<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">ARS</journal-id><journal-title-group><journal-title>Advances in Remote Sensing</journal-title></journal-title-group><issn pub-type="epub">2169-267X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ars.2013.22007</article-id><article-id pub-id-type="publisher-id">ARS-32664</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Computer Science&amp;Communications</subject></subj-group></article-categories><title-group><article-title>
 
 
  Spectral Models for Improving Atmospheric Correction Results in Complex Oceanic Waters around India
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>alanisamy</surname><given-names>Shanmugam</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Muniyandi</surname><given-names>Tholkapiyan</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Ocean Engineering, Indian Institute of Technology Madras, Chennai, India</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>pshanmugam@iitm.ac.in(AS)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>05</day><month>06</month><year>2013</year></pub-date><volume>02</volume><issue>02</issue><fpage>51</fpage><lpage>57</lpage><history><date date-type="received"><day>February</day>	<month>17,</month>	<year>2013</year></date><date date-type="rev-recd"><day>March</day>	<month>20,</month>	<year>2013</year>	</date><date date-type="accepted"><day>March</day>	<month>27,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   Atmospheric correction over turbid and productive waters continues to be problematic and often results in excessive errors in retrieved water-leaving radiance and bio-geo-physical products. This may be likely due to overestimation of L<sub>a</sub> + L<sub>ra</sub> (atmospheric signal due to aerosol and Rayleigh scattering) in the visible and thus reduction in L<sub>w</sub> which appears as an elevated pigment concentration. Spectral models for reconstructing the atmospherically distorted data are developed and their results are thoroughly validated with in-situ data from a wide range of waters. Good agreement was found between the retrieved products and in-situ data. Our results indicate that the new spectral models have the potential to improve the accuracy of ocean colour retrievals in optically complex waters, and can become an important part of the processing of data from ocean colour sensors (e.g., Ocean colour monitor OCM2) with only two near-infrared bands (i.e., 765 and 865 nm).
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</p></abstract><kwd-group><kwd>Ocean Colour; Spectral Models; MODIS-Aqua; Algal Blooms; Arabian Sea; India</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Ocean colour instruments measure the spectrum of sunlight reflected from the ocean-atmosphere system at several visible and near-infrared (NIR) wavebands. The major portion of these signals is from the contribution of scattering by molecules and particles (aerosols) in the atmosphere (~80% - 90%). The process of removing the atmospherically scattered signal in order to retrieve the ocean colour signal (i.e., water-leaving radiance L<sub>w</sub>) is referred to as atmospheric correction [<xref ref-type="bibr" rid="scirp.32664-ref1">1</xref>]. The current SeaDAS atmospheric correction (“SAC” for brevity) algorithm for producing the global ocean colour products from SeaWiFS and MODIS uses the algorithm of Gordon and Wang [<xref ref-type="bibr" rid="scirp.32664-ref2">2</xref>]. It specifically uses two near infrared (NIR) bands centered at MODIS 748 and 869 nm (SeaWiFS 765 and 865 nm) to determine aerosol type and estimate the atmospheric effects in the visible by extrapolating the aerosol effect from the NIR into visible bands. Though the basic assumption of negligible waterleaving radiance (L<sub>w</sub>) in the NIR for deriving aerosol properties was replaced by Stumpf et al. [<xref ref-type="bibr" rid="scirp.32664-ref3">3</xref>] and then updated by Bailey et al. [<xref ref-type="bibr" rid="scirp.32664-ref4">4</xref>], the SAC algorithm still produces low or negatively biased L<sub>w</sub> at short wavelengths in areas with absorbing aerosols or high biomass concentrations or sediment levels typical of productive coastal regions.</p><p>The principal difficulty in these waters is: 1) the adequacy of aerosol models is presently difficult to judge. This holds true for mineral dust aerosols (from deserts) because their absorption can seriously reduce L<sub>a</sub> + L<sub>ra</sub> (atmospheric signal due to aerosol and Rayleigh scattering) in the visible and their vertical distribution profoundly influences the TOA radiance in the visible (especially in the blue) [1,5]. Moreover, the absorption properties are very difficult to determine on the basis of the observations of L<sub>a</sub> + L<sub>ra</sub> in the NIR which means that in-situ measurements in the visible are required for correction. However, in the visible (especially blue) L<sub>w</sub> can be significant, and cannot be estimated a priori [<xref ref-type="bibr" rid="scirp.32664-ref1">1</xref>]. 2) The errors involved in extrapolating aerosol reflectance to visible bands are considerably higher and this may require a more realistic method [<xref ref-type="bibr" rid="scirp.32664-ref6">6</xref>]. 3) Assumption of negligible water-leaving radiance in the NIR is not valid in optically complex waters, as high sediment loads and phytoplankton will contribute NIR radiance [6-8]. 4) Although modifications to point 3 (i.e., “non-zero L<sub>w</sub> in the NIR” based on in-water models and spatial homogeneity assumption) [6,9] show noticeable improvements in turbid waters, the problems are still encountered in highly bloomed waters and could be attributed to the inadequacy of aerosol models and inadequate/inappropriate in-water models. Thus, an accurate retrieval of ocean colour has become a prolonging issue and requires an alternate and robust solution.</p><p>In this study, spectral models are developed to improve the results of atmospheric correction with standard methods and their results are validated with in-situ data sets. Preliminary results are also presented for a case study using MODIS-Aqua data over highly turbid and productive waters in the Arabian Sea.</p></sec><sec id="s2"><title>2. Data and Methods</title><sec id="s2_1"><title>2.1. In-Situ Data</title><p>In-situ data radiometric data at key wavelengths and pigment (Chlorophyll) concentrations for different regions were obtained from the NASA bio-Optical Marine Algorithm Data set (NOMAD) [<xref ref-type="bibr" rid="scirp.32664-ref10">10</xref>]. These data are global, high quality bio-optical datasets collected over a wide range of optical properties, trophic status, and geographical locations in open ocean waters, estuaries, and coastal waters. Despite the NOMAD data encompass large samples, only few cruises data (between 2003 and 2007) were considered because satellite sampling for a given station was masked by clouds or affected by sensor digitization problems.</p></sec><sec id="s2_2"><title>2.2. Satellite Data</title><p>MODIS-Aqua Level 1A data data were obtained from the US NASA GSFC (Goddard Space Flight Center), and processed using SeaDAS5 to generate Level 2 data (water-leaving radiance L<sub>w</sub>). Many of these data were collected coincidently with the above field data and few were acquired in highly bloomed waters of the Arabian Sea. For the reason that L<sub>w</sub> data at the short wavelengths are profoundly deteriorated by the SAC algorithm, all Level 2 L<sub>w</sub> data were reprocessed based on the new spectral models and then converted to remote sensing reflectance (R<sub>rs</sub> (l)) using the standard procedures available with SeaDAS. In theory, the spectral models developed in this study can be applied to the entire global ocean colour dataset. In practice, however, due to large volume of MODIS data, a few coastal and offshore regions were selected to demonstrate their accuracy and reliability.</p></sec></sec><sec id="s3"><title>3. Spectral Models</title><p>To avoid known problems with atmospheric correction at the short wavelengths (note the inaccuracy of the atmospheric correction grows for decreasing wavelengths so that the 412 nm waveband is the most affected one [<xref ref-type="bibr" rid="scirp.32664-ref11">11</xref>], a correction is carried out in two steps based on the definition of water into two types: relatively clear waters (Chl &lt; 0.5 mg/m<sup>3</sup>) and optically complex waters (bloom, plume and coloured waters where Chl &gt; 0.5 mg/m<sup>3</sup> and negative L<sub>w</sub> (412) as produced by the SAC algorithm). Accordingly, two separate sets of spectral models are developed considering the fact that the water-leaving radiance for clear waters is weakly variable with a smooth decrease towards the shorter wavelengths (412 nm) with increasing pigment concentration which is in contrast with that for optically complex waters. These models take into account a change (distortion) in spectral shape characteristics in the blue wavelengths (412 and 443 nm) for estimating the atmospheric correction distortion and reconstructing the L<sub>w</sub> spectra in the visible domain (412 - 555 nm). For optically complex waters (Chl &gt; 0.5 mg/m<sup>3</sup>; negative L<sub>w</sub> (412)), the spectral models rely on the normalized spectral difference between L<sub>w</sub> (412) and L<sub>w</sub> (443) multiplied by its wavelength ratio factor which is then added with measurements at each wavelength, as shown in Equation (1), where<img src="2-2630021\9afc9fb1-8d7b-4ba2-8dae-b5cc5124a993.jpg" />, <img src="2-2630021\3fa25624-70a7-47b9-853a-8b388573973d.jpg" />and<img src="2-2630021\5befb698-8456-4fef-b361-390b187124d2.jpg" />. To compensate for a maximum distortion at 412 nm and ensure spectral continuity, the normalized spectral values (sum) of L<sub>w</sub> (412) and L<sub>w</sub> (443) and coefficient <img src="2-2630021\67f03c78-f31f-44be-a25f-9f7d4bf3a353.jpg" /> are used in the above equations. These models ensure a maximal shift in L<sub>w</sub> (toward positive) when its distortion is elevated and a minimal shift in L<sub>w</sub> when it is undistorted.</p><disp-formula id="scirp.32664-formula56364"><label>(1)</label><graphic position="anchor" xlink:href="2-2630021\dc14f280-0a59-4c1f-b437-8dde9b2761d4.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.32664-formula56365"><label>(2)</label><graphic position="anchor" xlink:href="2-2630021\d1837021-14fa-4cf6-92f4-ba98b260483b.jpg"  xlink:type="simple"/></disp-formula><p>For relatively clear waters (Chl &lt; 0.5 mg/m<sup>3</sup>), a correction is achieved based on a set of spectral models (one for each band) to obtain the best spectral shape of L<sub>w</sub> (412 - 551 nm). These models that readjust the spectral shape of the L<sub>w</sub> from the SAC algorithm are defined in Equation (2).</p><p>The newly derived water-leaving radiance values will be helpful to reduce errors in bio-geochemical products such as chlorophyll concentration in optically complex waters (<xref ref-type="fig" rid="fig1">Figure 1</xref>). For example, the OC3 algorithm [<xref ref-type="bibr" rid="scirp.32664-ref12">12</xref>] estimates Chl a from a cubic polynomial formulation by using the maximum band ratio determined as the greater of the <img src="2-2630021\7ac70c56-4323-45b7-aa11-f98a630731e8.jpg" /> or<img src="2-2630021\d8148c96-1ced-4097-a8c3-503fc44a2ac3.jpg" />. It is then feasible to obtain error in the atmospheric correction and in the retrievals of pigment concentrations in both clear and optically complex waters.</p></sec><sec id="s4"><title>4. Results</title><p>The comparison between original (SAC) and reconstructed R<sub>rs</sub> (spectral models) is shown in <xref ref-type="fig" rid="fig2">Figure 2</xref> for</p><p>bloomed and turbid waters in the Arabian Sea, using several MODIS-Aqua data collected during the year 2007. It reveals dramatic anomalous differences between these two spectra, i.e., R<sub>rs</sub> produced by the SAC algorithm are significantly biased low and negative at short wavelengths (412 and 443 nm) and this resulted in a large distortion of the radiance structures across the visible spectrum (left). In particular, most of the distorted spectra were observed in bloomed waters. The effect of the spectral models on raising radiance values particularly at 412 and 443 is clearly seen in <xref ref-type="fig" rid="fig2">Figure 2</xref> (right). The physically realistic shape of R<sub>rs</sub>(l) is also typical for waters with phytoplankton blooms in the Arabian Sea [<xref ref-type="bibr" rid="scirp.32664-ref13">13</xref>].</p><p>Because the quality of the atmospheric correction affects the quality of the R<sub>rs</sub>(l) which is key to the estimation of pigments and other geophysical products, satellite-derived remote sensing reflectances were compared with those from the in-situ measurements in both clear and optically complex waters. <xref ref-type="fig" rid="fig3">Figure 3</xref> shows comparisons between the original (SAC) R<sub>rs</sub>(l) and reconstructed R<sub>rs</sub>(l) and in-situ R<sub>rs</sub>(l) at the selected five wavelengths. Although there is no remarkable difference, the results in these plots show a reasonably good matchup between reconstructed and in-situ reflectance measurements. Most of the corrected R<sub>rs</sub>(l) values are aligned closer to the 1:1 line as compared with those from the SAC algorithm. To gain further insight into the differences between the satellite R<sub>rs</sub>(l) and in-situ R<sub>rs</sub>(l), the mean relative error (MRE), root means square error (RMSE), slope (S), intercept (I), correlation coefficient (R<sup>2</sup>) and bias were calculated using the standard statistical procedures and the results are summarized in Tables 1(a) and (b). Notably, these statistics are better for the reconstructed R<sub>rs</sub>(l) than for the SAC algorithm (see relatively lower MRE, RMSE and I, higher S and R<sup>2</sup>, and almost same biases). This clearly indicates significant improvements over the SAC algorithm.</p><p>The effect of atmospheric correction errors on pigment retrievals was also assessed using the OC3 algorithm as applied to both the original R<sub>rs</sub>(l) and reconstructed R<sub>rs</sub>(l) (Figures 4(a) and (b)). As noted earlier, the uncorrected R<sub>rs</sub>(l) showed noticeable overestimations in Chl with</p><p>respect to in situ measurements in bloomed/coastal waters [<xref ref-type="bibr" rid="scirp.32664-ref13">13</xref>], although producing Chl consistent with the in-situ data in clear waters.</p><p>By contrast, the validation matchups between in-situ Chl and satellite Chl from the reconstructed R<sub>rs</sub>(l) are very excellent and demonstrate good agreement in both clear and optically complex waters (lower MRE, RMSE, I and bias, and higher S and R<sup>2</sup>). The averaged minimum, mean and maximum Chl values for this case are also in good agreement with in-situ data (<xref ref-type="table" rid="table1">Table 1</xref>(b)), with its mean value being 1.65 times lower than that produced by the former case.</p><p>Shown in Figures 4(c) and (d) are two hypothetical cases from the bloom water (c) and clear water (d). It should be noted that when Chl &gt; 5 mg/m<sup>3</sup>, the situation is even worse (also see <xref ref-type="fig" rid="fig4">Figure 4</xref>(b)) and an excessive overcorrection is often inevitable with the SAC algorithm because of its excessive aerosol correction. This overcorrection or reduction in L<sub>w</sub> eventually appears as an elevated pigment concentrations as observed in Figures</p><p>4(a) and (b). On the contrary, the spectral models have potential to not only improve L<sub>w</sub> retrievals (thus constituents’ concentrations) in optically complex waters but also reliably reproduce these spectra in clear waters.</p><p>Optically complex waters are consistently turbid due to the presence of suspended sediments and algal blooms and have large NIR water-leaving radiances. The enhanced water signal interferes with the SAC algorithm to produce unacceptable errors in retrieved water-leaving radiance and pigment concentrations. This leaves only two chaises for users who need to derive variables such as seasonal mean concentrations or annual primary production: either (1) to completely discord the spectrally distorted L<sub>w</sub> data or (2) to use them as is, in error. In either case the results will be biased. Our spectral models reduce errors in estimated water-leaving radiance for both optically complex and clear waters. The number of negative water-leaving radiance pixels drops significantly. Furthermore, data from many coastal areas with quality masks due to atmospheric correction failure can be recovered. Consequently, the spatial patterns in the masked areas, even if the accuracy in the estimated waterleaving radiance or pigment concentrations is doubtful, can be derived. The improvement in the water-leaving radiance data will be helpful to improve the accuracy bio-geo-physical products. This scheme is easy to use for any operational processing of the satellite ocean colour data on daily basis.</p></sec><sec id="s5"><title>5. Conclusion</title><p>In conclusion, the new models show promise in reconstructing the spectrally distorted water-leaving radiance in both clear and optically complex waters. The spectral shape/form produced by these models is found to be better consistent with in-situ measurements in the visible</p><table-wrap-group id="1"><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> (a) and (b) Comparison of algorithm performances using in-situ data sets (e.g., remote sensing reflectance R<sub>rs</sub> (sr<sup>−1</sup>) and Chlorophyll concentration (mg/m<sup>3</sup>))</title></caption></table-wrap-group><p>domain (412 - 555 nm) that allows more accurate estimations of constituents’ concentrations. The minimal errors of the satellite validation matchups imply that these spectral models can be used to improve the various biogeophysical products desired for coastal oceanic waters. Though the spectral models have been described for MODIS/SeaWiFS imagery, it can be applied rather generally to other satellite-based and probably also airborne ocean colour sensors (with only two near-infrared bands (i.e., 765 and 865 nm) and no shortwave bands). The directions for further research include a more detailed validation of these models with large in-situ data sets from highly turbid and productive waters, and an attempt to tune it to have a wider applicability. The effect of absorbing aerosols on the retrieved water-leaving radiance will be assessed and further refinements of the models will be anticipated.</p></sec><sec id="s6"><title>6. Acknowledgements</title><p>This work was supported by the ISRO-IITM cell project (ICSR/ISRO-IITMJPC34/2009). The author gratefully acknowledges the NASA Ocean Biology Processing Group for making available the global, high quality in situ bio-optical (NOMAD) dataset as well as the global coverage MODIS-Aqua data to this study.</p></sec><sec id="s7"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.32664-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">H. R. Gordon, “Atmospheric Correction of Ocean Colour Imagery in the Earth Observing System Era,” Journal of Geophysical Research, Vol. 102, No. D14, 1997, pp. 17081-17106. doi:10.1029/96JD02443</mixed-citation></ref><ref id="scirp.32664-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">H. R. Gordon and M. Wang, “Retrieval of Water-Leaving Radiance, Aerosol Optical Thickness over the Oceans with SeaWiFS: A Preliminary Algorithm,” Applied Optics, Vol. 33, No. 3, 1994, pp. 443-452.  
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