Monitoring and Modelling Volcanoes with Assessment of Their Hazards by Means of Remote Sensing and Analogue Modelling
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Placing World War I in the History of Mathematics David Aubin, Catherine Goldstein
Placing World War I in the History of Mathematics David Aubin, Catherine Goldstein To cite this version: David Aubin, Catherine Goldstein. Placing World War I in the History of Mathematics. 2013. hal- 00830121v1 HAL Id: hal-00830121 https://hal.sorbonne-universite.fr/hal-00830121v1 Preprint submitted on 4 Jun 2013 (v1), last revised 8 Jul 2014 (v2) HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Placing World War I in the History of Mathematics David Aubin and Catherine Goldstein Abstract. In the historical literature, opposite conclusions were drawn about the impact of the First World War on mathematics. In this chapter, the case is made that the war was an important event for the history of mathematics. We show that although mathematicians' experience of the war was extremely varied, its impact was decisive on the life of a great number of them. We present an overview of some uses of mathematics in war and of the development of mathematics during the war. We conclude by arguing that the war also was a crucial factor in the institutional modernization of mathematics. Les vrais adversaires, dans la guerre d'aujourd'hui, ce sont les professeurs de math´ematiques`aleur table, les physiciens et les chimistes dans leur laboratoire. -
No. 40. the System of Lunar Craters, Quadrant Ii Alice P
NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates. -
Los Morados Scoria Cone, Mendoza, Argentina
Cent. Eur. J. Geosci. • 3(2) • 2011 • 102-118 DOI: 10.2478/s13533-011-0008-4 Central European Journal of Geosciences The role of collapsing and cone rafting on eruption style changes and final cone morphology: Los Morados scoria cone, Mendoza, Argentina Research Article Karoly Németh1, Corina Risso2, Francisco Nullo3, Gabor Kereszturi1,4 1 Volcanic Risk Solutions, Massey University, Private Bag 11 222, Palmerston North, New Zealand 2 Departamento de Geología , Area Riesgo Volcánico, FCEyN-Universidad de Buenos Aires, Argentina 3 CONICET-SEGEMAR, Buenos Aires, Argentina 4 Geological Institute of Hungary, Stefánia út 14, Budapest, 1143, Hungary Received 30 November 2010; accepted 31 January 2011 Abstract: Payún Matru Volcanic Field is a Quaternary monogenetic volcanic field that hosts scoria cones with perfect to breached morphologies. Los Morados complex is a group of at least four closely spaced scoria cones (Los Morados main cone and the older Cones A, B, and C). Los Morados main cone was formed by a long lived eruption of months to years. After an initial Hawaiian-style stage, the eruption changed to a normal Strombolian, cone- building style, forming a cone over 150 metres high on a northward dipping (∼4˚) surface. An initial cone gradually grew until a lava flow breached the cone’s base and rafted an estimated 10% of the total volume. A sudden sector collapse initiated a dramatic decompression in the upper part of the feeding conduit and triggered violent a Strombolian style eruptive stage. Subsequently, the eruption became more stable, and changed to a regular Strombolian style that partially rebuilt the cone. -
The Impact of Star Cluster Environments on Planet Formation
The Impact of Star Cluster Environments on Planet Formation Rhana Bethany Nicholson A thesis submitted in partial fulfilment of the requirements of Liverpool John Moores University for the degree of Doctor of Philosophy June 2019 i Declaration of Authorship I, Rhana Bethany Nicholson, declare that this thesis titled, “The Impact of Star Cluster Environments on Planet Formation” and the work presented in it are my own. I confirm that: • This work was done wholly or mainly while in candidature for a research degree at this University. • Where any part of this thesis has previously been submitted for a degree or any other qualification at this University or any other institution, this has been clearly stated. • Where I have consulted the published work of others, this is always clearly attributed. • Where I have quoted from the work of others, the source is always given. With the exception of such quotations, this thesis is entirely my own work. • I have acknowledged all main sources of help. • Where the thesis is based on work done by myself jointly with others, I have made clear exactly what was done by others and what I have contributed myself. Signed: Date: ii To Mum and Dad, for making me do Kumon. iii “For all the tenure of humans on Earth, the night sky has been a companion and an inspiration... At the very moment that humans discovered the scale of the Universe and found that their most unconstrained fancies were in fact dwarfed by the true dimensions of even the Milky Way Galaxy, they took steps that ensured that their descendants would be unable to see the stars at all...” - Carl Sagan, Contact iv Acknowledgements Firstly I must begin by thanking my supervisor, Richard Parker, without whom this thesis would most definitely not exist. -
Petrogenesis of Natrocarbonatite at Oldoinyo Lengai, East Africa— Evidence from Fe and U Isotope Variations
PETROGENESIS OF NATROCARBONATITE AT OLDOINYO LENGAI, EAST AFRICA— EVIDENCE FROM FE AND U ISOTOPE VARIATIONS BY ZHENHAO ZHOU THESIS Submitted in partial fulfillment of the requirements for the degree of Master of Science in Geology in the Graduate College of the University of Illinois at Urbana-Champaign, 2017 Urbana, Illinois Adviser: Professor Craig C. Lundstrom Abstract Ol Doinyo Lengai (ODL), Tanzania, is the only active carbonatite volcano on earth. Cyclical activity that consists of quiescent natrocarbonatite lava flow, explosive silicate eruption and dormancy has been observed throughout the 20th century at ODL. From 2007 to 2008, ODL explosively erupted coexisting natrocarbonatites and nephelinites. Numerous studies have been aimed at understanding how ODL natrocarbonatite forms. Liquid immiscibility is a favored hypothesis although condensate fluid separation is an alternative model. However, the exact mechanism that forms the ODL natrocarbonatite remains unresolved. We carried out Fe and U isotope analyses among a variety of ODL samples. Our sample set includes natrocarbonatite that erupted in 2005, 2 comingled tephras (mixture of natrocarbonatite and nephelinite) and a sequence of 8 nephelinite tephras that erupted in 2007- 2008; as well as magnetites separated from 2005 natrocarbontite; Ti-andradites and clinopyroxenes that were separated from one of the nephelinite tephras. Our results show a lighter Fe isotope composition of natrocarbonatite (!56Fe of -0.08‰ relative to IRMM-14) compared to nephelinite tephras (-0.06 to 0.20 ‰ relative to IRMM-14). Magnetites yield heavier Fe isotope composition (0.03‰) than natrocarbonatite; Ti-andradite has the heaviest Fe isotope composition among all analyzed samples due to its enrichment in Fe3+. -
2017 Chicxulub Revealed
THE UNIVERSITY TEXAS OF AUSTIN AT JACKSON• SCHOOL GEOSCIENCES OF 2017 NEWSLETTER• Newsletter2 017 Chicxulub Revealed A first look at rocks from the crater left by the asteroid that wiped out non-avian dinosaurs WELCOME Dear Alumni and Friends he devastation that Hurricane Harvey brought to Texas communities in August was a tragic reminder of how vital it is to understand our planet and T its processes. Shortly after the hurricane struck, our scientists, through our Rapid Response program, began to conduct research to understand how Harvey has impacted the coast and offshore Gulf of Mexico. This research will help determine the best ways to deal with many coastal issues in the aftermath of the storm, and how we might better prepare for such events in the future. You can read more about the mission on page 18. Rapid response efforts on the effects of abrupt, catastrophic geoscience events COVER: GRANITE FROM THE PEAK RING OF provide critical science that can benefit society. This is what we strive to do here at the THE CHICXULUB CRATER FORMED BY THE Jackson School of Geosciences. This year’s Newsletter holds some tremendous examples. ASTEROID STRIKE THAT WIPED OUT ALL NON- AVIAN DINOSAURS I’d like to draw your attention to the story on page 58 about the scientific coring mission led by Peter Flemings to bring back samples of methane hydrate from ABOVE: MEMBERS OF THE JACKSON beneath the Gulf of Mexico. This is a cutting-edge research project on a potential SCHOOL-LED TEAM CORING FOR SAMPLES OF METHANE HYDRATE IN THE GULF OF MEXICO future energy source that very few schools in the world would be able to mount. -
Of 16 ADA PALMER Curriculum Vitae the University of Chicago 773-834
ADA PALMER Curriculum Vitae The University of Chicago 773-834-8178 Department of History Fax: 773-702-7550 1126 East 59th Street, Mailbox 47 [email protected] Chicago, IL 60637 adapalmer.com ● exurbe.com EDUCATION AND EMPLOYMENT Academic Employment University of Chicago, Department of History, Associate Professor 2018-present . Assistant Professor, 2014-2018 o Associate Member of the Department of Classics o Member of the Institute on the Formation of Knowledge o Affiliate Member of the Center for the Study of Gender and Sexuality Texas A&M University, Department of History, 2009 – 2014, Assistant Professor Education Ph.D., History, 2009, Harvard University, Cambridge, MA M.A., History, 2003, Harvard University, Cambridge, MA B.A., History, cum laude, 2001, Bryn Mawr College, Bryn Mawr, PA A.A., with distinction, 1999, Simon’s Rock College of Bard (now Bard College at Simon’s Rock), Great Barrington, MA Non-Degree Programs: o Seminario di Alta Cultura, 2010, Istituto Internazionale di Studi Piceni, Sassoferrato, Italy o Aestiva Romae Latinitatis, 2004, with Fr. Reginald Foster, Rome, Italy Languages: English, Italian, French, Latin, Ancient Greek, Gothic, German (reading). ACADEMIC PUBLICATIONS Books Reading Lucretius in the Renaissance. I Tatti Renaissance Studies Series. Cambridge, MA: Harvard University Press, 2014. The Recovery of Classical Philosophy in the Renaissance, a Brief Guide, Quaderni di Rinascimento 44. Co-author with James Hankins. Istituto Nazionale di Studi sul Rinascimento. Florence: Leo S. Olschki, 2008. Peer-Reviewed Articles and Book Chapters “Pomponio Leto’s Lucretius and the Negative Space of Humanist Latin Knowledge.” Erudition and the Republic of Letters, forthcoming. Page 1 of 16 Curriculum Vitae Ada Palmer “The Effects of Authorial Strategies for Transforming Antiquity on the Place of the Renaissance in the Current Philosophical Canon,” in Beyond Reception: Renaissance Humanism and the Transformation of Classical Antiquity, eds. -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
Glossary of Lunar Terminology
Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites. -
Early Greek Alchemy, Patronage and Innovation in Late Antiquity CALIFORNIA CLASSICAL STUDIES
Early Greek Alchemy, Patronage and Innovation in Late Antiquity CALIFORNIA CLASSICAL STUDIES NUMBER 7 Editorial Board Chair: Donald Mastronarde Editorial Board: Alessandro Barchiesi, Todd Hickey, Emily Mackil, Richard Martin, Robert Morstein-Marx, J. Theodore Peña, Kim Shelton California Classical Studies publishes peer-reviewed long-form scholarship with online open access and print-on-demand availability. The primary aim of the series is to disseminate basic research (editing and analysis of primary materials both textual and physical), data-heavy re- search, and highly specialized research of the kind that is either hard to place with the leading publishers in Classics or extremely expensive for libraries and individuals when produced by a leading academic publisher. In addition to promoting archaeological publications, papyrolog- ical and epigraphic studies, technical textual studies, and the like, the series will also produce selected titles of a more general profile. The startup phase of this project (2013–2017) was supported by a grant from the Andrew W. Mellon Foundation. Also in the series: Number 1: Leslie Kurke, The Traffic in Praise: Pindar and the Poetics of Social Economy, 2013 Number 2: Edward Courtney, A Commentary on the Satires of Juvenal, 2013 Number 3: Mark Griffith, Greek Satyr Play: Five Studies, 2015 Number 4: Mirjam Kotwick, Alexander of Aphrodisias and the Text of Aristotle’s Meta- physics, 2016 Number 5: Joey Williams, The Archaeology of Roman Surveillance in the Central Alentejo, Portugal, 2017 Number 6: Donald J. Mastronarde, Preliminary Studies on the Scholia to Euripides, 2017 Early Greek Alchemy, Patronage and Innovation in Late Antiquity Olivier Dufault CALIFORNIA CLASSICAL STUDIES Berkeley, California © 2019 by Olivier Dufault. -
Tezuka Dossier.Indd
Dossier de premsa Organitza Col·labora Del 31 d’octubre del 2019 al 6 de gener del 2020 Organitza i produeix: FICOMIC amb la col·laboració del Museu Nacional d’Art de Catalunya Comissari: Stéphane Beaujean Sala d’exposicions temporals 2 Astro Boy © Tezuka productions • El mangaka Osamu Tezuka, també conegut com a Déu del Manga per la seva immensa aportació a la vinyeta japonesa, és el protagonista d’una exposició que es podrà veure durant gairebé un parell de mesos al Museu Nacional d’Art de Catalunya, i que està integrada per gairebé 200 originals d’aquest autor. • L’exposició ha estat produïda per FICOMIC gràcies a l’estreta col·laboració amb el Mu- seu Nacional d’Art de Catalunya, Tezuka Productions i el Festival de la Bande Desinneè d’Angulema. Osamu Tezuka, el Déu del Manga és una mostra sense precedents al nos- tre país, que vol donar a conèixer de més a prop l’obra d’un creador vital per entendre l’evolució del manga després de la Segona Guerra Mundial, i també a un dels autors de manga més prestigiosos i prolífi cs a nivell mundial. • Osamu Tezuka, el Déu del Manga es podrà visitar a partir del 31 d’octubre d’aquest any, coincidint amb l’inici de la 25a edició del Manga Barcelona, fi ns al 6 de gener de 2020. 3 Fénix © Tezuka productions Oda a Kirihito © Tezuka productions El còmic al Museu Nacional Aquest projecte forma part de l’acord de col·laboració entre FICOMIC i el Museu Nacional d’Art de Catalunya gràcies al qual també es va produir l’exposició Corto Maltés, de Juan Díaz Canales i Rubén Pellejero, o la més recent El Víbora. -
Crater Lake National Park Natural Resource Condition Assessment
National Park Service U.S. Department of the Interior Natural Resource Stewardship and Science Crater Lake National Park Natural Resource Condition Assessment Natural Resource Report NPS/NRSS/WRD/NRR—2013/724 ON THE COVER Crater Lake in June. Photo courtesy of the National Park Service Crater Lake National Park Natural Resource Condition Assessment Natural Resource Report NPS/NRSS/WRD/NRR—2013/724 Paul R. Adamus Water Resources Science Program Oregon State University Corvallis, Oregon and Adamus Resource Assessment, Inc. Corvallis, Oregon Dennis C. Odion, Gregory V. Jones, Lorin C. Groshong, Ryan Reid Department of Environmental Studies Southern Oregon University Ashland, Oregon This report was prepared under Task Agreement J8W07100032 (Cooperative Agreement H8W07060001) between the National Park Service and Southern Oregon University. November 2013 U.S. Department of the Interior National Park Service Natural Resource Stewardship and Science Fort Collins, Colorado The National Park Service, Natural Resource Stewardship and Science office in Fort Collins, Colorado, publishes a range of reports that address natural resource topics. These reports are of interest and applicability to a broad audience in the National Park Service and others in natural resource management, including scientists, conservation and environmental constituencies, and the public. The Natural Resource Report Series is used to disseminate high-priority, current natural resource management information with managerial application. The series targets a general, diverse audience, and may contain NPS policy considerations or address sensitive issues of management applicability. Examples of the diverse array of reports published in this series include vital signs monitoring plans; monitoring protocols; "how to" resource management papers; proceedings of resource management workshops or conferences; annual reports of resource programs or divisions of the Natural Resource Program Center; resource action plans; fact sheets; and regularly-published newsletters.