Calculating precip anomalies with R & stars
Published:
Calculating climate anomalies with R & stars
Sami Rifai
2021-06-12
The stars library is a relatively new R framework for spatiotemporal arrays. In this demo, we will unpack a netcdf file to calculate the annual precipitation anomalies for southeastern Australia. This can also be effectively calculated using data frames, however my motivation here is to demonstrate how the stars array based workflow achieve this calculation faster and use far less memory.
Load the libraries
library(tidyverse) # data wrangler
library(stars) # the *star* of this tutorial
library(lubridate) # date wrangler
library(googledrive) # download data
library(scico) # sci-viz color palettesDownload the data
Here is a file with monthly averages for total precip, 2-m air temp, and 2-m dewpoint temperature that I got from the Copernicus Data Store for the ERA5-Land product.
fyi, the netcdf file is about 44 Mb.
Note that I am using stars::read_stars() instead of stars::read_ncdf
library(googledrive)
temp <- tempfile(fileext = ".nc")
dl <- googledrive::drive_download(
as_id("1Fo5F--2tfWWZfhTKBOatfM-bDs2stjhB"), path = temp, overwrite = TRUE)
raw <- stars::read_stars(temp)## d2m, t2m, tp,Get summary of the raw file:
raw## stars object with 3 dimensions and 3 attributes
## attribute(s), summary of first 1e+05 cells:
## d2m [K] t2m [K] tp [m]
## Min. :271.7 Min. :273.6 Min. :0.000
## 1st Qu.:279.6 1st Qu.:285.4 1st Qu.:0.001
## Median :281.2 Median :291.8 Median :0.001
## Mean :282.5 Mean :291.9 Mean :0.002
## 3rd Qu.:285.4 3rd Qu.:297.4 3rd Qu.:0.002
## Max. :295.0 Max. :305.6 Max. :0.016
## NA's :20998 NA's :20998 NA's :20998
## dimension(s):
## from to offset delta refsys point values x/y
## x 1 131 140.95 0.1 NA NA NULL [x]
## y 1 121 -26.95 -0.1 NA NA NULL [y]
## time 1 483 NA NA POSIXct NA 1981-01-01,...,2021-03-01Convert to mm/month
Following the ERA5-Land documentation for ‘accumulation’ variables:
The accumulations in synoptic monthly means (stream=mnth) have units that include “variable_units per forecast_step hours”. So for accumulations in this stream:The hydrological parameters are in units of “m of water equivalent per forecast_step hours” and so they should be multiplied by 1000 to convert to kgm-2 per forecast_step hours or mm per forecast_step hours.
So if I understood that correctly, we will multiply by 24 hours, and 1000 to get mm per month.
dp <- raw['tp']*(24*1000)Aggregate from monthly to yearly sum
dp_y30 = aggregate(dp %>%
filter(time>=ymd("1981-01-01",tz='UTC')) %>%
filter(time<ymd("2011-01-01")),
by='year', sum)
dim(dp_y30)## time x y
## 30 131 121Plot
always plot! stars has nice and fast plotting functions which are great for sprinkling sanity checks throughout your analyses.
plot(dp_y30, breaks='equal', col=viridis::inferno(100,direction = -1))
Calculate the Mean Annual Precip along the x & y dimensions
st_apply is our workhorse function here. Here we are just calculating the mean for each grid cell location ~ but we could do more complicated calculations such as rolling means, band-math, etc.
dp_map <- st_apply(dp_y30, MARGIN=c('x','y'), FUN=mean)
names(dp_map) <- 'MAP' # update the namePlot the Mean Annual Precip
plot(dp_map, breaks='equal', col=viridis::inferno(100,direction = -1),
main='Mean Annual Precip')
dp_y = aggregate(dp %>%
filter(time>=ymd("1981-01-01",tz='UTC')) %>%
filter(time<ymd("2021-01-01")),
by='year', sum)
dim(dp_y)## time x y
## 40 131 121So that is interesting. Any by interesting, I mean it’s a problem. The order of the dimensions is different from the input.
Reorder the dimensions as: x,y,time
aperm is a standard array transposition function which stars can use to realign our aggregated stars object.
dp_y <- aperm(dp_y, perm = c(2,3,1))
dim(dp_y)## x y time
## 131 121 40Great, so now the array dimensions are consistent.
Now we can do math.
dp_anom <- dp_y-dp_map## Warning in dim(e1) == dim(e2): longer object length is not a multiple of shorter
## object lengthNote we get the warning because dp_y has a time dimension and dp_map does not. But stars can do the math so long as we maintain the standard order of dimensions: x,y,time
Update the name of the variable in dp_anom object:
names(dp_anom) <- 'precip_anom'
dp_anom## stars object with 3 dimensions and 1 attribute
## attribute(s):
## precip_anom
## Min. :-722.57
## 1st Qu.: -91.21
## Median : -12.99
## Mean : -11.32
## 3rd Qu.: 65.29
## Max. : 666.14
## NA's :138280
## dimension(s):
## from to offset delta refsys point values x/y
## x 1 131 140.95 0.1 NA NA NULL [x]
## y 1 121 -26.95 -0.1 NA NA NULL [y]
## time 1 40 NA NA POSIXct NA 1981-01-01,...,2020-01-01Reset the time dimension to year
The time dimension is currently a POSIXct. This could be confused as the first date of each year, so let’s update them as a numeric corresponding to the calendar year.
dp_anom <- dp_anom %>%
st_set_dimensions(., which = 3, values=1981:2020, names = 'year')Plot the annual rainfall anomalies for southeastern Australia
plot(dp_anom,
join_zlim = T,
breaks = 'equal',
col=scico::scico(n=21, palette='roma'))
Ok, there are (at least) a couple of things here to nitpick. Should I have calculated the anomaly by some sort of hydraulic year instead of calendar year? Yes, probably. It is entirely possible to do this with stars, but I wanted to keep this example short and simple. Should I have retained the units from the original netcdf? Maybe, but I still drop them out of habit because I haven’t worked out how to (1) update them along the workflow, and (2) prevent them from breaking random functions. Maybe someday…
sessionInfo()## R version 4.0.3 (2020-10-10)
## Platform: x86_64-pc-linux-gnu (64-bit)
## Running under: Pop!_OS 20.04 LTS
##
## Matrix products: default
## BLAS: /usr/lib/x86_64-linux-gnu/openblas-pthread/libblas.so.3
## LAPACK: /usr/lib/x86_64-linux-gnu/openblas-pthread/liblapack.so.3
##
## locale:
## [1] LC_CTYPE=en_US.UTF-8 LC_NUMERIC=C
## [3] LC_TIME=en_US.UTF-8 LC_COLLATE=en_US.UTF-8
## [5] LC_MONETARY=en_US.UTF-8 LC_MESSAGES=en_US.UTF-8
## [7] LC_PAPER=en_US.UTF-8 LC_NAME=C
## [9] LC_ADDRESS=C LC_TELEPHONE=C
## [11] LC_MEASUREMENT=en_US.UTF-8 LC_IDENTIFICATION=C
##
## attached base packages:
## [1] stats graphics grDevices utils datasets methods base
##
## other attached packages:
## [1] scico_1.2.0 googledrive_1.0.1 lubridate_1.7.10 stars_0.5-2
## [5] sf_0.9-8 abind_1.4-5 forcats_0.5.1 stringr_1.4.0
## [9] dplyr_1.0.5 purrr_0.3.4 readr_1.4.0 tidyr_1.1.3
## [13] tibble_3.1.2 ggplot2_3.3.3 tidyverse_1.3.0
##
## loaded via a namespace (and not attached):
## [1] Rcpp_1.0.6 class_7.3-17 assertthat_0.2.1 digest_0.6.27
## [5] utf8_1.2.1 R6_2.5.0 cellranger_1.1.0 backports_1.2.1
## [9] reprex_2.0.0 evaluate_0.14 e1071_1.7-6 highr_0.8
## [13] httr_1.4.2 pillar_1.6.1 rlang_0.4.11 readxl_1.3.1
## [17] rstudioapi_0.13 jquerylib_0.1.3 rmarkdown_2.7 munsell_0.5.0
## [21] proxy_0.4-25 broom_0.7.6 compiler_4.0.3 modelr_0.1.8
## [25] xfun_0.22 pkgconfig_2.0.3 htmltools_0.5.1.1 tidyselect_1.1.1
## [29] gridExtra_2.3 viridisLite_0.4.0 fansi_0.4.2 crayon_1.4.1
## [33] dbplyr_2.1.1 withr_2.4.1 grid_4.0.3 lwgeom_0.2-6
## [37] jsonlite_1.7.2 gtable_0.3.0 lifecycle_1.0.0 DBI_1.1.1
## [41] magrittr_2.0.1 units_0.7-1 scales_1.1.1 KernSmooth_2.23-17
## [45] cli_2.4.0 stringi_1.5.3 cubelyr_1.0.1 viridis_0.6.0
## [49] fs_1.5.0 xml2_1.3.2 bslib_0.2.4 ellipsis_0.3.2
## [53] generics_0.1.0 vctrs_0.3.8 tools_4.0.3 glue_1.4.2
## [57] hms_1.0.0 prettydoc_0.4.1 parallel_4.0.3 yaml_2.2.1
## [61] colorspace_2.0-0 classInt_0.4-3 rvest_1.0.0 knitr_1.31
## [65] haven_2.3.1 sass_0.3.1