Earth As a System / Chapter 2: the Nature of Science
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Preprint Arxiv:1806.10939, 2018
Solid Earth Discuss., https://doi.org/10.5194/se-2019-4 Manuscript under review for journal Solid Earth Discussion started: 15 January 2019 c Author(s) 2019. CC BY 4.0 License. Bayesian geological and geophysical data fusion for the construction and uncertainty quantification of 3D geological models Hugo K. H. Olierook1, Richard Scalzo2, David Kohn3, Rohitash Chandra2,4, Ehsan Farahbakhsh2,4, Gregory Houseman3, Chris Clark1, Steven M. Reddy1, R. Dietmar Müller4 5 1School of Earth and Planetary Sciences, Curtin University, GPO Box U1987, Perth, WA 6845, Australia 2Centre for Translational Data Science, University of Sydney, NSW 2006 Sydney, Australia 3Sydney Informatics Hub, University of Sydney, NSW 2006 Sydney, Australia 4EarthByte Group, School of Geosciences, University of Sydney, NSW 2006 Sydney, Australia Correspondence to: Hugo K. H. Olierook ([email protected]) 10 Abstract. Traditional approaches to develop 3D geological models employ a mix of quantitative and qualitative scientific techniques, which do not fully provide quantification of uncertainty in the constructed models and fail to optimally weight geological field observations against constraints from geophysical data. Here, we demonstrate a Bayesian methodology to fuse geological field observations with aeromagnetic and gravity data to build robust 3D models in a 13.5 × 13.5 km region of the Gascoyne Province, Western Australia. Our approach is validated by comparing model results to independently-constrained 15 geological maps and cross-sections produced by the Geological Survey of Western Australia. By fusing geological field data with magnetics and gravity surveys, we show that at 89% of the modelled region has >95% certainty. The boundaries between geological units are characterized by narrow regions with <95% certainty, which are typically 400–1000 m wide at the Earth’s surface and 500–2000 m wide at depth. -
The History of Planet Earth
SECOND EDITION Earth’s Evolving The History of Systems Planet Earth Ronald Martin, Ph.D. University of Delaware Newark, Delaware © Jones & Bartlett Learning, LLC, an Ascend Learning Company. NOT FOR SALE OR DISTRIBUTION 9781284457162_FMxx_00i_xxii.indd 1 07/11/16 1:46 pm World Headquarters Jones & Bartlett Learning 5 Wall Street Burlington, MA 01803 978-443-5000 [email protected] www.jblearning.com Jones & Bartlett Learning books and products are available through most bookstores and online booksellers. To contact Jones & Bartlett Learning directly, call 800-832-0034, fax 978-443-8000, or visit our website, www.jblearning.com. Substantial discounts on bulk quantities of Jones & Bartlett Learning publications are available to corporations, professional associations, and other qualified organizations. For details and specific discount information, contact the special sales department at Jones & Bartlett Learning via the above contact information or send an email to [email protected]. Copyright © 2018 by Jones & Bartlett Learning, LLC, an Ascend Learning Company All rights reserved. No part of the material protected by this copyright may be reproduced or utilized in any form, electronic or mechanical, including photocopying, recording, or by any information storage and retrieval system, without written permission from the copyright owner. The content, statements, views, and opinions herein are the sole expression of the respective authors and not that of Jones & Bartlett Learning, LLC. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not constitute or imply its endorsement or recommendation by Jones & Bartlett Learning, LLC, and such reference shall not be used for advertis- ing or product endorsement purposes. -
Nature Based Solutions FEMA
PROMOTING NATURE-BASED HAZARD MITIGATION THROUGH FEMA MITIGATION GRANTS ABBREVIATIONS ADCIRC – Advanced Circulation Model HGM Approach – Hydrogeomorphic Approach BCA – Benefit-Cost Analysis HMA – Hazard Mitigation Assistance BCR – Benefit-Cost Ratio HMGP – Hazard Mitigation Grant Program BRIC – Building Resilient Infrastructure and MSCP – Multiple Species Conservation Program Communities NBS – Nature-Based Solution C&CB – Capability- and Capacity-Building NFIP – National Flood Insurance Program CDBG-DR – Community Development Block Grant- Disaster Recovery NFWF – National Fish and Wildlife Foundation CDBG-MIT – Community Development Block NOAA – National Oceanic and Atmospheric Grant-Mitigation Administration D.C. – District of Columbia NOFO – Notice of Funding Opportunity DEM – Department of Emergency Management NPV – Net Present Value DOI – Department of the Interior SCC – State Coastal Conservancy EDYS – Ecological Dynamics Simulation SDG&E – San Diego Gas & Electric EMA – Emergency Management Agency SFHA – Special Flood Hazard Area EPA SWMM – Environmental Protection Agency SHMO – State Hazard Mitigation Officer Storm Water Management Model SLAMM – Sea Level Affecting Marshes Model FEMA – Federal Emergency Management Agency SRH-2D – Sedimentation and River Hydraulics – FIRM – Flood Insurance Rate Map Two-Dimension FMA – Flood Mitigation Assistance STWAVE – Steady-State Spectral Wave Model FMAG – Fire Management Assistance Grant TNC – The Nature Conservancy HAZUS – Hazards US USACE – U.S. Army Corps of Engineers HEC-HMS – Hydrologic -
Amplify Science Earth's Changing Climate
Lawrence Hall of Science has new instructional materials that address the Next Generation Science Standards! Check out these Middle School Units… As just one example, compare Middle School units from three different Hall programs. See for yourself how each program goes about addressing the Middle School NGSS Standards related to Human Impacts and Climate Change, and choose the approach that best meets the needs of your school district. MS NGSS Performance Expectations: Human Impacts and Climate Change • MS-ESS3-2. Analyze and interpret data on natural hazards to forecast future catastrophic events and inform the development of technologies to mitigate their effects. • MS-ESS3-3. Apply scientific principles to design a method for monitoring and minimizing a human impact on the Environment. • MS-ESS3-4. Construct an argument supported by evidence for how increases in human population and per-capita consumption of natural resources impact Earth’s systems. • MS-ESS3-5. Ask questions to clarify evidence of the factors that have caused the rise in global temperatures over the past century. Sample Units from Three Different Hall Programs • Amplify Science—Earth’s Changing Climate: Vanishing Ice Earth’s Changing Climate Engineering Internship • FOSS—Weather and Water • Ocean Sciences Sequence—The Ocean-Atmosphere Connection and Climate Change ©The Regents of the University of California ©The Regents of the University of California Description of two Middle School units from Amplify Science Earth’s Changing Climate: Vanishing Ice and Earth’s Changing Climate Engineering Internship Grade 6-8 Units — requiring at least 19 and 10 45-minute class sessions respectively (two of 27 Middle School Amplify Science units) The Problem: Why is the ice on Earth’s surface melting? Students’ Role: In the role of student climatologists, students investigate what is causing ice on Earth’s surface to melt in order to help the fictional World Climate Institute educate the public about the processes involved. -
Planets of the Solar System
Chapter Planets of the 27 Solar System Chapter OutlineOutline 1 ● Formation of the Solar System The Nebular Hypothesis Formation of the Planets Formation of Solid Earth Formation of Earth’s Atmosphere Formation of Earth’s Oceans 2 ● Models of the Solar System Early Models Kepler’s Laws Newton’s Explanation of Kepler’s Laws 3 ● The Inner Planets Mercury Venus Earth Mars 4 ● The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects Beyond Neptune Why It Matters Exoplanets UnderstandingU d t di theth formationf ti and the characteristics of our solar system and its planets can help scientists plan missions to study planets and solar systems around other stars in the universe. 746 Chapter 27 hhq10sena_psscho.inddq10sena_psscho.indd 774646 PDF 88/15/08/15/08 88:43:46:43:46 AAMM Inquiry Lab Planetary Distances 20 min Turn to Appendix E and find the table entitled Question to Get You Started “Solar System Data.” Use the data from the How would the distance of a planet from the sun “semimajor axis” row of planetary distances to affect the time it takes for the planet to complete devise an appropriate scale to model the distances one orbit? between planets. Then find an indoor or outdoor space that will accommodate the farthest distance. Mark some index cards with the name of each planet, use a measuring tape to measure the distances according to your scale, and place each index card at its correct location. 747 hhq10sena_psscho.inddq10sena_psscho.indd 774747 22/26/09/26/09 111:42:301:42:30 AAMM These reading tools will help you learn the material in this chapter. -
The Solar System
5 The Solar System R. Lynne Jones, Steven R. Chesley, Paul A. Abell, Michael E. Brown, Josef Durech,ˇ Yanga R. Fern´andez,Alan W. Harris, Matt J. Holman, Zeljkoˇ Ivezi´c,R. Jedicke, Mikko Kaasalainen, Nathan A. Kaib, Zoran Kneˇzevi´c,Andrea Milani, Alex Parker, Stephen T. Ridgway, David E. Trilling, Bojan Vrˇsnak LSST will provide huge advances in our knowledge of millions of astronomical objects “close to home’”– the small bodies in our Solar System. Previous studies of these small bodies have led to dramatic changes in our understanding of the process of planet formation and evolution, and the relationship between our Solar System and other systems. Beyond providing asteroid targets for space missions or igniting popular interest in observing a new comet or learning about a new distant icy dwarf planet, these small bodies also serve as large populations of “test particles,” recording the dynamical history of the giant planets, revealing the nature of the Solar System impactor population over time, and illustrating the size distributions of planetesimals, which were the building blocks of planets. In this chapter, a brief introduction to the different populations of small bodies in the Solar System (§ 5.1) is followed by a summary of the number of objects of each population that LSST is expected to find (§ 5.2). Some of the Solar System science that LSST will address is presented through the rest of the chapter, starting with the insights into planetary formation and evolution gained through the small body population orbital distributions (§ 5.3). The effects of collisional evolution in the Main Belt and Kuiper Belt are discussed in the next two sections, along with the implications for the determination of the size distribution in the Main Belt (§ 5.4) and possibilities for identifying wide binaries and understanding the environment in the early outer Solar System in § 5.5. -
Geodynamics If the Entire Solid Earth Is Viewed As a Single Dynamic
http://www.paper.edu.cn Geodynamic Processes and Our Living Environment YANG Wencai, P. Robinson, FU Rongshan and WANG Ying Geological Publishing House: 2001 Geophysical System Yang Wencai, Institute of Geology, CAGS, China Key words: Geophysics, geodynamics, kinetics of the Earth, tectonics, energies of the Earth, driving forces, applied geophysics, sustainable development. Contents: I. About geophysical system II. Kinetics of the Earth III. About plate tectonics and plume tectonics IV. The contents in the topic V. Energies for the dynamic Earth VI. Driving Forces of Plate Tectonics VII. Geophysics and sustainable development of the society I. About geophysical system Rapid advance of sciences during the second half of the twentieth century has enabled man to make a successful star in the exploration of planetary space. The deep interior of the Earth, however, remains as inaccessible as ever. This is the realm of solid-Earth geophysics, which still mainly depends on observations made at or near the Earth's surface. Despite this limitation, a major revolution in knowledge of the Earth's interior has taken place over the last forty years. This has led to a new understanding of the processes which occur within the Earth that produce surface conditions outstandingly different from those of the other inner planets and the moon. How has this come about? It is mainly the results of the introduction of new experimental and computational techniques into geophysics. Geophysics as a major branch of the geosciences has been discussed in Topic 6.16.1. Theoretically and traditionally the geophysical system correlates to physical system, but specified st study the solid Earth, containing sub-branches such as gravitation and Earth-motion correlated with 转载 1 中国科技论文在线 http://www.paper.edu.cn mechanics, geothermics correlated with heat and thermics, seismology with acoustics and wave theory, geoelectricity and geomagnetism. -
Earth Science SCIH 041 055 Credits: 0.5 Units / 5 Hours / NCAA
UNIVERSITY OF NEBRASKA HIGH SCHOOL Earth Science SCIH 041 055 Credits: 0.5 units / 5 hours / NCAA Course Description Have you ever wondered where marble comes from? or how deep the ocean is? or why it rains more in areas near the Equator than in other places? In this course students will study a variety of topics designed to give them a better understanding of the planet on which we live. They will study the composition of Earth including minerals and different rock types, weathering and erosion processes, mass movements, and surface and groundwater. They will also explore Earth's atmosphere and oceans, including storms, climate and ocean movements, plate tectonics, volcanism, earthquakes, mountain building, and geologic time. This course concludes with an in-depth look at the connections between our Earth's vast resources and the human population's dependence and impact on them. Graded Assessments: 5 Unit Evaluations; 2 Projects; 2 Proctored Progress Tests, 5 Teacher Connect Activities Course Objectives When you have completed the materials in this course, you should be able to: 1. Describe how Earth materials move through geochemical cycles (carbon, nitrogen, oxygen) resulting in chemical and physical changes in matter. 2. Understand the relationships among Earth’s structure, systems, and processes. 3. Describe how heat convection in the mantle propels the plates comprising Earth’s surface across the face of the globe (plate tectonics). 4. Evaluate the impact of human activity and natural causes on Earth’s resources (groundwater, rivers, land, fossil fuels). 5. Describe the relationships among the sources of energy and their effects on Earth’s systems. -
Glossary of Terms
Glossary of Terms This glossary includes common words and phrases that the Biomimicry Institute often uses when talking about and teaching biomimicry. Most are true to definition, and some have a variation that is specific to their application in biomimicry. Term Definition A Abiotic Not associated with or derived from living organisms. Abiotic factors in an environment include sunlight, temperature, wind patterns, and precipitation, for example. Opposite of "biotic." Adaptation A feature of an organism that results from natural selection and by which the organism becomes better fitted to survive and reproduce in its environment. Analogous Similar in function and/or appearance but not in origin or development. B Biodiversity The variety of life and its processes; includes the variety of living organisms, the genetic differences among them, and the communities and ecosystems in which they occur. Biological Of or relating to biology or living organisms. Biologize [a question] To take a human need or function and rephrase it so that an answer may be found in biology, e.g., "How can I make the fabric red?" becomes, "How does nature create color?" Biomimicry The conscious emulation of life’s genius. Learning from and then emulating biological forms, processes, and ecosystems to create more sustainable designs. Biomimicry Taxonomy A function-based organization scheme cataloging how organisms meet different challenges. Information on AskNature.org is organized by this taxonomy. Biomorphic Sometimes confused with biomimicry, biomorphic describes anything resembling or suggesting the forms of living organisms. Biophilic / Biophilia Sometimes confused with biomimicry, biophilia is a term popularized by E.O. Wilson to describe the extent to which humans need connection with nature and other forms of life. -
Chapter 2 the Solid Materials of the Earth's Surface
CHAPTER 2 THE SOLID MATERIALS OF THE EARTH’S SURFACE 1. INTRODUCTION 1.1 To a great extent in this course, we will be dealing with processes that act on the solid materials at and near the Earth’s surface. This chapter might better be called “the ground beneath your feet”. This is the place to deal with the nature of the Earth’s surface materials, which in later sections of the chapter I will be calling regolith, sediment, and soil. 1.2 I purposely did not specify any previous knowledge of geology as a prerequisite for this course, so it is important, here in the first part of this chapter, for me to provide you with some background on Earth materials. 1.3 We will be dealing almost exclusively with the Earth’s continental surfaces. There are profound geological differences between the continents and the ocean basins, in terms of origin, age, history, and composition. Here I’ll present, very briefly, some basic things about geology. (For more depth on such matters you would need to take a course like “The Earth: What It Is, How It Works”, given in the Harvard Extension program in the fall semester of 2005– 2006 and likely to be offered again in the not-too-distant future.) 1.4 In a gross sense, the Earth is a layered body (Figure 2-1). To a first approximation, it consists of concentric shells: the core, the mantle, and the crust. Figure 2-1: Schematic cross section through the Earth. 73 The core: The core consists mostly of iron, alloyed with a small percentage of certain other chemical elements. -
New Research Opportunities in the Earth Sciences
New Research Opportunities in the Earth Sciences A national strategy to sustain basic research and training across all areas of the Earth sciences would help inform the response to many of the major challenges that will face the planet in coming years. Issues including fossil fuel and water resources, earthquake and tsunami hazards, and profound environmental changes due to shifts in the climate system could all be informed by new research in the Earth sciences. The National Science Foundation’s Division of Earth Sciences, as the only federal agency that maintains significant funding of both exploratory and problem-driven research in the Earth sciences, is central to these efforts, and coordinated research priorities are needed to fully capitalize on the contributions that the Earth sciences can make. ith Earth’s planet. However, it’s population important to note that this Wexpected to collaborative work builds reach 7 billion by the end on basic research in of 2011, and about 9.2 specific disciplines. Core billion by 2050, demand Earth science research for resources such as food, carried out by individual fuel, and water is investigators, or small increasing rapidly. At the groups of scientists, same time, humans are remains the most creative changing the landscape and effective way to and the temperature of the enhance the knowledge atmosphere is increasing. base upon which integra- Expanding basic research tive efforts can build. in the Earth sciences—the study of Earth’s solid Key Research surface, crust, mantle and Opportunities core, and the interactions Figure 1. Combining LiDAR data with geological Conceptual advances in observations helps determine how erosional processes between Earth and the basic Earth science theory respond to rock uplift at Dragon’s Back pressure ridge and technological improve- atmosphere, hydrosphere, along the San Andreas Fault. -
Chapter 11: Atmosphere
The Atmosphere and the Oceans ff the Na Pali coast in Hawaii, clouds stretch toward O the horizon. In this unit, you’ll learn how the atmo- sphere and the oceans interact to produce clouds and crashing waves. You’ll come away from your studies with a deeper understanding of the common characteristics shared by Earth’s oceans and its atmosphere. Unit Contents 11 Atmosphere14 Climate 12 Meteorology15 Physical Oceanography 13 The Nature 16 The Marine Environment of Storms Go to the National Geographic Expedition on page 880 to learn more about topics that are con- nected to this unit. 268 Kauai, Hawaii 269 1111 AAtmospheretmosphere What You’ll Learn • The composition, struc- ture, and properties that make up Earth’s atmos- phere. • How solar energy, which fuels weather and climate, is distrib- uted throughout the atmosphere. • How water continually moves between Earth’s surface and the atmo- sphere in the water cycle. Why It’s Important Understanding Earth’s atmosphere and its interactions with solar energy is the key to understanding weather and climate, which con- trol so many different aspects of our lives. To find out more about the atmosphere, visit the Earth Science Web Site at earthgeu.com 270 DDiscoveryiscovery LLabab Dew Formation Dew forms when moist air near 4. Repeat the experiment outside. the ground cools and the water vapor Record the temperature of the in the air changes into water droplets. water and the air outside. In this activity, you will model the Observe In your science journal, formation of dew. describe what happened to the out- 1.