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Remote sensing of zooplankton swarms


Zooplankton provide the key link between primary production and higher levels of the marine food web and they play an important role in mediating carbon sequestration in the ocean. All commercially harvested fish species depend on zooplankton populations. However, spatio-temporal distributions of zooplankton are notoriously difficult to quantify from ships. We know that zooplankton can form large aggregations that visibly change the color of the sea, but the scale and mechanisms producing these features are poorly known. Here we show that large surface patches (>1000 km2) of the red colored copepod Calanus finmarchicus can be identified from satellite observations of ocean color. Such observations provide the most comprehensive view of the distribution of a zooplankton species to date, and alter our understanding of the behavior of this key zooplankton species. Moreover, our findings suggest that high concentrations of astaxanthin-rich zooplankton can degrade the performance of standard blue-green reflectance ratio algorithms in operational use for retrieving chlorophyll concentrations from ocean color remote sensing.


Remote sensing of ocean color has led to major advances in understanding ocean-wide phytoplankton dynamics by providing much greater temporal and spatial coverage than is possible by ship-based sampling. Phytoplankton species rely on pigments for photosynthesis and other photophysiological processes. These different colored pigments affect the spectral characteristics of light redirected out of the sea and so becoming accessible to remote sensing detectors1,2. Surface-dwelling zooplankton, on the other hand, do not rely on capturing energy through pigments, and tend to be largely transparent to avoid the attention of visual predators. However, many crustaceans synthesize the red carotenoid astaxanthin from yellow and orange precursors in their diet and appear reddish3; this includes a few species that seasonally inhabit the surface ocean, such as copepods of the genus Calanus4. The widely distributed copepod Calanus finmarchicus (ca. 3 mm in size) is “often occurring in enormous shoals and thus sometimes giving the sea a conspicuous reddish hue”5, or “yellowish tint”6.

C. finmarchicus is a key species in the North Atlantic ecosystem, frequently constituting > 50% of mesozooplankton biomass7. Due to its large biomass and high lipid content this species is the principal prey for some of the world’s largest fish stocks, such as larvae of Northeast Arctic cod (Gadus morhua) and adult Norwegian spring spawning herring (Clupea harengus)8. It is also important for the transfer of energy to most marine animals at higher trophic levels throughout the ecosystem9. C. finmarchicus is also commercially exploited for the rich omega-3 fatty acid content of its lipids10. Intense UV-radiation at the sea surface can degrade the copepods’ lipids through peroxidation11, but nonetheless during spring and summer, species of the genus Calanus have repeatedly been observed right at the sea surface12,13,14,15,16,17. It has been suggested that one reason copepods synthesize astaxanthin is that it protects against oxidative damage of lipids by scavenging free radicals3,11. Due to its red astaxanthin pigmentation, and its importance as food for commercially important fish species, C. finmarchicus has been given the local common names ‘raudåte’ (Norwegian) and ‘rauðáta’ (Icelandic), meaning ‘red feed’.

Aggregative behavior is a universal feature in a wide range of animals18,19, and the majority of marine animals aggregate to some extent20,21,22,23,24. This includes zooplankton organisms that are mostly smaller than 4 mm and possess limited mobility25. However, mechanisms for spatial aggregations of zooplankton are still poorly understood and remain a central issue in marine ecology26,27,28. Progress is hindered by the difficulty of mapping zooplankton abundance and distribution from ships. Thus, although several sporadic observations indicate surface aggregations of Calanus spp. during daylight12,13,14,15,16,17, the frequency of occurrence and the extent of these zooplankton surface aggregations are not known. This impedes our ability to identify behavioral and physical drivers for zooplankton aggregations, and in turn inhibits our understanding and modelling of the consequences for the ecosystem.

Here we test the hypothesis that the presence of high concentrations of the pigment astaxanthin will enable discrimination of zooplankton surface swarms from phytoplankton blooms in ocean color remote sensing signals. By pairing satellite images with high-resolution in situ zooplankton data, and with detailed measurements of optical properties of seawater and of Calanus spp. at oceanographic stations, we aim to establish the potential for remote sensing of this copepod.


Large-scale zooplankton surface swarms

During an oceanographic cruise off the coast of Northern Norway in May 2017 large areas of red pixels were visible in enhanced Red-Green-Blue (RGB) images obtained from the VIIRS (Visible Infrared Imaging Radiometer Suite) satellite (Fig. 1). Similar features were observed in concurrent images from other ocean color satellite systems (not shown). The main patch stretched from the coast across the shelf and northward along the shelf break. It covered an area of several thousand km2, with mesoscale structures visible along the shelf break. At the same time, a suite of in situ instruments detected very high abundances of Calanus spp. in the surface layer (Fig. 2, Supplementary Figs 13), at locations matching the red pixels. Most of the observed copepods were highly pigmented, and many contained pigments not only in the lipid sac and antenna, but also in the carapace (Fig. 1, inset). Genetic analyses confirmed that C. finmarchicus was the dominant Calanus species in the patch, with a few individuals of the closely related C. glacialis identified at stations 6 (2 ind.) and 7 (1 ind.). Smaller-scale features within the large red-pixel patch were resolved by in situ optical plankton recorders (laser optical plankton counter and video plankton recorder). These instruments detected horizontal and vertical structures within the patch, and both sensors recorded abundances of >1,000 Calanus spp. m−3 in the upper 10 m (Fig. 2, Supplementary Figs 1 and 2). Abundance estimates based on net samples (180 µm mesh) were of the same order of magnitude, and at 7 out of 9 stations the highest abundance of pigmented copepods (copepodite stage IV and older) was observed in the upper 5 m (Fig. 2, Supplementary Fig. 3).

Figure 1

Weekly composite of VIIRS RGB images obtained during 27 April – 3 May 2017, showing large areas of red pixels. In situ sampling was performed in the study area off northern Norway between 28 April to 4 May 2017, using optical plankton counters towed along transects A to D (laser optical plankton counter – yellow lines, video plankton recorder – blue lines), and at eight stations (white triangles). Locations from which pixels were extracted for comparing Remote Sensing Reflectance (Fig. 3) are marked with white asterisks; O – open ocean, P – inside patch, C – coastal. The copepod Calanus finmarchicus (developmental stage CV) with red astaxanthin pigmentation in the antenna and across its body is depicted in the inset. Fully processed data for the satellite image were provided by NEODAAS.

Figure 2

Abundance and distribution of older developmental stages of Calanus spp. (copepodites IV and older) in the upper 10–30 m along transect A as observed by (a) a laser optical plankton counter, (b) a digital auto video plankton recorder, and (c) a MultiNet at station 4. Ticks along the top axis of panel a indicate start points for vertical sampling profiles.

Remote sensing reflectance and absorption of the copepod’s pigments

Comparison of satellite remote sensing reflectance (Rrs) spectra from inside the patch, in the open ocean, and in a coastal area (Fig. 3a) showed blue reflectance decreasing from open ocean to coastal waters as expected, and then decreasing further inside the patch. Radiative transfer modelling using in situ measurements of inherent optical properties from inside the patch consistently overestimated Rrs at wavelengths <550 nm compared with data from remote sensing (Fig. 3b). These observations led us to perform a serial addition experiment, where the absorption of copepods was measured in a point source integrated cavity absorption meter (PSICAM), which has previously been shown to measure absorption without errors due to particle scattering29. C. finmarchicus were found to absorb strongly in the blue-green, and absorption increased linearly with copepod numbers (Fig. 4a). The absorption of C. finmarchicus extended across the blue-green spectrum with a peak at 486 nm, where the discrepancy between modeled and measured Rrs was detected (Fig. 4b). The absorption of astaxanthin extracted from copepods in the laboratory peaked at 476 nm in acetone (Fig. 4c), confirming the role of the pigment in driving Calanus sp. absorption.

Figure 3

Remote sensing reflectance. (a) At three selected locations (nine pixels each, thin lines): in the open ocean (blue), inside the red pixel patch (red), and in a coastal area (green). Thick line: mean over the nine pixels. (b) At 8 stations in the study area. Red lines: VIIRS satellite data, blue lines: radiative transfer model populated with inherent optical properties measured at the stations. The Calanus spp. abundance in the upper 5 m as observed by MultiNet is indicated for each station.

Figure 4

Light absorption of Calanus pigments. (a) Absorption with increasing number of copepods during serial addition to a point source integrating cavity absorption meter (PSICAM) (b) In vivo absorption measured in the PSICAM. (c) in vitro absorption measured spectrophotometrically from pigments extracted in acetone. Thick line: mean over all 21 samples, gray area: 95% confidence interval.

In situ phytoplankton and satellite chlorophyll

In situ measurements of phytoplankton were relatively low, both in cell numbers (<50 × 103 cells m−3) and biomass (mostly < 2 mg chlorophyll a m−3). The spatial distribution of satellite-recorded chlorophyll a (Fig. 5) was essentially the same as that of the red pixels (Fig. 1) and both in situ and VIIRS remotely sensed chlorophyll concentrations inside the patch showed a similarly broad range of values up to approximately 6 mg m−3 (Fig. 6). However, the distribution of in patch VIIRS chlorophyll a data (Fig. 6a) was skewed to higher values, with very few data points < 1 mg m−3. In contrast, the in situ chlorophyll a data from the upper 5 m had a greater proportion of values < 1 mg m−3 (Fig. 6b) that was broadly consistent with the VIIRS data from outside the patch (Fig. 6c). It thus appears that there may be a tendency for the standard blue-green reflectance ratio algorithm to return overestimates of chlorophyll a for waters with high abundances of astaxanthin-rich zooplankton.

Figure 5

Weekly composite of VIIRS chlorophyll a during 27 April – 3 May 2017. Fully processed data for the satellite image were provided by NEODAAS.

Figure 6

Chlorophyll a concentration in the study area. (a) Measured by satellite inside the patch, defined as Rrs > 4 × 104 sr−1 (b) measured fluorometrically from filtered water samples (c) measured by satellite outside the patch, defined as Rrs < 2 × 104 sr−1.


The results corroborate our hypothesis that high abundances of astaxanthin-rich zooplankton in surface waters can influence bulk optical properties of these waters, and can be detected by ocean color remote sensing. To the best of our knowledge, this is the first time a larger, metazoan zooplankton species has been observed from space. The recording of super-swarms of Calanus spp. copepods at the sea surface alters our understanding of the behavior of this key zooplankton species in spring. Herbivorous copepods tend to display a flexible, unsynchronized, vertical migration behavior to balance food availability against predation pressure30,31. However, our observations of large-scale surface aggregations during daylight hours indicate that Calanus spp. at higher latitudes might maximize fitness by remaining in surface waters during the short productive season32,33. Note that our study region experiences 24 hours daylight from approximately mid-May to mid-July. Across the North Atlantic and the North Pacific, species of the genus Calanus have been observed in dense aggregations at the sea surface12,13,14,15,16,17,34. The new observations show that historical local sightings may be features of much larger spatial extent, involving vast numbers of animals of the utmost importance to fisheries and the broader marine food web.

The observed discrepancy between modeled and measured remote sensing reflectance (Rrs) at blue wavelengths (Fig. 3b) can be attributed to copepod absorption as revealed by the PSICAM measurements (Fig. 4a,b). These in vivo Calanus sp. absorption data are broadly consistent with the in vitro absorption of the copepods’ astaxanthin pigment in acetone (Fig. 4c), as well as with previous measurements of astaxanthin absorption in deep sea zooplankton35. Other astaxanthin-rich zooplankton such as krill likely absorb at similar wavelengths3. Rrs was modeled using measured in situ IOPs, with an approach that has previously yielded good agreement with in situ radiometry36. However, in this study we attribute the discrepancy in the blue-green to the sample volumes of the in situ IOP sensors being too small (maximal 30 mL) to resolve adequately the optical properties of C. finmarchicus and other astaxanthin-rich zooplankton, even at the high abundances observed here. Although the recorded abundances of Calanus spp. are comparatively high, quantifying abundance in the surface layer around large ships is challenging due to mixing by thrusters and other local disturbances. We thus cannot rule out that the copepods were concentrated in a very thin layer at the sea surface prior to our obtrusive sampling. There may also be effects associated with evasion response behaviors by larger astaxanthin-rich zooplankton, reducing the signals recorded by in situ sensors. Most krill species are strong swimmers and able to evade even towed sampling systems during daylight hours37. Astaxanthin-rich zooplankton optical signals (primarily absorption) were thus underrepresented in the radiative transfer model. In contrast, the satellite sensor does not disturb the zooplankton population and each satellite pixel integrates over much larger spatial scales (>100 m) with the result that the observed, high abundances of C. finmarchicus, and potentially larger, under-sampled zooplankton species, appear to have measurably influenced satellite Rrs. This highlights a general need to consider the impact of large (>1 mm), colored particles, such as but not limited to C. finmarchicus, on the propagation of light in the ocean and hence on Rrs signals. There is also a corresponding need to develop new techniques to adequately resolve IOPs of waters containing these particles.

The study area is highly advective, with eddies developing between the Norwegian Coastal Current that flows northeastward along the shore, and the saltier Norwegian Atlantic Current that flows in the same direction but further offshelf38. The main patch of Calanus spp. followed the shelf edge in a relatively narrow band from station 5 to station 8 and 12 (Fig. 1). Strong spatio-temporal variability limited our ability to perform direct comparisons between individual in situ and remotely sensed observations. At stations 5, 8 and 12, for example, relatively low Calanus spp. abundances were observed in net samples, but satellite Rrs was nevertheless substantially reduced in the blue-green (Fig. 3b), and the optical zooplankton sensors LOPC and VPR registered high abundances in that area between 28 and 30 April (Fig. 1, Supplementary Figs 1, 2). The most likely explanation is that the satellite captured a patch during the early days in the composite image (27 to 29 April), and that the patch had moved slightly when we took net samples (30 April to 3 May, Table 1) so that we were sampling in areas classified as “open ocean” according to the satellite image.

Table 1 Selected measurements at stations in the study area.

The discrepancy between satellite and modeled Rrs cannot be attributed to phytoplankton. Algal optical properties were well accounted for by the in situ IOP measurements, and were therefore included in the modeled Rrs spectra (Fig. 3b). Evidence to support this is found in the PSICAM data, where the absorption peak around 670 nm (Fig. 4a) is due to chlorophyll a. Very importantly, by influencing absorption and Rrs in the blue-green, high abundances of Calanus spp. and other astaxanthin-rich zooplankton could potentially affect the performance of standard blue-green reflectance algorithms, such as those used to estimate chlorophyll a concentrations by ocean color remote sensing (e.g.39,40). The distribution of VIIRS chlorophyll a (Fig. 5) shows strong spatial correlation with red pixels in the RGB image (Fig. 1). Due to the relatively low number of in situ measurements of chlorophyll a, and limited spatio-temporal match-ups, our data in this respect are not conclusive. However, the fact that Calanus spp. absorbed light strongly across the blue-green spectrum, and were present in high abundances at the surface in these waters, provides a plausible mechanism for influencing the bulk IOPs of the water, and hence the Rrs signals in the blue-green. It therefore seems likely that standard blue-green ratio algorithms to measure satellite chlorophyll a might be generally impacted in areas with high surface abundances of Calanus finmarchicus or other astaxantin-rich zooplankton.

On the positive side, the observed dependence of absorption on copepod numbers strongly suggests potential for development of new algorithms to estimate the abundance of a key species in the North Atlantic marine ecosystem. Quantitative remote sensing of surface abundances of the copepod C. finmarchicus might be possible in the near future. However, developing a quantitative algorithm for estimating total abundance of Calanus spp. is challenging because of the diel and seasonal vertical migrations performed by these copepods. Empirical relationships between surface abundance and abundance in deeper layers could potentially be established based on the vast amount of literature describing these migrations. Nevertheless, the benefits of remotely detecting surface C. finmarchicus abundance are substantial, and include increased understanding of zooplankton swarming behavior, better informed sustainable management of this harvested key species, and the possibility to track the species’ observed range expansion with climate change41. Here we report on the occurrence of red pixels in VIIRS RGB images associated with high abundances of C. finmarchicus in the Norwegian Sea during one week in early May 2017. We subsequently observed similar red pixel features in RGB images obtained on cloud-free days later in the season. Furthermore, the harvesting company Calanus AS reports surface swarms to occur regularly in this region between May and July (Kurt Tande, pers. comm.). This indicates that large-scale surface aggregations of Calanus sp. are a recurrent feature. We expect similar large-scale surface aggregations to occur in other higher latitude systems, where the productive season is short, and where local surface aggregations have been observed12,13,14,15,16,17,34. Remote sensing of Calanus spp might be possible in these systems as well, but the universality of the observed features remains to be established.

Material and Methods

Field sampling

In situ data were collected during a cruise on R/V “Helmer Hanssen” from April 28 to May 4, 2017 off the coast of northern Norway. Semi-automatic optical sampling of zooplankton was performed along four transects (Fig. 1). Irradiance, inherent optical parameters (IOPs), chlorophyll a concentration, phytoplankton abundance, and the abundance, vertical distribution, genetic species identity and pigment absorption of Calanus were measured at 8 stations within the study area (Table 1).

Satellite images

Real-time support from NEODAAS (NERC Earth Observation Data Acquisition and Analysis Service) provided RGB images and NetCDF data files from daily (cloud-free) VIIRS satellite overpasses, which were used to map water masses with distinct spectral signatures and provided a first indication on the location of red, i.e. potentially Calanus-rich, patches. NEODAAS also provided weekly composite images such as that shown in Fig. 1 (RGB) and 5 (chlorophyll a), from 27 April to 3 May 2017. April 27–29 contributed most to the weekly average image, due to relatively high percentage of cloud cover on the later days. To generate the RGB image, wavebands 551 nm, 486 nm and 443 nm were used, and each color was scaled to include 95% of all pixels. A gamma correction of 0.9 was applied to the blue channel to improve contrast. To illustrate the differences in spectral Rrs, three areas (three times three pixels from each area) with three different colors were selected randomly from the weekly composites, representing an open ocean site (blue), a Calanus spp. patch (red) and a coastal site (green) (Fig. 3a). Satellite image pixels were determined to be inside the patch if red reflectance, Rrs(671 nm), was greater than 0.004 steradian−1 (sr), while those pixels with Rrs(671 nm) <=0.002 sr−1 were determined to be outside the patch, with intermediate values of red reflectance forming an unattributed boundary region. Additionally, VIIRS Rrs spectra were extracted from fully processed NetCDF files provided by NEODAAS. Rrs spectra measured at the pixel closest to each sampling location were selected from the weekly average (for maximum number of cloud-free pixels) image and used for comparison against modeled Rrs spectra (Fig. 3b). These Rrs spectra are for illustrative purposes only as the temporal mis-match for any given match-up with the weekly composite image may be significant.

Zooplankton data

Along the transects (Fig. 1, yellow lines) optical zooplankton data were obtained with high spatial resolution using a Moving Vessel Profiler (MVP, ODIM-Brooke Oceans Rolls Royce Canada, Ltd.) equipped with a Laser Optical Plankton Counter (LOPC, ODIM-Brooke Oceans Rolls Royce Canada, Ltd.). The LOPC was towed behind the ship at 6 to 7 knots, mounted in a “fish” profiling between surface waters down to 10 m above the seabed at 3.5–4 m s−1 vertical speed. The LOPC counts and measures plankton and particles at 2 Hz in the size range from 0.1 to 35 mm, which pass through its sampling tunnel. Data were quality-controlled ensuring that sample abundance was sufficiently low to avoid erroneous counts. Particles with the characteristics (transparency and size) of older stages of Calanus spp. (copepodites stages IV and older) were extracted from the data as described in42. Figures of the spatial distribution were prepared by interpolating between the vertical profiles across the transects, using the function griddata in the python library scipy.interpolate ( version 0.18.1).

After completion of the semi-automatic MVP sampling, sections of two transects (Fig. 1, blue lines) were revisited with a digital auto Video Plankton Recorder (VPR, Seascan Inc.). The VPR is equipped with a camera that takes colour images at a rate of up to 15 Hz. From the images the abundance and distribution of Calanus spp. (copepodite stages IV and older) was estimated as in17. The VPR was towed along transects in a saw-tooth trajectory between the surface and ~50 m depth. Towing speed was 2.5–3 knots, and the vertical speed of the VPR was ~0.5–1 m s−1.

The abundance of Calanus spp. at each station was quantified based on vertically stratified net samples collected by a MultiNet Midi (0.5 m s−1 hauling speed, 180 µm mesh size, 0.25 m2 mouth opening, Hydro-Bios, Germany). Samples were preserved in a solution of 80% seawater and 20% fixation agent (75% formaldehyde buffered with hexamine, 25% anti-bactericide propane-1,2-diol), resulting in a final formaldehyde concentration of 4%. Sub-samples from the depth layers 30 to 5 or 4 m, 5 or 4 to 2 m, and 2 m to surface were enumerated under a stereo microscope. At least 450 zooplankton individuals and about 100 Calanus were identified from each sample. Abundance was calculated based on the filtered volume obtained from the MultiNet flow meter.

Live Calanus copepodite stages CIV, CV and adult females were collected from the upper 15 m using a Bongo net (mouth opening 0.28 m2, mesh size 200 and 500 µm) that was towed for 10 minutes at 2 knots, at all stations except station 12. For pigment analyses triplicates of 30 to 39 Calanus spp. CV were frozen at −80 °C until analysis ashore. Copepods from one triplicate were photographed under the microscope prior to freezing. On land, frozen copepods were mixed with acetone under nitrogen and stirred until the biological material was colorless. The filtered acetone extract was evaporated under reduced pressure to dryness, re-dissolved in 0.5 ml acetone and light absorption measured by a UV/visible light spectrophotometer (Cary 100 UV-Vis, Agilent), Fig. 4c. From the frozen Bongo net samples, triplicates of individual Calanus spp. (CV and females) were selected for molecular analyses. Copepods were identified to species level using six molecular InDel markers and following the procedure described in43.

Phytoplankton data

Chlorophyll a concentrations were determined fluorometrically (10-AU fluorimeter, Turner designs, USA) from pigment extracts in methanol obtained from filtered water samples (triplicates of 50 to 150 mL, GF/F filters, Whatman Inc., USA) from 0, 5, 10, 25, 50 and 100 m depth at all stations. Water samples were collected using Niskin bottles, filtered on board, and kept frozen at −80 °C before analysis ashore immediately after the cruise. Water samples for phytoplankton enumeration were collected from 0, 5 and 10 m at stations 11 and 12. They were fixed in a solution of formaldehyde in seawater with a final concentration of 4% formaldehyde. Ashore, samples were analyzed under the microscope after settling for 24 hours in Utermöhl chambers44.

Bio-optics and radiative transfer modelling

Spectral absorption, attenuation and backscattering coefficients (inherent optical properties, IOPs) were determined from surface water samples collected with a bucket. Spectral absorption and attenuation coefficients were determined at nine different wavebands centered on 440, 532, 590, 660, 676, 715, 750, 820 and 870 nm using an in situ spectrophotometer (ac-9, WET Labs Inc., USA) equipped with 10 cm flow tubes. The ac-9 was calibrated on board at the start and end of the cruise using purified water. At each station, at least 8 L surface water were carefully pumped through the instrument avoiding accumulation of bubbles inside the cuvettes (sample volume ca. 30 mL). Raw spectra were obtained from average values of all spectra for each surface water sample. Absorption and attenuation were corrected for changes in pure water absorption due to temperature and salinity effects using the coefficients by Röttgers et al.45. Absorption spectra were further corrected for scattering errors by applying the proportional correction46 using 870 nm as reference wavelength.

Spectral backscattering coefficients were calculated based on measurements of the volume scattering function at an effective scattering angle of 124° (sample volume ca. 1 mL). Data were recorded inside a black bucket using a BB9 (WET Labs Inc., USA) with a total of 18 kbyte data collected over a period of several minutes. Averaged volume scattering at 124° function data were converted to particulate backscattering coefficient as described in the BB9 manual using χ = 0.944. Spectral backscattering coefficients were determined at 412, 440, 488, 510, 532, 595, 650, 676 and 715 nm, which were subsequently interpolated to the ac-9 wavelengths.

Underwater and water-leaving light fields were simulated using EcoLight (version 5.0, Sequoia Scientific Inc., USA), a well-established radiative transfer model. The model was populated with measured IOPs and set up to generate Fournier-Forand scattering phase functions from derived particulate backscattering ratios47,48. Measured median above surface irradiance and estimated cloud cover percentage were used to parameterise incoming solar irradiation. Modelling of inelastic scattering was restricted to Raman scattering by water. Output was computed at IOP wavelengths to avoid artefacts due to inter- or extrapolation of the data.

The absorption of live copepods was measured in triplicate in the PSICAM between 350 and 800 nm using purified water as reference. A serial addition experiment was performed by sequentially adding seven to eight live Calanus spp. to sea water (Fig. 4a), which had been sieved through a 180 µm mesh to remove other large particles. The PSICAM has been shown to be virtually unaffected by scattering errors29 and is ideally suited to measure absorption of samples containing particulate matter such as Calanus spp. copepods. The PSICAM was calibrated multiple times per day using a Nigrosine solution29,49, and corresponding Nigrosine absorption spectra were measured using a long pathlength system. PSICAM absorption spectra were corrected for temperature and salinity effects using instrument specific correction factors50.

Data Availability

Remote sensing data from VIIRS were provided by the NERC Earth Observation Data Acquisition and Analysis Service. All other data that support the findings of this study are available from the corresponding author upon reasonable request.


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We thank captain and crew of R/V “Helmer Hanssen” and the engineers of UiT. The authors also thank the NERC Earth Observation Data Acquisition and Analysis Service (NEODAAS) for supplying data for this study. We thank three anonymous reviewers for helpful comments. This study is part of the project “Sustainable harvesting of a patchy resource: aggregation mechanisms and implications for stock size estimates (Sea Patches)” that was supported by the Norwegian Research Council (grant number 268391/E40).

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S.B. initiated the research, and together with D.M., S.F.P. and A.G. outlined the study. D.M. and I.L. collected and analysed inherent optical properties, performed the serial addition experiment and analysed the satellite data. M.D., S.F.P. and E.T. collected the zooplankton net samples, which were analysed by E.T. A.G. collected and analysed the video plankton recorder data. SB collected and analysed the laser optical plankton counter data. M.D. and E.T. sorted individual Calanus spp. M.C. performed the molecular analyses. ESE analysed the copepods’ pigments. SB prepared the figures and wrote most of the text. All authors contributed with text and/or comments to the manuscript and approved the final version.

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Correspondence to Sünnje L. Basedow.

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Basedow, S.L., McKee, D., Lefering, I. et al. Remote sensing of zooplankton swarms. Sci Rep 9, 686 (2019).

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