Editing Atmospheric science

{{Short description|Study of the atmosphere, its processes, and its interactions with other systems}}
{{Geophysics|all}}
{{Atmospheric sciences}}
{{Weather}}
'''Atmospheric science''' is the study of the [[Atmosphere of Earth|Earth's atmosphere]] and its various inner-working physical processes. [[Meteorology]] includes [[atmospheric chemistry]] and [[atmospheric physics]] with a major focus on [[weather forecasting]]. [[Climatology]] is the study of atmospheric conditions over timescales longer than those of [[weather|weather]], focusing on average climate conditions and their [[climate variability and change|variability over time]]. [[Aeronomy]] is the study of the upper layers of the atmosphere, where [[dissociation (chemistry)|dissociation]] and [[ionization]] are important. Atmospheric science has been extended to the field of [[planetary science]] and the study of the atmospheres of the [[planet]]s and [[natural satellite]]s of the [[Solar System]].

Experimental instruments used in atmospheric science include [[satellite]]s, [[rocketsonde]]s, [[radiosonde]]s, [[weather balloon]]s, [[radar]]s, and [[laser]]s.

The term '''aerology''' (from [[Ancient Greek|Greek]] ἀήρ, ''aēr'', "[[air]]"; and -λογία, ''[[-logy|-logia]]'') is sometimes used as an alternative term for the study of Earth's atmosphere;<ref>{{Cite web|url=https://www.oed.com/view/Entry/3176?redirectedFrom=aerology|title=Aerology|website=OED Online|publisher=Oxford University Press|access-date=December 4, 2019}}</ref> in other definitions, aerology is restricted to the [[free atmosphere]], the region above the [[planetary boundary layer]].<ref>{{Cite web|url=http://glossary.ametsoc.org/wiki/Aerology|title=Aerology - AMS Glossary|website=glossary.ametsoc.org|access-date=2019-09-08}}</ref>

Early pioneers in the field include [[Léon Teisserenc de Bort]] and [[Richard Assmann]].<ref>[https://books.google.com/books?id=OlckxY7BA_0C&pg=PA17 Ultraviolet radiation in the solar system] By Manuel Vázquez, Arnold Hanslmeier</ref>

== Atmospheric chemistry ==
{{main|Atmospheric chemistry}}
[[File:Atmosphere composition diagram-en.svg|left|thumb|250px|Composition diagram showing the evolution/cycles of various elements in Earth's atmosphere.]]
Atmospheric chemistry is a branch of atmospheric science in which the chemistry of the Earth's atmosphere and that of other planets is studied. It is a multidisciplinary field 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 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 has 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, photochemical smog and global warming. Atmospheric chemistry seeks 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.

== Atmospheric dynamics ==
{{See also|Synoptic scale meteorology}}
Atmospheric dynamics is the study of motion systems of meteorological importance, integrating observations at multiple locations and times and theories. Common topics studied include diverse phenomena such as [[thunderstorms]], [[tornado]]es, [[gravity wave]]s, [[tropical cyclone]]s, [[extratropical cyclone]]s, [[jet stream]]s, and global-scale circulations. The goal of dynamical studies is to explain the observed circulations on the basis of fundamental principles from [[physics]]. The objectives of such studies incorporate improving [[weather forecasting]], developing methods for predicting seasonal and interannual climate fluctuations, and understanding the implications of human-induced perturbations (e.g., increased carbon dioxide concentrations or depletion of the ozone layer) on the global climate.<ref>[[University of Washington]]. [http://www.atmos.washington.edu/academic/atmosdyn.html Atmospheric Dynamics.] Retrieved on 1 June 2007.</ref>

== Atmospheric physics ==
{{main|Atmospheric physics}}
Atmospheric physics is the application of physics to the study of the atmosphere. Atmospheric physicists attempt to model Earth's atmosphere and the atmospheres of the other planets using fluid flow equations, chemical models, radiation balancing, and energy transfer processes in the atmosphere and underlying oceans and land. In order to model weather systems, atmospheric physicists employ elements of scattering theory, [[wave propagation]] models, [[cloud physics]], [[statistical mechanics]] and spatial [[statistics]], each of which incorporate high levels of mathematics and physics. Atmospheric physics has close links to meteorology and climatology and also covers the design and construction of instruments for studying the atmosphere and the interpretation of the data they provide, including [[remote sensing]] instruments.

In the United Kingdom, atmospheric studies are underpinned by the Meteorological Office. Divisions of the U.S. [[National Oceanic and Atmospheric Administration]] (NOAA) oversee research projects and weather modeling involving atmospheric physics. The [[U.S. National Astronomy and Ionosphere Center]] also carries out studies of the high atmosphere.

The [[Earth's magnetic field]] and the [[solar wind]] interact with the atmosphere, creating the [[ionosphere]], [[Van Allen radiation belt]]s, [[telluric current]]s, and [[radiant energy]].

== Climatology ==
{{main|Climatology}}
Climatology is a science that derives knowledge and practices from the more specialized disciplines of meteorology, oceanography, geology, and astronomy to study climate. In contrast to [[meteorology]], which studies short-term [[weather]] systems lasting up to a few weeks, climatology studies the frequency and trends of those systems. It studies the periodicity of weather events over timescales ranging from years to millennia, as well as changes in long-term average weather patterns. [[List of climate scientists|Climatologists]], those who practice climatology, study both the nature of climates&nbsp;– local, regional or global&nbsp;– and the natural or human-induced factors that cause [[climate variability and change|climate variability]] and current ongoing [[global warming|global warming]]. Additionally, the occurrence of past climates on Earth, such as those arising from glacial periods and interglacials, can be used to [[prediction|predict]] future changes in climate.

Phenomena of climatological interest include the [[atmospheric boundary layer]], [[atmospheric circulation|circulation patterns]], [[heat transfer]] ([[thermal radiation|radiative]], [[convection|convective]] and [[latent heat flux|latent]]), interactions between the atmosphere, the [[oceans]] and [[Landform|land]] surface (particularly [[vegetation]], [[land use]] and [[topography]]), as well as the chemical and physical composition of the atmosphere. Related disciplines include [[astrophysics]], [[atmospheric physics]], [[chemistry]], [[ecology]], [[physical geography]], [[geology]], [[geophysics]], [[glaciology]], [[hydrology]], [[oceanography]], and [[volcanology]].

== Aeronomy ==
{{main|Aeronomy}}

Aeronomy is the scientific study of the [[upper atmosphere]] of the [[Earth]] — the atmospheric layers above the [[stratopause]] — and corresponding regions of the atmospheres of other planets, where the entire atmosphere may correspond to the Earth's upper atmosphere or a portion of it. A branch of both atmospheric chemistry and atmospheric physics, aeronomy contrasts with meteorology, which focuses on the layers of the atmosphere below the stratopause.<ref>{{cite book|first=Guy|last= Brasseur|pages=xi|title=''Aeronomy of the Middle Atmosphere : Chemistry and Physics of the Stratosphere and Mesosphere''|publisher=Springer |year=1984|isbn=978-94-009-6403-7}}</ref>  In atmospheric regions studied by aeronomers, [[dissociation (chemistry)|chemical dissociation]] and [[ionization]] are important phenomena.

== Atmospheres on other celestial bodies ==

[[File:Venus - October 29 2021 - Flickr - Kevin M. Gill.png|thumb|right|False-color image of the [[atmosphere of Venus]] in [[ultraviolet]] light, taken by the ''[[Akatsuki (spacecraft)|Akatsuki]]'' orbiter in October 2021]]
All of the Solar System's planets have atmospheres.  This is because their gravity is strong enough to keep gaseous particles close to the surface.  Larger gas giants are massive enough to keep large amounts of the light gases [[hydrogen]] and [[helium]] close by, while the smaller planets lose these gases into [[space]].<ref>{{Cite journal |last1=Sheppard |first1=S. S. |last2=Jewitt |first2=D. |last3=Kleyna |first3=J. |title=An Ultradeep Survey for Irregular Satellites of Uranus: Limits to Completeness |doi=10.1086/426329 |journal=[[The Astronomical Journal]] |volume=129 |issue=1 |pages=518–525 |year=2005 |arxiv=astro-ph/0410059 |bibcode=2005AJ....129..518S|s2cid=18688556 }}</ref> The composition of the Earth's atmosphere is different from the other planets because the various life processes that have transpired on the planet have introduced free molecular [[oxygen]].<ref name=zeilik>{{cite book |last=Zeilik |first=Michael A. |author2=Gregory, Stephan A. |title=Introductory Astronomy & Astrophysics |edition=4th |year=1998 |publisher=Saunders College Publishing |isbn=0-03-006228-4 |pages=67}}</ref> Much of Mercury's atmosphere has been blasted away by the [[solar wind]].<ref>Hunten D. M., Shemansky D. E., Morgan T. H. (1988), ''The Mercury atmosphere'', In: Mercury (A89-43751 19–91). University of Arizona Press, pp. 562–612</ref> The only moon that has retained a dense atmosphere is [[Atmospheric evolution of Titan|Titan]]. There is a thin atmosphere on [[Atmosphere of Triton|Triton]], and a trace of an atmosphere on the [[Atmosphere of the Moon|Moon]].

Planetary atmospheres are affected by the varying degrees of energy received from either the Sun or their interiors, leading to the formation of dynamic [[weather system]]s such as [[hurricane]]s (on Earth), planet-wide [[dust storm]]s ([[Climate of Mars|on Mars]]), an Earth-sized [[Anticyclonic storm|anticyclone]] on Jupiter (called the [[Great Red Spot]]), and [[Great Dark Spot|holes in the atmosphere]] (on Neptune).<ref name=Weather>{{cite web |last=Harvey |first=Samantha |date=1 May 2006 |url=http://solarsystem.nasa.gov/scitech/display.cfm?ST_ID=725 |title=Weather, Weather, Everywhere? |publisher=NASA |access-date=9 September 2007 |archive-url=https://web.archive.org/web/20070808201459/http://solarsystem.nasa.gov/scitech/display.cfm?ST_ID=725 |archive-date=8 August 2007  |url-status=dead}}</ref> At least one extrasolar planet, [[HD 189733 b]], has been claimed to possess such a weather system, similar to the Great Red Spot but twice as large.<ref name="knutson">{{cite journal |last=Knutson |first=Heather A. |author2=Charbonneau, David |author3=Allen, Lori E.|author3-link=Lori Allen (astronomer) |author4=Fortney, Jonathan J. |title=A map of the day-night contrast of the extrasolar planet HD 189733b |journal=Nature |year=2007 |volume=447 |pages=183–6 |doi=10.1038/nature05782 |pmid=17495920 |issue=7141 |bibcode=2007Natur.447..183K |arxiv=0705.0993|s2cid=4402268 }} (Related [http://www.cfa.harvard.edu/press/2007/pr200713.html press release])</ref>

Hot Jupiters have been shown to be losing their atmospheres into space due to stellar radiation, much like the tails of comets.<ref>{{cite web |author1=Weaver, D. |author2=Villard, R. |url=http://hubblesite.org/newscenter/archive/releases/2007/07/full/ |title=Hubble Probes Layer-cake Structure of Alien World's Atmosphere |work=University of Arizona, Lunar and Planetary Laboratory (Press Release) |date=31 January 2007 |access-date=15 August 2007 |archive-url=https://web.archive.org/web/20070808225656/http://hubblesite.org/newscenter/archive/releases/2007/07/full/ |archive-date=8 August 2007  |url-status=live}}</ref><ref>{{cite journal |journal=Nature |last=Ballester |first=Gilda E. |author2=Sing, David K. |author3=Herbert, Floyd |title=The signature of hot hydrogen in the atmosphere of the extrasolar planet HD 209458b |volume=445 |pages=511–4 |year=2007 |doi=10.1038/nature05525 |pmid=17268463 |issue=7127|bibcode=2007Natur.445..511B|hdl=10871/16060 |s2cid=4391861 |hdl-access=free }}</ref> These planets may have vast differences in temperature between their day and night sides which produce supersonic winds,<ref>{{cite journal |last=Harrington |first=Jason |author2=Hansen, Brad M.|author3=Luszcz, Statia H.|author4=Seager, Sara |title=The phase-dependent infrared brightness of the extrasolar planet Andromeda b |journal=Science |volume=314 |pages=623–6 |year=2006 |doi=10.1126/science.1133904 |pmid=17038587 |issue=5799|arxiv=astro-ph/0610491 |bibcode=2006Sci...314..623H|s2cid=20549014 }} (Related [http://www.nasa.gov/vision/universe/starsgalaxies/spitzer-20061012.html press release])</ref> although the day and night sides of HD 189733b appear to have very similar temperatures, indicating that planet's atmosphere effectively redistributes the star's energy around the planet.<ref name="knutson" />

== See also ==
* [[Air pollution]]

== References ==

{{Reflist|30em}}

==External links==
{{Commons category}}
*[http://www.stuffintheair.com/chasing-storms.html Atmospheric fluid dynamics applied to weather maps]&nbsp;– Principles such as Advection, Deformation and Vorticity
*[https://web.archive.org/web/20180619181214/https://www.archives.ucar.edu/ National Center for Atmospheric Research (NCAR) Archives, documents the history of the atmospheric sciences]

{{Earth science}}
{{Environmental science}}
{{Atmospheric electricity}}
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[[Category:Atmospheric sciences| ]]
[[Category:Fluid dynamics]]