Fact Sheet No. 13 – Upper Air Observations and the Tephigram
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On the Relationship Between Gravity Waves and Tropopause Height and Temperature Over the Globe Revealed by COSMIC Radio Occultation Measurements
atmosphere Article On the Relationship between Gravity Waves and Tropopause Height and Temperature over the Globe Revealed by COSMIC Radio Occultation Measurements Daocheng Yu 1, Xiaohua Xu 1,2,*, Jia Luo 1,3,* and Juan Li 1 1 School of Geodesy and Geomatics, Wuhan University, 129 Luoyu Road, Wuhan 430079, China; [email protected] (D.Y.); [email protected] (J.L.) 2 Collaborative Innovation Center for Geospatial Technology, 129 Luoyu Road, Wuhan 430079, China 3 Key Laboratory of Geospace Environment and Geodesy, Ministry of Education, 129 Luoyu Road, Wuhan 430079, China * Correspondence: [email protected] (X.X.); [email protected] (J.L.); Tel.: +86-27-68758520 (X.X.); +86-27-68778531 (J.L.) Received: 4 January 2019; Accepted: 6 February 2019; Published: 12 February 2019 Abstract: In this study, the relationship between gravity wave (GW) potential energy (Ep) and the tropopause height and temperature over the globe was investigated using COSMIC radio occultation (RO) dry temperature profiles during September 2006 to May 2013. The monthly means of GW Ep with a vertical resolution of 1 km and tropopause parameters were calculated for each 5◦ × 5◦ longitude-latitude grid. The correlation coefficients between Ep values at different altitudes and the tropopause height and temperature were calculated accordingly in each grid. It was found that at middle and high latitudes, GW Ep over the altitude range from lapse rate tropopause (LRT) to several km above had a significantly positive/negative correlation with LRT height (LRT-H)/ LRT temperature (LRT-T) and the peak correlation coefficients were determined over the altitudes of 10–14 km with distinct zonal distribution characteristics. -
CARI-7 Documentation: Radiation Transport in the Atmosphere
DOT/FAA/AM-21/5 Office of Aerospace Medicine Washington, DC 20591 CARI Documentation: Radiation Transport in the Atmosphere Kyle Copeland Civil Aerospace Medical Institute Federal Aviation Administration Oklahoma City, OK 73125Location/Address March 2021 Final Report 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/go/oamtechreports) Technical Report Documentation Page 1. Report No. 2. Government Accession No. 3. Recipient's Catalog No. DOT/FAA/AM-21/5 4. Title and Subtitle 5. Report Date CARI-7 DOCUMENTATION: RADIATION TRANSPORT IN March 2021 THE ATMOSPHERE 6. Performing Organization Code 7. Author(s) 8. Performing Organization Report No. Copeland, K. 9. Performing Organization Name and Address 10. Work Unit No. (TRAIS) Civil Aerospace Medical Institute FAA 11. Contract or Grant No. 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 Primary cosmic radiation from both the Sun and interstellar space enters Earth's atmosphere in varying amounts. Outside of Earth's atmosphere, cosmic radiation is modulated by solar activity and Earth's magnetic field. Once the radiation enters Earth's atmosphere, it interacts with Earth's atmosphere in the same manner regardless of its point of origin (solar or galactic). -
Nighttime Secondary Ozone Layer During Major Stratospheric Sudden Warmings in Specified-Dynamics WACCM Olga V
JOURNAL OF GEOPHYSICAL RESEARCH: ATMOSPHERES, VOL. 118, 8346–8358, doi:10.1002/jgrd.50651, 2013 Nighttime secondary ozone layer during major stratospheric sudden warmings in specified-dynamics WACCM Olga V. Tweedy,1,2 Varavut Limpasuvan,1 Yvan J. Orsolini,3,4 Anne K. Smith,5 Rolando R. Garcia,5 Doug Kinnison,5 Cora E. Randall,6,7 Ole-Kristian Kvissel,8 Frode Stordal,8 V. Lynn Harvey,6,7 and Amal Chandran 9 Received 26 March 2013; revised 5 July 2013; accepted 15 July 2013; published 9 August 2013. [1] A major stratospheric sudden warming (SSW) strongly impacts the entire middle atmosphere up to the thermosphere. Currently, the role of atmospheric dynamics on polar ozone in the mesosphere-lower thermosphere (MLT) during SSWs is not well understood. Here we investigate the SSW-induced changes in the nighttime “secondary” (90–105 km) ozone maximum by examining the dynamics and distribution of key species (like H and O) important to ozone. We use output from the National Center for Atmospheric Research Whole Atmosphere Community Climate Model with “Specified Dynamics” (SD-WACCM), in which the simulation is constrained by meteorological reanalyses below 1 hPa. Composites are made based on six major SSW events with elevated stratopause episodes. Individual SSW cases of temperature and MLT nighttime ozone from the model are compared against the Sounding of the Atmosphere using Broadband Emission Radiometry observations aboard the NASA’s Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED) satellite. The evolution of ozone and major chemical trace species is associated with the anomalous vertical residual motion during SSWs and consistent with photochemical equilibrium governing the MLT nighttime ozone. -
Popular Summary of “Extratropical Stratosphere-Troposphere Mass Exchange”
Popular Summary of “Extratropical Stratosphere-Troposphere Mass Exchange” Mark Schoeberl Understanding the exchange of gases between the stratosphere and the troposphere is important for determining how pollutants enter the stratosphere and how they leave. This study does a global analysis of that the exchange of mass between the stratosphere and the troposphere. While the exchange of mass is not the same as the exchange of constituents, you can’t get the constituent exchange right if you have the mass exchange wrong. Thus this kind of calculation is an important test for models which also compute trace gas transport. In this study I computed the mass exchange for two assimilated data sets and a GCM. The models all agree that amount of mass descending from the stratosphere to the troposphere in the Northern Hemisphere extra tropics is -1 0” kg/s averaged over a year. The value for the Southern Hemisphere by about a factor of two. ( 10” kg of air is the amount of air in 100 km x 100 km area with a depth of 100 m - roughly the size of the D.C. metro area to a depth of 300 feet.) Most people have the idea that most of the mass enters the stratosphere through the tropics. But this study shows that almost 5 times more mass enters the stratosphere through the extra-tropics. This mass, however, is quickly recycled out again. Thus the lower most stratosphere is a mixture of upper stratospheric air and tropospheric air. This is an important result for understanding the chemistry of the lower stratosphere. -
The Tropical Tropopause Layer in Reanalysis Data Sets
https://doi.org/10.5194/acp-2019-580 Preprint. Discussion started: 4 July 2019 c Author(s) 2019. CC BY 4.0 License. 1 2 The tropical tropopause layer in reanalysis data sets 3 4 Susann Tegtmeier1, James Anstey2, Sean Davis3, Rossana Dragani4, Yayoi Harada5, Ioana 5 Ivanciu1, Robin Pilch Kedzierski1, Kirstin Krüger6, Bernard Legras7, Craig Long8, James S. 6 Wang9, Krzysztof Wargan10,11, and Jonathon S. Wright12 7 8 9 1 10 GEOMAR Helmholtz Centre for Ocean Research Kiel, 24105 Kiel, Germany 11 2Canadian Centre for Climate Modelling and Analysis, ECCC, Victoria, Canada 12 3Earth System Research Laboratory, National Oceanic and Atmospheric Administration, 13 Boulder, CO 80305, USA 14 4European Centre for Medium-Range Weather Forecasts, Reading, RG2 9AX, UK 15 5Japan Meteorological Agency, Tokyo, 100-8122, Japan 16 6 Section for Meteorology and Oceanography, Department of Geosciences, University of Oslo, 17 0315 Oslo, Norway 18 7Laboratoire de Météorologie Dynamique, CNRS/PSL-ENS, Sorbonne University Ecole 19 Polytechnique, France 20 8Climate Prediction Center, National Centers for Environmental Prediction, National Oceanic 21 and Atmospheric Administration, College Park, MD 20740, USA 22 9Institute for Advanced Sustainability Studies, Potsdam, Germany 23 10Science Systems and Applications, Inc., Lanham, MD 20706, USA 24 11Global Modeling and Assimilation Office, Code 610.1, NASA Goddard Space Flight 25 Center, Greenbelt, MD 20771, USA 26 12Department of Earth System Science, Tsinghua University, Beijing, 100084, China 27 28 29 30 31 32 33 34 35 36 37 1 https://doi.org/10.5194/acp-2019-580 Preprint. Discussion started: 4 July 2019 c Author(s) 2019. CC BY 4.0 License. -
ESSENTIALS of METEOROLOGY (7Th Ed.) GLOSSARY
ESSENTIALS OF METEOROLOGY (7th ed.) GLOSSARY Chapter 1 Aerosols Tiny suspended solid particles (dust, smoke, etc.) or liquid droplets that enter the atmosphere from either natural or human (anthropogenic) sources, such as the burning of fossil fuels. Sulfur-containing fossil fuels, such as coal, produce sulfate aerosols. Air density The ratio of the mass of a substance to the volume occupied by it. Air density is usually expressed as g/cm3 or kg/m3. Also See Density. Air pressure The pressure exerted by the mass of air above a given point, usually expressed in millibars (mb), inches of (atmospheric mercury (Hg) or in hectopascals (hPa). pressure) Atmosphere The envelope of gases that surround a planet and are held to it by the planet's gravitational attraction. The earth's atmosphere is mainly nitrogen and oxygen. Carbon dioxide (CO2) A colorless, odorless gas whose concentration is about 0.039 percent (390 ppm) in a volume of air near sea level. It is a selective absorber of infrared radiation and, consequently, it is important in the earth's atmospheric greenhouse effect. Solid CO2 is called dry ice. Climate The accumulation of daily and seasonal weather events over a long period of time. Front The transition zone between two distinct air masses. Hurricane A tropical cyclone having winds in excess of 64 knots (74 mi/hr). Ionosphere An electrified region of the upper atmosphere where fairly large concentrations of ions and free electrons exist. Lapse rate The rate at which an atmospheric variable (usually temperature) decreases with height. (See Environmental lapse rate.) Mesosphere The atmospheric layer between the stratosphere and the thermosphere. -
Elemental Geosystems, 5E (Christopherson) Chapter 2 Solar Energy, Seasons, and the Atmosphere
Elemental Geosystems, 5e (Christopherson) Chapter 2 Solar Energy, Seasons, and the Atmosphere 1) Our planet and our lives are powered by A) energy derived from inside Earth. B) radiant energy from the Sun. C) utilities and oil companies. D) shorter wavelengths of gamma rays, X-rays, and ultraviolet. Answer: B 2) Which of the following is true? A) The Sun is the largest star in the Milky Way Galaxy. B) The Milky Way is part of our Solar System. C) The Sun produces energy through fusion processes. D) The Sun is also a planet. Answer: C 3) Which of the following is true about the Milky Way galaxy in which we live? A) It is a spiral-shaped galaxy. B) It is one of millions of galaxies in the universe. C) It contains approximately 400 billion stars. D) All of the above are true. E) Only A and B are true. Answer: D 4) The planetesimal hypothesis pertains to the formation of the A) universe. B) galaxy. C) planets. D) ocean basins. Answer: C 5) The flattened structure of the Milky Way is revealed by A) the constellations of the Zodiac. B) a narrow band of hazy light that stretches across the night sky. C) the alignment of the planets in the solar system. D) the plane of the ecliptic. Answer: B 6) Earth and the Sun formed specifically from A) the galaxy. B) unknown origins. C) a nebula of dust and gases. D) other planets. Answer: C 7) Which of the following is not true of stars? A) They form in great clouds of gas and dust known as nebula. -
Today: Upper Atmosphere/Ionosphere
Today: Upper Atmosphere/Ionosphere • Review atmospheric Layers – Follow the energy! – What heats the Stratosphere? • Mesosphere – Most turbulent layer – why? • Ionosphere – What is a Plasma? The Solar Spectrum: The amount of energy the Sun produces at a given wavelength is determined by its temperature. This is a general property of any Black Body such as a star or the heating element on the stove. • The Sun is about 5270 K and produces most light in the visible. • The atmosphere is transparent in the visible and so over half of the solar energy reaches the ground. • Some gasses absorb certain wavelengths of sunlight, and thus some energy is absorbed directly into the atmosphere. Depositing Energy Energy from the Sun may be transmitted directly to the ground, absorbed in the atmosphere, or reflected from clouds or the Sun back into space. Some re-radiated heat from the ground is absorbed by the atmosphere, further heating it. The Troposhphere The troposphere is the region of the atmosphere we live in. The primary source of energy in the troposphere is heat (infrared light ) radiated from the ground. This means that it is warmest at the bottom and coolest at the top. Temperature drops about 11.5 ° F for each km of altitude. When pressure and temperature (with temp. faster) drop with altitude it triggers convection . Convection makes the troposphere unstable, but in a good way. Dominant Region The Troposphere contains 80% of the mass in the atmosphere and 99% of the water in the atmosphere. Water Vapor, CO 2, methane, nitrous oxide, ozone, chloroflorocarbons are all greenhouse gases Convection (both horizontal and vertical) produces weather in the atmosphere. -
Tropical Tropopause Layer
Click Here for Full Article TROPICAL TROPOPAUSE LAYER S. Fueglistaler,1 A. E. Dessler,2 T. J. Dunkerton,3 I. Folkins,4 Q. Fu,5 and P. W. Mote3 Received 4 March 2008; revised 16 September 2008; accepted 14 October 2008; published 17 February 2009. [1] Observations of temperature, winds, and atmospheric 70 hPa, 425 K, 18.5 km. Laterally, the TTL is bounded by trace gases suggest that the transition from troposphere to the position of the subtropical jets. We highlight recent stratosphere occurs in a layer, rather than at a sharp progress in understanding of the TTL but emphasize that a ‘‘tropopause.’’ In the tropics, this layer is often called the number of processes, notably deep, possibly overshooting ‘‘tropical tropopause layer’’ (TTL). We present an overview convection, remain not well understood. The TTL acts in of observations in the TTL and discuss the radiative, many ways as a ‘‘gate’’ to the stratosphere, and dynamical, and chemical processes that lead to its time- understanding all relevant processes is of great importance varying, three-dimensional structure. We present a synthesis for reliable predictions of future stratospheric ozone and definition with a bottom at 150 hPa, 355 K, 14 km climate. (pressure, potential temperature, and altitude) and a top at Citation: Fueglistaler, S., A. E. Dessler, T. J. Dunkerton, I. Folkins, Q. Fu, and P. W. Mote (2009), Tropical tropopause layer, Rev. Geophys., 47, RG1004, doi:10.1029/2008RG000267. 1. INTRODUCTION [3] This paper examines and discusses observations in the TTL and the processes that contribute to its unique [2] The traditional definitions of the troposphere and properties. -
Analysis of Tropopause Variability in Observations and in an Idealized Model
UNIVERSIDAD COMPLUTENSE DE MADRID FACULTAD DE CIENCIAS FÍSICAS Departamento de Física de la Tierra, Astronomía y Astrofísica I (Geofísica y Meteorología) TESIS DOCTORAL Analysis of tropopause variability in observations and in an idealized model Análisis de la variabilidad de la tropopausa en observaciones y en un modelo idealizado MEMORIA PARA OPTAR AL GRADO DE DOCTOR PRESENTADA POR Jesús Ángel Barroso Pellico Director Pablo Zurita Gotor Madrid, 2018 © Jesús Ángel Barroso Pellico, 2017 Universidad Complutense de Madrid Facultad de Ciencias Físicas Departamento de Física de la Tierra, Astronomía y Astrofísica I (Geofísica y Meteorología) Analysis of tropopause variability in observations and in an idealized model Análisis de la variabilidad de la tropopausa en observaciones y en un modelo idealizado Memoria para optar al grado de doctor presentada por Jesús Ángel Barroso Pellico Director: Pablo Zurita Gotor III IV Contents Summary.......................................................................................................... VII Resumen.......................................................................................................... XI List of abbreviations......................................................................................... XIV 1. Introduction and objectives.................................................................................. 1 1.1 Properties of the tropopause.......................................................................................3 1.1.1 Definitions of the tropopause........................................................................ -
Response of the Mesosphere-Thermosphere- Ionosphere System to Global Change - CAWSES-II Contribution Jan Laštovička1*, Gufran Beig2 and Daniel R Marsh3
Laštovička et al. Progress in Earth and Planetary Science 2014, 1:21 http://www.progearthplanetsci.com/content/1/1/21 REVIEW Open Access Response of the mesosphere-thermosphere- ionosphere system to global change - CAWSES-II contribution Jan Laštovička1*, Gufran Beig2 and Daniel R Marsh3 Abstract Long-term trends in the mesosphere, thermosphere, and ionosphere are areas of research of increasing importance both because they are sensitive indicators of climatic change and because they affect satellite-based technologies which are increasingly important to modern life. Their study was an important part of CAWSES-II project, as they were a topic of Task Group 2 (TG-2) ‘How Will Geospace Respond to Changing Climate’. Three individual projects of TG-2 were focused on important problems in trend investigations. Significant progress was reached in several areas such as understanding and quantifying the role of stratospheric ozone changes in trends in the upper atmosphere, reaching reasonable agreement between observed and simulated trends in mesospheric temperatures and polar mesospheric clouds, or understanding of why the thermospheric density trends are much stronger under solar cycle minimum conditions. The TG-2 progress that is reviewed in this paper together with some results reached outside CAWSES-II so as to have the full context of progress in trends in the upper atmosphere and ionosphere. Keywords: Mesosphere; Thermosphere; Ionosphere; Long-term trends; Climatic change Review Laštovička et al. 2012). The thermosphere is the operating Introduction environment of many satellites, including the Inter- The anthropogenic emissions of greenhouse gases carbon national Space Station, and thousands of pieces of danger- dioxide (CO2), methane (CH4), and nitrous oxide (N2O) ous space debris, the orbital lifetime of which depends on influence the troposphere, weather, and particularly cli- long-term changes of thermospheric density. -
The Earth's Atmosphere
A Resource Booklet for SACE Stage 1 Earth and Environmental Science The following pages have been prepared by practicing teachers of SACE Earth and Environmental Science. The six Chapters are aligned with the six topics described in the SACE Stage 1 subject outline. They aim to provide an additional source of contexts and ideas to help teachers plan to teach this subject. For further information, including the general and assessment requirements of the course see: https://www.sace.sa.edu.au/web/earth-and-environmental- science/stage-1/planning-to-teach/subject-outline A Note for Teachers The resources in this booklet are not intended for ‘publication’. They are ‘drafts’ that have been developed by teachers for teachers. They can be freely used for educational purposes, including course design, topic and lesson planning. Each Chapter is a living document, intended for continuous improvement in the future. Teachers of Earth and Environmental Science are invited to provide feedback, particularly suggestions of new contexts, field-work and practical investigations that have been found to work well with students. Your suggestions for improvement would be greatly appreciated and should be directed to our project coordinator:: [email protected] Preparation of this booklet has been coordinated and funded by the Geoscience Pathways Project, under the sponsorship of the Geological Society of Australia (GSA) and the Teacher Earth Science Education Program (TESEP). In-kind support has been provided by the SA Department of Energy and Mining (DEM) and the Geological Survey of South Australia (GSSA). FAIR USE: The teachers named alongside each chapter of this document have researched available resources, selected and collated these notes and images from a wide range of sources.