Astrophysics (Index)About

adaptive mesh refinement

(AMR)
(numerical modeling method balancing detail with tractability)

Adaptive mesh refinement (AMR) is a design feature of numerical models handling multi-dimensional data such as fields. Examples include qualities spread over three dimensions such as gas density, pressure and flow, temperature, and magnetic fields. Models can make use of a mesh, modeling the values at mesh points, the amount of detail depending upon the mesh scale: how widely spaced are the points recorded and modeled. There may be a resolution (spacing of the mesh) that works for much of the modeling, is not detailed enough for some particular circumstances. AMR is the inclusion of programming logic to adjust to (and possibly from) the smaller mesh scale in just those regions and times where necessary, based upon detecting those circumstances. The goal is to provide model accuracy and precision while keeping the amount of calculation tractable.

The method, for example, can be used for atmospheric modeling (Earth weather prediction), for design of devices involving fluid dynamics (water pipes, rocket engines), for modeling astronomical phenomena including stars, stellar magnetic fields, galaxies, and for cosmological simulations.


(mathematics,models,software type,computation)
Further reading:
https://en.wikipedia.org/wiki/Adaptive_mesh_refinement
http://www-personal.umich.edu/~cjablono/amr.html
https://fluids.umn.edu/research/computational-fluid-dynamics/adaptive-mesh-refinement-amr
https://www.cttc.upc.edu/?q=node/165
https://perswww.kuleuven.be/~u0016541/MHD_sheets_pdf/SolaireBochum08B.pdf
https://depts.washington.edu/clawpack/v5.4.0alpha/amr_algorithm.html

Referenced by pages:
adaptive refinement tree (ART)
Castro
computational astrophysics
Enzo
numerical methods
RAMSES

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