2020 Course Catalog
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Climate Change and Human Health: Risks and Responses
Climate change and human health RISKS AND RESPONSES Editors A.J. McMichael The Australian National University, Canberra, Australia D.H. Campbell-Lendrum London School of Hygiene and Tropical Medicine, London, United Kingdom C.F. Corvalán World Health Organization, Geneva, Switzerland K.L. Ebi World Health Organization Regional Office for Europe, European Centre for Environment and Health, Rome, Italy A.K. Githeko Kenya Medical Research Institute, Kisumu, Kenya J.D. Scheraga US Environmental Protection Agency, Washington, DC, USA A. Woodward University of Otago, Wellington, New Zealand WORLD HEALTH ORGANIZATION GENEVA 2003 WHO Library Cataloguing-in-Publication Data Climate change and human health : risks and responses / editors : A. J. McMichael . [et al.] 1.Climate 2.Greenhouse effect 3.Natural disasters 4.Disease transmission 5.Ultraviolet rays—adverse effects 6.Risk assessment I.McMichael, Anthony J. ISBN 92 4 156248 X (NLM classification: WA 30) ©World Health Organization 2003 All rights reserved. Publications of the World Health Organization can be obtained from Marketing and Dis- semination, World Health Organization, 20 Avenue Appia, 1211 Geneva 27, Switzerland (tel: +41 22 791 2476; fax: +41 22 791 4857; email: [email protected]). Requests for permission to reproduce or translate WHO publications—whether for sale or for noncommercial distribution—should be addressed to Publications, at the above address (fax: +41 22 791 4806; email: [email protected]). The designations employed and the presentation of the material in this publication do not imply the expression of any opinion whatsoever on the part of the World Health Organization concerning the legal status of any country, territory, city or area or of its authorities, or concerning the delimitation of its frontiers or boundaries. -
Potential European Contributions to Europa Lander Mission
The Europa Initiative for ESA’s M5 mission Report to OPAG Michel Blanc, Geraint Jones, Olga Prieto-Ballesteros, Veerle Sterken, Javier Gomez-Elvira, David Mimoun, Adam Masters, Sascha Kempf, Luciano Iess, John Cooper, Zita Martins, Ralph Lorenz, Jérémie lasue, Nicolas André, Bruce Bills, Gael Choblet, Geoff Collins, Philippe Garnier, Kevin Hand, Paul Hartogh, Krishan Khurana, Andrea Longobardo, Katrin Stephan, Federico Tosi, Steve Vance, Tim van Hoolst, Roland Wagner, Frances Westall, Martin Wolverk, William Desprats, Ryan Russell, Georges Balmino, Julien Laurent-Varin and the Europa Initiative team August 11th, 2016 1 EI WORKING SCHEME Europa M5 for an ESA contribution to the Europa Lander mission Initiative Penetrator Contribution to Cubesat? Orbiter or… NASA lander A – GLOBAL GEOPHYSICSMagnetospheric interactions CHARACTERIZE EUROPA AS A COMPLEX DYNAMICAL SYSTEM B – ExosphereOF COUPLED LAYERS(neutrals, dust, plumes) FROM CORE TO PLASMA ENVELOPE THROUGH OCEAN AND CRYOSPHERE dimension RESPONDING TO E – Geophysics (internalJUPITER SYSTEM FORCING: TIDAL, MAGNETOSPHERICstructure, incl. Characterization of the ocean) themes ASTROBIOLOGY CONTRIBUTE TO NASA’s LANDER SCIENCE Science AND PROVIDE AN ADDITIONAL ELEMENT (AWL) As resources permit « Spacecraft » dimension EI contribution to EUROPA LanDer : SubmitteD LOI’s Joint Europa Mission (Blanc/Prieto-Ballesteros) • Baseline: Carrier-Orbiter + lander joint NASA/ESA mission: – P1a: Carrier-Orbiter provided by ESA, operated by NASA; – P1b: Alternative option: Carrier-Orbiter provided and operated by NASA; science platform (+ sub-systems?) provided by ESA – Science platform open to both ESA member states and NASA • Option 1: Augmented surface science: Astrobiology Wet Laboratory (AWL) provided by ESA + Member States to enhance landing site exploration. • Option 2: Augmented orbital science - cubesat released from carrier. -
ESA Strategy for Science at the Moon
ESA UNCLASSIFIED - Releasable to the Public ESA Strategy for Science at the Moon ESA UNCLASSIFIED - Releasable to the Public EXECUTIVE SUMMARY A new era of space exploration is beginning, with multiple international and private sector actors engaged and with the Moon as its cornerstone. This renaissance in lunar exploration will offer new opportunities for science across a multitude of disciplines from planetary geology to astronomy and astrobiology whilst preparing the knowledge humanity will need to explore further into the Solar System. Recent missions and new analyses of samples retrieved during Apollo have transformed our understanding of the Moon and the science that can be performed there. We now understand the scientific importance of further exploration of the Moon to understand the origins and evolution of Earth and the cosmic context of life’s emergence on Earth and our future in space. ESA’s priorities for scientific activities at the Moon in the next ten years are: • Analysis of new and diverse samples from the Moon. • Detection and characterisation of polar water ice and other lunar volatiles. • Deployment of geophysical instruments and the build up a global geophysical network. • Identification and characterisation of potential resources for future exploration. • Deployment long wavelength radio astronomy receivers on the lunar far side. • Characterisation of the dynamic dust, charge and plasma environment. • Characterisation of biological sensitivity to the lunar environment. ESA UNCLASSIFIED - Releasable to the Public -
A Future Mars Environment for Science and Exploration
Planetary Science Vision 2050 Workshop 2017 (LPI Contrib. No. 1989) 8250.pdf A FUTURE MARS ENVIRONMENT FOR SCIENCE AND EXPLORATION. J. L. Green1, J. Hol- lingsworth2, D. Brain3, V. Airapetian4, A. Glocer4, A. Pulkkinen4, C. Dong5 and R. Bamford6 (1NASA HQ, 2ARC, 3U of Colorado, 4GSFC, 5Princeton University, 6Rutherford Appleton Laboratory) Introduction: Today, Mars is an arid and cold world of existing simulation tools that reproduce the physics with a very thin atmosphere that has significant frozen of the processes that model today’s Martian climate. A and underground water resources. The thin atmosphere series of simulations can be used to assess how best to both prevents liquid water from residing permanently largely stop the solar wind stripping of the Martian on its surface and makes it difficult to land missions atmosphere and allow the atmosphere to come to a new since it is not thick enough to completely facilitate a equilibrium. soft landing. In its past, under the influence of a signif- Models hosted at the Coordinated Community icant greenhouse effect, Mars may have had a signifi- Modeling Center (CCMC) are used to simulate a mag- cant water ocean covering perhaps 30% of the northern netic shield, and an artificial magnetosphere, for Mars hemisphere. When Mars lost its protective magneto- by generating a magnetic dipole field at the Mars L1 sphere, three or more billion years ago, the solar wind Lagrange point within an average solar wind environ- was allowed to directly ravish its atmosphere.[1] The ment. The magnetic field will be increased until the lack of a magnetic field, its relatively small mass, and resulting magnetotail of the artificial magnetosphere its atmospheric photochemistry, all would have con- encompasses the entire planet as shown in Figure 1. -
Caverns Measureless to Man: Interdisciplinary Planetary Science & Technology Analog Research Underwater Laser Scanner Survey (Quintana Roo, Mexico)
Caverns Measureless to Man: Interdisciplinary Planetary Science & Technology Analog Research Underwater Laser Scanner Survey (Quintana Roo, Mexico) by Stephen Alexander Daire A Thesis Presented to the Faculty of the USC Graduate School University of Southern California In Partial Fulfillment of the Requirements for the Degree Master of Science (Geographic Information Science and Technology) May 2019 Copyright © 2019 by Stephen Daire “History is just a 25,000-year dash from the trees to the starship; and while it’s going on its wild and woolly but it’s only like that, and then you’re in the starship.” – Terence McKenna. Table of Contents List of Figures ................................................................................................................................ iv List of Tables ................................................................................................................................. xi Acknowledgements ....................................................................................................................... xii List of Abbreviations ................................................................................................................... xiii Abstract ........................................................................................................................................ xvi Chapter 1 Planetary Sciences, Cave Survey, & Human Evolution................................................. 1 1.1. Topic & Area of Interest: Exploration & Survey ....................................................................12 -
Thermosphere? Why Is It So Hot? Atmosphere Model and Thermosphere 5
UNIT 6, LESSON 1: EARTH LAYERS & ATMOSPHERE LET’S BUILD OUR EARTH AND THE ATMOSPHERE 1 & 2 Where is earth’s crust? What is the difference between the 1. Read/annotate the oceanic and continental crust? paragraph(s) Crust and Mantle Where is the earth’s mantle? What is a plate? What part of the 2. Answer the questions mantle is below the plates? that go with the 3 Where is the earth’s core? How is the core similar to the mantle? paragraph(s) Core 4 & 5 Where is the troposphere? What are you likely to find there? Name at least 3 things. 3. Show Mrs. Stoddard Troposphere and Stratosphere your answers Where is the stratosphere? Why would the air be warm in the 4. If you get it correct, get stratosphere? Where is the mesosphere? Why do meteors burn in this layer? a piece of your 6 & 7 Mesosphere Where is the thermosphere? Why is it so hot? atmosphere model And Thermosphere 5. Repeat until your 8 Where is the exosphere? Why do some experts ignore the exosphere and think the thermosphere is the outermost layer of Exosphere model is finished! the earth’s atmosphere? CHECK YOUR MODEL! Exosphere Thermosphere Mesosphere Stratosphere Troposphere Core Name Class Period Mantle Crust HOW DID WE DO ON THE ATMOSPHERE MODEL? LET’S SET UP OUR JOURNALS! Earth’s Layers and Atmosphere 1:301:291:281:271:261:251:241:231:221:211:201:191:181:171:161:151:141:131:121:111:101:091:081:071:061:051:041:031:021:011:000:590:580:570:560:550:540:530:520:510:500:490:480:470:460:450:440:430:420:410:400:390:380:370:360:350:340:330:320:310:300:290:280:270:260:250:240:230:220:210:200:190:180:170:160:150:140:130:120:110:100:090:080:070:060:050:040:030:020:01End -
Human Adaptation and Safety in Space
SICSA SPACE ARCHITECTURE SEMINAR LECTURE SERIES PART II : HUMAN ADAPTATION AND SAFETY IN SPACE www.sicsa.uh.edu LARRY BELL, SASAKAWA INTERNATIONAL CENTER FOR SPACE ARCHITECTURE (SICSA) GERALD D.HINES COLLEGE OF ARCHITECTURE, UNIVERSITY OF HOUSTON, HOUSTON, TX The Sasakawa International Center for SICSA routinely presents its publications, Space Architecture (SICSA), an research and design results and other organization attached to the University of information materials on its website Houston’s Gerald D. Hines College of (www.sicsa.uh.edu). This is done as a free Architecture, offers advanced courses service to other interested institutions and that address a broad range of space individuals throughout the world who share our systems research and design topics. In interests. 2003 SICSA and the college initiated Earth’s first MS-Space Architecture This report is offered in a PowerPoint format with degree program, an interdisciplinary 30 the dedicated intent to be useful for academic, credit hour curriculum that is open to corporate and professional organizations who participants from many fields. Some wish to present it in group forums. The document students attend part-time while holding is the second in a series of seminar lectures that professional employment positions at SICSA has prepared as information material for NASA, affiliated aerospace corporations its own academic applications. We hope that and other companies, while others these materials will also be valuable for others complete their coursework more rapidly who share our -
The Mutual Influence of Science Fiction and Innovation
Nesta Working Paper No. 13/07 Better Made Up: The Mutual Influence of Science fiction and Innovation Caroline Bassett Ed Steinmueller George Voss Better Made Up: The Mutual Influence of Science fiction and Innovation Caroline Bassett Ed Steinmueller George Voss Reader in Digital Media, Professor of Information and Research Fellow, Faculty of Arts, Research Centre for Material Technology, SPRU, University University of Brighton, Visiting Digital Culture, School of of Communication Sussex Fellow at SPRU, University of Media, Film and Music, Sussex University of Sussex Nesta Working Paper 13/07 March 2013 www.nesta.org.uk/wp13-07 Abstract This report examines the relationship between SF and innovation, defined as one of mutual engagement and even co-constitution. It develops a framework for tracing the relationships between real world science and technology and innovation and science fiction/speculative fiction involving processes of transformation, central to which are questions of influence, persuasion, and desire. This is contrasted with the more commonplace assumption of direct linear transmission, SF providing the inventive seed for innovation– instances of which are the exception rather than the rule. The model of influence is developed through an investigation of the nature and evolution of genre, the various effects/appeals of different forms of expression, and the ways in which SF may be appropriated by its various audiences. This is undertaken (i) via an inter- disciplinary survey of work on SF, and a consideration the historical construction of genre and its on-going importance, (ii) through the development of a prototype database exploring transformational paths, and via more elaborated loops extracted from the database, and (iii) via experiments with the development of a web crawl tool, to understand at a different scale, using tools of digital humanities, how fictional ideas travel. -
Arthur C. Clarke 2001: a Space Odyssey
Volume 33, Issue 2 AIAAAIAA HoustonHouston SectionSection www.aiaa-houston.orgwww.aiaa-houston.org April 2008 Arthur C. Clarke 1917 - 2008 2001: A Space Odyssey - 40 Years Later Yesterday’s Tomorrow Artwork by Jon C. Rogers and Pat Rawlings AIAA Houston Horizons April 2008 Page 1 April 2008 T A B L E O F C O N T E N T S From the Acting Editor 3 HOUSTON Chair’s Corner 4 2001: A Space Odyssey - 40 Years Later: Yesterday’s Tomorrow 5 Horizons is a quarterly publication of the Houston section of the American Institute of Aeronautics and Astronautics. International Space Activities Committee (ISAC) 14 Arthur C. Clarke: A Prophet Vindicated by Gregory Benford 16 Acting Editor: Douglas Yazell [email protected] Book Review (Subject: Ellington Field in Houston) & Staying Informed 18 Assistant Editors: Scholarship & Annual Technical Symposium (ATS 2008) 19 Jon Berndt Dr. Rattaya Yalamanchili Lunch-and-Learn Summary: Mars Rovers by Dr. Mark Adler/JPL 20 Don Kulba Robert Beremand Dinner Meeting Summary: John Frassanito & Associates 21 Lunch & Learn: Sailing the Space Station with Zero-Propellant Guidance 22 AIAA Houston Section Executive Council Membership 23 Chair: Douglas Yazell Inaugural Space Center Lecture Series: Harrison Schmitt of Apollo 17 24 Chair-Elect: Chad Brinkley Past Chair: Dr. Jayant Ramakrishnan Yuri’s Night Houston by AAS, co-sponsored by AIAA Houston Section 26 Secretary: Sarah Shull Constellation Earth, Michel Bonavitacola, AAAF , Toulouse, France 27 Treasurer: Tim Propp Calendar 30 JJ Johnson Sean Carter Cranium Cruncher and a Pre-College Event: Engineer for a Day 31 Vice-Chair, Vice-Chair, Operations Branch Technical Branch Odds and Ends: EAA Houston Chapter 12, James C. -
ESA Space Weather STUDY Alcatel Consortium
ESA Space Weather STUDY Alcatel Consortium SPACE Weather Parameters WP 2100 Version V2.2 1 Aout 2001 C. Lathuillere, J. Lilensten, M. Menvielle With the contributions of T. Amari, A. Aylward, D. Boscher, P. Cargill and S.M. Radicella 1 2 1 INTRODUCTION........................................................................................................................................ 5 2 THE MODELS............................................................................................................................................. 6 2.1 THE SUN 6 2.1.1 Reconstruction and study of the active region static structures 7 2.1.2 Evolution of the magnetic configurations 9 2.2 THE INTERPLANETARY MEDIUM 11 2.3 THE MAGNETOSPHERE 13 2.3.1 Global magnetosphere modelling 14 2.3.2 Specific models 16 2.4 THE IONOSPHERE-THERMOSPHERE SYSTEM 20 2.4.1 Empirical and semi-empirical Models 21 2.4.2 Physics-based models 23 2.4.3 Ionospheric profilers 23 2.4.4 Convection electric field and auroral precipitation models 25 2.4.5 EUV/UV models for aeronomy 26 2.5 METEOROIDS AND SPACE DEBRIS 27 2.5.1 Space debris models 27 2.5.2 Meteoroids models 29 3 THE PARAMETERS ................................................................................................................................ 31 3.1 THE SUN 35 3.2 THE INTERPLANETARY MEDIUM 35 3.3 THE MAGNETOSPHERE 35 3.3.1 The radiation belts 36 3.4 THE IONOSPHERE-THERMOSPHERE SYSTEM 36 4 THE OBSERVATIONS ........................................................................................................................... -
Ringworld Engineers Larry Niven PART ONE CHAPTER 1 UNDER the WIRE
Ringworld 02 Ringworld Engineers Larry Niven PART ONE CHAPTER 1 UNDER THE WIRE Louis Wu was under the wire when two men came to invade his privacy. He was in full lotus position on the lush yellow indoor-grass carpet. His smile was blissful, dreamy. The apartment was small, just one big room. He could see both doors. But, lost in the joy that only a wirehead knows, he never saw them arrive. Suddenly they were there: two pale youths, both over seven feet tall, studying Louis with contemptuous smiles. One snorted and dropped something weapon-shaped in his pocket. They were stepping forward as Louis stood up. It wasn't just the happy smile that fooled them. It was the fist-sized droud that protruded like a black plastic canker from the crown of Louis Wu's head. They were dealing with a current addict, and they knew what to expect. For years the man must have had no thought but for the wire trickling current into the pleasure center of his brain. He would be near starvation from self-neglect. He was small, a foot and a half shorter than either of the invaders. He — As they reached for him Louis bent far sideways, for balance, and kicked once, twice, thrice. One of the invaders was down, curled around himself and not breathing, before the other found the wit to back away. Louis came after him. What held the youth half paralyzed was the abstracted bliss with which Louis came to kill him. Too late, he reached for the stunner he'd pocketed. -
Ionizing Radiation in Earth's Atmosphere and in Space Near Earth May 2011 6
Federal Aviation Administration DOT/FAA/AM-11/9 Office of Aerospace Medicine Washington, DC 20591 Ionizing Radiation in Earth’s Atmosphere and in Space Near Earth Wallace Friedberg Kyle Copeland Civil Aerospace Medical Institute Federal Aviation Administration Oklahoma City, OK 73125 May 2011 Final Report OK-11-0024-JAH NOTICE This document is disseminated under the sponsorship of the U.S. Department of Transportation in the interest of information exchange. The United States Government assumes no liability for the contents thereof. ___________ This publication and all Office of Aerospace Medicine technical reports are available in full-text from the Civil Aerospace Medical Institute’s publications Web site: www.faa.gov/library/reports/medical/oamtechreports Technical Report Documentation Page 1. Report No. 2. Government Accession No. 3. Recipient's Catalog No. DOT/FAA/AM-11/9 4. Title and Subtitle 5. Report Date Ionizing Radiation in Earth's Atmosphere and in Space Near Earth May 2011 6. Performing Organization Code 7. Author(s) 8. Performing Organization Report No. Friedberg W, Copeland K 9. Performing Organization Name and Address 10. Work Unit No. (TRAIS) FAA Civil Aerospace Medical Institute P.O. Box 25082 11. Contract or Grant No. Oklahoma City, OK 73125 12. Sponsoring Agency name and Address 13. Type of Report and Period Covered Office of Aerospace Medicine Federal Aviation Administration 800 Independence Ave., S.W. Washington, DC 20591 14. Sponsoring Agency Code 15. Supplemental Notes 16. Abstract The Civil Aerospace Medical Institute of the FAA is charged with identifying health hazards in air travel and in commercial human space travel.