An open-source database for the synthesis of soil radiocarbon data: International Soil Radiocarbon Database (ISRaD) version 1.0
Radiocarbon is a critical constraint on our estimates of the timescales of soil carbon cycling that can aid in identifying mechanisms of carbon stabilization and destabilization and improve the forecast of soil carbon response to management or environmental change. Despite the wealth of soil radiocarbon data that have been reported over the past 75 years, the ability to apply these data to global-scale questions is limited by our capacity to synthesize and compare measurements generated using a variety of methods. Here, we present the International Soil Radiocarbon Database (ISRaD; http://soilradiocarbon.org, last access: 16 December 2019), an open-source archive of soil data that include reported measurements from bulk soils, distinct soil carbon pools isolated in the laboratory by a variety of soil fractionation methods, samples of soil gas or water collected interstitially from within an intact soil profile, CO2 gas isolated from laboratory soil incubations, and fluxes collected in situ from a soil profile. The core of ISRaD is a relational database structured around individual datasets (entries) and organized hierarchically to report soil radiocarbon data, measured at different physical and temporal scales as well as other soil or environmental properties that may also be measured and may assist with interpretation and context. Anyone may contribute their own data to the database by entering it into the ISRaD template and subjecting it to quality assurance protocols. ISRaD can be accessed through (1) a web-based interface, (2) an R package (ISRaD), or (3) direct access to code and data through the GitHub repository, which hosts both code and data. The design of ISRaD allows for participants to become directly involved in the management, design, and application of ISRaD data. The synthesized dataset is available in two forms: the original data as reported by the authors of the datasets and an enhanced dataset that includes ancillary geospatial data calculated within the ISRaD framework. ISRaD also provides data management tools in the ISRaD-R package that provide a starting point for data analysis; as an open-source project, the broader soil community is invited and encouraged to add data, tools, and ideas for improvement. As a whole, ISRaD provides resources to aid our evaluation of soil dynamics across a range of spatial and temporal scales. The ISRaD v1.0 dataset is archived and freely available at https://doi.org/10.5281/zenodo.2613911 (Lawrence et al., 2019).
The study of soil organic matter (SOM) dynamics is essential to an improved understanding of terrestrial ecosystem dynamics and the Earth's carbon cycle (Oades, 1988; Heimann and Reichstein, 2008). Current evaluations suggest that SOM accounts for up to 2770 Pg of organic carbon in the top 3 m of soil (Jackson et al., 2017; Le Quéré et al., 2018), which makes it one of the largest actively cycling terrestrial carbon reservoirs and an important modulator of climate change (Sulman et al., 2018). However, the lack of clarity about which fraction of that reservoir will respond to ongoing environmental changes (i.e., timescales of years to centuries) and which will respond only on millennial timescales (He et al., 2016) makes it imperative to improve our understanding of the controls on soil carbon cycling. Additionally, many studies and models focus on only the top 0.5 m of soil or less, despite deeper soils contributing a significant proportion of SOM storage by way of low carbon concentrations but large deep soil mass (Rumpel and Kögel-Knabner, 2010). There is an urgent need to synthesize a wide variety of soil data to model the role of soil in the climate system (Bradford et al., 2016), to develop more data-driven estimates of soil health (Harden et al., 2017), to inform policy and land management plans that preserve and enhance soil carbon storage (Minasny et al., 2017; Poulton et al., 2018), and to extend our detailed understanding of soil developed from observations made at the profile scale to both regional and global extents. Here we describe a new open-source database for the synthesis of soil data with a particular focus on soil radiocarbon data.
Radiocarbon (i.e., 14C) content of SOM is a useful tool for estimating the timescales of SOM cycling, including the turnover time, residence time, or mean age of carbon in soil – defined as the time it has been isolated in soil from the atmosphere (Sierra et al., 2017; Manzoni et al., 2009; Trumbore, 2006). Although it was recognized very early on that radiocarbon measurements could provide a useful measure of the stability of soil carbon (Broecker and Olson, 1960; Tamm and Ostlund, 1960), the need for several grams of carbon for decay-counting methods meant that there were relatively few publications before the mid-1980s (e.g., Scharpenseel, 1971; O'Brien and Stout, 1978). Many of these papers only published bulk-soil radiocarbon for the same reason (with some exceptions, e.g., Martel and Paul, 1974; Goh et al., 1977). These early papers indicated that carbon in soils is heterogeneous and made up of a range of different aged materials that could be separated chemically (Martel and Paul, 1974). Several of these studies use models of the uptake of bomb carbon (Goh et al., 1977; Cherinskii, 1981; O'Brien, 1984; Balesdent, 1987). In the 1980s the advent of accelerator mass spectrometry, a method that measures 14C atoms in a sample by accelerating them to high energy, allowed for radiocarbon analysis using milligrams of carbon instead of grams, while simultaneously increasing sample throughput (Trumbore, 2009). This development enabled analysis of small amounts of archived soils to track the incorporation of 14C derived from atmospheric testing of nuclear weapons over time as well as making it far easier to analyze physically and chemically isolated soil fractions (e.g., Trumbore, 1993). These applications have led to an explosion in the number of publications with radiocarbon measurements from soil, increasing from a few dozen papers annually during the 1980s to more than 150 per year in the last decade (based on papers with “soil” and “radiocarbon” as keywords). The database presented here is an attempt to provide an archive for all the previously published data but also a repository for organizing new data as it is published.
Two recent soil radiocarbon synthesis efforts demonstrate the utility of these data for improving predictions of SOM dynamics (He et al., 2016; Mathieu et al., 2015). Bulk soil radiocarbon measurements, if not part of repeated time series, provide only an approximation of the time elapsed since carbon in the soil was fixed from the atmosphere. In other words, soil carbon age as measured by radiocarbon is defined as the age of carbon stored in the soil, from the time it enters until a time of observation. However, this mean value is not representative of how fast soil carbon will respond to a change in inputs, as it has been repeatedly demonstrated that SOM is not homogeneous and that carbon stabilized by different physical, chemical, or biological mechanisms cycles at different rates. Models can be used to explain time series of bulk radiocarbon or physically and chemically separated SOM fractions, but this requires model structures with multiple pools cycling on different timescales to simultaneously explain the rate of bomb 14C uptake and the mean 14C signature of SOM (Gaudinski et al., 2000; Baisden et al., 2002a; Baisden and Keller, 2013; Sierra et al., 2012; Schrumpf et al., 2013). Partitioning SOM into pools is easily implemented in models, but in reality, measuring these pools is both challenging and dependent on the techniques used to fractionate the bulk soil (Moni et al., 2012) or to track throughput of bomb-derived carbon through repeat measurements (Baisden et al., 2013; Baisden and Keller, 2013). A second measure of carbon cycling rates in soils is the transit (residence) time, which is defined as the time it takes carbon to pass through the soil system, from the time it enters until it is observed in an output flux (Sierra et al., 2017). The modeled transit time can be constrained by measurements of the radiocarbon signature of carbon in these output fluxes, which include respired CO2 or dissolved organic carbon (DOC) leached from the soil. Critically, most approaches using radiocarbon to estimate the timescales of carbon cycling in soils require multiple measurements of carbon in distinct soil reservoirs (Trumbore, 2000) or a time series of measurements made over the course of several years (Baisden et al., 2013; Baisden and Keller, 2013). As the assumptions required for modeling radiocarbon data can lead to confusion in the terminology and concepts of SOM dynamics, it is imperative that we archive radiocarbon measurements in order to preserve the ability to reevaluate calculations and compare data across different modeling frameworks.
Ongoing study of soils has led to shifting conceptual views of the controls on SOM dynamics (Blankinship et al., 2018; Golchin et al., 1994; Lehmann and Kleber, 2015; Oades, 1988; Schmidt et al., 2011). Current conceptual views that emphasize the protection of SOM from microbial decomposition via physical isolation or sorption to soil mineral surfaces (Lehmann and Kleber, 2015) and within anaerobic microsites (Keiluweit et al., 2016) have largely replaced earlier paradigms of humification, selective preservation, and progressive decomposition. Three of the fundamental questions currently driving SOM research are (1) what are the controls on the partitioning of organic inputs between soil reservoirs cycling over different timescales; (2) what factors determine rates at which SOM in each reservoir is lost, retained, or transferred within the soil; and (3) which mechanisms contribute to transformation of SOM to stabilized or more protected forms? To address these questions, researchers typically measure the concentration or mass content of organic carbon along with other properties, including molecular composition, isotopic ratios, and the distribution of SOM between conceptually or operationally defined pools (e.g., Basile-Doelsch et al., 2009) or a time series of samples collected over the course of decades (e.g., Baisden et al., 2002a).
Soil fractionation is the operationally defined separation of soils into distinct pools or “fractions” through a variety of physical, chemical, and biological approaches. Soil fractionation is generally intended to isolate soil fractions that reflect SOM in different physico-chemical states or mechanisms of SOM protection (Trumbore and Zheng, 1996); these mechanisms may operate on distinct temporal scales (e.g., Khomo et al., 2017). For example, density fractionation of SOM is a commonly applied technique (Golchin et al., 1994, 1995; Crow et al., 2007; Sollins et al., 2006, 2009; Swanston et al., 2005). The “light” fraction of soil material that floats in a dense solution (e.g., sodium polytungstate) or gets picked up by electrostatic attraction (Kaiser et al., 2009) is sometimes used as a proxy for rapidly cycling SOM, as this material is generally observed to have a shorter mean residence time compared with the bulk-soil average, while the “heavy” or dense material is used as a proxy for mineral-associated SOM, which is assumed to cycle more slowly (e.g., Sollins et al., 2009). In some cases, sonication of the suspension may be used to further isolate occluded SOM, i.e., organic material in soil aggregates (Golchin et al., 1994; Kaiser and Berhe, 2014). Other methods for isolating SOM with different cycling rates in the soil include, but are not limited to, physical separation of aggregates by size and water stability (Jastrow et al., 2006; Plante et al., 2006; Six and Paustian, 2014) or of different-sized soil particles (Desjardins et al., 1994), biological incubation of soils (Torn et al., 2005; Trumbore, 2000; Paul et al., 2001), and chemical extractions (Heckman et al., 2018; Masiello et al., 2004).
Comparing the mass and radiocarbon signature of the carbon leaving or entering the soil system (fluxes) with those of specific soil fractions provides insight into the rates of transfer between pools and provides a means for differentiating between various measures of dynamics, ranging from mean age to the transit time of carbon for the whole soil, a given depth increment, or a given SOM pool (Gaudinski et al., 2000; Baisden et al., 2002a, b; 2003; Sierra et al., 2014; Ohno et al., 2017; Ziegler et al., 2017; Szymanski et al., 2019). Similarly, measurements of interstitial soil carbon (i.e., in soil water or gases collected from within an intact soil profile) and its isotopic signature provide key information about the dynamics of the carbon present in the soil solution (Sanderman et al., 2008). Soluble carbon is believed to be the dominant pathway for vertical transport of organic carbon (Kaiser and Kalbitz, 2012; Angst et al., 2016) and also an intermediate stage through which carbon exchanges from being vulnerable to microbial decomposition to being stabilized on mineral surfaces (Jackson et al., 2017; Leinemann et al., 2018).
Measurements of bulk soils as well as soil fractions are evaluated in the context of other soil properties to better understand the controls on SOM preservation. However, the diversity of soil fractionation methods makes it difficult to compare measurements across soils or to evaluate best practices (e.g., Trumbore and Zheng, 1996). Combining radiocarbon measurements of soil carbon fractions, time series, incubations, interstitial observations, and fluxes has proven useful in resolving the contribution of different soil carbon persistence mechanisms in a site-specific modeling context (Braakhekke et al., 2015), but the application of this approach beyond the site scale has thus far been limited due to the lack of globally synthesized data.
With a changing paradigm for SOM dynamics and ever-evolving SOM models, it is more important now than ever that we synthesize existing soil radiocarbon measurements and provide a central repository for new data. There have been previous efforts to develop a soil radiocarbon database (Becker-Heidmann, 1996, 2010; Trumbore et al., 2011), separately or integrated with a general-purpose soil carbon database (Harden et al., 2017). However, a challenge remains: to compile and organize soil radiocarbon data that have been collected in many different and complex ways (e.g., using various fractionation methods or including fluxes as well as organic matter pools). Addressing this challenge will provide new opportunities to leverage existing soil radiocarbon data for critical research, such as developing practical and theoretical insights into the information contained in various fractionation methods and how they relate to one another. This will expand our understanding of controls on soil carbon dynamics and facilitate broader integration of radiocarbon constraints on soil carbon turnover in Earth system models. For example, He et al. (2016) leveraged a synthesis of bulk-soil radiocarbon data to better constrain the age of carbon in five Earth system models, demonstrating that without this added constraint, these models overestimate soil carbon sequestration potential by an average of 40 %.
Here, we present a flexible database spanning broad spatial scales and capturing a range of data types, including diverse soil fractionation methods, incubations, fluxes, and interstitial measurements and spanning a range of spatial scales. Our goal is to provide an open-access data resource that will encourage the scientific community to apply the database for a variety of synthesis studies or metaanalyses and also contribute data to the repository.
The International Soil Radiocarbon Database (ISRaD) is designed to be an open-source platform that (1) provides a repository for soil radiocarbon and associated measurements, (2) is able to accommodate data collected from a large variety of soil radiocarbon studies, including the diversity of fractionation techniques applied to soils as well as repeated bulk measurements made over spatial or temporal gradients, and (3) is flexible and adaptable enough to accommodate new variables and data types. Although ISRaD was specifically developed with soil radiocarbon measurements in mind, it is well suited for synthesizing other soil measurements, including stable carbon and nitrogen isotopes. Importantly, we currently focus only on natural abundance isotopic measurements and therefore exclude data from isotopic tracer studies. The ISRaD v1.0 data are archived and freely available at https://doi.org/10.5281/zenodo.2613911 (Lawrence et al., 2019). Access to additional information as well as the various ISRaD resources described below is provided through the ISRaD website (http://soilradiocarbon.org, last access: 16 December 2019).
2.1 Database and dataset structure
In its most general form, ISRaD is an implicitly relational database. It consists of a linked hierarchical list of tables that contain soil measurements, i.e., variables (Fig. 1). The fundamental unit of organization in ISRaD is the entry, which corresponds to a unique dataset, i.e., a dataset with a digital object identifier (DOI), while each subordinate table corresponds to data from that entry with a particular spatial or temporal dimension.
Transparency and traceability are fundamental tenants of ISRaD. Accordingly, each entry, whether ingested individually or as a compilation, must have a DOI. For data from published studies, the DOI of the publication is acceptable. Data from unpublished studies must be registered for a DOI through a DOI registration agency (e.g., Zenodo, Pangaea, etc.) prior to ingestion into ISRaD. As it is equally important to be able to reconstruct prior data compilations, e.g., synthesis studies, the specific references for individual datasets making up a synthesis are ingested as part of the synthesis entry, and the entry is flagged within the database with an additional reference to the synthesis study itself. For example, several of the major data sources added to ISRaD were synthesis studies (e.g., He et al., 2016; Mathieu et al., 2015), and users can generate reports of data from these prior syntheses by constructing a query that utilizes this synthesis flag.
Each ISRaD release will be available in two forms: (1) a raw version of data (ISRaD_data), containing only values that were reported in the original source of each data entry, and (2) an expanded version of the database (ISRaD_extra). The ISRaD_extra version of the dataset includes additional parameters that have either been calculated or imported based on site coordinates, such as geospatially referenced climate information. Table 2 includes examples of some of the new variables included in ISRaD_extra; a more detailed list of this growing list of variables can be found on the ISRaD website in the ISRaD_extra Information File. Both versions of the database follow the general data hierarchy outlined below.
2.2 Data hierarchy
The ISRaD data hierarchy consists of eight levels of information (Fig. 2). The top level of the data hierarchy is the metadata table (1), which includes information describing the source of data for a particular entry. The remainder of the hierarchical levels can be defined by the spatial extent of the information included in each table. The site (2), profile (3), layer (4), and fraction (5) tables represent information captured from decreasing spatial extents: from the scale of the study area to individual mass fractions isolated from a single soil sample. Special cases of the last three spatial extents further accommodate the temporal context of repeated measurements: (6) fluxes, (7) interstitial, and (8) incubations. In the sub-sections below, we provide overviews and examples of the types of information reported at each level and for each of the tables that occupy these levels (Fig. 2).
The data hierarchy is maintained across tables through the use of unique keys, or linking variables (noted with a “*” in the following descriptions), that are required in each record (row) of data in each table. In addition to the table-specific key, each subordinate table in the hierarchy must also contain the key variables of the above tables. For example, in addition to a unique layer_name*, each record in the layer table must also be associated with an entry_name*, site_ name*, and pro_name* (profile name), i.e., the key variables for the metadata, site, and profile tables.
ISRaD provides basic quality assurance and quality control (QA/QC) protocols (described below) and expert review that are applied prior to ingesting entries. These protocols are used to ensure that required variables are complete, that the key variables match across levels of the hierarchy (more detail below), and that data entered match the specified data type and range for a given variable. Variables that are not designated as required need only be completed if those data are available. The ISRaD template and a detailed description containing the full list of variables along with instructions for populating the template can be downloaded or viewed from the “Contribute” page of the web interface (http://soilradiocarbon.org, last access: 16 December 2019).
For all variables across all hierarchical levels, it is important to observe the acceptable data types (character and numeric) and units. Variable names, descriptions, and reporting conventions are given in the heading columns of the ISRaD template file (ISRaD_Template.xlsx), and more detailed information is provided in the data dictionary (ISRaD_Template_Info.xlsx). Allowed values include unrestricted text, controlled text, or numeric variables with or without defined ranges. Unrestricted text is generally limited to naming and note data fields, while controlled text fields are implemented for certain variables in an attempt to standardize the data and simplify data analysis. In the event that desired variables are not included in the current version of ISRaD, users may submit a request to add new variables. This process is initiated by posting an issue at the ISRaD GitHub repository and is described in more detail in Sect. 3.4.
2.2.1 Metadata table
The metadata table provides information for the characterization of the entry itself. Required metadata include the entry name (i.e., entry_name*), the DOI, the data curator (the person who oversees template entry), and their contact information. The entry name is the key variable used to match the entry with measurements reported at the other data levels.
2.2.2 Site data table
Site-level data are limited to the geospatial details defining the coarsest scale of the study area(s) included in each entry. We define a site as a spatially defined location that includes one or more soil profiles. By convention, we define a site as having a ≥ 5 km radius, i.e., samples collected within 5 km of each other should be grouped under the same “site” designation. However, the 5 km radius is a convention only, as the distinction between site and profile may be study-specific, and geospatial data at this resolution are not always available for legacy datasets. Spatial coordinates are required to designate a site, and thus the required fields at the site level are limited to the site name (site_ name*), latitude, and longitude. Every entry must specify a minimum of one site location but can include multiple sites that do not need to be located in close proximity. For entries that do not report spatial coordinates, the data curator may estimate latitude and longitude based on the description of the study area using any of the widely acceptable mapping software (e.g., Google Earth, Google Maps, etc.). The site table does not include fields for reporting site properties. Such directly measured variables are reported at the profile level. The intended purpose of the site-level data is to provide at least coarse-scale geospatial coordinates for extracting consistently sourced parameters from geospatial datasets, which can then be compared against the range of measurements reported at the profile level.
2.2.3 Profile data table
Profile-level data include details pertaining to specific sampling locations. If available, profile-scale spatial coordinates should be provided in addition to site-scale coordinates.
Many variables that may initially appear to belong at the site level are instead included at the profile level to facilitate accurate representation of spatial heterogeneity at a finer scale than the site level (e.g., for multiple profiles observed at the same site). Examples include local mean annual temperature and precipitation, soil taxonomic classification, vegetation type, land cover, depth to bedrock, and parent material composition. Other than the entry name and site name, the only additional required variable at the profile level is the profile name (pro_name*).
2.2.4 Flux data table
Soil flux data present a special case of observations that correspond to the profile level of the database hierarchy. Flux-level data allow for reporting temporally explicit measurements of mass or energy transfer occurring at the profile scale. Both gas and liquid analytes (e.g., CO2, CH4, dissolved OC, particulate OC, etc.) may be reported in flux data. In addition to the profile name, records with flux data must also include the observation date (flx_obs_date). Data measured at multiple time points in a single location will have identical profile names but unique temporal data.
2.2.5 Layer data table
Layer-level data correspond to measurements made for a specific depth increment collected from a soil profile. The required variables at the layer level include layer name (lyr_name), depth of layer top, and depth of layer bottom. The latter two variables describe the upper and lower range of the sampling depth, respectively, in units of centimeters. We use a depth reporting system where the top of the mineral soil is denoted as zero and subsequent depths below that point are reported with incrementally increasing positive values. Organic horizons are thus reported as negative depth intervals. Special indicator fields (e.g., lyr_all_ org_neg) are used when the depth to the mineral soil is unknown, e.g., for deep organic horizons or peats. The layer level is where most common measurements of soil physical, chemical, and/or biological properties are reported. As such, there is an ever-increasing list of variables that may be reported in the layer table. Users should consult the up-to-date template instruction file for the complete list of accepted variables.
2.2.6 Interstitial data table
The interstitial level is a special case of layer-level data. Specifically, interstitial data refer to measurements made on material occupying the interstices of the soil structure. In most cases, this material can be thought of as being mobile relative to the rest of the soil matter. Some common examples include gases, liquids, and colloids. Like flux data, the interstitial data table accommodates repeated measurements of these properties through time, and as such, the observation date must be recorded for each record in the interstitial table. Because interstitial records may not correspond to the same depth increments defined for solid phase analyses, separate depth reporting is used in the interstitial table distinct from what is reported in the layer table. Both sampling methodology as well as the properties of interstitial samples are reported in the interstitial table.
2.2.7 Fraction data table
Compared with most other soil databases, the fraction data table of ISRaD is unique. The fraction data fields are designed to accommodate and allow for fair comparison of the wide-ranging methodologies utilized to partition soils into discrete fractions. As such, there are more required fields for the fraction level compared with the other hierarchical levels. These required fields include fraction name (frc_name*); the input source (frc_input), which can be the name of another fraction or bulk (unfractionated) soil layer fraction scheme (frc_scheme), which is a controlled set of terms describing the general class of fractionation procedure used; the fractionation agent (frc_agent), which provides additional detail for methods that have multiple options; the upper and lower boundaries (frc_lower and frc_upper), which allow for description of the fractionation thresholds used in the fractionation procedure; and finally the fraction scheme units (frc_scheme_units), which describe the units of reference for the cutoff thresholds.
For example (see Fig. 3), most soil density fraction (frc_scheme is density) procedures start with bulk soil from the layer in question (frc_input – bulk). The first distinct fraction, “free light”, is isolated by floating the soil in a heavy solution, e.g., sodium polytungstate (frc_agent – SPT). If the density of the sodium polytungstate used in density separation step was 1.6 g cm−3, frc_lower for the “free light” fraction is 0 and frc_upper is 1.6 (indicating that anything with a density less than 1.6 was included), and frc_scheme_units is grams per centimeter cubed (g cm−3). In addition to these required fields, the fraction-level data may include many of the same data fields that are reported for the layer-level data. Ideally the fraction data also include the mass percentage of the total sample represented by the fraction as well as the specific carbon concentration and carbon isotopic composition of the fraction, which are critical for relating bulk and fraction level observations.
2.2.8 Incubation data table
Flux rates and isotopic signatures of laboratory-incubated samples are reported in the incubation table. Sample processing data (e.g., whether or not roots have been removed from samples prior to incubation) are recorded as well as incubation conditions (e.g., temperature, moisture, and duration). Repeat measurements, such as incubation time series, can also be recorded. Incubation records must be linked either to a layer or both a fraction and a layer, e.g., roots isolated from a specific bulk layer sample.
2.3 Radiocarbon data – reporting conventions
Radiocarbon measurements of environmental samples have a long history, much of which is reviewed in Trumbore (2009), including common units. Radiocarbon data ingested to ISRaD are required to adhere to some basic reporting conventions. First, measurements of radiocarbon may be reported in units of either fraction modern (FM) or Δ14C. Within the ISRaD_extra version of the database, values reported in one or the other accepted units are internally converted and filled across all entries so that either unit may be used for analyses of the full dataset. Other units are not supported at this time – for example, calibrated radiocarbon dates are not accepted, as the calibration curves evolve over time. Such calibrated ages make sense only for certain fractions (e.g., macrofossils found in soils) and do not make sense in the context of most soil organic matter, which is an open system for carbon, with inputs that vary in Δ14C over time. For datasets where radiocarbon is reported in units other that FM or Δ14C (e.g., percentage of modern carbon or conventional radiocarbon age), it is up to the data curator or original author of the dataset to convert the reported values to one or both of the permitted units. Second, the year of measurement for each radiocarbon value must also be reported so that values may be internally converted between the two accepted units. In addition to these basic requirements, there are several other optional fields pertaining to radiocarbon data. These include the radiocarbon laboratory; the laboratory number, a unique identifier issued by each AMS facility; the analytical error reported for each measurement reported by most laboratories; and the environmental standard deviation of replicate samples (if analyzed). These variables are not required for data submission but should be included if they are available.
2.4 Data ingestion
New data entries are added, or ingested, into ISRaD through a user-initiated process. The most common means of ingesting entries is via the template provided on the ISRaD website (ISRaD_Master_Template.xlsx). The template is intended to be used in combination with the data dictionary (ISRaD_Template_Info.xlsx). These files and other supporting documentation (user guide and FAQ) are also available on the website (http://soilradiocarbon.org, last access: 16 December 2019). Completed entries that have been formatted for ingestion must also pass the automated QA/QC test before the ingestion process can proceed. Users can initiate QA/QC using the ISRaD-R package (described below) or directly from the ISRaD website. If the entry fails QA/QC, the report from the test can be used as a guide to make corrections. Once an entry passes QA/QC, it can be submitted for the final two steps of the ingestion process: expert review and final ingestion.
Data templates that have passed QA/QC should be submitted via email to ISRaD at firstname.lastname@example.org. These templates are then distributed to ISRaD expert reviewers, who inspect template files to ensure proper completion of the more complex aspects of the template, such as classification of soil fractionation methods. If problems are identified with a submitted dataset during the expert review process, reviewers will work with the data curator to ensure that these problems are corrected. Once the expert reviewer signs off on a submitted template, it will be ingested into the database.
3.1 ISRaD v1.0
The current version, v1.2.3, of ISRaD includes a total of 263 individual data entries and 730 sites spanning the globe (Fig. 4). The current distribution of data across the various levels of the database hierarchy is shown in Table 1, and a full list of data entry references is provided in Table S1 in the Supplement.
Users may access ISRaD and its supporting information three ways: (1) the website, (2) the ISRaD-R package, and (3) the GitHub repository. Each of these access points is described in more detail below.
3.2 The ISRaD website
Most simply, users can access ISRaD data and associated resources by way of the website (http://soilradiocarbon.org, last access: 16 December 2019). From the website, users can download pre-compiled versions of the database in a simple file format (.xlsx or .csv), which can be easily ingested into graphical or database software. The website also provides access to the most recent versions of the ISRaD entry template, the template information file, an up-to-date list of the datasets included in the latest version of ISRaD, the QA/QC tool, and a variety of other resources for assisting with filling out data templates and interacting with ISRaD data.
3.3 Accessing ISRaD within the R computing environment and the ISRaD-R package
ISRaD has been designed for ease of use in the R computing environment (R Foundation for Statistical Computing, Vienna, Austria) in order for users to be able to take advantage of the full suite of R capabilities and functionality to manipulate and analyze ISRaD data. Many of the basic functionalities, such as loading current versions of the ISRaD data objects, can be performed in the R environment without installation of the ISRaD-R package. A number of vignettes including R scripts for some commonly used data manipulations or plotting are given on the website.
Users who need to locally compile a version of ISRaD (e.g., using their own templates) or who want access to the full suite of reporting functions can access these features by installing the ISRaD-R package (also called ISRaD, which is available at the Comprehensive R Archive Network – CRAN – repository, http://cran.r-project.org/, last access: 16 December 2019). The ISRaD-R package primarily consists of the code that is used to assemble the database and perform the QA/QC checks for the ISRaD datasets. Users may ingest their own data within a local version of the ISRaD dataset by running the function ISRaD::compile(). This functionality is intended to allow researchers to interpret their own new or unpublished data in the context of ISRaD data. Additionally, the ISRaD-R package provides simple tools to download and quickly import the most recent ISRaD data into the R environment and produce basic data summaries and visualizations for the full dataset or user-defined subsets using report functions.
3.4 The ISRaD GitHub repository
The source code for the ISRaD-R package is hosted under version control on the GitHub repository ISRaD (https://github.com/International-Soil-Radiocarbon-Database/ISRaD, last access: 16 December 2019; GitHub Inc., San Francisco, CA). This platform is used to facilitate the open-source collaborative development of ISRaD data and additional database tools. Through the GitHub interface, users may (1) access data entries included in the compiled database; (2) evaluate and suggest modifications of the underlying code used for compilation, QA/QC, and calculation of the additional variables included in either the compiled ISRaD data object (ISRaD_data) or in the augmented data product (ISRaD_extra); and (3) report problems, questions, or other issues.
3.5 The soil carbon information hub
For students or non-experts interested in learning more about the science behind the data, we have developed the Soil Organic Carbon Information Hub (SOC-Hub). The SOC-Hub (https://international-soil-radiocarbon-database.github.io/SOC-Hub/, last access: 16 December 2019) is a set of articles in the form of blog posts providing background information on soils, radiocarbon, the terrestrial carbon cycle, and soil models. A large portion of the content for this site was created by students and whenever possible uses non-technical language to describe topics pertinent to ISRaD. Technical editing of the SOC-Hub is facilitated through the ISRaD GitHub repository. Users are welcome and encouraged to contribute to or improve the content in the SOC-Hub. We will update the SOC-Hub annually.
4.1 Accessing data entries
Individual data entries (i.e., completed templates or templates output from ingested compilations) that have passed QA/QC and the expert review process are hosted in the “ISRaD_data_files” folder of the GitHub repository. Users may download these entries in order to add new data or to make corrections to existing data if problems are discovered. Corrected files can be resubmitted to ISRaD once they pass QA/QC by emailing the updated template and a text file of the QA/QC report to the ISRaD editor (email@example.com) and will be reingested after passing the expert review process. This process of user-initiated revision of existing data entries is particularly useful when large data compilations are ingested into ISRaD from previously published syntheses (e.g., He et al., 2016; Mathieu et al., 2015) or when publications report treatment means. Depending on the scope of the synthesis efforts, entries ingested into ISRaD this way may omit data available from the original studies, and the entry modification process allows those data to be added or corrected as needed.
4.2 Accessing code
Access to the source code underlying the ISRaD database compilation and calculations allows for users to check for errors and contribute to the functionality of ISRaD. Users with a registered GitHub account are invited to write code that adds to or improves upon the existing database tools. Using standard GitHub tools, users will submit a “pull request”, and following code testing and evaluation of utility to the ISRaD community, user-submitted code will be incorporated into the ISRaD-R package.
4.3 Reporting issues, making suggestions, and asking questions
One of the most important tools available to ISRaD users is the ability to post questions, report issues, or make suggestions, including requests to incorporate new variables. We use issue tracking tools provided by GitHub to track and categorize user input including: suggestions for improvements; problems or errors with the website, the R package, code, or any other aspects of ISRaD; requests for new variables or issues related to existing variables (e.g., incorrect acceptable ranges used in QA/QC); or asking questions related to template entry or any other aspect of ISRaD. While the GitHub issue-reporting functionality is the preferred means for reporting questions or issues with the database or process, it does require that users register a GitHub account. Users who do not wish to or are not able to register with GitHub can also submit issues or questions via an email to the ISRaD editor (firstname.lastname@example.org); however, the response time may be slower.
4.4 Database versioning and archiving
Official releases of ISRaD data will be issued periodically, following major structural changes to the database or after the ingestion of a substantial amount of new data. Versioning is tracked using a three-tiered sequential numeric identifier, i.e., the version number (in the form of “major.minor.patch”) in addition to the date of the most recent change. The major version (i.e. the first numeral of the version number) is used to track official releases. Following each official release a DOI will be issued and the data will be archived by Zenodo (https://zenodo.org/, last access: 28 March 2019) and the USGS Science Base repository. These archives will be maintained in perpetuity to facilitate reproduction of any analyses conducted using a past version of the database. Ingestion of new data are considered minor updates and are tracked with the minor version number. Finally, the patch number of the version number, i.e., the third numeral, is used for tracking patches and minor changes to the code. All changes to the data or code-base are maintained under version control and are immediately available through the GitHub repository or via the website; however, only official releases will be issued a DOI. To ensure repeatability of analyses and accurate citations, users accessing the ISRaD dataset should always record both the full version number and the date. The names of ISRaD data files reflect the dataset versioning using the following standardized structure: (data name)(v.X.X.X.)(date).(format), where data name reflects the file type and structure (e.g., ISRaD_extra_flat_layer), v.X.X.X refers to the version number, date corresponds to date of the most recent regular update of the database in the GitHub repository, and format is the file type.
4.5 Citing ISRaD
Users citing ISRaD should cite this publication as well as the most recent official data release at the time that they accessed the data. In their citation of the official release, users should also reference the version of the data they used (e.g., v220.127.116.119-12-20).
4.6 Data sharing between soil databases
ISRaD is not the only soil database available to the international research community (Malhotra et al., 2019). The primary niche of ISRaD is the ability to synthesize soil radiocarbon data and provide a framework for comparing soil carbon fraction data. For other purposes, there may be other soil databases that are more applicable. However, as a benefit of adding data to ISRaD, we facilitate sharing of data ingested into ISRaD with other databases developed by the soil science community. At present, ISRaD has a reciprocal agreement with the International Soil Carbon Network (ISCN), which is focused on soil carbon content and related variables from bulk soils (i.e., no isotope or soil fraction information). As per this agreement, the ISCN retrieves bulk-soil data from ISRaD and is responsible for filtering duplicate entries and incorporating any new data into the ISCN database.
ISRaD is a community effort with multiple contributors operating at different levels. Governance of ISRaD is required in order to ensure continuity of services and to plan for the future evolution of this data repository. The governance structure of the ISRaD is pyramid-shaped (Fig. 5). The ISRaD scientific steering committee (SSC) consists of a rotating group of seven scientists and data managers. The committee members are nominated and voted into service by a majority vote of the existing steering committee. The role of the steering committee is to determine the feasibility of major changes to ISRaD proposed by the community; to oversee data management, archiving, and establishment of cooperative agreements; and to coordinate activities and funding of affiliated institutions.
Database maintainers oversee the development and maintenance of the technical resources underlying ISRaD. For example, these individuals are responsible for overseeing GitHub pull requests and managing major changes in the ISRaD data template and/or data structure. The ISRaD associate editor is a special case of maintainer, whose role also includes assigning submitted templates to expert reviewers (described below) and periodically rebuilding the database with new entries that have passed the expert review process.
Although the structure of the ISRaD governance pyramid is oriented around individual users, the nature of scientific research is often more group-focused. For example, teams of researchers generally work together to seek out funding and to conduct research. Thus, in some cases a group or team of individuals may seek to utilize or modify ISRaD for their purposes. Such groups can petition the scientific steering committee to be formally designated as an ISRaD organization. This process should be followed when groups seek to leverage the ISRaD resources beyond the scope of a basic user or contributor. The steering committee will consider the scope of the work proposed by the group and, when appropriate, provide a letter of support for funding proposals. Approved organizations should nominate a member to serve on the steering committee and, in the case of organizations making large changes or additions to ISRaD, a data maintainer to coordinate the technical aspects of that work.
As detailed above, ISRaD is an open-source project that provides several ways for participation. ISRaD v1.0 data (Lawrence et al., 2019) are archived and freely available at https://doi.org/10.5281/zenodo.2613911. Anyone may share or adapt the ISRaD dataset, provided they do so in accordance with the Creative Commons Attribution 4.0 International Public License (https://creativecommons.org/licenses/by/4.0/legalcode, last access: 13 March 2019), also referred to as CC BY. In addition, we strongly encourage ISRaD users to follow two simple guidelines for use:
When utilizing the resources provided by ISRaD, including the complete dataset, individually curated entries, or value-added calculations included in the R-package, users should cite this publication and reference the version of ISRaD that was used for their work (see Sect. 3.6 above). Additionally, if users leverage individual data entries from the database, they should also cite the original source dataset and/or paper.
When users interpret their own data in the context of data accessed from ISRaD, they should submit those new data for inclusion in ISRaD after they have published their results and/or obtained a DOI for their dataset.
ISRaD is an interactive open-source data repository specializing in radiocarbon data associated with measurements of soils spanning a broad range of spatial scales. The ISRaD dataset is unique in that it includes not only measurements of bulk soils but also measurements of soil water, gases, and the wide diversity of soil pools isolated through different fractionation methodologies. Most of the studies summarized in ISRaD were conducted with a goal of understanding the factors controlling timescales of carbon cycling in specific sites, regions, or biomes. ISRaD is an attempt to gather the data from these individual studies in one place and in the same format to facilitate comparisons and synthesis activities. There are three ways through which potential users can access ISRaD: (1) the web interface enables users to download the most recently compiled report formatted as a .csv file, (2) the ISRaD-R package provides access to the compiled reports as well as visualization tools and R-based querying tools, or (3) the GitHub repository provides direct access to the source code for the ISRaD-R package as well as data from individual entries and the compiled database. Currently, the ISRaD dataset contains ∼ 12 000 radiocarbon analyses, which, at a typical cost of approximately USD 500 each, represent over USD 6 000 000 of research investment. By providing a useful platform for existing data, we hope to encourage the community to increase the effectiveness of that investment and to use the ISRaD platform as a repository to increase the impact of new results. Many opportunities exist for applying ISRaD data for improving our understanding of controls on soil carbon dynamics, for comparing different methodologies of characterizing soils, or for constraining soil processes in models ranging from profile to global scales.
The supplement related to this article is available online at: https://doi.org/10.5194/essd-12-61-2020-supplement.
The creation of ISRaD was a community effort. The initial effort to build ISRaD started with the USGS Powell Center working group on Soil Carbon Storage and Feedbacks but benefited greatly from early efforts of the International Soil Carbon Network and other individual efforts to compile soil fraction or radiocarbon data. Scientists from the Max Planck Institute for Biogeochemistry joined forces with the Powell Center group to greatly expand the scope and technical complexity of ISRaD. CRL, JBM, AMH, GM, CAS, SS, KH, JCB, SEC, GMc, and ST designed and built ISRaD and led the preparation of the paper. PL, OV, KTB, CR, CEHP, CAS, KM, and SD provided technical contributions, including coding, to the creation of the database and assisted with the ingestion of data. CH, YH, CT, JH, MT, and CEA provided large datasets or data compilations. AAB, MK, AK, EMS, AFP, AT, JPS, LV, SFvF, and RW contributed to the conceptual framing of ISRaD and assisted with data ingestion. All authors read and commented on the paper. The USGS Powell Center working-group participants are CRL, JBM, AMH, GM, CAS, KH, JCB, SEC, ST, CR, CEHP, CS, AAB, MK, EMS, AFP, AT, JPS, and RW.
The authors declare that they have no conflict of interest.
We gratefully acknowledge our funding sources and the ESSD journal reviewers. We also thank Lisamarie Windham-Myers and Sanjay Advani, who provided thoughtful comments on an early version of this paper. Any use of trade, firm, or product names is for descriptive purposes only and does not imply endorsement by the U.S. Government.
This research has been supported by the US Geological Survey Powell Center for the working group on Soil Carbon Storage and Feedbacks, the Max Planck Institute for Biogeochemistry, the European Research Council (Horizon 2020 Research and Innovation Programme, grant agreement 695101), the USGS Land Change Science mission area, and the US Department of Agriculture (Soil Carbon Working Group award 2018-67003-27935).
This paper was edited by Giulio G. R. Iovine and reviewed by Jonathan Sanderman, Troy Baisden, and three anonymous referees.
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