sEddyProc_sMDSGapFillAfterUStarDistr: sEddyProc sMDSGapFillAfterUStarDistr

In bgctw/REddyProc: Post Processing of (Half-)Hourly Eddy-Covariance Measurements

sEddyProc sMDSGapFillAfterUStarDistr

Description

gapfilling for several filters of estimated friction velocity Ustar thresholds.

Usage

sEddyProc_sMDSGapFillAfterUStarDistr(..., 
    uStarTh, uStarSuffixes = colnames(uStarTh)[-1])

Arguments

...	other arguments to sEddyProc_sMDSGapFillAfterUstar and sEddyProc_sMDSGapFill such as fluxVar
uStarTh	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
uStarSuffixes	String vector to distinguish result columns for different ustar values. Its length must correspond to column numbers in UstarThres.m.n.

Details

This method is superseded by sEddyProc_sMDSGapFillUStarScens and only there for backward portability.

Author(s)

Department for Biogeochemical Integration at MPI-BGC, Jena, Germany <[e-mail]> [cph], Thomas Wutzler <[e-mail]> [aut, cre], Markus Reichstein <[e-mail]> [aut], Antje Maria Moffat <[e-mail]> [aut, trl], Olaf Menzer <[e-mail]> [ctb], Mirco Migliavacca <[e-mail]> [aut], Kerstin Sickel <[e-mail]> [ctb, trl], Ladislav <U+0160>igut <[e-mail]> [ctb]

bgctw/REddyProc documentation built on March 26, 2024, 11:35 p.m.