INTERNATIONAL JOURNAL OF REMOTE SENSING, 2017 http://dx.doi.org/10.1080/01431161.2017.1308034 TECHNICAL NOTE The effect of phytoplankton pigment composition and packaging on the retrieval of chlorophyll-a concentration from satellite observations in the Southern Ocean Babula Jena Polar Sciences, ESSO, National Centre for Antarctic and Ocean Research, Ministry of Earth Sciences (MoES), Goa, India ABSTRACT ARTICLE HISTORY The Antarctic waters are known to be optically unique and the standard empirical ocean colour algorithms applied to these waters may not address the regional bio-optical characteristics. This article sheds light on the performance of current empirical algorithms and a regionally optimized algorithm (ROA) for the retrieval of chlorophyll-a (chl-a) concentration from AquaModerate Resolution Imaging Spectroradiometer (Aqua-MODIS) and Sea-viewing Wide Field-of-view Sensor (SeaWiFS) in the Indian Ocean Sector of Southern Ocean (IOSO). Analysis indicated that empirical algorithms used for the retrieval of chl-a concentration from Aqua-MODIS and SeaWiFS underestimate by a factor varying from 2 to 2.9, resulting in underestimation when in situ chl-a exceeds about 0.3 mg m−3. To explain these uncertainties, a study was carried out to understand the effect of phytoplankton pigment composition and pigment packaging on remote-sensing reflectance (Rrs,λ), from the analysis of phytoplankton-specific absorption coefficient (aph,*λ). The spatial variation of phytoplankton groups analysed using diagnostics pigments (DP) indicated shifting of the phytoplankton community structure from offshore to coastal Antarctic, with a significant increasing trend for diatoms and a decreasing trend for haptophytes population. The diatomdominated population exhibits lower aph,*λ in the 405–510 nm region (with relative flattening in 443–489 nm) compared with the aph,*λ spectra of the haptophytes-dominated population that peaks near 443 nm. The flattening of aph,*λ spectra for the diatom-dominated population was attributed to its larger cell size, which leads to pigment packaging (intracellular shading) and in turn results in higher Rrs,λ. The relationship between pigment composition (normalized by chl-a) and blue:green absorption band ratios (aph,*443:aph,*555 and aph,*489:aph,*555) corresponding to the Aqua-MODIS and SeaWiFS bands showed in-phase associations with most of the pigments such as 19ʹ-hexanoyloxyfucoxanthin, 19ʹ-butanoyloxyfucoxanthin, peridinin, and zeaxanthin. In contrast, the out-of-phase association observed between the blue: green absorption ratios and fucoxanthin indicated apparent deviations from the general pigment retrieval algorithms, which assumes that blue:green ratios vary in a systematic form with chl-a. The out-of-phase correspondence suggests that the increasing trend of fucoxanthin pigments towards the Antarctic coast was Received 24 August 2016 Accepted 9 March 2017 CONTACT Babula Jena [email protected] ESSO, National Centre for Antarctic and Ocean Research, Ministry of Earth Sciences (MoES), Headland Sada, Goa 403804, India © 2017 Informa UK Limited, trading as Taylor & Francis Group 2 B. JENA associated with the decreasing trend of blue:green absorption ratios and in turn results in higher Rrs,λ. Therefore, an increase in Rrs,λ leads to underestimation of chl-a from Aqua-MODIS and SeaWiFS in the IOSO region. 1. Introduction Sea-surface chlorophyll-a (chl-a) concentration is considered one of the essential parameters for the estimation of primary production and study of carbon dioxide (CO2) dynamics. The observations are important to link the role of the Southern Ocean pelagic ecosystem in the global biogeochemical cycle. In situ observations are sparse around the Southern Ocean because of adverse weather condition, navigational hazards, remote location, and inhospitable environment with high sea states driven by strong winds. Satellite remote sensing of the Southern Ocean colour provides synoptic and time-series coverage of near-surface chl-a concentration dynamics affected by seasonality (Johnson et al. 2013). The synoptic coverage of chl-a concentration is widely used to investigate the dynamics of regional oceanographic features such as fronts, eddies, gyres, upwelling zones, plumes, and surface current patterns. These oceanographic features are useful to study the Southern Ocean ecosystem, which supports large assemblages of phytoplankton, zooplankton, seabirds, seals, and whales. This signifies the need for the retrieval of chl-a from ocean colour sensors with greater accuracy over the Southern Ocean. However, the retrieval is complicated at the regional and local scales as the spectral inherent optical properties (IOPs) of the ocean influencing the ocean colour are complex (Sauer et al. 2012). The satellite-derived chl-a concentration in the Indian Ocean of Southern Ocean (IOSO) may have large uncertainties owing to its different bio-optical characteristics, in addition to sparse matchup observations (in situ and satellite), being used for algorithm development and validation. For example, in order to address the regional biooptical characteristics of the IOSO region (60° E to 100° E and 40° S to the Antarctic coast) for retrieval of chl-a concentration, only 15 in situ bio-optical profiles are available at National Aeronautics and Space Administration (NASA), bio-Optical Marine Algorithm Data set (NOMAD). Mitchell and Holm-Hansen (1991) applied the Coastal Zone Colour Scanner (CZCS) global algorithm (GA; Gordon et al. 1983) in the coastal waters of the western Antarctic Peninsula and the adjacent open ocean waters of Drake Passage. They noticed underestimation of CZCS-derived chl-a and the study highlighted the need for regional algorithm development and validation. In Ross Sea, Moore et al. (1999) validated Sea-viewing Wide Field-of-view Sensor (SeaWiFS)-derived chl-a with in situ-extracted concentration for a range of 0.1–1.5 mg m−3 and the results revealed an underestimation of the SeaWiFS-derived chl-a value. Carder et al. (2003) analysed the Southern Ocean chl-a concentration using the SeaWiFS OC4 algorithm (O’reilly 2000) and revealed significant underestimation of the values between 0.2 and 10.0 mg m−3. Similarly, Korb, Whitehouse, and Ward (2004) reported that the SeaWiFS OC4 algorithm output values were only 87% of the in situ chl-aflu for concentrations lower than 1.0 mg m−3 and only 30% for concentrations above 5.0 mg m−3 in the South Georgia area, Southern Ocean. INTERNATIONAL JOURNAL OF REMOTE SENSING 3 In contrast to earlier studies, Marrari, Hu, and Daly (2006) reported that high-resolution (1 km) daily SeaWiFS chl-a data generated using the global OC4v4 algorithm was an accurate measure over the waters of Antarctic Peninsula, if concurrent in situ data were generated using high-performance liquid chromatography (HPLC). Further investigations by Szeto et al. (2011) showed that SeaWiFS chl-a using the global OC4v4 algorithm consistently underestimates the chl-a value by 50%, although HPLC-based measurements were considered as suggested by Marrari, Hu, and Daly (2006). A recent study by Johnson et al. (2013) reported that the relationship between the maximum band ratio of remotesensing reflectance (Rrs,λ) and in situ chl-a concentration in the Southern Ocean was poorly described by global empirical algorithms and concluded that the current algorithms significantly underestimated the chl-a concentration. They attempted to develop sitespecific algorithms over the entire Southern Ocean for Aqua-Moderate Resolution Imaging Spectroradiometer (Aqua-MODIS) and SeaWiFS, yet most of the matchup biooptical observations were located approximately along the 150° E meridian. The developed algorithms could improve the coefficients of determination (R2) from 0.26 to 0.51 for AquaMODIS and from 0.27 to 0.46 for SeaWiFS. The algorithm development process conducted by Johnson et al. (2013) has not addressed the issues associated with atmospheric corrections. In addition, the algorithm is yet to be validated in the IOSO waters where the regional and seasonal variations in the environment may lead to different bio-optical characteristics. Hence, the present study was carried out over the IOSO waters (60° E to 100° E and 40° S to Antarctic coast, Figure 1) with the detailed objectives as follows: (i) employ the current GA (O’reilly 2000) and the southern ocean algorithm (SOA) (Johnson et al. 2013) for the retrieval and validation of chl-a concentration from SeaWiFS and Aqua-MODIS; (ii) analyse Figure 1. Study area shows ETOPO 1 (Earth Topography One Arc-Minute Global Relief Model, 2009) bathymetric information along with locations of in situ bio-optical observations and HPLC phytoplankton pigments from station 1 to station 10 (filled circles) collected on cruise on board the R/V Roger Revelle (I8SI9 N), used for the development of regional optimized algorithm (ROA). In situ chlorophyll-a concentration collected on cruise on board the R/V Roger Revelle (filled triangles) and world ocean database (squares) were used for validation of ROA. 4 B. JENA the possibility of developing a regionally optimized algorithm (ROA) for the estimation of chl-a concentration; (iii) validate the robustness of the developed ROA, and (iv) diagnose the possible causes of uncertainties in satellite retrieval, particularly the effect of phytoplankton pigment composition on specific absorption coefficient (aph,*λ) through the pigment package effect. 2. Data analysis and methodology 2.1. Satellite measurements of chl-a concentration using current algorithms Generating chl-a data from ocean colour satellites involves two major steps, namely the atmospheric correction of visible bands to derive the water-leaving radiance (Gordon and Wang 1994a, 1994B; Bailey, Franz, and Werdell 2010) and the development of a suitable bio-optical algorithm to estimate the chl-a concentration (O’reilly 2000). NASA’s Ocean Biology Processing Group (OBPG) processes the global Level-0 ocean colour global data sets in near real-time mode and successively processes to generate science-quality product of Rrs,λ. In this article, Level-3 global Standard Mapped Images (SMI) of weekly mean Rrs,λ from Aqua-MODIS and SeaWiFS were acquired from the website (oceancolor.gsfc.nasa.gov). Afterwards, chl-a concentrations from SeaWiFS and Aqua-MODIS are retrieved using various algorithms such as (i) GA (O’reilly 2000), (ii) SOA (Johnson et al. 2013), and (iii) ROA for the IOSO region. The forms of GA, SOA, and ROAM are described in Equations 1–14. 2.1.1. Global algorithms 2.1.1.1. SeaWiFS, OC4v6 ChlorophyllðchlaÞ ¼ 100:32722:9940R þ 2:7218R 1:2259R Rrs;443 > Rrs;490 > Rrs;510 ; R ¼ log10 Rrs;555 2 3 0:5683R4 ; (1) (2) where Rrs is the remote-sensing reflectance 2.1.1.2. Aqua-MODIS, OC3 M-547 . 2 3 4 ChlorophyllðchlaÞ ¼ 100:24242:7423R þ 1:8017R þ0:0015R 1:2280R : Rrs;443 > Rrs;490 R ¼ log10 : Rrs;547 (3) (4) The above algorithm (OC4v6) yields a strong correlation coefficient (r = 0.892) with in situ chl-a concentration on a global scale, which includes samples from all water types (O’reilly 2000). Nevertheless, the accuracy of this algorithm varies regionally. In addition, to address the regional differences, various band combinations and regression coefficients were developed for different water types, with similar band-ratio forms. For example, empirical algorithms were proposed earlier to estimate chl-a concentrations in the Southern Ocean (Johnson et al. 2013) as described next. INTERNATIONAL JOURNAL OF REMOTE SENSING 5 2.1.2. SOA by JOHNSON ET AL. (2013) 2.1.2.1. SeaWiFS, OC4 . 2 3 ChlorophyllðchlaÞ ¼ 100:67362:0714R0:4939R þ 0:4756R : Rrs;443 > Rrs;490 > Rrs;510 R ¼ log10 : Rrs;555 (5) 2.1.2.2. Aqua-MODIS, OC3 . 2 3 ChlorophyllðchlaÞ ¼ 100:69942:0384R0:4656R þ 0:4337R : Rrs;443 > Rrs;490 R ¼ log10 : Rrs;547 (7) (6) (8) The chl-a concentration retrieved in the Southern Ocean using the above-mentioned algorithms yields R2 of 0.51 and 0.46 with in situ chl-a for Aqua-MODIS and SeaWiFS, respectively (Johnson et al. 2013). However, the performance of these proposed algorithms is yet to be validated in the IOSO region. In this article, uncertainties in the retrieval of chl-a concentration from GA and SOA were analysed initially by validating with fluorometrically determined surface in situ chl-aflu during the austral summer (January–February 2004; January–February–March 2006; and February–March 2007). High-quality chl-aflu observations were obtained from World Ocean Database (WOD), National Oceanographic Data Center (NODC), and NOMAD. Details of collection of water samples, data generation, calibration, and quality control for WOD and NOMAD are given in Boyer et al. (2009) and Werdell and Bailey (2005), respectively. A total of 76 in situ chl-aflu observations were available in the study region (Figure 1). The matchups between in situ and satellite observations were generated based on the optimum combinations of spatial and temporal averaging strategy (3 × 3 pixel mean and 8 days mean), a method adopted by several authors (Marrari, Hu, and Daly 2006; Johnson et al. 2013). After implementation of this validation strategy, the number of matchups reduced significantly (Table 1 and Figure 2). Table 1. Validation of chlorophyll-a concentration (mg m−3) derived from Aqua-MODIS and SeaWiFS using various ocean colour (OC) empirical algorithms such as global algorithm (GA), southern ocean algorithm (SOA; Johnson et al. 2013), and regionally optimized algorithm (ROA). Aqua-MODIS SeaWiFS SOA GA (OC3) (OC3) ROA (OC3) GA (OC4) SOA (OC4) ROA (OC2) ROA (OC4) Coefficient of determination (R2) 0.889 0.42 0.84 0.996 0.98 0.99 0.99 Standard error 0.27 0.10 0.27 0.03 0.11 0.04 0.06 4.2–03 4.62–06 1.42–04 4.95–05 1.39–05 p-value 4.31–05 6.6–03 Slope 0.47 0.14 0.13 0.26 0.33 0.27 0.22 Intercept 0.06 0.33 0.19 0.08 0.17 0.14 0.12 No. of observations 10 10 10 06 06 06 06 The rate of underestimation 2.30 2.35 2.46 2.90 2.01 2.32 2.71 6 B. JENA Figure 2. Observation on significant underestimation of chlorophyll-a concentration from (a) AquaMODIS and (b) SeaWiFS using the current empirical algorithms. 2.2. In situ bio-optical measurements for regional optimized algorithms (ROAs) Considering the uncertainties associated with current algorithms (GA, SOA), it was attempted to develop ROAs by utilizing NOMAD-based in situ bio-optical measurements collected on cruise on board the R/V Roger Revelle (I8SI9 N) (Figure 1). The measurements were sparse over the study region having a combination of HPLC- (n = 10) and Fluorometric (n = 05)-determined chl-a concentration corresponding to the period of 17 February 2007 to 6 March 2007. ChlaHPLC is considered for the development of ROAs because HPLC data sets were largely collocated with in situ optical observations and it also accomplishes the main scope of the article: studying the impact of phytoplankton pigment composition on satellite retrieval algorithms. The coincident chl-aHPLC and in situ water-leaving radiance (Lw,λ) observations were extracted for 10 observations. Since Rrs,λ is the standard input for the derivation of geophysical parameters, the Lw,λ converted into Rrs,λ by dividing with spectral solar irradiances (Es,λ) available for MODIS and SeaWiFS bands. Furthermore, empirical ROAs were developed by using coincident Rrs,λ and in situ chl-aHPLC (Equations 9–14, Figure 3), for the retrieval of chl-a concentrations from Aqua-MODIS and SeaWiFS. Earlier studies found that ocean colour satellite retrievals were always underestimated irrespective of comparison with chl-aflu or INTERNATIONAL JOURNAL OF REMOTE SENSING 7 Figure 3. Relationship between in situ chlorophyll-a concentration and the band ratios of in situ remote-sensing reflectance (Rrs,λ) symbolized as dashed lines with ‘+’ representing regionally optimized algorithms (ROAs). The algorithms were applied to (a) Aqua-MODIS, (b) SeaWiFSOC2, and (c) SeaWiFSOC4 for the estimation of chlorophyll-a concentration. Circle represents the relationship between in situ chlorophyll-a concentration and Rrs,λ satellite products from Aqua-MODIS and SeaWiFS as processed by NASA’s Ocean Biology Processing Group (OBPG) . chl-aHPLC (Stuart et al. 2004; Szeto et al. 2011). Hence, the performances of ROAs were evaluated using statistical and graphical criteria considering the in situ chl-aflu from WOD and NOMAD, in the absence of an adequate number of chl-aHPLC observations for validation (Table 1 and Figure 4). In addition, the spatial pattern of the oceanographic features from ROAderived chl-a concentration images was evaluated for its validity (Figure 5). The vertical profiles of in situ chl-a concentration and temperature data available with WOD were analysed to explain the variability of surface oceanographic features from ROA-derived chl-a concentration images (Figure 5). To explain the uncertainties in satellite retrievals, an analysis was carried out to understand the effect of phytoplankton pigment compositions and packaging on Rrs,λ through aph,*λ. The phytoplankton groups were classified through HPLC-determined marker diagnostics pigments (DP) after referring to the methodology given in Hirata et al. (2011) (Table 2), compiled from earlier works of Sieburth, Smetacek, and Lenz (1978), Uitz et al. (2006), and Brewin et al. (2010). The spatial variability of pigment compositions and phytoplankton groups is shown in Figure 6(a,b), respectively. Absorption by the phytoplankton component (aph,λ) was obtained by subtracting the detrital absorption coefficient 8 B. JENA Figure 4. Chlorophyll-a concentration retrieved from (a) Aqua-MODIS and (b) SeaWiFS using various empirical algorithms such as global algorithm (squares), southern ocean algorithm (circles), and regionally optimized algorithm, with (+ and) indicating significant underestimations for elevated values (ellipses) owing to the pigment packaging effect. (ad,λ) from particulate absorption (ap,λ) (data source: NOMAD). The aph,*λ was then calculated as a ratio of aph,λ to HPLC-determined chl-a concentration. The aph,*λ spectra of the dominant phytoplankton groups for various chl-a concentrations were analysed and compared with earlier studies by Ciotti, Lewis, and Cullen (2002) and Bricaud et al. (1995) (Figure 7). In addition, it was analysed to study the variability of aph,*443:aph,*555 and aph, *489:aph,*555 band ratios to determine their relationship with various pigments normalized by chl-a concentration (Figure 8). The effect of pigment composition and pigment packaging on satellite-based Rrs,λ was described in Equation 15. 2.3. Additional data sets To classify the sampling stations belonging to the onshore, offshore, and Kerguelen Plateau waters, ETOPO1 (Earth Topography One Arc-Minute Global Relief Model, 2009) geo-referenced bathymetric data (21,601 by 10,801 cells) was acquired from National Geophysical Data Center (NGDC) and subsetted for the study region (Figure 1). The northeast shifting of pixel location in ETOPO1 was rectified as the method specified in Jena et al. (2012). The data on mean dynamic topography (MDT) and Southern Ocean fronts were analysed to compare the physical features with the biological features (chl-a) derived from Aqua-MODIS and SeaWiFS (Figure 5(a,b)). The MDT of the sea surface was derived from the combined analysis of drifters, satellite altimetry, wind, and GRACE (Gravity Recovery and Climate Experiment) satellite-based geoid (Maximenko and Niiler 2005). Locations of various Southern Ocean fronts were obtained from Australian Antarctic Data Centre (Orsi, Whitworth, and Nowlin 1995). 3. Results and discussion 3.1. Validation of chl-a retrieved using standard GA In situ chl-a data sets during the austral summer (January–February 2004; January– February–March 2006; and February–March 2007) are presented in Figure 1. The chl-a INTERNATIONAL JOURNAL OF REMOTE SENSING 9 Figure 5. Application of regionally optimized algorithm (ROA)-derived chlorophyll-a images from (a) Aqua-MODIS and (b) SeaWiFS for the period of 18–25 February 2006, indicating elevated values all along the Antarctic coast, the Kerguelen plateau waters, and along the southern boundary of the Antarctic Circumpolar Current Front (sACCf). These features were evident in the WOD in situ profiles along (c–d) 60° E, (e–f) 70° E, and (g–h) 80° E transects. The deep-sea chlorophyll-a maxima (DCM) varied from 50 m to 100 m and correspond well with the temperature minimum layer (TML), which is known to be the winter remnant of the Antarctic Surface Water (AASW) that extends northwards from the coastal Antarctic. The mean dynamic topography (MDT) isolines (solid lines) during 18–25 February 2006 were overlaid to interpret the colour features associated with the circulation pattern. Locations of various major Southern Ocean fronts were represented as dashed lines (Orsi, Whitworth, and Nowlin 1995) . concentrations from 76 observations range from about 0.012 to 19 mg m−3 in the study region. After implementation of the validation strategy, the number of matchups between in situ and satellite observations reduced significantly, and the chl-a concentrations range between 0.14 and 5.16 mg m−3 with a mean value of 0.455 mg m−3. The comparative result revealed that in situ measurements in the IOSO waters had significant in-phase correspondence with chl-a concentrations derived from Aqua-MODISGA (R2 = 0.889, p = 4.31–05) and SeaWiFSGA (R2 = 0.996, p = 4.62–06) (Table 1 and 10 B. JENA Table 2. A description on phytoplankton size classes (PSCs) and phytoplankton functional types (PFTs) represented by their pigments (Hirata et al. 2011). PSCs/PFTs Microplankton (>20 μm)b Diatoms Dinoflagellates Nanoplankton (2–20 μm)a Green algae Prymnesiophytesd (Haptophytes) Picoplankton (0.2–2 μm)a Prokaryotes Pico-eukaryotese Prochlorococcus sp. Diagnostic pigments Estimation formula Fucoxanthin (Fuco), Peridinin (Perid) Fuco Perid 19ʹ-Hexanoyloxyfucoxanthin (Hex) Chlorophyll-b (chl-b) Butanoyloxyfucoxanthin (But) Alloxanthin (Allo) chl-b Hex, But 1.41 (Fuco + Perid)/Σ(DP)b 1.41 (Fuco)/Σ(DP)b 1.41 (Perid)/Σ(DP)b (Xn*1.27 Hex + 1.01 chl-b + 0.35 But + 0.60 Allo)/Σ(DP)c Zeaxanthin (Zea), Hex, chl-b Zea Hex, chl-b Divinyl chl-a (DVchl-a) (0.86 Zea + Yp1.27 Hex)/Σ(DP)c 0.86 (Zea)/Σ(DP)b 1.01 (chl-b)/Σ(DP)b 0.74 (DVchl-a)/(chl-a) a Sieburth, Smetacek, and Lenz (1978) b Σ(DP) = 1.41 Fuco + 1.41 Perid + 1.27 Hex + 0.6 Allo + 0.35 But + 1.01 chl-b + 0.86 Zea = chl-a (Uitz et al. 2006) c Xn indicates a proportion of nanoplankton contribution in Hex. Similarly Yp indicates a proportion of picoplankton in Hex (Brewin et al. 2010) d Given that the contributions of Allo to nanoplankton were only a few percentage points in our data set, haptophytes were approximated to Nano minus Green Algae (see also Figure 2 caption of Hirata et al. 2011) e Pico-eukaryotes can be determined from picoplankton minus prokaryotes (see also Figure 2 caption of Hirata et al. 2011). Figure 6. Distribution of HPLC-determined (a) surface phytoplankton pigment compositions and (b) different phytoplankton community structures from onshore (station 1) to offshore region (station 10) during 17 February to 6 March 2007, indicating shifting of the phytoplankton community structure with a significant increasing trend of diatom abundance from offshore to the Kerguelen plateau waters and coastal Antarctica. Station locations are depicted in Figure 1. INTERNATIONAL JOURNAL OF REMOTE SENSING 11 Figure 7. Variability of specific absorption spectra of phytoplankton (aph,*λ) for two typical samples in the Indian Ocean sector of Southern Ocean (dashed lines with circles) compared with earlier studies by Ciotti, Lewis, and Cullen (2002) and Bricaud et al. (1995). The mean spectral shape of aph, *λ for the size fractionation of phytoplanktons (red, green, and blue colour solid lines) was analysed to assess the extent to which the phytoplankton cell size drives the spectral variation of aph,*λ. The spectral characteristics of diatom-dominated phytoplankton populations exhibit lower aph,*λ in the 405–510 nm region (with relative flattening at 443–489 nm) compared to the aph,*λ spectra of haptophytes, which peak near 443 nm. An inverse relationship was observed between chlorophyll-a concentration and aph,*λ, meaning that when phytoplankton abundance increases, larger cell sizes are added incrementally to a background of smaller cells, which leads to pigment packaging (intracellular shading) and in turn aph,*λ decreases. Figure 2). However, there was a systematic underestimation in case of chl-a concentrations derived from Aqua-MODISGA and SeaWiFSGA when the in situ measurements exceeded about 0.3 mg m−3 (Figure 2). The overall magnitude of underestimation for Aqua-MODISGA and SeaWiFSGA was roughly a factor of 2.3 and 2.9, respectively (Table 1). These results of underestimation by satellite observations were well supported by the earlier studies over the Southern Ocean (Moore et al. 1999; Carder et al. 2003; Korb, Whitehouse, and Ward 2004; Stuart et al. 2004; Szeto et al. 2011). To address this issue, Johnson et al. (2013) developed a site-specific algorithm for the entire Southern Ocean with most of the bio-optical matchup observations located approximately along the 150° E meridian. They reported that Aqua-MODISSOA and SeaWiFSSOA (Equations 5–8) were the improved algorithms for the retrieval of chl-a concentration over the Southern Ocean, compared with the operational existing GAs (Equations 1–4). 3.2. Validation of chl-a retrieved using SOA To evaluate the SOA over the study region and validate the retrieved chl-a, Rrs,λ values from Aqua-MODIS and SeaWiFS were processed using Equations 5–8, which are further validated with in situ observations. Table 1 lists the statistics of comparative analysis. The R2 values for Aqua-MODISGA and in situ-measured chl-a values (R2 = 0.889) were much better than those measured from Aqua-MODISSOA and in situ (R2 = 0.42), indicating a better performance of Aqua-MODISGA in the study region. The overall rate of underestimation of chl-a concentration from Aqua-MODISGA (factor of 2.3) remains unaffected even after employing Aqua-MODISSOA (factor of 2.35). The R2 between SeaWiFSSOA and in situ chl-a measurements (R2 = 0.98) had no 12 B. JENA Figure 8. (a) Evident indication of a decrease in the blue:green absorption ratios corresponding to SeaWiFS and Aqua-MODIS bands as associated with an increase in Fucoxanthin:chlorophyll-a pigment. In contrast, other pigments that showed in-phase correspondence with the absorption ratios were (b) 19ʹ-Hexanoyloxyfucoxanthin, (c) 19ʹ-Butanoyloxyfucoxanthin, (d) Peridin, and (e) Zeaxanthin. improvement compared to SeaWiFSGA and in situ chl-a (R2 = 0.99). However, the rate of underestimation of chl-a concentration from SeaWiFSSOA was lesser (factor of 2.01) than that of SeaWiFSGA (factor of 2.9). Although SOA performed better than GA in terms of improvement in slope (Johnson et al. 2013), the SOA-derived chl-a concentration (both for Aqua-MODIS and for SeaWiFS) indicated significant underestimation at high chl-a concentrations and overestimation at low chl-a concentration in the IOSO region (Figures 2 and 4). Considering the uncertainty in GA and SOA, it was further attempted to narrow down the search for a suitable bio-optical algorithm for retrieval of chl-a concentration in the IOSO region. INTERNATIONAL JOURNAL OF REMOTE SENSING 13 3.3. Development of ROA and its application A variety of algorithms developed earlier for the retrieval of chl-a were based on theoretical, empirical, analytical, semi-analytical, or combinations of these approaches, which need to be fine-tuned or improved. The main problem associated with algorithm development or model formulation for parameter retrieval is the complexity of physical processes involved and the uncertainties associated with them (Jena, Swain, and Tyagi 2010). The development of a regional bio-optical algorithm requires a large number of in situ measurements, which is practically difficult to collect in the Southern Ocean considering the adverse weather condition and navigational hazards. In the absence of large bio-optical data sets in the study region, it was experimented with limited observations (n = 10) from NOMAD to construct an ROA. The data set encompasses surface chl-a concentration between 0.149 and 1.547 mg m−3 in the sampling stations from 1 to 10 (Figure 1). Typical chla concentrations between 0.05 and 1.50 mg m−3 were also reported earlier in the Southern Ocean (Arrigo et al. 1998; El- Sayed 2005). Interaction of irradiance, deep mixing, iron, and grazing is known to limit phytoplankton growth all over the Southern Ocean (Boyd 2002; Daly et al. 2001; Moline and Prézelin 1996; Venables and Moore 2010). Elevated chl-a concentrations between 1 and 30 mg m−3 were also reported in regions of continental shelf and ice edge areas (El- Sayed 2005; HolmHansen et al. 1989; Moore and Abbott 2000). The ocean colour algorithms based upon blue to green ratios of Rrs,λ have been used widely to derive chl-a concentration from ocean colour sensors (Carder et al. 2003; Gordon et al. 1988; O’reilly et al. 1998; O’reilly 2000). In this article, the NOMAD-based Rrs, λ versus in situ chl-aHPLC coincident data sets during 17 February 2007–6 March 2007 were utilized to develop empirical ROAs for the retrieval of chl-a concentration from Aqua-MODIS and SeaWiFS. The ROAs are presented below in Equations 9–14, and as a dashed line in Figure 3. 3.3.1. Aqua-MODISROA, OC3 ChlorophyllðchlaÞ ¼ 100:0803:705R þ 18:41R 42:41R Rrs;443 > Rrs;490 R ¼ log10 : Rrs;547 2 3.3.2. SeaWiFS ROA, 3 þ 30:02R4 : (9) (10) OC2 ChlorophyllðchlaÞ ¼ 100:1062:907R þ 8:885R Rrs;490 R ¼ log10 : Rrs;555 2 12:27R3 : (11) (12) 3.3.3. SeaWiFSROA, OC4 ChlorophyllðchlaÞ ¼ 100:2285:416R þ 25:1R 53:30R Rrs;443 > Rrs;490 > Rrs;510 R ¼ log10 : Rrs;555 2 3 þ 36:34R4 : (13) (14) 14 B. JENA The Aqua-MODISROA OC3 output yielded a strong R2 of 0.84, with in situ chl-a. Yet, the chl-a concentrations were underestimated by Aqua-MODISROA compared with in situ measurements (Figure 4). The SeaWiFSROA OC2 and OC4 outputs yielded a strong and one of the highest R2 with in situ chl-a (R2 = 0.99) (Table 1). The rate of underestimation and standard error were minimal in case of OC2 compared to that in OC4 (Table 1). The performance of OC2 was better than OC4 for SeaWiFS-based chl-a retrieval, because it employs the 490:555 nm band ratio and the atmospheric correction is much better in the 490 nm band compared to that in the 443 nm band (Carder et al. 2003). To evaluate the spatial pattern of oceanographic features from the ROA-derived chl-a images, the Rrs,λ from Aqua-MODIS and SeaWiFS was processed using Equations 9–14, for the period of 18–25 February 2006, and further compared with the WOD in situ profiles (Figure 5). Aqua-MODISROA and SeaWiFSROA chl-a images indicated elevated values all along the Antarctic coast, Kerguelen Plateau waters, and along the southern boundary of Antarctic Circumpolar Current Front, sACCf (Figure 5(a,b)). The elevated values of chl-a concentration from Aqua-MODISROA and SeaWiFSROA agreed well with the WOD in situ data collected along the 60° E, 70° E, and 80° E meridional transects (Figure 5(c–h)). The depth of deep-sea chl-a maxima (DCM) varied from 50 m to 100 m and corresponds well with the temperature minimum layer (TML), which is known to be the winter remnant of the Antarctic Surface Water (AASW) that extends northwards from the coastal Antarctic (Figure 5(c–h)) (Holm-Hansen, Kahru, and Hewes 2005). The surface oceanographic features such as fronts, eddies, and meanders were well captured by Aqua-MODISROA- and SeaWiFSROA-retrieved chl-a images. The features agreed well with the regional circulation pattern as inferred from the MDT data sets. Both Aqua-MODISROA and SeaWiFSROA images clearly indicated intense phytoplankton blooms above the Kerguelen plateau waters and its downstream section along the polar front (PF). The sedimentary source of iron from the island and the surrounding shallow plateau can fertilize the mixed layer, and possibly cause the bloom (Figure 5(a,b)). These blooms are important both as the base of the regional food web and for the carbon that they capture and export to the deep oceans (Jena 2016; Mishra, Naik, and Anilkumar 2015). Albeit the surface water above the Kerguelen plateau is rich in chl-a, an exception of the oligotrophic condition dominated in between the north Kerguelen plateau (NKP) and the south Kerguelen plateau (SKP) due to apparent intrusion of iron-limited high nutrient-low chlorophyll (HNLC)-regime waters from the Enderby basin through the Fawn trough current (Figure 5). All these distinct features were also observed by the chl-a concentration images retrieved using GA and SOA (figures not shown), and supported the validity of ROA in terms of the spatial patterns of features. Although the oceanographic features were well captured from Aqua-MODIS and SeaWiFS chl-a images using all empirical algorithms, an accurate quantitative estimate of phytoplankton biomass in the Southern Ocean remained inconclusive and challenging. For example, evidence from our present analysis in the IOSO waters in addition to earlier studies suggested that all empirical algorithms (GA, SOA, and ROA) used for the retrieval of chl-a concentration from Aqua-MODIS and SeaWiFS were found to underestimate by a factor of 2 at least and can be as large as 2.9 (Table 1). In particular, there was a significant underestimation by Aqua-MODIS and SeaWiFS chl-a concentrations when the in situ measurements exceeded about 0.3 mg m−3 (Figure 2) even after INTERNATIONAL JOURNAL OF REMOTE SENSING 15 employing any empirical algorithms. To explain these observed uncertainties, an analysis was carried out in the following section to understand the effect of phytoplankton pigment compositions on the marine Rrs,λ from the analysis of IOPs. Besides, the possible sources of uncertainties were also investigated when the standard atmospheric correction scheme was applied to the IOSO region. 3.4. Diagnosis on the potential causes of observed uncertainties The Antarctic waters are known to be optically unique and the standard empirical ocean colour algorithms applied to these waters may not address the regional bio-optical characteristics. Being Case-1 water, the algorithms that relate blue to green Rrs,λ ratio (OC2, OC3, OC4, etc.) should not fail to measure the chl-a concentration in the Antarctic waters. The reason for this failure is hypothesized first to the presence of optically complex waters due to the influx of glacial and sea-ice melted water, which can increase particle concentrations in the nearshore region and result in a conducive environment for a distinct phytoplankton assemblage with the dominance of large cell size planktons (e.g. large diatom cells). For example, few important studies by Smith and Nelson (1985) and Arrigo et al. (2012) provided evidence on increased phytoplankton growth and accumulation within the marginal ice zone (MIZ) due to melt water production and stratification. Second, the mesoscale physical process induced by baroclinic instabilities is hypothesized to alter the bio-optical characteristics of the Kerguelen Plateau waters and its downstream region after Antarctic Circumpolar Current (ACC) encounters the Kerguelen Plateau topography. The Kerguelen Ocean and Plateau compared Study (KEOPS) by Maraldi et al. (2009) showed an increase in chl-a concentration above the plateau and attributed it to the availability of iron coming up from the seafloor after the interaction of strong currents with the Kerguelen Plateau. The physical processes are known to enhance the particle concentrations and trigger phytoplankton blooms (Figure 5(a,b)) in the euphotic zone through nutrient injection, often accompanied by large-sized cells (e.g. large diatom cells). The increase in phytoplankton pigment concentration and size can have a significant impact on Rrs,λ through the variability of IOPs, and in turn the standard empirical algorithms may fail to accurately measure the chl-a concentration. These hypotheses were experimented further by determining the effect of phytoplankton pigment compositions on aλ and Rrs,λ. Since Rrs,λ depends both on the variability of IOPs (e.g. phytoplankton absorption and scattering coefficients) and the geometric distribution of the light field, IOPs can be used to model Rrs,λ. A brief summary of the Rrs,λ model used by Lee et al. (1994) and Carder et al. (2003), is described as follows: Rrs;λ ¼ fλ Qλ 2 t bb;λ ; n2 aλ þ bb;λ (15) where f(λ) is an empirical factor. Q(λ) is calculated as the upwelling radiance (Lu) to the corresponding upwelling irradiance Eu (Q = Eu/Lu), which describes the non-isotropic character of the radiance field. Both f and Q factors are variable and strongly dependent on the solar zenith angle, geometric distribution of the light field, and IOPs. t is the 16 B. JENA transmittance of the air–sea interface, and n is the refractive index of sea water. The value of t2/n2 is equivalent to 0.54, but can vary with sea-state condition and is relatively independent of wavelength (Carder et al. 2003). aλ and bb,λ are absorption and backscattering coefficients, respectively. The spectral behaviour of bb,λ is not as dynamic as that of aλ (Carder et al. 2003). Considering the variability of parameters described in the above-mentioned equation, aλ was hypothesized to affect Rrs,λ dominantly. To investigate it, the impact of phytoplankton pigment compositions on aλ was studied. The impact of aλ on Rrs,λ can explain the observed underestimation of satellite-retrieved chl-a concentration in the study region. 3.4.1. Phytoplankton pigment composition and spectral absorption properties Figure 6(a) shows the distribution of surface phytoplankton pigment composition during austral summer (17 February 2007 to 6 March 2007), indicating shifting of the phytoplankton community structure from the coastal Antarctic (station 1) to the offshore region (station 10). The most dominant pigments were fucoxanthin and 19ʹ-hexanoyloxyfucoxanthin (19ʹ-HF), in addition to the presence of a smaller proportion of diadinoxanthin, 19ʹ-butanoyloxyfucoxanthin (19ʹ-BF), peridinin, zeaxanthin, and other pigments. The chl-aHPLC concentration during this period ranges from 0.149 to 1.547 mg m−3, with the highest values observed near the Antarctic coast. The pigment compositions in the coastal Antarctic (station 1) and Kerguelen Plateau waters (stations 2–4) were characterized by the highest proportion of fucoxanthin pigments, indicating the presence of diatoms. In these waters, the phytoplankton populations were dominated by 53–78% of diatoms as determined using DP analysis (Table 2 and Figure 6(b)). Furthermore, the offshore stations off Kerguelen Plateau (stations 5–10) were characterized by the highest proportion of 19ʹ-HF pigments (indicative of haptophytes), dominated by 48–69% of phytoplankton populations (Figure 6(b)). Analysis indicated that there was a shifting of phytoplankton community structure from offshore to coastal Antarctic, with a significant increasing trend of diatoms population and a decreasing trend of haptophytes population (Figure 6(b)). The spectral absorption characteristics of these dominant phytoplankton groups were analysed further to determine its effect on Rrs,λ. The spectral characteristics of aph,*λ are known to vary as a function of pigment composition and pigment packaging, attributed to intracellular shading (Morel and Bricaud 1981). The decreased absorption of pigments in cells compared with the absorption potential of the same amount of pigments is being described as the pigment-packaging effect (Duysens 1956; Kirk 1976, 1994; Geider and Osborne 1987; Morel and Bricaud 1981; Sathyendranath, Lazzara, and Prieur 1987). Pigment packaging occurs when the cell size increases (e.g. large diatoms) or the internal concentration of pigments increases (Kirk 1976; Morel and Bricaud 1981; Sosik and Mitchell 1994), which yields flattening of absorption peaks in the blue spectrum (Dierssen and Smith 2000; Stuart et al. 2004). To examine the effect of pigment composition and packaging, the aph,*λ spectra of the dominant phytoplankton groups for various chl-a concentrations were analysed and compared with earlier studies by Ciotti, Lewis, and Cullen (2002) and Bricaud et al. (1995) (Figure 7). Analysis indicated that the spectral characteristics of diatom-dominated phytoplankton populations (diatoms = 74.1%; haptophytes = 21.7%) exhibit lower values of aph,*λ in the 405–510 nm region (relatively flattening at 443–489 nm) compared to the aph,*λ spectra of haptophytes-dominated phytoplankton INTERNATIONAL JOURNAL OF REMOTE SENSING 17 populations (haptophytes = 69%, diatoms = 17.6%) that peak near 443 nm. Increase in chl-a concentration was associated with a decrease in aph,*λ, which indicated that when the phytoplankton abundance increases, larger cell sizes are added incrementally to a background of smaller cells (Ciotti, Lewis, and Cullen 2002), leading to pigment packaging (intracellular shading) and in turn decreasing aph,*λ (Figure 7). To assess the extent to which the phytoplankton cell size drives the spectral variation of aph,*λ, the mean spectral shape of aph,*λ for the size fractionation of phytoplankton was studied by Ciotti, Lewis, and Cullen (2002). The study revealed the cell size (pico, nano, and micro phytoplanktons) could explain more than 80% variability in the spectral shape of aph, *λ. The effect of pigment packaging is prominent for microphytoplanktons (with the flattening of the blue region aph,*λ spectra) compared with pico- and nanophytoplankton (Figure 7). The relative flattening of the aph,*λ spectra in the 443–489 nm region for the diatom-dominated phytoplankton population can be attributed to pigment packaging (Figure 7), to the fact that the sizes of diatoms in the Antarctic waters are much larger (Brody et al. 1992). The observed flattening of the aph,*λ spectra (blue band) for the diatom-dominant phytoplankton population and the elevated chl-a concentration results in greater Rrs,λ since absorption is inversely related to Rrs,λ (Equation 15). Therefore, an increase in Rrs,λ leads to an underestimation of satellite-retrieved chl-a concentration for elevated in situ chl-a concentration. Furthermore, the variability of aph,*443:aph,*555 and aph,*489:aph,*555 band ratios (corresponding to SeaWiFS and Aqua-MODIS bands) was analysed to determine their relationship with pigment composition normalized by chl-a concentration (Figure 8). In-phase association was observed between blue:green band ratios and pigments such as 19ʹ-HF, 19ʹ-BF, peridinin, and zeaxanthin (Figure 8(b–e)). The proportion of 19ʹ-HF to chl-a could explain about 76% of the variance (r = 0.87) in aph,*443:aph,*555, and for aph,*489:aph,*555, it was about 73% (r = 0.85). In contrast, out-of-phase association was observed between blue:green band ratios and fucoxanthin pigments, indicating a decrease in the absorption ratio as associated with increase in fucoxanthin pigments (Figure 8(a)). Analysis indicated that 72.9% of the variance (r = −0.85) in aph,*443:aph,*555 could be explained by the proportion of fucoxanthin:chl-a, and for bands aph,*489:aph,*555 the variance explained was about 68% (r = −0.82). The out-of-phase correspondence suggests that the increasing trend of fucoxanthin pigments towards the Antarctic coast was associated with the decreasing trend of blue:green absorption ratios. The decrease in blue:green absorption ratio leads to greater Rrs,λ, which in turn underestimates the chl-a concentration from various empirical algorithms used for Aqua-MODIS and SeaWiFS. 3.5. Possibility of improper atmospheric correction algorithm In addition to the evidence of pigment composition and packaging effect on the empirical algorithms, the processes involved in atmospheric correction can be a major source of uncertainty for the derivation of Lw,λ and in turn effect the retrieval of chl-a concentration from satellite observations. High concentrations of secondary organic aerosols like isoprene found over the coastal Antarctica, especially in the Prydz Bay and the fluxes, were reported up to 1200 μg m–2 day–1 (Hu et al. 2013). Investigations are required to study the potentially complicated mixtures of different aerosol types and 18 B. JENA their spatio-temporal variations over the IOSO region, which can produce significant error in the atmospheric correction procedure. The classical atmospheric correction procedure assumes the Lw,λ is zero in the nearinfrared part of the electromagnetic spectrum. This assumption is known to be invalid over a high concentration of water-scattering constituents and shallow bathymetry (causing bottom reflectance). The recent atmospheric correction algorithms therefore account for the non-zero water-leaving signal in the Near Infrared (NIR) by applying a coupled approach for the separation of atmospheric and aquatic contributions to the signal (Sathyendranath 2000). In case of Antarctic waters, the presence of sea ice and icebergs in the field-of-view of the sensor would also contaminate the surrounding desired Lw,λ. Gregg and Casey (2004) provided evidence on the contamination of ocean colour observations by sea ice in their effort to validate the SeaWiFS chl-a concentration data. Similarly, Belanger, Ehn, and Babin (2007) and Wang and Shi (2009) examined the impact of backscattered photons from snow and sea ice on the desired Rrs,λ in the Arctic region, and indicated the impact can be several kilometres from the ice edge due to adjacency effect. The large solar zenith angle in the study area can be another source of uncertainty while performing atmospheric correction. Both f and Q in Equation 15 are known to be dependent on the solar zenith angle. The Southern Ocean regions have large solar zenith angles and the proportion of diffuse sky light is high, especially in the blue part of the spectrum (Dierssen and Smith 1997). Morel and Gentili (1993) modelled the changing trends in f:Q with latitudes and reported that the f:Q ratios are 5% greater in the polar regions than in the temperate regions. Since the f:Q ratio is directly proportional to Rrs,λ, an increase in the f:Q ratio would result in a higher Rrs,λ value (Equation 15) and in turn can lead to lower chl-a concentration. The effect of f:Q ratio can have a propounded effect on Rrs,λ in the study region considering the high latitudes, which range from 40° S to 41° S (Coastal Antarctic). Once all these issues are accounted for, the Lw,λ can be assessed precisely to further retrieve the chl-a concentration from the satellite observations. 4. Conclusion An accurate quantitative estimate of chl-a concentration from the satellite observations in the southern IOSO region remained inconclusive and challenging. For instance, it is confirmed that the chl-a concentration retrieved from Aqua-MODIS and SeaWiFS using empirical algorithms (GA, SOA, and ROA) indicated significant underestimations for elevated in situ values owing to the dominance of fucoxanthin pigments (a biomarker of diatom) and pigment packaging effect. Hence, the utilization of these empirical algorithms could lead to large erroneous result while studying the long-term trends of chl-a concentration and phytoplankton productivity in the context of climate change. An optimized bio-optical algorithm is required based on the absorption coefficient to account for the differences in the bio-optical characteristics of a diatom group of phytoplanktons. The utility of the algorithm must be improved and validated with the collection of more in situ bio-optical observations. The algorithm is essential for the monitoring of diatom-dominated phytoplankton blooms and for the precise estimation of the oceanic role in the biogeochemical cycle of carbon, specifically the importance of INTERNATIONAL JOURNAL OF REMOTE SENSING 19 the Southern Ocean as a sink for atmospheric CO2. The need for continuous long-term ocean colour observations indeed exists for the regular monitoring of Antarctic marine ecosystems. Acknowledgements Continuous support from Dr M. Ravichandran, Director, National Centre for Antarctic and Ocean Research (NCAOR), Dr Thamban Meloth (Group Director, Polar Sciences, NCAOR), and Dr Alvarinho Luis (NCAOR), is gratefully acknowledged. MODIS and SeaWiFS data sets were provided by National Aeronautics and Space Administration (NASA) Goddard Space Flight Center (NASA’s GSFC). The authors would like to acknowledge all scientists and crew members of R/V Revelle cruise (I8SI9N) who collected and analysed in situ bio-optical profiles and pigments that have gone into the NASA bio-Optical Marine Algorithm Data set (NOMAD). In situ chl-a and temperature profiles were obtained from National Oceanographic Data Center (NODC). Earth Topography One Arc-Minute Global Relief Model, 2009 (ETOPO1) bathymetric data was acquired from National Geophysical Data Center (NGDC). This is NCAOR contribution no 09/2017. Disclosure statement No potential conflict of interest was reported by the author. 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