Improving the Calculation of Fisheries Reference Points Influences of Density Dependence and Size Selectivity Van Gemert, Rob
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Imaginative Geographies of Mars: the Science and Significance of the Red Planet, 1877 - 1910
Copyright by Kristina Maria Doyle Lane 2006 The Dissertation Committee for Kristina Maria Doyle Lane Certifies that this is the approved version of the following dissertation: IMAGINATIVE GEOGRAPHIES OF MARS: THE SCIENCE AND SIGNIFICANCE OF THE RED PLANET, 1877 - 1910 Committee: Ian R. Manners, Supervisor Kelley A. Crews-Meyer Diana K. Davis Roger Hart Steven D. Hoelscher Imaginative Geographies of Mars: The Science and Significance of the Red Planet, 1877 - 1910 by Kristina Maria Doyle Lane, B.A.; M.S.C.R.P. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2006 Dedication This dissertation is dedicated to Magdalena Maria Kost, who probably never would have understood why it had to be written and certainly would not have wanted to read it, but who would have been very proud nonetheless. Acknowledgments This dissertation would have been impossible without the assistance of many extremely capable and accommodating professionals. For patiently guiding me in the early research phases and then responding to countless followup email messages, I would like to thank Antoinette Beiser and Marty Hecht of the Lowell Observatory Library and Archives at Flagstaff. For introducing me to the many treasures held deep underground in our nation’s capital, I would like to thank Pam VanEe and Ed Redmond of the Geography and Map Division of the Library of Congress in Washington, D.C. For welcoming me during two brief but productive visits to the most beautiful library I have seen, I thank Brenda Corbin and Gregory Shelton of the U.S. -
Hip # 987-1088
Hip No. Consigned by Tate Farms Hip No. 987 Jess Sizzlin SI 92 987 1997 Sorrel Mare Streakin La Jolla SI 99 {Streakin Six SI 104 Mr Jess Perry SI 113 { Bottom’s Up SI 82 Scoopie Fein SI 99 {Sinn Fein SI 98 Jess Sizzlin SI 92 Legs La Scoop SI 95 3654393 Easy Jet SI 100 {Jet Deck SI 100 Sizzlin Kim SI 86 Lena’s Bar TB SI 95 (1987) { Sun Spots {Double Bid SI 100 Winsum Miss SI 95 By MR JESS PERRY SI 113 (1992). Champion 2-year-old, $687,184 [G1]. Sire of 799 ROM, 107 stakes winners, $39,619,142, incl. champions APOL- LITICAL JESS SI 107 (world champion, $1,399,831, Los Alamitos Derby [G1]), ONE FAMOUS EAGLE SI 101 ($1,387,453 [G1]). Sire of the dams of 46 stakes winners, incl. BODACIOUS DASH SI 101 ($756,495 [G1]), JES A GAME SI 111 ($323,978 [G2]), TERRIFIC SYNERGY SI 92 ($288,066 [RG2]). 1st dam SIZZLIN KIM SI 86, by Easy Jet. Placed to 3. Dam of 7 foals, 6 to race, 3 winners, including– Jess Sizzlin SI 92 (f. by Mr Jess Perry). Stakes placed winner, below. Streakin Kim (f. by Streakin La Jolla). Unplaced. Dam of– Kims Corona SI 97 (g. by Corona Cocktail). 3 wins to 4, $38,666. 2nd dam SUN SPOTS, by Double Bid. Unraced. Dam of 13 starters, 7 ROM, incl.– SUN KISSES SI 102 (f. by Game Plan). 7 wins to 3, $68,935, Shebester Derby, Mystery Derby. Dam of Exquisite Expense SI 99 ($42,264 [G3]). -
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. -
Exponential Sums After Bombieri and Iwaniec Astérisque, Tome 198-199-200 (1991), P
Astérisque M. N. HUXLEY Exponential sums after Bombieri and Iwaniec Astérisque, tome 198-199-200 (1991), p. 165-175 <http://www.numdam.org/item?id=AST_1991__198-199-200__165_0> © Société mathématique de France, 1991, tous droits réservés. L’accès aux archives de la collection « Astérisque » (http://smf4.emath.fr/ Publications/Asterisque/) implique l’accord avec les conditions générales d’uti- lisation (http://www.numdam.org/conditions). Toute utilisation commerciale ou impression systématique est constitutive d’une infraction pénale. Toute copie ou impression de ce fichier doit contenir la présente mention de copyright. Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques http://www.numdam.org/ EXPONENTIAL SUMS AFTER BOMBIERI AND IWANIEC by M.N. HUXLEY BOMBIERI and IWANIEC [BI1, BI2] obtained 9 = 9/56 for the Lindelof exponent (the least 9 for which the Riemann zeta function satisfies C(l/2 + i<) = 0(te+£) as <->oo.) They remarked that their method might not be special to the Lindelof problem; in fact, as the saying goes, "they wrought [worked] better than they knew". To show that one property is uniformly distributed with respect to another property, one forms exponential sums 2M-1 5 = e{f[m)) , (1) M where e(x) = exp 2nix, f(m) = TF(m/M) with F(x) in the function class Cn[l — <5,2 + 6] for some 6 > 0 and n > 4. The case F(x) = log x gives Dirichlet series. If F(x) is a polynomial of degree d with rational coefficients, denominator g, and if T = Md, then the sum 5 is approximately MSJq , where Sq is a complete exponential sum with denominator q. -
Mosasaurs from Germany – a Brief History of the First 100 Years of Research
Netherlands Journal of Geosciences —– Geologie en Mijnbouw | 94 – 1 | 5-18 | 2015 doi: 10.1017/njg.2014.16 Mosasaurs from Germany – a brief history of the first 100 years of research Sven Sachs1,*,JahnJ.Hornung2 &MikeReich2,3 1 Im Hof 9, 51766 Engelskirchen, Germany 2 Georg-August University Gottingen,¨ Geoscience Centre, Department of Geobiology, Gottingen,¨ Germany 3 Georg-August University Gottingen,¨ Geoscience Museum, Gottingen,¨ Germany * Corresponding author. Email: [email protected] Manuscript received: 30 December 2013, accepted: 26 May 2014 Abstract In Germany, mosasaur remains are very rare and only incompletely known. However, the earliest records date back to the 1830s, when tooth crowns werefoundinthechalkoftheIsleofRugen.¨ A number of prominent figures in German palaeontology and geosciences of the 19th and 20th centuries focused on these remains, including, among others, Friedrich von Hagenow, Hermann von Meyer, Andreas Wagner, Hanns Bruno Geinitz and Josef Pompeckj. Most of these works were only short notes, given the scant material. However, the discovery of fragmentary cranial remains in Westphalia in 1908 led to a more comprehensive discussion, which is also of historical importance, as it illustrates the discussions on the highly controversial and radical universal phylogenetic theory proposed by Gustav Steinmann in 1908. This theory saw the existence of continuous lines of descent, evolving in parallel, and did not regard higher taxonomic units as monophyletic groups but as intermediate paraphyletic stages of evolution. In this idea, nearly all fossil taxa form part of these lineages, which extend into the present time, and natural extinction occurs very rarely, if ever. In Steinmann’s concept, mosasaurs were not closely related to squamates but formed an intermediate member in a anagenetic chain from Triassic thalattosaurs to extant baleen whales. -
Alpha ELT Listing
Lienholder Name Lienholder Address City State Zip ELT ID 1ST ADVANTAGE FCU PO BX 2116 NEWPORT NEWS VA 23609 CFW 1ST COMMAND BK PO BX 901041 FORT WORTH TX 76101 FXQ 1ST FNCL BK USA 47 SHERMAN HILL RD WOODBURY CT 06798 GVY 1ST LIBERTY FCU PO BX 5002 GREAT FALLS MT 59403 ESY 1ST NORTHERN CA CU 1111 PINE ST MARTINEZ CA 94553 EUZ 1ST NORTHERN CR U 230 W MONROE ST STE 2850 CHICAGO IL 60606 GVK 1ST RESOURCE CU 47 W OXMOOR RD BIRMINGHAM AL 35209 DYW 1ST SECURITY BK WA PO BX 97000 LYNNWOOD WA 98046 FTK 1ST UNITED SVCS CU 5901 GIBRALTAR DR PLEASANTON CA 94588 W95 1ST VALLEY CU 401 W SECOND ST SN BERNRDNO CA 92401 K31 360 EQUIP FIN LLC 300 BEARDSLEY LN STE D201 AUSTIN TX 78746 DJH 360 FCU PO BX 273 WINDSOR LOCKS CT 06096 DBG 4FRONT CU PO BX 795 TRAVERSE CITY MI 49685 FBU 777 EQUIPMENT FIN LLC 600 BRICKELL AVE FL 19 MIAMI FL 33131 FYD A C AUTOPAY PO BX 40409 DENVER CO 80204 CWX A L FNCL CORP PO BX 11907 SANTA ANA CA 92711 J68 A L FNCL CORP PO BX 51466 ONTARIO CA 91761 J90 A L FNCL CORP PO BX 255128 SACRAMENTO CA 95865 J93 A L FNCL CORP PO BX 28248 FRESNO CA 93729 J95 A PLUS FCU PO BX 14867 AUSTIN TX 78761 AYV A PLUS LOANS 500 3RD ST W SACRAMENTO CA 95605 GCC A/M FNCL PO BX 1474 CLOVIS CA 93613 A94 AAA FCU PO BX 3788 SOUTH BEND IN 46619 CSM AAC CU 177 WILSON AVE NW GRAND RAPIDS MI 49534 GET AAFCU PO BX 619001 MD2100 DFW AIRPORT TX 75261 A90 ABLE INC 503 COLORADO ST AUSTIN TX 78701 CVD ABNB FCU 830 GREENBRIER CIR CHESAPEAKE VA 23320 CXE ABOUND FCU PO BX 900 RADCLIFF KY 40159 GKB ACADEMY BANK NA PO BX 26458 KANSAS CITY MO 64196 ATF ACCENTRA CU 400 4TH -
VIRVĖ SAVO KARTUVĖMS Kapitalistų Sandėriai Su Komunistais Vytautas Meškauskas
T e oc. oi' 5 □ TL i r. s t r c ba š' 7243 So» Albanv fk., ' yi Chiccęp, III, ‘ 304.29 ; I0TEKA Į -----THE LITHUANIAN NATIONAL NEVVSPAPER -------- P.O. BOX 03206 > 6116 ST. CLAIR AVENUE > CLEVELAND, OHIO 44103 Vol.LXIV Balandis - April 19, 1979 Nr.16 *< TAUTINES MINTIES LIETUVIŲ LAIKRAŠTIS VIRVĖ SAVO KARTUVĖMS Kapitalistų sandėriai su komunistais Vytautas Meškauskas Turiu pasakyti, kad Leninas išpranašavo visą proce Konkrečiai kalbant, pereitų są. Leninas, kuris didesnę savo gyvenimo dalį praleido metų prekybos su sovietais Vakaruose, bet ne Rusijoje, kuris geriau pažinojo Vaka apyvarta siekė tik 2.8 biijonus rus kaip Rusiją, visados rašė ir sakė, jog Vakarų kapi dolerių, t.y. tik trečdalį pre talistai padarys viską, kad sustiprintų SSSR ekonomiją. kybos su ... Taiwanu. Biznie Jie konkuruos savo tarpe, kad mums parduoti gerybes rius tačiau vilioja ne tiek da pigiau ir greičiau, tik tam, kad sovietai jas pirktų ne iš bartinės, kiek ateities galimy bės. Šiaip ar taip, Sovietiją vieno, bet iš kito. Jis sakė: jie taip darys negalvodami sudaro rinką su 250 milijonų apie savo pačių ateitį. Vienu sunkiu momentu partijos gyventojų. posėdyje Maskvoje jis drąsino: "Draugai, nepasiduokit Nepaisant to, kad bolševi panikai, jei mums pasidarys labai sunku, mes duosime kai konfiskavo visus užsienie virvę buržuazijai, ir buržuazija pati pasikars." čių kapitalus, buvusius caro Tada, Kari Radek,... kuris buvo labai sąmojingas, Rusijoje - vien Singerio kom paklausė: Vladimire Iličiau, bet iš kur mes paimsime tiek panija prieš karą ten turėjo daug virvės buržuazijos pasikorimui?” Leninas nerūpes 27,000 tarnautojų. Vakarų tingai atsakė: "Jie mus ja aprūpins." kapitalistai padėjo sovietų (Iš Aleksandro Solženicyno 1975 m. -
NATURE [J'une 20, 1872 Aqueous Vapour in Condensing Developes
148 NATURE [J'une 20, 1872 aqueous vapour in condensing developes. ~ositive elec originally advanced, the data required for its mathematical tricity. No unusual development of electnc1ty has ever demonstration were entirely wanting. The evidence, been detected by him in a cloud when no rain is falling. however, by which it was sustained was sufficient to give The above results, though falling short of what has to it a high degree of probability. be done to complete the theory, are yet definite, and hence The existence of a divellent force by which comets valuable, the more so if supported by other observers near their perihelia have been separated into parts, is placed in equally favourable situations. But of the varia clearly shown by the facts enumerated in the following tions in intensi"ty of positive or negative electricity nothing lines. Whether this force, as suggested by Schiaparelli, has been said. is simply the unequal attraction of the sun on different Besides the fixed instruments at the Observatory others parts of the nebulous mass, or whether, in accordance are used on the mountain. Gases are collected from with the views of other astronomers, it is to be regarded cracks in the earth's crust, tubes being let down into as a cosmical force of repulsion, is a question left for them and the gas sucked up by a kind of bellows to be future discussion. examined at leisure. A portable spectroscope is also used I. Seneca informs us that Ephoras, a Greek writer of during eruptions, and there is a larger one by Hoffman in the fourth century B.c., had recorded the singular fact of the Observatory. -
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 -
RESEARCHES on CRUSTACEA Special Number 3
OKm iS 7 '"ic^mi n^^ ,',',. y^ ,^^o1»8 RESEARCHES ON CRUSTACEA Special Number 3 The Carcinological Society of Japan 1990 FRONTISPIECE The battle of the Heike and the Genji at Dannoura in 1185. Colored print by Kuniyoshi. RESEARCHES ON CRUSTACEA, SPECIAL NUMBER 3 Crabs of the Subfamily Dorippinae MacLeay, 1838, from the Indo-West Pacific Region (Crustacea: Decapoda: Dorippidae) L. B. Holthuis and Raymond B. Manning The Carcinological Society of Japan Tokyo June 1990 Copyright 1990 by The Carcinological Society of Japan Odawara Carcinological Museum Azabu-Juban 3-11-12, Minatoku, Tokyo 106 Japan Printed by Shimoda Printing, Inc. Matsubase, Shimomashiki-gun Kumamoto 869-05 Japan Issued 30 June 1990 Copies available from the Carcinological Society of Japan Contents Page Introduction 1 Methods 3 Acknowledgments 4 Systematic Account 5 Family Dorippidae MacLeay, 1838 5 Subfamily Dorippinae MacLeay, 1838 5 Key to Indo-West Pacific Genera of Dorippinae 5 Key to Genera of Dorippinae, Based on Male First Pleopods 6 Genus Dorippe Weber, 1795 7 Key to Species of Dorippe 9 Dorippe frascone (Herbst, 1785) 10 Dorippe irrorata Manning and Holthuis, 1986 15 Dorippe quadridens (Fabricius, 1793) 18 Dorippe sinica Chen, 1980 36 Dorippe tenuipes Chen, 1980 43 Genus Dorippoides Serene and Romimohtarto, 1969 47 Key to Species of Dorippoides 49 Dorippoides facchino (Herbst, 1785) 49 Dorippoides nudipes Manning and Holthuis, 1986 66 Heikea, new genus 71 Key to Species of Heikea 72 Heikea arachnoides (Manning and Holthuis, 1986), new combination 72 Heikea japonica -
Cambridge University Press 978-1-107-03629-1 — the Atlas of Mars Kenneth S
Cambridge University Press 978-1-107-03629-1 — The Atlas of Mars Kenneth S. Coles, Kenneth L. Tanaka, Philip R. Christensen Index More Information Index Note: page numbers in italic indicates figures or tables Acheron Fossae 76, 76–77 cuesta 167, 169 Hadriacus Cavi 183 orbit 1 Acidalia Mensa 86, 87 Curiosity 9, 32, 62, 195 Hadriacus Palus 183, 184–185 surface gravity 1, 13 aeolian, See wind; dunes Cyane Catena 82 Hecates Tholus 102, 103 Mars 3 spacecraft 6, 201–202 Aeolis Dorsa 197 Hellas 30, 30, 53 Mars Atmosphere and Volatile Evolution (MAVEN) 9 Aeolis Mons, See Mount Sharp Dao Vallis 227 Hellas Montes 225 Mars Chart 1 Alba Mons 80, 81 datum (zero elevation) 2 Hellas Planitia 220, 220, 226, 227 Mars Exploration Rovers (MER), See Spirit, Opportunity albedo 4, 5,6,10, 56, 139 deformation 220, See also contraction, extension, faults, hematite 61, 130, 173 Mars Express 9 alluvial deposits 62, 195, 197, See also fluvial deposits grabens spherules 61,61 Mars Global Surveyor (MGS) 9 Amazonian Period, history of 50–51, 59 Deimos 62, 246, 246 Henry crater 135, 135 Mars Odyssey (MO) 9 Amenthes Planum 143, 143 deltas 174, 175, 195 Herschel crater 188, 189 Mars Orbiter Mission (MOM) 9 Apollinaris Mons 195, 195 dikes, igneous 82, 105, 155 Hesperia Planum 188–189 Mars Pathfinder 9, 31, 36, 60,60 Aram Chaos 130, 131 domical mound 135, 182, 195 Hesperian Period, history of 50, 188 Mars Reconnaissance Orbiter (MRO) 9 Ares Vallis 129, 130 Dorsa Argentea 239, 240 Huygens crater 183, 185 massif 182, 224 Argyre Planitia 213 dunes 56, 57,69–70, 71, 168, 185, -
Leading Msl to Water: Paleolacustrine Landing Sites Redux
LEADING MSL TO WATER: PALEOLACUSTRINE LANDING SITES REDUX. J.W. Rice, Jr., Mars Space Flight Facility, Department of Geosciences, Arizona StateUniversity, Tempe, AZ 85287, [email protected] Introduction: The highest priority landing site tered bedrock outcrops. This is consistent with a for achieving the scientific objectives (assessment lacustrine setting. of local region for habitat potential for past or present life) of the Mars Science Laboratory will Holden Crater be a paleolacustrine basin containing accessible Location: 26.1.S,326E layered sediments. Ideally, this type of landing Diameter: 154 km site would be selected from both morphologic and Elevation: –2.200km mineralogic evidence. The MER Project had the Thermal Inertia: 320-470 SI units luxury of selecting two landing sites. One site Geology: Uzboi Vallis cuts the SW rim of based on mineralogy (Meridiani Planum) and one Holden. The southern floor of Holden contains on morphology (Gusev Crater). To date the Me- laterally continuous layered sediments, distribu- ridiani site has proven to be the wettest. The mor- tary fan (225km2), inverted channels and mean- phologic approach was unsuccessfully attempted dering channels. Medium thermal inertia repre- with the Gusev Crater site. However, it should be sents a combination of coarser loose particles, mentioned that some of us (voices in the wilder- crusted fines, a fair number of scattered rocks, ness) argued that the morphologic and geologic and/or perhaps a few scattered bedrock outcrops. evidence in Gusev Crater was much more com- This is consistent with a lacustrine setting. plicated and that the commonly accepted lacus- trine story was flawed. MSL will only get one Palos Crater chance.