Abstract
Phytoplankton functional diversity plays a key role in structuring the ocean carbon cycle and can be estimated using measurements of phytoplankton functional type (PFT) groupings. Concentrations of 18 phytoplankton pigments were calculated using a linear matrix inversion algorithm, with an average r2 value of 0.70 for all pigments with p-values below the statistical threshold of 0.05. The inversion algorithm was then used with a chlorophyll-based absorption spectra model and Moderate Resolution Imaging Spectroradiometer (MODIS-Aqua) chlorophyll observations to calculate phytoplankton pigment concentrations in an area of the Atlantic Ocean off the United States east coast. Pigment distributions were analyzed to assess the distribution of PFTs. Five unique PFTs were found and delineated into three distinct offshore, transition, and open ocean groups. Group 1 (Diatoms) had highest abundance along the coast. Group 2 (prymnesiophytes, prokaryotes, and green algae) was a year-round stable offshore community that extended at reduced levels into the coast. Group 3 (dinoflagellates) dominated offshore between the Groups 1 and 2. Phytoplankton communities were delineated into coastal and offshore populations, with Group 2 having a dampened seasonal cycle, relative to the coastal populations. Shannon Diversity Indices (H) for the PFTs showed both spatial and temporal variability and had a clear non-linear relationship with chlorophyll. Diversity levels varied seasonally with changes in chlorophyll a levels. Peak PFT H was observed on the shelf where frontal features dominate, with diversity levels declining nearshore and offshore. This region marks an ecotone for phytoplankton in the study domain, and is associated with the coastal-side boundary of dinoflagellate dominance. Highest levels of diversity were observed in the tidally well-mixed regions of the Gulf of Maine and along a band that ran along the shelf region of the study area that was narrowest in the summer periods and broadened during the winter. These peak diversity zones were associated with moderate levels (~0.8 mg m−3) of chlorophyll a. While the sign in the linear trends in chlorophyll between 2002 and 2016 varied depending on the region, the trends in the PFT H values were nearly all negative due to the non-linear relationship between chlorophyll levels and H.
Introduction
Climate change will alter the timing and magnitude of oceanic forcing conditions that affect phytoplankton biomass and productivity, both critical elements of the ocean carbon cycle (Levitus et al., ). Warmer ocean temperatures are expected to alter primary production rates, vertical stratification, mixing, and entrainment of nutrients from beneath deep mixed layers (Sarmiento et al., ). There is now ample evidence on the ecological impacts of recent climate change conditions at all latitudes, but especially in polar environments. The responses of both flora and fauna span an array of ecosystem and organizational hierarchies in both terrestrial and marine environments (Walther et al., 2002; Cermeño et al., ; Iglesias-Rodriguez et al., ). These observed changes are strong motivators for developing remote sensing approaches to observe the base of the food chain in order to monitor alterations in ecosystem function and to help improve biogeochemical and primary productivity models (Edwards et al., ; Striebel et al., 2009; Boyce et al., ).
Analysis of phytoplankton taxonomic composition in relation to satellite-derived chlorophyll a (ChlSAT) provides an ecological approach to understand the role of past and future climate changes on ecosystem function (Boyce et al., ). Knowledge of the spatial and temporal variability of various Phytoplankton Functional Types (PFTs) is critical for improving primary productivity models which estimate biologically mediated fluxes of elements between the ocean's mixed layer and its deep interior (Falkowski and Raven, ), and for understanding potential climate-linked feedbacks. Improved performance and accuracy has already been observed in marine biogeochemical models that have incorporated PFTs into their ecosystem dynamics (Gregg et al., ).
Our current knowledge about the global distribution and seasonality of PFTs originates from shipboard and satellite observations (Alvain et al., ; Hirata et al., ; IOCCG, ; Bracher et al., ). Several new approaches for detecting phytoplankton biomass and specific PFTs, including coccolithophores (Balch et al., , ; Bracher et al., ), Trichodesmium (Subramaniam and Carpenter, 1994; Subramaniam et al., 1999a,b, 2002; Hu et al., ), and diatoms (Sathyendranath et al., ; Soppa et al., 2014) have been developed. Other algorithms characterize size class distributions (Ciotti et al., ; Mouw and Yoder, , ; Kostadinov et al., ; Brewin et al., ; Devred et al., ; Hirata et al., ; Organelli et al., ; Roy et al., ), PFT groups (Alvain et al., ; Hardman-Mountford et al., ; Bracher et al., ; Hirata et al., ; Moisan et al., ; Sadeghi et al., ; Campbell et al., ; IOCCG, ; Navarro et al., ) and select pigment concentrations (Pan et al., ), while others have utilized abundance based approaches (Uitz et al., 2006; Hirata et al., ; Chase et al., ).
A fundamental goal of phytoplankton biogeography is to describe the phenology of different PFTs and understand their interannual variability, and how these patterns relate to processes that control phytoplankton community structure and primary production (Longhurst, ). Phytoplankton biogeography influences how climate is regulated on a seasonal basis and also controls carbon flux processes (Oliver and Irwin, ). The diversity of the PFTs modulates the biological processes and controls ecosystem linkages within the carbon cycle. Understanding how they are modulated requires a better understanding of how the base of the food web is controlled by environmental conditions, which are impacted by climate change scenarios. Community developed algorithms for taxonomic marker pigments and size distribution (Balch et al., ; Alvain et al., ; Hu et al., ; Mouw and Yoder, ; Hirata et al., ; Moisan et al., ) continue to increase in their number and applications for the study of ocean ecosystem dynamics and biogeochemistry processes.
Algorithm development for PFTs using remote sensing observations has historically been based on bio-optical inherent optical properties such as backscatter and absorption (Nair et al., ). Absorption is often utilized in algorithm development because of its dominant role in regulating spectral variability of remote sensing reflectance due to changes in pigmentation (Moisan et al., ; Chase et al., ; Wang et al., 2016). In addition, sophisticated algorithms focus on ecological patterns of the phytoplankton community in relation to many factors such as climate change and meteorological conditions (Sathyendranath et al., ; Alvain et al., ; Hardman-Mountford et al., ; Raitsos et al., ; D'Ortenzio and Ribera d'Alcalà, ).
Many theories have been developed regarding the processes that govern marine biological diversity and stability and the impact that these have in evolving ecosystem community dynamics (Sommer et al., 1993). Recent advances in genomic observations and evolutionary/dynamic models are causing a surge in interest for this topic (Bruggeman and Kooijman, ; Terseleer et al., 2014). Indicators of phytoplankton functional diversity can be used to observe the response of marine ecosystems to climate change and its relationship to human activities (Platt and Sathyendranath, ; Platt et al., ). Past satellite studies, primarily focused on the North Atlantic, have shown phenological characteristics of bloom initiation and peak productivity (Siegel et al., 2002; Ueyama and Monger, 2005; Henson et al., ; Pan et al., , ). Documenting additional phenological markers may lead to a better understanding of the processes that affect the phytoplankton community and help in monitoring the response of PFT processes to changes in the environment.
This paper presents results from a study that uses in situ observations of phytoplankton absorption spectra and High-Performance Liquid Chromatography (HPLC) chlorophyll-a pigment measurements (ChlHPLC) to develop a satellite-based model for PFTs. In previous work, an inverse model technique was developed that used HPLC pigments and phytoplankton absorption spectra to create a method to retrieve 18 phytoplankton pigment estimates using phytoplankton absorption spectra (Moisan et al., ). An extension of this work used a linear model for phytoplankton absorption spectra, based on satellite observations of ChlSAT, photosynthetically available radiation, and temperature to estimate pigments within a region along the northeastern U.S. coastal ocean (Moisan et al., ). Previous studies have utilized inversion methods and demonstrated their value in calculating a wide variety of oceanographic information such as inherent optical properties (Hoge and Lyon, ; Garver and Siegel, ), pigment absorption spectra (Lee and Carder, ), and chlorophyll retrievals (Hoogenboom et al., ). This present study modified and expanded these techniques to generate phytoplankton pigment maps across the larger ocean domain of the Northeast Atlantic over the period from 2002 to 2016. The resulting phytoplankton pigment maps were then used with pigment-based PFT algorithms (Hirata et al., ) to calculate maps of PFTs. These PFT estimates were then used to calculate the PFT diversity using the Shannon Diversity Index (H).
Materials and methods
Ocean color data retrieval
Satellite (MODIS Aqua) chlorophyll a OCI algorithm, ChlSAT, estimates were obtained for the period of 2002-2016 from the NASA GSFC Ocean Color Processing Group. The validation of satellite products using quasi-simultaneous and spatially collocated measurements (match-ups) of satellite and in situ data followed the general procedures of previous studies (Werdell and Bailey, 2005; Bailey and Werdell, ). Observations for ChlSAT were obtained using the 8-day averaged, 9 km spatial resolution, mapped, level 3 products.
Laboratory analysis
Data was collected from a variety of geographical areas, which included both coastal eutrophic and oligotrophic waters (Figures 1A,B). A total of 172 water samples for phytoplankton absorption spectra, aph (λ), and HPLC were collected at depths between 0 and 29 meters during different cruises from the open ocean and two U.S. eastern coastal ocean regions: (1) Delaware, Maryland and Virginia and (2) the coastal waters within the Gulf of Maine and near Martha's Vineyard (Figures 1A,B). The data set includes all seasons for the Delaware/Maryland/Virginia (USA) region during 2006 and 2007 and spring samples from the Gulf of Maine during 2007.
Figure 1
Phytoplankton absorption spectra
Phytoplankton absorption samples were processed using the filter pad technique that partitions absorption into the particulate and detrital fraction (Kishino et al., ) to yield a phytoplankton absorption coefficient (m−1; Mitchell, ). Absorption spectra were acquired on a Perkin Elmer LS800 UV/VIS Spectrophotometer at 1 nm intervals from 300 to 800 nm using a 4 nm slit-width.
Fluorometric chlorophyll a
Water samples were filtered with 0.7 μm Whatman GF/F filter (USA), stored in Histoprep tissue capsules, and flash frozen in liquid nitrogen until processing. Chlorophyll a fluorescence was then measured using a Turner Model 10-AU fluorometer (Sunnyvale, USA) according to the method of Welschmeyer (1994). Phytoplankton absorption values were converted to specific absorption (m2 mg chla−1) using fluorometric chlorophyll a measurements. Fluorometric chlorophyll a compared well to ChlHPLC values with an r2 of 0.94.
High-performance liquid chromatography (HPLC) pigments
Samples were collected from the same Niskin bottles as phytoplankton absorption samples and filtered onto 0.7 μm Whatman GF/F filters. Samples were placed in Histoprep tissue capsules and stored in liquid nitrogen. Phytoplankton pigment concentrations were measured by HPLC on a C18 column using the procedure described by Van Heukelem et al. (2002) at Hornpoint Laboratory. A total of 25 pigment groupings were identified in each of the samples, 18 are calculated in this model, and 8 are used as marker pigments in this study (Table 1). The model pigments are: chlorophyll c, chlorophyllide, phaeophorbide, peridinin, 19′butanoyloxyfucoxanthin, fucoxanthin, neoxanthin, violaxanthin, 19′hexanoyloxyfucoxanthin, diadinoxanthin, alloxanthin, diatoxanthin, zeaxanthin, lutein, chlorophyll b, chlorophyll a, phaeophytin a, and carotenoids (α-carotene, B-carotene, diatoxanthin, diadinoxanthin, alloxanthin, zeaxanthin, lutein, fucoxanthin, peridinin, violoxanthin, 19′butanoyloxyfucoxanthin, and 19′hexanoyloxyfucoxanthin) (Barlow et al., ).
Table 1
| Diagnostic pigments | Abbreviations | Taxonomic significance | Phytoplankton size class |
|---|---|---|---|
| Fucoxanthin | Fuco | Diatoms | Microplankton |
| Peridinin | Perid | Dinoflagellates | Microplankton |
| 19′-hexanoyloxyfucoxanthin | Hexa | Phaeocystis, coccolithophorids | Nanoplankton |
| 19′-butanoyloxyfucoxanthin | Buta | Chrysophyte, Chromophytes, | Nanoplankton |
| Alloxanthin | Allo | Pelagophytes | Nanoplankton |
| cryptophytes | |||
| Violaxanthin | Viol | Prasinophytes | Picoplankton |
| Chlorophyll b | Chl b | chlorophytes, prochlorophytes prasinophytes | picoplankton nanoplankton |
| Zeaxanthin | Zea | Cyanobacteria | Picoplankton |
| prochlorophytes |
Methods for modeling phytoplankton absorption spectra and pigments
Modeled total phytoplankton absorption by multiple linear regression
Total phytoplankton absorption spectra, aph (λ, m−1), was modeled as a second order function of chlorophyll a such that
where Chl a is the concentration of chlorophyll a [mg m−3] and C0, CC, and CC2 are the wavelength-dependent coefficients in the multiple linear regression. The Levenberg-Marquardt non-linear least squares minimization routine (Marquardt, ) was used to perform the linear fits using in situ ChlHPLC and aph (λ).
In order to account for pigment packaging effects, the phytoplankton absorption spectra were “normalized” to 675 nm by a normalization term based on the expected unpackaged absorption at 675 nm. The unpackaged or “normalized” absorption spectra is calculated with,
where ci is the concentration of the individual pigments derived from the HPLC analysis and (λ = 675 nm) is the pigment-specific (a.k.a. weight-specific) absorption coefficient at 675 nm for the individual phytoplankton pigments, obtained courtesy of Annick Bricaud (Bricaud et al., ).
Modeled phytoplankton pigment-specific spectra by matrix inversion
A goal in modeling phytoplankton absorption spectra, aph(λ) (m−1), is to make use of the reconstruction models to estimate phytoplankton pigments directly from the observed phytoplankton absorption spectra (Moisan et al., ). By combining phytoplankton pigment concentrations and pigment-specific absorption spectra, it is possible to reconstruct the total phytoplankton absorption spectra aph (λ) for the sample, such that
where ci (mg pigment m−3) is the concentration of the individual pigments and ai∗(λ) (m2/mg) are phytoplankton pigment-specific absorption coefficients. When a large number (n) of phytoplankton absorption spectra and HPLC observations are available it becomes possible to relate the pigment-specific absorption coefficients and HPLC pigment concentrations to the total phytoplankton absorption measured at a specific wavelength as,
where ci,j is the observed pigment concentration of the ith pigment and the jth sample, (λ) is the derived pigment-specific absorption for the ith pigment, and aph,j(λ) is the total absorption due to phytoplankton for the jth sample and at a given wavelength (λ). At this point the various concentrations and absorption terms are members of a system of linear equations that can be inverted successively using the Singular Value Decomposition (SVD, Press et al., ) inversion technique on each wavelength to solve for each of the modeled pigment-specific absorption spectra, (λ).
Pigment concentrations from observed and modeled aph(λ) spectra
Once estimates for pigment-specific absorption coefficients are available, either through laboratory measurements (Bidigare et al., ; Bricaud et al., ) or through the numerical inversions such as the SVD approach outlined above, they can be used with phytoplankton total absorption spectra, aph(λ), to estimate the individual pigment concentrations using a second matrix inversion application (Moisan et al., ). In this study, we utilized SVD-derived pigment-specific absorption and measured total absorption in the process of estimating phytoplankton pigment concentrations. By expanding the phytoplankton absorption spectra reconstruction technique (Equation 3) of Bidigare et al. () into matrix form, total phytoplankton absorption for a suite of (n) samples can be written as
where (λ) is the estimated pigment-specific absorption of the ith pigment for a given wavelength (λ) obtained from the SVD inversion described in the preceding section, c ai is the estimated concentration of ith pigment for the jth sample, and aph(λ) is the measured total absorption due to phytoplankton at a given wavelength for each j sample.
Phytoplankton pigments were estimated using the resulting pigment-specific absorption spectra obtained from SVD inversion with observed aph(λ). Because solutions to SVD inversions are not guaranteed to produce positive concentrations (negative pigment concentrations have yet to be measured in the ocean), the Non-Negative Least Squares (NNLS, Lawson and Hanson, ) inversion method was used to estimate the pigment concentrations to guarantee positive solutions. Moisan et al. () demonstrated that out of all the inversion models tested, SVD-NNLS gave the best results when comparing modeled and measured pigment concentrations. Similarly, this technique has previously been verified in Moisan et al. () through random division of the phytoplankton absorption spectra and pigment measurement pairs. Two independent pools of data were created by randomly separating the full data set in order to carry out the inversions to calculate the pigment-specific absorption spectra and the other to estimate pigment concentrations using the second inversion procedure to validate the model.
In order to apply this matrix inversion technique to satellite data and generate pigment maps, the MODIS Aqua Ocean Color chlorophyll a (ChlSAT) was used with the resulting coefficients from the multiple linear absorption spectra model (Equation 1) to generate predictions of the mapped absorption spectra. These modeled absorption spectra were then inverted, pixel-by-pixel, using the SVD-derived pigment specific absorption spectra from Equation 4 and the NNLS inversion model (Equation 5) to yield maps of pigment concentration for the ocean region of the northeastern United States. Both the linear regression coefficients from Equation 1 and pigment-specific absorption spectra from Equation 4 were obtained using the normalized in situ aph(λ) (Equation 2) and HPLC pigment data. A flowchart of the method summary is detailed in Figure 2.
Figure 2
The matrix inversion technique applied to satellite data uses modeled instead of in situ absorption. In order to assess how the pigment inversions are affected by the use of modeled absorption, the results from the inversion model using modeled versus measured absorption spectra is compared.
Phytoplankton functional type maps and diversity
Once maps of the various 18 phytoplankton pigments were obtained, they were used to generate estimates of the various PFTs for the region by using the estimation formulas outlined in Table 1 of Hirata et al. (
Table 2
| PFT | Pigments used | Estimation formula |
|---|---|---|
| Diatoms | Fucoxanthin (Fuco) | 1.41Fuco/(∑DP*)2 |
| Dinoflagellates | Peridinin (Perid) | 1.41Fuco/∑DP2 |
| Green Algae | Chlorophyll-b (Chl-b) | 1.01Chl-b/∑DP2 |
| Prymnesiophytes | 19-Hexanoyloxyfucoxanthin (Hex), Chl-b, Alloxanthin (Allo) 19′-Butanoyloxyfucoxanthin (But), | (δ⊕1.27Hex + 1.01Chl-b + 0.35But + 0.60Allo)/∑DP3 - 1.01Chl-b/∑DP2 |
| Prokaryotes | Zeaxanthin (Zea) | 0.86Zea/∑DP2 |
Phytoplankton Functional Type (PFT) equations (Hirata et al.,
∑DP = 1.41Fuco + 1.41Perid + 1.27Hex + 0.6Allo + 0.35But + 1.01Chl-b + 0.86Zea.
δ quantifies the proportion of nanoplankton contribution in Hex, (Brewin et al.,
After calculation of the PFT fields, the PFTs Diversity was calculated using the Shannon Diversity Index (H) equation,
where pi is the ith proportionality of the N phytoplankton functional groups (Shannon,
Results
Observations of absorption spectra
Values of aph(λ) showed large variability in the ultraviolet (UV) and visible region (Figure 3). UV absorption was high, presumably due to mycosporine-like amino acids (MAAs, Moisan and Mitchell,
Figure 3

In situ phytoplankton absorption (m−1) from samples collected during the study.
Modeling of the total absorption spectra
In order to model the absorption spectra, the spectrally-dependent, linear model coefficients from Equation 1 were used with ChlHPLC values. The r2 values of in situ versus modeled absorption, when normalized to 675 nm, are between 0.76 and 1.00 from 400 to 700 nm and drop by about 25%, as calculated by dividing the mean r2 of UV and visible groups, in the ultraviolet region (Figure 4) where MAAs provide sun screening to phytoplankton and increase the observed value of aph(λ). Accuracies were substantially improved using the “normalized” absorption spectra in Equation 1, compared to original in vivo absorption spectra (Moisan et al.,
Figure 4

Measured total absorption (m−1) normalized to 675 nm (horizontal axis) versus the predicted total absorption (m−1) (vertical axis) using the multiple linear regression of ChlHPLC and ChlHPLC2.
To assess how much of the variability in the absorption curve is accounted for in the absorption model, the root mean square error (RMSE) was calculated for the first, second, and third order absorption models. The RMSE is the square root of the mean of the square of all the error. The variance drops by half from the observed spectra to the first order modeled spectra (RMSE = 0.113 and 0.063, respectively), and only slightly decreases with the second and third orders (RMSE = 0.063 and 0.060, respectively). Beyond the first order regression model there are only small improvements in modeling the absorption spectra. However, while the second order model is only slightly better than the first order in representing the variability of the absorption spectra, a larger improvement is observed in the pigment retrieval solutions. This may be because small improvements in modeling the absorption spectra can have a significant impact on the solution of those pigments that have smaller contributions to the total absorption spectra. The second order ChlHPLC model was chosen because there are only marginal difference between first, second, and third order in modeling absorption and second order produces the best pigments retrievals.
Observations of pigments in relation to absorption spectra
The contribution of each of the 18 pigments estimated by the inverse model to total absorption was determined by reconstructing the absorption spectra following the technique developed by Bidigare et al. (
Figure 5

(A) Reconstructed mean pigment-specific total absorption spectra (m−1) of the different pigment biomarkers resolved in this study. The black line is the total absorption of all pigments. The lowest standard deviation values were insignificant, while higher standard deviation values for the pigments ranged from 0.0015 to 0.0686. (B) Cumulative fraction of the reconstructed pigment absorption to total absorption compared to the r2 from the inverse model versus predicted HPLC pigments from SVD-NNLS.
Individual photosynthetic and photo-protective pigment retrievals
Pigments were estimated by the NNLS matrix inversion (Equation 5) with the SVD-derived pigment-specific absorption from Equation 4 and in situ absorption spectra. A comparison of in situ measured to SVD-NNLS-derived HPLC pigments shows varying results with coefficients of determination ranging from very high (near 1.0) for chlorophyll a () to a low of 0.33 for zeaxanthin (Figure 6). While 18 different pigments were estimated, only 10 had r2 values greater than 0.68. The p-values of the algorithm were calculated with a threshold value of 0.05. All pigments had p-values of less than 0.001, demonstrating that the results are significant (Table 3). Similarly, the pigment concentrations on a normal scale produced relatively small RMSE for most pigments, with normalized RMSE less than 22% for all pigments, except zeaxanthin and lutein. Normalized RMSE is the RMSE divided by the pigment range and bias is the tendency of a statistic to overestimate or underestimate a parameter. Pigments that correlate best with ChlHPLC, such as chlorophyll c, fucoxanthin, and carotenoids, along with ChlHPLC account for the majority of the total absorption spectra (Figure 5B). These pigments are also shown to have the best prediction results when modeled pigment concentrations are compared with in situ concentrations: they have the highest r2 values, their slopes are very close to 1 with y-intercepts close to 0, normalized RMSE below 5%, and all have p-values below the 0.05 threshold. While the coefficients of determination for the predicted pigments vary, all are within the acceptable range of algorithms that predict PFTs (Hirata et al.,
Figure 6

HPLC measured pigments (horizontal axis) versus the predicted pigments (vertical axis) using SVD to obtain the pigment-specific absorption spectra and NNLS to obtain pigment estimates.
Table 3
| Diagnostic Pigments | r2-Values | Slope | Intercept | RMSE | Normalized RMSE | Bias | p-Values |
|---|---|---|---|---|---|---|---|
| Chlorophyll a | 1.00 (0.99) | 0.99 (1.01) | −0.00 (−0.01) | 0.14 (0.15) | 0.01 (0.01) | 0.03 (−0.01) | <0.001 |
| Chlorophyll b | 0.41 (0.43) | 0.79 (0.83) | 0.03 (0.07) | 0.12 (0.12) | 0.22 (0.23) | 0.00 (−0.04) | <0.001 |
| Chlorophyll c | 0.88 (0.86) | 0.98 (0.96) | 0.03 (−0.02) | 0.14 (0.16) | 0.05 (0.06) | −0.02 (0.04) | <0.001 |
| Chlorophyllide | 0.73 (0.40) | 1.01 (0.82) | 0.02 (0.01) | 0.11 (0.15) | 0.10 (0.14) | −0.02 (0.01) | <0.001 |
| Phaeophorbide | 0.49 (0.68) | 0.89 (0.79) | 0.03 (0.01) | 0.17 (0.14) | 0.13 (0.12) | −0.02 (0.01) | <0.001 |
| Peridinin | 0.43 (0.34) | 0.88 (0.94) | 0.03 (0.04) | 0.12 (0.15) | 0.17 (0.21) | −0.02 (−0.03) | <0.001 |
| 19′-butanoyloxy-fucoxanthin | 0.54 (0.55) | 0.95 (0.86) | 0.02 (0.02) | 0.04 (0.05) | 0.11 (.012) | −0.02 (−0.02) | <0.001 |
| Fucoxanthin | 0.95 (0.92) | 0.96 (0.96) | −0.06 (−0.06) | 0.21 (0.32) | 0.05 (0.07) | 0.09 (0.10) | <0.001 |
| Neoxanthin | 0.47 (0.38) | 0.77 (0.68) | 0.01 (0.01) | 0.01 (0.01) | 0.14 (0.17) | −0.00 (−0.01) | <0.001 |
| Violaxanthin | 0.71 (0.60) | 0.94 (0.91) | −0.00 (0.01) | 0.01 (0.01) | 0.12 (0.14) | 0.00 (−0.00) | <0.001 |
| 19′-hexanoyloxy-fucoxanthin | 0.77 (0.64) | 0.99 (0.86) | 0.00 (0.03) | 0.05 (0.07) | 0.07 (0.08) | −0.00 (−0.02) | <0.001 |
| Diadinoxanthin | 0.82 (0.66) | 1.02 (1.01) | −0.01 (0.01) | 0.10 (0.14) | 0.07 (0.09) | 0.00 (−0.01) | <0.001 |
| Alloxanthin | 0.53 (0.41) | 0.85 (0.83) | 0.02 (0.04) | 0.08 (0.10) | 0.16 (0.20) | −0.01 (−0.03) | <0.001 |
| Diatoxanthin | 0.68 (0.63) | 1.06 (0.89) | 0.01 (0.02) | 0.04 (0.04) | 0.10 (0.10) | −0.01 (−0.01) | <0.001 |
| Zeaxanthin | 0.3 (0.02) | 1.03 (0.22) | 0.01 (0.05) | 0.05 (0.06) | 0.26 (0.31) | −0.01 (−0.02) | <0.001 |
| Lutein | 0.35 (0.27) | 0.95 (0.80) | 0.00 (0.01) | 0.01 (0.01) | 0.24 (0.26) | −0.00 (−0.00) | <0.001 |
| Phaeophytin a | 0.69 (0.70) | 0.99 (1.04) | −0.00 (−0.00) | 0.02 (0.02) | 0.12 (0.11) | 0.00 (0.00) | <0.001 |
| Carotenoids | 0.97 (0.94) | 1.00 (0.94) | −0.03 (0.17) | 0.21 (0.30) | 0.02 (0.03) | 0.03 (−0.08) | <0.001 |
Statistical values derived from comparison of measured pigment concentrations with those estimated from the SVD-NNLS inversions using the measured (modeled) absorption spectra.
Applying inversion model to satellite data
Modeling phytoplankton absorption spectra at every 5 nm using satellite chlorophyll a observations allows for extrapolation of observed relationships and can account for changes due to spectral shape, pigment composition, and pigment packaging (Figure 4). To apply the inversion model to satellite data, we calculated absorption (Equation 1) and inverted the modeled absorption values to obtain estimates for 18 HPLC pigments over a series of remote sensing images of the northeastern US coastal ocean. To demonstrate that the modeled absorption (as opposed to in situ absorption) would not have a significant effect on the pigment retrievals, we ran the SVD-NNLS inversion model using HPLC pigments and absorption modeled from Equation 1 and compared the resulting modeled pigment concentrations with in situ concentrations. While the r2 values in general decreased and the normalized RMSEs increased, compared to the inversion with in situ absorption, the r2 values of the predicted pigments that are addressed in detail in the analysis were not significantly less (Table 2). The statistical comparison of the two methods demonstrated that using modeled absorption in the satellite inversions does not significantly impact the pigment retrievals.
The results from the satellite-based inversion model show that the resulting estimates of chlorophyll a () maps are similar to those from the standard MODIS Aqua ChlSAT product (data not shown). A linear comparison of ChlSAT and ChlSAT results in an r2 of 1.00. While the OC-4 algorithm, applied to any of the NASA ocean color satellites (SeaWiFS, MODIS Terra and Aqua) has known issues with predicting chlorophyll a in coastal regions, the results from this study demonstrate that on a larger regional scale the features for both the OC-4 algorithm and the SVD-NNLS model solutions have very similar spatial scales and features.
To quantify the inherent error of using ChlSAT in the inversion model, we gradually introduced normal random error ranging from zero to a level comparable to the MODIS Aqua ChlSAT (r2 ~0.75) into the ChlHPLC and ran it through the SVD-NNLS inversion model. After hundreds of iterations, our mean r2 values for pigment retrieval dropped by 15–30 percent when errors were compatible to the satellite error which implied that the introduction of the satellite error does not greatly diminish the results of the inversion analysis (Figure 7).
Figure 7

The x-axes are the r2 of the ChlHPLC versus the ChlHPLC with normal random error added, where 1 is ChlHPLC with no error and 0.75 is equivalent to the error of ChlSAT. The y-axes depict the mean (left) and standard deviation (right) of the r2 values of the measured versus predicted pigment concentrations after the inversions are run with errored ChlHPLC for hundred of iterations.
In addition to , inversion of absorption spectra over a larger regional domain yielded estimates of 18 photosynthetic and photo-protective pigments for the year 2007 (Table 2). A number of these are useful as biomarkers for certain PFTs and can aid in resolving phytoplankton community structure (Table 1). Maps of pigments normalized to biomass (using ) are markers for the distribution of PFTs within a region (Figure 8).
Figure 8

Maps of the satellite-based inversion model estimates of chlorophyll a, and the ratios of chlorophyll c, fucoxanthin, 19′hexanoyloxyfucoxanthin, carotenoids (α-carotene, B-carotene, diatoxanthin, diadinoxanthin, alloxanthin, zeaxanthin, lutein, fucoxanthin, peridinin, violoxanthin, 19′butanoyloxyfucoxanthin, and 19′hexanoyloxyfucoxanthin) to (upper panel) using MODIS Aqua 2007 chlorophyll a observations. Similar ratios of peridinin, alloxanthin, chlorophyll b, violaxanthin, and 19′butanoyloxyfucoxanthin to are shown in the lower panel. Note that the nonlinear colored scale bars differ for each pigment, and the scales from left to right are associated with the pigments from top to bottom. Regions where the inverse model yielded zero concentrations are shown in black.
Chlorophyll a distribution
Modeled distribution from the SVD-NNLS inversion process compares well with MODIS Aqua ChlSAT distribution with r2 value of 1.00, and they both were inversely correlated to observed MODIS Aqua SST (data not shown), with highest (coldest) levels of ChlSAT (SST) located along the coast and over the well tidally-mixed region of the Grand Banks, with lowest (warmest) levels offshore to the southeast near the Gulf Stream Province, as noted by Longhurst (
Phytoplankton functional type marker pigment distributions
Identification of the presence of specific PFTs using marker pigments has been shown to be possible for a number of functional types (Wright, 2005). Although most pigments are not unique to specific phytoplankton taxa, and only a limited number are unambiguous pigments for specific phytoplankton taxa (Nair et al.,
Maps of several key PFT marker pigments, normalized to chlorophyll a, obtained from the inverse model (Figure 8) solutions for 2007 show a range of different spatial distributions over the study region. A small group of pigments (notably chlorophyll a, and fucoxanthin) show a strong spatial correlation with chlorophyll levels, and are highest in the coastal regions and lowest offshore. Fucoxanthin is primarily a marker pigment for diatoms, though it is also associated with other phytoplankton types and therefore has been argued to be ambiguous as a marker pigment (Nair et al.,
Spatial distribution and phenology of phytoplankton marker pigments
The seasonality of the functional type marker pigments (Figure 8) co-varied strongly with phytoplankton biomass levels, estimated by chlorophyll a concentrations, even though the ratios of the marker pigment concentrations to biomass levels varied spatially over the study region. Three specific regions related to the MAA sample area (coastal Gulf of Maine), the BIOME sample area (coastal region of the mid-Atlantic Bight), and for an open ocean region near the southeast associated with the Gulf Stream Extension domain were chosen as representative study regions (not shown). MODIST Aqua from 2002 to 2016 was taken for these three square areas and run through the inversion method to calculate 18 pigment concentrations that were averaged over each region. The spatially-averaged time series of the phenologically related marker pigments within each of the three regions from 2002 to 2016 (not shown) demonstrates that these key pigments vary differently from region to region.
levels for all regions showed seasonal variability, but no similarities (Figure 8). A review of the variability in this region is given by O'Reilly and Zetlin (
Fucoxanthin to ratios, a marker pigment for diatoms, showed high variance and an inverse correlated with SST over the time series (2002–2016) analyzed. The open ocean region showed the highest variance and a bi-annual peak in ratios in the spring and fall, possibly due to spring and fall diatom blooms. The BIOME region (northern coastal) showed high, low variance and nearly constant ratios during the fall through winter period, with a decrease during the summer seasons only. Finally, the MAA (southern coastal) had the highest observed variability, which, like the BIOME region, showed large decreases, but timed to occur primarily during the winter periods.
The 19′hexanoyloxyfucoxanthin to ratios (prymnesiophytes, Phaeocystis pouchetii and coccolithophorids) covaried with SST, with peak levels observed in the open ocean during the summer months, followed by the BIOME, with lowest peaks at the MAA site.
Peridinin: ratios (dinoflagellates) on the other hand showed an inverse correlation with SST except in the Biome region, peaking in concentration in the winter months when temperatures were at their lowest and mixed layer depths were at their greatest. Like the phenology of the 19′hexanoyloxyfucoxanthin-related PFTs, peridinin showed highest ratios in the open ocean site. However, higher peaks in the ratios were observed for the MAA region with lower levels in the BIOME region, noting that the dinoflagellates preferred more northerly coastal regions.
Phytoplankton functional type distributions, phenology, and diversity
Maps of five PFTs (diatoms, dinoflagellates, prymnesiophytes, prokaryotes, and green algae) calculated using the equations developed by Hirata et al. (
Diatom distributions
Diatom distribution was assessed by utilizing fucoxanthin as its biomarker pigment. Fucoxanthin is a useful marker for the bacillariophyceae or diatoms (Table 1) and also occurs in the raphidophytes and some prymnesiophytes (Jeffrey and Vest,
Figure 9

Modeled weekly-mean phytoplankton functional types and calculated Shannon Diversity Index during 2007. Starting from the upper row of images are distribution maps of Diatoms, Dinoflagellates, Prymnesiophytes, Prokaryotes, and Green Algae (% chlorophyll a). Weekly maps of the Shannon Index (H; n.d.) for the PFT diversity are shown along the lower row of panels. Regions where the inverse model yielded zero concentrations are shown in black.
Figure 10

The temporal distribution for sea surface temperature (°C), ChlSAT, Shannon Diversity Index (H; n.d.), and phytoplankton functional types (% chlorophyll a) for Diatoms, Dinoflagellates, Prymnesiophytes, Prokaryotes, and Green Algae from 2006 to 2011 for three stations including the Mid Atlantic Bight, Gulf of Maine, and open ocean.
Within the study region, diatoms played a dominant role in shaping the diversity in areas with chlorophyll levels greater than 0.45 mg chla m−3 (Figure 11). A peak of ~1.5 in diversity levels is observed at chlorophyll levels of ~0.82 mg chla m−3 which is driven entirely by the rise in contribution in total biomass from the diatom fraction of the PFTs. Below the 0.45 mg chla m−3, diatoms play little to no role in determining the functional type diversity levels.
Figure 11

Phytoplankton functional types (fraction of chlorophyll a) for Diatoms, Dinoflagellates, Prymnesiophytes, Prokaryotes, and Green Algae, and Shannon Diversity Index (H; n.d.) plotted against the log of ChlSAT over the whole study region.
Dinoflagellate distributions
Peridinin was the biomarker pigment used to calculate the distribution of dinoflagellates (Table 1) according to Hirata et al. (
Unlike the diatom populations, dinoflagellates influence diversity across all levels of biomass. Their peak influence in diversity occurs at chlorophyll levels of 0.45 mg chla m−3, which is where the diatom populations, or more correctly where fucoxanthin estimates go to zero. At lower phytoplankton biomass, or chlorophyll levels below the peak, the contribution of dinoflagellates to phytoplankton functional diversity levels decreases to zero at chlorophyll a concentrations of 0.1 mg chla m−3. At higher phytoplankton biomass or chlorophyll levels above the peak, the contribution of dinoflagellates to PFT diversity also decreases but at a much slower rate, reaching a near constant level at the higher chlorophyll levels.
Green algae
Green algae is a large, diverse and informal group, in the planktonic ocean realm this group is composed primarily of chlorophytes (Prasinophyceae (i.e. Ostreococcus), micromonas). The distribution of this PFT's taxonomic importance closely resembles that of the Prokaryotes and Prymnesiophytes. Concentrations of green algae were estimated according to Hirata et al. (
Figure 12

The trend line slopes of (A) seatellite chlorophyll a [mg chla m−3 year−1] and (B) shannon Diversity Index [H; year−1] at each point over a 15-year period (2002–2016) in the study region. Regions where the slopes were insignificant are shown in black.
Prymnesiophyte (haptophyte) distributions
Concentrations of haptophytes were estimated according to Hirata et al. (
Prymnesiophytes influence the PFT diversity levels (Figure 11) only at chlorophyll levels greater than 0.45 mg chla m−3, with highest influence at this transition chlorophyll concentration and a minimal impact at chlorophyll levels of ~3.2 mg chla m−3. Below 0.45 mg chla m−3, its contribution to the PFT diversity is equal to that of the green algae and constant at around 35%. Prymnesiophytes and the green algae showed strong correlations in terms of their spatial distribution and their contribution to PFT diversity as a function of chlorophyll a levels.
Prokaryotes
Maps of the prokaryotes (cyanobacteria) show distributional patterns that correlate strongly with the patterns observed in the green algae and Prymnesiophyte distributions. Estimates of the distribution of this group shows that they are more taxonomically important in the warmer, more stratified region of the study domain, and highest concentrations in the southeastern region where low nutrient gulf stream waters are found. In terms of percent chlorophyll, the Prokaryotes accounted for the lowest percentage of total biomass, with the highest percentages found in the offshore southeastern domain with values near 5%, and diminishing to near 2% for both the MAA and BIOME regions. During the warmer season, when nutrients are lower and stratification is high they have been observed to thrive in the coastal regions that have highly stratified water, such as the coastal areas off the Delmarva Peninsula region (Moisan et al.,
Phytoplankton functional type diversity
Maps of the PFT diversity (Figure 9), calculated using the Shannon Diversity Index (H, Equation 6) and PTF proportionality values of the various five (diatoms, dinoflagellates, prymnesiophytes, prokaryotes, and green algae), show that a dynamic field of PFT diversity exists in the study domain. Highest levels of diversity are seen between the nearshore high chlorophyll regions and the offshore oligatrophic regions, with the most extensive areas showing up during the winter and spring time and having lowest extent in the summer when the region is isolated to the Gulf of Maine and along the coastal shelf region along the entire study domain.
Because of the methods used to generate PFT estimates, the suites of phytoplankton pigment estimates, the PFT concentrations, and the Shannon Diversity Index (H) are all non-linear functions of chlorophyll a concentrations (Figure 11). The results show that the majority of the PFT concentrations or relative abundances vary smoothly across chlorophyll levels ranging from 0.01 to 10.0 mg chla m−3. A peak in the diversity is seen at chlorophyll levels of 0.63 mg chla m−3, with diversity levels decreasing at lower and higher concentrations of chlorophyll a. The peak itself is part of a localized higher (>0.8) diversity estimate for chlorophyll levels ranging between ~0.45 and ~1.0 mg chla m−3. This high PFT diversity region is located along the shelf at all times of the year and within the majority of the Gulf of Maine except along the near coastal areas. The overall area of high diversity expands to larger open ocean areas in the winter (Figure 9), when diatom levels are lower and become closer to the concentrations of the green algae, dinoflagellates and prymnesiophytes.
The local time series dynamics of both the PFTs and the resulting H show a wide range of variability (Figure 10). Overall, along the southern coastal BIOME region, the climatology in H shows a smooth seasonally varying relationship with a maximum level of diversity in the summer season. In the coastal Gulf of Maine MAA domain, the seasonal cycle in the H values shows high levels in the winter and summer season, with lows in the spring and fall due to the diatom bloom. In both the MAA and BIOME regions, increases in H are directly correlated with decreases in chlorophyll a or phytoplankton biomass. In the open ocean, chlorophyll a levels fluctuate around the peak in the H versus chlorophyll a relationship (Figure 11), leading to a much more variable climatology in H for this region. For instance, during the start of the spring bloom period in the open ocean domain, when the diatom population begin blooms and the winter population of prymnesiophytes, prokaryotes, and green algae are in decline, H increases until the chlorophyll a levels pass beyond the 0.63 mg chla m−3 level, above which H levels drop as the diatom population continues to bloom. This peak in the H versus phytoplankton biomass or chlorophyll a levels creates a much more complex H climatology for areas of the domain where the mean chlorophyll a levels are at this peak in H. Surprisingly enough, this chlorophyll a level is very near the peak in the histogram (not shown) of the chlorophyll a values for the domain. The belief is that this is merely serendipity from the choice in the domain under study, and not an ecological observation.
In addition to the complexities arising from the non-linear relationship between chlorophyll a levels and PFT diversity, the impact of climate-scale changes in the chlorophyll a field can also result in changes in PFT H values. For instance, for the 3 × 3 pixel region of the MODIS Aqua data centered on the location of the Woods Hole Oceanographic Institution's Air-Sea Interaction Tower (ASIT; 41° 19.5′ N, 70° 34.0′ W), the PFT diversity time series (not shown) has a seasonal cycle and a significant (p-value was 0.028) negative trend in the overall PFT diversity for that location. This trend is due to changes in the chlorophyll a levels during that period of time.
Maps of chlorophyll a linear trends for the study domain (not shown) reveal that the coastal ocean areas have positive trends in chlorophyll levels but negative trends are seen in the open ocean regions. The majority of the domain (~70%) shows no significant trends in the chlorophyll a levels. So for the study domain, some areas have observed rising chlorophyll a levels (along the coast) and in other regions chlorophyll a levels fall (open ocean). However, because the relationship between chlorophyll a levels and PFT diversity is non-linear, the long-term trends in PFTs can also vary. So, while the resulting trends in the chlorophyll maps for the region showed some areas of positive and negative trends, the trends for the PFT H values were nearly all negative.
Discussion
The aim of this study is to demonstrate how a technique that uses both an inverse model (Moisan et al.,
The accuracy in terms of r2 of the pigments predictions from inverting absorption spectra are highest when in situ data are used (Table 2). The accuracies increase when regressing absorption spectra with an additional pigment packaging parameter (O'Reilly and Zetlin,
The techniques's use of pigments estimates with algorithms for PFTs should be used with caution because pigment ratios can vary with phytoplankton species composition, light history, and acclimation to temperature and nutrients (Moisan and Mitchell,
Distribution, seasonality, and biodiversity in the phytoplankton community
The PFTs can be roughly divided into three groups, based on their contribution to PFT diversity as a function of total chlorophyll a (Figure 11). On a large scale, the phytoplankton community was delineated into coastal, mixed and open ocean populations, with open ocean populations having reduced seasonal cycles in terms of biomass but not in terms of PFT diversity. Group 1 consisted of the diatoms. This group dominates the high chlorophyll regions along the coast. This group's distribution becomes insignificant at chlorophyll a levels below 0.45 mg chla m−3. Group 2 is made up of the dinoflagellates, who are found across the coastal and out into the open ocean, but flourish best in the mid ocean shelf region, at the region where diatom disappear. Group 3 is composed of the green algae and the prymnesiophytes and prokaryotes. This group dominates the open ocean region and transitions in the mid-shelf regions to a less dominant group in the coastal region. Although Pan et al. (
Diatoms (Group 1) play a major quantitative role in the coastal zone and had a high relative contribution to total aph(λ) (Figure 5B). Seasonal variability of diatoms was observed in all of the study domain, with much larger variability in the open ocean region associated with the shelf zone, where they dominated in the spring bloom and nearly again in the late fall blooms when they co-existed with the dinoflagellates and prymnesiophytes. In both coastal regions, the diatoms dominated throughout the year and showed much milder seasonal cycles in terms of their relative importance to the chlorophyll levels. In terms of overall biomass, the dominance of diatoms in this highly productive coastal region was high during winter and was lower in the summer (Marshall and Cohn,
The seasonal and spatial variability in the relative dominance (% chlorophyll a) of Group 2 (dinoflagellates) is limited primarily to the shelf regions of the domain, where they are present throughout the year and with a spatial expansion of the population in the fall and winter. They have been found at modest levels in the open ocean ranging from ~200 to 800 cells mL-1 (Makinen and Moisan,
Group 3 algae (prymnesiophytes [coccolithophorids and Phaeocystis], prokatyotes [cyanobacteria] and green algae) are dominant algae in the open ocean regions of the study domain. Of the three PFTs, the prymnesiphytes and green algae are nearly equally important, each accounting for ~40% of the chlorophyll a field. Prokaryotes contributed to only about 10% of chlorophyll a levels and was observed in offshore shore waters and was near absent in onshore coastal waters.
In terms of the biomass (chlorophyll a) levels, the spatial and temporal variance appears to be lower in offshore waters, implying a year-round, stable community (Stramma and Siedler, 1988; Holligan et al.,
Phenology of diatoms, prymnesiophytes, green algae, and dinoflagellates
Climate change will alter environmental conditions within the ocean and invoke a response in the timing and magnitude of phytoplankton diversity, biomass and primary production. The seasonal cycles of the PFTs shows that diatoms had a broad summer minima while prymnesiophytes had a summer peaking maxima and dinoflagellates had a very weak seasonal cycle. PFTs were distributed into unique biomes in the Atlantic Ocean, with one PFT marking the location of the PFT ecotone that has a strong correlation to SST. The seasonality of the pigments that are markers for PFTs was linked to temperature in different ways, with some peaking at a maximal temperature while others responded to a decrease in temperature with increases in biomass (Table 4). Predicted phytoplankton marker pigments revealed seasonal changes in individual PFTs with respect to timing of initiation, peak duration, and demise (Figure 8, Table 4). To understand the phenology of the phytoplankton community over time, three sites of interest were chosen including the Mid-Atlantic Bight, the Gulf of Maine and open ocean, to observe seasonal shifts in phytoplankton community by running the PFT calculations with inputs of MODIS Aqua ChlSAT for nearly fifteen years (2002-2016). Three regions were chosen that represented two coastal and an open ocean regimes. In studying the trends of the time series, we found that the timing of the PFT maxima was different for the three groupings of PFTs and some peaks were sharp while others were broad. The phenology of the phytoplankton communities was related to the oceanographic conditions within each region.
Table 4
| Marker pigment | Location | Duration of initiation | Duration of peak | Duration of termination |
|---|---|---|---|---|
| Chlorophyll a | BIOME | July 28–August 4 | January 17–24 | July 20–27 |
| MAA | January 24–February 1 | April 15–22 | January 17–24 | |
| Open Ocean | June 26−July 3 | March 30−April 6 | June 18−25 | |
| Fucoxanthin | BIOME | July 11−18 | January 17–24 | July 3−10 |
| MAA | March 6−13 | April 23−30 | February 26−March 5 | |
| Open Ocean | September 14−21 | March 22−29 | September 6−13 | |
| Peridinin | BIOME | July 28−August 4 | May 17−24 | July 20−27 |
| MAA | August 13−20 | January 17−24 | August 5−12 | |
| Open Ocean | August 13−20 | February 2−9 | August 5−12 | |
| 19′-Hexa-fuco | BIOME | February 18−25 | August 5−12 | February 2−9 |
| MAA | January 17−24 | August 21−28 | January 9−16 | |
| Open Ocean | March 22−29 | August 5−12 | March 14−21 |
Phenology of certain PFT markers in the study region for 2006 as defined by the dates of the initiation, peak and termination of the seasonal maximum/bloom period.
Diatoms were present in highest concentrations along the coasts and dominated the phytoplankton community and were at a minimum during summer in all zones. During spring and summer, values of 19′hexanoyloxyfucoxanthin (prymnesiophytes) peaked, suggesting that they competed better against the diatoms (Figure 8). Diatoms appeared to tolerate deep mixed layers and cool temperatures during their winter maxima in both coastal and open ocean regions (Longhurst,
Dinoflagellates showed a similar seasonal trend as the diatoms, but with more variability, especially in the open ocean where their fall bloom was relatively stronger than the higher biomass diatoms. Dinoflagellates were closely linked to temperature with higher concentrations at the coast from December to February, with concentrations decreasing in this region during warm summer months. Dinoflagellate concentrations to ratios peaked in the Gulf of Maine and open ocean around January and decreased in summer. Surprisingly, dinoflagellates appear low in concentration in the Mid Atlantic Bight and showed a dampened seasonality. Dinoflagellates may not only be responding physiologically to temperature, but may also respond to temperature indirectly if stratified conditions appear early in the season (Edwards and Richardson,
Prymnesiophytes (19′hexanoyloxyfucoxanthin), a major feature in the North Atlantic, showed distinct peaks in biomass during the summer (July) with an initiation of their bloom in February at all sites (Holligan et al.,
General mechanistic explanations for the phenology of certain PFTs are still controversial, as most phenology has focused on chlorophyll a biomass (Siegel et al., 2002; Ji et al.,
Phytoplankton functional type diversity and climate
A review of the various methods presently in use to estimate PFTs using remote sensing observation (IOCCG,
The assessment of the PTF diversity patterns in the study domain is the first study that has been done which utilizes a number of techniques to yield PFT estimates from phytoplankton absorption spectra modeled using satellite observations. There are a number of recent studies that have created PFT diversity maps using other techniques, including models. Phytoplankton diversity was compared to primary productivity estimates in the California Current region (Goebel et al.,
Are these satellite-derived estimates of H more informative than the traditional species-resolved H estimates, which the Goebel et al. (
In addition to assessments of the ecosystem function for various ocean regions, maps of PFT diversity can be used to monitor any changes to the ocean's ecosystem over longer time. An analysis of satellite chlorophyll a observations demonstrated that while there is no significant trend in the global scale chlorophyll a levels, there are regions in the ocean where chlorophyll levels have increased and decreased over the SeaWiFS satellite lifetime, 1998-2012 (Gregg et al.,
Conclusion
In summary, the process of inverting modeled phytoplankton absorption spectra generated using satellite chlorophyll observations into biomarker pigments and then utilizing the Hirata et al. (
Statements
Author contributions
TM was the senior author of the manuscript and contributed to understanding the relationship between absorption and pigmentation in order to understand diversity in the phytoplankton community. TM was an ecologist who sought to understand the linkages between phytoplankton diversity and Carbon Cycle science. She utilized inherent optical properties to link to satellite oceanography to understand biogeochemical cycles in the ocean. KR is a programmer who participated in all of the mathematical calculations that linked phytoplankton optics to community dynamics in the ocean. She is responsible for all of the graphics and calculations for the paper. She is an early oceanographer budding into satellite oceanography. JM is a physical oceanographer and is responsible for formulating the calculations for the biodiversity of phytoplankton. He is responsible for overseeing mathematical calculations and putting them into an ecological framework to understand carbon Cycle Science. His interest is in understanding climate change and how it relates to phytoplankton diversity. ML participated in the collection and processing of samples from ocean cruises. He also worked with JM and TM in developing the matrix inversion algorithms.
Funding
Funding for this research was provided for by the NASA Ocean Biology and Biogeochemistry Research Program, NASA Goddard Space Flight Center, and The Gordon and Betty Moore Foundation. Grant Number 3292 for Gordon and Betty Moore Foundation and 600-14-4316 for Ocean Biology and Biogeochemistry Research Program.
Acknowledgments
We thank Ms. Kristin Golmon for earlier testing and development of our inversion algorithm through the NASA USRP Student Program. We thank Carla Makinen and Kristen Blattner participation in filtration and cruise logistics. John Morrow helped to deploy the PRR-800 on several of the BIOME cruises. Our HPLC samples (BIOME, COBY, and MAA cruises) were processed through Laurie van Heukelum (HPEL). The authors wish to thank the Ocean Color Processing Group (OBPG) at the NASA Goddard Space Flight Center (Code 616.0), Greenbelt, Maryland for the production and distribution of the MODIS-Aqua data. We thank our reviewers including Astrid Bracher for their excellent and generous comments that improved our work. Our work was partially funded by the NASA Biodiversity Program 05-TEB/05-0016 and NOAA. The paper was prepared under award #NA03NOS4730220 from NOAA, U.S. Department of Commerce and NASA Climate Adaptation Science Initiative (CASI). The statements, findings, and conclusions are those of the authors and do not necessarily reflect the views of NOAA or the U.S. Department of Commerce.
Conflict of interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
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Summary
Keywords
phytoplankton, absorption, diversity, phytoplankton functional type, phytoplankton community, pigments, biodiversity, climate change
Citation
Moisan TA, Rufty KM, Moisan JR and Linkswiler MA (2017) Satellite Observations of Phytoplankton Functional Type Spatial Distributions, Phenology, Diversity, and Ecotones. Front. Mar. Sci. 4:189. doi: 10.3389/fmars.2017.00189
Received
31 March 2017
Accepted
31 May 2017
Published
19 June 2017
Volume
4 - 2017
Edited by
Astrid Bracher, Alfred-Wegener-Institute Helmholtz Center for Polar and Marine Research, Germany
Reviewed by
Hongyan Xi, Helmholtz-Zentrum Geesthacht Centre for Materials and Coastal Research (HZG), Germany; Guoqing Wang, University of Massachusetts System, United States
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© 2017 Moisan, Rufty, Moisan and Linkswiler.
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*Correspondence: John R. Moisan john.r.moisan@nasa.gov
This article was submitted to Ocean Observation, a section of the journal Frontiers in Marine Science
†Deceased 5 June, 2016.
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