"""
xyz2grd - Convert data table to a grid.
"""
from pygmt.clib import Session
from pygmt.helpers import (
    GMTTempFile,
    build_arg_string,
    fmt_docstring,
    kwargs_to_strings,
    use_alias,
)
from pygmt.io import load_dataarray
[docs]@fmt_docstring
@use_alias(
    A="duplicate",
    G="outgrid",
    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(R="sequence")
def xyz2grd(data=None, x=None, y=None, z=None, **kwargs):
    r"""
    Create a grid file from table data.
    Reads one or more tables with *x, y, z* columns and creates a binary grid
    file. 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 or {table-like}
        Pass in (x, y, z) or (longitude, latitude, elevation) values by
        providing a file name to an ASCII data table, a 2D {table-classes}.
    x/y/z : 1d arrays
        The arrays of x and y coordinates and z data points.
    outgrid : str or None
        Optional. The name of the output netCDF file with extension .nc to
        store the grid in.
    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 **-A** to change this behavior, except it is
        ignored if **-Z** 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 miminum value
        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.
    {I}
    {J}
    {R}
    {V}
    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: **-ZTLa**.
        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.
    {b}
    {d}
    {e}
    {f}
    {h}
    {i}
    {r}
    {w}
    Returns
    -------
    ret: xarray.DataArray or None
        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``)
    """
    with GMTTempFile(suffix=".nc") as tmpfile:
        with Session() as lib:
            file_context = lib.virtualfile_from_data(
                check_kind="vector", data=data, x=x, y=y, z=z, required_z=True
            )
            with file_context as infile:
                if "G" not in kwargs:  # if outgrid is unset, output to tempfile
                    kwargs.update({"G": tmpfile.name})
                outgrid = kwargs["G"]
                arg_str = " ".join([infile, build_arg_string(kwargs)])
                lib.call_module("xyz2grd", arg_str)
        return load_dataarray(outgrid) if outgrid == tmpfile.name else None