Outline of air pollution dispersion explained

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

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:

Air pollution dispersion models

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

Air pollutant emission

Characterization of atmospheric turbulence

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

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: The Pasquill stability classes

width=23%"Stability class Definition  Stability class Definition
Avery unstable   Dneutral
Bunstable   Eslightly stable
Cslightly unstable  Fstable

Table 2: Meteorological conditions that define the Pasquill stability classes

Surface windspeedDaytime incoming solar radiationNighttime cloud cover
m/s mi/h Strong Moderate Slight> 50%< 50%
< 2< 5AA – B BEF
2 – 35 – 7A – B BCEF
3 – 57 – 11B B – CC DE
5 – 611 – 13C C – D DDD
> 6> 13C D DDD
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

The stability class can be defined also by using the

Advanced methods of categorizing atmospheric turbulence

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

(Work on this section is continuously in progress)

[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.

See also

Air pollution dispersion models

Others

Further reading

External links

Notes and References

  1. [List of atmospheric dispersion models]
  2. http://apollo.lsc.vsc.edu/classes/met130/notes/chapter18/dispersion_intro.html Air Pollution Dispersion: Ventilation Factor
  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|Atmospheric Dispersion Modeling]
  5. Book: Beychok, Milton R.. Fundamentals Of Stack Gas Dispersion. 4th. author-published. 2005. 0-9644588-0-2. Fundamentals Of Stack Gas Dispersion. (Chapter 8, page 124)
  6. http://rem.jrc.ec.europa.eu/etex/37.htm Features of Dispersion Models
  7. http://www.epa.gov/scram001/dispersion_alt.htm DEGADIS Technical Manual and User's Guide
  8. http://www.epa.gov/scram001/models/nonepa/SLAB.PDF UCRL-MA-105607, User's Manual For Slab: An Atmospheric Dispersion Model For Denser-Than-Air Releases
  9. Web site: HEGADIS Technical Reference Manual.
  10. Walton. John. April 1973. Scale-Dependent Diffusion. Journal of Applied Meteorology. 12. 3. 548. 10.1175/1520-0450(1973)012<0547:sdd>2.0.co;2. 1973JApMe..12..547W . free.
  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. Book: Seinfeld, John. Atmospheric Chemistry and Physics: From Air Pollution to Climate Change. John Wiley & Sons, Inc.. 2006. 978-0-471-72018-8. Hoboken, New Jersey. 750.
  14. Web site: Pasquill Stability Classes. NOAA.
  15. 10.1016/0004-6981(80)90128-6. A comparison of turbulence classification schemes. Atmospheric Environment . 14. 7. 741–750. Leon. Sedefian. Edward. Bennett. 1980. 1980AtmEn..14..741S.
  16. https://ac.els-cdn.com/0004698179902609/1-s2.0-0004698179902609-main.pdf?_tid=0195b1c1-7a65-4f00-b5e1-f3e388a3a2fa&acdnat=1528110370_85643c66e9905b407badb6a571a8a980
  17. Web site: AERMOD:Description of Model Formulation. 13 July 2016 .
  18. http://www.cerc.co.uk/environmental-software/ADMS-model.html ADMS 4