c_cssgridd(3NCARG)
π c_cssgridd β tension spline interpolation on a sphere π
okay bestie, sit down, hydrate, because we're about to talk about c_cssgridd from the NCAR GRAPHICS manual (that's 3NCARG, iykyk). it's giving β¨mathβ¨ but make it cute. no cap, this one is a whole vibe. π¦
β¨ FUNCTION PROTOTYPE β¨
here's the exact signature, copy it like your life depends on it (it does):
double *c_cssgridd(int, double [], double [], double [],
int, int, double [], double [], int *);
πΈ SYNOPSIS πΈ
and here it is with the actual argument names, because we're extra like that:
double *c_cssgridd (n, rlat, rlon, f, ni, nj, plat, plon, ier)
π DESCRIPTION π
every single argument, no skips, periodt:
nβ the number of input data points you're feeding in. and it has to ben > 2, okay?? like, we need at least three, that's the floor, that's the bare minimum, bestie.rlatβ an array holding the latitudes of your input data, in degrees. β οΈ big warning energy here: the first three points must not be collinear, meaning they cannot all lie on a common great circle. do not test this. she will know.rlonβ an array with the longitudes of your input data, also in degrees. πfβ the array of data values.f[i]is the functional value at(rlat[i],rlon[i])fori = 0ton-1. so like, index-matched, they're a set, they come as a group, do not separate them. π«Άniβ the number of latitudes in the interpolated grid you want back.njβ the number of longitudes in the interpolated grid. and here's the fun part:niandnjcan both be 1, which lets you interpolate at a single point. one point! main character energy, honestly. βplatβ an array of the latitudes of the points where you want the interpolated values computed. the values inplatshould be in degrees. πplonβ an array of lengthnjcontaining the longitudes of the output grid lines. the values inplonshould be in degrees too. consistent queen. πierβ the error return value, aka the vibe check. if*iercomes back as0, then no errors were detected, we ate, we're slaying. if*ieris non-zero, then go refer to the error list incssgrid_errorsfor the details. π
π USAGE π
you call c_cssgridd when you want to find an interpolating tension spline for randomly positioned data on a unit sphere. yes, a sphere. we're doing spherical geometry, we're doing it cute. π
also, tiny flex: c_cssgridd is the double precision version of c_cssgrid. so if you want the double precision girlies, that's her. β¨
π₯ RETURN VALUE π₯
c_cssgridd returns a pointer to a linear array of data that holds the interpolated values at the user-specified lat/lon pairs. and the way it stores them?? as if it were a 2-dimensional C array with latitude as the first dimension and longitude as the second dimension. structured. organized. iconic. π
so if out is declared like this:
double *out;
and then we set:
out = c_cssgridd(n, rlat, rlon, f, nlat, nlon, plat, plon, &ier);
then out[i*nlon+j] is the interpolated function value at coordinate point (plat[i], plon[j]) for 0 <= i < nlat and 0 <= j < nlon. that's the indexing math, bestie, memorize it. π§ β¨
and the space for out is allocated internal to c_cssgridd, and it's nlat * nlon doubles in size. so don't you dare allocate it yourself, she's handling it, she's got it. π«Ά
π ACCESS π
to use c_cssgridd, you load the NCAR Graphics library ngmath. that's it, that's the whole trick. π
π¦ SEE ALSO π¦
c_cssgridcss_overviewcssgrid_errors
and also!! complete documentation for Cssgrid is available at this URL:
http://ngwww.ucar.edu/ngdoc/ng/ngmath/cssgrid/csshome.html
go read it, bestie, it's right there. π
π COPYRIGHT π
Copyright (C) 2000 University Corporation for Atmospheric Research
The use of this Software is governed by a License Agreement.
okay that's the whole page, you're officially educated on c_cssgridd πβ¨ this was written up for the UNIX manual, May 2000, and yes she's been serving interpolation excellence since then. now go interpolate something cute. mwah. π
ππ¦
π¦ where this page comes from
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- ubuntu stonking: libncarg-dev 6.6.2.dfsg.1-12build2
- π girlified by deepseek-ai/DeepSeek-V4.1-Flash on : a language model's rewrite of the original, under its terms