Source code for pygmt.src.grdgradient

"""
grdgradient - Create a gradient from a grid.
"""

import xarray as xr
from pygmt.clib import Session
from pygmt.helpers import (
    GMTTempFile,
    build_arg_string,
    fmt_docstring,
    kwargs_to_strings,
    use_alias,
)


[docs]@fmt_docstring @use_alias( A="azimuth", D="direction", E="radiance", G="outgrid", R="region", V="verbose", ) @kwargs_to_strings( A="sequence", R="sequence", ) def grdgradient(grid, **kwargs): r""" Full option list at :gmt-docs:`grdgradient.html` {aliases} Parameters ---------- grid : str or xarray.DataArray The file name of the input grid or the grid loaded as a DataArray. outgrid : str or None The name of the output netCDF file with extension .nc to store the grid in. azimuth : str or list or xarray.DataArray *azim*\ [/*azim2*]. Azimuthal direction for a directional derivative; *azim* is the angle in the x,y plane measured in degrees positive clockwise from north (the +y direction) toward east (the +x direction). The negative of the directional derivative, -[dz/dx\*sin(*azim*) + dz/dy\*cos(\ *azim*)], is found; negation yields positive values when the slope of z(x,y) is downhill in the *azim* direction, the correct sense for shading the illumination of an image by a light source above the x,y plane shining from the *azim* direction. Optionally, supply two azimuths, *azim*/*azim2*, in which case the gradients in each of these directions are calculated and the one larger in magnitude is retained; this is useful for illuminating data with two directions of lineated structures, e.g., *0*/*270* illuminates from the north (top) and west (left). Finally, if *azim* is a file it must be a grid of the same domain, spacing and registration as *ingrid* that will update the azimuth at each output node when computing the directional derivatives. direction : str [**a**][**c**][**o**][**n**]. Find the direction of the positive (up-slope) gradient of the data. To instead find the aspect (the down-slope direction), use **a**. By default, directions are measured clockwise from north, as *azim* in ``azimuth``. Append **c** to use conventional Cartesian angles measured counterclockwise from the positive x (east) direction. Append **o** to report orientations (0-180) rather than directions (0-360). Append **n** to add 90 degrees to all angles (e.g., to give local strikes of the surface). radiance : str [**m**\|\ **s**\|\ **p**]\ *azim/elev*\ [**+a**\ *ambient*][**+d**\ *diffuse*][**+p**\ *specular*][**+s**\ *shine*]. Compute Lambertian radiance appropriate to use with ``grdimage`` and ``grdview``. The Lambertian Reflection assumes an ideal surface that reflects all the light that strikes it and the surface appears equally bright from all viewing directions. Here, *azim* and *elev* are the azimuth and elevation of the light vector. Optionally, supply *ambient* [0.55], *diffuse* [0.6], *specular* [0.4], or *shine* [10], which are parameters that control the reflectance properties of the surface. Default values are given in the brackets. Use **s** for a simpler Lambertian algorithm. Note that with this form you only have to provide azimuth and elevation. Alternatively, use **p** for the Peucker piecewise linear approximation (simpler but faster algorithm; in this case the *azim* and *elev* are hardwired to 315 and 45 degrees. This means that even if you provide other values they will be ignored.) {R} {V} """ with GMTTempFile(suffix=".nc") as tmpfile: with Session() as lib: file_context = lib.virtualfile_from_data(check_kind="raster", data=grid) with file_context as infile: if "G" not in kwargs.keys(): # 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("grdgradient", arg_str) if outgrid == tmpfile.name: # if user did not set outgrid, return DataArray with xr.open_dataarray(outgrid) as dataarray: result = dataarray.load() _ = result.gmt # load GMTDataArray accessor information else: result = None # if user sets an outgrid, return None return result