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Vertically- resolved phytoplankton carbon and net primary production from a high spectral resolution lidar

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Abstract

Passive ocean observing sensors are unable to detect subsurface structure in ocean properties, resulting in errors in water column integrated phytoplankton biomass and net primary production (NPP) estimates. Active lidar (light detection and ranging) sensors make quantitative measurements of depth-resolved backscatter (bbp) and diffuse light attenuation (Kd) coefficients in the ocean and can provide critical measurements for biogeochemical models. Sub-surface phytoplankton biomass, light, chlorophyll, and NPP fields were characterized using both in situ measurements and coincident airborne high spectral resolution lidar (HSRL-1) measurements collected as part of the SABOR (Ship-Aircraft Bio-Optical Research) field campaign. We found that depth-resolved data are critical for calculating phytoplankton stocks and NPP, with improvements in NPP estimates up to 54%. We observed strong correlations between coincident HSRL-1 and in situ IOP measurements of both bbp (r = 0.94) and Kd (r = 0.90).

© 2017 Optical Society of America

1. Introduction

It has been widely recognized since the Coastal Zone Color Scanner (CZCS) era that the inability of passive ocean color measurements to resolve phytoplankton vertical structure can be a primary source of error in global phytoplankton biomass and net primary production (NPP) estimates [1,2]. Stramska and Stramski (2005) [3] used HydroLight to model the effects of non-uniform chlorophyll distributions on remote-sensing reflectance (RRS) and found sub-surface chlorophyll maxima could result in relative errors in chlorophyll (calculated as an RRS ratio) of up to 70% under oligotrophic conditions. Platt and Sathyendranath (1988) [4] evaluated the impact of vertical structure in chlorophyll on integrated NPP measurements and found that errors in NPP were considerably larger when the chlorophyll feature was located in the upper water column. Here we use data collected during the 2104 NASA SABOR (Ship-Aircraft Bio-Optical Research) campaign to evaluate the utility of lidar (light detection and ranging) measurements for characterizing vertical variability in plankton and optical properties. Active lidar sensors make quantitative measurements of depth-resolved backscatter (bbp) and diffuse light attenuation (Kd) coefficients in the ocean [5–9] and can provide critical measurements for biogeochemical models.

The SABOR campaign was conducted in the western North Atlantic with the goal of advancing key technologies for plankton characterizations from space. We evaluated sub-surface phytoplankton biomass, light, and chlorophyll fields using both high spectral resolution lidar (HSRL-1) and coincident in-water IOP (inherent optical property) measurements. These data were then employed as inputs to the carbon-based production model (CbPM) [10,11] to calculate vertically resolved NPP. SABOR sampling stations covered continental shelf, slope, and offshore waters and provided a large dynamic range in bio-optical states. Previous work has found that NPP in this region is seasonally variable and often exhibits strong water column stratification and subsurface chlorophyll and production features that persist through the summer season [12,13].

We show that depth-resolved measurements of ocean properties are critical for calculating biomass and NPP in the upper ocean and enable up to 54% more accurate estimates of NPP compared to calculations made without information on the vertical structure. We also show that phytoplankton biomass features of a given magnitude have a significantly larger impact on NPP estimates if they are located in the top two optical depths of the water column compared to deeper features. This critical upper layer can be effectively characterized by either an airborne or satellite ocean-optimized lidar.

2. Methods

The SABOR campaign was conducted onboard the R/V Endeavor in the northwest Atlantic from 18 July to 6 August 2014. Profiles of optical properties, conductivity, temperature, and depth (CTD) were collected at 23 stations. Data collected at these stations were used to quantify the effects of vertical structure in phytoplankton biomass, light attenuation, and chlorophyll on NPP calculations. Casts where the photic zone depth was greater than the depth of the water column (5 stations) were excluded from the analyses. Concurrent measurements with an ocean-optimized airborne lidar were compared to in-water measurements and used to evaluate how future satellite lidar data may complement passive ocean color observations to reduce uncertainties in retrieved ocean ecosystem properties.

Ship-based (hereafter referred to as ‘in situ’) absorption and attenuation data at 9 wavelengths (412, 440, 488, 510, 532, 555, 650, 676, and 715 nm) were collected using a WET Labs (Philomath, OR) ac-9. The ac-9 was calibrated with Milli-Q ultrapure water following the protocols in Twardowski et al. (1999) [14]. Absorption was corrected for scattering effects using the proportional method of Zaneveld et al. (1994) [15]. Data were corrected for temperature and salinity effects using the coefficients of Twardowski et al. (1999) [14] and in situ CTD data (SeaBird SBE49 CTD; Bellevue, WA). Chlorophyll was calculated from phytoplankton absorption using the method of Sullivan et al. (2005) [16]. Backscatter was measured using a WET Labs ECO-BB9 (412, 440, 488, 510, 532, 595, 660, 676, and 715 nm). Backscatter data were linearly interpolated for wavelengths not matching the ac-9 (555 and 650 nm). Volume scattering function data were converted to backscattering coefficients following the protocol in Sullivan et al. (2013) [17]. Light attenuation coefficients at 532 nm were calculated as a function of total absorption at 532 nm, backscattering at 532 nm, and sun angle according to Gordon et al. (1988) [18]. Solar zenith angle was assumed to be 0° for comparison to HSRL-1 measurements. All data were averaged into 1 m depth bins and smoothed using a five-point moving average.

HSRL-1 measurements of ocean bbp and Kd at 532 nm were collected onboard the NASA LaRC King Air aircraft at approximately 9 km altitude [8]. In situ optics casts were matched to HSRL-1 measurements within one day and half a degree. On average, HSRL-1 and in situ comparisons were made between measurements collected 3.3 km and 6.8 hours apart (Table 1). The median of the ten nearest lidar profiles (~4 km radius) was used for comparisons with in situ data. Phytoplankton carbon (Cphyto; mg m−3) was calculated from bbp according to Graff et al. (2015) [19] for both in situ and HSRL-1 measurements. HSRL-1 Cphyto data were converted to chlorophyll concentrations using depth-dependent changes in chlorophyll:Cphyto resulting from nutrient-replete photoacclimation [11]:

Photoacclimation=0.022+(0.0450.022)e3Ig,
Chlorophyll=photoacclimation*Cphyto,
where Ig = growth irradiance (see below). Data were smoothed vertically using a five-point moving average. The HSRL-1 data were matched by depth to the in situ measurements using linear interpolation, reducing the vertical resolution from 0.94 to 1 m. The HSRL-1 measures ocean properties to approximately 2.5-3 optical depths below the surface. The measured bbp and Kd values below this depth were fixed to the value measured at the maximum penetration depth.

Tables Icon

Table 1. Distances between the HSRL-1 nearest profile and optics cast

NPP (mg m−3 d−1) was calculated using the CbPM where inputs include bbp (m−1), Kd (PAR; m−1), PAR (Ein m−2 d−1), mixed layer depth (MLD), euphotic zone depth (Zeu), day length (dl), nutricline depth, and Ig (Ein m−2). The light attenuation coefficient for PAR was calculated from Kd(532) following Austin and Petzold (1990) [20] and Morel et al. (2007) [21]. PAR was measured using an Eppley PSP (Eppley Laboratories, Newport, RI) mounted to the top of the crane cab eight meters above the waterline. MLD was calculated using a fixed density threshold of 0.03 kg m−3 following de Boyer Montegut et al. (2004) [22]. The CbPM was used to model NPP because calculations are vertically resolved and thus provide depth-dependent values for comparison to calculations with vertically-resolved measurements. Growth irradiance (Ig) is the light level to which phytoplankton are acclimated. Growth irradiance in the mixed layer was calculated as [10,11]:

Ig=(PAR*0.975/dl)eKd*MLD2,
where Kd is the median light attenuation coefficient for PAR in the mixed layer and 0.975 accounts for Fresnel reflection. Growth irradiance at depths below the mixed layer was taken as PAR at that depth. For HSRL-based calculations of chlorophyll, Kd was proportionally adjusted to match the in situ data before solving for Ig. Euphotic zone depth was defined as the 0.415 mol quanta m−2 d−1 isolume depth [23]. Nutrients were not measured as part of SABOR and, thus, nutricline depths employed in the CbPM were taken from the World Ocean Atlas [24]. Stratification indices were calculated by taking the difference between densities at 10 m and 40 m. If the maximum depth was less than 40 m, the density at the maximum depth was used to calculate the stratification index.

A single surface-weighted value was calculated from the in situ profiles of Kd and Cphyto following Zaneveld et al. (2005) [25]. These values were then extended through the water column to create the unstructured condition used to quantify the effect of uncharacterized vertical structure. Surface measurements of Cphyto, the underwater light field, and chlorophyll were used to calculate NPP using the traditional CbPM and compared to NPP calculated with vertically-resolved measurements. Percent relative error rel) was used as a measure of vertical structure and calculated as:

rel(%)=100*rely¯,
rel=i=1n(yiyi)^n,
where yi and y^jare the measured ocean properties from, respectively, a uniform and vertically-resolved water column at depth i, and y¯is equal to the mean of the vertically-resolved measurements. This metric gives no indication of the residual magnitudes, so the percent mean absolute error (δ) was also calculated:
(%)=100*y¯,
=i=1n|yiyi|^n.
These metrics were also used to compare the HSRL-1 to in situ measurements where yi and y^iare the in situ and HSRL-1 measurements of ocean properties, respectively, and y¯ is the mean of the in situ values. Pearson correlation coefficients were used to compare HSRL-1 and in situ measurements and additionally to evaluate depth-dependent differences between measurements. Finally, percent root mean square error (%RMSE) was calculated as:

RMSE(%)=100*RMSEy¯,
RMSE=i=1n(yiyi)2^n.

3. Results

3.1 In situ data

Phytoplankton and optical properties exhibited significant vertical structure at each SABOR station. Comparison of euphotic zone-integrated Cphyto values (ΣCphyto) calculated using depth-resolved in situ data and values based solely on surface properties within the passive ocean color detection layer produced δrel values ranging from −45.6% to −6.2% (δ¯rel = −19.9%) (Fig. 1(a)). The ‘ocean color type’ values thus consistently underestimated ΣCphyto at all stations. Furthermore, previous studies in the region have shown that sub-surface chlorophyll structure is observed under stratified conditions [13]. In a similar manner, we found that the largest relative errors were correlated with the stratification index (r = 0.72). Comparison of depth-resolved and surface-only based Kd(532) values showed a similar degree of discrepancy, with δrel values ranging from −36.3% to −2.7% (δ¯rel = −20.2%) (Fig. 1(b)). Largest relative errors in depth-integrated Kd (ΣKd) were correlated, though not as strongly, with the stratification index (r = 0.52).

 figure: Fig. 1

Fig. 1 SABOR stations plotted as a function of percent relative error in (a) Cphyto and (b) Kd(532), where percent relative error is a measure of vertical structure. Isobaths are plotted at 1000 m intervals.

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Knowledge of the vertical variability in Cphyto and Kd is critical to obtaining accurate column and vertically-resolved estimates of NPP. We tested the significance of this structure by comparing vertically-resolved calculations of NPP to values where uniform properties were assumed from surface-weighted properties, as would be applied to passive ocean color data. The vertically-resolved in situ Cphyto and Kd data enabled much more accurate estimates of NPP compared to calculations made without information on the vertical structure (δrel = −43.2 – 54.0%; δ¯rel = −8.4% and δ = 11.7 – 54.0%; δ¯ = 33.4%) (Fig. 2). Larger absolute errors, or differences between in situ measurements and an assumed constant profile, were observed deeper in the water column, leading to larger absolute differences in sub-surface NPP. To understand the relative impact of Cphyto on NPP calculations as a function of depth, errors in NPP were normalized to Cphyto errors and binned by optical depth. Normalized NPP errors decreased exponentially from the first to third optical depths. Thus, biomass features located near the surface had a significantly larger impact on NPP estimates than errors located deeper in the water column.

 figure: Fig. 2

Fig. 2 NPP (mg C m−3 d−1) profiles from the carbon-based production model (CbPM) at every station where the maximum depth is greater than the euphotic depth. The black lines are the in situ optics-based estimates. The profiles which use surface-weighted values in the traditional CbPM are shown in blue. Panels (a) and (h) are the stations with replicate casts (∆t < 1 day, same station) with the error bars representing one standard deviation.

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HSRL-1 retrieves optical properties that are limited to the first 2.5-3 optical depths. Therefore, in situ values of bbp and Kd from three optical depths to the bottom of the photic zone were held constant to test how much error is introduced to integrated biomass and light attenuation calculations when this modification is applied. Mean absolute errors were only 4.4% and 3.1% for Cphyto and Kd, respectively, indicating that applying this extrapolation to HSRL-1 data at depth has only a small effect on integrated biomass and light calculations in the photic zone.

3.2 HSRL-1 measurements of ocean properties

A strong correlation (r = 0.94) was observed between in situ and HSRL-1 measurements of bbp (Fig. 3(a)). Similarly, in situ and HSRL-1 values of Kd also showed high correlation (r = 0.90) (Fig. 3(b)). The HSRL-1 measurements of bbp and Kd were high compared to in situ data, with δrel values of −9.26% and −12.92% for bbp and Kd, respectively. Measurement differences were not correlated with depth for bbp or Kd (r = 0.18 and −0.13).

 figure: Fig. 3

Fig. 3 HSRL-1 and in situ measurements of (a) bbp (m−1) and (b) Kd (m−1) with marker color indicating optical depth. The dotted red lines show the 1:1 relationship.

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Spatial and temporal variability in geophysical properties is one factor contributing to differences between in situ and HSRL-1 retrievals and this issue may be particularly important in the highly variable region studied during SABOR. HSRL-1 and in situ profiles were often collected more than 10 km away. Given the spatial scale of variability in coastal waters (~200 m) observed by Moses et al. (2016) [26], we would expect differences between the two measurements (Figs. 4 and 5). When we applied more stringent matchup criteria (<0.01° and <3 hours) [27], only 7 profiles were available for comparison. Surprisingly, the correlation coefficients for bbp decreased slightly to 0.92 and increased to 0.92 for Kd.

 figure: Fig. 4

Fig. 4 HSRL-1 and in situ measurements of bbp (m−1). The black profiles are the in situ measurements where panels (a) and (h) show the stations with replicate casts (∆t < 1 day, same station) with the error bars representing one standard deviation. The red profiles are the HSRL-1 measurements (median of ten nearest profiles to in situ cast) with the error bars representing one standard deviation within profiles. The error bars are a measure of the spatial variability around each station. The dotted lines show the first and second optical depths.

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 figure: Fig. 5

Fig. 5 HSRL-1 and in situ measurements of Kd (m−1). The black profiles are the in situ measurements where panels (a) and (h) show the stations with replicate casts (∆t < 1 day, same station) with the error bars representing one standard deviation. The red profiles are the HSRL-1 measurements (median of ten nearest profiles to in situ cast) with the error bars representing one standard deviation within profiles. The error bars are a measure of the spatial variability around each station. The dotted lines show the first and second optical depths.

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The carbon-based production model (CbPM) employs information on chlorophyll concentration to characterize physiological variability within plankton communities. The HSRL-1 currently does not retrieve chlorophyll directly so we made a first order calculation of chlorophyll from HSRL-1 bbp data using the chlorophyll:Cphyto relationship of Westberrry et al. (2008) [11]. Vertical profiles of chlorophyll calculated in this manner (Eqs. (1a) and (1b) from the HSRL-1 data exhibited a significant correlation with in situ optically-based chlorophyll values (r = 0.84) (Fig. 6(a)). Given the temporal variability in vertical plankton properties discussed above and the implications this has on profiles of NPP, we observed an exceptional correlation between HSRL-1 and in situ optics-based NPP values (r = 0.81) (Fig. 6(b)). Stations 11 and 18 were not included in this analysis because there were no spatial matchups fitting distance criteria.

 figure: Fig. 6

Fig. 6 HSRL-1 and in situ measurements of (a) chlorophyll a (Chl; mg m−3) and (b) net primary production (NPP; mg m−3 d−1). The inset in panel (b) shows the full range of data with x and y-axes limits set to 200 mg m−3d−1. The red lines show the 1:1 relationship.

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4. Discussion

Passive ocean observing sensors do not measure subsurface structure in ocean properties, resulting in errors in water column integrated phytoplankton biomass, light attenuation, and NPP estimates. In situ data show relative errors of up to 45.6% and 36.3% in phytoplankton biomass and light attenuation, respectively, when compared to no vertical structure. Measured ocean properties were underestimated at every station relative to in situ data and NPP errors up to 54% were observed when the vertically-weighted surface data were used. Furthermore, the vertical structure observed during SABOR does not capture the full range of variability globally, so the potential errors in products derived from ocean color are likely to be even larger than measured during this field campaign. Our findings, therefore, indicate that the ability to resolve upper ocean vertical structure in phytoplankton stocks and the underwater light field significantly improves estimates of NPP over ‘ocean color type’ values.

The largest proportional errors in integrated NPP were associated with biomass features above two optical depths. These results are consistent with the conclusions of Churnside (2015) [1] who found that using passive remote sensing methods introduced significant errors to NPP estimates when subsurface phytoplankton layers were present and this error was largest when the chlorophyll layer was located in the upper water column. The penetration depth expected for an ocean-optimized satellite lidar is within this upper zone which suggests that a satellite ocean-optimized lidar would significantly improve global estimates of integrated phytoplankton biomass and NPP.

Matchups between in situ and HSRL-1 measurements were good with correlation coefficients for bbp and Kd of 0.94 and 0.90, respectively, despite the high spatial and temporal variability that characterizes the SABOR region. This is quite remarkable given that point measurements from in situ profiles were compared to measurements averaged up to 70 km away (see Table 1). The different spatial and temporal resolutions between measurements likely contributed to the observed discrepancies in matchups.

Although SABOR provided several coincident matchups between HSRL-1 and in situ optics, the data are still limited. An important avenue for future studies will be to expand matchup analyses with data from a broader range of environmental conditions, such as data collected as part of the NAAMES (North Atlantic Aerosols and Marine Ecosystems Study) campaign. Such comparative analyses between coincident HSRL-1 and in situ measurements will provide important information for evaluating science objectives and design criteria for a future ocean-optimized space-based lidar.

The current study demonstrates the utility of the HSRL technique for depth-resolved profiles on bbp and Kd, which, by analogy to the improvements achieved with the depth-resolved in situ data, would enable much higher accuracy in remote-sensing estimates of NPP. Applying the technique at more than one wavelength could provide even greater accuracy in NPP. The more advanced NASA HSRL-2 instrument currently implements the HSRL technique at both 355 and 532 nm for atmospheric measurements and is in the process of being upgraded for higher vertical resolution (~1 m) to optimize it for ocean profiling. Measurements of Kd at these two wavelengths will enable separation of different ocean constituents contributing to the attenuation of light in the water column, e.g., colored dissolved organic matter (CDOM), which is the primary light-absorbing agent in the UV spectrum. The light attenuation coefficient is a function of scattering and absorption, and since the backscattering coefficient is directly measured by the HSRL, the only unknown property is absorption, which includes absorption by CDOM, water, and particles, including phytoplankton. Chlorophyll (i.e., phytoplankton absorption) could thus be calculated directly by subtracting from Kd the effects of scattering and CDOM and water absorption. The effects of nutrient limitation on chlorophyll:Cphyto are accounted for in this calculation and thus represent an improvement over the methods used here. Chlorophyll is a critical variable for most NPP algorithms, particularly because of the information it provides on phytoplankton physiology when retrieved concurrently with independent estimates of biomass. Improvements in the estimation of vertical profiles of chlorophyll are critical for improving NPP results.

We are entering a new era in satellite oceanography where satellite lidar observations can address many of the issues that challenge passive ocean color techniques. Already, observations from the CALIOP lidar have been used to quantify global stocks of Cphyto and total POC and to evaluate complete annual plankton cycles in the polar regions that are particularly problematic for passive sensors [28,29]. Despite these successes, the CALIOP lidar sensor has limitations for ocean retrievals. First, CALIOP was designed for atmospheric applications and its vertical binning resolution (22.5 m) is too coarse for retrieving information on vertical structure in the oceans. Second, CALIOP is unable to directly separate the backscatter and attenuation coefficients. Behrenfeld et al. (2013) [28] retrieved bbp estimates from CALIOP by using independent estimates of Kd from the MODIS passive ocean color sensor and an estimate of the reflectance of the laser beam from CloudSat radar surface reflection data or wind speed data from the Microwave Scanning Radiometer-EOS. In the subsequent polar-focused study of Behrenfeld et al. (2016) [29], an empirical relationship between lidar depolarization and Kd was used to retrieve bbp, due to lack of coincident ocean color data particularly during the winter months. These parameterizations have been tested from data acquired on episodic intervals during which CALIOP was pointed 30° off nadir to minimize the laser surface reflection. However, the parameterization scheme for nominal near-nadir operations were still dependent on an empirically derived relationship between collated MODIS and CALIOP bbp and Kd at lower latitudes [29]. Major advantages over the standard elastic backscatter lidar approach of CALIOP is achieved via the HSRL technique. HSRL permits independent, direct retrievals of bbp and Kd with minimal assumptions and no reliance on ancillary data. This major advantage, along with the high vertical-resolution sampling (~1 m), allowed the HSRL-1 instrument to collect vertically resolved retrievals of Kd and phytoplankton biomass during SABOR. While an HSRL has not yet been flown in space, there is no technological barrier to either implementing the technique or achieving high vertical resolution (e.g., 3 m) for ocean profiling. Such an instrument flown in space would provide independent and more accurate ocean property retrievals than a standard CALIOP-like backscatter lidar and an enormous independent data set to evaluate and improve passive ocean color retrievals.

Funding

National Atmospheric and Space Administration (NASA) grants NNX15AI15G, NNX15AF30G, and NNX15AN17G.

Acknowledgments

We thank James Churnside for his numerous invaluable discussions. We thank Nicole Stockley for support with in situ data collection. We acknowledge Kimberley Halsey and Jason Graff for providing in situ chlorophyll, carbon, and NPP data for comparisons to optics-based values and for their insightful comments. We additionally thank the captain and crew of the R/V Endeavor.

References and links

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Figures (6)

Fig. 1
Fig. 1 SABOR stations plotted as a function of percent relative error in (a) Cphyto and (b) Kd(532), where percent relative error is a measure of vertical structure. Isobaths are plotted at 1000 m intervals.
Fig. 2
Fig. 2 NPP (mg C m−3 d−1) profiles from the carbon-based production model (CbPM) at every station where the maximum depth is greater than the euphotic depth. The black lines are the in situ optics-based estimates. The profiles which use surface-weighted values in the traditional CbPM are shown in blue. Panels (a) and (h) are the stations with replicate casts (∆t < 1 day, same station) with the error bars representing one standard deviation.
Fig. 3
Fig. 3 HSRL-1 and in situ measurements of (a) bbp (m−1) and (b) Kd (m−1) with marker color indicating optical depth. The dotted red lines show the 1:1 relationship.
Fig. 4
Fig. 4 HSRL-1 and in situ measurements of bbp (m−1). The black profiles are the in situ measurements where panels (a) and (h) show the stations with replicate casts (∆t < 1 day, same station) with the error bars representing one standard deviation. The red profiles are the HSRL-1 measurements (median of ten nearest profiles to in situ cast) with the error bars representing one standard deviation within profiles. The error bars are a measure of the spatial variability around each station. The dotted lines show the first and second optical depths.
Fig. 5
Fig. 5 HSRL-1 and in situ measurements of Kd (m−1). The black profiles are the in situ measurements where panels (a) and (h) show the stations with replicate casts (∆t < 1 day, same station) with the error bars representing one standard deviation. The red profiles are the HSRL-1 measurements (median of ten nearest profiles to in situ cast) with the error bars representing one standard deviation within profiles. The error bars are a measure of the spatial variability around each station. The dotted lines show the first and second optical depths.
Fig. 6
Fig. 6 HSRL-1 and in situ measurements of (a) chlorophyll a (Chl; mg m−3) and (b) net primary production (NPP; mg m−3 d−1). The inset in panel (b) shows the full range of data with x and y-axes limits set to 200 mg m−3d−1. The red lines show the 1:1 relationship.

Tables (1)

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Table 1 Distances between the HSRL-1 nearest profile and optics cast

Equations (9)

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P h o t o a c c lim a t i o n = 0.022 + ( 0.045 0.022 ) e 3 I g ,
C h l o r o p h y l l = p h o t o a c c lim a t i o n * C p h y t o ,
I g = ( P A R * 0.975 / d l ) e K d * M L D 2 ,
r e l ( % ) = 100 * r e l y ¯ ,
r e l = i = 1 n ( y i y i ) ^ n ,
( % ) = 100 * y ¯ ,
= i = 1 n | y i y i | ^ n .
R M S E ( % ) = 100 * R M S E y ¯ ,
R M S E = i = 1 n ( y i y i ) 2 ^ n .
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