Source code for pygmt.datasets.moon_relief

"""
Function to download the Moon relief dataset from the GMT data server, and load as
:class:`xarray.DataArray`.

The grids are available in various resolutions.
"""

from collections.abc import Sequence
from typing import Literal

import xarray as xr
from pygmt.datasets.load_remote_dataset import _load_remote_dataset

__doctest_skip__ = ["load_moon_relief"]


[docs] def load_moon_relief( resolution: Literal[ "01d", "30m", "20m", "15m", "10m", "06m", "05m", "04m", "03m", "02m", "01m", "30s", "15s", "14s", ] = "01d", region: Sequence[float] | str | None = None, registration: Literal["gridline", "pixel", None] = None, ) -> xr.DataArray: r""" Load the Moon relief dataset in various resolutions. .. figure:: https://www.generic-mapping-tools.org/remote-datasets/_images/GMT_moon_relief.jpg :width: 80% :align: center Moon relief dataset. This function downloads the dataset from the GMT data server, caches it in a user data directory (usually ``~/.gmt/server/moon/moon_relief/``), and load the dataset as an :class:`xarray.DataArray`. An internet connection is required the first time around, but subsequent calls will load the dataset from the local data directory. The dataset can also be accessed by specifying a file name in any grid processing function or plotting method, using the following file name format: **@moon_relief**\_\ *res*\_\ *reg*. *res* is the grid resolution; *reg* is the grid registration type (**p** for pixel registration, **g** for gridline registration). If *reg* is omitted (e.g., ``@moon_relief_01d``), the gridline-registered grid will be loaded for grid processing functions and the pixel-registered grid will be loaded for plotting functions. If *res* is also omitted (i.e., ``@moon_relief``), GMT automatically selects a suitable resolution based on the current region and projection settings. This dataset comes with a color palette table (CPT) file, ``@moon_relief.cpt``. To use the dataset-specific CPT when plotting the dataset, explicitly set ``cmap="@moon_relief.cpt"``, otherwise GMT's default CPT (*turbo*) will be used. If the dataset is referenced by the file name in a grid plotting method, the dataset-specific CPT file is used automatically unless another CPT is specified. Refer to :gmt-datasets:`moon-relief.html` for more details about available datasets, including version information and references. Parameters ---------- resolution The grid resolution. The suffix ``d``, ``m`` and ``s`` stand for arc-degrees, arc-minutes and arc-seconds. Note that ``"14s"`` refers to a resolution of 14.0625 arc-seconds. region The subregion of the grid to load, in the form of a sequence [*xmin*, *xmax*, *ymin*, *ymax*] or an ISO country code. Required for grids with resolutions higher than 5 arc-minutes (i.e., ``"05m"``). registration Grid registration type. Either ``"pixel"`` for pixel registration or ``"gridline"`` for gridline registration. Default is ``None``, which means ``"gridline"`` for all resolutions except for ``"14s"`` which is ``"pixel"`` only. Returns ------- grid The Moon relief grid. Coordinates are latitude and longitude in degrees. Relief is in meters. Note ---- The registration and coordinate system type of the returned :class:`xarray.DataArray` grid can be accessed via the *gmt* accessor. Refer to :class:`pygmt.GMTDataArrayAccessor` for detailed explanations and limitations. Examples -------- >>> from pygmt.datasets import load_moon_relief >>> # Load the default grid (gridline-registered 1 arc-degree grid) >>> grid = load_moon_relief() >>> # Load the 30 arc-minutes grid with "gridline" registration >>> grid = load_moon_relief(resolution="30m", registration="gridline") >>> # Load high-resolution (5 arc-minutes) grid for a specific region >>> grid = load_moon_relief( ... resolution="05m", ... region=[120, 160, 30, 60], ... registration="gridline", ... ) """ grid = _load_remote_dataset( name="moon_relief", prefix="moon_relief", resolution=resolution, region=region, registration=registration, ) return grid