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Outline of air pollution dispersion

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The following outline is provided as an overview of and topical guide to air pollution dispersion: In environmental science, air pollution dispersion is the distribution of air pollution into the atmosphere. Air pollution is the introduction of particulates, biological molecules, or other harmful materials into Earth's atmosphere, causing disease, death to humans, damage to other living organisms such as food crops, and the natural or built environment. Air pollution may come from anthropogenic or natural sources. Dispersion refers to what happens to the pollution during and after its introduction; understanding this may help in identifying and controlling it.

Air pollution dispersion has become the focus of environmental conservationists and governmental environmental protection agencies (local, state, province and national) of many countries (which have adopted and used much of the terminology of this field in their laws and regulations) regarding air pollution control.

Air pollution emission plumes

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Visualization of a buoyant Gaussian air pollutant dispersion plume

Air pollution emission plume – flow of pollutant in the form of vapor or smoke released into the air. Plumes are of considerable importance in the atmospheric dispersion modelling of air pollution. There are three primary types of air pollution emission plumes:

  • Buoyant plumes – Plumes which are lighter than air because they are at a higher temperature and lower density than the ambient air which surrounds them, or because they are at about the same temperature as the ambient air but have a lower molecular weight and hence lower density than the ambient air. For example, the emissions from the flue gas stacks of industrial furnaces are buoyant because they are considerably warmer and less dense than the ambient air. As another example, an emission plume of methane gas at ambient air temperatures is buoyant because methane has a lower molecular weight than the ambient air.
  • Dense gas plumes – Plumes which are heavier than air because they have a higher density than the surrounding ambient air. A plume may have a higher density than air because it has a higher molecular weight than air (for example, a plume of carbon dioxide). A plume may also have a higher density than air if the plume is at a much lower temperature than the air. For example, a plume of evaporated gaseous methane from an accidental release of liquefied natural gas (LNG) may be as cold as −161 °C (−258 °F).
  • Passive or neutral plumes – Plumes which are neither lighter or heavier than air.

Air pollution dispersion models

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There are five types of air pollution dispersion models, as well as some hybrids of the five types:[1]

  • Box model – The box model is the simplest of the model types.[2] It assumes the airshed (i.e., a given volume of atmospheric air in a geographical region) is in the shape of a box. It also assumes that the air pollutants inside the box are homogeneously distributed and uses that assumption to estimate the average pollutant concentrations anywhere within the airshed. Although useful, this model is very limited in its ability to accurately predict dispersion of air pollutants over an airshed because the assumption of homogeneous pollutant distribution is much too simple.
  • Gaussian model – The Gaussian model is perhaps the oldest (circa 1936)[3] and perhaps the most commonly used model type. It assumes that the air pollutant dispersion has a Gaussian distribution, meaning that the pollutant distribution has a normal probability distribution. Gaussian models are most often used for predicting the dispersion of continuous, buoyant air pollution plumes originating from ground-level or elevated sources. Gaussian models may also be used for predicting the dispersion of non-continuous air pollution plumes (called puff models). The primary algorithm used in Gaussian modeling is the Generalized Dispersion Equation For A Continuous Point-Source Plume.[4][5]
  • Lagrangian model – a Lagrangian dispersion model mathematically follows pollution plume parcels (also called particles) as the parcels move in the atmosphere and they model the motion of the parcels as a random walk process. The Lagrangian model then calculates the air pollution dispersion by computing the statistics of the trajectories of a large number of the pollution plume parcels. A Lagrangian model uses a moving frame of reference[6] as the parcels move from their initial location. It is said that an observer of a Lagrangian model follows along with the plume.
  • Eulerian model – an Eulerian dispersion model is similar to a Lagrangian model in that it also tracks the movement of a large number of pollution plume parcels as they move from their initial location. The most important difference between the two models is that the Eulerian model uses a fixed three-dimensional Cartesian grid[6] as a frame of reference rather than a moving frame of reference. It is said that an observer of an Eulerian model watches the plume go by.
  • Dense gas model – Dense gas models are models that simulate the dispersion of dense gas pollution plumes (i.e., pollution plumes that are heavier than air). The three most commonly used [citation needed] [dubious – discuss] dense gas models are:

Air pollutant emission

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Air pollution emission source
  • Types of air pollutant emission sources – named for their characteristics
    • Sources, by shape – there are four basic shapes which an emission source may have. They are:
      • Point source – single, identifiable source of air pollutant emissions (for example, the emissions from a combustion furnace flue gas stack). Point sources are also characterized as being either elevated or at ground-level. A point source has no geometric dimensions.
      • Line source – one-dimensional source of air pollutant emissions (for example, the emissions from the vehicular traffic on a roadway).
      • Area source – two-dimensional source of diffuse air pollutant emissions (for example, the emissions from a forest fire, a landfill or the evaporated vapors from a large spill of volatile liquid).
      • Volume source – three-dimensional source of diffuse air pollutant emissions. Essentially, it is an area source with a third (height) dimension (for example, the fugitive gaseous emissions from piping flanges, valves and other equipment at various heights within industrial facilities such as oil refineries and petrochemical plants). Another example would be the emissions from an automobile paint shop with multiple roof vents or multiple open windows.
    • Sources, by motion
    • Sources, by urbanization level – whether the source is within a city or not is relevant in that urban areas constitute a so-called heat island and the heat rising from an urban area causes the atmosphere above an urban area to be more turbulent than the atmosphere above a rural area
      • Urban source – emission is in an urban area
      • Rural source – emission is in a rural area
    • Sources, by elevation
      • Surface or ground-level source
      • Near surface source
      • Elevated source
    • Sources, by duration
      • Puff or intermittent source – short term sources (for example, many accidental emission releases are short term puffs)
      • Continuous source – long term source (for example, most flue gas stack emissions are continuous)

Characterization of atmospheric turbulence

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Effect of turbulence on dispersion – turbulence increases the entrainment and mixing of unpolluted air into the plume and thereby acts to reduce the concentration of pollutants in the plume (i.e., enhances the plume dispersion). It is therefore important to categorize the amount of atmospheric turbulence present at any given time. This type of dispersion is scale dependent.[10] Such that, for flows where the cloud of pollutant is smaller than the largest eddies present, there will be mixing. There is no limit on the size on mixing motions in the atmosphere and therefore bigger clouds will experience larger and stronger mixing motions. And hence, this type of dispersion is scale dependent.

The Pasquill atmospheric stability classes

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Pasquill atmospheric stability classes – oldest and, for a great many years, the most commonly used method of categorizing the amount of atmospheric turbulence present was the method developed by Pasquill in 1961.[11] He categorized the atmospheric turbulence into six stability classes named A, B, C, D, E and F with class A being the most unstable or most turbulent class, and class F the most stable or least turbulent class.

  • Table 1 lists the six classes
  • Table 2 provides the meteorological conditions that define each class. The stability classes demonstrate a few key ideas. Solar radiation increases atmospheric instability through warming of the Earth's surface so that warm air is below cooler (and therefore denser) air promoting vertical mixing. Clear nights push conditions toward stable as the ground cools faster establishing more stable conditions and inversions. Wind increases vertical mixing, breaking down any type of stratification and pushing the stability class towards neutral (D).[12]

Table 1: The Pasquill stability classes

Stability class Definition   Stability class Definition
A very unstable   D neutral
B unstable   E slightly stable
C slightly unstable   F stable

Table 2: Meteorological conditions that define the Pasquill stability classes

Surface windspeed Daytime incoming solar radiation Nighttime cloud cover
m/s mi/h Strong Moderate Slight > 50% < 50%
< 2 < 5 A A – B B E F
2 – 3 5 – 7 A – B B C E F
3 – 5 7 – 11 B B – C C D E
5 – 6 11 – 13 C C – D D D D
> 6 > 13 C D D D D
Note: Class D applies to heavily overcast skies, at any windspeed day or night

Incoming solar radiation is based on the following: strong (> 700 W m−2), moderate (350–700 W m−2), slight (< 350 W m−2)[13]

Other parameters that can define the stability class

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The stability class can be defined also by using the

Advanced methods of categorizing atmospheric turbulence

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Advanced air pollution dispersion models – they do not categorize atmospheric turbulence by using the simple meteorological parameters commonly used in defining the six Pasquill classes as shown in Table 2 above. The more advanced models use some form of Monin–Obukhov similarity theory. Some examples include:

Miscellaneous other terminology

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(Work on this section is continuously in progress)
  • Building effects or downwash: When an air pollution plume flows over nearby buildings or other structures, turbulent eddies are formed in the downwind side of the building. Those eddies cause a plume from a stack source located within about five times the height of a nearby building or structure to be forced down to the ground much sooner than it would if a building or structure were not present. The effect can greatly increase the resulting near-by ground-level pollutant concentrations downstream of the building or structure. If the pollutants in the plume are subject to depletion by contact with the ground (particulates, for example), the concentration increase just downstream of the building or structure will decrease the concentrations further downstream.
  • Deposition of the pollution plume components to the underlying surface can be defined as either dry or wet deposition:
    • Dry deposition is the removal of gaseous or particulate material from the pollution plume by contact with the ground surface or vegetation (or even water surfaces) through transfer processes such as absorption and gravitational sedimentation. This may be calculated by means of a deposition velocity, which is related to the resistance of the underlying surface to the transfer.
    • Wet deposition is the removal of pollution plume components by the action of rain. The wet deposition of radionuclides in a pollution plume by a burst of rain often forms so called hot spots of radioactivity on the underlying surface.
  • Inversion layers:[5] Normally, the air near the Earth's surface is warmer than the air above it because the atmosphere is heated from below as solar radiation warms the Earth's surface, which in turn then warms the layer of the atmosphere directly above it. Thus, the atmospheric temperature normally decreases with increasing altitude. However, under certain meteorological conditions, atmospheric layers may form in which the temperature increases with increasing altitude. Such layers are called inversion layers. When such a layer forms at the Earth's surface, it is called a surface inversion. When an inversion layer forms at some distance above the earth, it is called an inversion aloft (sometimes referred to as a capping inversion). The air within an inversion aloft is very stable with very little vertical motion. Any rising parcel of air within the inversion soon expands, thereby adiabatically cooling to a lower temperature than the surrounding air and the parcel stops rising. Any sinking parcel soon compresses adiabatically to a higher temperature than the surrounding air and the parcel stops sinking. Thus, any air pollution plume that enters an inversion aloft will undergo very little vertical mixing unless it has sufficient momentum to completely pass through the inversion aloft. That is one reason why an inversion aloft is sometimes called a capping inversion.
  • Mixing height:[5] When an inversion aloft is formed, the atmospheric layer between the Earth's surface and the bottom of the inversion aloft is known as the mixing layer and the distance between the Earth's surface and the bottom of inversion aloft is known as the mixing height. Any air pollution plume dispersing beneath an inversion aloft will be limited in vertical mixing to that which occurs beneath the bottom of the inversion aloft (sometimes called the lid). Even if the pollution plume penetrates the inversion, it will not undergo any further significant vertical mixing. As for a pollution plume passing completely through an inversion layer aloft, that rarely occurs unless the pollution plume's source stack is very tall and the inversion lid is fairly low.

See also

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Air pollution dispersion models

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Others

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References

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  1. ^ List of atmospheric dispersion models
  2. ^ Air Pollution Dispersion: Ventilation Factor by Dr. Nolan Atkins, Lyndon State College
  3. ^ Bosanquet, C.H. and Pearson, J.L. (1936).The spread of smoke and gases from chimney, Trans. Faraday Soc., 32:1249.
  4. ^ Atmospheric Dispersion Modeling
  5. ^ a b c Beychok, Milton R. (2005). Fundamentals Of Stack Gas Dispersion (4th ed.). author-published. ISBN 0-9644588-0-2. (Chapter 8, page 124)
  6. ^ a b Features of Dispersion Models Archived 2012-12-18 at archive.today publication of the European Union Joint Research Centre (JRC)
  7. ^ DEGADIS Technical Manual and User's Guide (US EPA's download website)
  8. ^ UCRL-MA-105607, User's Manual For Slab: An Atmospheric Dispersion Model For Denser-Than-Air Releases, Donald Ermak, June 1990.
  9. ^ "HEGADIS Technical Reference Manual" (PDF).
  10. ^ Walton, John (April 1973). "Scale-Dependent Diffusion". Journal of Applied Meteorology. 12 (3): 548. Bibcode:1973JApMe..12..547W. doi:10.1175/1520-0450(1973)012<0547:sdd>2.0.co;2.
  11. ^ Pasquill, F. (1961). The estimation of the dispersion of windborne material, The Meteorological Magazine, vol 90, No. 1063, pp 33-49.
  12. ^ Pasquill, F. (February 1961). "The estimation of the dispersion of windborne material". Meteorological Magazine. 90: 33–49.
  13. ^ Seinfeld, John (2006). Atmospheric Chemistry and Physics: From Air Pollution to Climate Change. Hoboken, New Jersey: John Wiley & Sons, Inc. p. 750. ISBN 978-0-471-72018-8.
  14. ^ a b "Pasquill Stability Classes". NOAA.
  15. ^ a b Sedefian, Leon; Bennett, Edward (1980). "A comparison of turbulence classification schemes". Atmospheric Environment. 14 (7): 741–750. Bibcode:1980AtmEn..14..741S. doi:10.1016/0004-6981(80)90128-6.
  16. ^ [1][dead link‍]
  17. ^ "AERMOD:Description of Model Formulation" (PDF). 13 July 2016.
  18. ^ ADMS 4 Description of the model by the developers, Cambridge Environmental Research Consultants.

Further reading

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