Fit a Light Response Curve (LRC) by an index to get a parameter file
Source:R/LRC_PARMS_06.R
LRC_PARMS_06.Rd
This function uses the equation: $$\text{NEE} \sim a_x \left( 1 - \exp \left( a_1 \cdot \left( \text{PAR} - I_{\text{comp}} \right) \right) \right)$$
Where NEE is daytime net ecosystem exchange (\(\mu\)mol CO2 m-2 s-1), \(a_x\) is the maximum photosynthesis rate (\(\mu\)mol CO2 m-2 s-1), \(a_1\) is a coefficient, and \(I_{\text{comp}}\) is the compensation light level with the same unit of PAR.
The equation requires photosynthetically active radiation, PAR, in \(\mu\)mol m-2 s-1 and net ecosystem exchange, NEE, in \(\mu\)mol m-2 s-1.
Usage
LRC_PARMS_06(
data.frame = NULL,
iterations = NULL,
priors.lrc = brms::prior("normal(-5, 5)", nlpar = "ax", lb = -30, ub = 0) +
brms::prior("normal(0.1, 1)", nlpar = "alpha", lb = 0, ub = 1) +
brms::prior("normal(300, 100)", nlpar = "Icomp", lb = 0, ub = 500),
idx.colname = NULL,
NEE.colname = NULL,
PAR.colname = NULL
)
Arguments
- data.frame
(dataframe) A dataframe that contains net ecosystem exchange (NEE), an index, and photosynthetically active radiation (PAR).
- iterations
(numeric) The number of iterations to run
brms::brm()
.- priors.lrc
(brmsprior dataframe) The priors for
brms::brm()
to use. Default priors are as follows:- idx.colname
(character) The name of the column containing the index.
- NEE.colname
(character) The name of the column containing NEE.
- PAR.colname
(character) The name of the column containing PAR.
Details
Model parameters are fit using the R package brms
.
Rhat (Potential Scale Reduction Factor): Indicates how well the different Markov chains in your analysis have converged to the same posterior distribution. Ideally, Rhat should be close to 1 for all parameters. A high Rhat value suggests potential convergence issues and the need to run the chains longer.
Bulk ESS (Effective Sample Size - Bulk): Estimates the effective number of independent samples from the central part of the posterior distribution.
Tail ESS (Effective Sample Size - Tail): Estimates the effective number of independent samples from the tails of the posterior distribution. Important for assessing the reliability of quantile estimates (e.g., 95% confidence intervals).
Key points to remember: Aim for Rhat close to 1 and high values for both Bulk ESS and Tail ESS.
Examples
# Import flux tower data
tower.data <- read.csv(system.file("extdata", "AMF_US-Skr_BASE_HH_2-5_Formatted.csv",
package = "CarbonExchangeParameters"))
# Fit curve parameters for each YearMon:
Example_LRC_PARMS_06 <- LRC_PARMS_06(data.frame = tower.data,
iterations = 1000,
priors.lrc = brms::prior("normal(-5, 5)",
nlpar = "ax", lb = -30, ub = 0) +
brms::prior("normal(0.1, 1)",
nlpar = "alpha", lb = 0, ub = 1) +
brms::prior("normal(300, 100)",
nlpar = "Icomp", lb = 0, ub = 500),
idx.colname = 'YearMon',
NEE.colname = 'NEE_PI',
PAR.colname = 'SW_IN')
#> [1] "GREAT JOB! your dataframe contains idx"
#> [1] "YIPEE! your dataframe contains nee"
#> [1] "Hooray! your dataframe contains PAR"
#> Your dataframe looks good and you are now ready to start fitting models
#> [1] "2004-07"
#> Error : CmdStan path has not been set yet. See ?set_cmdstan_path.
#> Error in LRC_PARMS_06(data.frame = tower.data, iterations = 1000, priors.lrc = brms::prior("normal(-5, 5)", nlpar = "ax", lb = -30, ub = 0) + brms::prior("normal(0.1, 1)", nlpar = "alpha", lb = 0, ub = 1) + brms::prior("normal(300, 100)", nlpar = "Icomp", lb = 0, ub = 500), idx.colname = "YearMon", NEE.colname = "NEE_PI", PAR.colname = "SW_IN"): object 'model.brms' not found