Jump to content

Atmospheric chemistry: Difference between revisions

From Wikipedia, the free encyclopedia
Content deleted Content added
allow free table with to avoid whitespace
Edited the tables (for a simpler and cleaner view), removed a few dead links in the further reading section, added citations in the models section, and added a brief overview of the applications in the methodology.
(21 intermediate revisions by 3 users not shown)
Line 2: Line 2:
{{about|field of academic study|composition of the Earth's atmosphere|Atmosphere of Earth}}
{{about|field of academic study|composition of the Earth's atmosphere|Atmosphere of Earth}}
{{Atmospheric sciences}}
{{Atmospheric sciences}}
{{Weather}}
'''Atmospheric chemistry''' is a branch of [[atmospheric science]] in which the [[chemistry]] of the [[Atmosphere of Earth|Earth's atmosphere]] and that of other planets is studied.<ref>{{Cite web |title=Atmospheric chemistry - Latest research and news {{!}} Nature |url=https://www.nature.com/subjects/atmospheric-chemistry |access-date=2022-10-06 |website=www.nature.com}}</ref> 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]].
'''Atmospheric chemistry''' is a branch of [[atmospheric science]] that studies the [[chemistry]] of the [[Atmosphere of Earth|Earth's atmosphere]] and that of other planets. This [[multidisciplinary approach]] of research draws on [[environmental chemistry]], [[physics]], [[meteorology]], [[computer modeling]], [[oceanography]], [[geology]] and [[volcanology]], [[climatology]] and other disciplines to understand both natural and human-induced changes in atmospheric composition. Key areas of research include the behavior of trace gasses, the formation of pollutants, and the role of aerosols and greenhouse gasses. Through a combination of observations, laboratory experiments, and computer modeling, atmospheric chemists investigate the causes and consequences of atmospheric changes.


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 [[solar corona|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 gas]]es 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.
The composition and chemistry of the Earth's atmosphere is important for several reasons, but primarily because of the interactions between the atmosphere and [[living organisms]]. Natural processes such as [[volcano]] emissions, [[lightning]] and bombardment by solar particles from [[Solar corona|corona]] changes the composition of the Earth's atmosphere. It has also been changed by human activity and some of these changes are harmful to human health, crops and ecosystems. Examples of problems addressed in atmospheric chemistry include [[acid rain]], [[ozone depletion]], [[photochemical smog]], [[Greenhouse gas|greenhouse gasses]] and [[global warming]]. Atmospheric chemists work to understand the causes of these problems. By developing a theoretical understanding, they can test potential solutions and evaluate the effects of changes in government policy.


== Atmospheric composition ==
== Atmospheric composition ==
[[Image:Atmospheric composition Langley.svg|thumb|upright=1.3|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 [http://www.nasa.gov/centers/langley/pdf/245893main_MeteorologyTeacherRes-Ch2.r4.pdf NASA Langley].]] [[File:Dry Air NOx Composition vs Temperature.svg|thumb|The composition of common [[nitrogen oxide]]s in [[Atmosphere of Earth|dry air]] vs. [[temperature]]]]
[[Image:Atmospheric composition Langley.svg|thumb|upright=1.35 |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 [http://www.nasa.gov/centers/langley/pdf/245893main_MeteorologyTeacherRes-Ch2.r4.pdf NASA Langley].]]
[[File:Dry Air NOx Composition vs Temperature.svg|thumb |upright=1.15|The composition of common [[nitrogen oxide]]s in [[Atmosphere of Earth|dry air]] vs. [[temperature]]]]
[[File:Chemical composition of atmosphere accordig to altitude.png|thumb|Chemical composition of atmosphere according to [[altitude]].<ref name="composition-altitude">{{cite web |last=Cairns |first=Iver |author-link= |title=Earth's Atmosphere |url=http://www.physics.usyd.edu.au/~cairns/teaching/lecture16/node2.html |date=23 September 1999 |work=[[The University of Sydney]] |access-date=7 April 2021 }}</ref> Axis: Altitude (km), Content of volume (%).]]
[[File:Chemical composition of atmosphere accordig to altitude.png |thumb|upright=1.15|Chemical composition of atmosphere according to [[altitude]].<ref name="composition-altitude">{{cite web |last=Cairns |first=Iver |author-link= |title=Earth's Atmosphere |url=http://www.physics.usyd.edu.au/~cairns/teaching/lecture16/node2.html |date=23 September 1999 |work=[[The University of Sydney]] |access-date=7 April 2021 }}</ref> Axis: Altitude (km), Content of volume (%).]]


{| class="wikitable"
{| class="wikitable"
! colspan=3 | Average composition of dry atmosphere ([[mole fraction]]s)
! colspan="2" | '''Average Composition of Dry Atmosphere ([[Mole fraction|mole fractions]])'''
|-
|-
| '''Gas'''
| '''Gas'''
| '''Dry air per [http://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html NASA]'''
| '''Dry air per [http://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html NASA]'''
| '''Dry clean air near sea level<br>(standard ISO 2533 - 1975)'''
|-
|-
| [[Nitrogen]], N<sub>2</sub>
| [[Nitrogen]], N<sub>2</sub>
| 78.084%
| 78.084%
| 78.084%
|-
|-
| [[Oxygen]], O<sub>2</sub><ref name="NYT-20131003">{{cite news |last=Zimmer |first=Carl |author-link=Carl Zimmer |title=Earth's Oxygen: A Mystery Easy to Take for Granted |url=https://www.nytimes.com/2013/10/03/science/earths-oxygen-a-mystery-easy-to-take-for-granted.html |date=3 October 2013 |work=[[The New York Times]] |access-date=3 October 2013 }}</ref>
| [[Oxygen]], O<sub>2</sub><ref name="NYT-20131003">{{cite news |last=Zimmer |first=Carl |author-link=Carl Zimmer |title=Earth's Oxygen: A Mystery Easy to Take for Granted |url=https://www.nytimes.com/2013/10/03/science/earths-oxygen-a-mystery-easy-to-take-for-granted.html |date=3 October 2013 |work=[[The New York Times]] |access-date=3 October 2013 }}</ref>
| 20.946%
| 20.946%
| 20.946%
|-
|-
! colspan=3 | '''Minor constituents (mole fractions in [[Parts per million|ppm]])'''
! colspan="2" | Minor Constituents (mole fractions in [[Parts per million|ppm]])
|-
|-
| [[Argon]], Ar
| [[Argon]], Ar
| 9340
| 9340
| 9340
|-
|-
| [[Carbon dioxide]]*<sup>[a]</sup>, CO<sub>2</sub>
| [[Carbon dioxide]], CO<sub>2</sub>
| 430
| 430
| 430
|-
|-
| [[Neon]], Ne
| [[Neon]], Ne
| 18.18
| 18.18
| 18.18
|-
|-
| [[Helium]], He
| [[Helium]], He
| 5.24
| 5.24
| 5.24
|-
|-
| [[Methane]]<sup>[a]</sup>, CH<sub>4</sub>
| [[Methane]], CH<sub>4</sub>
| 1.9
| 1.9
| 1.9
|-
|-
| [[Krypton]], Kr
| [[Krypton]], Kr
| 1.14
| 1.14
| 1.14
|-
|-
| [[Hydrogen]], H<sub>2</sub>
| [[Hydrogen]], H<sub>2</sub>
| 0.53
| 0.53
| 0.53
|-
|-
| [[Nitrous oxide]], N<sub>2</sub>O
| [[Nitrous oxide]], N<sub>2</sub>O
|0.34
|
| 0.34
|-
|-
| [[Xenon]], Xe
| [[Xenon]], Xe
|0.087
|
| 0.087
|-
|-
| [[Nitrogen dioxide]], NO<sub>2</sub>
| [[Nitrogen dioxide]], NO<sub>2</sub>
|up to 0.02
|
| up to 0.02
|-
|-
| [[Ozone]]*, O<sub>3</sub>, in summer
| [[Ozone]], O<sub>3</sub>, in summer
|up to 0.07
|
| up to 0.07
|-
|-
| [[Ozone]]*, O<sub>3</sub>, in winter
| [[Ozone]], O<sub>3</sub>, in winter
|up to 0.02
|
| up to 0.02
|-
|-
| [[Sulphur dioxide]]*, SO<sub>2</sub>
| [[Sulphur dioxide]], SO<sub>2</sub>
|up to 1
|
| up to 1
|-
|-
| [[Iodine]]*, I<sub>2</sub>
| [[Iodine]], I<sub>2</sub>
|0.01
|
| 0.01
|-
|-
! colspan=3 | '''Water'''
! colspan="2" | '''Water'''
|-
|-
| [[Water vapour]]*
| [[Water vapour]]*
| colspan=2 | Highly variable (about 0–3%);<br>typically makes up about 1%
| Highly variable (about 0–3%);<br>typically makes up about 1%
|-
|-
! colspan=3 | '''Notes'''
! colspan="2" | '''Notes'''
|-
|-
| colspan=3 | 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. <sup>[a]</sup>The [[concentration]] of CO<sub>2</sub> and CH<sub>4</sub> vary by season and location.
| colspan="2" | 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. The [[concentration]] of CO<sub>2</sub> and CH<sub>4</sub> vary by season and location.
|}
|}


=== Trace gas composition ===
=== 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 [[Chlorofluorocarbon|CFCs/HCFCs]] which are particularly damaging to the ozone layer, and [[Hydrogen sulfide|{{chem|H|2|S}}]] 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.
Besides the major components listed above, the Earth's atmosphere contains many trace gas species that vary significantly depending on nearby sources and sinks. These trace gasses include compounds such as [[Chlorofluorocarbon|CFCs/HCFCs]] which are particularly damaging to the ozone layer, and [[Hydrogen sulfide|H2S]] 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 gasses are listed below. In addition to gasses, the atmosphere contains particles such as [[aerosol]], which includes examples such as droplets, ice crystals, bacteria, and dust.


{| class="wikitable" style=width:45em
{| class="wikitable"
! Gas
! colspan=3 | Composition (ppt by volume unless otherwise stated)
!Composition (ppt by volume unless otherwise stated)
|-
| '''Gas'''
| '''Clean continental, Seinfeld & Pandis (2016)'''<ref>{{cite book |last1=Seinfeld |first1=John |last2=Pandis |first2=Spyros |date=2016 |title=Atmospheric Chemistry and Physics - from Air Pollution to Climate Change, 3rd ed. |url= |location=Hoboken, New Jersey |publisher=[[Wiley (publisher)|Wiley]] |page= |isbn=9781119221173}}</ref>
| '''Simpson et al. (2010)'''<ref name="SimpsonBlake2010">{{cite journal|last1=Simpson|first1=I. J.|last2=Blake|first2=N. J.|last3=Barletta|first3=B.|last4=Diskin|first4=G. S.|last5=Fuelberg|first5=H. E.|last6=Gorham|first6=K.|last7=Huey|first7=L. G.|last8=Meinardi|first8=S.|last9=Rowland|first9=F. S.|last10=Vay|first10=S. A.|last11=Weinheimer|first11=A. J.|last12=Yang|first12=M.|last13=Blake|first13=D. R.|title=Characterization of trace gases measured over Alberta oil sands mining operations: 76 speciated C<sub>2</sub>–C<sub>10</sub> volatile organic compounds (VOCs), CO<sub>2</sub>, CH<sub>4</sub>, CO, NO, NO<sub>2</sub>, NO, O<sub>3</sub> and SO<sub>2</sub>|journal=Atmospheric Chemistry and Physics|volume=10|issue=23|year=2010|pages=11931–11954|issn=1680-7324|doi=10.5194/acp-10-11931-2010|bibcode=2010ACP....1011931S |s2cid=62782723 |doi-access=free}}</ref>
|-
|-
| [[Carbon monoxide]], CO
| [[Carbon monoxide]], CO
| 40-200 ppb <sup>p39</sup><ref name=":3">{{cite book |last1=Seinfeld |first1=John |url= |title=Atmospheric Chemistry and Physics - from Air Pollution to Climate Change, 3rd ed. |last2=Pandis |first2=Spyros |date=2016 |publisher=[[Wiley (publisher)|Wiley]] |isbn=9781119221173 |location=Hoboken, New Jersey |page=}}</ref>
| 40-200 ppb <sup>p39</sup>
| 97 ppb
|-
|-
| [[Nitric oxide]], NO
| [[Nitric oxide]], NO
|16<ref name="SimpsonBlake2010">{{cite journal |last1=Simpson |first1=I. J. |last2=Blake |first2=N. J. |last3=Barletta |first3=B. |last4=Diskin |first4=G. S. |last5=Fuelberg |first5=H. E. |last6=Gorham |first6=K. |last7=Huey |first7=L. G. |last8=Meinardi |first8=S. |last9=Rowland |first9=F. S. |last10=Vay |first10=S. A. |last11=Weinheimer |first11=A. J. |last12=Yang |first12=M. |last13=Blake |first13=D. R. |year=2010 |title=Characterization of trace gases measured over Alberta oil sands mining operations: 76 speciated C<sub>2</sub>–C<sub>10</sub> volatile organic compounds (VOCs), CO<sub>2</sub>, CH<sub>4</sub>, CO, NO, NO<sub>2</sub>, NO, O<sub>3</sub> and SO<sub>2</sub> |journal=Atmospheric Chemistry and Physics |volume=10 |issue=23 |pages=11931–11954 |bibcode=2010ACP....1011931S |doi=10.5194/acp-10-11931-2010 |issn=1680-7324 |s2cid=62782723 |doi-access=free}}</ref>
|
| 16
|-
|-
| [[Ethane]], C<sub>2</sub>H<sub>6</sub>
| [[Ethane]], C<sub>2</sub>H<sub>6</sub>
|781<ref name="SimpsonBlake2010" />
|
| 781
|-
|-
| [[Propane]], C<sub>3</sub>H<sub>8</sub>
| [[Propane]], C<sub>3</sub>H<sub>8</sub>
|200<ref name="SimpsonBlake2010" />
|
| 200
|-
|-
| [[Isoprene]], C<sub>5</sub>H<sub>8</sub>
| [[Isoprene]], C<sub>5</sub>H<sub>8</sub>
|311<ref name="SimpsonBlake2010" />
|
| 311
|-
|-
| [[Benzene]], C<sub>6</sub>H<sub>6</sub>
| [[Benzene]], C<sub>6</sub>H<sub>6</sub>
|11<ref name="SimpsonBlake2010" />
|
| 11
|-
|-
| [[Methanol]], CH<sub>3</sub>OH
| [[Methanol]], CH<sub>3</sub>OH
|1967<ref name="SimpsonBlake2010" />
|
| 1967
|-
|-
| [[Ethanol]], C<sub>2</sub>H<sub>5</sub>OH
| [[Ethanol]], C<sub>2</sub>H<sub>5</sub>OH
|75<ref name="SimpsonBlake2010" />
|
| 75
|-
|-
| [[Trichlorofluoromethane]], CCl<sub>3</sub>F
| [[Trichlorofluoromethane]], CCl<sub>3</sub>F
| 237 <sup>p41</sup>
| 237 <sup>p41</sup><ref name=":3" />
| 252.7
|-
|-
| [[Dichlorodifluoromethane]], CCl<sub>2</sub>F<sub>2</sub>
| [[Dichlorodifluoromethane]], CCl<sub>2</sub>F<sub>2</sub>
| 530 <sup>p41</sup>
| 530 <sup>p41</sup><ref name=":3" />
| 532.3
|-
|-
| [[Chloromethane]], CH<sub>3</sub>Cl
| [[Chloromethane]], CH<sub>3</sub>Cl
|503<ref name="SimpsonBlake2010" />
|
| 503
|-
|-
| [[Bromomethane]], CH<sub>3</sub>Br
| [[Bromomethane]], CH<sub>3</sub>Br
| 9–10 <sup>p44</sup>
| 9–10 <sup>p44</sup><ref name=":3" />
| 7.7
|-
|-
| [[Iodomethane]], CH<sub>3</sub>I
| [[Iodomethane]], CH<sub>3</sub>I
|0.36<ref name="SimpsonBlake2010" />
|
| 0.36
|-
|-
| [[Carbonyl sulfide]], OCS
| [[Carbonyl sulfide]], OCS
| 510 <sup>p26</sup>
| 510 <sup>p26</sup><ref name=":3" />
| 413
|-
|-
| [[Sulfur dioxide]], SO<sub>2</sub>
| [[Sulfur dioxide]], SO<sub>2</sub>
| 70–200 <sup>p26</sup>
| 70–200 <sup>p26</sup><ref name=":3" />
| 102
|-
|-
| [[Hydrogen sulfide]], H<sub>2</sub>S
| [[Hydrogen sulfide]], H<sub>2</sub>S
| 15–340 <sup>p26</sup>
| 15–340 <sup>p26</sup><ref name=":3" />
|
|-
|-
| [[Carbon disulfide]], CS<sub>2</sub>
| [[Carbon disulfide]], CS<sub>2</sub>
| 15–45 <sup>p26</sup>
| 15–45 <sup>p26</sup><ref name=":3" />
|
|-
|-
| [[Formaldehyde]], H<sub>2</sub>CO
| [[Formaldehyde]], H<sub>2</sub>CO
| 9.1 ppb <sup>p37, ''polluted''</sup>
| 9.1 ppb <sup>p37, ''polluted''</sup> ''<ref name=":3" />''
|
|-
|-
| [[Acetylene]], C<sub>2</sub>H<sub>2</sub>
| [[Acetylene]], C<sub>2</sub>H<sub>2</sub>
| 8.6 ppb <sup>p37, ''polluted''</sup>
| 8.6 ppb <sup>p37, ''polluted''</sup> ''<ref name=":3" />''
|
|-
|-
| [[Ethene]], C<sub>2</sub>H<sub>4</sub>
| [[Ethene]], C<sub>2</sub>H<sub>4</sub>
| 11.2 ppb <sup>p37, ''polluted''</sup>
| 11.2 ppb <sup>p37, ''polluted''</sup> ''<ref name=":3" />''
| 20
|-
|-
| [[Sulfur hexafluoride]], SF<sub>6</sub>
| [[Sulfur hexafluoride]], SF<sub>6</sub>
| 7.3 <sup>p41</sup>
| 7.3 <sup>p41</sup><ref name=":3" />
|
|-
|-
| [[Carbon tetrafluoride]], CF<sub>4</sub>
| [[Carbon tetrafluoride]], CF<sub>4</sub>
| 79 <sup>p41</sup>
| 79 <sup>p41</sup><ref name=":3" />
|
|-
|-
| Total gaseous [[Mercury (element)|mercury]], Hg
| Total gaseous [[Mercury (element)|mercury]], Hg
| 0.209 <sup>p55</sup>
| 0.209 <sup>p55</sup><ref name=":3" />
|
|}
|}


== History ==
== History ==
[[Image:Atmosphere composition diagram-en.svg|thumb|upright=1.3|Schematic of chemical and transport processes related to atmospheric composition]]
[[Image:Atmosphere composition diagram-en.svg|thumb|upright=1.15 |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.{{citation needed|date=April 2023}}
The first scientific studies of atmospheric composition began in the 18th century when chemists such as [[Joseph Priestley]], [[Antoine Lavoisier]] and [[Henry Cavendish]] made the first measurements of the composition of the atmosphere.<ref>{{Cite journal |last=Weeks |first=M. E. |date=1934 |title=Daniel Rutherford and the discovery of nitrogen |journal=Chemistry Education |volume=11 |pages=101}}</ref>


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.<ref>{{Cite book |last=Shoenbein |first=C. |url=http://archive.org/details/philtrans03578905 |title=On the Production of Ozone by Chemical Means |date=1843-01-01 |publisher=Royal Society of London}}</ref>
In the late 19th and early 20th centuries, researchers shifted their interest towards trace constituents with very low concentrations. An important finding from this era was the discovery of [[ozone]] by [[Christian Friedrich Schönbein]] in 1840.<ref>{{Cite journal |last=Schönbein |first=C. F |date=1840 |title=On the odour accompanying electricity and on the probability of its dependency on the presence of a new substance |journal=Philosophical Magazine |volume=17 |pages=293-294}}</ref>


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 (astronomer)|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]].<ref name= "NobelPrize1995">{{cite web |url=https://www.nobelprize.org/prizes/chemistry/1995/press-release/ |title=Press Release - 1995 Nobel Prize in Chemistry |author=<!--Not stated--> |date=October 11, 1995 |website=The Nobel Prize |publisher=Nobel Prize Org }}</ref>
In the 20th century atmospheric science moved from studying the composition of air to consider how the concentrations of trace gasses in the atmosphere have changed over time and the chemical processes which create and destroy compounds in the air. Two important outcomes were the explanation by [[Sydney Chapman (astronomer)|Sydney Chapman]] and [[Gordon Dobson]] of how the [[ozone layer]] is created and maintained, and [[Arie Jan Haagen-Smit]]’s explanation of [[photochemical smog]]. Further studies on ozone issues led to the 1995 Nobel Prize in Chemistry award shared between [[Paul Crutzen]], [[Mario Molina]] and [[Frank Sherwood Rowland]]. The late 20th century also introduced [[green chemistry]], which prioritizes the sustainable, safe, and efficient use of chemicals. Green atmospheric chemistry research led to government regulations minimizing the use of harmful chemicals like [[Chlorofluorocarbon|CFCs]] and [[DDT]].<ref>{{Cite book |last=Anastas |first=Paul |title=Origins and Early History of Green Chemistry |date=2018 |publisher=World Scientific Publishing}}</ref>


In the 21st century the focus is now shifting again. Atmospheric chemistry is increasingly studied as one part of the [[Earth science#Earth system science|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 [[Earth's atmosphere|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]].{{citation needed|date=April 2023}}
In the 21st century the focus is now shifting again. Instead of concentrating on atmospheric chemistry in isolation, it is now seen as one part of the [[Earth science#Earth system science|Earth system]] with the rest of the [[Earth's atmosphere|atmosphere]], [[biosphere]] and [[geosphere]]. A driving force for this link is the relationship between chemistry and [[climate]]. The changing climate and the recovery of the ozone hole and the interaction of the composition of the atmosphere with the oceans and terrestrial [[ecosystems]] are examples of the interdependent relationships between Earth's systems.<ref name=":1" /> A new field of [[Extraterrestrial atmosphere|extraterrestrial atmospheric]] chemistry has also recently emerged. Astrochemists analyze the atmospheric compositions of our solar system and [[Exoplanet|exoplanets]] to determine the formation of astronomical objects and find habitual conditions for Earth-like life.<ref>{{Cite news |last=Gertner |first=Jon |date=September 15, 2022 |title=The Search for Intelligent Life Is About to Get a Lot More Interesting |url=https://www.nytimes.com/2022/09/15/magazine/extraterrestrials-technosignatures.html# |access-date=November 30, 2024 |work=The New York Times Magazine}}</ref> {{multiple image |caption_align=center |align=center |width= |direction=horizontal

{{multiple image |caption_align=center |align=center |width= |direction=horizontal
|image1=M15-162b-EarthAtmosphere-CarbonDioxide-FutureRoleInGlobalWarming-Simulation-20151109.jpg
|image1=M15-162b-EarthAtmosphere-CarbonDioxide-FutureRoleInGlobalWarming-Simulation-20151109.jpg
|caption1=[[Carbon dioxide in Earth's atmosphere]] if ''half'' of anthropogenic CO<sub>2</sub> emissions<ref name="NYT-20151110">{{cite news |last=St. Fleur |first=Nicholas |title=Atmospheric Greenhouse Gas Levels Hit Record, Report Says |url=https://www.nytimes.com/2015/11/11/science/atmospheric-greenhouse-gas-levels-hit-record-report-says.html |date=10 November 2015 |work=The New York Times |access-date=11 November 2015 }}</ref><ref name="AP-20151109">{{cite news |last=Ritter |first=Karl |title=UK: In 1st, global temps average could be 1 degree C higher |url=http://apnews.excite.com/article/20151109/climate_countdown-greenhouse_gases-d8a21f0397.html |date=9 November 2015 |work=[[AP News]] |access-date=11 November 2015 }}</ref> are ''not'' absorbed<br>([[NASA]] [[Computer simulation|simulation]]; 9 November 2015)
|caption1=[[Carbon dioxide in Earth's atmosphere]] if ''half'' of anthropogenic CO<sub>2</sub> emissions<ref name="NYT-20151110">{{cite news |last=St. Fleur |first=Nicholas |title=Atmospheric Greenhouse Gas Levels Hit Record, Report Says |url=https://www.nytimes.com/2015/11/11/science/atmospheric-greenhouse-gas-levels-hit-record-report-says.html |date=10 November 2015 |work=The New York Times |access-date=11 November 2015 }}</ref><ref name="AP-20151109">{{cite news |last=Ritter |first=Karl |title=UK: In 1st, global temps average could be 1 degree C higher |url=http://apnews.excite.com/article/20151109/climate_countdown-greenhouse_gases-d8a21f0397.html |date=9 November 2015 |work=[[AP News]] |access-date=11 November 2015 }}</ref> are ''not'' absorbed<br>([[NASA]] [[Computer simulation|simulation]]; 9 November 2015)
Line 217: Line 174:


== Methodology ==
== Methodology ==
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.{{citation needed|date=April 2023}}
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 modeling and laboratory studies which will increase our scientific understanding to a level where we can explain the observations.<ref>{{Cite book |last=Brasseur |first=Guy |title=Atmospheric Chemistry in a Changing World |last2=Prinn |first2=Ronald |last3=Pszenny |first3=Alexander |publisher=Springer-Verlag BerIin Heidelberg |year=2003 |isbn=978-3-642-62396-7 |location=New York}}</ref>


=== Observation ===
=== Observation ===
Field observations of chemical systems are essential to understanding atmospheric processes and determining the accuracy of models. Atmospheric chemistry measurements are long term to observe continuous trends or short term to observe smaller variations. In situ and remote measurements can be made using observatories, satellites, field stations, and laboratories.
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 [[Carbon dioxide in Earth's atmosphere#Measurement techniques|ongoing measurements of atmospheric CO<sub>2</sub>]]). 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 [[European Remote-Sensing Satellite|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]].{{citation needed|date=April 2023}}

Routine observations of chemical composition show changes in atmospheric composition over time. Observatories such as the [[Mauna Loa Observatory|Mauna Loa]] and mobile platforms such as aircraft ships and balloons (e.g. the UK's [[Facility for Airborne Atmospheric Measurements]]) study chemical compositions and weather dynamics. An application of long term observations is the [[Keeling Curve]] - a series of measurements from 1958 to today which show a steady rise in the concentration of [[carbon dioxide]] (see also [[Carbon dioxide in Earth's atmosphere#Measurement techniques|ongoing measurements of atmospheric CO<sub>2</sub>]]). Observations of atmospheric composition are increasingly made by [[satellites]] by passive and active remote sensing with important instruments such as [[European Remote-Sensing Satellite|GOME]] and [[MOPITT]] giving a global picture of air pollution and chemistry.<ref>{{Cite web |date=November 30, 2024 |title=In-Situ and Remote Sensing Measurements |url=https://www.e-education.psu.edu/meteo3/node/2224 |website=PennState College of Earth and Mineral Sciences Introductory Meteorology}}</ref>

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 aerosols but are still restricted in the horizontal region they can cover. Many observations are available online in [[Atmospheric Chemistry Observational Databases]]<ref>{{Cite web |last= |date=March 19, 2024 |title=Air Quality Modeling - Surface and Upper Air Databases |url=https://www.epa.gov/scram/air-quality-modeling-surface-and-upper-air-databases |website=U.S. Environmental Protection Agency}}</ref>


=== Laboratory studies ===
=== Laboratory studies ===
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.<ref>{{Cite book|title=Future of Atmospheric Research: Remembering Yesterday, Understanding Today, Anticipating Tomorrow|vauthors = ((National Academies of Sciences, Engineering, and Medicine))|publisher=The National Academies Press|year=2016|isbn=978-0-309-44565-8|location=Washington, DC|pages=15}}</ref> Types of analysis that are of interest includes both those on gas-phase reactions, as well as [[Homogeneity and heterogeneity|heterogeneous]] reactions that are relevant to the formation and growth of [[aerosol]]s. 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.{{citation needed|date=April 2023}}
Laboratory studies help understand the complex interactions from Earth’s systems that can be difficult to measure on a large scale. Experiments are performed in controlled environments, such as aerosol chambers, that allow for the individual evaluation of specific chemical reactions or the assessment of properties of a particular atmospheric constituent.<ref>{{Cite book |title=Future of Atmospheric Research: Remembering Yesterday, Understanding Today, Anticipating Tomorrow |vauthors=((National Academies of Sciences, Engineering, and Medicine)) |publisher=The National Academies Press |year=2016 |isbn=978-0-309-44565-8 |location=Washington, DC |pages=15}}</ref> A closely related subdiscipline is atmospheric [[photochemistry]], which quantifies the rate that molecules are split apart by sunlight, determines the resulting products, and obtains [[thermodynamic]] data such as [[Henry's law]] coefficients.

Laboratory measurements are essential to understanding the sources and sinks of pollutants and naturally occurring compounds. Types of analysis that are of interest include both those on gas-phase reactions, as well as [[Homogeneity and heterogeneity|heterogeneous]] reactions that are relevant to the formation and growth of [[Aerosol|aerosols]]. Commonly used instruments to measure aerosols include ambient and [[Particulate matter sampler|particulate air samplers]], [[Scanning mobility particle sizer|scanning mobility particle sizers]], and [[Mass spectrometry|mass spectrometers]].<ref>{{Cite web |last=Choularton |first=Tom |last2=Vaughan |first2=Geraint |date=November 30, 2024 |title=Centre for Atmospheric Science Instruments |url=http://www.cas.manchester.ac.uk/restools/instruments/}}</ref>
[[File:Box Model Diagram Atmospheric Chemistry.jpg|alt=Three boxes stacked on top of one another with vertical arrows to show elevation and horizontal arrows to show transportation. Aerosols enter the box via human, plant, and wind transport and exit via dry or wet deposition. |thumb|Schematic diagram of a one-dimensional column model depicting the movement and transformation of aerosols.<ref name=":2">{{Cite book |last=Jacobs |first=Daniel |title=Introduction to Atmospheric Chemistry |date=January 1999 |publisher=Princeton University Press |isbn=9780691001852}}</ref>]]


=== Modeling ===
=== Modeling ===
{{unreferenced section|date=June 2019}}
{{unreferenced section|date=June 2019}}
Models are essential tools for interpreting observational data, testing hypotheses about chemical reactions, and predicting future concentrations of atmospheric chemicals. To synthesize and test theoretical understanding of atmospheric chemistry, researchers commonly use computer models, such as [[Chemical transport model|chemical transport models (CTMs)]]. CTMs provide realistic descriptions of the three-dimensional transport and evolution of the atmosphere.<ref name=":1">{{Cite book |last=Brasseur |first=Guy P. |title=Modeling of Atmospheric Chemistry |last2=Jacob |first2=Daniel J. |date=May 2017 |publisher=Cambridge University Press |isbn=9781316544754 |pages=2-23}}</ref> [[Atmospheric model|Atmospheric models]] can be seen as mathematical representations that replicate the behavior of the atmosphere. These numerical models solve the differential equations governing the concentrations of chemicals in the atmosphere.
In order to synthesize and test theoretical understanding of atmospheric chemistry, computer models (such as [[chemical transport model]]s) 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.


Depending on the complexity, these models can range from simple to highly detailed. Models can be zero-, one-, two-, or three-dimensional, each with various uses and advantages. Three-dimensional chemical transport models offer the most realistic simulations but require substantial computational resources. These models can be global e.g. [[General circulation model|GCM]], simulating the atmospheric conditions across the Earth, or regional, e.g. [[Regional Atmospheric Modeling System|RAMS]] focusing on specific areas with greater resolution. Global models typically have lower horizontal resolution and represent less complex chemical mechanisms but they cover a larger area, while regional models can represent a limited area with higher resolution and more detail.<ref name=":0">{{Cite book |last=Brasseur |first=Guy P. |title=Atmospheric Chemistry and Global Change |last2=Orlando |first2=John J. |last3=Tyndall |first3=Geoffrey S. |publisher=The National Academies Press |year=1999 |isbn=0-19-510521-4 |location=United States |pages=439–441}}</ref>
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.

A major challenge in atmospheric modeling is balancing the number of chemical compounds and reactions included in the model with the accuracy of physical processes such as transport and mixing in the atmosphere. Two simpliest types of models include box models and [[Puff model|puff models]]. For example, [[box modeling]] is relatively simple and may include hundreds or even thousands of chemical reactions, but they typically use a very crude representation of atmospheric [[mixed layer]].<ref name=":2" /> This makes them useful for studying specific chemical reactions, but limited in stimulating real-world dynamics. In contrast, [[3D modeling|3D models]] are more complex, representing a variety of physical processes such as wind, convection, and atmospheric mixing. They also provide more realistic representations of transportation and mixing. However, computational limits often simply chemical reactions and typically include fewer chemical reactions than box models. The trade-off between the two approaches lies in resolution and complexity.

To simplify the creation of these complex models, some researchers use automatic code generators like [[Autochem]] or [[Kinetic PreProcessor]]. These tools help automate the model-building process by selecting relevant chemical reactions from databases based on a [[user-defined function]] of chemical constituents.<ref>{{Cite web |last=Lockard |first=David |date=November 2005 |title=AutoChem |url=https://ntrs.nasa.gov/enwiki/api/citations/20110016385/downloads/20110016385.pdf}}</ref> Once the reactions are chosen, the code generator automatically constructs the [[ordinary differential equations]] that describe their time evolution, greatly reducing the time and effort required for model construction.

Differences between model prediction and real-world observations can arise from errors in model input parameters or flaws representations of processes in the model. Some input parameters like surface emissions are often less accurately quantified from observations compared to model results. The model can be improved by adjusting poorly known parameters to better match observed data<ref name=":1" />. A formal method for applying these adjustments is through [[Bayesian optimization|Bayesian Optimization]] through an inverse modeling framework, where the results from the CTMs are inverted to optimize selected parameters. This approach has gained attention over the past decade as an effective method to interpret large amounts of data generate by models and observations from satellites.

One important current trend is using atmospheric chemistry as part of [[Earth System Modeling Framework|Earth system models]]. These models integrate atmospheric chemistry with other Earth system components, enabling the study of complex interactions between climate, atmospheric composition, and ecosystems.

=== Applications ===
Atmospheric chemistry is a multidisciplinary field with wide-ranging applications that influence environmental policy, human health, technology development, and climate science. Key applications include [[greenhouse gas monitoring]], air quality and pollution control, weather prediction and meteorology, energy and emissions, sustainable energy development, and public health and toxicology.

Advances in remote sensing technology allow scientists to monitor atmospheric chemical composition from satellites and ground-based stations. Instruments such as the [[Ozone monitoring instrument|Ozone Monitoring Instrument (OMI)]] and [[Atmospheric infrared sounder|Atmospheric Infrared Sounder (AIRS)]] provide data on pollutants, greenhouse gasses, and aerosols, enabling real-time monitoring of air quality<ref>{{Cite web |title=Ozone Monitoring Instrument (OMI) |url=https://www.knmiprojects.nl/projects/ozone-monitoring-instrument |url-status=live |website=Aura - NASA Science}}</ref><ref>{{Cite journal |last=Pagano |first=T. S. |last2=Payne |first2=V. H. |date=2023 |title=Handbook of Air Quality and Climate Change |url=https://doi.org/10.1007/978-981-15-2760-9_64 |journal=Springer}}</ref>.

Atmospheric chemistry is vital for evaluating the environmental impacts of energy production, including fossil fuels and renewable energy sources. By studying emissions, researchers can develop cleaner energy technologies and assess their effects on air quality and climate. Atmospheric chemistry also helps quantify the concentration and persistence of toxic substances in the air, including [[Particulates|particulate matter]] and [[Volatile organic compound|volatile organic compounds (VOCs)]], guiding public health measures and exposures assessments.


==See also==
==See also==
{{Weather}}
* [[Oxygen cycle]]
* [[Oxygen cycle]]
* [[Ozone-oxygen cycle]]
* [[Ozone-oxygen cycle]]
Line 243: Line 221:


== Further reading ==
== Further reading ==
* Brasseur, Guy P.; Orlando, John J.; Tyndall, Geoffrey S. (1999). ''Atmospheric Chemistry and Global Change''. Oxford University Press. {{ISBN|0-19-510521-4}}.
* Finlayson-Pitts, Barbara J.; Pitts, James N., Jr. (2000). ''Chemistry of the Upper and Lower Atmosphere''. Academic Press. {{ISBN|0-12-257060-X}}.
* Finlayson-Pitts, Barbara J.; Pitts, James N., Jr. (2000). ''Chemistry of the Upper and Lower Atmosphere''. Academic Press. {{ISBN|0-12-257060-X}}.
* Iribarne, J. V. Cho, H. R. (1980). ''Atmospheric Physics'', D. Reidel Publishing Company.
* Seinfeld, John H.; Pandis, Spyros N. (2006). ''Atmospheric Chemistry and Physics: From Air Pollution to Climate Change'' (2nd Ed.). John Wiley and Sons, Inc. {{ISBN|0-471-82857-2}}.
* Seinfeld, John H.; Pandis, Spyros N. (2006). ''Atmospheric Chemistry and Physics: From Air Pollution to Climate Change'' (2nd Ed.). John Wiley and Sons, Inc. {{ISBN|0-471-82857-2}}.
* Warneck, Peter (2000). ''Chemistry of the Natural Atmosphere'' (2nd Ed.). Academic Press. {{ISBN|0-12-735632-0}}.
* Warneck, Peter (2000). ''Chemistry of the Natural Atmosphere'' (2nd Ed.). Academic Press. {{ISBN|0-12-735632-0}}.
* Wayne, Richard P. (2000). ''Chemistry of Atmospheres'' (3rd Ed.). Oxford University Press. {{ISBN|0-19-850375-X}}.
* Wayne, Richard P. (2000). ''Chemistry of Atmospheres'' (3rd Ed.). Oxford University Press. {{ISBN|0-19-850375-X}}.
* J. V. Iribarne, H. R. Cho, ''Atmospheric Physics'', D. Reidel Publishing Company, 1980


== External links ==
== External links ==
Line 258: Line 235:
* [http://jpldataeval.jpl.nasa.gov/index.html NASA-JPL Chemical Kinetics and Photochemical Data for Use in Atmospheric Studies]
* [http://jpldataeval.jpl.nasa.gov/index.html NASA-JPL Chemical Kinetics and Photochemical Data for Use in Atmospheric Studies]
* [http://www.iupac-kinetic.ch.cam.ac.uk/ Kinetic and photochemical data evaluated by the IUPAC Subcommittee for Gas Kinetic Data Evaluation]
* [http://www.iupac-kinetic.ch.cam.ac.uk/ Kinetic and photochemical data evaluated by the IUPAC Subcommittee for Gas Kinetic Data Evaluation]
* [http://www.shsu.edu/~chm_tgc/Glossary/glos.html Atmospheric Chemistry Glossary] at [[Sam Houston State University]]
* [http://www.atmosp.physics.utoronto.ca/people/loic/chemistry.html Tropospheric chemistry]
* [http://www.atmosp.physics.utoronto.ca/people/loic/chemistry.html Tropospheric chemistry]
* [http://www.esf.edu/chemistry/dibble/AtmosChemCalc.htm/ Calculators for use in atmospheric chemistry] {{Webarchive|url=https://web.archive.org/web/20101209050705/http://www.esf.edu/chemistry/dibble/AtmosChemCalc.htm |date=2010-12-09 }}
* [http://www.chemistryland.com/CHM107/AirWeBreathe/Comp/AirComposition.html An illustrated elementary assessment of the composition of air]
* [http://www.chemistryland.com/CHM107/AirWeBreathe/Comp/AirComposition.html An illustrated elementary assessment of the composition of air]
{{Authority control}}
{{Authority control}}

Revision as of 08:33, 1 December 2024

Atmospheric chemistry is a branch of atmospheric science that studies the chemistry of the Earth's atmosphere and that of other planets. This multidisciplinary approach of research draws on environmental chemistry, physics, meteorology, computer modeling, oceanography, geology and volcanology, climatology and other disciplines to understand both natural and human-induced changes in atmospheric composition. Key areas of research include the behavior of trace gasses, the formation of pollutants, and the role of aerosols and greenhouse gasses. Through a combination of observations, laboratory experiments, and computer modeling, atmospheric chemists investigate the causes and consequences of atmospheric changes.

The composition and chemistry of the Earth's atmosphere is important for several reasons, but primarily because of the interactions between the atmosphere and living organisms. Natural processes such as volcano emissions, lightning and bombardment by solar particles from corona changes the composition of the Earth's atmosphere. It has also been changed by human activity and some of these changes are harmful to human health, crops and ecosystems. Examples of problems addressed in atmospheric chemistry include acid rain, ozone depletion, photochemical smog, greenhouse gasses and global warming. Atmospheric chemists work to understand the causes of these problems. By developing a theoretical understanding, they can test potential solutions and evaluate the effects of changes in government policy.

Atmospheric composition

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.[1] Axis: Altitude (km), Content of volume (%).
Average Composition of Dry Atmosphere (mole fractions)
Gas Dry air per NASA
Nitrogen, N2 78.084%
Oxygen, O2[2] 20.946%
Minor Constituents (mole fractions in ppm)
Argon, Ar 9340
Carbon dioxide, CO2 430
Neon, Ne 18.18
Helium, He 5.24
Methane, CH4 1.9
Krypton, Kr 1.14
Hydrogen, H2 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. The concentration of CO2 and CH4 vary by season and location.

Trace gas composition

Besides the major components listed above, the Earth's atmosphere contains many trace gas species that vary significantly depending on nearby sources and sinks. These trace gasses include compounds such as CFCs/HCFCs which are particularly damaging to the ozone layer, and H2S 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 gasses are listed below. In addition to gasses, the atmosphere contains particles such as aerosol, which includes examples such as droplets, ice crystals, bacteria, and dust.

Gas Composition (ppt by volume unless otherwise stated)
Carbon monoxide, CO 40-200 ppb p39[3]
Nitric oxide, NO 16[4]
Ethane, C2H6 781[4]
Propane, C3H8 200[4]
Isoprene, C5H8 311[4]
Benzene, C6H6 11[4]
Methanol, CH3OH 1967[4]
Ethanol, C2H5OH 75[4]
Trichlorofluoromethane, CCl3F 237 p41[3]
Dichlorodifluoromethane, CCl2F2 530 p41[3]
Chloromethane, CH3Cl 503[4]
Bromomethane, CH3Br 9–10 p44[3]
Iodomethane, CH3I 0.36[4]
Carbonyl sulfide, OCS 510 p26[3]
Sulfur dioxide, SO2 70–200 p26[3]
Hydrogen sulfide, H2S 15–340 p26[3]
Carbon disulfide, CS2 15–45 p26[3]
Formaldehyde, H2CO 9.1 ppb p37, polluted [3]
Acetylene, C2H2 8.6 ppb p37, polluted [3]
Ethene, C2H4 11.2 ppb p37, polluted [3]
Sulfur hexafluoride, SF6 7.3 p41[3]
Carbon tetrafluoride, CF4 79 p41[3]
Total gaseous mercury, Hg 0.209 p55[3]

History

Schematic of chemical and transport processes related to atmospheric composition

The first scientific studies of atmospheric composition began in the 18th century when chemists such as Joseph Priestley, Antoine Lavoisier and Henry Cavendish made the first measurements of the composition of the atmosphere.[5]

In the late 19th and early 20th centuries, researchers shifted their interest towards trace constituents with very low concentrations. An important finding from this era was the discovery of ozone by Christian Friedrich Schönbein in 1840.[6]

In the 20th century atmospheric science moved from studying the composition of air to consider how the concentrations of trace gasses in the atmosphere have changed over time and the chemical processes which create and destroy compounds in the air. Two important outcomes were the explanation by Sydney Chapman and Gordon Dobson of how the ozone layer is created and maintained, and Arie Jan Haagen-Smit’s explanation of photochemical smog. Further studies on ozone issues led to the 1995 Nobel Prize in Chemistry award shared between Paul Crutzen, Mario Molina and Frank Sherwood Rowland. The late 20th century also introduced green chemistry, which prioritizes the sustainable, safe, and efficient use of chemicals. Green atmospheric chemistry research led to government regulations minimizing the use of harmful chemicals like CFCs and DDT.[7]

In the 21st century the focus is now shifting again. Instead of concentrating on atmospheric chemistry in isolation, it is now seen as one part of the Earth system with the rest of the atmosphere, biosphere and geosphere. A driving force for this link is the relationship between chemistry and climate. The changing climate and the recovery of the ozone hole and the interaction of the composition of the atmosphere with the oceans and terrestrial ecosystems are examples of the interdependent relationships between Earth's systems.[8] A new field of extraterrestrial atmospheric chemistry has also recently emerged. Astrochemists analyze the atmospheric compositions of our solar system and exoplanets to determine the formation of astronomical objects and find habitual conditions for Earth-like life.[9]

Carbon dioxide in Earth's atmosphere if half of anthropogenic CO2 emissions[10][11] are not absorbed
(NASA simulation; 9 November 2015)
Nitrogen dioxide 2014 - global air quality levels
(released 14 December 2015)[12]

Methodology

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 modeling and laboratory studies which will increase our scientific understanding to a level where we can explain the observations.[13]

Observation

Field observations of chemical systems are essential to understanding atmospheric processes and determining the accuracy of models. Atmospheric chemistry measurements are long term to observe continuous trends or short term to observe smaller variations. In situ and remote measurements can be made using observatories, satellites, field stations, and laboratories.

Routine observations of chemical composition show changes in atmospheric composition over time. Observatories such as the Mauna Loa and mobile platforms such as aircraft ships and balloons (e.g. the UK's Facility for Airborne Atmospheric Measurements) study chemical compositions and weather dynamics. An application of long term observations is the Keeling Curve - a series of measurements from 1958 to today which show a steady rise in the concentration of carbon dioxide (see also ongoing measurements of atmospheric CO2). Observations of atmospheric composition are increasingly made by satellites by passive and active remote sensing with important instruments such as GOME and MOPITT giving a global picture of air pollution and chemistry.[14]

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 aerosols but are still restricted in the horizontal region they can cover. Many observations are available online in Atmospheric Chemistry Observational Databases[15]

Laboratory studies

Laboratory studies help understand the complex interactions from Earth’s systems that can be difficult to measure on a large scale. Experiments are performed in controlled environments, such as aerosol chambers, that allow for the individual evaluation of specific chemical reactions or the assessment of properties of a particular atmospheric constituent.[16] A closely related subdiscipline is atmospheric photochemistry, which quantifies the rate that molecules are split apart by sunlight, determines the resulting products, and obtains thermodynamic data such as Henry's law coefficients.

Laboratory measurements are essential to understanding the sources and sinks of pollutants and naturally occurring compounds. Types of analysis that are of interest include both those on gas-phase reactions, as well as heterogeneous reactions that are relevant to the formation and growth of aerosols. Commonly used instruments to measure aerosols include ambient and particulate air samplers, scanning mobility particle sizers, and mass spectrometers.[17]

Three boxes stacked on top of one another with vertical arrows to show elevation and horizontal arrows to show transportation. Aerosols enter the box via human, plant, and wind transport and exit via dry or wet deposition.
Schematic diagram of a one-dimensional column model depicting the movement and transformation of aerosols.[18]

Modeling

Models are essential tools for interpreting observational data, testing hypotheses about chemical reactions, and predicting future concentrations of atmospheric chemicals. To synthesize and test theoretical understanding of atmospheric chemistry, researchers commonly use computer models, such as chemical transport models (CTMs). CTMs provide realistic descriptions of the three-dimensional transport and evolution of the atmosphere.[8] Atmospheric models can be seen as mathematical representations that replicate the behavior of the atmosphere. These numerical models solve the differential equations governing the concentrations of chemicals in the atmosphere.

Depending on the complexity, these models can range from simple to highly detailed. Models can be zero-, one-, two-, or three-dimensional, each with various uses and advantages. Three-dimensional chemical transport models offer the most realistic simulations but require substantial computational resources. These models can be global e.g. GCM, simulating the atmospheric conditions across the Earth, or regional, e.g. RAMS focusing on specific areas with greater resolution. Global models typically have lower horizontal resolution and represent less complex chemical mechanisms but they cover a larger area, while regional models can represent a limited area with higher resolution and more detail.[19]

A major challenge in atmospheric modeling is balancing the number of chemical compounds and reactions included in the model with the accuracy of physical processes such as transport and mixing in the atmosphere. Two simpliest types of models include box models and puff models. For example, box modeling is relatively simple and may include hundreds or even thousands of chemical reactions, but they typically use a very crude representation of atmospheric mixed layer.[18] This makes them useful for studying specific chemical reactions, but limited in stimulating real-world dynamics. In contrast, 3D models are more complex, representing a variety of physical processes such as wind, convection, and atmospheric mixing. They also provide more realistic representations of transportation and mixing. However, computational limits often simply chemical reactions and typically include fewer chemical reactions than box models. The trade-off between the two approaches lies in resolution and complexity.

To simplify the creation of these complex models, some researchers use automatic code generators like Autochem or Kinetic PreProcessor. These tools help automate the model-building process by selecting relevant chemical reactions from databases based on a user-defined function of chemical constituents.[20] Once the reactions are chosen, the code generator automatically constructs the ordinary differential equations that describe their time evolution, greatly reducing the time and effort required for model construction.

Differences between model prediction and real-world observations can arise from errors in model input parameters or flaws representations of processes in the model. Some input parameters like surface emissions are often less accurately quantified from observations compared to model results. The model can be improved by adjusting poorly known parameters to better match observed data[8]. A formal method for applying these adjustments is through Bayesian Optimization through an inverse modeling framework, where the results from the CTMs are inverted to optimize selected parameters. This approach has gained attention over the past decade as an effective method to interpret large amounts of data generate by models and observations from satellites.

One important current trend is using atmospheric chemistry as part of Earth system models. These models integrate atmospheric chemistry with other Earth system components, enabling the study of complex interactions between climate, atmospheric composition, and ecosystems.

Applications

Atmospheric chemistry is a multidisciplinary field with wide-ranging applications that influence environmental policy, human health, technology development, and climate science. Key applications include greenhouse gas monitoring, air quality and pollution control, weather prediction and meteorology, energy and emissions, sustainable energy development, and public health and toxicology.

Advances in remote sensing technology allow scientists to monitor atmospheric chemical composition from satellites and ground-based stations. Instruments such as the Ozone Monitoring Instrument (OMI) and Atmospheric Infrared Sounder (AIRS) provide data on pollutants, greenhouse gasses, and aerosols, enabling real-time monitoring of air quality[21][22].

Atmospheric chemistry is vital for evaluating the environmental impacts of energy production, including fossil fuels and renewable energy sources. By studying emissions, researchers can develop cleaner energy technologies and assess their effects on air quality and climate. Atmospheric chemistry also helps quantify the concentration and persistence of toxic substances in the air, including particulate matter and volatile organic compounds (VOCs), guiding public health measures and exposures assessments.

See also

References

  1. ^ Cairns, Iver (23 September 1999). "Earth's Atmosphere". The University of Sydney. Retrieved 7 April 2021.
  2. ^ Zimmer, Carl (3 October 2013). "Earth's Oxygen: A Mystery Easy to Take for Granted". The New York Times. Retrieved 3 October 2013.
  3. ^ a b c d e f g h i j k l m n Seinfeld, John; Pandis, Spyros (2016). Atmospheric Chemistry and Physics - from Air Pollution to Climate Change, 3rd ed. Hoboken, New Jersey: Wiley. ISBN 9781119221173.
  4. ^ a b c d e f g h i Simpson, I. J.; Blake, N. J.; Barletta, B.; Diskin, G. S.; Fuelberg, H. E.; Gorham, K.; Huey, L. G.; Meinardi, S.; Rowland, F. S.; Vay, S. A.; Weinheimer, A. J.; Yang, M.; Blake, D. R. (2010). "Characterization of trace gases measured over Alberta oil sands mining operations: 76 speciated C2–C10 volatile organic compounds (VOCs), CO2, CH4, CO, NO, NO2, NO, O3 and SO2". Atmospheric Chemistry and Physics. 10 (23): 11931–11954. Bibcode:2010ACP....1011931S. doi:10.5194/acp-10-11931-2010. ISSN 1680-7324. S2CID 62782723.
  5. ^ Weeks, M. E. (1934). "Daniel Rutherford and the discovery of nitrogen". Chemistry Education. 11: 101.
  6. ^ Schönbein, C. F (1840). "On the odour accompanying electricity and on the probability of its dependency on the presence of a new substance". Philosophical Magazine. 17: 293–294.
  7. ^ Anastas, Paul (2018). Origins and Early History of Green Chemistry. World Scientific Publishing.
  8. ^ a b c Brasseur, Guy P.; Jacob, Daniel J. (May 2017). Modeling of Atmospheric Chemistry. Cambridge University Press. pp. 2–23. ISBN 9781316544754.
  9. ^ Gertner, Jon (September 15, 2022). "The Search for Intelligent Life Is About to Get a Lot More Interesting". The New York Times Magazine. Retrieved November 30, 2024.
  10. ^ St. Fleur, Nicholas (10 November 2015). "Atmospheric Greenhouse Gas Levels Hit Record, Report Says". The New York Times. Retrieved 11 November 2015.
  11. ^ Ritter, Karl (9 November 2015). "UK: In 1st, global temps average could be 1 degree C higher". AP News. Retrieved 11 November 2015.
  12. ^ Cole, Steve; Gray, Ellen (14 December 2015). "New NASA Satellite Maps Show Human Fingerprint on Global Air Quality". NASA. Retrieved 14 December 2015.
  13. ^ Brasseur, Guy; Prinn, Ronald; Pszenny, Alexander (2003). Atmospheric Chemistry in a Changing World. New York: Springer-Verlag BerIin Heidelberg. ISBN 978-3-642-62396-7.
  14. ^ "In-Situ and Remote Sensing Measurements". PennState College of Earth and Mineral Sciences Introductory Meteorology. November 30, 2024.
  15. ^ "Air Quality Modeling - Surface and Upper Air Databases". U.S. Environmental Protection Agency. March 19, 2024.
  16. ^ National Academies of Sciences, Engineering, and Medicine (2016). Future of Atmospheric Research: Remembering Yesterday, Understanding Today, Anticipating Tomorrow. Washington, DC: The National Academies Press. p. 15. ISBN 978-0-309-44565-8.
  17. ^ Choularton, Tom; Vaughan, Geraint (November 30, 2024). "Centre for Atmospheric Science Instruments".
  18. ^ a b Jacobs, Daniel (January 1999). Introduction to Atmospheric Chemistry. Princeton University Press. ISBN 9780691001852.
  19. ^ Brasseur, Guy P.; Orlando, John J.; Tyndall, Geoffrey S. (1999). Atmospheric Chemistry and Global Change. United States: The National Academies Press. pp. 439–441. ISBN 0-19-510521-4.
  20. ^ Lockard, David (November 2005). "AutoChem" (PDF).
  21. ^ "Ozone Monitoring Instrument (OMI)". Aura - NASA Science.{{cite web}}: CS1 maint: url-status (link)
  22. ^ Pagano, T. S.; Payne, V. H. (2023). "Handbook of Air Quality and Climate Change". Springer.

Further reading

  • Finlayson-Pitts, Barbara J.; Pitts, James N., Jr. (2000). Chemistry of the Upper and Lower Atmosphere. Academic Press. ISBN 0-12-257060-X.
  • Iribarne, J. V. Cho, H. R. (1980). Atmospheric Physics, D. Reidel Publishing Company.
  • Seinfeld, John H.; Pandis, Spyros N. (2006). Atmospheric Chemistry and Physics: From Air Pollution to Climate Change (2nd Ed.). John Wiley and Sons, Inc. ISBN 0-471-82857-2.
  • Warneck, Peter (2000). Chemistry of the Natural Atmosphere (2nd Ed.). Academic Press. ISBN 0-12-735632-0.
  • Wayne, Richard P. (2000). Chemistry of Atmospheres (3rd Ed.). Oxford University Press. ISBN 0-19-850375-X.