sEddyProc_sMDSGapFillUStarScens.Rdgapfilling for several filters of estimated friction velocity Ustar thresholds.
sEddyProc_sMDSGapFillUStarScens(...)other arguments to
sEddyProc_sMDSGapFillAfterUstar and
sEddyProc_sMDSGapFill
such as fluxVar
sEddyProc$sMDSGapFillUStarDistr: calling
sEddyProc_sMDSGapFillAfterUstar for several filters of
friction velocity Ustar.
The scenarios need to be set before by
sEddyProc_sSetUstarScenarios or accepting the defaults
annual estimates of link{sEddyProc_sEstimateUstarScenarios}.
Then the difference between output columns NEE_U05_f and NEE_U95_f corresponds to the uncertainty introduced by the uncertain estimate of the u* threshold.
Matrix (columns correspond to u* Scenarios) with quality flag from filtering ustar (0 - good data, 1 - filtered data)
Gap filling results in sTEMP data frame (with renamed columns), that
can be retrieved by sEddyProc_sExportResults.
Each of the outputs is calculated for several u* r-estimates and
distinguished by a suffix after the variable.
E.g. with an an entry "U05" in uStarSuffixes in
sEddyProc_sSetUstarScenarios
the corresponding filled NEE can be found in output column "NEE_U05_f".