convert objects into a stars object
st_as_stars(.x, ...)# S3 method for list
st_as_stars(.x, ..., dimensions = NULL)
# S3 method for default
st_as_stars(.x = NULL, ..., raster = NULL)
# S3 method for stars
st_as_stars(.x, ..., curvilinear = NULL,
crs = st_crs(4326))
# S3 method for bbox
st_as_stars(.x, ..., nx = 360, ny = 180,
xlim = .x[c("xmin", "xmax")], ylim = .x[c("ymin", "ymax")],
values = runif(nx * ny))
# S3 method for sf
st_as_stars(.x, ...)
# S3 method for Raster
st_as_stars(.x, ...)
# S3 method for stars_proxy
st_as_stars(.x, ..., downsample = 0)
object to convert
ignored
object of class dimensions
character; the names of the dimensions that denote raster dimensions
only for creating curvilinear grids: named length 2 list holding longitude and latitude matrices; the names of this list should correspond to raster dimensions to be replaced
object of class crs with the coordinate reference system of the values in curvilinear; see details
integer; number of cells in x direction
integer; number of cells in y direction
length 2 numeric vector with extent in x direction
length 2 numeric vector with extent in y direction
value(s) to populate the raster values with
integer: if larger than 0, downsample with this rate (number of pixels to skip in every row/column)
if curvilinear is a stars object with longitude and latitude values, its coordinate reference system is typically not that of the latitude and longitude values.