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Variability of particulate backscattering ratio and its relations to particle intrinsic features in the Bohai Sea, Yellow Sea, and East China Sea

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Abstract

Using two field cruise observations collected during September and December 2016 in the Bohai Sea (BS), Yellow Sea (YS), and East China Sea (ECS), our study explores the variability of the particulate backscattering ratio (i.e., a ratio of particulate backscattering, bbp in m−1, to particulate scattering, bp in m−1, denoted as b˜bp, dimensionless). A large variation of b˜bp (using 550 nm as a delegate) in magnitude is observed in the study regions, ranging from 0.0004 to 0.043 (with an average of 0.015 ± 0.0082), which implies optically complex water conditions. Spectral variation in b˜bp is analyzed quantitatively by our proposed so-called “spectral dependence index,” K, recommended as a standard way to determine quantitatively the spectral dependence of b˜bp in water bodies worldwide. The driving mechanism on the b˜bp variability in the study regions is researched for the first time, based on those synchronous data on particle intrinsic attributes, herein mainly referring to particle concentration (TSM, for the content of total suspended matter), composition (using a ratio of Chla/TSM as a surrogate, where Chla refers to the content of chlorophyll a), mean particle size (DA), and mean apparent density (ρa). The TSM, Chla/TSM, and DA cumulatively contribute most (97.8%) of the b˜bp variability, while other factors, such as the ρa, show a weak influence (0.04%). Meanwhile, we model b˜bp with direct linkages to TSM, Chla/TSM, and DA by using a linear regression method, with low estimation errors (such as mean absolute percentage error, MAPE, of about 14%). In short, our findings promote an understanding on the essence of the b˜bp in the BS, YS, and ECS, and are significantly beneficial to the comprehensive grasp of those complex features on suspended particles and those related to biogeochemical processes in marine waters.

© 2019 Optical Society of America under the terms of the OSA Open Access Publishing Agreement

1. Introduction

The particulate backscattering ratio (b˜bp, see symbols in Table 1), conventionally defined as a ratio of particulate backscattering coefficient (bbp) to scattering coefficient (bp), is an important optical quantity for characterizing the suspended particles in marine waters [1–7]. This parameter can provide significant information on suspended particles, such as their material composition and size distribution [2,8–10]. It has also been used in radiative transfer simulation of water columns, and semianalytical remote sensing algorithms, to detect those inherent optical properties [2,3,11–13]. Thus, a detailed understanding and documentation of b˜bp variability is of fundamental importance to the overall comprehensive cognition of the complex features of the suspended particles and many marine ecological and biogeochemical processes.

Tables Icon

Table 1. Symbols and Units for the Parameters Used in This Study

The b˜bp, along with the bp, is commonly used to model the bbp, which is a more direct inherent optical quantity used to simulate the remote sensing signals of water bodies in bio-optical models [11,14,15]. Therein, this parameter is initially assumed to be constant, or to change inversely with pigment concentrations [11,15]. However, the subsequent investigations demonstrate that the b˜bp may be not constant and will vary among different particulate features in different water conditions [1,2,4,8–10]. Qualitative analysis on the influence of the particulate feature factors on the b˜bp changes can be found in previous studies. Those related factors can be summarized as the composition of the particulate assemblage [1,2,4,5,10,16], the particulate sizes, structures, and shapes [2,7–10], the small particles [2,8–10], and the bulk refractive index [9].

Indeed, the association of the b˜bp with the particulate feature factors can be verified by Mie scattering theory, where the b˜bp for a collection of particles can be expressed as follows [9]:

b˜bp=0Qbbex2f(x)dx0Qbex2f(x)dx

where x is the size parameter given by x = (πDnw)/λ, where D is the particle diameter, nw is the seawater refractive index, and λ is the wavelength; f(x) is the probability density function that can derive the particle size distribution, i.e., Kf(x), where K is the total number of particles per unit volume; Qbbe and Qbe are the effective backscattering and scattering efficiency factors, respectively; Note that the optical efficiency factors are essentially influenced by the composition, size distribution, density, and refractive index of the suspended particles [9,17–21]. In theory, the b˜bp is closely related to those feature factors of the suspended particles.

Nevertheless, we do not know or adequately understand the b˜bp variability, in spite of the abovementioned theoretical relationship and limited qualitative analysis shown in the previous studies. Questions remain as to how the b˜bp changes and whether these changes are in spectrum or in value magnitude. Factors that play important roles in the variability of the b˜bp remain unknown. Providing clear answers to these questions is of great significance to the true understanding of b˜bp changes, particulate backscattering/scattering properties, the underwater radiative transfer of light, and even water color remote sensing.

The current study selects the Bohai Sea (BS), Yellow Sea (YS), and East China Sea (ECS) as the investigated water areas, which are typically large shallow and turbid coastal waters, and represent those so-called optically complex Case II water conditions. By means of an in situ observed data set from two cruise surveys, conducted for the study areas in Sep. and Dec. 2016, the purpose of this study is to explore the variability of the b˜bp, such as its spectral dependence features and value changes. More importantly, this study focuses on the influence of various particulate feature factors to the b˜bp, which are analyzed quantitatively for the first time. Corresponding discussion is attached subsequently.

2. Data and methods

2.1 Study areas and cruise surveys

The investigated water regions of this study are the BS, YS, and ECS [Fig. 1], which are typically large and shallow marginal seas of the western North Pacific. The BS shows a mean depth of 18 m, with most water areas less than 30 m [22], whereas the average depth of the YS is approximately 44 m [23], and the ECS shows an average depth of approximately 370 m, with most areas (~70%) below 200 m [24,25]. These marginal seas (BS, YS and ECS) are significantly influenced by a large quantity of sediment loads from river discharge, together with productive waters induced from industrial and agricultural pollutions, as well as domestic sewage [26,27]. Our study areas are thus typically turbid coastal water bodies with complex optical conditions.

 figure: Fig. 1

Fig. 1 Study areas in the BS, YS, and ECS, overlaid by those stations during two cruises that are carried out in Sep. and Dec. 2016, respectively. Bathymetric contours are color coded.

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Two cruise surveys were carried out during Sep. and Dec. 2016 in the BS, YS and ECS (Table 2). A total of 118 sampling stations were collected for this study. For each station, a series of measurements were implemented by means of optical instruments including a WET Labs AC-S, a HOBI Labs Hydroscat-6 (HS-6), a Sequoia LISST-100X, and a Seabird SBE49 CTD. They were formed to an optical profiling package. This optical package was first fastened to a hydrological winch that could control the raising and lowering of the package. Before the official observation, the optical package would be descended into the water column at a depth of several meters for environment adaptation about 4 min. Then, this package was lifted up to just beneath the surface of water bodies, and then dropped down slowly to the bed.

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Table 2. Description of the Two Cruise Surveys in This Study

2.2 Determination of optical parameters

The optical parameters used in this study covered bbp, bp, and b˜bp. The bbp could be observed by using the HS-6 meter, whereas the bp was measured by means of the AC-S instrument. Before the cruise surveys, the HS-6 meter was first calibrated to assure its accurate and stable performance within factory specifications. The HS-6 used in the current study has six spectral bands, i.e., 442, 488, 550, 620, 700, and 852 nm bands. This instrument measures a single-angle (about 140°) volume scattering function at the backward direction [28], which can be further transformed into backscattering by using corresponding calibration coefficients. The effects by path length attenuation were corrected by carrying out the sigma correction (see details in Hydroscat-6 User’s Manual from www.hobiservices.com). The AC-S meter had been calibrated by using Milli-Q water before and after the cruise surveys, with repeatable readings in all spectral bands below 0.005 m−1. The effects of temperature and salinity were corrected by using the method described by WET Laboratories User’s Guide from www.wetlabs.com, and absorption measurements were calibrated for the effects of reflective tube scattering following Sullivan et al. (2006) [29]. Detailed descriptions on HS-6 and AC-S measurements to obtain the bbp and bp can be found in Sun et al. (2017) [30]. After obtaining the bbp and bp, the b˜bp can be thus derived by dividing bbp by bp. However, it should be noted that particulate backscattering ratios at five bands, namely, 442, 488, 550, 620, and 700 nm bands, were finally used in our study, since the AC-S measurements do not cover the 852 nm band of the HS-6.

2.3 Determination of physical and biogeochemical parameters

Those physical and biogeochemical parameters, analyzed in the present study, include Chla (in mg m−3), TSM (in mg l−1), ISM (in mg l−1), OSM (in mg l−1), DA (in μm), and ρa (in kg l−1). The Chla measurement required a first filtering of 1-2 L water samples by means of 47-mm Whatman GF/F filters. Then, the filters were frozen and stored in liquid nitrogen, and transferred to the laboratory on land. A reverse-phase HPLC technique was used to analyze the pigments; furthermore, the method of Van Heukelem and Thomas (2001) [31] was utilized to separate and quantitatively extract the Chla. For the measurements of suspended matter concentrations, the collected 0.5-2 L water samples were first percolated onto preweighed 47-mm Whatman GF/F filters. After rinsing the filters with distilled water at least three times, they were stored in a freezer at 20 °C and transferred to the laboratory on land. Then, these filters were dried under 105 °C for approximately four hours, which were reweighed for achieving the TSM. Subsequently, they were transferred into a muffle furnace for one hour under 500 °C and reweighed to derive the ISM. The OSM could thus be calculated by subtracting the ISM from the TSM.

This study used a LISST-100X (Type-C) instrument to observe the size distribution of suspended particles in waters. This instrument could directly measure the near- forward-angles light, which could be used to derive the V(Di) (particle volume concentration, in μl l−1, where Di refers to the i-th diameter, in μm) based on Mie theory. The details on the LISST measurements can be seen in our previous publication [30]. According to the following equation, the N(Di) (particle number concentration, in counts m−3), can be calculated:

N(Di)=6V(Di)/πDi3

The [AC]i (particulate cross-sectional area concentration at size bin i, in m−1) can be deduced as follows:

[AC]i=32DiV(Di)

By summing all size bins, we can obtain the [AC]t (the total of particulate cross-sectional area concentrations at all size bins, in m−1). Accordingly, the DA (in μm) can be obtained as follows:

DA=i=231[AC]iDi[AC]t

The ρa (in kg l−1) can be calculated as below (Bowers et al., 2009):

ρa=TSMV(Dt)

2.4 Mathematical statistic methods

This study implemented a statistical description analysis on the optical, physical, and biogeochemical parameters collected in the study areas. When descriptive statistics for these parameters were calculated, mathematical analyses (such as correlation and regression methods) were performed to find the potential links between different quantities. Several error indicators, used to assess the model’s performance in the present study, include the MAPE, RMSE (root mean square error), NRMS (normalized root mean square error), and mean ratio, which can be obtained as below:

MAPE=1ni=1n|xiyixi|(100%)
RMSE=1ni=1n(xiyi)2
NRMS=stdev(|xiyixi|)
meanratio=1ni=1n(xiyi)
where xi and yi denote the observed and estimated values, respectively; n is the sample number.

3. Results

3.1 Variability of water bio-optical conditions

The investigated water bodies of the current study show relatively large variations in bio-optical conditions. The observed Chla ranges from 0.20 to 6.55 mg m−3, with a mean of 1.37 mg m−3 (S.D. = 0.97 mg m−3, CV = 71%), whereas TSM shows a large span of magnitude, i.e., from 0.41 to 223.87 mg l−1, with a CV of 190% (Table 3). There generally exists more ISM (mean = 15.57 mg l−1) in the total suspended particles than OSM, with a mean of 1.81 mg l−1, which indicates a potentially important influence from terrigenous discharge and sediment resuspension. Correspondingly, the bp and bbp (using 550 nm as a reference) also show large variation of magnitude (Table 3). In this study, we observe a variation of b˜bp(550) ranging from 0.0004 to 0.043, and a mean of 0.015 (S.D. = 0.0082, CV = 55%). Meanwhile, the parameters that characterize the intrinsic characteristics of the suspended particles, including DA, ρa, and Chla/TSM, are also measured with their variations, as shown in Table 3 in this study.

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Table 3. Statistical Distribution of Those Water Bio-Optical Parameters

3.2 Spectral dependence of particulate backscattering ratio

The b˜bp(λ) observed in this study generally shows few large spectral variations [Fig. 2(A)], though there still exist several individual stations with somewhat great changes between different wave bands. As shown in Fig. 2, the averaged b˜bp(λ) spectrum presents a roughly gentle trend from the short to long wave bands. Even so, in order to accurately characterize the spectral dependence of theb˜bp(λ), this study used b˜bp(550) as a reference and then analyzed the relationships between b˜bp(λ) with b˜bp(550), using a linear regression function such as y = K * x. Here, the parameter K can be defined as “spectral dependence index” to quantitatively indicate the spectral dependence of the b˜bp(λ). It can be conveniently calculated without a unit, and importantly easy-to-use to reflect a general spectral variability normalized to a reference baseline. It would show a potentially important application in future. Very close relationships between b˜bp(λ) with b˜bp(550) can be obtained with corresponding determination coefficients (R2) above 0.917 (p<0.0001) [Figs. 3(A)-3(D)]. The obtained parameter K for the 442, 488, 620, and 700 nm bands are 0.954, 0.940, 0.943, and 0.965, respectively, with K = 1 for the reference 550 nm band [Fig. 3(E)].

 figure: Fig. 2

Fig. 2 Spectra of particulate backscattering ratios, depicted by the in situ data sets collected in this study.

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 figure: Fig. 3

Fig. 3 Statistical linear relationships between the particulate backscattering ratios at wavelengths including 442 nm (A), 488 nm (B), 620 nm (C), and 700 nm (D), with that at the 550 nm reference. These regressions were produced by using 118 in situ samples, observed by the HS-6 instrument. Panel E refers to the spectral dependence index, K, defined in this study.

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3.3 Influence of various factors on the particulate backscattering ratio

Correlation coefficients (R) between the b˜bp(550) and factors including Chla, TSM, ISM, OSM, DA, ρa, and Chla/TSM, are calculated in this study. As shown in Table 4, the TSM shows a relatively high R value (0.516), with a level of significance (p < 0.001). As the inorganic part of the TSM, the ISM also exhibits a close correlation (R = 0.508, p < 0.001) with the b˜bp(550), since the TSM is mainly dominated by the ISM (the R between them can reach 0.984 with p < 0.001). The DA and Chla/TSM all show a significantly negative correlation with the b˜bp(550), and their corresponding R are −0.349 and −0.432 (p < 0.001), respectively. Note that the Chla and ρa all show very low correlations with the b˜bp(550), indicative of their potentially weak influence on the variability of the b˜bp(550) in this study area.

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Table 4. Correlations between Various Parameters with the Particulate Backscattering Ratio

To further quantitatively determine the influence of these factors on the particulate backscattering ratio, this study implemented the regression analysis. The obtained equations for b˜bp(550) vs. Chla, TSM, ISM, OSM, DA, ρa, and Chla/TSM are shown in Fig. 4. Many mathematical functions, such as linear, exponential, cubic quadratic, power, logarithmic, compound, inverse, and logistic functions, have been tested for these pairs of relationships in the present study. Note that the fitting performances by using the equations, shown in Fig. 4, outperform that of other forms.

 figure: Fig. 4

Fig. 4 Scatter plots of b˜bp(550) vs. (A) Chla, (B) TSM, (C) ISM, (D) OSM, (E) Chla/TSM, (F) ρa, and (G) DA.

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The formed relationships between b˜bp(550) vs. Chla and b˜bp(550) vs. ρa do not pass the significance test [Figs. 4(A) and 4(F)], and accordingly are excluded in the subsequent analysis on the influence of b˜bp(550) variability. Meanwhile, the fitted equations between b˜bp(550) with ISM and OSM are also removed, despite their close relationships, since the ISM and OSM represent parts of the TSM and their influences can be reflected in the formed relationship between b˜bp(550) with TSM. Therefore, the final determined influencing factors in this study are the TSM, Chla/TSM, and DA.

The largest degree (47.0%) for the b˜bp(550) variability can be ascribed to the TSM (particulate concentration), when 38.5% and 12.3 of the variability in b˜bp(550) can be accounted for by the Chla/TSM (particulate composition) and the DA (particulate size), respectively. Note that these three factors, i.e., TSM, Chla/TSM, and DA, cumulatively contribute to the overwhelming percentage (a total of ~98%) of the b˜bp(550) variability, while the remaining variability, with a much smaller proportion (approximately <4%), may be controlled by other features such as particulate density, structure, shapes, etc.

3.4 Modeling b˜bp(550) from TSM, Chla/TSM, and DA

According to the above findings, the particulate concentration (TSM), composition (Chla/TSM), and size (DA) are regarded as the main factors influencing the b˜bp(550) variability. By means of these factors, this study used a linear regression method with multivariate to model the b˜bp(550). Seventy-five in situ samples were selected randomly from 118 samples to calibrate the b˜bp(550) model, while the remaining 43 samples were used for model validation. Relatively high precision of fitting by the model calibration can be obtained [Fig. 5(A)], with a determination coefficient (R2) of 0.955 at a very high significance level (p<0.001). Meanwhile, the established b˜bp(550) model [Eq. (10)] also shows acceptable performances by using independent validation samples, with relatively low predictive errors, such as a MAPE of 14.0% [Fig. 5].

 figure: Fig. 5

Fig. 5 Calibration of the multivariate linear regression model by using the calibration samples (n = 75) and the validation of the model by using independent validation samples (n = 43). The solid red lines refer to the linear fit between measured and estimated values, and the pairs of two dotted red lines indicate the scope of ± RMSE, along the 1:1 lines.

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ln(b˜bp)=0.083ln(TSM)+0.208ln(Chla/TSM)1.121ln(DA)(R2=0.955,p<0.001,n=75)

4. Discussion

4.1 Essence of theb˜bp spectral dependence

The spectral dependence of the b˜bp essentially reflects the spectral variation in the capability of percentages of particulate scattering in the backward direction to the total particulate scattering. According to Mie scattering theory, the b˜bp should show a spectral consistency between different wavelengths for the ideal homogeneous and spherical particles, which have a constant refractive index and abide by a Junge law in particle size distribution [9]. Nevertheless, the suspended particles in natural waters do not usually show very ideal conditions in most cases. This induces the presence of two different views on the b˜bp spectral dependence based on those in situ observations, namely, wavelength-independent [7,8,32,33] and wavelength-dependent [34–37]. In our opinion, the two views are not ambivalent to each other, since the b˜bp spectral variability in nature depends on the intrinsic characteristics of the particulates (such as their size and composition [38],). The occurrence of the wavelength-independent b˜bp indicates a closer approach to the ideal assumption for the features of the suspended particles, whereas the wavelength-dependent cases possibly imply large deviations in the particulate features from ideal conditions that are assumed in Mie scattering theory.

Strictly speaking, the spectral dependence in the b˜bp exists in any natural waters, and simply exhibits different degrees in the spectral dependence between various water columns. For instance, Macdonald et al. (2000) [39] reported an ~10% variability of the b˜bp between wave bands that was roughly regarded as wavelength-independent. Similar variation scales were also reported in Whitmire et al. (2007) [7], which revealed no spectral dependence of the b˜bp. A maximum relative error of the b˜bp between five bands (i.e., 442, 488, 532, 589, and 676 nm) was reported to be approximately 14% in Zhang et al. (2010) [33]. Interestingly, Chami et al. (2005) [34] reported two existing cases in their observations, i.e., both low (within 4% for the average backscattering ratio) and high (~30%) spectral variability of the b˜bp, indicative of the potential inaccuracy by using a flat spectral shape of b˜bp in the investigated coastal zones. Meanwhile, a relatively significant spectral variability of the b˜bp has also been reported, especially in turbid inland and coastal waters [35,37,40].

In this study, the averaged b˜bp were observed to vary below 6%, between different wavelengths (550 nm as the reference here) [Fig. 2(B)], and the maximum variability reached up to 40% for several individual measurements. To quantitatively analyze the spectral variability of the b˜bp in waters, the current study proposes a new method of definition, i.e., the so-called “spectral dependence index (K)”. This index essentially reflects a general spectral variability normalized to a reference baseline, based on a suite of in situ observations. For the investigated water regions, the K values have been calculated, varying in a range from 0.94 - 0.97. In short, this dependence index provides an effective method to document the spectral variability of the b˜bp, which should be calculated in the future for a consistent comparison and record in various water areas.

4.2 Implications for the physical mechanism of the b˜bp changes

This study shows a relatively large variability in the observed b˜bp (using 550 nm as a delegate) in the BS, YS, and ECS, ranging from 0.0004 to 0.043, with a mean value of 0.015 ± 0.0082. This scope of change is comparable to those reported in the previous studies on open ocean and coastal waters all over the world [Fig. 6] [1,2,7,10,33,35,36]. The question remains as to what factors affect the b˜bp changes. This may still be difficult to answer, since many suspended particles’ physical and biogeochemical characteristics in natural waters are not yet accessible in synchronism.

 figure: Fig. 6

Fig. 6 Comparisons of the observed b˜bp variability between this study and previous studies all over the world.

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In this study, we utilized a ratio of Chla to TSM to denote the particulate composition, and found a significantly high inverse correlation (R = −0.432, p<0.001) with the b˜bp. This fact implies that low b˜bp values generally correspond to those particulate populations dominated by phytoplankton, whereas high values tend to appear in the waters with high inorganic particle content. This is consistent with those results presented in Loisel et al. (2007) [2], Neukermans et al. (2012) [4], Slade and Boss, (2015) [16], and Xi et al., (2015) [10] and indeed indicates an important contribution of the particulate composition to the b˜bp change. We found a distinct inverse correlation (R = −0.349, p<0.001) between DA and b˜bp, indicating that small size particles would lead to a higher b˜bp than large size particles. A similar rule was also elaborated in Loisel et al. (2007) [2] and Xi et al. (2015) [10]. Meanwhile, there existed a very weak relationship between Chla and b˜bp in our data (Fig. 4), which is in good agreement with those reported in previous studies [3,5,9,10,41,42]. These similar findings adequately indicate a weak contribution of the Chla absolute content to the b˜bp.

The bulk refractive index of particles is closely related to particulate composition, and typically, a high refractive index refers to a higher proportion of inorganic minerals in the composition of the particulate assemblage; whereas a low refractive index indicates the presence of more phytoplankton and organic materials [2,9,16]. As expected, this law of variation also appears in our investigated water areas (Fig. 7); that is, low Chla/TSM represents high inorganic particle content in the particulate assemblage and corresponds to high refraction, and then leads to a high backscattering ratio and vice versa. Therefore, the influence of the particulate refraction on the b˜bp is actually hidden in that of the particulate composition, which is not necessary for the redundant reanalysis in this study. Additionally, data on the particulate structure and shapes are not available to us, and their accurate impact on the b˜bp is beyond the scope of the current study.

 figure: Fig. 7

Fig. 7 A: b˜bp versus particle size distribution (PSD) slope, overlain by the n˜p contours (blue solid curves), as derived by Twardowski et al. (2001) model. Red and green solid circles denote different data points with the Chla/TSM < 0.3 and Chla/TSM ≥ 0.3, respectively. B: Statistical histogram of the Chla/TSM (10−3) collected in this study.

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In summary, this study exhibits similar findings to those in the previous studies, such as the similar effects from the particulate composition and sizes, and the weak contribution of Chla. However, it should be noted that the present study simultaneously finds a significant influence from TSM on the b˜bp. This implies that the increase of TSM shows a larger degree in augmenting the bbp than changing the bp in the water areas of the study. The reason is probably due to the high proportion of inorganic materials in the total particulate populations (R = 0.984 for ISM vs. TSM, p < 0.001, Table 3), which leads to a stronger backscattering capability. As in Loisel et al. (2007) [2], high b˜bp(λ) values are generally observed for a particle population dominated by inorganic particles.

4.3 Suggestions for bio-optical modeling

The particulate backscattering ratio essentially reflects a proportion of the particulate backscattering, accounting for its scattering; that is, the contribution of backscattering to scattering of particles. This ratio has been used in semianalytical algorithms for inherent the estimation of optical properties from radiometric measurements [3,11,12] and supports the derivation of an approximate scattering phase function of particles, serving for radiative transfer computations of water columns [13]. An accurate input of the backscattering ratio is thus of great importance to the bio-optical modeling of water bodies. This study comprehensively analyzes the influence of those particulate feature factors, including concentrations (Chla, TSM, OSM, and ISM), composition, size, density, and refraction on the backscattering ratio and then determines the potentially significant influencing factors. Unlike the backscattering coefficient that is determined to the first order by the particulate concentrations, the backscattering ratio exhibits more complex influences from multiple factors together. In this study, the particle composition and size are quantitatively analyzed to show important contributions to the change of the backscattering ratio, as well as the concentration. On this basis, we model the change of the backscattering ratio through those determined factors for the first time, with relatively acceptable predictive accuracies. A novel bridge is built to link the physical and biogeochemical characteristics of particles with optical parameters, which enriches the framework of bio-optical modeling. Even so, note that other factors, such as particle shape, internal structure, etc., might also have important influence on the particulate backscattering ratio. More comprehensive data on the particle features is expected in future to participate in the research on the nature of its backscattering ratio. Indeed, potential discrepancies in the driving factors of the backscattering ratio may appear between different water regions and thus, more investigations, together with multiple physical and biogeochemical factors, should be carried out in the future for a much deeper understanding of the change of the backscattering ratio. This is undoubtedly of vital importance to the field of marine optics.

5. Conclusions

The present study mainly obtains the following findings: 1) the spectral dependence ofb˜ bp in the investigated water areas, also thought to exist in other natural waters, with more or less degrees of dependence, is quantitatively determined by our proposed spectral dependence index (K, approximately 0.94 - 0.97 for the visible light range), which is recommended as a standard method; 2) TSM accounts for the largest degree (47.0%) of the b˜bp variability, where 38.5% and 12.3 of its variability can be attributed to Chla/TSM and DA, respectively. The above three factors cumulatively contribute most (97.8%) of the b˜bp variability, whereas others, such as the ρa, show weak influence; 3) b˜bp can be effectively modeled with TSM, Chla/TSM, and DA, through a multivariate regression method, which produces a relatively high precision of fitting (R2 = 0.955, p<0.001) and acceptable predictive errors (MAPE = 14%). Our findings here go deep into the nature of particulate backscattering ratios and serve as a template for the understanding and parameterizing of its variations for other water regions, where further investigation is needed.

Funding

National Key Research and Development Program of China (2016YFC1400904, 2016YFC1400901); National Natural Science Foundation of China (41876203, 41576172); Jiangsu Six Talent Summit Project (JY-084); Jiangsu Provincial Programs for Marine Science and Technology Innovation (HY2017-5); State Key Laboratory of Satellite Ocean Environment Dynamics, Second Institute of Oceanography (QNHX1812); the Qing Lan Project; and NSFC Open Research Cruise (NORC 2018-01), funded by Ship-time Sharing Project of NSFC.

Acknowledgments

We acknowledge captains, officers, and crews of R/V Dongfanghong 2 and Science 3 for providing excellent assistance during field sampling and measurements.

References

1. E. Boss, W. S. Pegau, M. Lee, M. Twardowski, E. Shybanov, G. Korotaev, and F. Baratange, “Particulate backscattering ratio at LEO 15 and its use to study particle composition and distribution,” J. Geophys. Res. Oceans109 (2004). [CrossRef]  

2. H. Loisel, X. Mériaux, J. F. Berthon, and A. Poteau, “Investigation of the optical backscattering to scattering ratio of marine particles in relation to their biogeochemical composition in the eastern English Channel and southern North Sea,” Limnol. Oceanogr. 52(2), 739–752 (2007). [CrossRef]  

3. A. Morel and S. Maritorena, “Bio-optical properties of oceanic waters: a reappraisal,” J. Geophys. Res. Oceans 106(C4), 7163–7180 (2001). [CrossRef]  

4. G. Neukermans, H. Loisel, X. Mériaux, R. Astoreca, and D. Mckee, “In situ variability of mass-specific beam ttenuation and backscattering of marine particles with respect to article size, density, and composition,” Limnol. Oceanogr. 57(1), 124–144 (2012). [CrossRef]  

5. M. S. Twardowski, E. Boss, J. B. Macdonald, W. S. Pegau, A. H. Barnard, and J. R. V. Zaneveld, “A model for estimating bulk refractive index from the optical backscattering ratio and the implications for understanding particle composition in case I and case II waters,” J. Geophys. Res. D Atmospheres 106(C7), 14129–14142 (2001). [CrossRef]  

6. M. Twardowski, H. Claustre, S. Freeman, D. Stramski, and Y. Huot, “Optical backscattering properties of the clearest natural waters,” Biogeosciences Discuss. 4(4), 2441–2491 (2007). [CrossRef]  

7. A. L. Whitmire, E. Boss, T. J. Cowles, and W. S. Pegau, “Spectral variability of the particulate backscattering ratio,” Opt. Express 15(11), 7019–7031 (2007). [CrossRef]   [PubMed]  

8. D. Risović, “Effect of suspended particulate-size distribution on the backscattering ratio in the remote sensing of seawater,” Appl. Opt. 41(33), 7092–7101 (2002). [CrossRef]   [PubMed]  

9. O. Ulloa, S. Sathyendranath, and T. Platt, “Effect of the particle-size distribution on the backscattering ratio in seawater,” Appl. Opt. 33(30), 7070–7077 (1994). [CrossRef]   [PubMed]  

10. H. Xi, P. Larouche, C. Michel, and S. Tang, “Beam attenuation, scattering and backscattering of marine particles in relation to particle size distribution and composition in Hudson Bay (Canada),” J. Geophys. Res. Oceans 120(5), 3286–3300 (2015). [CrossRef]  

11. H. R. Gordon, O. B. Brown, R. H. Evans, J. W. Brown, R. C. Smith, K. S. Baker, and D. K. Clark, “A semianalytic radiance model of ocean color,” J. Geophys. Res. D Atmospheres 93(D9), 10909–10924 (1988). [CrossRef]  

12. B. Lubac and H. Loisel, “Variability and classification of remote sensing reflectance spectra in the eastern English Channel and southern North Sea,” Remote Sens. Environ. 110(1), 45–58 (2007). [CrossRef]  

13. C. D. Mobley, L. K. Sundman, and E. Boss, “Phase function effects on oceanic light fields,” Appl. Opt. 41(6), 1035–1050 (2002). [CrossRef]   [PubMed]  

14. S. Sathyendranath and T. Platt, “The spectral irradiance field at the surface and in the interior of the ocean: a model for applications in oceanography and remote sensing,” J. Geophys. Res. Oceans 93(C8), 9270–9280 (1988). [CrossRef]  

15. A. Morel, “Optical modeling of the upper ocean in relation to its biogenous matter content (case I waters),” J. Geophys. Res. Oceans 93(C9), 10749–10768 (1988). [CrossRef]  

16. W. H. Slade and E. Boss, “Spectral attenuation and backscattering as indicators of average particle size,” Appl. Opt. 54(24), 7264–7277 (2015). [CrossRef]   [PubMed]  

17. M. Babin, A. Morel, V. Fournier-Sicre, F. Fell, and D. Stramski, “Light Scattering Properties of Marine Particles in Coastal and Open Ocean Waters as Related to the Particle Mass Concentration,” Limnol. Oceanogr. 48(2), 843–859 (2003). [CrossRef]  

18. D. G. Bowers, K. M. Braithwaite, W. A. M. Nimmo-Smith, and G. W. Graham, “Light scattering by particles suspended in the sea: The role of particle size and density,” Cont. Shelf Res. 29(14), 1748–1755 (2009). [CrossRef]  

19. D. G. Bowers, P. S. Hill, and K. M. Braithwaite, “The effect of particulate organic content on the remote sensing of marine suspended sediments,” Remote Sens. Environ. 144, 172–178 (2014). [CrossRef]  

20. E. N. Flory, P. S. Hill, T. G. Milligan, and J. Grant, “The relationship between floc area and backscatter during a spring phytoplankton bloom,” Deep Sea Res. Part I Oceanogr. Res. Pap. 51(2), 213–223 (2004). [CrossRef]  

21. J. T. O. Kirk, Light and photosynthesis in aquatic ecosystems, 2nd ed. (Cambridge: Cambridge University Press), 509 (1994).

22. H. Wei, J. Sun, A. Moll, and L. Zhao, “Phytoplankton dynamics in the Bohai Sea—observations and modelling,” J. Mar. Syst. 44(3-4), 233–251 (2004). [CrossRef]  

23. Y. He, X. Lu, Z. Qiu, and J. Zhao, “Shallow water tidal constituents in the Bohai Sea and the Yellow Sea from a numerical adjoint model with TOPEX/POSEIDON altimeter data,” Cont. Shelf Res. 24(13-14), 1521–1529 (2004). [CrossRef]  

24. C. Bian, W. Jiang, Q. Quan, T. Wang, R. J. Greatbatch, and W. Li, “Distributions of suspended sediment concentration in the Yellow Sea and the East China Sea based on field surveys during the four seasons of 2011,” J. Mar. Syst. 121–122, 24–35 (2013). [CrossRef]  

25. H. Zhang, S. Wang, Z. Qiu, D. Sun, J. Ishizaka, S. Sun, and Y. He, “Phytoplankton size class in the East China Sea derived from MODIS satellite data,” Biogeosciences 15(13), 4271–4289 (2018). [CrossRef]  

26. X. Gao and J. Song, “Phytoplankton distributions and their relationship with the environment in the Changjiang Estuary, China,” Mar. Pollut. Bull. 50(3), 327–335 (2005). [CrossRef]   [PubMed]  

27. L. Qiao, L. Huang, Z. Wang, Z. Yao, and S. Liu, “Flux and its seasonal variation of suspended particulate matter in the Bohai Sea, Yellow Sea and East China Sea,” Geol. J. 51, 22–34 (2016). [CrossRef]  

28. R. A. Maffione and D. R. Dana, “Instruments and methods for measuring the backward-scattering coefficient of ocean waters,” Appl. Opt. 36(24), 6057–6067 (1997). [CrossRef]   [PubMed]  

29. J. M. Sullivan, M. S. Twardowski, J. R. Zaneveld, C. M. Moore, A. H. Barnard, P. L. Donaghay, and B. Rhoades, “Hyperspectral temperature and salt dependencies of absorption by water and heavy water in the 400-750 nm spectral range,” Appl. Opt. 45(21), 5294–5309 (2006). [CrossRef]   [PubMed]  

30. D. Sun, S. Chen, Z. Qiu, S. Wang, Y. Huan, Y. He, and T. Zhang, “Second‐order variability of inherent optical properties of particles in Bohai Sea and Yellow Sea: Driving factor analysis and modeling,” Limnol. Oceanogr. 62(3), 1266–1287 (2017). [CrossRef]  

31. L. Van Heukelem and C. S. Thomas, “Computer-assisted high-performance liquid chromatography method development with applications to the isolation and analysis of phytoplankton pigments,” J. Chromatogr. A 910(1), 31–49 (2001). [CrossRef]   [PubMed]  

32. Y. Huot, A. Morel, M. Twardowski, D. Stramski, and R. Reynolds, “Particle optical backscattering along a chlorophyll gradient in the upper layer of the eastern South Pacific Ocean,” Biogeosciences Discuss. 4(6), 4571–4604 (2007). [CrossRef]  

33. M. Zhang, J. Tang, Q. Song, and Q. Dong, “Backscattering ratio variation and its implications for studying particle composition: A case study in Yellow and East China seas,” J. Geophys. Res. Oceans115 (2010). [CrossRef]  

34. M. Chami, E. B. Shybanov, T. Y. Churilova, G. A. Khomenko, M. E.-G. Lee, O. V. Martynov, G. A. Berseneva, and G. K. Korotaev, “Optical properties of the particles in the Crimea coastal water (Black Sea),” J. Geophys. Res. Oceans110 (2005).

35. D. McKee and A. Cunningham, “Identification and characterisation of two optical water types in the Irish Sea from in situ inherent optical properties and seawater constituents,” Estuar. Coast. Shelf Sci. 68(1-2), 305–316 (2006). [CrossRef]  

36. W. A. Snyder, R. A. Arnone, C. O. Davis, W. Goode, R. W. Gould, S. Ladner, G. Lamela, W. J. Rhea, R. Stavn, M. Sydor, and A. Weidemann, “Optical scattering and backscattering by organic and inorganic particulates in U.S. coastal waters,” Appl. Opt. 47(5), 666–677 (2008). [CrossRef]   [PubMed]  

37. D. Sun, Y. Li, Q. Wang, J. Gao, H. Lv, C. Le, and C. Huang, “Light scattering properties and their relation to the biogeochemical composition of turbid productive waters: a case study of Lake Taihu,” Appl. Opt. 48(11), 1979–1989 (2009). [CrossRef]   [PubMed]  

38. A. Morel and A. Bricaud, “Theoretical results concerning light absorption in a discrete medium, and application to specific absorption of phytoplankton,” Deep-Sea Res. A, Oceanogr. Res. Pap. 28(11), 1375–1393 (1981). [CrossRef]  

39. J. Macdonald, M. Twardowski, W. Pegau, A. Barnard, E. Boss, and J. Zaneveld, “Characterization of spectral backscattering in the Gulf of California,” Eos (Wash. D.C.) 80, 49 (2000).

40. D. McKee, M. Chami, I. Brown, V. S. Calzado, D. Doxaran, and A. Cunningham, “Role of measurement uncertainties in observed variability in the spectral backscattering ratio: a case study in mineral-rich coastal waters,” Appl. Opt. 48(24), 4663–4675 (2009). [CrossRef]   [PubMed]  

41. J. M. Sullivan, M. S. Twardowski, P. L. Donaghay, and S. A. Freeman, “Use of optical scattering to discriminate particle types in coastal waters,” Appl. Opt. 44(9), 1667–1680 (2005). [CrossRef]   [PubMed]  

42. A. L. Whitmire, E. Boss, T. J. Cowles, and W. S. Pegau, “Spectral variability of the particulate backscattering ratio,” Opt. Express 15(11), 7019–7031 (2007). [CrossRef]   [PubMed]  

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Figures (7)

Fig. 1
Fig. 1 Study areas in the BS, YS, and ECS, overlaid by those stations during two cruises that are carried out in Sep. and Dec. 2016, respectively. Bathymetric contours are color coded.
Fig. 2
Fig. 2 Spectra of particulate backscattering ratios, depicted by the in situ data sets collected in this study.
Fig. 3
Fig. 3 Statistical linear relationships between the particulate backscattering ratios at wavelengths including 442 nm (A), 488 nm (B), 620 nm (C), and 700 nm (D), with that at the 550 nm reference. These regressions were produced by using 118 in situ samples, observed by the HS-6 instrument. Panel E refers to the spectral dependence index, K, defined in this study.
Fig. 4
Fig. 4 Scatter plots of b ˜ bp(550) vs. (A) Chla, (B) TSM, (C) ISM, (D) OSM, (E) Chla/TSM, (F) ρa, and (G) DA.
Fig. 5
Fig. 5 Calibration of the multivariate linear regression model by using the calibration samples (n = 75) and the validation of the model by using independent validation samples (n = 43). The solid red lines refer to the linear fit between measured and estimated values, and the pairs of two dotted red lines indicate the scope of ± RMSE, along the 1:1 lines.
Fig. 6
Fig. 6 Comparisons of the observed b ˜ bp variability between this study and previous studies all over the world.
Fig. 7
Fig. 7 A: b ˜ bp versus particle size distribution (PSD) slope, overlain by the n ˜ p contours (blue solid curves), as derived by Twardowski et al. (2001) model. Red and green solid circles denote different data points with the Chla/TSM < 0.3 and Chla/TSM ≥ 0.3, respectively. B: Statistical histogram of the Chla/TSM (10−3) collected in this study.

Tables (4)

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Table 1 Symbols and Units for the Parameters Used in This Study

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Table 2 Description of the Two Cruise Surveys in This Study

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Table 3 Statistical Distribution of Those Water Bio-Optical Parameters

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Table 4 Correlations between Various Parameters with the Particulate Backscattering Ratio

Equations (10)

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b ˜ b p = 0 Q b b e x 2 f ( x ) d x 0 Q b e x 2 f ( x ) d x
N ( D i ) = 6 V ( D i ) / π D i 3
[ A C ] i = 3 2 D i V ( D i )
D A = i = 2 31 [ A C ] i D i [ A C ] t
ρ a = T S M V ( D t )
M A P E = 1 n i = 1 n | x i y i x i | ( 1 00 % )
R M S E = 1 n i = 1 n ( x i y i ) 2
N R M S = s t d e v ( | x i y i x i | )
m e a n r a t i o = 1 n i = 1 n ( x i y i )
ln ( b ˜ b p ) = 0.083 ln ( T S M ) + 0.208 ln ( C h l a / T S M ) 1.121 ln ( D A ) ( R 2 = 0.955 , p < 0.001 , n = 75 )
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