كيمياء الغلاف الجوي

علوم الغلاف الجوي [تص.]
	علم الأرصاد الجوية [تص.] طقس [تص.] أعاصير إستوائية [تص.]
	علم المناخ [تص.] مناخ [تص.] تغير مناخي [تص.]
	بوابة علوم الغلاف الجوي بوابة الطقس

Atmospheric chemistry is a branch of atmospheric science in which the chemistry of the Earth's atmosphere and that of other planets is studied.^[1] It is a multidisciplinary approach of research and draws on environmental chemistry, physics, meteorology, computer modeling, oceanography, geology and volcanology and other disciplines. Research is increasingly connected with other areas of study such as climatology.

The composition and chemistry of the Earth's atmosphere is of importance for several reasons, but primarily because of the interactions between the atmosphere and living organisms. The composition of the Earth's atmosphere changes as result of natural processes such as volcano emissions, lightning and bombardment by solar particles from corona. It has also been changed by human activity and some of these changes are harmful to human health, crops and ecosystems. Examples of problems which have been addressed by atmospheric chemistry include acid rain, ozone depletion, photochemical smog, greenhouse gases and global warming. Atmospheric chemists seek to understand the causes of these problems, and by obtaining a theoretical understanding of them, allow possible solutions to be tested and the effects of changes in government policy evaluated.

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تكوين الغلاف الجوي

Visualisation of composition by volume of Earth's atmosphere. Water vapour is not included as it is highly variable. Each tiny cube (such as the one representing krypton) has one millionth of the volume of the entire block. Data is from NASA Langley.

The composition of common nitrogen oxides in dry air vs. temperature

Chemical composition of atmosphere according to altitude.^[2] Axis: Altitude (km), Content of volume (%).

Average composition of dry atmosphere (mole fractions)
Gas	Dry air per NASA	Dry clean air near sea level (standard ISO 2533 - 1975)
Nitrogen, N₂	78.084%	78.084%
Oxygen, O₂^[3]	20.946%	20.946%
Minor constituents (mole fractions in ppm)
Argon, Ar	9340	9340
Carbon dioxide*^[a], CO₂	430	430
Neon, Ne	18.18	18.18
Helium, He	5.24	5.24
Methane^[a], CH₄	1.9	1.9
Krypton, Kr	1.14	1.14
Hydrogen, H₂	0.53	0.53
Nitrous oxide, N₂O		0.34
Xenon, Xe		0.087
Nitrogen dioxide, NO₂		up to 0.02
Ozone*, O₃, in summer		up to 0.07
Ozone*, O₃, in winter		up to 0.02
Sulphur dioxide*, SO₂		up to 1
Iodine*, I₂		0.01
Water
Water vapour*	Highly variable (about 0–3%); typically makes up about 1%
Notes
The mean molecular mass of dry air is 28.97 g/mol. *The content of the gas may undergo significant variations from time to time or from place to place. ^[a]The concentration of CO₂ and CH₄ vary by season and location.

Trace gas composition

Besides the more major components listed above, Earth's atmosphere also has many trace gas species that vary significantly depending on nearby sources and sinks. These trace gases can include compounds such as CFCs/HCFCs which are particularly damaging to the ozone layer, and H 2S which has a characteristic foul odor of rotten eggs and can be smelt in concentrations as low as 0.47 ppb. Some approximate amounts near the surface of some additional gases are listed below. In addition to gases, the atmosphere contains particulates as aerosol, which includes for example droplets, ice crystals, bacteria, and dust.

Composition (ppt by volume unless otherwise stated)
Gas	Clean continental, Seinfeld & Pandis (2016)^[4]	Simpson et al. (2010)^[5]
Carbon monoxide, CO	40-200 ppb ^p39	97 ppb
Nitric oxide, NO		16
Ethane, C₂H₆		781
Propane, C₃H₈		200
Isoprene, C₅H₈		311
Benzene, C₆H₆		11
Methanol, CH₃OH		1967
Ethanol, C₂H₅OH		75
Trichlorofluoromethane, CCl₃F	237 ^p41	252.7
Dichlorodifluoromethane, CCl₂F₂	530 ^p41	532.3
Chloromethane, CH₃Cl		503
Bromomethane, CH₃Br	9–10 ^p44	7.7
Iodomethane, CH₃I		0.36
Carbonyl sulfide, OCS	510 ^p26	413
Sulfur dioxide, SO₂	70–200 ^p26	102
Hydrogen sulfide, H₂S	15–340 ^p26
Carbon disulfide, CS₂	15–45 ^p26
Formaldehyde, H₂CO	9.1 ppb ^{p37, polluted}
Acetylene, C₂H₂	8.6 ppb ^{p37, polluted}
Ethene, C₂H₄	11.2 ppb ^{p37, polluted}	20
Sulfur hexafluoride, SF₆	7.3 ^p41
Carbon tetrafluoride, CF₄	79 ^p41
Total gaseous mercury, Hg	0.209 ^p55

تاريخ

Schematic of chemical and transport processes related to atmospheric composition

The first scientific studies of atmospheric composition began in the 18th century, as chemists such as Joseph Priestley, Antoine Lavoisier and Henry Cavendish made the first measurements of the composition of the atmosphere.^{[بحاجة لمصدر]}

In the late 19th and early 20th centuries interest shifted towards trace constituents with very small concentrations. One particularly important discovery for atmospheric chemistry was the discovery of ozone by Christian Friedrich Schönbein in 1840.^[6]

In the 20th century atmospheric science moved on from studying the composition of air to a consideration of how the concentrations of trace gases in the atmosphere have changed over time and the chemical processes which create and destroy compounds in the air. Two particularly important examples of this were the explanation by Sydney Chapman and Gordon Dobson of how the ozone layer is created and maintained, and the explanation of photochemical smog by Arie Jan Haagen-Smit. Further studies on ozone issues led to the 1995 Nobel Prize in Chemistry award shared between Paul Crutzen, Mario Molina and Frank Sherwood Rowland.^[7]

In the 21st century the focus is now shifting again. Atmospheric chemistry is increasingly studied as one part of the Earth system. Instead of concentrating on atmospheric chemistry in isolation the focus is now on seeing it as one part of a single system with the rest of the atmosphere, biosphere and geosphere. An especially important driver for this is the links between chemistry and climate such as the effects of changing climate on the recovery of the ozone hole and vice versa but also interaction of the composition of the atmosphere with the oceans and terrestrial ecosystems.^{[بحاجة لمصدر]}

Carbon dioxide in Earth's atmosphere if half of anthropogenic CO₂ emissions^[8]^[9] are not absorbed
(NASA simulation; 9 November 2015)

Nitrogen dioxide 2014 - global air quality levels
(released 14 December 2015)^[10]

المنهاج

Observations, lab measurements, and modeling are the three central elements in atmospheric chemistry. Progress in atmospheric chemistry is often driven by the interactions between these components and they form an integrated whole. For example, observations may tell us that more of a chemical compound exists than previously thought possible. This will stimulate new modelling and laboratory studies which will increase our scientific understanding to a point where the observations can be explained.^{[بحاجة لمصدر]}

الرصد

Observations of atmospheric chemistry are essential to our understanding. Routine observations of chemical composition tell us about changes in atmospheric composition over time. One important example of this is the Keeling Curve - a series of measurements from 1958 to today which show a steady rise in of the concentration of carbon dioxide (see also ongoing measurements of atmospheric CO₂). Observations of atmospheric chemistry are made in observatories such as that on Mauna Loa and on mobile platforms such as aircraft (e.g. the UK's Facility for Airborne Atmospheric Measurements), ships and balloons. Observations of atmospheric composition are increasingly made by satellites with important instruments such as GOME and MOPITT giving a global picture of air pollution and chemistry. Surface observations have the advantage that they provide long term records at high time resolution but are limited in the vertical and horizontal space they provide observations from. Some surface based instruments e.g. LIDAR can provide concentration profiles of chemical compounds and aerosol but are still restricted in the horizontal region they can cover. Many observations are available on line in Atmospheric Chemistry Observational Databases.^{[بحاجة لمصدر]}

الدراسات المعملية

Measurements made in the laboratory are essential to understanding the sources and sinks of pollutants and naturally occurring compounds. These experiments are performed in controlled environments that allow for the individual evaluation of specific chemical reactions or the assessment of properties of a particular atmospheric constituent.^[11] Types of analysis that are of interest includes both those on gas-phase reactions, as well as heterogeneous reactions that are relevant to the formation and growth of aerosols. Also of high importance is the study of atmospheric photochemistry which quantifies how the rate in which molecules are split apart by sunlight and what resulting products are. In addition, thermodynamic data such as Henry's law coefficients can also be obtained.^{[بحاجة لمصدر]}

النمذجة

In order to synthesize and test theoretical understanding of atmospheric chemistry, computer models (such as chemical transport models) are used. Numerical models solve the differential equations governing the concentrations of chemicals in the atmosphere. They can be very simple or very complicated. One common trade off in numerical models is between the number of chemical compounds and chemical reactions modeled versus the representation of transport and mixing in the atmosphere. For example, a box model might include hundreds or even thousands of chemical reactions but will only have a very crude representation of mixing in the atmosphere. In contrast, 3D models represent many of the physical processes of the atmosphere but due to constraints on computer resources will have far fewer chemical reactions and compounds. Models can be used to interpret observations, test understanding of chemical reactions and predict future concentrations of chemical compounds in the atmosphere. These models can be global (simulating the entire earth) or they can be regional (focused on only a specific region). The trade-off between the two approaches is their resolution as well as the amount of detail they can provide; global models usually have lower horizontal resolution and represent less complex chemical mechanisms but they simulate a larger area, while regional models do not simulate the entire globe but focus on one area with higher resolution and more detail. One important current trend is for atmospheric chemistry modules to become one part of earth system models in which the links between climate, atmospheric composition and the biosphere can be studied. These types of models allow the coupling of different compartments of the earth, such as the atmosphere, the biosphere and the hydrosphere; allowing the users to analyze the complicated interactions between them.

Some models are constructed by automatic code generators (e.g. Autochem or Kinetic PreProcessor). In this approach a set of constituents are chosen and the automatic code generator will then select the reactions involving those constituents from a set of reaction databases. Once the reactions have been chosen the ordinary differential equations that describe their time evolution can be automatically constructed.