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For a better version of the stars vignettes see https://r-spatial.github.io/stars/articles/
NetCDF data sources are available via more and less granular
files and/or OPeNDAP endpoints. This article demonstrates how
stars
enables discovery, access, and processing of NetCDF
data across a wide range of such source-data organization schemes.
We’ll start with some basics using datasets included with the
stars
installation. A call to read_ncdf()
, for
a dataset smaller than the default threshold, will just read in all the
data. Below we read in and display the reduced.nc
NetCDF
file.
library(stars)
f <- system.file("nc/reduced.nc", package = "stars")
(nc <- read_ncdf(f))
## no 'var' specified, using sst, anom, err, ice
## other available variables:
## lon, lat, zlev, time
## 0-360 longitude crossing the international date line encountered.
## Longitude coordinates will be 0-360 in output.
## Will return stars object with 16200 cells.
## No projection information found in nc file.
## Coordinate variable units found to be degrees,
## assuming WGS84 Lat/Lon.
## stars object with 4 dimensions and 4 attributes
## attribute(s):
## Min. 1st Qu. Median Mean 3rd Qu. Max. NA's
## sst [°C] -1.80 -0.03 13.655 12.9940841 24.8125 32.97 4448
## anom [°C] -7.95 -0.58 -0.080 -0.1847324 0.2100 2.99 4449
## err [°C] 0.11 0.16 0.270 0.2626872 0.3200 0.84 4448
## ice [percent] 0.01 0.47 0.920 0.7178118 0.9600 1.00 13266
## dimension(s):
## from to offset delta refsys values x/y
## lon 1 180 -1 2 WGS 84 (CRS84) NULL [x]
## lat 1 90 -90 2 WGS 84 (CRS84) NULL [y]
## zlev 1 1 NA NA NA 0
## time 1 1 NA NA POSIXct 1981-12-31 UTC
Let’s assume reduced.nc
was 10 years of hourly data,
rather than 1 time step. It would be over 10GB rather than about 130KB
and we would not be able to just read it all into memory. In this case,
we need a way to read the file’s metadata such that we could iterate
over it in a way that meets the needs of our workflow objectives. This
is where proxy = TRUE
comes in. Below, we’ll lower the
option that controls whether read_ncdf()
defaults to proxy
and use proxy = TRUE
to show both ways of getting
the same result.
old_options <- options("stars.n_proxy" = 100)
(nc <- read_ncdf(f, proxy = TRUE))
## no 'var' specified, using sst, anom, err, ice
## other available variables:
## lon, lat, zlev, time
## 0-360 longitude crossing the international date line encountered.
## Longitude coordinates will be 0-360 in output.
## No projection information found in nc file.
## Coordinate variable units found to be degrees,
## assuming WGS84 Lat/Lon.
## netcdf source stars proxy object from:
## [1] "[...]/reduced.nc"
##
## Available nc variables:
## sst
## anom
## err
## ice
##
## dimension(s):
## from to offset delta refsys values x/y
## lon 1 180 -1 2 WGS 84 (CRS84) NULL [x]
## lat 1 90 -90 2 WGS 84 (CRS84) NULL [y]
## zlev 1 1 NA NA NA 0
## time 1 1 NA NA POSIXct 1981-12-31 UTC
options(old_options)
The above shows that we have a NetCDF sourced stars proxy derived
from the reduced.nc
file. We see it has four variables and
their units are displayed. The normal stars
dimension(s)
are available and a nc_request
object is also available. The nc_request
object contains
the information needed to make requests for data according to the
dimensions of the NetCDF data source. With this information, we have
what we need to request a chunk of data that is what we want and not too
large.
(nc <- read_ncdf(f,
var = "sst",
ncsub = cbind(start = c(90, 45, 1 , 1),
count = c(90, 45, 1, 1))))
## 0-360 longitude crossing the international date line encountered.
## Longitude coordinates will be 0-360 in output.
## Will return stars object with 4050 cells.
## No projection information found in nc file.
## Coordinate variable units found to be degrees,
## assuming WGS84 Lat/Lon.
## stars object with 4 dimensions and 1 attribute
## attribute(s):
## Min. 1st Qu. Median Mean 3rd Qu. Max. NA's
## sst [°C] -1.8 -1.04 14 12.92722 25.13 29.81 757
## dimension(s):
## from to offset delta refsys values x/y
## lon 1 90 177 2 WGS 84 (CRS84) NULL [x]
## lat 1 45 -2 2 WGS 84 (CRS84) NULL [y]
## zlev 1 1 NA NA NA 0
## time 1 1 NA NA POSIXct 1981-12-31 UTC
plot(nc)
The ability to view NetCDF metadata so we can make well formed requests against the data is useful, but the real power of a proxy object is that we can use it in a “lazy evaluation” coding style. That is, we can do virtual operations on the object, like subsetting with another dataset, prior to actually accessing the data volume.
Lazy operations.
There are two kinds of lazy operations possible with
stars_proxy
objects. Some can be applied to the
stars_proxy
object itself without accessing underlying
data. Others must be composed as a chain of calls that will be applied
when data is actually required.
Methods applied to a stars_proxy
object:
[
- Nearly the same as stars_proxy[[<-
- stars_proxy method worksprint
- unique method for nc_proxy to facilitate unique
workflowsdim
- stars_proxy method worksc
- stars_proxy method worksst_redimension
- Not sure what this entails but it
might not make sense for nc_proxy.st_mosaic
* Calls read_stars on assembled list. Not
supported for now.st_set_bbox
Methods that add a call to the call_list
.
[<-
adrop
aperm
is.na
split
st_apply
predict
merge
st_crop
drop_levels
Ops
(group generic for +, -, etc.)Math
(group generic for abs, sqrt, tan, etc.)filter
mutate
tansmute
select
rename
pull
slice
* hyperslabbing for NetCDF could be as
above?pull
replace_na
Methods that cause a stars_proxy
object to be fetched
and turned into a stars
object.
as.data.frame
plot
st_as_stars
aggregate
st_dimensions<-
* https://github.com/r-spatial/stars/issues/494hist
st_downsample
st_sample
st_as_sf
write_stars
These binaries (installable software) and packages are in development.
They may not be fully stable and should be used with caution. We make no claims about them.