1 2 3 4 5 | est_ustar_scens(temp, ctrl_est = control_ustar(),
ctrl_sub = subset_ustar(), ustar = "ustar", NEE = "NEE",
Tair = "Tair", Rg = "Rg", ..., sf = create_sf(data$timestamp, type
= "month"), reps = 200L, probs = c(0.05, 0.5, 0.95),
verbose = TRUE)
|
ctrl_est |
Control parameters for estimating ustar on a single binned
series, see |
ctrl_sub |
Control parameters for subsetting time series (number of
temperature and ustar classes), see |
ustar |
Column name for ustar. |
NEE |
Column name for NEE. |
Tair |
Column name for air temperature. |
Rg |
Column name for solar radiation. |
... |
Further arguments to |
sf |
Factor of seasons to split (data is resampled only within the seasons). |
reps |
Number of repetitions in the bootstrap. |
probs |
Quantiles of the bootstrap sample to return. Default is the 5 median and 95 \itemverboseSet to FALSE to omit printing progress. |
A data frame with columns agg_mod
, year
, and
ustar
estimate based on the non-resampled data. The other columns
correspond to the quantiles of ustar estimate for given probabilities
(argument probs
) based on the distribution of estimates using
resampled the data.
Original name: sEddyProc_sEstimateUstarScenarios
The choice of the criterion for sufficiently turbulent conditions (ustar >
chosen threshold) introduces large uncertainties in calculations based on
gap-filled Eddy data. Hence, it is good practice to compare derived
quantities based on gap-filled data using a range of ustar threshold
estimates.
This method explores the probability density of the threshold by repeating
its estimation on a bootstrapped sample. By default it returns the 90
confidence interval (argument probs
). For larger intervals the sample
number must be increased (argument probs
).
If more than ctrl_est$min_boot
(default 40
report a threshold, no quantiles (i.e. NA) are reported.
TW
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