Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
General circulation model
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Grid=== The fluid equations for AGCMs are made discrete using either the [[finite difference method]] or the [[spectral method]]. For finite differences, a grid is imposed on the atmosphere. The simplest grid uses constant angular grid spacing (i.e., a latitude/longitude grid). However, non-rectangular grids (e.g., icosahedral) and grids of variable resolution{{nnbsp}}<ref name="jablonowski-etal-2004"> {{cite report | last1 = Jablonowski | first1 = Christiane | last2 = Herzog | first2 = M | last3 = Penner | first3 = JE | last4 = Oehmke | first4 = RC | last5 = Stout | first5 = QF | last6 = van Leer | first6 = B | title = Adaptive grids for weather and climate models | date = 2004 | publisher = National Center for Atmospheric Research (NCAR) | location = Boulder, Colorado, United States | url = https://citeseerx.ist.psu.edu/document?repid=rep1&type=pdf&doi=3919a358564b1533666e55cb1ebda7180cb245d6 | access-date = 2024-10-13 }} PDF create date 2004-10-28. See also {{cite web |first=Christiane |last=Jablonowski |url=http://www-personal.umich.edu/~cjablono/amr.html |title=Adaptive Mesh Refinement (AMR) for Weather and Climate Models |archive-url=https://web.archive.org/web/20160828124836/http://www-personal.umich.edu/~cjablono/amr.html |archive-date=28 August 2016 |access-date=24 July 2010 |url-status=live}}</ref> are more often used.<ref>NCAR Command Language documentation: [http://www.ncl.ucar.edu/Document/Graphics/contour_grids.shtml Non-uniform grids that NCL can contour] {{webarchive |url=https://web.archive.org/web/20160303171034/http://www.ncl.ucar.edu/Document/Graphics/contour_grids.shtml |date=3 March 2016 }} (Retrieved 24 July 2010)</ref> The LMDz model can be arranged to give high resolution over any given section of the planet. [[HadGEM1]] (and other ocean models) use an ocean grid with higher resolution in the tropics to help resolve processes believed to be important for the [[El Niño|El Niño Southern Oscillation]] (ENSO). Spectral models generally use a [[Gaussian grid]], because of the mathematics of transformation between spectral and grid-point space. Typical AGCM resolutions are between 1 and 5 degrees in latitude or longitude: HadCM3, for example, uses 3.75 in longitude and 2.5 degrees in latitude, giving a grid of 96 by 73 points (96 x 72 for some variables); and has 19 vertical levels. This results in approximately 500,000 "basic" variables, since each grid point has four variables ([[Wind speed|''u'',''v'']], [[Temperature|''T'']], [[Humidity|''Q'']]), though a full count would give more (clouds; soil levels). HadGEM1 uses a grid of 1.875 degrees in longitude and 1.25 in latitude in the atmosphere; HiGEM, a high-resolution variant, uses 1.25 x 0.83 degrees respectively.<ref>{{cite web |url=http://higem.nerc.ac.uk/ |title=High Resolution Global Environmental Modelling (HiGEM) home page |publisher=Natural Environment Research Council and Met Office |date= 18 May 2004}}</ref> These resolutions are lower than is typically used for weather forecasting.<ref>{{cite web|title=Mesoscale modelling |url=http://www.metoffice.gov.uk/science/creating/hoursahead/mesoscale.html |access-date=5 October 2010 |url-status=dead |archive-url=https://web.archive.org/web/20101229170731/http://www.metoffice.gov.uk/science/creating/hoursahead/mesoscale.html |archive-date=29 December 2010 }}</ref> Ocean resolutions tend to be higher, for example, HadCM3 has 6 ocean grid points per atmospheric grid point in the horizontal. For a standard finite difference model, uniform gridlines converge towards the poles. This would lead to computational instabilities (see [[Courant–Friedrichs–Lewy condition|CFL condition]]) and so the model variables must be filtered along lines of latitude close to the poles. Ocean models suffer from this problem too, unless a rotated grid is used in which the North Pole is shifted onto a nearby landmass. Spectral models do not suffer from this problem. Some experiments use [[geodesic grid]]s<ref>{{cite web |url=http://www.unisci.com/stories/20013/0924011.htm |title=Climate Model Will Be First To Use A Geodesic Grid |publisher=Daly University Science News |date=24 September 2001}}</ref> and icosahedral grids, which (being more uniform) do not have pole-problems. Another approach to solving the grid spacing problem is to deform a [[Cartesian coordinate system|Cartesian]] [[cube]] such that it covers the surface of a sphere.<ref>{{cite web|title=Gridding the sphere|url=http://mitgcm.org/projects/cubedsphere/|work=MIT GCM|access-date=9 September 2010}}</ref>
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)