Humic substances may control dissolved iron distributions in the global ocean: Implications from numerical simulations
Environmental Science Research Laboratory, Central Research Institute of Electric Power Industry, Abiko, Japan
Corresponding author: K. Misumi, Environmental Science Research Laboratory, Central Research Institute of Electric Power Industry, 1646 Abiko, Abiko, Chiba 270–1194, Japan. (firstname.lastname@example.org)
 This study used an ocean general circulation model to simulate the marine iron cycle in an investigation of how simulated distributions of weak iron-binding ligands would be expected to control dissolved iron concentrations in the ocean, with a particular focus on deep ocean waters. The distribution of apparent oxygen utilization was used as a proxy for humic substances that have recently been hypothesized to account for the bulk of weak iron-binding ligands in seawater. Compared to simulations using a conventional approach with homogeneous ligand distributions, the simulations that incorporated spatially variable ligand concentrations exhibited substantial improvement in the simulation of global dissolved iron distributions as revealed by comparisons with available field data. The improved skill of the simulations resulted largely because the spatially variable ligand distributions led to a more reasonable basin-scale variation of the residence time of iron when present at high concentrations. The model results, in conjunction with evidence from recent field studies, suggest that humic substances play an important role in the iron cycle in the ocean.
 It is now broadly accepted that organic ligands play a crucial role in determining dissolved iron concentrations in seawater. Electrochemical measurements have revealed that more than 99% of dissolved iron is complexed with organic ligands [Gledhill and van den Berg, 1994; Rue and Bruland, 1995; van den Berg, 1995]. Two iron-binding ligand classes are operationally defined: a strong ligand class L1 observed predominantly in surface waters and a weak ligand class L2 observed more ubiquitously throughout the whole water column [Rue and Bruland, 1995]. Whereas L1 ligands control iron availability for phytoplankton, L2 ligands strongly influence dissolved iron distributions below surface waters by regulating the residence time of dissolved iron [Hunter and Boyd, 2007; Misumi et al., 2011].
 Although these ligands have not been fully identified chemically, previous field studies have suggested what their origin and fate may be. Possible sources of L1 ligands are siderophore production by marine microbes [Reid et al., 1993; Macrellis et al., 2001; Hunter and Boyd, 2007; Mawji et al., 2008; Ibisanmi et al., 2011], zooplankton grazing on phytoplankton [Sato et al., 2007], and viral cell lysis [Poorvin et al., 2011]; whereas L2 ligands are hypothesized to comprise a portion of the refractory dissolved organic carbon (DOC) pool produced during bacterial degradation of sinking particles [Hunter and Boyd, 2007; Laglera and van den Berg, 2009; Boyd et al., 2010; Boyd and Ellwood, 2010; Kondo et al., 2012].
 Iron complexation by ligands has been incorporated into most iron cycle/ocean general circulation coupled models (FeGCMs) [Moore et al., 2004; Parekh et al., 2005; Aumont and Bopp, 2006; Doney et al., 2006; Moore and Braucher, 2008]. The representation of ligands, however, is still rudimentary, and because knowledge regarding the geochemical cycle of ligands is limited, these models assume a single ligand class with a spatially homogeneous distribution. Application of the results of recent field studies to development of a better ligand parameterization for FeGCMs has therefore been a subject of great interest.
Ye et al.  have proposed an iron cycle model that includes fully prognostic ligand dynamics for both L1 and L2 ligand classes. The model assumes that phytoplankton produce L1 ligands under iron-limiting conditions, the rationale being that siderophores mediate iron acquisition and that L2 ligands result from the decomposition of detritus. The model considers photolysis and remineralization to be ligand sinks. Sensitivity experiments using a one-dimensional ocean model suggest that L2 ligands must have a long remineralization time scale and hence support the inference from field studies that L2 ligands are refractory DOC [Ye et al., 2009]. However, because a one-dimensional approach cannot consider the importance of lateral advection on such a long timeframe, Ye et al.  restored the L2 ligand concentrations to a typical L2 concentration in the deep Atlantic Ocean (2.5 nM) and did not discuss the details.
 More recently, Tagliabue and Völker  have described an FeGCM that incorporates a diagnostic method to simulate both L1 and L2 ligands based on an empirical relationship between iron-binding ligands and DOC [Wagener et al., 2008a]. Total ligand concentrations are calculated as a function of total DOC, which is equated to the sum of simulated semi-labile DOC concentration and a spatially homogeneous refractory DOC concentration (40 μM). Because refractory DOC accounts for most of the DOC in deep waters, the simulated deep-water L2 concentrations are almost homogeneous. The assumption that L2 ligands are proportional to total DOC may be inappropriate. Laglera and van den Berg  found that humic substances, which amounted to only 4% of the total dissolved organic matter in their deep Pacific sample, accounted for the bulk of the iron-binding capacity, the implication being that L2 ligands should be parameterized as a function of the abundance of humic substances rather than total DOC. Because humic substances contribute to the humic-type fluorescence (H-flu) intensity of chromophoric dissolved organic matter (CDOM) [Laglera and van den Berg, 2009], this suggestion is supported by many field observations that have shown significant correlations between iron solubility and the H-flu intensity of CDOM [Tani et al., 2003; Takata et al., 2005; Kitayama et al., 2009; Nishimura et al., 2012].
 Although the oceanic distribution of humic substances is still unclear, relatively well-established patterns in apparent oxygen utilization (AOU) can serve as good proxies for the distribution of L2 ligands. There is a linear relationship between the distributions of the H-flu intensity of CDOM and AOU over the Pacific Ocean basin [Yamashita and Tanoue, 2008]. Because three-dimensional, objectively analyzed AOU data are available on a global scale [Garcia et al., 2010], we can estimate the global distribution of L2 ligands by using that linear relationship. The apparent association between L2 ligands and AOU likely reflects the fact that particle remineralization controls both variables. Shipboard incubations have shown that release of L2 ligands accompanies remineralization of biogenic sinking particles [Boyd et al., 2010], which simultaneously consumes dissolved oxygen and increases AOU.
 The purpose of this study was to conduct a suite of FeGCM experiments to test the hypothesis that L2 ligands can be parameterized as a function of AOU. Use of the AOU-based formulation enables more skillful simulation of available dissolved iron concentrations, the implication being that humic substances, which are a small fraction of the refractory DOC pool, are a major component of L2 ligands and are playing an important role in the oceanic iron cycle.
2 Model and Experimental Design
 We used the biogeochemical elemental cycling (BEC) model [Moore et al., 2004; Moore and Braucher, 2008, J. K. Moore et al., Marine ecosystem dynamics and biogeochemical cycling in the Community Earth System Model (CESM1.0), submitted to Journal of Climate] embedded in the Parallel Ocean Program version 2 (POP2) [Smith et al., 2010; Danabasoglu et al., 2012], which is the ocean component of the Community Earth System Model (CESM1; available online at http://www.cesm.ucar.edu). We used a course resolution configuration [Shields et al., 2012] with a nominal 3° irregular horizontal grid [Yeager et al., 2006] and 60 vertical layers [Yeager and Jochum, 2009] to conduct a number of long-term sensitivity experiments. Coupled to the model was a sea ice component, the Community Ice CodE version 4 (CICE4) [Hunke and Lipscomb, 2008; Holland et al., 2012], with the same horizontal mesh as the POP2. The atmospheric and terrestrial components were turned off, because interaction with these components was beyond the scope of this study. The ocean and sea ice components were driven by a synthetic, cyclical “normal year” forcing [Large and Yeager, 2004]: 6 h average atmospheric state data based on the National Centers for Environmental Prediction reanalysis [Kalnay et al., 1996], daily satellite radiation data [Zhang et al., 2004], and monthly precipitation from Xie and Arkin  and the Global Precipitation Climatology Project [Huffman et al., 1997].
 The BEC model includes four classes of phytoplankton functional types: pico/nanoplankton, coccolithophores, diatoms, and diazotrophs; one class of zooplankton; five nutrients: dissolved nitrate, ammonium, phosphorus, iron, and silicate; inorganic carbon system geochemistry; and oxygen cycling. The simulated ecology and biogeochemistry, including the iron cycle, are well documented in previous studies [Moore et al., 2004; Moore and Braucher, 2008; Doney et al., 2009a; Doney et al., 2009b; Misumi et al., 2011; Moore et al., submitted manuscript].
 The model considers two external iron sources: aeolian dust [Luo et al., 2003] and seafloor sediments [Moore and Braucher, 2008]. Aeolian dust is assumed to contain a constant fraction of iron (3.5 wt.%), and 1% of the iron in the dust dissolves instantaneously at the sea surface. The model also considers dissolution of dust-associated iron during sinking in the water column [Moore and Braucher, 2008]. Dissolved iron is utilized for phytoplankton growth and is subject to particle scavenging.
 The current BEC model considers a single iron-binding ligand class without explicit representation of the chemical equilibrium between iron and the binding ligand [Moore and Braucher, 2008]. However, the simulated iron-scavenging rates are similar to those calculated by a model that explicitly represents a chemical equilibrium with a conditional stability constant for L2 ligands (log10KFe′L2 ~ 11–12; where KFe′L2 = [FeL2]/[Fe′][L2′], Fe′ is free iron, L2′ is free L2 ligand, and FeL2 is iron bound by L2 ligands) [see Misumi et al., 2011, appendix]. The BEC model is therefore applicable to investigating the distribution of L2 ligands. We acknowledge, however, that the current BEC model does not represent competitive reactions of L1 and L2 ligands with dissolved iron, which may be important in the upper ocean.
 We assumed a linear relationship between L2 ligands and AOU because L2 ligands are suggested to be composed primarily of humic substances [Laglera and van den Berg, 2009], the concentrations of which are proportional to AOU [Yamashita and Tanoue, 2008]:
where L2 and AOU are L2 ligands and AOU, respectively, and α and β are the rate of L2 ligand production per unit oxygen consumption and a background L2 ligand concentration, respectively.
 Because there are no literature values for α and β, we transformed equation (1) by expressing the background L2 ligand concentration β as a fraction of the global spatial average L2 ligand concentration, <L2>:
where f represents the fraction and the angle brackets represent the global spatial average. Substituting equation (2) into equation (1), taking the global spatial average of both sides, and solving for α give
 The equation for L2 thus involves two new parameters, <L2> and f. The parameter f can be interpreted as the importance of the background term (the second term on the right-hand side (RHS)) relative to the AOU-dependent term (the first term on the RHS) in equation (2).
 In this study, we adopted an objectively analyzed, data-based AOU [World Ocean Atlas, 2009; Garcia et al., 2010] to calculate L2 ligand concentrations rather than the simulated AOU because of the known AOU bias in the model (Moore et al., submitted manuscript). Figures 1a and 1b illustrate the L2 ligand distribution for <L2> = 0.6 nM and f = 0.0. In this case, the L2 concentrations are determined solely by the AOU term; the concentrations are generally lower in the Atlantic, Southern, and Arctic Oceans (Figure 1b; locations A, C, and F) and higher in equatorial regions and in the Indian and Pacific oceans (Figure 1b; locations B, D, and E), a pattern consistent with the distribution of AOU. At a depth of 500 m (Figure 1a), there is an influence from wind-driven circulation: L2 concentrations on depth surfaces in the thermocline are higher and lower because of Ekman upwelling and downwelling, respectively.
 We conducted three series of experiments designated CONST, AOU, and AOU-f (Table 1). In the CONST series, we fixed f at 1.0 and let <L2> range from 0.0 to 1.2 nM. Fixing f at 1.0 eliminated the first term on the RHS of equation (4), the result being a series of spatially homogeneous L2 concentrations. The CONST_06 and CONST_12 cases (Table 1) corresponded to the standard experiments in Moore and Braucher  and Misumi et al. , respectively. In contrast, we set f equal to 0.0 in the AOU series, thereby eliminating the second term on the RHS of equation (4), the result being that L2 ligand concentrations were directly proportional to AOU; i.e., the background concentration was zero. In the AOU-f series, we fixed <L2> at 0.6 nM, a best estimate from the CONST and AOU series, and varied the value of f from 0.0 to 1.0. Note that the AOU_06_100 and AOU_06_000 cases (Table 1) are the same as the CONST_06 and AOU_06 cases, respectively.
CONST Series: Spatially Homogeneous L2 Ligand Distribution
The parameters <L2> and f represent the global spatial average L2 ligand concentration and the ratio of the background L2 ligand concentration to <L2>, respectively. In all cases involving AOU-based L2 ligands other than AOU_MDL, an objectively analyzed AOU [World Ocean Atlas, 2009; Garcia et al., 2010] was used for calculating the concentrations of L2 ligands. In the AOU_MDL case, the simulated AOU was used for the calculation.
AOU-f Series: AOU-Based L2 Ligand Distribution With Different Fractions of the Background Ligand Concentration
The same case as CONST_06
The same case as AOU_06
The same settings as the AOU_06, but simulated AOUs were used for calculating the L2 ligand distribution.
The same settings as the AOU_06, but surface ligand concentrations were diagnosed from the simulated DOC distribution.
 We conducted two additional experiments designated AOU_MDL and AOU_DOC. In these cases, <L2> and f were fixed at 0.6 nM and 0.0, respectively, the best values among the CONST, AOU, and AOU-f series. In the AOU_MDL case, we calculated L2 ligand concentrations from simulated AOU. This experiment was intended to evaluate the influence of the bias in the simulated AOU on the simulated dissolved iron concentrations. It is also noteworthy that use of the simulated AOU created a feedback between iron and binding ligand concentrations: iron concentrations constrain primary production and hence export production, which in turn modulates AOU and thus the simulated ligand concentrations.
 In the AOU_DOC case, we tested a combination of our formulation with the DOC-based formulation of Tagliabue and Völker . They calculated total ligand concentrations, LT in nM, with the equation
where DOCTOT represents the sum of semi-labile DOC (DOCsemi) and refractory DOC (DOCref) in μM; the factor 0.09 and the offset 3.2 are in units of nM (μM)−1 and nM, respectively. They used a simulated DOCsemi concentration and assumed a homogeneous DOCref concentration of 40 μM to calculate LT from equation (5). They apportioned two thirds of the ligands associated with DOCsemi to L1 and the remaining one third to L2; all LT associated with DOCref was apportioned to L2, and an adjustment was made to account for the background L2 concentration:
 Because semi-labile DOC is not found in deep waters, the simulated deepwater L2 concentration is spatially homogeneous (0.4 nM). In the AOU_DOC case, we tested a combination of equations (4) and (6). Because our model has only a single ligand class, we equated the ligand concentration to the sum of L1 and L2 calculated from equations (4) and (6), respectively. The surface ligand concentrations so calculated in the AOU_DOC case were generally lower than those in Tagliabue and Völker  (Figure 1c), the difference being due mainly to the lower surface L2 concentrations calculated with our method. We acknowledge that the AOU_DOC case ignores competitive reactions involving the two ligand classes with dissolved iron and underestimates the binding strength of L1 ligands. This experiment was intended only to evaluate the first-order impact of using a best possible combination of L1 and L2 for the ligand distribution.
 The initial conditions for the model simulations were based on field data: temperatures and salinities were taken from the Polar Science Center Hydrographic Climatology 2 [Steele et al., 2001]; macronutrients from the World Ocean Atlas 98 [Conkright et al., 1998]; and preindustrial dissolved inorganic carbon and alkalinity from the Global Data Analysis Project [Key et al., 2004]. Dissolved iron concentrations were taken from a long-term BEC model simulation. The atmospheric CO2 concentration was fixed at the preindustrial value (289 ppm). The model was first spun-up for 150 years in the CONST_06 configuration; from the end of the spin-up calculation, the model was then further integrated for 150 years in the individual case (Table 1) configurations. The simulated dissolved iron concentrations changed significantly from the spin-up simulation, and 150 years are long enough for coming into new quasi steady state. The simulated dissolved iron concentrations exhibited reasonably small temporal trends both in surface and deep waters (i.e., the absolute values of the linear regression coefficients for the global mean dissolved iron concentrations for the last 10 years at surface and 3000 m depth were less than 0.0001 nM yr−1 in all cases). Here we discuss the results from the last year of the simulation.
 We compared the simulated dissolved iron concentrations with field data compiled by Tagliabue et al. , thereby roughly doubling the total number of data compiled by Moore and Braucher . We excluded two subsets of field data from the comparison. Data within 500 km of the coast (referred to as the “COAST” subset) were excluded because the coarse global model does not do a good job resolving the finer-scale patterns and processes in coastal systems. Also excluded were outliers (referred to as the “OUT” subset), which were defined as data exceeding a threshold of
where xi is an individual field datum, and mi and σi are averages and standard deviations for data within a water column having its center at the location of xi, a radius of 3000 km, and a thickness of 200 m (±100 m from the sampling locations). Because research cruises are often planned to observe sporadic, small-scale events, excluding data by specifying a large spatial scale is reasonable when comparing observed dissolved iron data with simulated results. Skill scores based on a comparison of the simulated results with all the field data and data excluding the subsets are summarized in Table 2. This data screening removed 4546 out of 8238 observations in surface water (0–200 m) and 2463 out of 3788 observations in deep water (200–5000 m). Although the skill scores were improved by this screening, the skill score of the AOU_06 case, which produced the best skill score among the AOU series, was always higher than the skill score of the CONST_06 case, which produced the best skill score among the CONST series, the implication being that our main conclusions were not a result of this screening procedure.
Table 2. Skill Scores Comparing the Simulated Results With Field Dataa
“N,” “R2,” and “RMSE” are the number of data, the coefficients of determination, and the root mean square errors, respectively. Subscripts “surf” and “deep” represent N, R2, and RMSE for the surface (0–200 m) and deep (200–5000 m) waters, respectively. Each column of the table compares the simulated results with different subsets of the field data: “ALL” represents all the data compiled by Tagliabue et al. ; “ALL–COAST” represents the same data as “ALL” but excluding data near the coast (within 500 km); “ALL–COAST–OUT” represents the same data as “ALL–COAST” but excluding outliers (see text). The subset of “ALL–COAST–OUT” was used for comparison with the simulated results. The simulated data were subsampled from the same month, location, and depth as the field data.
 We first describe results for five characteristic cases: CONST_00, CONST_06, CONST_12, AOU_06, and AOU_DOC. Surface dissolved iron concentrations were simulated reasonably well in all of these cases (Figures 2 and 3). The concentrations in the iron-limited areas, the Southern Ocean and the equatorial and subarctic North Pacific, were less than 0.3 nM in the open ocean in all of these cases, a result that is consistent with field data. The insensitivity of the results in the iron-limited areas to differences in ligand concentrations reflects the fact that biological uptake buffers changes in iron concentrations. Even in the case without ligands (CONST_00), the model overestimated the surface iron concentrations in the Atlantic and Indian oceans, where dust depositions are large (Figure 3a). The overestimations became more prominent as <L2> increased (Figures 3a–3c). The model greatly underestimated surface iron concentrations in the Arctic Ocean in all cases.
 In deep waters we found larger differences among the cases (Figures 4 and 5). The CONST_00 case underestimated the iron concentrations, especially in the Pacific (Figures 4a and 5a), whereas the CONST_12 case markedly overestimated iron concentrations in the Atlantic (Figures 4c and 5c). Compared to these two extreme cases, the CONST_06 case simulated deep-water iron concentrations reasonably well, though the concentrations in the Atlantic (Pacific) were overestimated (underestimated) (Figures 4b and 5b). The AOU_06 case produced lower (higher) concentrations in the Atlantic (Pacific) than did the CONST_06 case, the result being better skill scores for the AOU_06 case (the coefficient of determination, R = 0.61; and the root mean square error, RMSE = 0.23 nM) than for the CONST_06 case (R2 = 0.46, and RMSE = 0.27 nM). Use of the DOC-based ligand distribution in surface water (AOU_DOC case) hardly changed the simulated deep-water dissolved iron concentrations compared to the AOU_06 case (Figures 4d, 4e, 5d, and 5e).
 We next describe results for all the cases, with a focus on the sensitivity of the skill scores to the parameters (Figure 6). The surface water R2 values were insensitive (0–200 m; R2 = 0.30–0.37) to choices of <L2>, f, and the ligand formulations (Figures 6a–6d). This insensitivity reflects the fact that external iron inputs and biological uptake primarily determine the large-scale distribution of iron in surface waters. In the CONST series, the surface water RMSEs increased monotonically with increasing <L2> (Figure 6e). The increase of the RMSE was driven by the elevated surface water iron concentrations in the Atlantic and Indian Oceans (Figures 3a–3c). Because the surface water L2 concentrations remained low in the AOU series (Figure 1b), the surface water RMSEs were similar to those in the CONST_00 and CONST_02 cases (Figures 6e and 6f). High surface water ligand concentrations in the AOU_DOC case (Figure 1c) and elevated surface water iron concentrations in the Atlantic and Indian Oceans (Figure 3e) resulted in a large surface water RMSE (Figure 6h). The surface water R2 and RMSE in the AOU_MDL case were similar to those in the AOU_06 case.
 Results for the deep water (200–5000 m) showed a maximum R2 and a minimum RMSE for <L2> = 0.6–0.8 nM for both the CONST and the AOU series (Figures 6a, 6b, 6e, and 6f). A comparison of cases with the same <L2> revealed that the skill scores in the AOU series were always better than those in the CONST series. Decreasing f and increasing the contribution from the AOU term improved both skill scores (Figures 6c and 6g). Simulated deep-water iron concentrations for the AOU_MDL and AOU_DOC cases were comparable to those in the AOU_06 case (Figures 6d and 6h).
4.1 Plausible L2 Ligand Concentrations and Distributions
 Because L2 ligands primarily control dissolved iron concentrations, results for deep waters (200–5000 m) are a good metric for investigating the distribution of L2 ligands. Both the CONST and AOU series show the highest R2 and the lowest RMSE for <L2> = 0.6–0.8 nM in deep water, the implication being that 0.6–0.8 nM is a plausible range of concentrations for L2 ligands. The optimal L2 concentration in the model is within 1σ of observed deep-water ligand concentrations measured by competitive ligand equilibration, adsorptive cathodic stripping voltammetry (CLE/ACSV) (Table 3). However, use of the average ligand concentration in the observed data (e.g., the global average of 1.17 nM (Table 3)) as the <L2> parameter in the model overestimates simulated dissolved iron concentrations (e.g., the CONST_12 and AOU_12 cases).
Table 3. Basin-Averaged and Globally Averaged Ligand Concentrations and Standard Deviations in Deep Waters (Below 500 m) Measured by CLE/ACSV
Ligand Concentration (nM)
Boye et al. , Cullen et al. , and Thuróczy et al. .
Boye et al. , Croot et al. , Gerringa et al. , Boye et al. , Ibisanmi et al. , Thuróczy et al. , and Kondo et al. .
Rue and Bruland , Kondo et al. , and Kondo et al. .
 The fact that the optimal L2 ligand concentrations in the model were low compared to observations can be attributed to an underestimation of simulated iron removal rates, because lowering the ligand concentrations compensates for the underestimation. Many previous field studies have shown that a substantial fraction of dissolved iron in seawater actually exists as colloids [Wu et al., 2001; Nishioka et al., 2001; Nishioka et al., 2003; Cullen et al., 2006; Nishioka et al., 2007; Boye et al., 2010], and colloidal iron likely aggregates into larger particles and settles out from seawater. A recent mesocosm experiment has confirmed that formation of colloids and subsequent aggregation removes dissolved iron rapidly after dust addition to seawater [Ye et al., 2011]. Their model simulation suggests that models lacking an explicit aggregation removal mechanism need to use high iron-removal rate constants to represent the combined effects of direct scavenging and colloidal aggregation. Because our model does not explicitly consider aggregation removal, it may underestimate the rate of iron removal, the result being a systematically low optimal L2 ligand concentration.
 Another possible explanation for the low optimal L2 concentration is competitive reactions between L2 ligands and transition metals. In coordination chemistry, constructing an organic ligand that binds nonspecifically to transition metals is much easier than constructing a ligand that binds to a particular metal [Hunter and Boyd, 2007]. In fact, Hirose and Tanoue  suggested that binding of organic ligands to metal ions in seawater is nonspecific. Copper is considered to be bound by a large fraction of organic ligands [Hirose and Tanoue, 1994] and is the greatest competitor with iron for ligand acquisition. Simulated competitive reactions among organic ligands, iron, and copper have shown that iron can acquire only 0.1–0.4 nM (10–40%) of a 1 nM concentration of bulk organic ligands [Hirose, 2007] if the total copper concentration in seawater is 0.5–5 nM [Nozaki, 2001]. Because our model does not consider the copper cycle and competitive reactions, we may need to subtract a copper-bound fraction from the total ligand concentrations observed by CLE/ACSV to compare them with the model ligand concentrations.
 The large standard deviations observed in the field data (Table 3) can be partly attributed to analytical difference among studies. Expanding ligand intercalibration exercises to ensure comparability will decrease the standard deviations and provide better constraints for FeGCMs.
 The fact that hypothesizing L2 ligand concentrations to be a linear function of AOUs greatly improved simulated dissolved iron concentrations is consistent with the hypothesis, the implication being that L2 ligand concentrations should increase from the North Atlantic to the North Pacific. A possible explanation that accounts for the basin-scale gradients is that L2 ligands are a biologically refractory fraction of the DOC that is produced by bacterial degradation of sinking organic matter. The L2 ligands then accumulate in deep ocean water as it circulates along the pathways of deep-water circulation [Broecker and Peng, 1982]. In addition, our results have shown better model skill with lower f values. The second term on the RHS of equation (4), f<L2>, is the L2 ligand concentration when AOU equals zero, i.e., the concentration in surface waters. The fact that optimal f values are low probably reflects photodegradation of L2 ligands in sunlit surface waters. The processes controlling L2 ligand and AOU are likely different in surface waters because air-sea exchange controls AOU. The situation is different in deep waters where remineralization controls both variables. To adequately represent the difference in surface waters, we will need to formulate L2 ligand as a prognostic variable independent from AOU.
 Our model simulations do not provide any information about the chemical composition of L2 ligands. However, the linear relationship between H-flu intensity and AOU [Yamashita and Tanoue, 2008], the iron-binding capacity of humic substances [Liu and Millero, 1999; Laglera and van den Berg, 2009], and observed significant correlations between H-flu intensity and iron solubility [Tani et al., 2003; Takata et al., 2005; Kitayama et al., 2009; Nishimura et al., 2012] all make humic substances strong candidates for L2 ligands.
 The observed ligand concentrations show only small basin-scale gradients (Table 3). It is possible ,however, that analytical inconsistencies associated with reported ligand concentrations conceal basin-scale gradients. In fact, soluble ligand concentrations in the North Atlantic and North Pacific determined with the same methodology [Wu et al., 2001] have revealed higher ligand concentrations in the North Pacific than in the North Atlantic, the vertical profiles being similar to those of the L2 ligand concentrations in the AOU_06 case (Figure 7). Note that Wu et al.  actually measured the soluble fraction of [FeL] rather than the total ligand concentration usually measured by CLE/ACSV. More recently, Kondo et al.  reported the latitudinal distribution of iron-binding ligands throughout the Pacific and the Southern Ocean by using CLE/ACSV and showed that the ligand distribution in deep waters is roughly similar to the distribution of the H-flu intensity of CDOM and AOU measured by Yamashita and Tanoue . Thus, the large-scale ligand distributions in deep waters determined with the same methodology are consistent with our hypothesis. Ensuring the comparability of reported ligand concentrations is essential to further test the hypothesis.
 Our results do not provide constraints on the surface L2 ligand distribution. The surface R2 values are insensitive to choices of <L2> and f; the monotonic RMSE increase with increasing <L2> seems problematic, because it is driven by the elevated surface iron concentrations in the Atlantic and Indian Oceans, where the model overestimates the concentrations, even for the case without ligands. The overestimation of surface dissolved iron can be partly attributed to overestimation of the fraction of dust that dissolves at sea surface assumed in the model (1%). Mahowald et al.  indicated that the fraction of aerosols from desert dust is thought to be 0.4% that is less than half of the fraction assumed in this study. Because the estimated fractions vary widely (0.01–80%) [Mahowald et al., 2009 and references therein], reducing the uncertainty is essential to better simulate surface dissolved iron concentrations. Because multiple processes other than iron scavenging control surface water dissolved iron concentrations, we will need to evaluate the distribution of ligands in surface waters by considering various uncertainties.
 Adding the DOC-based surface ligand concentration (equation (6)) to the AOU-based ligand concentration (equation (4)) (i.e., the AOU_DOC case) greatly increases the surface RMSE. However, because of the model bias in surface waters, we cannot exclude the possibility of such a distribution of ligands. It is important to note, however, that the simulated deep-water dissolved iron concentrations hardly change between the AOU_06 and AOU_DOC cases, the implication being that the simulated deep-water dissolved iron concentrations are almost independent of the ligand distribution in the surface water. Thus, our conclusions with respect to the deep water L2 distribution are robust, despite the model bias in surface waters.
 The results of the AOU_MDL and AOU_06 cases are similar, indicating that the influences of the bias in the simulated AOU and the interaction between iron and the binding ligands are small. It is, however, important to note that the interaction can lead to positive feedback in a future climate change scenario. Intensified stratification of surface waters can increase ligand concentrations in underlying waters by reducing photodegradation of ligands. The elevated ligand availability in subsurface waters will increase the supply of iron to surface waters from below, the result being higher productivity in surface waters and more ligand production in subsurface waters. The importance of this positive feedback needs to be evaluated in future work.
4.2 Mechanism to Improve Simulated Dissolved Iron Distributions
Misumi et al.  introduced the iron-scavenging time scale (Stime) defined as
where dFe is the total dissolved iron concentration and scav is the rate of change of dFe due to iron scavenging. Stime equals the residence time of dissolved iron if scavenging is the sole iron removal process. Here we calculate Stime values for a typical high iron concentration of 0.9 nM (Stime0.9) at a depth of 500 m. In the CONST_06 case, the model Stime0.9 values are short (Figure 8a), on the order of days (Stime0.9 < 0.01 year) in the global simulation. Because this short residence time prohibits advection of high iron concentrations from source areas, high concentrations (>0.9 nM) are observed only in areas directly influenced by large external iron fluxes (Figure 4b): the equatorial Atlantic and the Indian Ocean from aeolian dust and coastal areas from seafloor sediments. In contrast, the Stime0.9 values in the CONST_12 case (Figure 8b) are long, on the order of years, in the global simulation. The long Stime0.9 values allow high iron concentrations to advect far from source areas, the result being improved simulation of iron distributions in the North Pacific (Figures 4c and 5c) because of the importance of horizontal advection of sedimentary iron to the open ocean [Johnson et al., 1997; Lam et al., 2006; Nishioka et al., 2007; Moore and Braucher, 2008; Misumi et al., 2011]. However, the long Stime0.9 values in the North Atlantic result in excess northward transport of high iron concentrations by the Gulf Stream and North Atlantic Current, the result being considerable overestimation of iron concentrations in the North Atlantic (Figures 4c and 5c).
 Moderate concentrations of iron (~0.5 nM) observed in the midlatitudes of the North Atlantic (Figure 4f), despite its being located downstream of the equatorial Atlantic, a large dust deposition area, indicate that the Stime values for high concentrations must be short in the North Atlantic. If we assume an advection speed of 5 cm s−1 and spatial scales for an anomaly of high iron concentrations advected from source areas of less than 500 km, then the Stime values for high concentrations must be shorter than 0.3 year in the North Atlantic. That scavenging time is an order of magnitude shorter than in the North Pacific, where the scavenging time is on the order of years [Misumi et al., 2011]. Such a large Stime difference between the North Atlantic and North Pacific is difficult to reconcile with the homogeneous distribution of ligands. The assumption that the L2 ligand concentrations are proportional to AOUs leads to reasonable basin-scale gradients in Stime at high iron concentrations (Figure 8c), the result being better simulated dissolved iron concentrations (Figure 4d).
 Basin-scale biases still remain in the simulated dissolved iron distributions in case AOU_06 (Figures 4d and 5d). The overestimation in the Southern Ocean may be attributable to overestimation of the rate of dust deposition in this study [Luo et al., 2003]. Wagener et al. [2008b] noted that the dust deposition estimates calculated by Luo et al.  are up to 2 orders of magnitudes higher than in situ measurements in Southern Hemisphere oceans. Relatively poor representation of the spatial pattern of dissolved iron in the deep waters of the Southern Ocean (Table 2; R2 = 0.26, for 200–5000 m) may also be attributed in part to lack of iron inputs from hydrothermal activity in our model [Tagliabue et al., 2010]. The large underestimation in the surface Arctic Ocean is possibly attributed to lack of riverine input of both dissolved iron and organic ligands in our simulation. Recent studies suggested that surface Arctic Ocean waters are strongly influenced by lateral transport of riverine dissolved iron and humic-type CDOM [Nakayama et al., 2011; Nishimura et al., 2012; Klunder et al., 2012]. Too much phytoplankton growth and biological drawdown of dissolved iron in the Arctic Ocean due to insufficient light limitation in the model (Moore et al., submitted manuscript) also likely contribute to the underestimation. In the North Atlantic, the AOU_06 case simulates iron concentrations very well at depths of 200–1000 m (R2 = 0.71), but the model shows poor skill at depths of 1000–5000 m (R2 = 0.25) and generally underestimates the concentrations. This underestimation reflects simulated ligand concentrations that are too low in the deep waters of the Atlantic in the AOU_06 case (i.e., the locations “A” and “B” in Figure 1). Nelson et al.  showed that CDOM concentrations are almost homogeneous below 1000 m in the Atlantic, and there is no statistically significant correlation between CDOM and AOU in the deep Atlantic. Thus, if humic-type CDOM concentrations can be used as a direct proxy for concentrations of L2 ligands, simulated dissolved iron concentrations will likely be further improved in the North Atlantic.
 We have investigated the simulated distribution of weak iron-binding ligands (L2 ligands) by using the biogeochemical elemental cycling model, a global 3-D ocean simulation. We used an objectively analyzed, data-based AOU distribution as a proxy for L2 ligand concentrations based on previously published observational studies. We found that introducing the AOU-based L2 ligand distribution led to iron residence times that were more than an order of magnitude shorter at high iron concentrations in the North Atlantic (on the order of days) than in the North Pacific (on the order of years), leading to a substantial improvement in the simulated dissolved iron distribution compared to simulations with homogeneous ligand concentrations. The basin-scale L2 ligand gradients are consistent with the assumption that L2 ligands are a biologically refractory fraction of DOC produced by bacterial degradation of sinking organic matter and are subjected to photodegradation in sunlit surface waters. In conjunction with previous observational evidence, our model results suggest that humic substances probably account for a large fraction of L2 ligands. Ensuring comparability of reported ligand concentrations, incorporating into models the effects of colloidal aggregation, the copper cycle, and competitive reactions among L1 ligands, L2 ligands, iron, and copper, and investigating global distributions of humic-type CDOM can further improve iron cycle models.
 We thank F. O. Bryan for his scientific support and input to this project. We acknowledge A. Tagliabue for providing the compiled dissolved iron data. This paper has also benefited from insightful comments from K. Hirose, K. Kuma, Y. Yamashita, J. Nishioka, T. Yoshimura, K. Sugie, and two anonymous reviewers. S. C. Doney acknowledges support from the U.S. National Science Foundation (EF-0424599). This work was also supported by NSF grant OCE-0928204 to J. K. Moore. The National Center for Atmospheric Research is sponsored by the National Science Foundation.