sEddyProc_sMDSGapFillAfterUStarDistr.Rdgapfilling for several filters of estimated friction velocity Ustar thresholds.
sEddyProc_sMDSGapFillAfterUStarDistr(...,
uStarTh, uStarSuffixes = colnames(uStarTh)[-1])other arguments to
sEddyProc_sMDSGapFillAfterUstar and sEddyProc_sMDSGapFill
such as fluxVar
data.frame with first column, season names,
and remaining columns different estimates of uStar Threshold.
If the data.frame has only one row, then each uStar threshold estimate
is applied to the entire dataset.
Entries in first column must match levels in argument seasonFactor
String vector
to distinguish result columns for different ustar values.
Its length must correspond to column numbers in UstarThres.m.n.
This method is superseded by
sEddyProc_sMDSGapFillUStarScens and only there
for backward portability.