sEddyProc_sMRFluxPartitionUStarScens: sEddyProc sMRFluxPartitionUStarScens

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

sEddyProc sMRFluxPartitionUStarScens

Description

Flux partitioning after Reichstein et al. (2005)

Usage

sEddyProc_sMRFluxPartitionUStarScens(..., 
    uStarScenKeep = character(0))

Arguments

...	arguments to sEddyProc_sMRFluxPartition
uStarScenKeep	Scalar string specifying the scenario for which to keep parameters (see sEddyProc_sApplyUStarScen. Defaults to the first scenario.

Details

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

Value

NULL, it adds output columns in the class

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 May 3, 2024, 11 a.m.