Introduction to the Atmosphere
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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. -
Aristotle University of Thessaloniki School of Geology Department of Meteorology and Climatology
1 ARISTOTLE UNIVERSITY OF THESSALONIKI SCHOOL OF GEOLOGY DEPARTMENT OF METEOROLOGY AND CLIMATOLOGY School of Geology 541 24 – Thessaloniki Greece Tel: 2310-998240 Fax:2310995392 e-mail: [email protected] 25 August 2020 Dear Editor We have submitted our revised manuscript with title “Fast responses on pre- industrial climate from present-day aerosols in a CMIP6 multi-model study” for potential publication in Atmospheric Chemistry and Physics. We considered all the comments of the reviewers and there is a detailed response on their comments point by point (see below). I would like to mention that after uncovering an error in the set- up of the atmosphere-only configuration of UKESM1, the piClim simulations of UKESM1-0-LL were redone and uploaded on ESGF (O'Connor, 2019a,b). Hence all ensemble calculations and Figures were redone using the new UKESM1-0-LL simulations. Furthermore, a new co-author (Konstantinos Tsigaridis), who has contributed in the simulations of GISS-E2-1-G used in this work, was added in the manuscript. Yours sincerely Prodromos Zanis Professor 2 Reply to Reviewer #1 We would like to thank Reviewer #1 for the constructive and helpful comments. Reviewer’s contribution is recognized in the acknowledgments of the revised manuscript. It follows our response point by point. 1) The Reviewer notes: “Section 1: Fast response vs. slow response discussion. I understand the use of these concepts, especially in view of intercomparing models. Imagine you have to talk to a wider audience interested in the “effective response” of climate to aerosol forcing in a naturally coupled climate system. -
Photochemically Driven Collapse of Titan's Atmosphere
REPORTS has escaped, the surface temperature again Photochemically Driven Collapse decreases, down to about 86 K, slightly of Titan’s Atmosphere above the equilibrium temperature, because of the slight greenhouse effect resulting Ralph D. Lorenz,* Christopher P. McKay, Jonathan I. Lunine from the N2 opacity below (longward of) 200 cm21. Saturn’s giant moon Titan has a thick (1.5 bar) nitrogen atmosphere, which has a These calculations assume the present temperature structure that is controlled by the absorption of solar and thermal radiation solar constant of 15.6 W m22 and a surface by methane, hydrogen, and organic aerosols into which methane is irreversibly converted albedo of 0.2 and ignore the effects of N2 by photolysis. Previous studies of Titan’s climate evolution have been done with the condensation. As noted in earlier studies assumption that the methane abundance was maintained against photolytic depletion (5), when the atmosphere cools during the throughout Titan’s history, either by continuous supply from the interior or by buffering CH4 depletion, the model temperature at by a surface or near surface reservoir. Radiative-convective and radiative-saturated some altitudes in the atmosphere (here, at equilibrium models of Titan’s atmosphere show that methane depletion may have al- ;10 km for 20% CH4 surface humidity) lowed Titan’s atmosphere to cool so that nitrogen, its main constituent, condenses onto becomes lower than the saturation temper- the surface, collapsing Titan into a Triton-like frozen state with a thin atmosphere. -
Geography and Atmospheric Science 1
Geography and Atmospheric Science 1 Undergraduate Research Center is another great resource. The center Geography and aids undergraduates interested in doing research, offers funding opportunities, and provides step-by-step workshops which provide Atmospheric Science students the skills necessary to explore, investigate, and excel. Atmospheric Science labs include a Meteorology and Climate Hub Geography as an academic discipline studies the spatial dimensions of, (MACH) with state-of-the-art AWIPS II software used by the National and links between, culture, society, and environmental processes. The Weather Service and computer lab and collaborative space dedicated study of Atmospheric Science involves weather and climate and how to students doing research. Students also get hands-on experience, those affect human activity and life on earth. At the University of Kansas, from forecasting and providing reports to university radio (KJHK 90.7 our department's programs work to understand human activity and the FM) and television (KUJH-TV) to research project opportunities through physical world. our department and the University of Kansas Undergraduate Research Center. Why study geography? . Because people, places, and environments interact and evolve in a changing world. From conservation to soil science to the power of Undergraduate Programs geographic information science data and more, the study of geography at the University of Kansas prepares future leaders. The study of geography Geography encompasses landscape and physical features of the planet and human activity, the environment and resources, migration, and more. Our Geography integrates information from a variety of sources to study program (http://geog.ku.edu/degrees/) has a unique cross-disciplinary the nature of culture areas, the emergence of physical and human nature with pathway options (http://geog.ku.edu/geography-pathways/) landscapes, and problems of interaction between people and the and diverse faculty (http://geog.ku.edu/faculty/) who are passionate about environment. -
Air Pressure
Name ____________________________________ Date __________ Class ___________________ SECTION 15-3 SECTION SUMMARY Air Pressure Guide for ir consists of atoms and molecules that have mass. Therefore, air has Reading A mass. Because air has mass, it also has other properties, includ- ing density and pressure. The amount of mass per unit volume of a N What are some of substance is called the density of the substance. The force per unit area the properties of air? is called pressure. Air pressure is the result of the weight of a column of N What instruments air pushing down on an area. The molecules in air push in all directions. are used to mea- This is why air pressure doesn’t crush objects. sure air pressure? Falling air pressure usually indicates that a storm is approaching. Rising N How does increas- air pressure usually means that the weather is clearing. A ing altitude affect barometer is an instrument that measures changes in air pressure. There air pressure and are two kinds of barometers: mercury barometers and aneroid density? barometers. A mercury barometer consists of a glass tube open at the bottom end and partially filled with mercury. The open end of the tube rests in a dish of mercury, and the space above the mercury in the tube contains no air. The air pressure pushing down on the surface of the mer- cury in the dish is equal to the weight of the column of mercury in the tube. At sea level, the mercury column is about 76 centimeters high, on average. An aneroid barometer has an airtight metal chamber that is sen- sitive to changes in air pressure. -
Earth System Climatology (ESS200A)
EarthEarth SystemSystem ClimatologyClimatology (ESS200A)(ESS200A) Course Time Lectures: Tu, Th 9:00-10:20 Discussion: 3315 Croul Hall Text Book The Earth System, 2nd Edition, Kump, Kasting, and Crane, Prentice-Hall Global Physical Climatology, Hartmann; Academic Press Meteorology Today, 7th Edition, Ahrens, Brooks Cool. Grade Homework (40%), Final (60%) Homework Issued and due every Thursday ESS200A Prof. Jin-Yi Yu ESS200A Prof. Jin-Yi Yu CourseCourse DescriptionDescription A general description of the Earth climate system and its subcomponents: the atmosphere, ocean, land surface, ice, and solid earth. ESS200A Prof. Jin-Yi Yu SyllabusSyllabus Week 1 - Global Energy Balance Week 3-4: Ocean Planetary Energy Balance Basic Structure and Dynamics Greenhouse Effect Surface Ocean Circulation: Wind-Driven Atmospheric Composition and Structure Deep Ocean Circulation: Density-Driven Role of Cloud Week 4: Land Surface and Cryosphere Week 2 - Atmospheric General Circulation Land Surface Properties (Soil and Vegetation) Hydrostatic Balance Surface Energy and Water Balance General Circulation in the Troposphere Sea Ice and Land Ice General Circulation in the Stratosphere Climate Roles of Land Surface and Ice Jetstreams Regional Circulation Systems Week 5 – Climate Change and Variation Week 2-3 - Weather Past Climate Change Air Masses and Fronts Short-term Climate variation (ENSO, NAO) Mid-Latitude Cyclones Ozone Hole Tropical Hurricane *** FINAL (October 27, Thursday) *** ESS200A Prof. Jin-Yi Yu GlobalGlobal EnergyEnergy CycleCycle Planetary energy balance Energy absorbed by Earth = Energy emitted by Earth Role of the atmosphere Greenhouse effect Role of oceans Polarward energy transport Role of land surface not significant due to its low heat capacity (from Climate Change 1995) ESS200A Prof. -
Effect of Tropospheric Air Density and Dew Point Temperature on Radio (Electromagnetic) Waves and Air Radio Wave Refractivity
International Journal of Scientific & Engineering Research, Volume 7, Issue 6, June-2016 356 ISSN 2229-5518 Effect of Tropospheric Air density and dew point temperature on Radio (Electromagnetic) waves and Air radio wave refractivity <Joseph Amajama> University of Calabar, Department of Physics, Electronics and Computer Technology Unit Etta-agbor, Calabar, Nigeria [email protected] Abstract: Signal strengths measurements were obtained half hourly for some hours and simultaneously, the atmospheric components: atmospheric temperature, atmospheric pressure, relative humidity and wind direction and speed were registered to erect the effects of air density and dew point temperature on radio signals (electromagnetic waves) as they travel through the atmosphere and air radio wave refractivity. The signal strength from Cross River State Broadcasting Co-operation Television (CRBC-TV), (4057'54.7''N, 8019'43.7''E) transmitted at 35mdB and 519.25 MHz (UHF) were measured using a Cable TV analyzer in a residence along Ettaabgor, Calabar, Nigeria (4057'31.7''N, 8020'49.7''E) using the digital Community – Access (Cable) Television (CATV) analyzer with 24 channels, spectrum 46 – 870 MHz, connected to a domestic receiver antenna of height 4.23 m. Results show that: on the condition that the wind speed and direction are the same or (0 mph NA), the radio signal strength is near negligibly directly proportional to the air density, mathematically Ss / ∂a1.3029 = K, where Ss is Signal Strength in dB, ∂a is Density of air Kg/m3 and K is constant; radio -
Light, Color, and Atmospheric Optics
Light, Color, and Atmospheric Optics GEOL 1350: Introduction To Meteorology 1 2 • During the scattering process, no energy is gained or lost, and therefore, no temperature changes occur. • Scattering depends on the size of objects, in particular on the ratio of object’s diameter vs wavelength: 1. Rayleigh scattering (D/ < 0.03) 2. Mie scattering (0.03 ≤ D/ < 32) 3. Geometric scattering (D/ ≥ 32) 3 4 • Gas scattering: redirection of radiation by a gas molecule without a net transfer of energy of the molecules • Rayleigh scattering: absorption extinction 4 coefficient s depends on 1/ . • Molecules scatter short (blue) wavelengths preferentially over long (red) wavelengths. • The longer pathway of light through the atmosphere the more shorter wavelengths are scattered. 5 • As sunlight enters the atmosphere, the shorter visible wavelengths of violet, blue and green are scattered more by atmospheric gases than are the longer wavelengths of yellow, orange, and especially red. • The scattered waves of violet, blue, and green strike the eye from all directions. • Because our eyes are more sensitive to blue light, these waves, viewed together, produce the sensation of blue coming from all around us. 6 • Rayleigh Scattering • The selective scattering of blue light by air molecules and very small particles can make distant mountains appear blue. The blue ridge mountains in Virginia. 7 • When small particles, such as fine dust and salt, become suspended in the atmosphere, the color of the sky begins to change from blue to milky white. • These particles are large enough to scatter all wavelengths of visible light fairly evenly in all directions. -
Air Infiltration Glossary (English Edition)
AIRGLOSS: Air Infiltration Glossary (English Edition) Carolyn Allen ~)Copyrlght Oscar Faber Partnership 1981. All property rights, Including copyright ere vested In the Operating Agent (The Oscar Faber Partnership) on behalf of the International Energy Agency. In particular, no part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior written permluion of the operat- ing agent. Contents (i) Preface (iii) Introduction (v) Umr's Guide (v) Glossary Appendix 1 - References 87 Appendix 2 - Tracer Gases 93 Appendix 3 - Abbreviations 99 Appendix 4 - Units 103 (i) (il) Preface International Energy Agency In order to strengthen cooperation In the vital area of energy policy, an Agreement on an International Energy Program was formulated among a number of industrialised countries In November 1974. The International Energy Agency (lEA) was established as an autonomous body within the Organisation for Economic Cooperation and Development (OECD) to administer that agreement. Twenty-one countries are currently members of the lEA, with the Commission of the European Communities participating under a special arrangement. As one element of the International Energy Program, the Participants undertake cooperative activities in energy research, development, and demonstration. A number of new and improved energy technologies which have the potential of making significant contributions to our energy needs were identified for collaborative efforts. The lEA Committee on Energy Research and Development (CRD), assisted by a small Secretariat staff, coordinates the energy research, development, and demonstration programme. Energy Conservation in Buildings and Community Systems The International Energy Agency sponsors research and development in a number of areas related to energy. -
Project Horizon Report
Volume I · SUMMARY AND SUPPORTING CONSIDERATIONS UNITED STATES · ARMY CRD/I ( S) Proposal t c• Establish a Lunar Outpost (C) Chief of Ordnance ·cRD 20 Mar 1 95 9 1. (U) Reference letter to Chief of Ordnance from Chief of Research and Devel opment, subject as above. 2. (C) Subsequent t o approval by t he Chief of Staff of reference, repre sentatives of the Army Ballistic ~tissiles Agency indicat e d that supplementar y guidance would· be r equired concerning the scope of the preliminary investigation s pecified in the reference. In particular these r epresentatives requested guidance concerning the source of funds required to conduct the investigation. 3. (S) I envision expeditious development o! the proposal to establish a lunar outpost to be of critical innportance t o the p. S . Army of the future. This eva luation i s appar ently shar ed by the Chief of Staff in view of his expeditious a pproval and enthusiastic endorsement of initiation of the study. Therefore, the detail to be covered by the investigation and the subs equent plan should be as com plete a s is feas ible in the tin1e limits a llowed and within the funds currently a vailable within t he office of t he Chief of Ordnance. I n this time of limited budget , additional monies are unavailable. Current. programs have been scrutinized r igidly and identifiable "fat'' trimmed awa y. Thus high study costs are prohibitive at this time , 4. (C) I leave it to your discretion t o determine the source and the amount of money to be devoted to this purpose. -
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.