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Studies on the Circulation of the Atmospheres of the Sun
166 MONTHLY WEATEER REVIEW. APRIL,1904 STUDIES ON THE CIRCULATION OF THE ATMOSPHERES strato-cumulus as belonging to the cumulus level, and have OF THE SUN AND OF THE EARTH. used the reduction factor 0.5 instead of 0.9 in drawing the By Prof. FRANKH. BIGELOW. charts. V.-RESULTS OF THE NEPHOSCOPE OBSERVATIONS IN THE At Bridgetown the vector systems of the alto-stratus and WEST INDIES DURING THE TEARS 1899-1903. t,he cirro-cumulus levels have apparently been interchanged. As they now stand at Bridgetown they are inconsistent with METEODS OF OBSERVATION AND REDUCTION. the flow of air as determined at Basseterre, Roseau, Port of The observers of the United States Weather Bureau OCCII- Spain, and Willemstad; but if they are transposed, then there pied eleven stations in the West Indies during the years 1899- is harmony. The observation sheets indicate that the ob- 1903, and the opportunity was utilized to make a survey of the servers hare an unusually large number of cirro-cumulus en- motions of the atmosphere in that region of the Tropics by tries and comparatively few alto-stratus, so that apparently means of nephoscopes. they were accustomed to name many alto-stratus clods as The instruments were of the Marvin pattern, and the metliocl cirro-cumulus clouds. It is not easy to secure identical esti- of observation, to obtain the aziniuth and velocity of motion, mates of cloud forms at so many independent stations as we was identical with that described in t8heReport of the Chief of have used, and these fern instances of apparent discrepancies the Weather Bureau, 1S9S-99, T’ol. -
Caribbean.Pdf
WANG CENTER CENTER WANG Image from CIA World Factbook with formatting All photos compliments of Rebecca Wilkin J-TERM STUDY AWAY STUDY J-TERM PROGRAM OVERVIEW This program offers students an opportunity to experience a broad range of Caribbean locations and cultures during a 22 day program. Students will learn about Caribbean literature or Marketing in diverse cultural environments. The student experience will include learning about cultures and diversity, engaging in critical reflection and gaining a respect for the people and diverse places of the Caribbean, as well as completing one of two complete academic courses. Photo compliments of Kati Fisher Principles of Marketing/Literature and History of the Caribbean The Caribbean PROGRAM HIGHLIGHTS* • San Juan, Puerto Rico • St. Croix, US Virgin Islands • Basseterre, St. Kitts • Philipsburg, St. Maarten • Roseau, Dominica • Bridgetown, Barbados • Castries, St. Lucia • St. John’s, Antigua • Charlotte Amalie, St. Thomas • Oranjestad, Aruba • Willemstad, Curacao • St. George’s, Grenada Photo compliments of Nancy Albers-Miller *May be subject to change Educating to achieve a just, healthy, sustainable and peaceful world, both locally and globally. ACADEMICS APPLICATION PROCEDURE •BUSA 308/489 or ENGL 216 • February 20, 2015 - Application available (C, LT) -- 4 credits • April 20, 2015 - Application deadline Prerequisite: NONE ($50 non-refundable application fee) • May 8, 2015 - Notifications sent Program fee will be finaized by • May 22, 2015 - Confirmation deadline April 1, 2015. Check the Wang ($300 confirmation deposit) Center/Study Away Website for final pricing. Fees generally include the FACULTY LEADERS: following (check website for more details): • Airfare Nancy Albers-Miller • Lodging Dean of the School of • Study tours Business • Foreign travel insurance Professor of Marketing • Some meals [email protected] Participants in this program may apply for a Global Scholar Award. -
Memorial Day Sale Exclusive Rates· Book a Balcony Or Above and Receive up to $300 Onboard Credit ^ Plus 50% Reduced Deposit'
Memorial Day Sale Exclusive Rates· Book a Balcony or above and receive Up to $300 Onboard Credit ^ plus 50% Reduced Deposit' Voyage No. Sail Date Itinerary Voyage Description Nights Japan and Alaska Tokyo (tours from Yokohama), Hakodate, Sakaiminato, Busan, Sasebo, Kagoshima, Tokyo (tours from Yokohama), Hakodate, Aomori, Otaru, Cross Q216B 5/8/2022 International DateLine(Cruise-by), Anchorage(Seward), Hubbard Glacier (Cruise-by), Juneau, Glacier Bay National Park (Cruise-by), Ketchikan, Japan and Alaska 38 Victoria, Vancouver, Glacier Bay National Park (Cruise-by), Haines, Hubbard Glacier (Cruise-by), Juneau, Sitka, Ketchikan, Victoria, Vancouver Tokyo (tours from Yokohama), Hakodate, Aomori, Otaru, Cross International Date Line (Cruise-by), Anchorage (Seward), Hubbard Glacier (Cruise- Q217B 5/17/2022 by), Juneau, Glacier Bay National Park (Cruise-by), Ketchikan, Victoria, Vancouver, Glacier Bay National Park (Cruise-by), Haines, Hubbard Glacier Japan and Alaska 29 (Cruise-by), Juneau, Sitka, Ketchikan, Victoria, Vancouver Tokyo (tours from Yokohama), Hakodate, Aomori, Otaru, Cross International Date Line (Cruise-by), Anchorage (Seward), Hubbard Glacier (Cruise- Q217N 5/17/2022 Japan and Alaska 19 by), Juneau, Glacier Bay National Park (Cruise-by), Ketchikan, Victoria, Vancouver Alaska Q218N 6/4/2022 Vancouver, Glacier Bay National Park (Cruise-by), Haines, Hubbard Glacier (Cruise-by), Juneau, Sitka, Ketchikan, Victoria, Vancouver Alaska 10 Q219 6/14/2022 Vancouver, Juneau, Hubbard Glacier (Cruise-by), Skagway, Glacier Bay National Park -
Imagining Outer Space Also by Alexander C
Imagining Outer Space Also by Alexander C. T. Geppert FLEETING CITIES Imperial Expositions in Fin-de-Siècle Europe Co-Edited EUROPEAN EGO-HISTORIES Historiography and the Self, 1970–2000 ORTE DES OKKULTEN ESPOSIZIONI IN EUROPA TRA OTTO E NOVECENTO Spazi, organizzazione, rappresentazioni ORTSGESPRÄCHE Raum und Kommunikation im 19. und 20. Jahrhundert NEW DANGEROUS LIAISONS Discourses on Europe and Love in the Twentieth Century WUNDER Poetik und Politik des Staunens im 20. Jahrhundert Imagining Outer Space European Astroculture in the Twentieth Century Edited by Alexander C. T. Geppert Emmy Noether Research Group Director Freie Universität Berlin Editorial matter, selection and introduction © Alexander C. T. Geppert 2012 Chapter 6 (by Michael J. Neufeld) © the Smithsonian Institution 2012 All remaining chapters © their respective authors 2012 All rights reserved. No reproduction, copy or transmission of this publication may be made without written permission. No portion of this publication may be reproduced, copied or transmitted save with written permission or in accordance with the provisions of the Copyright, Designs and Patents Act 1988, or under the terms of any licence permitting limited copying issued by the Copyright Licensing Agency, Saffron House, 6–10 Kirby Street, London EC1N 8TS. Any person who does any unauthorized act in relation to this publication may be liable to criminal prosecution and civil claims for damages. The authors have asserted their rights to be identified as the authors of this work in accordance with the Copyright, Designs and Patents Act 1988. First published 2012 by PALGRAVE MACMILLAN Palgrave Macmillan in the UK is an imprint of Macmillan Publishers Limited, registered in England, company number 785998, of Houndmills, Basingstoke, Hampshire RG21 6XS. -
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. -
Widespread Crater-Related Pitted Materials on Mars: Further Evidence for the Role of Target Volatiles During the Impact Process ⇑ Livio L
Icarus 220 (2012) 348–368 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process ⇑ Livio L. Tornabene a, , Gordon R. Osinski a, Alfred S. McEwen b, Joseph M. Boyce c, Veronica J. Bray b, Christy M. Caudill b, John A. Grant d, Christopher W. Hamilton e, Sarah Mattson b, Peter J. Mouginis-Mark c a University of Western Ontario, Centre for Planetary Science and Exploration, Earth Sciences, London, ON, Canada N6A 5B7 b University of Arizona, Lunar and Planetary Lab, Tucson, AZ 85721-0092, USA c University of Hawai’i, Hawai’i Institute of Geophysics and Planetology, Ma¯noa, HI 96822, USA d Smithsonian Institution, Center for Earth and Planetary Studies, Washington, DC 20013-7012, USA e NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA article info abstract Article history: Recently acquired high-resolution images of martian impact craters provide further evidence for the Received 28 August 2011 interaction between subsurface volatiles and the impact cratering process. A densely pitted crater-related Revised 29 April 2012 unit has been identified in images of 204 craters from the Mars Reconnaissance Orbiter. This sample of Accepted 9 May 2012 craters are nearly equally distributed between the two hemispheres, spanning from 53°Sto62°N latitude. Available online 24 May 2012 They range in diameter from 1 to 150 km, and are found at elevations between À5.5 to +5.2 km relative to the martian datum. The pits are polygonal to quasi-circular depressions that often occur in dense clus- Keywords: ters and range in size from 10 m to as large as 3 km. -
Recent Channel Systems Emanating from Hale Crater Ejecta: Implications for the Noachian Landscape Evolution of Mars
Lunar and Planetary Science XXXIX (2008) 2180.pdf RECENT CHANNEL SYSTEMS EMANATING FROM HALE CRATER EJECTA: IMPLICATIONS FOR THE NOACHIAN LANDSCAPE EVOLUTION OF MARS. L. L. Tornabene1, 2, A. S. McEwen1, and the HiRISE Team1, 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, [email protected] Introduction: Impact cratering is a fundamental into linear elements that do not appear to be typical crater geologic process that dominated the distant geologic past rays, but like rays lie radial to Hale (e.g., 315°E, 32°S; of the terrestrial planets. Thereby, impacts played a 323.6°E, 35.7°S). Further, Hale has pristine morphologic significant role in the formation and evolution of planetary features at the decameter scale such as a sharp but crusts in the form of impact effects and byproducts (e.g., complexly terraced rim, a prominent central peak and only ejecta, breccias, impact melts, etc.). On Mars, impacts may small (<1 km) and few superimposed craters. The ejecta have liberated subsurface volatiles that, in the form of and secondaries from Hale are superimposed over liquid water, modified both surface morphology and surrounding terrains covering a large expanse of Mars, composition (e.g., phyllosilicates [e.g., 1]), and possibly with one swath of secondaries spanning >500 km wide. influenced early habitable environments. Although such an Hale also possesses ponded materials and channelized interaction has been inferred by studies of crater flows, which is an indication of the presence of impact- morphology [e.g., 2] and impact models [e.g., 3], direct melt bearing materials, as well as a testament to the evidence for the release of liquid water or other volatiles youthfulness and excellent state of preservation of the by Martian impacts was lacking [4]. -
Crater Geometry and Ejecta Thickness of the Martian Impact Crater Tooting
Meteoritics & Planetary Science 42, Nr 9, 1615–1625 (2007) Abstract available online at http://meteoritics.org Crater geometry and ejecta thickness of the Martian impact crater Tooting Peter J. MOUGINIS-MARK and Harold GARBEIL Hawai‘i Institute of Geophysics and Planetology, University of Hawai‘i, Honolulu, Hawai‘i 96822, USA (Received 25 October 2006; revision accepted 04 March 2007) Abstract–We use Mars Orbiter Laser Altimeter (MOLA) topographic data and Thermal Emission Imaging System (THEMIS) visible (VIS) images to study the cavity and the ejecta blanket of a very fresh Martian impact crater ~29 km in diameter, with the provisional International Astronomical Union (IAU) name Tooting crater. This crater is very young, as demonstrated by the large depth/ diameter ratio (0.065), impact melt preserved on the walls and floor, an extensive secondary crater field, and only 13 superposed impact craters (all 54 to 234 meters in diameter) on the ~8120 km2 ejecta blanket. Because the pre-impact terrain was essentially flat, we can measure the volume of the crater cavity and ejecta deposits. Tooting crater has a rim height that has >500 m variation around the rim crest and a very large central peak (1052 m high and >9 km wide). Crater cavity volume (i.e., volume below the pre-impact terrain) is ~380 km3 and the volume of materials above the pre-impact terrain is ~425 km3. The ejecta thickness is often very thin (<20 m) throughout much of the ejecta blanket. There is a pronounced asymmetry in the ejecta blanket, suggestive of an oblique impact, which has resulted in up to ~100 m of additional ejecta thickness being deposited down-range compared to the up-range value at the same radial distance from the rim crest. -
SYSTEMATIZATION Strengthening Early Warning Systems in The
BIBLIOGRAPHY AMA. 2016. Cuba: Methodologies for Determining Disaster Risks At Local Level Part 1, Havana: UNDP Cuba. Acosta, M. 2018. Informe reunión de presentación link encuesta lista de verificación SAT para las instituciones enlaces operativas del Centro de Operaciones de Emergencias, St. Domingo: UNDP. Acosta, M. 2018. Informe del Encuentro de conocimiento entre Equipo Técnicos del Centro de Operaciones de Emergencia, Enlaces operativos institucionales y técnicos, y expertos cubanos en SAT, Dominican Republic: UNDP. Acosta, M. 2018. Borrador de Informe basado en respuestas las partes interesadas a la encuesta de lista verificación SAT y la revisión del documento, Dominican Republic: UNDP. Alphonse, U. 2018. Consultancy Report: Multi - Hazard Early Warning Systems Report for Saint Lucia, St. Lucia: NEMO. Andrews, D. 2019. Early Warning Systems: Community Awareness & Knowledge (Bethesda, Grays Farm, Point & Urlings) Survey Results [Draft], St. Johns: NODS. Andrews, D. 2018. Workshop Report: Early Warning Systems-Drill Training and Alert Scripting, 13- 15 November 2018, Antigua and Barbuda, St. Johns: NODS. Civil Defense/HVR Group. 2018. Informe de viaje. Misión cubana a República Dominicana, 8 de abril 2018, Havana: PNUD Cuba. Civil Defense/HVR Group. 2018. Informe de viaje. Misión cubana San Vicente y las Granadinas y Dominica 28 a 31 de mayo 2018, Havana: PNUD Cuba. CITMA. 2018. Informe de viaje Misión Dominica 18-28 noviembre 2018, Havana: CITMA. COE. 2018. Reporte de brechas en Sistemas de Alerta Temprana Multi-Amenazas: República Dominicana, Rep. Dominicana: COE. COE/NEMO/NODS/ODM, 2018. Priority Action Proposals: Antigua & Barbuda, Dominica, Dominican Republic, St. Lucia, SVG, n/d. COE. 2018. Matriz Mapa de Ruta de Republica Dominicana, Santo Domingo: COE. -
List of Participants
Regional Conference on the Convention for the Safeguarding of the Intangible Cultural Heritage, Roseau, Dominica February 18 – 19, 2005 Antigua & Barbuda Heather Doram The Cultural Development Commission Lower Nevis Street St. John’s, Antigua & Barbuda Tel: 268.562.1723 Fax: 268.462.4757 Email: [email protected] Antigua & Barbuda (Observer) Hon. Elseston Adams Ministry of Housing, Culture & Social Transformation Popeshead Street & Dickenson Bay Street St. John’s, Antigua Tel: 268.562.5302/3 or 727.0080 or 764.0180 Aruba Ruby Figaroa-Eckmeyer Ministry of Labour, Culture and Sports Tel: 297.588.0900 Fax: 297.588.0331 Email: [email protected] Bahamas Nicolette Bethel Ministry of Youth, Sports & Culture 3rd Floor, Ministry of Education Building Thompson Boulevard P.O. Box N-4891, Nassau, Bahamas Tel: 242.502.0632 Fax: 242.325.0416 Email: [email protected] Belize Vivien Andy Palacio National Institute of Culture and History Museum Building Culvert Road, Belmopan Belize, Central America Tel: 501.822.3302 Fax: 501.822.3815 Email: [email protected] British Virgin Islands Luce Hodge Smith Ministry of Education and Culture Central Administration Complex Road Town, Tortola, British Virgin Islands Tel: 284.494.3701 Ext. 2242 Fax: 284.494.5421 [email protected] Cuba Margarita Victoria Elorza Echevarria National Council of Cultural Heritage 4th Street & 13 No. 810 Vedado Havana City, Cuba Tel: 53-7 55-1984/1981 Fax: 53-7 833-2106 Email: [email protected] Dominica Raymond Lawrence Division of Culture Ministry of Community Development, Gender Affairs & Information Government Headquarters Roseau, Dominica Tel: 767.449.1804/3075 Fax: 767.449.0461 Email: [email protected] Dominica (Presenter) Lennox Honychurch P.O. -
Dominica Flash Appeal 2017
FLASH 2017 APPEAL HURRICANE MARIA SEPTEMBER TO DECEMBER 2017 DOMINICA Photo: OCHA/Audrey Janvier TOTAL POPULATION PEOPLE PEOPLE IN NEED PEOPLE TARGETED REQUIREMENTS OF DOMINICA AFFECTED (US$) 71K 71K 65K 65K 31.1M Portsmouth SAINT JOHN SAINT ANDREW Marigot Populated areas SAINT PETER Anguilla 6 Sep, 06:00 ANTIGUA AND BARBUDA Barbuda 6 Sep, 00:00 Saint Kitts Nevis Antigua SAINT JOSEPH Grande-Terre SAINT DAVID Basse-Terre Guadeloupe H urr ican e M Marie-Galante ari a t rac k DOMINICA 18 Sep 18:00 Roseau SAINT PAUL Detailed map k HurricaneHurricane IrMariama trac gust footprints SAINT GEORGE Roseau 18 Sep, 06:01800 mph SAINT PATRICK Martinique Hurrica ne Ma Castries 170 ria t rack BARBADOS 160 17 Sep, 12:00 SAINT Bridgetow150n LUKE 140 SAINT 130 MARK TRINIDAD AN120D TOBAGO 110 100 90 DOMINICA FLASH APPEAL 2017 DOMINICA SITUATION OVERVIEW On 18 September, Hurricane Maria evolved from a category cent in Portsmouth (St. John Parish), 70 per cent in South 1 storm to a category 5 storm in less than 18 hours, just Roseau (St. George Parish) and 70 per cent in Pointe Michel before it slammed the Caribbean island of Dominica (Source: (St. Luke Parish). Copernicus, the European satellite-mapping NASA). It thrashed the country with extreme winds and rain system, suggests that approximately 25 per cent of buildings and destroyed all in its path. At the time of landfall, sustained in St. Paul Parish (15 per cent in Roseau only) and 61 per cent winds, which were reported to be 260 km/h, affected the in St. -
Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ 2014
Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ 2014 Edited by: James A. Skinner, Jr. U. S. Geological Survey, Flagstaff, AZ David Williams Arizona State University, Tempe, AZ NOTE: Abstracts in this volume can be cited using the following format: Graupner, M. and Hansen, V.L., 2014, Structural and Geologic Mapping of Tellus Region, Venus, in Skinner, J. A., Jr. and Williams, D. A., eds., Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ, June 23-25, 2014. SCHEDULE OF EVENTS Monday, June 23– Planetary Geologic Mappers Meeting Time Planet/Body Topic 8:30 am Arrive/Set-up – 2255 N. Gemini Drive (USGS) 9:00 Welcome/Logistics 9:10 NASA HQ and Program Remarks (M. Kelley) 9:30 USGS Map Coordinator Remarks (J. Skinner) 9:45 GIS and Web Updates (C. Fortezzo) 10:00 RPIF Updates (J. Hagerty) 10:15 BREAK / POSTERS 10:40 Venus Irnini Mons (D. Buczkowski) 11:00 Moon Lunar South Pole (S. Mest) 11:20 Moon Copernicus Quad (J. Hagerty) 11:40 Vesta Iterative Geologic Mapping (A. Yingst) 12:00 pm LUNCH / POSTERS 1:30 Vesta Proposed Time-Stratigraphy (D. Williams) 1:50 Mars Global Geology (J. Skinner) 2:10 Mars Terra Sirenum (R. Anderson) 2:30 Mars Arsia/Pavonis Montes (B. Garry) 2:50 Mars Valles Marineris (C. Fortezzo) 3:10 BREAK / POSTERS 3:30 Mars Candor Chasma (C. Okubo) 3:50 Mars Hrad Vallis (P. Mouginis-Mark) 4:10 Mars S. Margaritifer Terra (J. Grant) 4:30 Mars Ladon basin (C. Weitz) 4:50 DISCUSSION / POSTERS ~5:15 ADJOURN Tuesday, June 24 - Planetary Geologic Mappers Meeting Time Planet/Body Topic 8:30 am Arrive/Set-up/Logistics 9:00 Mars Upper Dao and Niger Valles (S.