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Aerosols. What is the mean diameter of the particles?"  The answer to this question changes with your point of view.  What size particles carry the.

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Presentation on theme: "Aerosols. What is the mean diameter of the particles?"  The answer to this question changes with your point of view.  What size particles carry the."— Presentation transcript:

1 Aerosols

2 What is the mean diameter of the particles?"  The answer to this question changes with your point of view.  What size particles carry the most mass? (Biogeochemical cycles)  What size particles cover the largest surface area? (visibility)  What is the size of the most abundant particles? (cloud microphysics)

3 Aerosol Distributions Number  cloud formation Surface  visibility Volume  mass Mass & Number  human health

4 Number distribution function  The number of particles with diameter between D p and D p + dD p in a cm 3 f n (D p ) dD p (particles cm -3 /  m)  The total number of particles, N: N =  f n (D p ) dD p (particles cm -3 )

5 Surface Area Distribution Function  The surface area of particles in a size range per cm 3 of air f s (D p )dD p =  D p 2 f n (D p ) (  m 2  m -1 cm -3  The total surface area of the particles, S, is given by the integral over all diameters: S =  f s (D p ) dD p =  D p 2 f n (D p ) dD p (  m 2 cm -3 )

6 Volume Distribution Function  The Volume distribution function can be defined f v (D p ) dD p = {  /6} D p 3 f n (D p ) (  m 3  m -1 cm -3 )  So the total volume occupied can be written V =  f v (D p ) dD p =   /6 D p 3 f n (D p ) dD p (  m 3 cm -3 )

7 Log Normal  Distributions based on log D p can be defined n(log D p )dlogD p is the number of particles in one cm 3 with diameter from D p to D p + log D p. The total number is: N =  n(log D p ) d(logD p ) (particles cm -3 ) n (log D p ) = {dN} / {N dlogD p } n s (log D p ) = {dS} / {S dlogD p } n v (log D p ) = {dV} / {V dlogD p } This is the common notation for expressing the variation in particle number, surface area or volume with the log of the diameter.

8 8 Aerosol particle size distribution

9 Distributions which look like Gaussian distributions (“normal” distributions) when plotted with a logarithmic x-axis are called lognormal This size distribution has 2 lognormal modes

10 TYPICAL U.S. AEROSOL SIZE DISTRIBUTIONS Fresh urban Aged urban rural remote Warneck [1999]

11 SAMPLE AEROSOL SIZE DISTRIBUTION (MARINE AIR) Sea salt Sulfate (natural)

12 COMPOSITION OF PM2.5 (NARSTO PM ASSESSMENT)

13 Aerosols: Visibility Washington, DC

14 Light Extinction  I/I = e (-b  X) I0I0 I absorption scattering XX Intensity Extinction Coefficientb (in a few more slides)

15 EPA REGIONAL HAZE RULE: FEDERAL CLASS I AREAS TO RETURN TO “NATURAL” VISIBILITY LEVELS BY 2064  Acadia National Park clean day moderately polluted day http://www.hazecam.net/ …will require essentially total elimination of anthropogenic aerosols!

16 Radiation and fine particles

17 Atmospheric Visibility Atmospheric Visibility (absorption & scattering) 1.Residual 2.Scattered away 3.Scattered into 4.Airlight

18 b ext = b gas + b particles b ext = b abs + b scatt b abs (gases) = Beer's Law absorption b scatt (gases) = Rayleigh Scattering b abs (particles) = Usually < 10% of extinction b scatt (particles) = Mie Scattering = (b sp ) Extinction Coefficient

19 Visibility  The ultimate limit in a very clean atmosphere is Rayleigh scattering  Mie scattering usually dominates.  The range of b sp is 10 -5 m -1 to 10 -3 m -1.

20 Single scattering albedo   is a measure of the fraction of aerosol extinction caused by scattering:  = b sp /(b sp + b ap )

21 Optical Properties of Small Particles m = n + ik m = complex index of refraction n = scattering (real part) k = absorption (imaginary part) The real part of the index of refraction is only a weak function of wavelength, while the imaginary part, ik, depends strongly on wavelength.

22 Refractive indicies of aerosol particles at = 589 nm m = n + ik Substancenk Water1.33310 -8 Ice1.30910 -8 NaCl1.5440 H 2 SO 4 1.4260 NH 4 HSO 4 1.4730 (NH 4 ) 2 SO41.5210 SiO 2 1.550 Black Carbon (soot)1.960.66 Mineral dust~1.53~0.006

23 The scattering cross section is the product of the mass loading, and the surface area per unit mass; note the ln of 0.02 is about -3.9, thus Visibility ≈ 3.9(b sp ) -1 b sp = S  m Where b sp is the scattering coefficient in units of m -1 m is the mass loading in units of g m -3 S is the surface area per unit mass in units of m 2 g -1 For sulfate particles, S is about 3.2 m 2 g -1 where the humidity is less than about 70%; for other materials it can be greater. Visibility = 3.9/(3.2 m) = 1.2 /(m) Scattering Cross Section

24 Example: Visibility improvement during the 2003 North American Blackout Normal conditions over Eastern US during an air pollution episode: b sp ≈ 120 Mm -1 = 1.2 x 10 -4 m -1 at 550 nm b ap = 0.8 x 10 -5 m -1 b ext = 1.28 x 10 -4 m -1 Visual Range ≈ 3.9/b ext = 30 km During blackout b sp = 40 Mm -1 = 0.4 x 10 -4 m -1 b ap = 1.2 x 10 -5 m -1 b ext = 0.52 x 10 -4 m -1 Visual Range = 3.9/b ext = 75 km

25 Example: Visibility improvement during the 2003 North American Blackout Single scattering albedo, , normal = 1.20/1.28 = 0.94 Blackout = 0.4/0.52 = 0.77 With the sulfate from power plants missing, and the soot from diesel engines remaining the visual range is up, but the single scattering albedo is down. Ozone production inhibited. See: Marufu et al., Geophys Res. Lett., 2004.

26 Extinction Coefficient as a PM2.5 Surrogate PM 2.5 = 7.6  g/m 3 PM 2.5 = 21.7  g/m 3 PM 2.5 = 65.3  g/m 3 Glacier National Park images are adapted from Malm, An Introduction to Visibility (1999) http://webcam.srs.fs.fed.us/intropdf.htm

27 ANNUAL MEAN PARTICULATE MATTER (PM) CONCENTRATIONS AT U.S. SITES, 1995-2000 NARSTO PM Assessment, 2003 PM10 (particles > 10  m)PM2.5 (particles > 2.5  m) Red circles indicate violations of national air quality standard: 50  g m -3 for PM10 15  g m -3 for PM2.5

28 AEROSOL OPTICAL DEPTH (GLOBAL MODEL) Annual mean

29 AEROSOL OBSERVATIONS FROM SPACE Biomass fire haze in central America (4/30/03) Fire locations in red Modis.gsfc.nasa.gov

30 BLACK CARBON EMISSIONS Chin et al. [2000] DIESEL DOMESTIC COAL BURNING BIOMASS BURNING

31 RADIATIVE FORCING OF CLIMATE 1750-PRESENT “Kyoto also failed to address two major pollutants that have an impact on warming: black soot and tropospheric ozone. Both are proven health hazards. Reducing both would not only address climate change, but also dramatically improve people's health.” (George W. Bush, June 11 2001 Rose Garden speech) IPCC [2001]

32 ASIAN DUST INFLUENCE IN UNITED STATES Dust observations from U.S. IMPROVE network April 16, 2001 Asian dust in western U.S. April 22, 2001 Asian dust in southeastern U.S. Glen Canyon, AZ Clear day April 16, 2001: Asian dust! 0 2 4 6 8  g m -3

33 LONGITUDE ALTITUDE (km) 100E150E150W 100W TRANSPACIFIC TRANSPORT OF ASIAN DUST PLUMES Subsidence over western U.S. Source region (inner Asia) Asian plumes over Pacific GEOS-CHEM Longitude cross-section at 40N, 16 April, 2001 0 5 10 ASIA UNITED STATES T.D. Fairlie, Harvard

34 Aerosols in the Atmosphere: Abundance and size  Aerosol concentration is highly variable in space and time. Concentrations are usually highest near the ground and near sources.  A concentration of 10 5 cm -3 is typical of polluted air near the ground, but values may range from 2 orders of magnitude higher in very polluted regions to several lower in very clean air.  Radii range from ~ 10 -7 cm for the for small ions to more than 10 µm (10 -3 cm) for the largest salt and dust particles.  Small ions play almost no role in atmospheric condensation because of the very high supersaturations required for condensation.  The largest particles, however, are only able to remain airborne for a limited time

35 1. Condensation and sublimation of of vapors and the formation of smokes in natural and man-made combustion. 2. Reactions between trace gases in the atmosphere through the action of heat, radiation, or humidity. 3. The mechanical disruption and dispersal of matter at the earth’s surface, either as sea spray over the oceans, or as mineral dusts over the continents. 4.Coagulation of nuclei which tends to produce larger particles of mixed constitution Summary:Origins of Atmospheric Aerosols

36 Cloud Condensation Nuclei - CCN  Comprises a small fraction of the total aerosol population  Sea salt is the predominant constituent of CCN with D > 1µm  For 0.1 µm < D < 1 µm, the main component is thought to be sulfate, which may be present as sulfuric acid, ammonium sulfate, or from phytoplankton produced dimethylsulfide (see Charlson et al., Nature, 326, 655-661).

37 37 INDOEX, 1999 INDOEX: Indian Ocean Experiment

38 38 Mean Aerosol Optical Depth over INDOEX region from Dec 2001 to May 2003 from MODIS (Ramanathan & Ramana, Environ. Managers, Dec. 2003). + RV Ronald Brown INDOEX

39 39 INDOEX From Ramanathan 2001 0 to 3 km layer

40 40 NOAA R/V Ronald Brown

41 41 Air Flow During INDOEX 1999

42 42 Field data showing the high variability of aerosol light absorption coefficient with latitude and longitude, measured by NOAA/PMEL scientists aboard the NOAA Research Vessel Ron Brown during the Aerosols 99 and INDOEX (Indian Ocean Experiment) cruises. The aerosol light absorption coefficient is presented in all figures in units of Mm -1. Measurements are made at a wavelength of 550nm. (Courtesy of P.Quinn and T. Bates, NOAA/PMEL.)

43 Summary of Aerosol Physics  How big are atmospheric particles depends on which effect interests you.  CCN – number (r < 0.1  m)  Radiative transfer & health – surface area (0.1 < r < 1.0  m)  Biogeochemical cycles – mass (r > 0.5  m).  Composition varies with size.  Single scattering albedo and visibility


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