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mpim-sw
cdo
Commits
5f5e6cf3
Commit
5f5e6cf3
authored
Sep 11, 2017
by
Uwe Schulzweida
Browse files
Docu update.
parent
9ac8387b
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doc/tex/mod/Spectral
doc/tex/mod/Spectral
+4
-3
doc/tex/mod/Wind
doc/tex/mod/Wind
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-1
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doc/tex/mod/Spectral
View file @
5f5e6cf3
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@@ -8,7 +8,8 @@
@Operators = sp2gp sp2gpl gp2sp gp2spl sp2sp
@BeginDescription
This module transforms fields on Gaussian grids to spectral coefficients and vice versa.
This module transforms fields on a global regular Gaussian grids to spectral coefficients and vice versa.
Missing values are not supported.
@EndDescription
@EndModule
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@@ -17,7 +18,7 @@ This module transforms fields on Gaussian grids to spectral coefficients and vic
@Title = Spectral to gridpoint
@BeginDescription
Convert all fields with spectral coefficients to a regular Gaussian grid. The number of
Convert all fields with spectral coefficients to a
global
regular Gaussian grid. The number of
latitudes of the resulting Gaussian grid is calculated from the triangular truncation by:
@IfMan
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@@ -37,7 +38,7 @@ latitudes of the resulting Gaussian grid is calculated from the triangular trunc
@Title = Spectral to gridpoint (linear)
@BeginDescription
Convert all fields with spectral coefficients to a regular Gaussian grid. The number of
Convert all fields with spectral coefficients to a
global
regular Gaussian grid. The number of
latitudes of the resulting Gaussian grid is calculated from the triangular truncation by:
@IfMan
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...
doc/tex/mod/Wind
View file @
5f5e6cf3
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@@ -11,7 +11,7 @@
This module converts relative divergence and vorticity to U and V wind and vice versa.
Divergence and vorticity are spherical harmonic coefficients in spectral space and
U and V are on a global regular Gaussian grid. The Gaussian latitudes need to be ordered from
north to south.
north to south.
Missing values are not supported.
@EndDescription
@EndModule
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