"""
xyz2grd - Convert data table to a grid.
"""
import xarray as xr
from pygmt.clib import Session
from pygmt.exceptions import GMTInvalidInput
from pygmt.helpers import build_arg_list, fmt_docstring, kwargs_to_strings, use_alias
__doctest_skip__ = ["xyz2grd"]
[docs]
@fmt_docstring
@use_alias(
A="duplicate",
I="spacing",
J="projection",
R="region",
V="verbose",
Z="convention",
b="binary",
d="nodata",
e="find",
f="coltypes",
h="header",
i="incols",
r="registration",
w="wrap",
)
@kwargs_to_strings(I="sequence", R="sequence")
def xyz2grd(
data=None, x=None, y=None, z=None, outgrid: str | None = None, **kwargs
) -> xr.DataArray | None:
r"""
Create a grid file from table data.
Reads one or more tables with *x, y, z* columns and creates a binary grid
file. :func:`pygmt.xyz2grd` will report if some of the nodes are not filled
in with data. Such unconstrained nodes are set to a value specified by the
user [Default is NaN]. Nodes with more than one value will be set to the
mean value.
Full option list at :gmt-docs:`xyz2grd.html`
{aliases}
Parameters
----------
data : str, {table-like}
Pass in (x, y, z) or (longitude, latitude, elevation) values by
providing a file name to an ASCII data table, a 2-D {table-classes}.
x/y/z : 1-D arrays
The arrays of x and y coordinates and z data points.
{outgrid}
duplicate : str
[**d**\|\ **f**\|\ **l**\|\ **m**\|\ **n**\|\
**r**\|\ **S**\|\ **s**\|\ **u**\|\ **z**].
By default we will calculate mean values if multiple entries fall on
the same node. Use ``duplicate`` to change this behavior, except it is
ignored if ``convention`` is given. Append **f** or **s** to simply
keep the first or last data point that was assigned to each node.
Append **l** or **u** or **d** to find the lowest (minimum) or upper
(maximum) value or the difference between the maximum and minimum
values at each node, respectively. Append **m** or **r** or **S** to
compute mean or RMS value or standard deviation at each node,
respectively. Append **n** to simply count the number of data points
that were assigned to each node (this only requires two input columns
*x* and *y* as *z* is not consulted). Append **z** to sum multiple
values that belong to the same node.
{spacing}
{projection}
{region}
{verbose}
convention : str
[*flags*].
Read a 1-column ASCII [or binary] table. This assumes that all the
nodes are present and sorted according to specified ordering
convention contained in *flags*. If incoming data represents rows,
make *flags* start with **T**\ (op) if first row is y
= ymax or **B**\ (ottom) if first row is y = ymin.
Then, append **L** or **R** to indicate that first element is at
left or right end of row. Likewise for column formats: start with
**L** or **R** to position first column, and then append **T** or
**B** to position first element in a row. **Note**: These two
row/column indicators are only required for grids; for other tables
they do not apply. For gridline registered grids: If data are periodic
in x but the incoming data do not contain the (redundant) column at
x = xmax, append **x**. For data periodic in y without redundant row at
y = ymax, append **y**. Append **s**\ *n* to skip the first *n* number
of bytes (probably a header). If the byte-order or the words needs
to be swapped, append **w**. Select one of several data types (all
binary except **a**):
- **A** ASCII representation of one or more floating point values per
record
- **a** ASCII representation of a single item per record
- **c** int8_t, signed 1-byte character
- **u** uint8_t, unsigned 1-byte character
- **h** int16_t, signed 2-byte integer
- **H** uint16_t, unsigned 2-byte integer
- **i** int32_t, signed 4-byte integer
- **I** uint32_t, unsigned 4-byte integer
- **l** int64_t, long (8-byte) integer
- **L** uint64_t, unsigned long (8-byte) integer
- **f** 4-byte floating point single precision
- **d** 8-byte floating point double precision
[Default format is scanline orientation of ASCII numbers: **La**].
The difference between **A** and **a** is that the latter can decode
both *date*\ **T**\ *clock* and *ddd:mm:ss[.xx]* formats but expects
each input record to have a single value, while the former can handle
multiple values per record but can only parse regular floating point
values. Translate incoming *z*-values via the ``incols`` parameter.
{binary}
{nodata}
{find}
{coltypes}
{header}
{incols}
{registration}
{wrap}
Returns
-------
ret
Return type depends on whether the ``outgrid`` parameter is set:
- :class:`xarray.DataArray`: if ``outgrid`` is not set
- None if ``outgrid`` is set (grid output will be stored in file set by
``outgrid``)
Example
-------
>>> import numpy as np
>>> import pygmt
>>> # generate a grid for z=x**2+y**2, with an x-range of 0 to 3,
>>> # and a y-range of 10.5 to 12.5. The x- and y-spacings are 1.0 and 0.5.
>>> x, y = np.meshgrid([0, 1, 2, 3], [10.5, 11.0, 11.5, 12.0, 12.5])
>>> z = x**2 + y**2
>>> xx, yy, zz = x.flatten(), y.flatten(), z.flatten()
>>> grid = pygmt.xyz2grd(
... x=xx, y=yy, z=zz, spacing=(1.0, 0.5), region=[0, 3, 10, 13]
... )
"""
if kwargs.get("I") is None or kwargs.get("R") is None:
raise GMTInvalidInput("Both 'region' and 'spacing' must be specified.")
with Session() as lib:
with (
lib.virtualfile_in(
check_kind="vector", data=data, x=x, y=y, z=z, required_z=True
) as vintbl,
lib.virtualfile_out(kind="grid", fname=outgrid) as voutgrd,
):
kwargs["G"] = voutgrd
lib.call_module(
module="xyz2grd", args=build_arg_list(kwargs, infile=vintbl)
)
return lib.virtualfile_to_raster(vfname=voutgrd, outgrid=outgrid)