Comparison of the Greenhouse Effect Between Earth and Venus Using Multiple Atmospheric Layer Models
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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. -
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 -
Atmospheric Pressure
Atmospheric pressure We all know that the atmosphere of Earth exerts a pressure on all of us. This pressure is the result of a column of air bearing down on us. However, in the seventeenth century, many scientists and philosophers believed that the air had no weight, which we already proved to be untrue in the lab (Remembered the fun you had sucking air out of the POM bottle?). Evangelista Torricelli, a student of Galileo’s, proved that air has weight using another experiment. He took a glass tube longer than 760 mm that is closed at one end and filled it completely with mercury. When he inverted the tube into a dish of mercury, some of the mercury flows out, but a column of mercury remained inside the tube. Torricelli argued that the mercury surface in the dish experiences the force of Earth’s atmosphere due to gravity, which held up the column of mercury. The force exerted by the atmosphere, which depends on the atmospheric pressure, equals the weight of mercury column in the tube. Therefore, the height of the mercury column can be used as a measure of atmospheric pressure. Although Torricelli’s explanation met with fierce opposition, it also had supporters. Blaise Pascal, for example, had one of Torricelli’s barometers carried to the top of a mountain and compared its reading there with the reading on a duplicate barometer at the base of the mountain. As the barometer was carried up, the height of the mercury column decreased, as expected, because the amount of air pressing down on the mercury in the dish decreased as the instrument was carried higher. -
Global Warming Climate Records
ATM S 111: Global Warming Climate Records Jennifer Fletcher Day 24: July 26 2010 Reading For today: “Keeping Track” (Climate Records) pp. 171-192 For tomorrow/Wednesday: “The Long View” (Paleoclimate) pp. 193-226. The Instrumental Record from NASA Global temperature since 1880 Ten warmest years: 2001-2009 and 1998 (biggest El Niño ever) Separation into Northern/ Southern Hemispheres N. Hem. has warmed more (1o C vs 0.8o C globally) S. Hem. has warmed more steadily though Cooling in the record from 1940-1975 essentially only in the N. Hem. record (this is likely due to aerosol cooling) Temperature estimates from other groups CRUTEM3 (RG calls this UEA) NCDC (RG calls this NOAA) GISS (RG calls this NASA) yet another group Surface air temperature over land Thermometer between 1.25-2 m (4-6.5 ft) above ground White colored to reflect away direct sunlight Slats to ensure fresh air circulation “Stevenson screen”: invented by Robert Louis Stevenson’s dad Thomas Yearly average Central England temperature record (since 1659) Temperatures over Land Only NASA separates their analysis into land station data only (not including ship measurements) Warming in the station data record is larger than in the full record (1.1o C as opposed to 0.8o C) Sea surface temperature measurements Standard bucket Canvas bucket Insulated bucket (~1891) (pre WWII) (now) “Bucket” temperature: older style subject to evaporative cooling Starting around WWII: many temperature measurements taken from condenser intake pipe instead of from buckets. Typically 0.5 C warmer -
Atmospheric Thermal and Dynamic Vertical Structures of Summer Hourly Precipitation in Jiulong of the Tibetan Plateau
atmosphere Article Atmospheric Thermal and Dynamic Vertical Structures of Summer Hourly Precipitation in Jiulong of the Tibetan Plateau Yonglan Tang 1, Guirong Xu 1,*, Rong Wan 1, Xiaofang Wang 1, Junchao Wang 1 and Ping Li 2 1 Hubei Key Laboratory for Heavy Rain Monitoring and Warning Research, Institute of Heavy Rain, China Meteorological Administration, Wuhan 430205, China; [email protected] (Y.T.); [email protected] (R.W.); [email protected] (X.W.); [email protected] (J.W.) 2 Heavy Rain and Drought-Flood Disasters in Plateau and Basin Key Laboratory of Sichuan Province, Institute of Plateau Meteorology, China Meteorological Administration, Chengdu 610072, China; [email protected] * Correspondence: [email protected]; Tel.: +86-27-8180-4913 Abstract: It is an important to study atmospheric thermal and dynamic vertical structures over the Tibetan Plateau (TP) and their impact on precipitation by using long-term observation at represen- tative stations. This study exhibits the observational facts of summer precipitation variation on subdiurnal scale and its atmospheric thermal and dynamic vertical structures over the TP with hourly precipitation and intensive soundings in Jiulong during 2013–2020. It is found that precipitation amount and frequency are low in the daytime and high in the nighttime, and hourly precipitation greater than 1 mm mostly occurs at nighttime. Weak precipitation during the daytime may be caused by air advection, and strong precipitation at nighttime may be closely related with air convection. Both humidity and wind speed profiles show obvious fluctuation when precipitation occurs, and the greater the precipitation intensity, the larger the fluctuation. Moreover, the fluctuation of wind speed Citation: Tang, Y.; Xu, G.; Wan, R.; Wang, X.; Wang, J.; Li, P. -
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. -
Characterising the Three-Dimensional Ozone Distribution of a Tidally Locked Earth-Like Planet
Proedrou and Hocke Earth, Planets and Space (2016) 68:96 DOI 10.1186/s40623-016-0461-x FULL PAPER Open Access Characterising the three‑dimensional ozone distribution of a tidally locked Earth‑like planet Elisavet Proedrou1,2*† and Klemens Hocke1,2,3† Abstract We simulate the 3D ozone distribution of a tidally locked Earth-like exoplanet using the high-resolution, 3D chemistry- climate model CESM1(WACCM) and study how the ozone layer of a tidally locked Earth (TLE) (�TLE = 1/365 days) differs from that of our present-day Earth (PDE) �( PDE = 1/1 day). The middle atmosphere reaches a steady state asymptotically within the first 80 days of the simulation. An upwelling, centred on the subsolar point, is present on the day side while a downwelling, centred on the antisolar point, is present on the night side. In the mesosphere, we find similar global ozone distributions for the TLE and the PDE, with decreased ozone on the day side and enhanced ozone on the night side. In the lower mesosphere, a jet stream transitions into a large-scale vortex around a low-pressure system, located at low latitudes of the TLE night side. In the middle stratosphere, the concentration of odd oxygen is approximately equal to that of the ozone [(Ox) ≈ (O3)]. At these altitudes, the lifetime of odd oxygen is ∼16 h and the transport processes significantly contribute to the global distribution of stratospheric ozone. Compared to the PDE, where the strong Coriolis force acts as a mixing barrier between low and high latitudes, the transport processes of the TLE are governed by jet streams variable in the zonal and meridional directions. -
CO2 Mitigation Through Biofuels in the Transport Sector
ifeu - Institute for Energy and Environmental Research Heidelberg Germany CO2 Mitigation through Biofuels in the Transport Sector Status and Perspectives Main Report supported by FVV, Frankfurt and UFOP, Berlin CO2 Mitigation through Biofuels in the Transport Sector Status and Perspectives Main Report Heidelberg, Germany, August 2004 Authors Dr. Markus Quirin Dipl.-Phys. Ing. Sven O. Gärtner Dr. Martin Pehnt Dr. Guido A. Reinhardt This report was executed by IFEU – Institut für Energie- und Umweltforschung Heidelberg GmbH (Institute for Energy and Environmental Research Heidelberg) Wilckensstrasse 3, 69120 Heidelberg, Germany Tel: +49-6221-4767-0, Fax -19 E-Mail: [email protected] www.ifeu.de Funding organisations F V V – Research Association for Combustion Engines F V V e. V. im VDMA, Lyoner Straße 18, 60528 Frankfurt am Main, Germany www.fvv-net.de UFOP – Union for the Promotion of Oil and Protein Plants UFOP e. V., Reinhardtstraße 18, 10117 Berlin, Germany www.ufop.de FAT – German Association for Research on Automobile-Technique FAT e. V. im VDA, Westendstraße 61, 60325 Frankfurt am Main, Germany www.vda.de/de/vda/intern/organisation/abteilungen/fat.html More information on this project can be found on www.ifeu.de/co2mitigation.htm Acknowledgements We thank the Research Association for Combustion Engines (Forschungsvereinigung Verbrennungskraftmaschinen e. V., FVV) that called this study into existence. Thanks are also due to the Union for the Promotion of Oil and Protein Plants (Union zur Förderung von Oel- und Proteinpflanzen e. V., UFOP) and the German Association for Research on Automobile-Technique (Forschungsvereinigung Automobiltechnik e. V., FAT) that, together with FVV, financed this research. -
What Is Ozone Layer? a Layer in the Atmosphere of Earth That Protects Us from Harmful UV Rays from the Sun
International Day for Preservation of Ozone Layer 16 September 2020 Image Source: https://sfxstl.org/circleofcreation What is Ozone layer? A layer in the atmosphere of Earth that protects us from harmful UV rays from the Sun. It’s responsible for preserving life on the planet! What is happening? The ozone layer has begun to deplete because of harmful chemical substances and gases. This problem is not only contributing to global warming and climate change, but also allowing the dangerous radiation from the sun to affect human beings and ecosystems! Source: https://www.un.org/en/events/ozoneday/ What is causing its depletion? ● Human activities are the biggest cause of the ozone layer depletion ● When we burn coal, natural gas and other fuels for electricity, they release harmful gases such as carbon dioxide, nitrous oxide, etc that spread into the atmosphere and surround us like a blanket ● These harmful gases, called greenhouse gases, trap heat and radiation from the sun, which is causing the depletion as well as global warming. Clorofluorocarbons (CFCs), which are found in ACs and halogens, are other harmful greenhouse gases. Sources: https://e360.yale.edu/features/geoengineer-the-planet-more-scientists-now-say-it-must-be-an-option https://www.ucsusa.org/resources/ozone-hole-and-global-warming What can we do? Some things we can do to reduce our contribution to ozone layer depletion are: 1. Minimize use of cars. 2. Maintain your ACs regularly. 3. Avoid using products that are harmful to the environment and to us. 4. Buy local products which are more eco- friendly. -
A Study on the Concentration and Dispersion of Pm10 in Uthm by Using Simple Modelling and Meteorological Factors
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by UTHM Institutional Repository i A STUDY ON THE CONCENTRATION AND DISPERSION OF PM10 IN UTHM BY USING SIMPLE MODELLING AND METEOROLOGICAL FACTORS MALEK FAIZAL B ABD RAHMAN A Project Report submitted in partial fulfilment of the requirements for the award of the Degree of Master of Engineering in Civil Engineering Faculty of Civil and Environmental Engineering Universiti Tun Hussein Onn Malaysia FEBRUARY, 2013 v ABSTRACT Air pollution is the introduction of chemicals, particulate matter, or biological materials that cause harm or discomfort to humans or other living organisms, or cause damage to the natural environment or built environment, into the atmosphere. Air pollution can also be known as degradation of air quality resulting from unwanted chemicals or other materials occurring in the air. The simple way to know how polluted the air is to calculate the amounts of foreign and/or natural substances occurring in the atmosphere that may result in adverse effects to humans, animals, vegetation and/or materials. The objective of this study is to create a simulation of air quality dispersion in UTHM campus by using computer aided design mechanism such as software and calculating tools. Another objective is to compare the concentration obtained from the end result of calculation with past studies. The air pollutant in the scope of study is Particulate Matter (PM10). The highest reading recorded for E-Sampler was 305µg/m3. It was recorded in Structure Lab sampling point while the highest expected concentration by the Gaussian Dispersion Model was 184µg/m3 for UTHM Stadium. -
Global Warming
Global warming From Wikipedia, the free encyclopedia Global surface temperature increased 0.74 ± 0.18 °C (1.33 ± 0.32 °F) between the start and the end of the 20th century … Climate model projections summarized in the latest IPCC report indicate that the global surface temperature is likely to rise a further 1.1 to 6.4 °C (2.0 to 11.5 °F) during the 21st century. Global mean surface temperature difference relative to the 1961– 1990 average Comparison of ground based (blue) and satellite based (red: UAH; green: RSS) records of temperature variations since 1979. Trends plotted since January 1982. (red: University_of_Alabama_in_Huntsville; green: Remote_Sensing_Systems) Temperature is believed to have been relatively stable over the one or two thousand years before 1850, with regionally-varying fluctuations such as the Medieval Warm Period and the Little Ice Age. Two millennia of mea n surface temperatures according to different reconstructions, each smoothed on a decadal scale. The instrumental record and the unsmoothed annual value for 2004 are shown in black. Greenhouse gases The greenhouse effect is the process by which absorption and emission of infrared radiation by gases in the atmosphere warm a planet's lower atmosphere and surface. It was discovered by Joseph Fourier in 1824. Existence of the greenhouse effect as such is not disputed, even by those who do not agree that the recent temperature increase is attributable to human activity. The question is instead how the strength of the greenhouse effect changes when human activity increases the concentrations of greenhouse gases in the atmosphere. Naturally occurring greenhouse gases have a mean warming effect of about 33 °C (59 °F).