Changing Climate a Guide for Teaching Climate Change in Grades 3 to 8 the Climate System 1 and Greenhouse Effect by Lindsey Mohan and Jenny D
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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. -
Cryosphere: a Kingdom of Anomalies and Diversity
Atmos. Chem. Phys., 18, 6535–6542, 2018 https://doi.org/10.5194/acp-18-6535-2018 © Author(s) 2018. This work is distributed under the Creative Commons Attribution 4.0 License. Cryosphere: a kingdom of anomalies and diversity Vladimir Melnikov1,2,3, Viktor Gennadinik1, Markku Kulmala1,4, Hanna K. Lappalainen1,4,5, Tuukka Petäjä1,4, and Sergej Zilitinkevich1,4,5,6,7,8 1Institute of Cryology, Tyumen State University, Tyumen, Russia 2Industrial University of Tyumen, Tyumen, Russia 3Earth Cryosphere Institute, Tyumen Scientific Center SB RAS, Tyumen, Russia 4Institute for Atmospheric and Earth System Research (INAR), Physics, Faculty of Science, University of Helsinki, Helsinki, Finland 5Finnish Meteorological Institute, Helsinki, Finland 6Faculty of Radio-Physics, University of Nizhny Novgorod, Nizhny Novgorod, Russia 7Faculty of Geography, University of Moscow, Moscow, Russia 8Institute of Geography, Russian Academy of Sciences, Moscow, Russia Correspondence: Hanna K. Lappalainen (hanna.k.lappalainen@helsinki.fi) Received: 17 November 2017 – Discussion started: 12 January 2018 Revised: 20 March 2018 – Accepted: 26 March 2018 – Published: 8 May 2018 Abstract. The cryosphere of the Earth overlaps with the 1 Introduction atmosphere, hydrosphere and lithosphere over vast areas ◦ with temperatures below 0 C and pronounced H2O phase changes. In spite of its strong variability in space and time, Nowadays the Earth system is facing the so-called “Grand the cryosphere plays the role of a global thermostat, keeping Challenges”. The rapidly growing population needs fresh air the thermal regime on the Earth within rather narrow limits, and water, more food and more energy. Thus humankind suf- affording continuation of the conditions needed for the main- fers from climate change, deterioration of the air, water and tenance of life. -
Statement Climate Change Greenhouse Effect
Western Region Technical Attachment No. 91-07 February 19, 1991 STATEMENT ON CLIMATE. CHANGE AND THE GREENHOUSE EFFECT STATEMENT ON CLIMATE CHANGE AND THE GREENHOUSE EFFECT by REGIONAL CLIMATE CENTERS High Plains Climate Center· University of Nebraska Midwestern Climate Center • Illinois State Water Survey Northeast Regional Climate Center - Cornell University Southern Regional Climate Center • Louisiana State University Southeastern Regional Climate Center • South Carolina Water Commission "'estern Regional Climate Center - Desert Research Institute March 1990 STATEMENT ON CLIMATE CHANGE AND THE GREENHOUSE EFFECT by Regional Climate Centers The Issue Many scientists have issued claims of future global climate changes towards warmer conditions as a result of the ever increasing global release of Carbon Dioxide (C02) and other trace gases from the burning of fossil fuels and from deforestation. The nation experienced an unexpected and severe drought in 1988 which continued through 1989 in parts of the western United States.Is there a connection between these two atmospheric issues? Was the highly unusual 1988-89 drought the first symptom of the climate change atmospheric scientists had been talking about for the past 10 years? Most of the scientific community say "no." The 1988 drought was probably not tied to the ever increasing atmospheric burden of our waste gases. The 1988 drought fits within the historical range of climatic extremes over the past 100 years. Regardless, global climate. change due to the greenhouse effect is an issue of growing national and international concern. It joins the acid rain and ozone layer issues as major atmospheric problems arising primarily from human activities. The term "Greenhouse Effect" derives from the loose analogy between the behavior of the absorbing trace gases in the atmosphere and the window glass in a greenhouse. -
Agriculture, Forestry, and Other Human Activities
4 Agriculture, Forestry, and Other Human Activities CO-CHAIRS D. Kupfer (Germany, Fed. Rep.) R. Karimanzira (Zimbabwe) CONTENTS AGRICULTURE, FORESTRY, AND OTHER HUMAN ACTIVITIES EXECUTIVE SUMMARY 77 4.1 INTRODUCTION 85 4.2 FOREST RESPONSE STRATEGIES 87 4.2.1 Special Issues on Boreal Forests 90 4.2.1.1 Introduction 90 4.2.1.2 Carbon Sinks of the Boreal Region 90 4.2.1.3 Consequences of Climate Change on Emissions 90 4.2.1.4 Possibilities to Refix Carbon Dioxide: A Case Study 91 4.2.1.5 Measures and Policy Options 91 4.2.1.5.1 Forest Protection 92 4.2.1.5.2 Forest Management 92 4.2.1.5.3 End Uses and Biomass Conversion 92 4.2.2 Special Issues on Temperate Forests 92 4.2.2.1 Greenhouse Gas Emissions from Temperate Forests 92 4.2.2.2 Global Warming: Impacts and Effects on Temperate Forests 93 4.2.2.3 Costs of Forestry Countermeasures 93 4.2.2.4 Constraints on Forestry Measures 94 4.2.3 Special Issues on Tropical Forests 94 4.2.3.1 Introduction to Tropical Deforestation and Climatic Concerns 94 4.2.3.2 Forest Carbon Pools and Forest Cover Statistics 94 4.2.3.3 Estimates of Current Rates of Forest Loss 94 4.2.3.4 Patterns and Causes of Deforestation 95 4.2.3.5 Estimates of Current Emissions from Forest Land Clearing 97 4.2.3.6 Estimates of Future Forest Loss and Emissions 98 4.2.3.7 Strategies to Reduce Emissions: Types of Response Options 99 4.2.3.8 Policy Options 103 75 76 IPCC RESPONSE STRATEGIES WORKING GROUP REPORTS 4.3 AGRICULTURE RESPONSE STRATEGIES 105 4.3.1 Summary of Agricultural Emissions of Greenhouse Gases 105 4.3.2 Measures and -
Study of the Geoeffectiveness of Coronal Mass Ejections
Study of the geoeffectiveness of coronal mass ejections Katarzyna Bronarska Jagiellonian University Faculty of Physics, Astronomy and Applied Computer Science Astronomical Observatory PhD thesis written under the supervision of dr hab. Grzegorz Michaªek September 2018 Acknowledgements Pragn¦ wyrazi¢ gª¦bok¡ wdzi¦czno±¢ moim rodzicom oraz m¦»owi, bez których »aden z moich sukcesów nie byªby mo»liwy. Chc¦ równie» podzi¦kowa¢ mojemu promotorowi, doktorowi hab. Grzogorzowi Michaªkowi, za ci¡gªe wsparcie i nieocenion¡ pomoc. I would like to express my deepest gratitude to my parents and my husband, without whom none of my successes would be possible. I would like to thank my superior, dr hab. Grzegorz Michaªek for continuous support and invaluable help. Abstract This dissertation is an attempt to investigate geoeectiveness of CMEs. The study was focused on two important aspects regarding the prediction of space weather. Firstly, it was presented relationship between energetic phenomena on the Sun and CMEs producing solar energetic particles. Scientic considerations demonstrated that very narrow CMEs can generate low energy particles (energies below 1 MeV) in the Earth's vicinity without other activity on the Sun. It was also shown that SEP events associated with active regions from eastern longitudes have to be complex to produce SEP events at Earth. On the other hand, SEP particles originating from mid-longitudes (30<latitude<70) on the west side of solar disk can be also associated with the least complex active regions. Secondly, two phenomena aecting CMEs detection in coronagraphs have been dened. During the study the detection eciency of LASCO coronagraphs was evaluated. It was shown that the detection eciency of the LASCO coronagraphs with typical data availability is sucient to record all potentially geoeective CMEs. -
Continuous Magnetic Reconnection at the Earth's Magnetopause
Why Study Magnetic Reconnection? Fundamental Process • Sun: Solar flares, Flare loops, CMEs • Interplanetary Space • Planetary Magnetosphere: solar wind plasma entry, causes Aurora Ultimate goal of the project – observe magnetic reconnection by satellite in situ through predictions of reconnection site in model Regions of the Geosphere • Solar wind: made up of plasma particles (pressure causes field distortion) • Bow shock: shock wave preceding Earth’s magnetic field • Magnetosheath: region of shocked plasma (higher density) • Magnetopause: Boundary between solar wind/geosphere • Cusp region: region with open field lines and direct solar wind access to upper atmosphere Magnetic Reconnection • Two antiparallel magnetized plasmas, separated by current sheet • Occurs in a very small area (Diffusion Region) At the Earth’s Magnetopause: • IMF reconnects with Earth’s magnetic field across the magnetopause • Southward IMF reconnects near equator • Forms open field lines, which convect backwards to cusp Instrument Overview Polar –TIMAS Wind - SWE instrument • Outside • Measures 3D velocity geospheric distributions influence • Focused on H+ data • Provides solar wind data Magnetic Reconnection Observed in the Cusp Magnetopause Fast Particle Magnetospheric Slow Particle • Color spectrogram Cusp • Measures energy and intensity (flux) of protons from solar wind Solar Wind in cusp with respect to time and latitude • Latitude changes due to convection Color spectrogram produced by IDL program written by mentor Methodology to Determine Where Reconnection -
Causes of Sea Level Rise
FACT SHEET Causes of Sea OUR COASTAL COMMUNITIES AT RISK Level Rise What the Science Tells Us HIGHLIGHTS From the rocky shoreline of Maine to the busy trading port of New Orleans, from Roughly a third of the nation’s population historic Golden Gate Park in San Francisco to the golden sands of Miami Beach, lives in coastal counties. Several million our coasts are an integral part of American life. Where the sea meets land sit some of our most densely populated cities, most popular tourist destinations, bountiful of those live at elevations that could be fisheries, unique natural landscapes, strategic military bases, financial centers, and flooded by rising seas this century, scientific beaches and boardwalks where memories are created. Yet many of these iconic projections show. These cities and towns— places face a growing risk from sea level rise. home to tourist destinations, fisheries, Global sea level is rising—and at an accelerating rate—largely in response to natural landscapes, military bases, financial global warming. The global average rise has been about eight inches since the centers, and beaches and boardwalks— Industrial Revolution. However, many U.S. cities have seen much higher increases in sea level (NOAA 2012a; NOAA 2012b). Portions of the East and Gulf coasts face a growing risk from sea level rise. have faced some of the world’s fastest rates of sea level rise (NOAA 2012b). These trends have contributed to loss of life, billions of dollars in damage to coastal The choices we make today are critical property and infrastructure, massive taxpayer funding for recovery and rebuild- to protecting coastal communities. -
Extraformational Sediment Recycling on Mars Kenneth S
Research Paper GEOSPHERE Extraformational sediment recycling on Mars Kenneth S. Edgett1, Steven G. Banham2, Kristen A. Bennett3, Lauren A. Edgar3, Christopher S. Edwards4, Alberto G. Fairén5,6, Christopher M. Fedo7, Deirdra M. Fey1, James B. Garvin8, John P. Grotzinger9, Sanjeev Gupta2, Marie J. Henderson10, Christopher H. House11, Nicolas Mangold12, GEOSPHERE, v. 16, no. 6 Scott M. McLennan13, Horton E. Newsom14, Scott K. Rowland15, Kirsten L. Siebach16, Lucy Thompson17, Scott J. VanBommel18, Roger C. Wiens19, 20 20 https://doi.org/10.1130/GES02244.1 Rebecca M.E. Williams , and R. Aileen Yingst 1Malin Space Science Systems, P.O. Box 910148, San Diego, California 92191-0148, USA 2Department of Earth Science and Engineering, Imperial College London, South Kensington, London SW7 2AZ, UK 19 figures; 1 set of supplemental files 3U.S. Geological Survey, Astrogeology Science Center, 2255 N. Gemini Drive, Flagstaff, Arizona 86001, USA 4Department of Astronomy and Planetary Science, Northern Arizona University, P.O. Box 6010, Flagstaff, Arizona 86011, USA CORRESPONDENCE: [email protected] 5Department of Planetology and Habitability, Centro de Astrobiología (CSIC-INTA), M-108, km 4, 28850 Madrid, Spain 6Department of Astronomy, Cornell University, Ithaca, New York 14853, USA 7 CITATION: Edgett, K.S., Banham, S.G., Bennett, K.A., Department of Earth and Planetary Sciences, The University of Tennessee, 1621 Cumberland Avenue, 602 Strong Hall, Knoxville, Tennessee 37996-1410, USA 8 Edgar, L.A., Edwards, C.S., Fairén, A.G., Fedo, C.M., National Aeronautics -
Global Warming Impacts on Severe Drought Characteristics in Asia Monsoon Region
water Article Global Warming Impacts on Severe Drought Characteristics in Asia Monsoon Region Jeong-Bae Kim , Jae-Min So and Deg-Hyo Bae * Department of Civil & Environmental Engineering, Sejong University, 209 Neungdong-ro, Gwangjin-Gu, Seoul 05006, Korea; [email protected] (J.-B.K.); [email protected] (J.-M.S.) * Correspondence: [email protected]; Tel.: +82-2-3408-3814 Received: 2 April 2020; Accepted: 7 May 2020; Published: 12 May 2020 Abstract: Climate change influences the changes in drought features. This study assesses the changes in severe drought characteristics over the Asian monsoon region responding to 1.5 and 2.0 ◦C of global average temperature increases above preindustrial levels. Based on the selected 5 global climate models, the drought characteristics are analyzed according to different regional climate zones using the standardized precipitation index. Under global warming, the severity and frequency of severe drought (i.e., SPI < 1.5) are modulated by the changes in seasonal and regional precipitation − features regardless of the region. Due to the different regional change trends, global warming is likely to aggravate (or alleviate) severe drought in warm (or dry/cold) climate zones. For seasonal analysis, the ranges of changes in drought severity (and frequency) are 11.5%~6.1% (and 57.1%~23.2%) − − under 1.5 and 2.0 ◦C of warming compared to reference condition. The significant decreases in drought frequency are indicated in all climate zones due to the increasing precipitation tendency. In general, drought features under global warming closely tend to be affected by the changes in the amount of precipitation as well as the changes in dry spell length. -
Energy Budget: Earth’S Most Important and Least Appreciated Planetary Attribute by Lin Chambers (NASA Langley Research Center) and Katie Bethea (SSAI)
© 2013, Astronomical Society of the Pacific No. 84 • Summer 2013 www.astrosociety.org/uitc 390 Ashton Avenue, San Francisco, CA 94112 Energy Budget: Earth’s most important and least appreciated planetary attribute by Lin Chambers (NASA Langley Research Center) and Katie Bethea (SSAI) asking in the Sun on a warm day, it’s easy for know some species of animals can see ultraviolet people to realize that most of the energy on light and portions of the infrared spectrum. NASA Earth comes from the Sun; students know satellites use instruments that can “see” different Bthis as early as elementary school. We all know parts of the electromagnetic spectrum to observe plants use this energy from the Sun for photosyn- various processes in the Earth system, including the thesis, and animals eat plants, creating a giant food energy budget. web. Most people also understand the Sun’s energy The Sun is a very hot ball of plasma emitting large drives evaporation and thus powers the water cycle. amounts of energy. By the time it reaches Earth, this But many people do not realize the Sun’s energy it- energy amounts to about 340 Watts for every square self is also part of an important interconnected sys- meter of Earth on average. That’s almost 6 60-Watt tem: Earth’s energy budget or balance. This energy light bulbs for every square meter of Earth! With budget determines conditions on our planet — just all of that energy shining down on the Earth, how like the energy budget of other planets determines does our planet maintain a comfortable balance that conditions there. -
Directed Reading Packet
Directed Reading Packet Geosphere Unit Name:_______________________________ Teacher: _________________ Period: ____ Section 1.2: A View of Earth This section explains the physical structure of Earth. Reading Strategy Predicting Before you read, predict the meaning of the vocabulary terms. After you read, revise your definition if your prediction was incorrect. For more information on this Reading Strategy, see the Reading and Study Skills in the Skills and Reference Handbook at the end of your textbook. Vocabulary Term Before You Read After You Read hydrosphere a. b. atmosphere c. d. geosphere e. f. biosphere g. h. core i. j. mantle k. l. crust m. n. Earth’s Major Spheres 1. Earth can be thought of as consisting of four major spheres: the , , , and . Match each term to its description. Term Description 2. hydrosphere a. all life-forms on Earth 3. atmosphere b. composed of the core, mantle, and crust 4. geosphere c. dense, heavy inner sphere of Earth 5. biosphere d. thin outside layer of Earth’s surface 6. core e. the water portion of Earth 7. mantle f. the gaseous envelope around Earth 8. crust g. located between the crust and core of Earth 9. What does each letter in the diagram below represent? A. B. C. D. E. F. G. H. I. J. Plate Tectonics 10. Is the following sentence true or false? Forces such as weathering and erosion that work to wear away high points and flatten out Earth’s surface are called constructive forces. 11. Circle the letter of each type of constructive force. a. gravity b. -
Session B-1: Model Building in Planetary Science and the NGSS
Model Building in Planetary Science and the NGSS Dr. Eric Hawker IMSA Science Faculty March 4th , 2016 Planetary Science • Planets are complicated dynamic systems. • There are many planetary attributes that interact with each other. • The dynamic changes that planets go through are driven by energy. Model Building • Usually these are not physical models! • A set of concepts that describe a system. • NGSS Science and Engineering Practices: Developing and Using Models: Modeling in 9–12 builds on K–8 experiences and progresses to using, synthesizing, and developing models to predict and show relationships among variables between systems and their components in the natural and designed world(s). • Develop a model based on evidence to illustrate the relationships between systems or between components of a system. (HS-ESS2-1), (HS-ESS2-3),(HS-ESS2-6) • Use a model to provide mechanistic accounts of phenomena. (HS- ESS2-4) Model Building • HS-ESS2-1. Develop a model to illustrate how Earth’s internal and surface processes operate at different spatial and temporal scales to form continental and ocean-floor features. • HS-ESS2-3. Develop a model based on evidence of Earth’s interior to describe the cycling of matter by thermal convection. • HS-ESS2-6. Develop a quantitative model to describe the cycling of carbon among the hydrosphere, atmosphere, geosphere, and biosphere. Heat from Planetary Formation • The initial solar nebula of dust and gas that the Solar System formed from had a lot of gravitational potential energy. • This gravitational potential energy was turned into thermal energy (heat) during planetary formation. Atacama Large Millimeter Array image of HL Tauri Radioactivity • When the planets formed, radioactive isotopes such as uranium, thorium, and potassium were trapped deep underground.