export read_mdim()
, a reader using GDAL’s
multidimensional array API (for sf <= 1.0-8)
remove tos_O1_2001-2002.nc
from packaged datasets to
keep source package size below 5 Mb
as.POSIXct.stars()
converts PCICt
dimensions to POSIXct
values.
improve handling of PCICt
360 or 365 day calendars;
read them in read_mdim
(requires sf >= 1.0-9)
read_stars()
reads factor levels better from
attribute table; #484 thanks to @ailich
read_stars()
puts band names from
band_meta
DESCRIPTION= tags into
values
;
improve handling of categorical rasters, and their exchange with
terra
; #484
plot()
handles auto colors better for factor
arrays
read_ncdf()
handles units more formally in setting
crs; #533
print message that dimensions of proxy objects do not reflect unevaluated operations; #530
passing na.action = na.omit
to
geom_stars()
removes NA
values; #532
read_stars()
detects curvilinear grids
automatically; #513
st_warp()
warps curvilinear grids (using Euclidean
distances only on coordinates); #513
Ops.stars()
errors when (common) dimension are not
identical; #506
guess_raster()
accepts empty rows/columns and sparse
grids; #509
speed up rgb
plotting; #503
Added a new helper function st_tile()
to specify the
block parameters (nXOff
, nYOff
,
nXsize
, nYSize
) required by
RasterIO
argument in read_stars()
; #492 thanks
to Krzysztof Dyba
st_as_stars.bbox()
creates an empy raster file if
proxy = TRUE
; #489
st_rasterize()
has option align = TRUE
to use a template for aligning the new raster to; #489
adrop.stars()
with missing dimensions no longer
drops x/y raster dimensions; #485
aggregate.stars()
propagates units of arrays;
#477
c.stars()
fails if it tries to merge arrays with
different units; #475
For NetCDF files, read_stars()
uses the
long_name
as array name; #475
add rename()
method; #470
refresh CRS of packaged L7_ETMs.tif
; #466
as.data.frame.stars()
works for mixed regular and
rectilinear dimension; #458
plot.stars()
plots curvilinear rasters with color
table, or without table but col
argument passed;
#456
st_extract()
accepts a matrix with points as
at
argument, for when performance is important; see
e.g. https://github.com/rspatial/terra/issues/341
fix bug in st_crop()
when cropping area is larger
than grid; #455
export st_downsample()
, e.g. to be used by
tmap
; https://github.com/r-tmap/tmap/issues/597
argument downsample
in plot.stars()
and
st_as_stars.stars_proxy()
and st_downsample()
has the same effect (removed a one-offset between them).
st_redimension()
works for curvilinear grids;
#441
downsample
is propagated to subexpressions like
r[r < 50] = NA
predict.stars()
obtains an argument
drop_dimensions
that, if TRUE
, drops
dimensions from the prediction data.frame
; #362
extend options in st_rgb()
, #432, by Gabo
Gaona
allow subsetting with [
by using labels, e.g. of
band names.
read_stars()
accepts a function (or list with
functions) as first argument, allowing for saving stars
objects that read from package directories resolving platform-dependent
paths at run-time
handle categorical rasters starting at value 0 (by adding 1, and warning); #428
add %in%
method; #424
read_stars()
gains an argument
tolerance
to control tolerance in dimension value
comparisons; #414
binary Ops (like +
, -
, *
etc.) work for stars_proxy
objects; #390
st_rasterize()
rasterizes multiple attributes, and
handles factors (when sf >= 0.9-9)
write_stars()
deals better with
stars_proxy
objects; #404
fix regression in reading some stars_proxy
objects;
#379
add [<-
(partially) and is.na
methods for stars_proxy
objects; #402
add replace_na()
methods; #402
read and write factor levels as GDAL category names; write color table; #392
handle normalize_path
for choosing to
proxy
; #391
ignore units when there are different units accross bands of a subdataset
speed up st_rgb()
using faster
st_apply()
approach; #315, #390
improve handling of crs in Spatial objects (avoid loss of wkt comments)
correctly write band subsets for smaller proxy objects; #291
write arbitrarily cropped proxy objects; #291
speed up st_apply()
when a function is provided that
works on chunks at a time; #390
warn when breaks = “quantile” results in a single class; #388
fix [
bug selecting bands in proxy objects;
#388
for stars_proxy
objects, write_stars()
writes all objects into a multi-layer file; #385
multi-file proxy objects can be st_warp()
ed with
use_gdal = TRUE
; #385
fix weird GDAL-related bug in stars2 vignette
read_ncdf()
does not take time as mid-points of
regular intervals, but as starting points; #378
fix handling of rasters with color tables; #375
st_apply()
and other methods for
stars_proxy
objects handle … ; #374
add st_bbox()
, st_crs()
methods for
terra’s SpatVector
objects;
https://github.com/mtennekes/tmap/issues/536
add st_bbox()
, st_crs()
and
st_as_stars()
methods for terra’s SpatRaster
objects; https://github.com/mtennekes/tmap/issues/536
allow for multi-resolution attributes in stars_proxy
objects (e.g., all gray scale sentinel-2 bands); see vignettes 2 and 7
for examples.
plot()
defaults to a categorical color scale when
plotting a factor variable;
https://github.com/mtennekes/tmap/issues/526
st_extract()
extracts space-time points if
time_column
is specified, and handles time intervals;
#352
add [[<-.stars
method, which is now called by
$<-.stars
, so that array names can be set
programmatically
add transmute()
methods
plot.stars()
calls droplevels
if a
factor array has any NA
levels; #339
read_stars()
reads NaN
s as
NA
; #333
improve st_extract()
method for both
stars
and stars_proxy
objects; interpolation
options are reduced to bilinear; #322, #279, #290
better handle categorical rasters that do not start at value 1; #329
plot layout can be controlled with mfrow = c(nr, nc)
argument
stars_proxy
objects have a normalized path;
#331
cropping or selecting with bbox
treats cells always
as small polygons; #330
add faster st_extract()
method for
stars
objects; #322
added vignette: “How raster
functions map to
stars
functions”, by Sebastien Rochette; #122,
#325
fix bug in dimension values
field when downsampling;
#324
write_stars()
also writes out band names;
#323
add rgdal
to Suggests:
each call_list
entry of a stars_proxy
object carries its proper calling environment; #309
st_as_sf.stars()
copes with zero attribute (empty)
stars objects
add st_set_bbox()
generic, to set raster extent,
motivated by #315
set up tic, with great help from @pat-s, #313
get rid of more proj4string
s for representing
coordinate reference systems; #312
as(x, “Spatial”) correctly handles from
dimension
values different from one
read_stars()
now sets the BANDNAME
GDAL
metadata item, or else the band’s GetDescription() as the band’s
dimension values
st_as_stars.data.frame()
reads simple tables
(non-raster data) if dims
has length less than 2
band descriptions are in the band dimension values
dimension tables are simpler, and are shown properly in Rstudio
st_rgb()
gains a probs
argument, to cut
off and stretch based on quantiles
as(x, "Raster")
merges multiple attributes before
converting to raster brick
fix bug in st_as_stars.Raster
; set crs to the one
assigned by raster;
https://github.com/mtennekes/tmap/issues/471
add s2
to Suggests:
new function st_rgb()
collapses (reduces) a
dimension to rgb hex value; #302
aggregate.stars()
handles arrays with NA values now
correctly; brought up in #299 by Thorsten Simon
aggregate.stars()
gains an argument
exact
which, if TRUE
, calls
exactextractr
for polygonal aggregation; #289
read_stars()
reads all subdatasets with dimensions
equal to first, and warns when ignoring others; #296
make copying over of dimensions somewhat easier; #295
st_as_stars.Raster()
tries to read from file if the
raster object is not an in-memory object.
write_stars()
normalizes path, as
read_stars
already did; #293
merge()
for proxy objects acts, and is no longer
lazy; #290
st_as_stars.Raster()
returns a proxy object if the
raster layer is on disk
add st_extract()
to extract e.g. time series from
grids at point locations; #279; #290
read_stars()
chooses a value for proxy
that depends on the data dimensions; #281
x/y range subsetting of stars_proxy
objects now only
reads that range, similar to how crop already did this.
st_warp()
preserves levels and colors;
https://github.com/mtennekes/tmap/issues/429
st_crop()
works with bounding boxes larger than the
downsampled bounding box; #276
st_crop()
has a non-zero default for
epsilon
(bounding box shrinkage) to exclude cells touching
the crop bounding box; #275
image.stars()
(and hence plot.stars
)
gains an extent
argument for setting the extent of a plot;
https://github.com/r-spatial/sf/issues/1193
st_warp()
(stars native) flips longitudes a full
cycle; #256, #264, #269
handle axis order in st_transform
(requires sf >=
0.9-1)
depend on sf 0.9-0
adapt to cubelyr split-off from dplyr; add cubelyr to Suggests:; https://github.com/hadley/cubelyr/issues/2
add droplevels()
method
handle color tables, category tables and raster attribute tables read through GDAL; #128, #245; https://github.com/r-spatial/mapview/issues/208
handle dimension crs
specially, for proxy objects
now.
handle new-style crs
objects from upcoming sf,
moving away from proj4strings
handle full crs
objects as refsys
element in a spatial dimensions, rather than proj4string only
st_raster_type(x)
reveals the raster type of
x
; #248,
https://github.com/mtennekes/tmap/issues/368
add st_as_stars.OpenStreetMap()
method; #241 by
@mtennekes
add st_flip()
to flip arrays along one or more
dimensions without changing dimension properties
add as.owin()
method to convert (2D raster) stars
objects to spatstat owin
;
https://github.com/r-spatial/sf/issues/1233
for temporal aggregation, aggregate.stars
now also
takes by
arguments like “week”, “month”, or “5
days”
add st_as_stars()
method for xts
objects; improve as.xts
for stars
objects
skip some tests on solaris
plot()
now uses all data to figure out breaks, in
order to also find extremes; #216
st_mosaic()
creates mosaics from spatially disjoint
rasters; #210
#205 large refactoring of read_ncdf
, by David
Blodgett and Mike Sumner, affecting #199, #89, #30, #86, #175
allow for funny units like m s**-1
; #201
add contour()
method for stars
objects;
#196
plot uses rasterImage
by default if available;
#194
the x
and y
raster dimensions can be
set and unset with xy
argument in
st_set_dimensions
; #190
retain factor
levels with dimension values when set
in st_set_dimensions
; #188
add conversion from stars_proxy
to
Raster
: #193
make plotting of multiple curvilinear grids work
plot by default no cell borders in case of curvilinear, rotated or sheared grids
robustify handling of units
allow read_ncdf()
to ignore bounds
scale was applied wrongly on multi-band images; #189, this requires sf >= 0.7-5
.nc
is now recognized correctly by
write_stars
and will write a NetCDF file; #186
[
subset now works correctly with negative or
logical indices; #184, #185
NA
values for float32 grids are now correctly
detected; #182, this requires sf >= 0.7-5
cropping of a stars_proxy
object now works;
#179
st_apply()
can now loop over Raster layers; examples
in #176
st_as_stars.bbox
now has an ncells
and
pretty
argument, to better choose default raster
dimensions
geom_stars
now works with stars_proxy
objects, but needs downsample
to be set; #21
NA
values in Float32 rasters are now read correctly
with read_stars
; #182
handle bounds, when given, in read_ncdf
provide time parsing (POSIXct, PCICt) for read_ncdf
;
#115
add st_area
method to return raster grid cell sizes;
#99
fix st_warp
with use_gdal=TRUE
,
allowing for multi-band warps
add st_get_dimension_values
to get the values of a
particular dimension (if meaningful); #100
allow for setting intervals as dimension values; see examples of
st_dimensions
add st_contour
, and clean up st_as_sf
;
#99
experimental color table support; https://github.com/r-spatial/mapview/issues/208
rewrote vignettes, added vignettes; #99
deprecate st_write.stars
for
write_stars
; #96
use “native” R array-factor support
support for PCICt
360- and 365-day calendars;
#29
remove import of ncdf4
in favour of
RNetCDF
, now in line with practice in ncmeta
package. Thanks to David Blodgett for motivation and testing (see #87,
#94).
st_as_sf
uses date/time column names when
appropriate
allow missing trailing comma’s when subsetting:
a[1,,]
and a[1,]
now do the same.
move rlang
to Imports: ; rewrite [
subset using rlang.
add conversion to and from Spatial*
classes,
including the gridded ones, taking care of factor
variables
depend on sf 0.7-2
add logz support for log-scale keys to plot
and
image
vignettes now use an external package, starsdata
,
for larger dataset examples
support [<-.stars
e.g. to mask out values;
support is.na.stars
to replace NA masks
support cut
methods and factor arrays (plot,
subset); #56
add st_rasterize
, which uses
GDALRasterize
to rasterize an sf object; #13
st_as_sf.stars
now uses
GDAL(F)Polygonize
when give a regular or sheared grid grid
cells are not points, and returns contour bands using
GDALContourGenerateEx
(requiring GDAL 2.4.0) in case cells
are points; #13
support curvilinear grids; see #54 and the
data_model
vignette
add vignette about how stars_proxy
objects
work
stars_proxy
objects defer processing of
st_apply
jobs until after subsampling; #50
allow reading sections of a raster, raster at a lower resolution, selected bands; #48
allow reading vectors (arrays) with more than 2^31 elements; #48
fold all higher dimensions into the third dimension before
coercing to Raster
; #40
read_stars
add merge
(merge attributes into array dimension)
and split
(split dimension over attributes)
interface to sf, raster and spacetime
improve plotting
handle logical
arrays in plot
add st_apply
, analogous to
apply
add cropping/masking when used as x[buf] with buf an
sf
, sfc
or bbox
object; masking
when x[buf, crop = FALSE]
add Ops (+,-,/ etc) and Math (sqrt, pow, sin etc) methods
add dimnames
and dimnames<-
methods
for stars objects
downsample large grids to only plot pixels actually shown
can plot rectilinear grids (but will plot rgb images as regular grids)
rgb
argument to image
works
[
array-like subsetting works; first index is
attribute selector
gdal_utils()
(now part of sf
)