Source code for pygmt.datasets.earth_night

"""
Function to download the NASA Black Marble image datasets from the GMT data server, and
load as :class:`xarray.DataArray`.

The images are available in various resolutions.
"""

import contextlib
from collections.abc import Sequence
from typing import Literal

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

with contextlib.suppress(ImportError):
    # rioxarray is needed to register the rio accessor
    import rioxarray  # noqa: F401

__doctest_skip__ = ["load_black_marble"]


[docs] def load_black_marble( resolution: Literal[ "01d", "30m", "20m", "15m", "10m", "06m", "05m", "04m", "03m", "02m", "01m", "30s", ] = "01d", region: Sequence[float] | str | None = None, ) -> xr.DataArray: r""" Load NASA Black Marble images in various resolutions. .. figure:: https://www.generic-mapping-tools.org/remote-datasets/_images/GMT_earth_daynight.jpg :width: 80% :align: center Earth day/night dataset. This function downloads the dataset from the GMT data server, caches it in a user data directory (usually ``~/.gmt/server/earth/earth_night/``), 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: **@earth_night**\_\ *res*. *res* is the grid resolution. If *res* is omitted (i.e., ``@earth_night``), GMT automatically selects a suitable resolution based on the current region and projection settings. Refer to :gmt-datasets:`earth-daynight.html` for more details about available datasets, including version information and references. Parameters ---------- resolution The image resolution. The suffix ``d``, ``m``, and ``s`` stand for arc-degrees, arc-minutes, and arc-seconds. region The subregion of the image to load, in the form of a sequence [*xmin*, *xmax*, *ymin*, *ymax*]. Returns ------- image The NASA Black Marble image. Coordinates are latitude and longitude in degrees. Note ---- The registration and coordinate system type of the returned :class:`xarray.DataArray` image can be accessed via the GMT accessors (i.e., ``image.gmt.registration`` and ``image.gmt.gtype`` respectively). However, these properties may be lost after specific image operations (such as slicing) and will need to be manually set before passing the image to any PyGMT data processing or plotting functions. Refer to :class:`pygmt.GMTDataArrayAccessor` for detailed explanations and workarounds. Examples -------- >>> from pygmt.datasets import load_black_marble >>> # Load the default image (pixel-registered 1 arc-degree image) >>> image = load_black_marble() """ image = _load_remote_dataset( name="earth_night", prefix="earth_night", resolution=resolution, region=region, registration="pixel", ) # If rioxarray is installed, set the coordinate reference system if hasattr(image, "rio"): image = image.rio.write_crs(input_crs="OGC:CRS84") return image