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https://github.com/annarufas/rufas_etal_2024_grl
Code and data necessary to reproduce the figures in our study "Can we Constrain Geographical Variability in the Biological Carbon Pump's Transfer Efficiency from Observations?".
https://github.com/annarufas/rufas_etal_2024_grl
biological-carbon-pump carbon-cycle matlab ocean-data particulate-organic-carbon
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Code and data necessary to reproduce the figures in our study "Can we Constrain Geographical Variability in the Biological Carbon Pump's Transfer Efficiency from Observations?".
- Host: GitHub
- URL: https://github.com/annarufas/rufas_etal_2024_grl
- Owner: annarufas
- License: mit
- Created: 2024-07-11T09:48:32.000Z (5 months ago)
- Default Branch: master
- Last Pushed: 2024-11-16T12:38:41.000Z (about 1 month ago)
- Last Synced: 2024-11-16T13:27:24.753Z (about 1 month ago)
- Topics: biological-carbon-pump, carbon-cycle, matlab, ocean-data, particulate-organic-carbon
- Language: MATLAB
- Homepage:
- Size: 125 MB
- Stars: 0
- Watchers: 1
- Forks: 0
- Open Issues: 0
-
Metadata Files:
- Readme: README.md
- License: LICENSE
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README
[![DOI](https://zenodo.org/badge/827257897.svg)](https://doi.org/10.5281/zenodo.12722805)
# Can we Constrain Geographical Variability in the Biological Carbon Pump's Transfer Efficiency from Observations?
![Comparison of published BCP mesopelagic transfer efficiency metrics across six
ocean sites associated with time-series programs](https://github.com/user-attachments/assets/a97488b3-3234-4993-b64c-3a38e6624162)This repository contains the MATLAB scripts and datasets used for the data analysis and figure generation in the study:
**"Can We Constrain Geographical Variability in the Biological Carbon Pump's Transfer Efficiency from Observations?"**
A. Rufas1, S. Khatiwala1, K. M. Bisson2,3, A. P. Martin4, H. A. Bouman1
1Department of Earth Sciences, University of Oxford, Oxford, UK
2Ocean Biology and Biogeochemistry Program, NASA Headquarters, Earth Science Division, Washington, D.C., USA
3Department of Botany and Plant Pathology, Oregon State University, Corvallis, OR, USA
4National Oceanography Centre, Southampton, UKFind the pre-print in the [Earth and Space Science Open Archive](https://essopenarchive.org/users/806280/articles/1197117-can-we-constrain-geographical-variability-in-the-biological-carbon-pump-s-transfer-efficiency-from-observations).
## Requirements
To use the content of this repository, ensure you have the following.
- [MATLAB](https://mathworks.com/products/matlab.html) version R2021a or later installed.
- Third-party functions downloaded from [MATLAB's File Exchange](https://mathworks.com/matlabcentral/fileexchange/): `worstcase`, `MCErrorPropagation`, `swtest.m`, `FMINSEARCHBND`, `m_map`, `brewermap`, `longhurst_v4_2010`, `subaxis` and `plotBarStackGroups`. Once downloaded, please place the functions in the `./resources/external/` directory.
- MATLAB toolboxes: the [Optimization Toolbox](https://mathworks.com/products/optimization.html), necessary to run `worstcase`, the [Statistics and Machine Learning Toolbox](https://mathworks.com/products/statistics.html), necessary to run `MCErrorPropagation` and `swtest.m`, and the [Curve Fitting Toolbox](https://www.mathworks.com/products/curvefitting.html), necessary to run `fittype`.## Repository Structure
- `./code/`: contains the MATLAB scripts for analysing and visualising data (*provided, see "MATLAB Scripts" section*).
- `./data/`
- `./raw/`: raw data compiled for this study (*partly provided, see "Obtaining Raw Data" section*).
- `./interim/`: input processed data for MATLAB scripts (*provided, see "Obtaining Interim Data" section*).
- `./processed/`: intermediate or input data used by the MATLAB scripts for further processing (*provided*).
- `./resources/`
- `./external/`: third-party resources for plotting and functions (*see "Requirements" section*).
- `./internal/`: custom MATLAB functions generated specifically for calculating (*provided*).
- `./figures/`: figures generated from processed data (*provided*).## Obtaining Raw Data
- **Particulate organic carbon (POC) flux measurements** from sediment traps and radionuclides, a compilation that we made for this study. The file, `dataset_s0_trap_and_radionuclide_compilation.xlsx`, is not available within this repository as it contains data owned by other authors that are not in a preservation repository. References for constructing this dataset are provided in the Supporting Information of our paper (Tables S1-S6), and a processed version of the dataset is available in the folder `./data/processed/pocflux_compilation.mat`.
- **Particle concentration measurements** from the Underwater Vision Profiler 5 (UVP5) downloaded from the EcoPart repository hosted by [IFREMER](https://ecopart.obs-vlfr.fr). This data are stored in the subfolder `./data/raw/UVP5/` and also in a processed format in `./data/processed/UVP5/pocflux_bisson_45sc.mat`.## Obtaining Interim Data
- World Ocean Atlas 2023 annual climatology for **temperature**. This dataset, which I downloaded from the [NCEI NOAA website](https://www.ncei.noaa.gov/products/world-ocean-atlas), is stored in the file `temp_annual_woa23.mat`. It is required for running the Marsay et al. ([2015](https://doi.org/10.1073/pnas.1415311112)) algorithm (refer to Text S5 in the Supporting Information).
- The VHRR Pathfinder v.5.0 global 4 km monthly climatology (1985–2001) for **sea surface temperature** (SST). This dataset, which I downloaded from the [NCEI NOAA website](https://www.ncei.noaa.gov/products/avhrr-pathfinder-sst), is stored in the file `sst_pathfinder_v5.mat`. It is required for running the Henson et al. ([2012](https://doi.org/10.1029/2011GB004099)) algorithm (refer to Text S5 in the Supporting Information).
- Carr 2002 **net primary production** (NPP) monthly climatology. I constructed this climatology using the Carr [2002](https://doi.org/10.1016/S0967-0645(01)00094-7) algorithm for NPP, which incorporated inputs from (i) the SeaWiFS 9 km monthly climatology (1997-2010) for **chlorophyll concentration** and **photosynthetically available radiation** (PAR0), available for download from the [NASA website](https://oceancolor.gsfc.nasa.gov/l3/), and (ii) the AVHRR Pathfinder v.5.0 global 4 km monthly climatology (1985–2001) for SST. The resulting file, `npp_carr2002_seawifs_pathfinder.mat`, is essential for running the Henson et al. ([2012](https://doi.org/10.1029/2011GB004099)) algorithm (refer to Text S5 in the Supporting Information).
- **Euphotic layer depth** (*zeu*) monthly climatology. I constructed this climatology using two data products from the E.U. Copernicus Marine Service (CMEMS): the **diffuse attenuation coefficient at 490 nm** ([kd(490)](https://data.marine.copernicus.eu/product/OCEANCOLOUR_GLO_BGC_L4_MY_009_104/description)) from the Copernicus-GlobColour merged product based on satellite observations, and the **mixed layer depth** ([MLD](https://data.marine.copernicus.eu/product/GLOBAL_MULTIYEAR_PHY_001_030/services)) from the physics reanalysis product. I have used the 0.1% light depth for the calculation, as recommended by Buesseler et al. ([2020](https://www.pnas.org/doi/10.1073/pnas.1918114117)). The file, `zeu_calculated_kdcmems_mldcmems_pointonepercentpar0.mat`, is necessary to run the functions for fitting Martin's *b* and the remineralisation length scale coefficient (*z**).The scripts that I used to read the `.nc` files downloaded from the web repositories and generate the `.mat` files presented above are available in this related [repository](https://github.com/annarufas/ocean-data-lab).
## MATLAB Scripts
The following scripts have been run in this order to analyse the data and reproduce the figures in our paper.
| Num| Script name | Script action |
|----|----------------------------------------------|--------------------------------------------------------------------
| 1 | plotGlobalMapWithTimeseriesStations.m | Creates **Figure 1** |
| 2 | processPocFluxFromTrapAndRadCompilation.m | Processes **Dataset S0** |
| 3 | plotPocFluxFromTrapAndRadCompilation.m | Creates **Figure 2**, **S1** and **S2** |
| 4 | processPocFluxFits.m | Calculates *b* for various scenarios using **Dataset S0** and generates **Dataset S1** |
| 5 | plotPocFluxFits.m | Creates **Figure S3** |
| 6 | processPocFluxFromUvp.m | Processes the **UVP5 dataset** downloaded from Ecopart |
| 7 | plotPocFluxFromUvp.m | Creates **Figure S5** |
| 8 | findAndPlotUvpVsCompilationPocFluxMatchups.m | Creates **Figure 3** |
| 9 | processBcpMetrics.m | Calculates *b*, *z** and Teff using the best method determined after script 7 and generates **Dataset S2** |
| 10 | plotBcpMetrics.m | Creates **Figure 4** |
| 11 | examineEffectSampleSize.m | Analyses Dataset S0 to examine effect of sample size in the calculations of the relative error of *b* and *z** |The following are helper functions used by the scripts above:
| Num| Script name | Script action |
|----|------------------------------------------------|--------------------------------------------------------------------
| 12 | calculateBcpMetricsFromTrapAndRadCompilation.m | Steps to calculate and propagate error for *b*, *z** and Teff from Dataset S0; called by scripts 4 and 9 |
| 13 | calculateBcpMetricsFromUvp.m | Steps to calculate and propagate error for *b*, *z** and Teff from the UVP5 dataset; called by script 9 |
| 14 | calculateBcpMetricsFromHenson2012.m | Steps to calculate and propagate error for *b*, *z** and Teff using the algorithm of Henson et al. ([2012](https://doi.org/10.1029/2011GB004099)); called by script 9 |
| 15 | calculateBcpMetricsFromMarsay2015.m | Steps to calculate and propagate error for *b*, *z** and Teff using the algorithm of Marsay et al. ([2015](https://doi.org/10.1073/pnas.1415311112)); called by script 9 |
| 16 | propagateErrorWithMCforMartinbAndZstar.m | Monte Carlo error propagation algorithm for *b* and *z** fits; called by scripts 12 and 13 |
| 17 | propagateErrorWithMCforTeff.m | Monte Carlo error propagation algorithm for Teff; called by scripts 12 and 13 |
| 18 | solveMartinbAndZstar.m | Algorithm to solve *b* and *z**; called by scripts 11 and 16 |
| 19 | samplePocFluxWithLH.m | Latin Hypercube sampling algorithm for POC flux profiles; called by scripts 11 and 16 |
| 20 | binPocFluxDataAtRegularDepthIntervals.m | Low-level function, bins POC flux data by depth intervals; called by scripts 11 and 12 |
| 21 | extractDataBelowZref.m | Low-level function, extracts POC flux data below the reference depth; called by scripts 5, 11, 12 and 13 |
| 22 | constructFilenameFitMetrics.m | Low-level function, constructs file names for *b* fits for different scenarios; called by scripts 5, 6 and 16 |## Reproducibility
Our scripts showcase the application of Monte Carlo-based techniques for error propagation across diverse datasets of biological carbon pump (BCP) mesopelagic transfer efficiency metrics. Specifically, the scripts are hard-wired to handle data from our six designated study sites:
- the Hawaii Ocean Time-series (HOT) station ALOHA (HOT/ALOHA), in the subtropical NE Pacific (22.45ºN, 158ºW);
- the Bermuda Atlantic Time-Series/Oceanic Flux Program joint site (BATS/OFP), in the subtropical NW Atlantic (31.6ºN, 64.2ºW);
- the US JGOFS Equatorial Pacific process study experimental site (EqPac), in the central equatorial Pacific upwelling system (–2 to 2ºN, 140ºW);
- the Porcupine Abyssal Plain time-Series Observatory (PAP-SO), in the subpolar NE Atlantic (49.0ºN, 16.5ºW);
- Ocean Station Papa (OSP), in the HNLC region of the subpolar NE Pacific (50ºN, 145ºW), and
- the Long-Term Ecological Research (LTER) observatory HAUSGARTEN, in the polar Atlantic-Arctic boundary (79ºN, 4.0ºE).## Acknowledgments
This work was completed as part of my PhD project at the University of Oxford under the NERC large grant COMICS (Controls over Ocean Mesopelagic Interior Carbon Storage, NE/M020835/2). I also acknowledge funding from the University of Oxford's Covid-19 Scholarship Extension Fund and Oxford's Wolfson College Covid-19 Hardship Fund.