A Study of the Lifestyle and Health Parameters of Nuns from Convents on the Iberian Peninsula in Modern Times”
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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. -
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. -
2018 Tese Plnbarreto.Pdf
1 UNIVERSIDADE FEDERAL DO CEARÁ FACULDADE DE EDUCAÇÃO PROGRAMA DE PÓS-GRADUAÇÃO EM EDUCAÇÃO BRASILEIRA CURSO DE DOUTORADO EM EDUCAÇÃO POLLIANA DE LUNA NUNES BARRETO EDUCAÇÃO E SANTIDADE: AS REPRESENTAÇÕES DO FEMININO NA REGIÃO DO CARIRI CEARENSE . FORTALEZA 2018 2 POLLIANA DE LUNA NUNES BARRETO EDUCAÇÃO E SANTIDADE: AS REPRESENTAÇÕES DO FEMININO NA REGIÃO DO CARIRI CEARENSE Tese apresentada ao Programa de Pós- graduação em Educação da Universidade Federal do Ceará, como parte dos requisitos para obtenção do título de Doutor em Educação. Área de Concentração: Educação Brasileira. Orientadora: Prof.ª. Drª. Patrícia Helena Carvalho Holanda. FORTALEZA 2018 3 FICHA CATALOGRÁFICA B223e BARRETO, Polliana de Luna Nunes Educação e Santidade: as representações do feminino na região do Cariri cearense. Polliana de Luna Nunes Barreto – Fortaleza, 2018. 220f.: il. Orientadora: Prof.ª. Drª. Patrícia Helena Carvalho Holanda. Tese (Programa de Pós-graduação em Educação) - UFC, 2018. 1. Educação - Santidade. 2. História - Gênero. Holanda, Drª. Patrícia Helena Carvalho, Orient. II. Título. CDD 253 Bibliotecária Responsável: Francisca Lunara da Cunha Alcantara – CRB- 3/1420 4 POLLIANA DE LUNA NUNES BARRETO EDUCAÇÃO E SANTIDADE: AS REPRESENTAÇÕES DO FEMININO NA REGIÃO DO CARIRI CEARENSE Tese apresentada ao Programa de Pós- graduação em Educação da Universidade Federal do Ceará, como parte dos requisitos para obtenção do título de Doutor em Educação. Área de Concentração: Educação Brasileira. Orientadora: Prof.ª. Drª. Patrícia Helena Carvalho Holanda. Aprovada em _____/______/________. ___________________________________________________________ Prof.ª. Drª. Patrícia Helena Carvalho Holanda (Orientadora) Universidade Federal do Ceará (UFC) ___________________________________________________________ Prof. Dr. Gisafran Nazareno Mota Jucá Universidade Federal do Ceará (UFC) ___________________________________________________________ Prof. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
International Magazine on Sea and ■ Vita Mari Ph
INTERNATIONAL MAGAZINE ON SEA AND ■ VITA MARI PH Nautilus Shells as collectors’ items (3) The Neritidae from the circumarabian seas VITA MARINA A magazine on marine Zoology, with emphasis Een blad op het gebied van mariene zoölogie, on molluscs met nadruk op weekdieren. EDITORIAL STAFF Jan Paul Buijs REDACTIE Henk Dekker Willem Faber David Feld Dr.Theo Kemperman Gijs Kronenberg Freek Titselaar Dr. Tom Walker COVER PLATE Leo Man in ’t Veld PLAAT OMSLAG ADVISORY BOARD Dr. A.C. van Bruggen REDACTIE ADVIESRAAD Dr. H.E. Coomans Prof. Dr. E. Gittenberger Prof. Dr. L.B. Holthuis PUBLISHER VITA MARINA AND STICHTING UITGEVER VITA MARINA EN SPIRULA BIOLOGIA MARITIMA SPIRULA BOARD BESTUUR PRESIDENT Jan Paul Buijs VOORZITTER SECRETARY Henk Dekker SECRETARIS TREASURER Gab Mulder PENNINGMEESTER Jeroen Goud ADDRESS P.O. Box 64628 ADRES NL-2506 CA DEN HAAG The Netherlands TELEPHONE +31(0)70-3551245 TELEFOON +31(0)70-3600434 FAX +31(0)70-3551245 FAX E-MAIL [email protected] E-MAIL WWW http://home.wxs.nl/~spirula WWW GIRO BANK ACCOUNT 606100 POSTGIROREKENING PRINTER RIBBERINK VAN DER GANG DRUKKER ZOETERMEER The Netherlands ISSN-0165-8980 Vita Marina 47(2): 25-28 August 2000 Nautilus Shells as collectors’ items in the “Kunst- und Wunderkammer”. Supplementary notes (2) Nautilusschelpen als verzamelobjecten in de “Kunst- und Wunderkammer”. Aanvullende notities (2) C.J.H.M. TAX Kempkeshoeve 55, NL-5256 NV Vught, the Netherlands As a sequel to my article with the above title (1995) and In aanvulling op mijn artikel met bovenstaande titel to the first supplement thereof (1996), 1 would like to (1995) en het eerste supplement hierop (1996), wil ik comment on some Nautilus objects that have been treat bij deze gelegenheid gaarne nog enkele tot dusverre ed in literature only once before or not at all. -
Ecce Mater Tua Vol. 1
Ecce Mater Tua A Journal of Mariology VOL. 1 January 1, 2018 Solemnity of Mary the Mother of God Editorial Board Editor Dr. Mark Miravalle, S.T.D. Franciscan University of Steubenville, Ohio Associate Editor Mr. Kevin Clarke, Ph.D. (cand.) Ave Maria University, Florida Advisory Board Msgr. Arthur Calkins, S.T.D. Vatican Ecclesia Dei, Emeritus Fr. Giles Dimock, O.P., S.T.D. Pontifical University of St. Thomas Aquinas (Angelicum), Emeritus Robert Fastiggi, S.T.D. Sacred Heart Major Seminary, Michigan Fr. Peter D. Fehlner, O.F.M. Conv. Ellicott City, Maryland Dr. Luis Bejar Fuentes Independent Editor and Journalist Mr. Daniel Garland, Jr., Ph.D. (cand.) Institute for Catholic Culture Scott Hahn, Ph.D. Franciscan University of Steubenville, Ohio Dr. Stephen Miletic Franciscan University of Steubenville, Ohio Christopher Malloy, Ph.D. University of Dallas, Texas John-Mark Miravalle, S.T.D. Mount St. Mary’s Seminary, Maryland Petroc Willey, Ph.D. Franciscan University of Steubenville, Ohio ii Ecce Mater Tua iii Ecce Mater Tua: A Journal of Mariology ISSN: 2573-5799 Instructions for Authors: To submit a paper for consideration, please first make sure that all personal references are stripped from the text and file properties, then email the document in Microsoft Word format (.doc or .docx) or in rich-text format (.rtf) to [email protected]. To ensure a smooth editorial process, please include a 250-350 word abstract at the beginning of the article, and be sure that formatting follows Chicago style. Ecce Mater Tua practices blind review. Submissions are evaluated anonymously by members of the editorial board and other scholars with appropriate expertise. -
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 -
The Very Forward CASTOR Calorimeter of the CMS Experiment
EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN) CERN-EP-2020-180 2021/02/11 CMS-PRF-18-002 The very forward CASTOR calorimeter of the CMS experiment The CMS Collaboration* Abstract The physics motivation, detector design, triggers, calibration, alignment, simulation, and overall performance of the very forward CASTOR calorimeter of the CMS exper- iment are reviewed. The CASTOR Cherenkov sampling calorimeter is located very close to the LHC beam line, at a radial distance of about 1 cm from the beam pipe, and at 14.4 m from the CMS interaction point, covering the pseudorapidity range of −6.6 < h < −5.2. It was designed to withstand high ambient radiation and strong magnetic fields. The performance of the detector in measurements of forward energy density, jets, and processes characterized by rapidity gaps, is reviewed using data collected in proton and nuclear collisions at the LHC. ”Published in the Journal of Instrumentation as doi:10.1088/1748-0221/16/02/P02010.” arXiv:2011.01185v2 [physics.ins-det] 10 Feb 2021 © 2021 CERN for the benefit of the CMS Collaboration. CC-BY-4.0 license *See Appendix A for the list of collaboration members Contents 1 Contents 1 Introduction . .1 2 Physics motivation . .3 2.1 Forward physics in proton-proton collisions . .3 2.2 Ultrahigh-energy cosmic ray air showers . .5 2.3 Proton-nucleus and nucleus-nucleus collisions . .5 3 Detector design . .6 4 Triggers and operation . .9 5 Event reconstruction and calibration . 12 5.1 Noise and baseline . 13 5.2 Gain correction factors . 15 5.3 Channel-by-channel intercalibration . -
Rua Do Norte, 44 • 1200-286 Lisboa • PORTUGAL
LIVRARIA CASTRO E SILVA LIVROS ANTIGOS – RARE BOOKS Rua do Norte, 44 • 1200-286 Lisboa • PORTUGAL Telefone +351 213 467 380 • Telemóvel +351 967 201 362 CATÁLOGO 140 –Janeiro de 2013 http://www.castroesilva.com/ • [email protected] Este documento permite visualizar imagens de cada obra do catálogo, clicando sobre o título da mesma. This document allows visualizing images from each of the works present in the catalogue by clicking on the title 1. ALBUM DE DESENHO COM 25 RETRATOS. De 15x22 cm. (formato oblongo). Cerca 100 fólios. S/l. S/d. (Circa 1790-1830). Encadernação da época em tela (pele diabo) com danos exteriores e marginais. Caderno de desenho executado com grande qualidade artística, ilustrado manualmente com 25 esboços (todos a carvão) com bustos masculinos retratados de perfil, todos com vestuário da época, provavelmente todos pertencendo a uma família aristocrática ou da alta burguesia do início do século xix. Terá servido de estudo para a execução de uma gravura? A proveniência indicia que o álbum terá tido eventual origem na ilha da Madeira. SKETCHBOOK. Oblong 15x22 cm. With 100 folium. (Circa 1790-1830). Binding: contemporary fabric. Illustrated with 25 hand drawings (all charcoal) of profiled males, fashioned with contemporary attires. Non identified author nor subjects; possibly belonging to an aristocratic or high bourgeoisie family. €200 2. ALMANACH DÉDIÉ AUX DAMES pour l’An 1826. À Paris chez Le Fuel, Lib edi. Et Delaunay, Palais Royal. Junto com: SOUVENIR. À Paris. Chez Le Fuel, Libraire Éditeur. S/d [1826]. In 12.º de 12x7,5 cm. Com 152, [7] pags. -
Downloaded for Personal Non-Commercial Research Or Study, Without Prior Permission Or Charge
MacArtney, Adrienne (2018) Atmosphere crust coupling and carbon sequestration on early Mars. PhD thesis. http://theses.gla.ac.uk/9006/ Copyright and moral rights for this work are retained by the author A copy can be downloaded for personal non-commercial research or study, without prior permission or charge This work cannot be reproduced or quoted extensively from without first obtaining permission in writing from the author The content must not be changed in any way or sold commercially in any format or medium without the formal permission of the author When referring to this work, full bibliographic details including the author, title, awarding institution and date of the thesis must be given Enlighten:Theses http://theses.gla.ac.uk/ [email protected] ATMOSPHERE - CRUST COUPLING AND CARBON SEQUESTRATION ON EARLY MARS By Adrienne MacArtney B.Sc. (Honours) Geosciences, Open University, 2013. Submitted in partial fulfilment of the requirements for the degree of Doctor of Philosophy at the UNIVERSITY OF GLASGOW 2018 © Adrienne MacArtney All rights reserved. The author herby grants to the University of Glasgow permission to reproduce and redistribute publicly paper and electronic copies of this thesis document in whole or in any part in any medium now known or hereafter created. Signature of Author: 16th January 2018 Abstract Evidence exists for great volumes of water on early Mars. Liquid surface water requires a much denser atmosphere than modern Mars possesses, probably predominantly composed of CO2. Such significant volumes of CO2 and water in the presence of basalt should have produced vast concentrations of carbonate minerals, yet little carbonate has been discovered thus far. -
Drug-Rich Phases Induced by Amorphous Solid Dispersion: Arbitrary Or Intentional Goal in Oral Drug Delivery?
pharmaceutics Review Drug-Rich Phases Induced by Amorphous Solid Dispersion: Arbitrary or Intentional Goal in Oral Drug Delivery? Kaijie Qian 1 , Lorenzo Stella 2,3 , David S. Jones 1, Gavin P. Andrews 1,4, Huachuan Du 5,6,* and Yiwei Tian 1,* 1 Pharmaceutical Engineering Group, School of Pharmacy, Queen’s University Belfast, 97 Lisburn Road, Belfast BT9 7BL, UK; [email protected] (K.Q.); [email protected] (D.S.J.); [email protected] (G.P.A.) 2 Atomistic Simulation Centre, School of Mathematics and Physics, Queen’s University Belfast, 7–9 College Park E, Belfast BT7 1PS, UK; [email protected] 3 David Keir Building, School of Chemistry and Chemical Engineering, Queen’s University Belfast, Stranmillis Road, Belfast BT9 5AG, UK 4 School of Pharmacy, China Medical University, No.77 Puhe Road, Shenyang North New Area, Shenyang 110122, China 5 Laboratory of Applied Mechanobiology, Department of Health Sciences and Technology, ETH Zurich, Vladimir-Prelog-Weg 4, 8093 Zurich, Switzerland 6 Simpson Querrey Institute, Northwestern University, 303 East Superior Street, 11th Floor, Chicago, IL 60611, USA * Correspondence: [email protected] (H.D.); [email protected] (Y.T.); Tel.: +41-446339049 (H.D.); +44-2890972689 (Y.T.) Abstract: Among many methods to mitigate the solubility limitations of drug compounds, amor- Citation: Qian, K.; Stella, L.; Jones, phous solid dispersion (ASD) is considered to be one of the most promising strategies to enhance D.S.; Andrews, G.P.; Du, H.; Tian, Y. the dissolution and bioavailability of poorly water-soluble drugs. -
In Pdf Format
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