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