The Baltic States and Tourism Development
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Planetary Geologic Mappers Annual Meeting
Program Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Planetary Geologic Mappers Annual Meeting June 12–14, 2018 • Knoxville, Tennessee Institutional Support Lunar and Planetary Institute Universities Space Research Association Convener Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Science Organizing Committee David Williams, Chair Arizona State University Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Robert Jacobsen Earth and Planetary Sciences Department, University of Tennessee Knoxville Bradley Thomson Earth and Planetary Sciences Department, University of Tennessee Knoxville Abstracts for this meeting are available via the meeting website at https://www.hou.usra.edu/meetings/pgm2018/ Abstracts can be cited as Author A. B. and Author C. D. (2018) Title of abstract. In Planetary Geologic Mappers Annual Meeting, Abstract #XXXX. LPI Contribution No. 2066, Lunar and Planetary Institute, Houston. Guide to Sessions Tuesday, June 12, 2018 9:00 a.m. Strong Hall Meeting Room Introduction and Mercury and Venus Maps 1:00 p.m. Strong Hall Meeting Room Mars Maps 5:30 p.m. Strong Hall Poster Area Poster Session: 2018 Planetary Geologic Mappers Meeting Wednesday, June 13, 2018 8:30 a.m. Strong Hall Meeting Room GIS and Planetary Mapping Techniques and Lunar Maps 1:15 p.m. Strong Hall Meeting Room Asteroid, Dwarf Planet, and Outer Planet Satellite Maps Thursday, June 14, 2018 8:30 a.m. Strong Hall Optional Field Trip to Appalachian Mountains Program Tuesday, June 12, 2018 INTRODUCTION AND MERCURY AND VENUS MAPS 9:00 a.m. Strong Hall Meeting Room Chairs: David Williams Devon Burr 9:00 a.m. -
The Granat Family History
The Granat Family History by Virginia Mapes March 17, 2012 Sweden The number of Swedes doubled between 1750 and 1850, and the growth continued. In a country with few industries and cities, the burden had to be carried by the primitive agricultural society. At the end of the 1860s, Sweden was struck by the last of a series of severe hunger catastrophes. The agriculture which was still only partially modernized had been struggling with difficult times. Now came a series of crop failures. 1867 thus became "the wet year" of rotting grain, 1868 became the "dry year" of burned fields, and 1869 became "the severe year" of epidemics and begging children. Sixty thousand people left Sweden during these three "starvation years." It was the beginning of the mass emigration which, with short intervals, was to continue up to World War I. (Written by Ulf Beijbom) John Richard Karlsson Per (John) Richard Karlsson was born May 24, 1882 in Hova, Sweden to Karl Karlsson and Lovisa Johansdotter. [Richard’s last name was changed from Karlsson to Granat when he was in the Swedish Military Service in 1905.] Richard recalled walking the trails to school. However when winter came and the snow was deep, he would ski to school. It was so much faster because he could ski over the tops of the fences creating a shorter route. Richard’s childhood years in Sweden are somewhat vague. He had a sister Ellen and there may have been other brothers and sisters. They were a very poor farm family. Richard remembered that he and the other children in the family were always hungry, for these were the starvation years for the farm workers. -
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. -
11 Prospectus.Indd
2011 SPRING PROSPECTUS Portland State VIKINGS 2011 PORTLAND STATE VIKINGS SCHEDULE Date Opponent Location Kickoff Sept. 3 SOUTHERN OREGON JELD-WEN FIELD TBA Sept. 10 open Sept. 17 NORTHERN ARIZONA* JELD-WEN FIELD TBA Sept. 24 @ TCU Fort Worth, TX TBA Oct. 1 @ Idaho State* Pocatello, ID TBA Oct. 8 MONTANA STATE* JELD-WEN FIELD TBA Oct. 15 @ Montana* Missoula, MT TBA Oct. 22 WILLAMETTE JELD-WEN FIELD TBA Oct. 29 @ Eastern Washington* Cheney, WA TBA Nov. 5 SACRAMENTO STATE* JELD-WEN FIELD TBA Nov. 12 @ Northern Colorado* Greeley, CO TBA Nov. 19 WEBER STATE* JELD-WEN FIELD TBA NCAA Playoffs: First Round, Nov. 20; Second Round, Dec. 3; Quarterfinals, Dec. 10 Semifinals, Dec. 16/17; National Championship, Jan. 6, Frisco, TX * Big Sky Conference game Game times will be released in June Radio: KXFD Freedom 970 AM TV: TBA Live Streaming Video: www.b2tv.com Live Stats: www.GoViks.com SR QB Connor Kavanaugh SR RB Cory McCaffrey Honorable Mention 1st team All-Big Sky All-Big Sky Conference Conference 2011 Spring Practice Portland State will practice every Monday, Wednesday and Friday from April 4 through May 4. Practice takes place at Stott Com- munity Field on the PSU campus from 1:30-4 p.m. 2011 Spring Game SR SS DeShawn Shead Portland State’s Annual Spring Game takes place on Saturday, 2nd team All-Big Sky Conference May 7, at 1 p.m. at Lincoln High School 2011 SPRING PROSPECTUS Portland State VIKINGS Physical Address ____________ 527 SW Hall, Suite 415, Portland, OR 97201 VIKING FOOTBALL COACHING STAFF Mailing Address _______________________ -
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. -
Style Specifications
Site Soundscapes Landscape architecture in the light of sound Per Hedfors Department of Landscape Planning Ultuna Uppsala Doctoral thesis Swedish University of Agricultural Sciences Uppsala 2003 Acta Universitatis Agriculturae Sueciae Agraria 407 ISSN 1401-6249 ISBN 91-576-6425-0 © 2003 Per Hedfors, Uppsala Tryck: SLU Service/Repro, Uppsala 2003 Abstract Hedfors, Per. 2003. Site Soundscapes – landscape architecture in the light of sound. Doctor’s dissertation. issn 1401-6249, isbn 91-576-6425-0. This research was based on the assumption that landscape architects work on pro- jects in which the acoustic aspects can be taken into consideration. In such projects activities are located within the landscape and specific sounds belong to specific activities. This research raised the orchestration of the soundscape as a new area of concern in the field of landscape architecture; a new method of approaching the problem was suggested. Professionals can learn to recognise the auditory phenom- ena which are characteristic of a certain type of land use. Acoustic sources are obvious planning elements which can be used as a starting point in the develop- ment process. The effects on the soundscape can subsequently be evaluated according to various planning options. The landscape is viewed as a space for sound sources and listeners where the sounds are transferred and coloured, such that each site has a specific soundscape – a sonotope. This raised questions about the landscape’s acoustic characteristics with respect to the physical layout, space, material and furnishing. Questions related to the planning process, land use and conflicts of interest were also raised, in addition to design issues such as space requirements and aesthetic considerations. -
Last Name First Name/Middle Name Course Award Course 2 Award 2 Graduation
Last Name First Name/Middle Name Course Award Course 2 Award 2 Graduation A/L Krishnan Thiinash Bachelor of Information Technology March 2015 A/L Selvaraju Theeban Raju Bachelor of Commerce January 2015 A/P Balan Durgarani Bachelor of Commerce with Distinction March 2015 A/P Rajaram Koushalya Priya Bachelor of Commerce March 2015 Hiba Mohsin Mohammed Master of Health Leadership and Aal-Yaseen Hussein Management July 2015 Aamer Muhammad Master of Quality Management September 2015 Abbas Hanaa Safy Seyam Master of Business Administration with Distinction March 2015 Abbasi Muhammad Hamza Master of International Business March 2015 Abdallah AlMustafa Hussein Saad Elsayed Bachelor of Commerce March 2015 Abdallah Asma Samir Lutfi Master of Strategic Marketing September 2015 Abdallah Moh'd Jawdat Abdel Rahman Master of International Business July 2015 AbdelAaty Mosa Amany Abdelkader Saad Master of Media and Communications with Distinction March 2015 Abdel-Karim Mervat Graduate Diploma in TESOL July 2015 Abdelmalik Mark Maher Abdelmesseh Bachelor of Commerce March 2015 Master of Strategic Human Resource Abdelrahman Abdo Mohammed Talat Abdelziz Management September 2015 Graduate Certificate in Health and Abdel-Sayed Mario Physical Education July 2015 Sherif Ahmed Fathy AbdRabou Abdelmohsen Master of Strategic Marketing September 2015 Abdul Hakeem Siti Fatimah Binte Bachelor of Science January 2015 Abdul Haq Shaddad Yousef Ibrahim Master of Strategic Marketing March 2015 Abdul Rahman Al Jabier Bachelor of Engineering Honours Class II, Division 1 -
HAND-ROLLED Omelets GERMAN PANCAKES TRADITIONAL
Add “the ADD FRUIT HAND-ROLLED omelets works” to GERMAN PANCAKES Topping! crepes & waffles sandwiches your hash Northwest Triple-Berry, Fluffy three-egg omelets served with choice of Famous Buttermilk browns Almost as big as Crater Lake! A delightful combination of farm-fresh “AA” Strawberry, Freshly-made crepes and waffles accompanied by two farm-fresh “AA” eggs*, and your choice of Served with your choice of Northwest Fries, cottage cheese or creamy coleslaw. Substitute sweet Pancakes, Northwest Hash Browns or fresh seasonal fruit. Hash brown Daily’s® smokehouse bacon, eggs, milk and flour is blended and baked to golden brown. Cinnamon Apple breakfast meat. onion rings, a cup of soup or a Yellow Bowl Dinner Salad for an additional charge. Tillamook® Cheddar cheese, or Lingonberry Butter and seasonal fruit choice also accompanied by a freshly-baked buttermilk green onions and a dollop biscuit. Omelets may be prepared with egg whites upon request. of sour cream for an CLASSIC GERMAN PANCAKE BELGIAN WAFFLE FRUIT FESTIVAL CREPES CASCADE CLUB GARDEN FRESH additional charge. Lemon wedges, whipped butter and powdered sugar. Thick and crispy Belgian waffle served with whipped Two freshly-made crepes with your choice of Daily’s® smokehouse bacon, honey-cured ham, Fresh avocado, baby spinach, sweet onion, DENVER & TILLAMOOK® FARMER’s Add fruit topping for an additional charge. butter and your choice of warm Elmer’s pancake Northwest triple-berry, strawberry, or cinnamon roasted turkey breast, Tillamook® Cheddar cheese provolone cheese, sliced hard-boiled egg, tomato CHEDDAR Hickory smoked ham, Daily’s® smokehouse syrup or Oregon Marionberry syrup. apple drizzled with cream cheese icing. -
Martian Subsurface Properties and Crater Formation Processes Inferred from Fresh Impact Crater Geometries
Martian Subsurface Properties and Crater Formation Processes Inferred From Fresh Impact Crater Geometries The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Stewart, Sarah T., and Gregory J. Valiant. 2006. Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries. Meteoritics and Planetary Sciences 41: 1509-1537. Published Version http://meteoritics.org/ Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:4727301 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA Meteoritics & Planetary Science 41, Nr 10, 1509–1537 (2006) Abstract available online at http://meteoritics.org Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries Sarah T. STEWART* and Gregory J. VALIANT Department of Earth and Planetary Sciences, Harvard University, 20 Oxford Street, Cambridge, Massachusetts 02138, USA *Corresponding author. E-mail: [email protected] (Received 22 October 2005; revision accepted 30 June 2006) Abstract–The geometry of simple impact craters reflects the properties of the target materials, and the diverse range of fluidized morphologies observed in Martian ejecta blankets are controlled by the near-surface composition and the climate at the time of impact. Using the Mars Orbiter Laser Altimeter (MOLA) data set, quantitative information about the strength of the upper crust and the dynamics of Martian ejecta blankets may be derived from crater geometry measurements. -
Arxiv:2003.06799V2 [Astro-Ph.EP] 6 Feb 2021
Thomas Ruedas1,2 Doris Breuer2 Electrical and seismological structure of the martian mantle and the detectability of impact-generated anomalies final version 18 September 2020 published: Icarus 358, 114176 (2021) 1Museum für Naturkunde Berlin, Germany 2Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany arXiv:2003.06799v2 [astro-ph.EP] 6 Feb 2021 The version of record is available at http://dx.doi.org/10.1016/j.icarus.2020.114176. This author pre-print version is shared under the Creative Commons Attribution Non-Commercial No Derivatives License (CC BY-NC-ND 4.0). Electrical and seismological structure of the martian mantle and the detectability of impact-generated anomalies Thomas Ruedas∗ Museum für Naturkunde Berlin, Germany Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany Doris Breuer Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany Highlights • Geophysical subsurface impact signatures are detectable under favorable conditions. • A combination of several methods will be necessary for basin identification. • Electromagnetic methods are most promising for investigating water concentrations. • Signatures hold information about impact melt dynamics. Mars, interior; Impact processes Abstract We derive synthetic electrical conductivity, seismic velocity, and density distributions from the results of martian mantle convection models affected by basin-forming meteorite impacts. The electrical conductivity features an intermediate minimum in the strongly depleted topmost mantle, sandwiched between higher conductivities in the lower crust and a smooth increase toward almost constant high values at depths greater than 400 km. The bulk sound speed increases mostly smoothly throughout the mantle, with only one marked change at the appearance of β-olivine near 1100 km depth. -
Seasonal Melting and the Formation of Sedimentary Rocks on Mars, with Predictions for the Gale Crater Mound
Seasonal melting and the formation of sedimentary rocks on Mars, with predictions for the Gale Crater mound Edwin S. Kite a, Itay Halevy b, Melinda A. Kahre c, Michael J. Wolff d, and Michael Manga e;f aDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA bCenter for Planetary Sciences, Weizmann Institute of Science, P.O. Box 26, Rehovot 76100, Israel cNASA Ames Research Center, Mountain View, California 94035, USA dSpace Science Institute, 4750 Walnut Street, Suite 205, Boulder, Colorado, USA eDepartment of Earth and Planetary Science, University of California Berkeley, Berkeley, California 94720, USA f Center for Integrative Planetary Science, University of California Berkeley, Berkeley, California 94720, USA arXiv:1205.6226v1 [astro-ph.EP] 28 May 2012 1 Number of pages: 60 2 Number of tables: 1 3 Number of figures: 19 Preprint submitted to Icarus 20 September 2018 4 Proposed Running Head: 5 Seasonal melting and sedimentary rocks on Mars 6 Please send Editorial Correspondence to: 7 8 Edwin S. Kite 9 Caltech, MC 150-21 10 Geological and Planetary Sciences 11 1200 E California Boulevard 12 Pasadena, CA 91125, USA. 13 14 Email: [email protected] 15 Phone: (510) 717-5205 16 2 17 ABSTRACT 18 A model for the formation and distribution of sedimentary rocks on Mars 19 is proposed. The rate{limiting step is supply of liquid water from seasonal 2 20 melting of snow or ice. The model is run for a O(10 ) mbar pure CO2 atmo- 21 sphere, dusty snow, and solar luminosity reduced by 23%. -
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