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Warfare in a Fragile World: Military Impact on the Human Environment
Recent Slprt•• books World Armaments and Disarmament: SIPRI Yearbook 1979 World Armaments and Disarmament: SIPRI Yearbooks 1968-1979, Cumulative Index Nuclear Energy and Nuclear Weapon Proliferation Other related •• 8lprt books Ecological Consequences of the Second Ihdochina War Weapons of Mass Destruction and the Environment Publish~d on behalf of SIPRI by Taylor & Francis Ltd 10-14 Macklin Street London WC2B 5NF Distributed in the USA by Crane, Russak & Company Inc 3 East 44th Street New York NY 10017 USA and in Scandinavia by Almqvist & WikseH International PO Box 62 S-101 20 Stockholm Sweden For a complete list of SIPRI publications write to SIPRI Sveavagen 166 , S-113 46 Stockholm Sweden Stoekholol International Peace Research Institute Warfare in a Fragile World Military Impact onthe Human Environment Stockholm International Peace Research Institute SIPRI is an independent institute for research into problems of peace and conflict, especially those of disarmament and arms regulation. It was established in 1966 to commemorate Sweden's 150 years of unbroken peace. The Institute is financed by the Swedish Parliament. The staff, the Governing Board and the Scientific Council are international. As a consultative body, the Scientific Council is not responsible for the views expressed in the publications of the Institute. Governing Board Dr Rolf Bjornerstedt, Chairman (Sweden) Professor Robert Neild, Vice-Chairman (United Kingdom) Mr Tim Greve (Norway) Academician Ivan M£ilek (Czechoslovakia) Professor Leo Mates (Yugoslavia) Professor -
BULLETIN of the ALLYN MUSEUM 3621 Bayshore Rd
BULLETIN OF THE ALLYN MUSEUM 3621 Bayshore Rd. Sarasota, Florida 33580 Published By The Florida State Museum University of Florida Gainesville. Florida 32611 Number 107 30 December 1986 A REVIEW OF THE SATYRINE GENUS NEOMINOIS, WITH DESCRIPriONS OF THREE NEW SUBSPECIES George T. Austin Nevada State Museum and Historical Society 700 Twin Lakes Drive, Las Vegas, Nevada 89107 In recent years, revisions of several genera of satyrine butterflies have been undertaken (e. g., Miller 1972, 1974, 1976, 19781. To this, I wish to add a revision of the genus Neominois. Neominois Scudder TYPE SPECIES: Satyrus ridingsii W. H. Edwards by original designation (Scudder 1875b, p. 2411 Satyrus W. H. Edwards (1865, p. 2011, Rea.kirt (1866, p. 1451, W. H. Edwards (1872, p. 251, Strecker (1873, p. 291, W. H. Edwards (1874b, p. 261, W. H. Edwards (1874c, p. 5421, Mead (1875, p. 7741, W. H. Edwards (1875, p. 7931, Scudder (1875a, p. 871, Strecker (1878a, p. 1291, Strecker (1878b, p. 1561, Brown (1964, p. 3551 Chionobas W. H. Edwards (1870, p. 1921, W. H. Edwards (1872, p. 271, Elwes and Edwards (1893, p. 4591, W. H. Edwards (1874b, p. 281, Brown (1964, p. 3571 Hipparchia Kirby (1871, p. 891, W. H. Edwards (1877, p. 351, Kirby (1877, p. 7051, Brooklyn Ent. Soc. (1881, p. 31, W. H. Edwards (1884, p. [7)l, Maynard (1891, p. 1151, Cockerell (1893, p. 3541, Elwes and Edwards (1893, p. 4591, Hanham (1900, p. 3661 Neominois Scudder (1875b, p. 2411, Strecker (1876, p. 1181, Scudder (1878, p. 2541, Elwes and Edwards (1893, p. 4591, W. -
Workshop on Mars Telescopic Observations
WORKSHCPON MARS TELESCOPIC OBSERVATIONS 90' 180'-;~~~~~~------------------..~~------------~~----..~o~,· 270' LPI Technical Report Number 95-04 Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPIITR--95-04 WORKSHOP ON MARS TELESCOPIC OBSERVATIONS Edited by J. F. Bell III and J. E. Moersch Held at Cornell University, Ithaca, New York August 14-15, 1995 Sponsored by Lunar and Planetary Institute Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Technical Report Number 95-04 LPIITR--95-04 Compiled in 1995 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This report may be cited as Bell J. F.III and Moersch J. E., eds. (1995) Workshop on Mars Telescopic Observations. LPI Tech. Rpt. 95-04, Lunar and Planetary Institute, Houston. 33 pp. This report is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Mail order requestors will be invoiced for the cost ofshipping and handling. Cover: Orbits of Mars (outer ellipse) and Earth (inner ellipse) showing oppositions of the planet from 1954to 1999. From C. Aammarion (1954) The Flammarion Book ofAstronomy, Simon and Schuster, New York. LPl Technical Report 95-04 iii Introduction The Mars Telescopic Observations Workshop, held August 14-15, 1995, at Cornell University in Ithaca, New York, was organized and planned with two primary goals in mind: The first goal was to facilitate discussions among and between amateur and professional observers and to create a workshop environment fostering collaborations and comparisons within the Mars ob serving community. -
Global Spectral Classification of Martian Low-Albedo Regions with Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) Data A
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, E02004, doi:10.1029/2006JE002726, 2007 Global spectral classification of Martian low-albedo regions with Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) data A. Deanne Rogers,1 Joshua L. Bandfield,2 and Philip R. Christensen2 Received 4 April 2006; revised 12 August 2006; accepted 13 September 2006; published 14 February 2007. [1] Martian low-albedo surfaces (defined here as surfaces with Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) albedo values 0.15) were reexamined for regional variations in spectral response. Low-albedo regions exhibit spatially coherent variations in spectral character, which in this work are grouped into 11 representative spectral shapes. The use of these spectral shapes in modeling global surface emissivity results in refined distributions of previously determined global spectral unit types (Surface Types 1 and 2). Pure Type 2 surfaces are less extensive than previously thought, and are mostly confined to the northern lowlands. Regional-scale spectral variations are present within areas previously mapped as Surface Type 1 or as a mixture of the two surface types, suggesting variations in mineral abundance among basaltic units. For example, Syrtis Major, which was the Surface Type 1 type locality, is spectrally distinct from terrains that were also previously mapped as Type 1. A spectral difference also exists between southern and northern Acidalia Planitia, which may be due in part to a small amount of dust cover in southern Acidalia. Groups of these spectral shapes can be averaged to produce spectra that are similar to Surface Types 1 and 2, indicating that the originally derived surface types are representative of the average of all low-albedo regions. -
Sources of Shape Variation in Lunar Impact Craters: Fourier Shape Analysis
Sources of shape variation in lunar impact craters: Fourier shape analysis DUANE T. EPPLER Polar Oceanography Programs, Naval Ocean Research and Development Activity, NSTL Station, Mississippi 39529 ROBERT EHRLICH Department of Geology, University of South Carolina, Columbia, South Carolina 29208 DAG NUMMEDAL Department of Geology, Louisiana State University, Baton Rouge, Louisiana 70803 PETER H. SCHULTZ The Lunar and Planetary Institute, 3303 NASA Road One, Houston, Texas 77058 ABSTRACT outline of Tsiolkovsky crater is tectonically controlled. Shoemaker (1960) and Roddy (1978) show that the quadrate shape of Meteor R-mode factor analysis of Fourier harmonics that describe the Crater in Arizona is related directly to the orientation of regional shape-in-plan-view of 716 large (diameter > 15 km) nearside lunar faults and joints in Colorado Plateau rocks. craters shows that two factors explain 84.3% of shape variance Impact crater shape could be used to indicate structural pat- observed in the sample. Factor 1 accounts for 68.2% of the sample terns in heavily cratered terrane but has not received wide use as a variance and describes moderate-scale roughness defined by har- supplement to conventional sources of geologic structural data. In monics 7 through 10. Shape variation described by these harmonics part, this is due to previous absence of shape descriptors with which is related to surficial lunar processes of degradation that modify shape features that are related to structural variables can be dis- crater shape-in-plan. Dominant among these processes are ejecta criminated from those related to nonstructural variables. Although scour from large impact events and ongoing aging. -
The Subsurface Structure of Oblique Impact Craters
The subsurface structure of oblique impact craters Dissertation vorgelegt von Dipl.-Geol. Michael H. Poelchau vom Fachbereich Geowissenschaften der Freien Universität Berlin zur Erlangung des akademischen Grades doctor rerum naturalium (Dr. rer. nat.) Berlin, 2010 The subsurface structure of oblique impact craters Dissertation vorgelegt von Dipl.-Geol. Michael H. Poelchau vom Fachbereich Geowissenschaften der Freien Universität Berlin zur Erlangung des akademischen Grades doctor rerum naturalium (Dr. rer. nat.) Berlin, 2010 Gutachter: 1. PD Dr. Thomas Kenkmann 2. Prof. Wolf-Uwe Reimold Tag der Disputation: 23.02.2010 Statement regarding the contributions of the author and others to this thesis This thesis is comprised of three published, peer-reviewed articles and one submitted manuscript, which each form separate chapters within this thesis. The chapters “Introduction” and “General Conclusions” were written especially for this thesis. The PhD candidate is the first author of two of these articles, and the second author of the third article. The PhD candidate is also the first author of a manuscript currently submitted to Earth and Planetary Science Letters. Therefore, these four chapters have their own introduction, methodology, discussion, conclusions and references. The articles and manuscripts used in this thesis are the following: Poelchau, M. H., and T. Kenkmann, 2008. Asymmetric signatures in simple craters as an indicator for an oblique impact direction, Meteoritcal and Planetary Science, 43, 2059-2072. Poelchau M. H., Kenkmann T. and Kring D. A., 2009. Rim uplift and crater shape in Meteor Crater: the effects of target heterogeneities and trajectory obliquity. Journal of Geophysical Research, 114, E01006, doi:10.1029/2008JE003235. Kenkmann, T. -
Observations of Mars and Its Satellites by the Mars Imaging Camera (MIC) on Planet-B
Earth Planets Space, 50, 183–188, 1998 Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B Tadashi Mukai1, Tokuhide Akabane2, Tatsuaki Hashimoto3, Hiroshi Ishimoto1, Sho Sasaki4, Ai Inada1, Anthony Toigo5, Masato Nakamura6, Yutaka Abe6, Kei Kurita6, and Takeshi Imamura6 1The Graduate School of Science and Technology, Kobe University, Kobe 657-8501, Japan 2Hida Observatory, Kyoto University, Kamitakara, Gifu 506-13, Japan 3Institute of Space and Astronautical Science, Kanagawa 229-8510, Japan 4Geological Institute, University of Tokyo, Tokyo 113, Japan 5Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, U.S.A. 6Space and Planetary Science, University of Tokyo, Tokyo 113, Japan (Received August 7, 1997; Revised December 16, 1997; Accepted January 30, 1998) We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same region of Mars at various times of day and various solar phase angles with spatial resolution of about 60 m from a distance of 150 km altitude (at periapsis), and (2) to monitor changes of global atmospheric conditions on Mars near an apoapsis of 15 Mars radii. In addition, (3) several encounters of Planet-B with each of the two Martian satellites are scheduled during the mission lifetime of two years from October 1999 to observe their shapes and surface structures with three color filters, centered on 450, 550, and 650 nm. -
The Sand Ships of Mars By: Jeffrey D
The Sand Ships of Mars By: Jeffrey D. Beish (Rev. 12-19-2018) INTRODUCTION It was Ray Bradbury who wrote of the "Sand Ships of Mars" in his science fiction novel, The Martian Chronicles (Bradbury, 1950). One can imagine the fictional inhabitants of Mars trekking across its deserts in their floating machines stirring up huge dust devils. This great science fiction story set the stage for this author’s interest in Mars and who now writes about similar accounts of the real dusty whirlwinds on the Red Planet. [NOTE: see Mars Chart in Reference section for location names]. One of the most spectacular events to watch in our Solar System is the development of a major Martian dust storm. From Earth a Martian dust cloud may seem to be just a nuisance to any would-be telescopic explorer on that planet. However, if you consider the actual size of these clouds then you suddenly realize that many of them would cover entire western United States! Imagine if a Mars-sized planet-encircling dust storm would occur on Earth; it would blank out most of an entire Hemisphere! Some would-be Mars experts claim that after dust storms the dust settles quickly to the surface and reduces contrast of albedo features. This is contrary to the known facts; dust remains in the atmosphere of Mars for weeks -- at times months -- before settling to the surface [Pollack, 1989], [Kahn, 1992]. This dust is very fine particles of volcanic ash and when raised aloft during these storms they reach heights of several kilometers. -
The Opposition of Mars, 1999
The opposition of Mars, 1999 Richard McKim A report of the Mars Section (Director: R. J. McKim) The 1999 martian apparition was followed by BAA members while Mars Global Surveyor was monitoring the planet from martian orbit. The planet’s surface showed little change from 1997, indicating the absence of any great dust storm since solar conjunction. The long period of telescopic coverage enabled us to conclude that neither was there any planet-encircling storm in the southern martian spring or summer in 1999−2000. Three small telescopic storms were followed along the Valles Marineris, and two were seen at the edge of the summer N. polar cap. Dust storms commencing at the historically rarely-active Margaritifer Sinus emergence site (MGS data) point to ongoing changes in the fallout pattern of atmospheric dust. White cloud activity was high before and around opposition time − in northern midsummer − with morning and evening limb hazes, the equatorial cloud band (ECB) and orographic clouds. The ECB ‘season’ was identical to 1997, pointing to an equally low level of atmospheric dust-loading. Comparison with historical records suggests that the seasonal ‘wave of darkening’ may be partly attributable to the annual disappearance of the ECB. A ‘polar cyclone’ imaged by the Hubble Space Telescope between Mare Acidalium and the northern cap was followed over several days. The seasonal behaviour of the NPC, including its transition to the polar hood, was well observed. Its recession (observed from northern mid-spring) was a little slower than usual. The formation of the SPC from its winter hood, and its early recession, was also recorded. -
Surveys of the Distribution of Seabirds Found in the Vicinity of Proposed Geothermal Project Subzones in the District of Puna, Hawaii
University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Wildlife Damage Management, Internet Center Other Publications in Wildlife Management for August 1994 SURVEYS OF THE DISTRIBUTION OF SEABIRDS FOUND IN THE VICINITY OF PROPOSED GEOTHERMAL PROJECT SUBZONES IN THE DISTRICT OF PUNA, HAWAII Michelle Reynolds U.S. Fish and Wildlife Service George Ritchotte U.S. Fish and Wildlife Service Anthony Viggiano U.S. Fish and Wildlife Service Jill Dwyer U.S. Fish and Wildlife Service Bonnie Nielson U.S. Fish and Wildlife Service See next page for additional authors Follow this and additional works at: https://digitalcommons.unl.edu/icwdmother Part of the Environmental Sciences Commons Reynolds, Michelle; Ritchotte, George ; Viggiano, Anthony; Dwyer, Jill; Nielson, Bonnie ; and Jacobi, James D., "SURVEYS OF THE DISTRIBUTION OF SEABIRDS FOUND IN THE VICINITY OF PROPOSED GEOTHERMAL PROJECT SUBZONES IN THE DISTRICT OF PUNA, HAWAII" (1994). Other Publications in Wildlife Management. 38. https://digitalcommons.unl.edu/icwdmother/38 This Article is brought to you for free and open access by the Wildlife Damage Management, Internet Center for at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Other Publications in Wildlife Management by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. Authors Michelle Reynolds, George Ritchotte, Anthony Viggiano, Jill Dwyer, Bonnie Nielson, and James D. Jacobi This article is available at DigitalCommons@University of Nebraska - Lincoln: https://digitalcommons.unl.edu/ icwdmother/38 Centimeter 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 mm _t_i_i_i`_i__'_i_l_'_l_'_'_'_l_'_'_'j_'_1,_i_1_.`_i_._1_`,_ 1 2 3 4 5 Inches IIII1",_ oIII1°-_ ,7-,Illll_ I.I _ lill,i 11111,.8 IIII1_IIIIl_Ilili:_ MANUFACTURED TO PlIIIMSTANDARDS ,,_ _ _,_ BY APPLIED IMPI_E, INC. -
The Medusae Fossae Formation As the Single Largest Source of Dust on Mars
ARTICLE DOI: 10.1038/s41467-018-05291-5 OPEN The Medusae Fossae Formation as the single largest source of dust on Mars Lujendra Ojha1, Kevin Lewis1, Suniti Karunatillake 2 & Mariek Schmidt3 Transport of fine-grained dust is one of the most widespread sedimentary processes occurring on Mars today. In the present climate, eolian abrasion and deflation of rocks are likely the most pervasive and active dust-forming mechanism. Martian dust is globally 1234567890():,; enriched in S and Cl and has a distinct mean S:Cl ratio. Here we identify a potential source region for Martian dust based on analysis of elemental abundance data. We show that a large sedimentary unit called the Medusae Fossae Formation (MFF) has the highest abundance of S and Cl, and provides the best chemical match to surface measurements of Martian dust. Based on volume estimates of the eroded materials from the MFF, along with the enrichment of elemental S and Cl, and overall geochemical similarity, we propose that long-term deflation of the MFF has significantly contributed to the global Martian dust reservoir. 1 Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD 21218, USA. 2 Department of Geology and Geophysics, Louisiana State University, Baton Rouge, LA 70803, USA. 3 Department of Earth Sciences, Brock University, St. Catharines, ON L2S 3A1, Canada. Correspondence and requests for materials should be addressed to L.O. (email: [email protected]) NATURE COMMUNICATIONS | (2018) 9:2867 | DOI: 10.1038/s41467-018-05291-5 | www.nature.com/naturecommunications 1 ARTICLE NATURE COMMUNICATIONS | DOI: 10.1038/s41467-018-05291-5 ust is ubiquitous on Mars and plays a key role in con- formation on Mars today is likely abrasion of mechanically weak temporary atmospheric and surface processes. -
New Business List Portland, OR 97201
City of Portland Revenue Division September 2019 111 SW Columbia St, Suite 600 New Business List Portland, OR 97201 Owner/Business Name Mailing Address Business Description 10 LUX LLC 6232 SE 47TH AVE Site Preparation Contractors PORTLAND OR 97206-7045 168 REALTY LLC GUO Z CHEN Real Estate and Rental and Leasing 15964 SW WREN LN BEAVERTON OR 97007-9401 302 SE 7TH OZ LLC CRAIG FIRPO Lessors of Nonresidential Buildings 210 SE MADISON ST STE 19 (except Miniwarehouses) PORTLAND OR 97214-4192 3807 SE MAIN ST (TIC) 3810 SE SALMON ST Lessors of Residential Buildings and PORTLAND OR 97214-4340 Dwellings 650 GAINES LLC GRIFFIS RESIDENTIAL Real Estate and Rental and Leasing DBA: GRIFFIS SOUTH WATERFRONT 6400 S FIDDLERS GREEN CIR STE 1200 GREENWOOD VILLAGE CO 80111-4913 A PRASAD, LLC 6315 SE EVERGREEN HWY Other Activities Related to Real VANCOUVER WA 98661-7628 Estate ABDELRAHIM, AHMED A MR 6139 NE 14TH CT Other Services (except Public VANCOUVER WA 98665-1311 Administration) ABDI, ALI 13210 SE DIVISION ST APT 43 Other Services (except Public PORTLAND OR 97236-3059 Administration) ABEBE, FIKIRTE 17266 SE HARRISON ST Community Care Facilities for the DBA: BETHEL ADULT CARE HOME PORTLAND OR 97233-4477 Elderly ABEDRABUH, ZAIDAN 14309 NE 86TH CIRCLE Private for Hire Transportation VANCOUVER WA 98682 ABERNATHY, LISA M 5312 NE LOWER OAK HILL DR Other Services (except Public BATTLE GROUND WA 98604-2607 Administration) ABREU SOLIS, LUIS A 1307 NE 20TH AVE Other Services (except Public BATTLE GROUND WA 98604-4662 Administration) ABRIGO, JAY 15000 SW MILLIKAN