sEddyProc_sMDSGapFillAfterUstar.RdsEddyProc$sMDSGapFillAfterUstar - MDS gap filling algorithm after u* filtering
sEddyProc_sMDSGapFillAfterUstar(fluxVar, 
    uStarVar = "Ustar", uStarTh = .self$sGetUstarScenarios()[, 
        c("season", uStarSuffix), drop = FALSE], 
    uStarSuffix = "uStar", isFlagEntryAfterLowTurbulence = FALSE, 
    isFilterDayTime = FALSE, swThr = 10, 
    RgColName = "Rg", ...)Flux variable to gap fill after ustar filtering
Column name of friction velocity u * (ms-1), default 'Ustar'
data.frame with first column, season names, and second column estimates of uStar Threshold. Alternatively, a single value to be used as threshold for all records If only one value is given, it is used for all records.
Different suffixes required are for different u * scenarios
Set to TRUE for flagging the first entry after low turbulence as bad condition (by value of 2).
Set to TRUE to also filter day-time values, default only filters night-time data
threshold of solar radiation below which data is marked as night time respiration.
Column name of incoming short wave radiation
Other arguments passed to sEddyProc_sMDSGapFill
Calling sEddyProc_sMDSGapFill after filtering for
(provided) friction velocity u*
The u* threshold(s) are provided with argument uStarTh for
filtering the conditions of low turbulence.
After filtering, the data is gap filled using the MDS algorithm
sEddyProc_sMDSGapFill.
With isFlagEntryAfterLowTurbulence set to TRUE, to be more
conservative, in addition
to the data acquired when uStar is below the threshold,
the first half hour measured with good turbulence conditions
after a period with low turbulence is also removed (Papale et al. 2006).
Vector with quality flag from filtering (here 0: good data
, 1: low turbulence, 2: first half hour after low turbulence
, 3: no threshold available, 4: missing uStar value)
Gap filling results are in sTEMP data frame (with renamed columns)
that can be retrieved by sEddyProc_sExportResults.
sEddyProc_sEstimateUstarScenarios and
link{sEddyProc_sEstUstarThold} for estimating the
u* threshold from the data.
sEddyProc_sMDSGapFillUStarScens for
automated gapfilling for several scenarios of u* threshold estimates.