Everything about Gaussian Grid totally explained
A
Gaussian grid is used in the
earth sciences as a
grid for
scientific modeling on a
sphere (for example, the approximate
shape of the
Earth). The grid is rectangular, with a set number of
orthogonal coordinates (usually
latitude and
longitude), such that they can be easily accessed in a fixed
array.
The longitudes are equally spaced, while the latitudes are
not equally spaced, and are defined by their
Gaussian quadrature. There are no grid points at the
poles, and the number of longitudes are usually double the number of latitudes.
A
reduced Gaussian grid can also be used, in which the number of gridpoints in the rows decreases towards the poles, which keeps the grid-point separation approximately constant across the sphere.
Naming conventions
The names of Gaussian grids often have a
T,
R, or
N, followed by a number (for example, T62). This indicates the type of
spectral truncation used and the
wavenumber. The
T indicates
triangular truncation, the
R indicates
rhomboidal truncation, while the
N indicates the largest
associated Legendre polynomial for the
wavenumber (which is also the number of grid points between the
equator and
pole). Grid names can also have an
L followed again by a number, which indicates the number of vertical levels to the model grid (for example,
CGCM2 has a T32L10 atmospheric grid).
Examples of Gaussian grids
Further Information
Get more info on 'Gaussian Grid'.
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