn, Sc, Cr, Fe, Co, and Ni in a suite of more than 500 chondrules from 26 distinct meteorites. These meteorite specimens represent the H, L, LL and C chemical classes and most of the petrologic types. In addition radiochemical activation analysis has been used to determine K, Rb and Cs in a suite of chon- drules from the LL chemical class. To a limited extent trace element data on individual chondrules were correlated with petrographic obser- vations on the same chondrules. I. In general it was found that the siderophilic elements Fe, Co, Ni and Ir are depleted in chondrules compared to the whole chon- drite. The lithophilic elements Na, Mn, Sc, Cr and Al are generally enriched in chondrules compared to the whole chondrite. In contrast to the other lithophilic elements, Rb and Cs are generally depleted in the chondrules. Both major and trace elements may exhibit multi- modal population distributions for the chondrules sets. II. Petrographic observations of the same chondrules for which trace element contents were determined by INAA suggest that the trace element distribution may be consistent with the mineral assemblages except for a positive Ir-Al and Al-Sc correlations which occur in many chondrule sets. Correlations between chondrule mass and Al, Na, Sc, Co, Lr and Cu contents were observed for certain chondrule sets.