sEddyProc_sGLFluxPartitionUStarScens: sEddyProc sGLFluxPartitionUStarScens

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

sEddyProc sGLFluxPartitionUStarScens

Description

Flux partitioning after Lasslop et al. (2010)

Usage

sEddyProc_sGLFluxPartitionUStarScens(..., 
    uStarScenKeep = suffixes[1], isWarnReplaceColumns = FALSE, 
    warnOnOtherErrors = FALSE, controlGLPart = partGLControl())

Arguments

...	arguments to sEddyProc_sGLFluxPartition
uStarScenKeep	Scalar string specifying the scenario for which to keep parameters (see sEddyProc_sApplyUStarScen. Defaults to the first scenario, which is usually the uStar without bootstrap: "uStar".
isWarnReplaceColumns	overriding default to avoid the warning on replacing output columns, because this is intended when processing several uStar scenarios.
warnOnOtherErrors	Set to TRUE to only display a warning on errors in uStarScenarios other than uStarScenKeep instead of stopping.
controlGLPart	further default parameters

Details

Daytime-based partitioning of measured net ecosystem fluxes into gross primary production (GPP) and ecosystem respiration (Reco) for all u* threshold scenarios.

For the uStarScenKeep, a full set of output columns is returned. For the other scenarios, the bootstrap of GPP uncertainty is omitted and columns "FP_<x>" are overridden.

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]

REddyProc documentation built on March 18, 2022, 5:41 p.m.