DOCSLIB.ORG

Elements Vol3

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Elements Vol3 ELEMENTS The Citadel School of Science and Mathematics Newsletter Vol. 3 No. 1 Fall 2010 DEAN’S MESSAGE Dear Friends of the School of Science and Mathematics: The faculty and staff of the School of Science and Mathematics have had a very active and productive AY’09-’10. Despite tight budget constraints and the challenges they presented, the faculty has not wavered in its efforts to deliver top quality education, out-of-classroom enrichment experiences, and dedicated mentoring to our students. Our professors continue to advance in scholarship and in the disciplines as they actively seek opportunities for professional growth. The Citadel launched several initiatives in ’09-’10 that involve the School of Science and Mathematics in significant ways. STEM (Science Technology Engineering and Mathematics) education has been named a strategic priority in the Citadel BLUEPRINT and a STEM Center of Excellence has been inaugurated as a new collaborative entity among the Schools of Education, Engineering, and Science and Mathematics. Carolyn Kelly has come on board as the director of the STEM Center. The Citadel has become a participating institution in the Piedmont Southeast Atlantic Cooperative Ecosystem Study Units (see the news from Biology below), and the Department of Health Exercise and Sport Science has established, with funding from BiteTech, Inc. the Dr. Hank Cross Human Performance Laboratory under the directorship of Dr. Dena Garner. The School of Science and Mathematics said farewell to two veteran faculty members (see below) and welcomes three new faculty members in 2010 - all in the Department of Mathematics and Computer Science. Doctors Upasana Kashyap and Antara Mukherjee join the department as tenure track assistant professors in mathematics and Stephen Cotter will be a mathematics instructor. Dr. Kashyap is a specialist in operator theory (operator algebras) with a Ph.D. from the University of Houston and Dr. Mukherjee, Ph.D., University of Oklahoma, is a geometer specializing in geometric group theory. Mr. Cotter (Col USAF, ret.; Citadel ’70) holds an MAT degree in mathematics from The Citadel and has taught high school mathematics in Charleston and Summerville. More information on activities and events in the School may be found in the pages that follow. We always strive to keep lines of communication open. Please phone (843-953-5300) or email ( [email protected] ) me with your thoughts, suggestions or concerns relating to science and mathematics education or the workings of The Citadel School of Science and Mathematics. Chuck Groetsch, Dean 2010 Distinguished Alumnus Award Tom Trotter William T. (Tom) Trotter was the First Honor Graduate (B.S., Mathematics) of the class of 1965. Tom was a member of F Company, serving as Guidon Corporal, First Sergeant and then Battalion Executive Officer. Also, he was Editor-in-Chief of the Guidon, a member of the Roundtable and the Junior Sword Drill, and co-captain of the swimming team. After summer employment with NASA in Huntsville, Tom was awarded a NASA Fellowship at the University of Alabama, completing his Ph.D. in topology in 1969 and returning to The Citadel as an Assistant Professor in the fall of 1969. In 1971, Tom made a substantial change in research directions and began to tackle problems in combinatorial mathematics. On the basis of research advances made at an NSF summer conference in 1971, Tom was invited to Dartmouth College as a Visiting Assistant Professor for the 1972-73 academic year. In the fall of 1973, he moved to the University of South Carolina, where he advanced through the ranks and was named a Carolina Research Professor in 1985. He also served as Assistant Dean of the College of Sciences (1979- 85) and played a major role in the establishment of the Departments of Computer Science and Statistics. In 1987, Tom was recruited to Arizona State University, where he served as Professor and Chair of the Department of Mathematics (1987-91 and 1995-97), Vice Provost for Academic Affairs (2000-02), and was named Regents Professor in 1992. From 1991-94, he served as Director of Combinatorics and Optimization at Bellcore in Morristown, New Jersey. In 2002, Tom was recruited to the Georgia Institute of Technology as Professor and Chair of the School of Mathematics. His term as Chair ended in the summer of 2009 and he continues to serve as Professor of Mathematics. Throughout his career, Tom has maintained a very active research profile with more then 120 refereed journal publications and a very successful research monograph on partially ordered sets which is still a top seller after nearly two decades in print. Tom’s work has been consistently funded by grants from the National Science Foundation and the Department of Defense. He has served on numerous grant panels and review teams, and he has held several editorial positions, including eight years as Editor-in-Chief of Order. He has given about 150 invited lectures at international conferences, and at leading universities and national meetings in the US and abroad. Tom has supervised eight Ph.D. students and currently has three students working toward their degree under his supervision. Two will finish in spring of 2010, and one of them (Mitch Keller) has just received a Marshall Sherfield Fellowship for post-doctoral study in England. Mitch is the first mathematics Ph.D. to receive this fellowship. Tom and his wife Millie have three children, Laura, Russ and Matt. In his spare time, he loves to hit golf balls, continuing a life-time love affair with all things athletic. DR. HANK CROSS HUMAN PERFORMANCE LABORATORY In May 2010, construction of the Dr. Hank Cross Human Performance Laboratory began. This new lab is located on the first floor of Deas Hall and includes a conference room and a 12-person computer lab. The project will be completed in August 2010, and has been made possible through a very generous gift from Bite Tech, Incorporated, which has supported research in the Department of Health, Exercise, and Sport Science for several years. The Dr. Hank Cross Human Performance Laboratory will be a state-of-the-art, high-technology learning laboratory used for: Continuing research on use of the Bite Tech mouthpiece during exercise as it relates to changes in levels of the stress hormone cortisol, airway openings, lactate levels, and changes in oxygen and carbon dioxide kinetics in various populations such as college-aged, middle-aged, and older populations. This research will help move this beneficial product to market, and also increase the profile of The Citadel as the research center for the product, which is being promoted and marketed by Under Armour and Patterson Dental. Assessing other hormonal and stress markers related to athletes and their performance. Understanding effects of exercise and nutrition on cancer survivors. Conducting a multitude of other research and studies related to human performance and physical fitness including height/weight assessments for on- campus students and others off-campus who want an understanding of their physical fitness levels related to body composition. A center for cooperative research with other universities and The Department of Defense with the goal of improving performance of military personnel. HESS alumni have been asked to consider sending a monetary gift to the Citadel Foundation for one or more of the equipment needs for the lab. All donors will be invited to the grand opening and dedication of the Dr. Hank Cross Human Performance Laboratory in fall 2010, possibly to coincide with Homecoming November 5-6, 2010. Donors will also be recognized with a plaque in the new lab. The Citadel at the iGEM Competition A new research team has formed at The Citadel. Two Biology majors, Hunter Matthews and Brian Burnley, and one Electrical Engineering major, Patrick Sullivan are participating in the international competition for synthetic biology, known as iGEM (International Genetically Engineered Machines). This competition was organized by MIT in 2004, and is recognized as a premiere venue for genetic engineering at the undergraduate level. The main purpose of the competition is to promote the use of standard and interchangeable parts (known as “BioBricks”) in designing new genetic systems in microbial species. The organizers provide each team with a kit of “Bookracks”, and include instructions for the students to make their own. By the end of the summer, the genetic systems built by the teams should be able to operate in living cells and introduce a new and interesting function. The competition has received acclaim for fostering scientific skills like team-work, self-organization, independent learning and biosafety. Several members of the team recently attended the annual iGEM national meeting held at the University of Illinois at Urbana-Champagne. The students and their mentors learned about projects at other participating institutions and were able to take some of what they learned back to The Citadel to apply to their project. The students also set up a booth at the Charleston Farmer’s Market to provide information about synthetic biology to the general public. During this summer the Citadel-Charleston team has been working on “Appetite Regulation Proteins in E.coli ”, and will be presenting its work at the iGEM Jamboree in Boston this November. Their project has had the financial support of the Office of the Provost and the Department of Biology. Scientific support has been provided by Dr. David Donnell and Dr. Claudia Rocha from the Department of Biology. The Citadel iGEM team at the iGEM national conference held at the University of Illinois. Pictured are (l to r) Patrick Sullivan, Dr. David Donnell, Dr. Claudia Rocha, and Brian Burnley Brian Burnley explains the concept and use of synthetic biology at the Charleston Farmer’s Market. Citadel Community Bids Farewell to Comer and Greim Steve Comer and Peter Greim This year the School of Science and Mathematics bids a fond farewell to two long-time stalwarts in the Department of Mathematics and Computer Science: Steve Comer and Peter Greim.
Load more

Recommended publications
  • INFORMATION to USERS the Most Advanced Technology Has Been Used to Photo­ Graph and Reproduce This Manuscript from the Microfilm Master
    INFORMATION TO USERS The most advanced technology has been used to photo­ graph and reproduce this manuscript from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are re­ produced by sectioning the original, beginning at the upper left-hand corner and continuing from left to right in equal sections with small overlaps. Each original is also photographed in one exposure and is included in reduced form at the back of the book. These are also available as one exposure on a standard 35mm slide or as a 17" x 23" black and white photographic print for an additional charge. Photographs included in the original manuscript have been reproduced xerographically in this copy. Higher quality 6" x 9" black and white photographic prints are available for any photographs or illustrations appearing in this copy for an additional charge. Contact UMI directly to order. University Microfilms International A Bell & Howell Information Company 300 North Zeeb Road, Ann Arbor, Ml 48106-1346 USA 313/761-4700 800/521-0600 Order Number 9002012 Laser-tissue interactions in the arterial wall Roberts, Cynthia Jane, Ph.D.
    [Show full text]
  • No. 40. the System of Lunar Craters, Quadrant Ii Alice P
    NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates.
    [Show full text]
  • 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.
    [Show full text]
  • Getting out of Jail Free: Sentence Credit for Periods of Mistaken Liberty
    Catholic University Law Review Volume 45 Issue 2 Winter 1996 Article 3 1996 Getting out of Jail Free: Sentence Credit for Periods of Mistaken Liberty Gabriel J. Chin Follow this and additional works at: https://scholarship.law.edu/lawreview Recommended Citation Gabriel J. Chin, Getting out of Jail Free: Sentence Credit for Periods of Mistaken Liberty, 45 Cath. U. L. Rev. 403 (1996). Available at: https://scholarship.law.edu/lawreview/vol45/iss2/3 This Article is brought to you for free and open access by CUA Law Scholarship Repository. It has been accepted for inclusion in Catholic University Law Review by an authorized editor of CUA Law Scholarship Repository. For more information, please contact [email protected]. GETTING OUT OF JAIL FREE: SENTENCE CREDIT FOR PERIODS OF MISTAKEN LIBERTY Gabriel J. Chin* "The criminal is to go free because the constable has blundered."' When an individual is convicted of a crime and sentenced to a term of imprisonment, it generally is assumed that the convicted person is taken into custody after sentencing as ordered by the court. Surprisingly, how- ever, ministerial officers of the criminal justice system sometimes improp- erly release convicted criminals from custody or fail to take them into custody after sentencing. If the error never comes to the attention of the government, no legal issue is raised, and the convicted person may simply remain at liberty. Sometimes, however, the erroneously released pris- oner raises the issue with the government, or the government discovers the error on its own. In such cases, the law must determine whether a convict should receive credit for the time erroneously at liberty.
    [Show full text]
  • Biodiversity: the UK Overseas Territories. Peterborough, Joint Nature Conservation Committee
    Biodiversity: the UK Overseas Territories Compiled by S. Oldfield Edited by D. Procter and L.V. Fleming ISBN: 1 86107 502 2 © Copyright Joint Nature Conservation Committee 1999 Illustrations and layout by Barry Larking Cover design Tracey Weeks Printed by CLE Citation. Procter, D., & Fleming, L.V., eds. 1999. Biodiversity: the UK Overseas Territories. Peterborough, Joint Nature Conservation Committee. Disclaimer: reference to legislation and convention texts in this document are correct to the best of our knowledge but must not be taken to infer definitive legal obligation. Cover photographs Front cover: Top right: Southern rockhopper penguin Eudyptes chrysocome chrysocome (Richard White/JNCC). The world’s largest concentrations of southern rockhopper penguin are found on the Falkland Islands. Centre left: Down Rope, Pitcairn Island, South Pacific (Deborah Procter/JNCC). The introduced rat population of Pitcairn Island has successfully been eradicated in a programme funded by the UK Government. Centre right: Male Anegada rock iguana Cyclura pinguis (Glen Gerber/FFI). The Anegada rock iguana has been the subject of a successful breeding and re-introduction programme funded by FCO and FFI in collaboration with the National Parks Trust of the British Virgin Islands. Back cover: Black-browed albatross Diomedea melanophris (Richard White/JNCC). Of the global breeding population of black-browed albatross, 80 % is found on the Falkland Islands and 10% on South Georgia. Background image on front and back cover: Shoal of fish (Charles Sheppard/Warwick
    [Show full text]
  • Science Concept 5: Lunar Volcanism Provides a Window Into the Thermal and Compositional Evolution of the Moon
    Science Concept 5: Lunar Volcanism Provides a Window into the Thermal and Compositional Evolution of the Moon Science Concept 5: Lunar volcanism provides a window into the thermal and compositional evolution of the Moon Science Goals: a. Determine the origin and variability of lunar basalts. b. Determine the age of the youngest and oldest mare basalts. c. Determine the compositional range and extent of lunar pyroclastic deposits. d. Determine the flux of lunar volcanism and its evolution through space and time. INTRODUCTION Features of Lunar Volcanism The most prominent volcanic features on the lunar surface are the low albedo mare regions, which cover approximately 17% of the lunar surface (Fig. 5.1). Mare regions are generally considered to be made up of flood basalts, which are the product of highly voluminous basaltic volcanism. On the Moon, such flood basalts typically fill topographically-low impact basins up to 2000 m below the global mean elevation (Wilhelms, 1987). The mare regions are asymmetrically distributed on the lunar surface and cover about 33% of the nearside and only ~3% of the far-side (Wilhelms, 1987). Other volcanic surface features include pyroclastic deposits, domes, and rilles. These features occur on a much smaller scale than the mare flood basalts, but are no less important in understanding lunar volcanism and the internal evolution of the Moon. Table 5.1 outlines different types of volcanic features and their interpreted formational processes. TABLE 5.1 Lunar Volcanic Features Volcanic Feature Interpreted Process
    [Show full text]
  • Arxiv:2012.11628V3 [Astro-Ph.EP] 26 Jan 2021
    manuscript submitted to JGR: Planets The Fundamental Connections Between the Solar System and Exoplanetary Science Stephen R. Kane1, Giada N. Arney2, Paul K. Byrne3, Paul A. Dalba1∗, Steven J. Desch4, Jonti Horner5, Noam R. Izenberg6, Kathleen E. Mandt6, Victoria S. Meadows7, Lynnae C. Quick8 1Department of Earth and Planetary Sciences, University of California, Riverside, CA 92521, USA 2Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 3Planetary Research Group, Department of Marine, Earth, and Atmospheric Sciences, North Carolina State University, Raleigh, NC 27695, USA 4School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA 5Centre for Astrophysics, University of Southern Queensland, Toowoomba, QLD 4350, Australia 6Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA 7Department of Astronomy, University of Washington, Seattle, WA 98195, USA 8Planetary Geology, Geophysics and Geochemistry Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA Key Points: • Exoplanetary science is rapidly expanding towards characterization of atmospheres and interiors. • Planetary science has similarly undergone rapid expansion of understanding plan- etary processes and evolution. • Effective studies of exoplanets require models and in-situ data derived from plan- etary science observations and exploration. arXiv:2012.11628v4 [astro-ph.EP] 8 Aug 2021 ∗NSF Astronomy and Astrophysics Postdoctoral Fellow Corresponding author: Stephen R. Kane, [email protected] {1{ manuscript submitted to JGR: Planets Abstract Over the past several decades, thousands of planets have been discovered outside of our Solar System. These planets exhibit enormous diversity, and their large numbers provide a statistical opportunity to place our Solar System within the broader context of planetary structure, atmospheres, architectures, formation, and evolution.
    [Show full text]
  • DMAAC – February 1973
    LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base.
    [Show full text]
  • NINETY-NINE 9\Je\Ns
    NINETY-NINE THE INTERNATIONAL WOMEN PILOT S MAGAZINE J _________ November-December,N 1993 • Crater Lake Flyers • !Ange(s — Corporate Angel Network • Becoming a “FED” Successful Board Meeting Reflects Fresh Outlook Just ask the Governors who were present; they didn’t pick up their knitting once - well, maybe once! The fall Board agenda was packed with items for discussion and action. On pages 10, 11 and 15 of this issue you’ll find detailed reports covering many of the items we evaluated, discussed, voted on, remanded for additional President’s Message information or to a committee, etc. We selected a new N e w s editor, Betty Rowley, and extended our thanks to Ann Cooper for her wonderful effort as editor. We discussed an informal proposal made by a member of the Atchison Historical Society Board that The 99s consider deeding 60 percent ownership of the Amelia Earhart Birthplace Museum to the Historical Society. In exchange, an undefined amount of funding for restoration would be made available. The Board unanimously decided they needed considerably more information Board members Alexis Koehler, Connie Woods, Joyce Wells, Gene Nora Jessen, Doris before an accurate assessment of this Abbate, Lee Orr, Carolyn Carpp, Lu Hollander and Lois Erickson pause during a full early-stage proposal could be fairly Board meeting schedule to look at one of the many early-day scrapbooks housed at 99s' International Headquarters. evaluated and acted upon. This addi­ tional information has been requested from the 99s’ Birthplace Museum Board, and will be available for further consideration prior to the spring Board meeting.
    [Show full text]
  • 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
    [Show full text]
  • National Blue Ribbon Schools Recognized 1982-2015
    NATIONAL BLUE RIBBON SCHOOLS PROGRAM Schools Recognized 1982 Through 2015 School Name City Year ALABAMA Academy for Academics and Arts Huntsville 87-88 Anna F. Booth Elementary School Irvington 2010 Auburn Early Education Center Auburn 98-99 Barkley Bridge Elementary School Hartselle 2011 Bear Exploration Center for Mathematics, Science Montgomery 2015 and Technology School Beverlye Magnet School Dothan 2014 Bob Jones High School Madison 92-93 Brewbaker Technology Magnet High School Montgomery 2009 Brookwood Forest Elementary School Birmingham 98-99 Buckhorn High School New Market 01-02 Bush Middle School Birmingham 83-84 C.F. Vigor High School Prichard 83-84 Cahaba Heights Community School Birmingham 85-86 Calcedeaver Elementary School Mount Vernon 2006 Cherokee Bend Elementary School Mountain Brook 2009 Clark-Shaw Magnet School Mobile 2015 Corpus Christi School Mobile 89-90 Crestline Elementary School Mountain Brook 01-02, 2015 Daphne High School Daphne 2012 Demopolis High School Demopolis 2008 East Highland Middle School Sylacauga 84-85 Edgewood Elementary School Homewood 91-92 Elvin Hill Elementary School Columbiana 87-88 Enterprise High School Enterprise 83-84 EPIC Elementary School Birmingham 93-94 Eura Brown Elementary School Gadsden 91-92 Forest Avenue Academic Magnet Elementary School Montgomery 2007 Forest Hills School Florence 2012 Fruithurst Elementary School Fruithurst 2010 George Hall Elementary School Mobile 96-97 George Hall Elementary School Mobile 2008 1 of 216 School Name City Year Grantswood Community School Irondale 91-92 Guntersville Elementary School Guntersville 98-99 Heard Magnet School Dothan 2014 Hewitt-Trussville High School Trussville 92-93 Holtville High School Deatsville 2013 Holy Spirit Regional Catholic School Huntsville 2013 Homewood High School Homewood 83-84 Homewood Middle School Homewood 83-84, 96-97 Indian Valley Elementary School Sylacauga 89-90 Inverness Elementary School Birmingham 96-97 Ira F.
    [Show full text]
  • User Guide to 1:250,000 Scale Lunar Maps
    CORE https://ntrs.nasa.gov/search.jsp?R=19750010068Metadata, citation 2020-03-22T22:26:24+00:00Z and similar papers at core.ac.uk Provided by NASA Technical Reports Server USER GUIDE TO 1:250,000 SCALE LUNAR MAPS (NASA-CF-136753) USE? GJIDE TO l:i>,, :LC h75- lu1+3 SCALE LUNAR YAPS (Lumoalcs Feseclrch Ltu., Ottewa (Ontario) .) 24 p KC 53.25 CSCL ,33 'JIACA~S G3/31 11111 DANNY C, KINSLER Lunar Science Instltute 3303 NASA Road $1 Houston, TX 77058 Telephone: 7131488-5200 Cable Address: LUtiSI USER GUIDE TO 1: 250,000 SCALE LUNAR MAPS GENERAL In 1972 the NASA Lunar Programs Office initiated the Apollo Photographic Data Analysis Program. The principal point of this program was a detailed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17. One of the requirements of this program was the production of detailed photo base maps at a useable scale. NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas. This paper is designed to present in outline form the neces- sary background informatiox or users to become familiar with the program. MAP FORMAT * The scale chosen for the project was 1:250,000 . The re- search being done required a scale that Principal Investigators (PI'S) using orbital photography could use, but would also serve PI'S doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west.
    [Show full text]