Autumn 07: ATMS/CHEM 458 Global Atmospheric Chemistry MWF 10:30 – 11:20 Tu 10:30 – 12:20 610 ATG Building Course Goals This class will provide an overview of atmospheric chemistry and the fundamental underpinnings so that you will be able to: •Describe the workings of the atmosphere as a chemical reactor •Explain several important atmospheric phenomena from the molecular to the global scale •Critically evaluate and participate in public discussions of air pollution and climate change Course Related Activities (see course website for more information) Lectures/Discussions Lectures are for you, not me. Please interact! 3 in-class debates: – national air quality standards - funding studies of strat ozone chemistry? - geo-engineering of climate? Problem Sets Are certainly doable, but require some thought. Never wait until the last minute. Projects Choose a topic from class for further investigation, write a 10 – 15 pg report and give a 15 minute presentation to the class. -further guided analysis of data provided in class -run and maintain O3 and CO instruments during quarter -propose a research question or review current literature This Week READING: Chapter 1 - 2 of text Tasks: Find a computer on which you can use Matlab. If you don’t have easy (free) access, let me know and I’ll set you up. A problem set will be handed out on Friday, due the following week which suggests the use of Matlab. • Goals, Topic Overview •Atmospheric Physical and Chemical Properties • Fundamentals Goal of Atmospheric Chemistry To develop a detailed understanding of the chemical and physical processes which control the amounts and spatial and temporal distributions of atmospheric constituents. Why? The atmosphere plays a critical role in Earth’s energy balance (climate) Protects/Sustains life at the surface Couples land,oceans, equator and poles Human activity changes its composition Atmosphere in the Earth System Clouds Aerosols, O3 Atmosphere-Biosphere Exchange The Atmosphere Moves CO Movie How Do We Begin? Describe the general physical characteristics mass, temperature, vertical extent, motions Determine the major and minor components describe absolute and relative amounts Develop a physical-chemical framework to: predict how a species evolves in time and space Apply this framework to answer: Why is Earth’s atmosphere mainly N2, O2, H2O, and CO2? How does composition help explain Earth’s climate? How and where are humans affecting this composition? Urban Smog Problem • Global chemistry and climate implications • Complex regulatory issues Houston, TX Stratospheric Ozone Depletion Climate – Chemistry Connections Does composition change drive climate change, or vise versa, or both? Spatial and Temporal Scales of Change Gases trapped in ice show changes over millennial and annual timescales. Ozone, NO2, and NO near Nashville, TN O3 100 NO2 NO Mixing Ratio (ppbv) 80 60 Chemical change occurs on time scales ranging from <1 second to >millennia 40 20 0 171 171.5 172 172.5 173 Day of Year (mid June 1999) 173.5 174 In-class activity Let’s start thinking about the atmosphere… Break into a couple groups, and determine how to: 1. Calculate the absolute amount of a specific gas (e.g. CO2) that resides in the atmosphere if you know its relative amount (e.g. 0.0004%) 2. Calculate the mass of the entire atmosphere. This is not an aptitude test! The goal is to get you thinking about the atmosphere, period. Describing Amounts The atmosphere contains gases (mostly) and some liquids/solids – aerosols and clouds. All gases can be described by ideal gas law Aerosols and clouds need: Px = (nx/V)RT Ptotal = (Px) Size, Number, Composition, and Phase State mass and volume concentrations Mass ma of the Atmosphere Mean surface pressure: 984 hPa Radius of Earth: 6378 km 4 R PS 18 ma 5.2 10 kg g 2 Total number of moles of air in atmosphere: ma Na 1.8 1020 moles Ma Today • Atmospheric structure •Vertical profiles of pressure and temperature •A slightly closer look at composition •H2O phases •Aerosol particles •Working with PV=nRT Atmospheric Structure Vertical profiles of pressure and temperature (means for 30oN, March) Stratopause Everest ~ 9 km Tropopause Average Composition as Mixing Ratios Trace gases GAS MIXING RATIO (dry air) [mol mol-1] Nitrogen (N2) 0.78 Oxygen (O2) 0.21 Argon (Ar) 0.0093 Carbon dioxide (CO2) 365x10-6 Neon (Ne) 18x10-6 Ozone (O3) (0.01-10)x10-6 Helium (He) 5.2x10-6 Methane (CH4) 1.7x10-6 Krypton (Kr) 1.1x10-6 Mixing Ratio is a mole fraction (Moles X/Total Moles) • Air also contains variable H2O vapor (10-6-10-2 mol mol-1) and aerosol particles • Trace gas mixing ratio units: 1 ppmv = 1x10-6 mol mol-1 1 ppbv = 1x10-9 mol mol-1 1 pptv = 1x10-12 mol mol-1 Related Measures of Composition Mixing Ratio CX moles of X total moles of air Number Density NX # molecules of X unit volume of air •Constant w.r.t. changes in air density proper measure for • calculation of reaction rates • optical properties of atmosphere NX and CX are related by the ideal gas law: N X N air C X N Avag Pair RT CX Also define the mass concentration (g cm-3 of air): M X N X ( g / mol )(molec / cm3 ) mass of X X unit volume of air N Avag (molec / mol ) Not to be confused with the density of a substance (g cm-3 of substance) H2O Phase Diagram PH2O,SAT(T) Saturation Vapor Pressure Amount of water vapor volume of air can hold. Determines when condensed phase H2O can exist Formation of condensed phase H2O often leads to removal by precipitation Relative humidity (%) = 100(PH2O/PH2O,SAT) Dew point: Temperature Td such that PH2O = PH2O,SAT(Td) Visibility Reduction by Aerosols (Haze) • clean day moderately polluted day Acadia National Park (Northeastern Maine) http://www.hazecam.net/ Typical U.S. Aerosol Size Distributions Maxima are most common sizes volume frequency Fresh urban Aged urban rural remote Warneck [1999] Annual Mean Particulate Matter (PM) Concentrations at U.S. Sites, 1995-2000 PM2.5 (aerosol particles < 2.5 mm diameter) EPA particulate matter assessment document (NARSTO), 2003 U.S. air quality standard: PM2.5 = 15 mg m-3 (annual mean) Red circles indicate sites in violation of the standard STANDARD IS EXPRESSED AS A MASS CONCENTRATION Total Mass of Particles PER UNIT VOLUME AIR Chemical Composition of PM2.5 (EPA/NARSTO PM ASSESSMENT, 2003) Sulfate Esther (1995-99) Egbert (1994-99) 4.6 ug m -3 8.9 ug m -3 Nitrate Toronto (1997-99) 12.3 ug m -3 Ammonium Black carbon Abbotsford (1994-95) Organic carbon 7.8 ug m -3 Soil Other St. A ndrews (1994-97) 5.3 ug m -3 Fresno (1988-89) 39.2 ug m -3 Quaker City OH (1999) 12.4 ug m -3 Kern Wildlife Refuge (1988-89) 23.3 ug m -3 Los Angeles (1995-96) Arendstville PA (1999) 10.4 ug m -3 Mexico City Netzahualcoyotl (1997) 55.4 ug m -3 Washington DC (1996-99) 14.5 ug m -3 30.3 ug m -3 Colorado Plateau (1996-99) 3.0 ug m -3 Mexico City - Pedregal (1997) 24.6 ug m -3 Yorkville (1999) 14.7 ug m -3 Atlanta (1999) 19.2 ug m -3 Questions 1. How many molecules of air are in 1 cm3 of this room? 2. The mixing ratio of CO2 is currently ~ 380 ppm throughout the atmosphere, sketch its partial pressure versus altitude. 3. A typical ozone number density at the surface is 1x1012 molec/cm3, while at 30 km it is 5x1012 molec/cm3. Where is its mixing ratio highest? 4. The tropics are clearly warmer on average than the poles. If the vertically averaged temperature is higher in the tropics than at the poles, how will the pressure at some altitude compare between the equator and poles? QUESTIONS 1. Oxygen has a constant mixing ratio in the atmosphere. How does its number density measured in surface air vary between day and night? 2. Give a rough order of magnitude for the number of molecules present in a typical 1 micrometer aerosol particle. 3. Does it make sense to talk about the mixing ratio of aerosol particles in air? To express the concentration of soot aerosol in units of ppbv? This Week—Transport Timescales READING: Chapter 4 of text •Tropical and Mid-latitude Circulation •Vertical transport and stability: Buoyancy Today&Tomorrow: General Circulation Global Heat Engine Coriolis Effect Hadley Circulation Upper level westerlies and surface trades Convergence/Divergence Uplift/Subsidence Making Air Move Pressure Gradient Force Fluid will move from high to low pressure Fluid with horizontal pressure gradient Applies to horizontal (parallel to earth’s surface) and vertical (perpendicular to earth’s surface) Buoyant Forces Recall ideal gas law: density 1/T buoyancy: when pressure gradient force in vertical direction not equal to force due to gravity When an air parcel’s density is lower/higher than the surrounding air, it will rise/sink The Engine’s Heat Source Latitudinal gradient in solar insolation The equator receives a greater solar radiation energy flux (J/m2/s) than the poles Isobars (Constant Pressure Lines) Suggest Eq. To pole flow Alt. PGF The picture is roughly symmetric for the Southern Hemisphere (SH) Early Picture of General Circulation Based on Hadley’s 1735 paper: “Tropopause” divergence subsidence Uplift (convection) subsidence L H H convergence 90 45 0 -45 -90 Cold high lats Warm Tropics Cold high lats higher pressure Lower pressure higher pressure Hadley Circulation (in 1735) COLD HOT COLD Explains: Intertropical Convergence Zone (ITCZ) Wet Tropics Dry Poles But it has some problems. Saturation Vapor Pressure Amount of water vapor volume of air can hold. Determines when condensed phase H2O can exist Formation of condensed phase H2O often leads to removal by precipitation Relative humidity (%) = 100(PH2O/PH2O,SAT) Dew point: Temperature Td such that PH2O = PH2O,SAT(Td) Intertropical Convergence Zone (ITCZ) Surface warming by intense solar radiation leads to warm air rising, creating surface low pressure. Convergence and uplift leads to saturation/condensation Today’s ITCZ Moist Deep Convection—Where? divergence Questions 1. Subsidence of air leads to compression, which causes an air parcel to warm. This will lead to: a) rainy weather b) dry weather c) lower pressure at the surface 2. Large scale subsidence tends to occur near 30oN/S as a result of the Hadley circulation. This subsidence exacerbates air quality problems in cities like Los Angeles, Houston, Athens, Cairo, Shanghai, etc. a) True b) False Hadley Didn’t Know About Coriolis Effect Earth rotates from West to East (an Easterly direction) The equator is rotating with a larger velocity than higher latitudes Air (or any object) on Earth always has an easterly velocity component. Object moving northward from the equator has easterly velocity greater than the Earth at northern latitudes coriolis effect movie Coriolis Effect: Modifies Hadley Circulation Questions 1. Suppose Earth were a cylinder. Where would there be a coriolis effect? A B a) b) c) d) A only B only C only A, B, and C C 2. In the stratosphere over Antarctica during polar winter, air cools and descends causing air in the midlatitude stratosphere to head poleward. What direction does it end up going? Surface Winds In the tropics air flows towards the ITCZ, impacted by Coriolis effect and friction. These are the “trades” Subsidence leads to surface highs and divergence subsidence subsidence Mean Horizontal Transport Times 1-2 months 2 weeks 1-2 months 1 year Vertical Transport Importance to composition Buoyancy Stability and Instability Vertical Transport: Overview 1. Vertical transport critical for air quality and the vertical distribution of surface emitted species (CO2, PM, H2O, etc). 2. Determined by temperature differences between air parcels and their surroundings. LA Smog/Fog Cumulonimbus Vertical Transport: Buoyancy Buoyancy refers to the density of an object in a fluid, relative to the density of that fluid. PGF Fluid (f) Fg PGF object (ob) Fbuoyancy = PGF - Fg Fg If obj > fluid, Fgobj will be > PGF, and so object will sink. If obj < fluid, PGF > Fgobj and so object will rise. Vertical Transport: Buoyancy Key Points 1. Buoyant forces in atmosphere driven by temperature differences (which lead to density differences). 2. Solar heating and “latent heat” of condensation drive temperature differences between a parcel of air and the surrounding atmosphere. 3. Warmer air rises, but as it rises, it cools due to expansion. Colder air sinks, but as it sinks, it warms due to compression. 4. Must compare “parcel” T to that of “surrounding” atmosphere to know extent/likelihood of vertical mixing Adiabatic Lapse Rate Rising air parcel does expansion work on surroundings. Work done on surroundings causes loss of internal energy Internal energy of ideal gas directly related to T Stratopause ?? dT = 9.8 K/km dz DRY dT 6.5 K/km < < 9.8 K/km dz actual Tropopause Vertical Transport: Stability/Instability How do vertical motions get started and stopped? Conduction: air warmed by contact w/surface. Z Warm parcels become buoyant or are lifted mechanically to where they are buoyant. 0 km Compare Tparcel to TATM at a given (z) to determine sign of buoyancy ~ 2 km Tparcel follows dry adiabatic slope from expansion work Tatm T Slope of Tatm(z) greater than dry adiabatic lapse rate because of surface heating Vertical Transport: Stability/Instability dT dz > 9.8 K/km: UNSTABLE w.r.t. ATM vertical motion (well mixed) dT < 9.8 K/km: STABLE w.r.t. vertical dz ATM motion (vertical mixing suppressed) ~ 2 km 0 km Dry adiabatic slope from expansion work T -Slope greater than dry adiabatic lapse rate because of surface heatingUNSTABLE Temperature Structure and Air Quality Daily cycle of surface heating and cooling and the depth of the “well mixed” layer z Subsidence inversion MIDDAY Temperature inversions cap mixing depth IMPORTANT FOR 1 km POLLUTANT CONCENTRATIONS Mixing depth NIGHT 0 MORNING T NIGHT MORNING AFTERNOON Typical Timescales for Vertical Mixing tropopause 10 km 5 km 1 week 1 day months 10 years 2 km “planetary boundary layer” 0 km Question 1. If it only takes months for air at the surface to mix to the top of the troposphere (tropopause), why does it then take 10 years for air in the troposphere to cross into the stratosphere? 2. Due to respiration, CO2 is emitted into the atmosphere by plants and soil microbes throughout the night. At what time of day would you expect CO2 concentrations to maximize at the ground and why?