Environmental factors influencing benthic communities in the oxygen minimum zones on the Angolan and Namibian margins
- 1Department of Ocean Systems, NIOZ Royal Netherlands Institute for Sea Research and Utrecht University, Texel, 1797SH, the Netherlands
- 2MARUM–Center for Marine Environmental Sciences, University of Bremen, 28359 Bremen, Germany
- 3GEOMAR Helmholtz Centre for Ocean Research, 24148 Kiel, Germany
- 4Department for Marine Research, Senckenberg Institute, 26382 Wilhelmshaven, Germany
- 5Faculty of Geosciences, Earth Sciences Department, Utrecht University, Utrecht, 3512JE, the Netherlands
Correspondence: Ulrike Hanz (email@example.com)
Thriving benthic communities were observed in the oxygen minimum zones along the southwestern African margin. On the Namibian margin, fossil cold-water coral mounds were overgrown by sponges and bryozoans, while the Angolan margin was characterized by cold-water coral mounds covered by a living coral reef. To explore why benthic communities differ in both areas, present-day environmental conditions were assessed, using conductivity–temperature–depth (CTD) transects and bottom landers to investigate spatial and temporal variations of environmental properties. Near-bottom measurements recorded low dissolved oxygen concentrations on the Namibian margin of 0–0.15 mL L−1 (≜0 %–9 % saturation) and on the Angolan margin of 0.5–1.5 mL L−1 (≜7 %–18 % saturation), which were associated with relatively high temperatures (11.8–13.2 ∘C and 6.4–12.6 ∘C, respectively). Semidiurnal barotropic tides were found to interact with the margin topography producing internal waves. These tidal movements deliver water with more suitable characteristics to the benthic communities from below and above the zone of low oxygen. Concurrently, the delivery of a high quantity and quality of organic matter was observed, being an important food source for the benthic fauna. On the Namibian margin, organic matter originated directly from the surface productive zone, whereas on the Angolan margin the geochemical signature of organic matter suggested an additional mechanism of food supply. A nepheloid layer observed above the cold-water corals may constitute a reservoir of organic matter, facilitating a constant supply of food particles by tidal mixing. Our data suggest that the benthic fauna on the Namibian margin, as well as the cold-water coral communities on the Angolan margin, may compensate for unfavorable conditions of low oxygen levels and high temperatures with enhanced availability of food, while anoxic conditions on the Namibian margin are at present a limiting factor for cold-water coral growth. This study provides an example of how benthic ecosystems cope with such extreme environmental conditions since it is expected that oxygen minimum zones will expand in the future due to anthropogenic activities.
Cold-water corals (CWCs) form 3-D structures in the deep sea, providing important habitats for dense aggregations of sessile and mobile organisms ranging from mega- to macrofauna (Henry and Roberts, 2007; van Soest et al., 2007) and fish (Costello et al., 2005). Consequently, CWC areas are considered as deep-sea hotspots of biomass and biodiversity (Buhl-Mortensen et al., 2010; Henry and Roberts, 2017). Moreover, they form hotspots for carbon cycling by transferring carbon from the water column towards associated benthic organisms (Oevelen et al., 2009; White et al., 2012). Some framework-forming scleractinian species, with Lophelia pertusa and Madrepora oculata being the most common species in the Atlantic Ocean (Freiwald et al., 2004; White et al., 2005; Roberts et al., 2006; Cairns, 2007), are capable of forming large elevated seabed structures, so-called coral mounds (Wilson, 1979; Wienberg and Titschack, 2017; Titschack et al., 2015; De Haas et al., 2009). These coral mounds, consisting of coral debris and hemipelagic sediments, commonly reach heights between 20 and 100 m and can be several kilometers in diameter. They are widely distributed along the North Atlantic margins, being mainly restricted to water depths between 200 and 1000 m, while records of single colonies of L. pertusa are reported from a broader depth range of 50–4000 m depth (Roberts et al., 2006; Hebbeln et al., 2014; Davies et al., 2008; Mortensen et al., 2001; Freiwald et al., 2004; Freiwald, 2002; Grasmueck et al., 2006; Wheeler et al., 2007).
A global ecological-niche factor analysis by Davies et al. (2008) and Davies and Guinotte (2011), predicting suitable habitats for L. pertusa, showed that this species generally thrives in areas which are nutrient rich, well oxygenated and affected by relatively strong bottom water currents. Other factors potentially important for proliferation of L. pertusa include chemical and physical properties of the ambient water masses, for example aragonite saturation state, salinity and temperature (Davies et al., 2008; Dullo et al., 2008; Flögel et al., 2014; Davies and Guinotte, 2011). L. pertusa is most commonly found at temperatures between 4 and 12 ∘C and a very wide salinity range between 32 and 38.8 (Freiwald et al., 2004). The link of L. pertusa to particular salinity and temperature within the NE Atlantic led Dullo et al. (2008) to suggest that they are restricted to a specific density envelope of sigma-theta (σΘ)=27.35–27.65 kg m−3. In addition, the majority of occurrences of live L. pertusa comes from sites with dissolved oxygen (DO) concentrations between 6 and 6.5 mL L−1(Davies et al., 2008), with lowest recorded oxygen values being 2.1–3.2 mL L−1 at CWC sites in the Gulf of Mexico (Davies et al., 2010; Schroeder, 2002; Brooke and Ross, 2014) or even as low as 1–1.5 mL L−1 off Mauritania, where CWC mounds are in a dormant stage presently showing only scarce living coral occurrences (Wienberg et al., 2018; Ramos et al., 2017). Dissolved oxygen levels hence seem to affect the formation of CWC structures as was also shown by Holocene records obtained from the Mediterranean Sea, which revealed periods of reef demise and growth in conjunction with hypoxia (with 2 mL L−1 seemingly forming a threshold value for active coral growth; Fink et al., 2012).
Another essential constraint for CWC growth and therefore mound development in the deep sea is food supply. L. pertusa is an opportunistic feeder, exploiting a wide variety of different food sources, including phytodetritus, phytoplankton, mesozooplankton, bacteria and dissolved organic matter (Kiriakoulakis et al., 2005; Dodds et al., 2009; Gori et al., 2014; Mueller et al., 2014; Duineveld et al., 2007). Not only quantity but also quality of food particles are of crucial importance for the uptake efficiency as well as ecosystem functioning of CWCs (Ruhl, 2008; Mueller et al., 2014). Transport of surface organic matter towards CWC sites at intermediate water depths has been found to involve either active swimming (zooplankton), passive sinking, advection, local downwelling, and internal waves and associated mixing processes resulting from interactions with topography (Davies et al., 2009; van Haren et al., 2014; Thiem et al., 2006; White et al., 2005; Mienis et al., 2009; Frederiksen et al., 1992). With worldwide efforts to map CWC communities, L. pertusa was also found under conditions which are environmentally stressful or extreme in the sense of the global limits defined by Davies et al. (2008) and by Davies and Guinotte (2011). Examples are the warm and salty waters of the Mediterranean and the high bottom water temperatures along the US coast (Cape Lookout; Freiwald et al., 2009; Mienis et al., 2014; Taviani et al., 2005). Environmental stress generally increases energy needs for organisms to recover and maintain optimal functioning, which accordingly increases their food demand (Sokolova et al., 2012).
For the SW African margin one of the few records of living CWC comes from the Angolan margin (at 7∘ S; Le Guilloux et al., 2009), which raises the questions whether environmental factors limit CWC growth due to the presence of an oxygen minimum zone (OMZ; see Karstensen et al. 2008), or whether this is related to a lack of data. Hydroacoustic campaigns revealed extended areas off Angola and Namibia with structures that morphologically resemble coral mound structures known from the NE Atlantic (M76-3, MSM20-1; Geissler et al., 2013; Zabel et al., 2012). Therefore two of such mound areas on the margins off Namibia and Angola were visited during the RV Meteor cruise M122 “ANNA” (ANgola and NAmibia) in January 2016 (Hebbeln et al., 2017). During this cruise, fossil CWC mound structures were found near Namibia, while flourishing CWC reef-covered mound structures were observed on the Angolan margin. The aim of the present study was to assess present-day environmental conditions at the southwestern African margin to explore why CWCs thrive on the Angolan margin and are absent on the Namibian margin. Key parameters influencing CWCs, hydrographic parameters as well as chemical properties of the water column were measured to characterize the difference in environmental conditions and food supply. These data are used to improve understanding of the potential fate of CWC mounds in a changing ocean.
2.1.1 Oceanographic setting
The SW African margin is one of the four major eastern boundary regions in the world and is characterized by upwelling of nutrient-rich cold waters (Shannon and Nelson, 1996). The availability of nutrients triggers a high primary production, making it one of the most productive marine areas worldwide with an estimated production of 0.37 Gt C yr−1 (Carr and Kearns, 2003). Remineralization of high fluxes of organic particles settling through the water column results in severe mid-depth oxygen depletion and an intense OMZ over large areas along the SW African margin (Chapman and Shannon, 1985). The extension of the OMZ is highly dynamic, being controlled by upwelling intensity, which depends on the prevailing winds and two current systems along the SW African margin, i.e., the Benguela and the Angola currents (Kostianoy and Lutjeharms, 1999; Chapman and Shannon, 1987; Fig. 1). The Benguela Current originates from the South Atlantic Current, which mixes with water from the Indian Ocean at the southern tip of Africa (Poole and Tomczak, 1999; Mohrholz et al., 2008; Rae, 2005) and introduces relatively cold and oxygen-rich Eastern South Atlantic Central Water (ESACW; Poole and Tomczak, 1999) to the SW African margin (Mohrholz et al., 2014). The Angola Current originates from the South Equatorial Counter Current and introduces warmer, nutrient-poor and less oxygenated South Atlantic Central Water (SACW; Poole and Tomczak, 1999) to the continental margin (Fig. 1a). SACW is defined by a linear relationship between temperature and salinity in a T–S plot (Shannon et al., 1987). While the SACW flows along the continental margin the oxygen concentration is decreasing continuously due to remineralization processes of organic matter on the SW African shelf (Mohrholz et al., 2008). Both currents converge at around 14–16∘ S, resulting in the Angola–Benguela front (Lutjeharms and Stockton, 1987). In austral summer, the Angola–Benguela front can move southward to 23∘ S (Shannon et al., 1986), thus increasing the influence of the SACW along the Namibian coast (Junker et al., 2017; Chapman and Shannon, 1987), contributing to the pronounced OMZ due to its low initial oxygen concentration (Poole and Tomczak, 1999). ESACW is the dominant water mass at the Namibian margin during the main upwelling season in austral winter, expanding from the oceanic zone about 350 km towards the coast (Mohrholz et al., 2014). The surface water mass at the Namibian margin is a mixture of sun-warmed upwelled water and water of the Agulhas Current, which mixes in complex eddies and filaments and is called South Atlantic Subtropical Surface Water (SASSW) (Hutchings et al., 2009). At the Angolan margin the surface water is additionally influenced by water from the Cuanza and Congo rivers (Kopte et al., 2017, Fig. 1). Antarctic Intermediate Water (AAIW) is situated in deeper areas at the African continental margin and can be identified as the freshest water mass around 700–800 m depth (Shannon and Nelson, 1996).
2.1.2 Coral mounds along the Angolan and Namibian margins
During RV Meteor cruise M122 in 2016, over 2000 coral mounds were observed between 160 and 260 m water depth on the Namibian shelf (Hebbeln et al., 2017). All mounds were densely covered with coral rubble and dead coral framework, while no living corals were observed in the study area (Hebbeln et al., 2017; Fig. 2a, b). Few species were locally very abundant, viz. a yellow cheilostome bryozoan which was the most common species, and five sponge species. The bryozoans were encrusting the coral rubble, whereas some sponge species reached heights of up to 30 cm (Fig. 2a, b). The remaining community consisted of an impoverished fauna overgrowing L. pertusa debris. Commonly found sessile organism were actiniarians, zoanthids, hydroids, some thin encrusting sponges, serpulids and sabellid polychaetes. The mobile fauna comprised asteroids, ophiuroids, two shrimp species, amphipods, cumaceans and holothurians. Locally high abundances of Suffogobius bibarbatus, a fish that is known to be adapted to hypoxic conditions, were observed in cavities in the coral framework (Hebbeln, 2017). Dead corals collected from the surface of various Namibian mounds date back to about 5 ka pointing to a simultaneous demise of these mounds during the mid-Holocene (Tamborrino et al., 2019).
On the Angolan margin CWC structures varied from individual mounds to long ridges. Some mounds reached heights of more than 100 m above the seafloor. At shallow depths (∼250 m) some isolated smaller mounds were also present (Hebbeln et al. 2017). All mounds showed a thriving CWC cover, which was dominated by L. pertusa (estimated 99 % relative abundance), along with some M. oculata and solitary corals. Mounds with a flourishing coral cover were mainly situated at water depths between 330 and 470 m, whereas single colonies were found over a broader depth range between 250 and 500 m (Fig. 2c, d; Hebbeln et al., 2017). Additionally, large aggregations of hexactinellid sponges (Aphrocallistes, Sympagella) were observed. First estimates for coral ages obtained from a gravity core collected at one of the Angolan coral mounds revealed continuous coral mound formation during the last 34 kyr until today (Wefing et al., 2017).
During RV Meteor expedition M122 in January 2016, two conductivity–temperature–depth (CTD) transects and three short-term bottom lander deployments (Table 1, Fig. 1) were carried out to measure environmental conditions influencing benthic habitats. In addition, weather data were continuously recorded by the RV Meteor weather station, providing real-time information on local wind speed and wind direction.
2.2.1 Lander deployments
Sites for deployment of the NIOZ-designed lander (ALBEX) were selected based on multibeam bathymetric data. On the Namibian margin the bottom lander was deployed on top of a mound structure (water depth 220 m). Off Angola the lander was deployed in the relatively shallow part of the mound zone at 340 m water depth and in the deeper part at 530 m (Fig. 1, Table 1). Additionally, a GEOMAR satellite lander module (SLM) was deployed off-mound at 230 m depth at the Namibian margin and at 430 m depth at the Angolan margin (Fig. 1, Table 1). The lander was equipped with an ARO-USB oxygen sensor (JFE Advantech™), a combined OBS-fluorometer (Wet Labs™) and an Aquadopp (Nortek™) profiling current meter. The lander was furthermore equipped with a Technicap PPS4/3 sediment trap with 12 bottles (allowing daily samples) and a McLane particle pump (24 filter units for each 7.5 L of seawater, 2 h interval) to sample particulate organic matter in the near-bottom water (40 cm above bottom).
The SLM was equipped with a 600 kHz ADCP Workhorse Sentinel 600 from RDI, a CTD (SBE SBE16V2™), a combined fluorescence and turbidity sensor (WET Labs ECO-AFL/FL), a dissolved oxygen sensor (SBE™) and a pH sensor (SBE™) (Hebbeln et al., 2017). From the SLM only pH measurements are used here, complementing the data from the NIOZ lander.
2.2.2 CTD transects
Vertical profiles of hydrographic parameters in the water column, viz. temperature, conductivity, oxygen and turbidity, were obtained using a Sea-Bird CTD–Rosette system (Sea-Bird SBE 9 plus). The additional sensors on the CTD were a dissolved oxygen sensor (SBE 43 membrane-type DO Sensor) and a combined fluorescence and turbidity sensor (WET Labs ECO-AFL/FL). The CTD was combined with a rosette water sampler consisting of 24 Niskin® water sampling bottles (10 L). CTD casts were carried out along two downslope CTD transects (Fig. 1). Owing to technical problems turbidity data were only collected on the Angolan slope.
2.2.3 Hydrographic data processing
The CTD data were processed using the processing software Sea-Bird data SBE 11plus V 5.2 and were visualized using the program Ocean Data View (Schlitzer, 2011; Version 4.7.8).
Hydrographic data recorded by the landers were analyzed and plotted using the program R (R Core Team, 2017). Data from the different instruments (temperature, turbidity, current speed, oxygen concentration, fluorescence) were averaged over a period of 1.5 h to remove shorter-term trends and occasional spikes. Correlations between variables were assessed by Spearman's rank correlation tests.
2.2.4 Suspended particulate matter
Near-bottom suspended particulate organic matter (SPOM) was sampled by means of a phytoplankton sampler (McLane PPS) mounted on the ALBEX lander. The PPS was fitted with 24 GF/F filters (47 mm Whatman™ GF/F filters pre-combusted at 450 ∘C). A maximum of 7.5 L was pumped over each filter during a 2 h period, yielding a time series of near-bottom SPOM supply and its variability over a period of 48 h.
C / N analysis and isotope measurements
Filters from the phytoplankton sampler were freeze-dried before further analysis. Half of each filter was used for phytopigment analysis and a 1∕4 section of each filter was used for analyzing organic carbon, nitrogen and their stable isotope ratios. The filters used for carbon analysis were decarbonized by vapor of concentrated hydrochloric acid (2 M HCl supra) prior to analyses. Filters were transferred into pressed tin capsules (12 mm×5 mm, Elemental Microanalysis), and δ15N, δ13C and total weight percent of organic carbon and nitrogen were analyzed by a Delta V Advantage isotope ratio MS coupled online to an Elemental Analyzer (Flash 2000 EA-IRMS) by a ConFlo IV (Thermo Fisher Scientific Inc.). The reference gas was purified atmospheric N2. As standards for δ13C benzoic acid and acetanilide were used, for δ15N acetanilide, urea and casein were used. For δ13C analysis a high-signal method was used including a 70 % dilution. Values are reported relative to v-pdb and the atmosphere respectively. Precision and accuracy based on replicate analyses and comparison with international standards for δ13C and δ15N was ±0.15 ‰. The C∕N ratio is based on the weight ratios between total organic carbon (TOC) and N.
Phytopigments were measured by reverse-phase high-performance liquid chromatography (RP-HPLC, Waters Acquity UPLC) with a gradient based on the method published by Kraay et al. (1992). For each sample half of a GF/F filter was used and freeze-dried before extraction. Pigments were extracted using 95 % methanol and sonification. All steps were performed in a dark and cooled environment. Pigments were identified by means of their absorption spectrum, fluorescence and the elution time. Identification and quantification took place as described by Tahey et al. (1994). The absorbance peak areas of chlorophyll a were converted into concentrations using conversion factors determined with a certified standard. The ∑phaeopigment ∕ chlorophyll a ratio gives an indication of the degradation status of the organic material, since phaeopigments form as a result of bacterial or autolytic cell lysis and grazing activity (Welschmeyer and Lorenzen, 1985).
2.2.5 Tidal analysis
The barotropic (due to the sea level and pressure change) and baroclinic (internal “free waves” propagating along the pycnoclines) tidal signals obtained by the Aquadopp (Nortek™) profiling current meter were analyzed from the bottom pressure and from the horizontal flow components recorded 6 m above the sea floor, using the T_Tide Harmonic Analysis Toolbox (Pawlowicz et al., 2002). The data mean and trends were subtracted from the data before analysis.
3.1 Water column properties
3.1.1 Namibian margin
The hydrographic data obtained by CTD measurements along a downslope transect from the surface to 1000 m water depth revealed distinct changes in temperature and salinity throughout the water column. These are ascribed to the different water masses in the study area (Fig. 3a). In the upper 85 m of the water column, temperatures were above 14 ∘C and salinities > 35.2, which correspond to South Atlantic Subtropical Surface Water (SASSW). SACW was situated underneath the SASSW and reaches down to about 700 m, characterized by a temperature from 14 to 7 ∘C and a salinity from 35.4 to 34.5 (Fig. 3a). A deep CTD cast about 130 km from the coastline recorded a water mass with the signature of ESACW, having a lower temperature (Δ1.3 ∘C) and lower salinity (Δ0.2) than SACW (in 200 m depth, not included in CTD transects of Fig. 4). Underneath these two central water masses Antarctic Intermediate Water (AAIW) was found with a temperature < 7 ∘C.
The CTD transect showed decreasing DO (dissolved oxygen) concentration from the surface (6 mL L−1) towards a minimum in 150 to 200 m depth (0 mL L−1). Lowest values for DO concentrations were found on the continental margin between 100 and 335 m water depth. The DO concentrations in this pronounced OMZ ranged from < 1 mL L−1 down to 0 mL L−1 (≜9 % to 0 % saturation). The zone of low DO concentrations (< 1 mL L−1) stretched horizontally over the complete transect from about 50 km to at least 100 km offshore (Fig. 4c). The upper boundary of the OMZ was relatively sharp compared to its lower limits and corresponded with the border between SASSW at the surface and SACW below.
Within the OMZ, a small increase in fluorescence (0.2 mg m−3) was recorded, whereas fluorescence was otherwise not traceable below the surface layer (Fig. 4d). Within the surface layer, highest surface fluorescence (> 2 mg m−3) was found ∼40 km offshore. Above the center of the OMZ fluorescence reached only 0.4 mg m−3.
3.1.2 Angolan margin
The hydrographic data obtained by CTD measurements along a downslope transect from the surface to 800 m water depth revealed distinct changes in temperature and salinity throughout the water column, related to four different water masses. At the surface a distinct shallow layer (> 20 m) with a distinctly lower salinity (27.3–35.5) and higher temperature (29.5–27 ∘C, Fig. 3b) was observed. Below the surface layer, SASSW was found down to a depth of 70 m, characterized by a higher salinity (35.8). SACW was observed between 70 and 600 m, showing the expected linear relationship between temperature and salinity. Temperature and salinity decreased from 17.5 ∘C and 35.8 to 7 ∘C and 34.6. At 700 m depth AAIW was recorded, characterized by a low salinity (< 34.4) and temperature (< 7 ∘C, Fig. 3b).
The CTD transect showed a sharp decrease in the DO concentrations underneath the SASSW from 5 to < 2 mL L−1 (Fig. 5). DO concentrations decreased further to a minimum of 0.6 mL L−1 at 350 m and then increased to > 3 mL L−1 at 800 m depth. Lowest DO concentrations were not found at the slope but 70 km offshore in the center of the zone of reduced DO concentrations between 200 and 450 m water depth (< 1 mL L−1). Compared to the Namibian margin (see Fig. 4), the hypoxic layer was situated further offshore, slightly deeper, and overall DO concentrations were higher (compare Fig. 4c). Also, the boundaries of the hypoxic zone were not as sharp. Fluorescence near the sea surface was generally low (around 0.2 with small maxima of 0.78 mg m−3) and not detectable deeper than 150 m depth. A distinct zone of enhanced turbidity was observed on the continental margin between 200 and 350 m water depth.
3.2 Near-bottom environmental data
3.2.1 Namibian margin
Bottom temperature ranged from 11.8 to 13.2 ∘C during the deployment of the ALBEX lander (Table 2, Fig. 6), showing oscillating fluctuations with a maximum semidiurnal (ΔT∼6 h) change of ∼Δ1 ∘C (on 9 January 2016). The DO concentrations fluctuated between 0 and 0.15 mL L−1 and were negatively correlated with temperature (, p<0.01). Fluorescence ranged from 42 to 45 NTU during the deployment and was positively correlated with temperature (r=0.38, p<0.01). Hence, both temperature and fluorescence were negatively correlated with DO concentrations (, p<0.01) and turbidity (optical backscatter, , p<0.01). Turbidity was low until it increased markedly during the second half of the deployment. During this period on the 6 January, wind speed increased from 10 m s−1 to a maximum of 17 m s−1 and remained high for the next 6 . The wind direction changed from counterclockwise cyclonic rotation towards alongshore winds. During the strong wind period, colder water (correlation between wind speed and water temperature, , p<0.01) with a higher turbidity (correlation of wind speed and turbidity, r=0.42, p<0.01) and on average higher DO concentrations was present. The SLM lander recorded an average pH of 8.01.
Maximum current speeds measured during the deployment period were 0.21 m s−1, with average current speeds of 0.09 m s−1 (Table 2). The tidal cycle explained > 80 % of the pressure fluctuations (Table 3), with a semidiurnal signal, M2 (principal lunar semidiurnal), generating an amplitude of > 0.35 dbar and thus being the most important constituent. Before the 6 January, the current direction oscillated between SW and SE after which it changed to a dominant northerly current direction (Fig. 6).
The observed fluctuations in bottom water temperature at the deployment site imply a vertical tidal movement of around 70 m. This was estimated by comparing the temperature change recorded by the lander to the respective temperature–depth gradient based on water column measurements (CTD site GeoB20553, 12.58 ∘C at 245 m, 12.93 ∘C at 179 m). Due to these vertical tidal movements, the oxygen-depleted water from the core of the OMZ is regularly being replaced with somewhat colder and slightly more oxygenated water (Δ up to 0.2 mL L−1).
3.2.2 Angolan margin
Mean bottom water temperatures were 6.73 ∘C at the deeper site (530 m) and 10.06 ∘C at the shallower site (340 m, Fig. 7, Table 2). The maximum semidiurnal (ΔT∼6 h) temperature change was Δ1.60 ∘C at the deepest site and Δ2.4 ∘C at the shallow site (Fig. 7). DO concentrations at the deep site were a factor of 2 higher than those at the shallow site, i.e., 0.9–1.5 vs. 0.5–0.8 mL L−1 respectively (≜ range between 4 % and 14 % saturation of both sites), whereas the range of diurnal fluctuations was much smaller compared to the shallow site. DO concentrations were negatively correlated with temperature at the deep site (, p<0.01), while positively correlated at the shallow site (r=0.91, p<0.01). Fluorescence was low during both deployments and showed only small fluctuations, being slightly higher at the shallow site (between 38.5 and 41.5 NTU at both sites). Current speeds were relatively high (between 0 and 0.3 m s−1, average 0.1 m s−1) and positively correlated with temperature at the shallow site (r=0.31, p<0.01) and negatively correlated at the deep site (, p<0.01). Analysis of the tidal cycle showed that it explained 29.8 %–54.9 % of the horizontal current fluctuations. The M2 amplitude was 0.06–0.09 s−1 and was the most important signal (Table 3). A decrease in turbidity was observed during the deployment at the shallow station. This station was located directly below the turbidity maximum between 200 and 350 m depth as observed in the CTD transect (Fig. 5). In contrast, a relative constant and low turbidity was observed for the deep deployment. Turbidity during both deployments was positively correlated to DO concentrations (r=0.47, p<0.01, shallow deployment and r=0.50, p<0.01, deep deployment). The SLM lander recorded an average pH of 8.12.
The short-term temperature fluctuations imply a vertical tidal movement of around 130 m (12.9–9.1 ∘C measured by lander, ≜218–349 m depth in CTD above lander at station GeoB20966).
3.3 Suspended particulate matter
3.3.1 Namibian margin
The nitrogen (N) concentration of the SPOM measured on the filters of the McLane pump fluctuated between 0.25 and 0.45 mg L−1(Fig. 8). The highest N concentration corresponded with a peak in turbidity (r=0.42, p<0.01). The δ15N values of the lander time series fluctuated between 5.1 and 6.9 with an average value of 5.7 ‰. Total organic carbon (TOC) showed a similar pattern as nitrogen, with relative concentrations ranging between 1.8 and 3.5 mg L−1. The δ13C value of the TOC increased during the surveyed time period from −22.39 ‰ to −21.24 ‰ with an average of −21.7 ‰ (Fig. 8a). The C∕N ratio ranged from 8.5–6.8 and was on average 7.4 (Fig. 8b). During periods of low temperature and more turbid conditions TOC and N as well as the δ13C values of the SPOM were higher.
Chlorophyll a concentrations of SPOM were on average 0.042 µg L−1 and correlated with the record of the fluorescence (r=0.43, p=0.04). A 6 times higher amount of chlorophyll a degradation products was found during the lander deployment (0.248 µg L−1) compared to the amount of chlorophyll a, giving a ∑phaeopigment ∕ chlorophyll a ratio of 6.5 (not shown). Additionally, carotenoids (0.08–0.12 µg L−1) and fucoxanthin (0.22 µg L−1), which are common in diatoms, were major components of the pigment fraction. Zeaxanthin, indicating the presence of prokaryotic cyanobacteria, was only observed in small quantities (0.066 µg L−1).
3.3.2 Angolan margin
In general TOC and N concentrations of SPOM were higher at the shallow site compared to the deep site. Nitrogen concentrations varied around 0.14 mg L−1 at 340 m and around 0.1 mg L−1 at 530 m depth (Fig. 8b). The δ15N values at the shallow site ranged from 1.6 ‰ to 6.2 ‰ (3.7 ‰ average) and were even lower deeper in the water column, viz. range 0.3–3.7 ‰ with an average of 1.4 ‰. The TOC concentrations were on average 1.43 mg L−1 at 340 m and 0.9 mg L−1 at 530 m, with corresponding δ13C values ranging between −23.0 and −24.2 (average of −23.6 ‰) at the shallow, and between −22.9 and −23.9 (average −23.4 ‰) at the deep site.
The chlorophyll a concentrations of the SPOM collected by the McLane pump varied between 0.1 and 0.02 µg L−1, with average ∑phaeopigment ∕ chlorophyll a ratios of 2.6 and 0.5 at the shallow and deep sites, respectively. Phytopigments recorded by the shallow deployment included 0.3 µg L−1 of fucoxanthin, while at the deep site only a concentration of 0.1 µg L−1 was found. No zeaxanthin was recorded in the pigment fraction.
Even though the ecological-niche factor analyses of Davies et al. (2008) and Davies and Guinotte (2011) predict L. pertusa to be absent along the oxygen-limited southwestern African margin, CWC mounds with two distinct benthic ecosystems were found. The coral mounds on the Namibian shelf host no living CWCs; instead the dead coral framework covering the mounds was overgrown with fauna dominated by bryozoans and sponges. Along the slope of the Angolan margin an extended coral mound area with thriving CWC communities was encountered. It is probably that differences in present-day environmental conditions between the areas influence the faunal assemblages inhabiting them. The potential impact of the key environmental factors will be discussed below.
4.1 Short-term vs. long-term variations in environmental properties
On the Namibian margin, seasonality has a major impact on local mid-depth oxygen concentration due to the periodically varying influence of the Angola current and its associated low DO concentrations (Chapman and Shannon, 1987). The lowest DO concentration is expected from February to May when SACW is the dominating water mass on the Namibian margin and the contribution of ESACW is smaller (Mohrholz et al., 2008). Due to this seasonal pattern, the DO concentrations measured in this study (January; Fig. 4) probably do not represent minimum concentrations, which are expected to occur in the following months, but nevertheless give a valuable impression about the extent of the OMZ (February to May; Mohrholz et al., 2014). Interestingly, we captured a flow reversal after 6 January from a southward to an equatorward current direction during high wind conditions on the Namibian margin (Fig. 6), leading to an intrusion of ESACW with higher DO concentrations (Δ 0.007 mL L−1 on average) and lower temperatures (Δ 0.23 ∘C on average, Fig. 5) than the SACW. This led to a temporal increase in the DO concentrations. This shows that variations in the local flow field have the capability to change water properties on relatively short time scales, which might provide an analogue to the water mass variability related to the different seasons (Mohrholz et al., 2008). Such relaxations are possibly important for the survival of the abundant benthic fauna present on the relict coral mounds (Gibson et al., 2003). Other seasonal changes, like riverine outflow, do not have decisive impacts on the ecosystem since only relatively small rivers discharge from the Namibian margin. This is also reflected by the dominant marine isotopic signature of the isotopic ratios of δ15N and δ13C of the SPOM at the mound areas (Fig. 8, cf. Tyrrell and Lucas, 2002).
Flow reversals were not observed during the lander deployments on the Angolan margin, where winds are reported to be weak throughout the year providing more stable conditions (Shannon, 2001). Instead river outflow seems to exert a strong influence on the DO concentrations on the Angolan margin. The runoff of the Cuanza and Congo river reach their seasonal maximum in December and January (Kopte et al., 2017), intensifying upper water column stratification. This stratification is restricting vertical mixing and thereby limits ventilation of the oxygen-depleted subsurface water masses. In addition rivers transport terrestrial organic matter to the margin, which is reflected by the isotopic signals of the SPOM (−1 ‰ to 3 ‰; Montoya, 2007) which is well below the average isotopic ratio of the marine waters of 5.5 ‰ (Meisel et al., 2011). Also δ13C values are in line with the δ13C values of terrestrial matter which is on average −27 ‰ in this area (Boutton, 1991; Mariotti et al., 1991). The C∕N ratio of SPOM is higher compared to material from the Namibian margin, also confirming admixing of terrestrial matter (Perdue and Koprivnjak, 2007). This terrestrial matter contains suitable food sources as well as less suitable food sources, like carbon-rich polymeric material (cellulose, hemicellulose and lignin), which cannot easily be taken up by marine organisms (Hedges and Oades, 1997). The combined effects of decreased vertical mixing and additional input of organic matter potentially result in the lowest DO concentrations of the year during the investigated time period (January), since the highest river outflow and therefore strongest stratification is expected during this period.
4.2 Main stressors – oxygen and temperature
Environmental conditions marked by severe hypoxia and temporal anoxia (< 0.17 mL L−1) likely explain the present-day absence of living CWCs along the Namibian margin. During the measurement period the DO concentrations off Namibia were considerably lower than the thus far recorded minimum concentrations near living CWCs (1–1.3 mL L−1), which were found off Mauritania where only isolated living CWCs are found (Ramos et al., 2017). Age dating of the Namibian fossil coral framework showed that CWCs disappeared about 5 ka which coincides with an intensification in upwelling and therefore most likely a decline of DO concentrations (Tamborrino et al., 2019), supporting the assumption that the low DO concentrations are responsible for the demise of CWCs on the Namibian margin. Although no living corals were observed on the Namibian coral mounds, we observed a dense living community dominated by sponges and bryozoans (Hebbeln et al., 2017). Several sponge species have been reported to survive at extremely low DO concentrations within OMZs. For instance, along the lower boundary of the Peruvian OMZ, sponges were found at DO concentrations as low as 0.06–0.18 mL L−1 (Mosch et al., 2012). Mills et al. (2018) recently found a sponge (Tethya wilhelma) to be physiologically almost insensitive to oxygen stress and respires aerobically under low DO concentrations (0.02 mL L−1). Sponges can potentially stop their metabolic activity during unfavorable conditions and restart their metabolism when some oxygen becomes available, for instance during diurnal irrigation of water with somewhat higher DO concentrations. The existence of a living sponge community off Namibia might therefore be explained by the diurnal tides occasionally flushing the sponges with more oxic water, enabling them to metabolize, when food availability is highest (Fig. 6). Increased biomass and abundances in these temporary hypoxic–anoxic transition zones were already observed for macro- and megafauna in other OMZs and is referred to as the “edge effect” (Mullins et al., 1985; Levin et al., 1991; Sanders, 1969). It is very likely that this mechanism plays a role for the benthic communities on the Namibian as well as the Angolan margin.
Along the Angolan margin, low oxygen concentrations apparently do not restrict the proliferation of thriving CWC reefs even though DO concentrations are considered hypoxic (0.5–1.5 mL L−1). The DO concentrations measured off Angola are well below the lower DO concentration limits for L. pertusa based on laboratory experiments and earlier field observations (Schroeder, 2002; Brooke and Ross, 2014). The DO concentrations encountered at the shallow mound sites (< 0.8 mL L−1) are even below the so far lowest limits known for single CWC colonies from the Mauritanian margin (Ramos et al., 2017b). Since in the present study measured DO concentrations were even lower than the earlier established lower limits, this could suggest a much higher tolerance of L. pertusa to oxygen levels as low as 0.5 mL L−1at least in a limited time period (4 % O2 saturation).
In addition to oxygen stress, heat stress is expected to put additional pressure on CWCs. Temperatures at the CWC mounds off Angola ranged from 6.4 to 12.6∘C, with the upper limit being close to reported maximum temperatures (∼12–14.9 ∘C; Davies and Guinotte 2011) and are hence expected to impair the ability of CWCs to form mounds (see Wienberg and Titschack 2017). The CWCs were also occurring outside of the expected density envelope of 27.35–27.65 kg m−3in densities well below 27 kg m−3 (Fig. 3, Dullo et al., 2008). In most aquatic invertebrates, respiration rates roughly double with every 10 ∘C increase (Q10 temperature coefficient = 2–3, e.g., Coma, 2002), which at the same time doubles energy demand. Dodds et al. (2007) found a doubling of the respiration rate of L. pertusa with an increase at ambient temperature of only 2 ∘C (viz. Q10=7–8). This would limit the survival of L. pertusa at high temperatures to areas where the increased demand in energy (due to increased respiration) can be compensated by high food availability. Higher respiration rates also imply that enough oxygen needs to be available for the increased respiration. However this creates a negative feedback, since with increased food availability and higher temperatures the oxygen concentration will decrease due to bacterial decomposition of organic substances.
Survival of L. pertusa under hypoxic conditions along the shallow Angolan CWC areas is probably positively influenced by the fact that periods of highest temperatures coincide with highest DO concentrations during the tidal cycle. Probably here the increase of one stressor is compensated by a reduction of another stressor. On the Namibian margin and the deeper Angolan mound sites the opposite pattern was found, with highest temperatures during lowest DO concentrations. However, at the deeper Angolan mound sites DO concentrations are higher and temperatures more within a suitable range compared to the shallow sites (0.9–1.5 mL L−1, 6.4–8 ∘C, Fig. 7). Additionally it was shown by ex situ experiments that L. pertusa is able to survive periods of hypoxic conditions similar to those found along the Angolan margin for several days, which could be crucial in periods of most adverse conditions (Dodds et al., 2007).
4.3 Food supply
As mentioned above, environmental stresses like high temperature or low DO concentration result in a loss of energy (Odum, 1971; Sokolova et al., 2012), which needs to be balanced by an increased energy (food) availability. Food availability therefore plays a significant role for faunal abundance under hypoxia or unfavorable temperatures (Diaz and Rosenberg, 1995). Above, we argued that survival of sponges and bryozoans on the relict mounds off Namibia and of CWCs, and their associated fauna at the Angolan margin, may be partly due to a high input of high-quality organic matter, compensating oxygen and thermal stresses. The importance of the food availability for CWCs was already suggested by Eisele et al. (2011), who mechanistically linked CWC mound growth periods with enhanced surface water productivity and hence organic matter supply. Here we found evidence for high quality and quantity of SPOM in both areas indicated by high TOC and N concentrations (Figs. 6 and 7) in combination with a low C∕N ratio (Fig. 8), a low isotopic signature of δ15N and only slightly degraded pigments.
The Namibian margin is known for its upwelling cells, where phytoplankton growth is fueled by nutrients from deeper water layers producing high amounts of phytodetritus (Chapman and Shannon, 1985), which subsequently sinks down to the relict mounds on the slope. Benthic communities on the mounds off Namibia occur at relatively shallow depths, hence downward transport of SPOM from the surface waters is rapid and time for decomposition of the sinking particles in the water column is limited. The higher turbidity during lower current speeds provides additional evidence that the material settling from the surface is not transported away with the strong currents (Fig. 6).
At the Angolan coral mounds, SPOM appeared to have a signature corresponding to higher quality organic matter compared to the SPOM off Namibia. The phytopigments were less degraded and the δ15N, TOC and N concentrations of the SPOM were lower. However, here lower δ15N and a higher ∑phaeopigment ∕ chlorophyll a ratio are likely connected to a mixture with terrestrial OM input, which might constitute a less suitable food source for CWCs (Hedges and Oades, 1997). On the other hand, the riverine input delivers dissolved nutrients, which can support the growth of phytoplankton, indirectly influencing food supply (Kiriakoulakis et al., 2007; Mienis et al., 2012). Moreover, the variations in food quality at the shallow Angolan reefs, which were relatively small during this study, did not seem to be related to the presence of other environmental stressors. At the Angolan margin we see a rather constant availability of SPOM. The slightly higher turbidity during periods of highest DO concentrations (Fig. 7) suggests that the SPOM on the Angolan margin originates from the bottom nepheloid layer on the margin directly above the CWC mounds (Fig. 5e), which may represent a constant reservoir of fresh SPOM. This reservoir is probably fueled by directly sinking as well as advected organic matter from the surface ocean.
4.4 Tidal currents
The semidiurnal tidal currents observed probably play a major role in the survival of benthic fauna on the SW African margin. On the Namibian margin, internal waves deliver oxygen from the surface and deeper waters to the OMZ and thereby enable benthic fauna on the fossil coral framework to survive in hypoxic conditions (Fig. 9a). At the same time these currents are probably responsible for the delivery of fresh SPOM from the surface productive zone to the communities on the margin, since they promote mixing between the water masses as well as they vertically displace the different water layers.
On the Angolan margin, internal tides produce slightly faster currents and vertical excursions of up to 130 m which are twice as high as those on the Namibian margin. Similar to the Namibian margin, these tidal excursions deliver oxygen from shallower and deeper waters to the mound zone and thereby deliver water with more suitable characteristics over the whole extent of the parts of the OMZ which otherwise may be unsuitable for CWCs (Fig. 9b). Internal tides are also responsible for the formation of a bottom nepheloid layer at 200–350 m depth (Fig. 5e). This layer is formed by trapping of organic matter as well as bottom erosion due to turbulence created by the interaction of internal waves with the margin topography, which intensifies near-bottom water movements. These internal waves are able to move on the density gradient between water masses, which are located at 225 and 300 m depth (Fig. 3). Tidal waves will be amplified due to a critical match between the characteristic slope of the internal M2 tide and the bottom slope of the Angolan margin, as is known from other continental slope regions (Dickson and McCave, 1986; Mienis et al., 2007). As argued above, this turbid layer is likely important for the nutrition of the slightly deeper situated CWC mounds, since vertical mixing is otherwise hindered by the strong stratification.
Different environmental properties explain the present conditions of the benthic communities on the southwestern African margin including temperature, DO concentration, food supply and tidal movements. The DO concentrations probably define the limits of a suitable habitat for CWCs along the Namibian and the Angolan margin, whereas high temperatures constitute additional stress by increasing the respiration rate and therefore energy demand. On the Namibian margin, where DO concentrations dropped below 0.01 mL L−1, only fossil CWC mounds covered by a community dominated by sponges and bryozoans were found. This benthic community survives as it receives periodically waters with slightly higher DO concentrations (> 0.03 mL L−1) due to regular tidal oscillations (semidiurnal) and erratic wind events (seasonal). At the same time, a high quality and quantity of SPOM sinking down from the surface water mass enables the epifaunal community to survive despite the oxygen stress and to sustain its metabolic energy demand at the Namibian OMZ, while CWCs are not capable to withstand such extreme conditions. In contrast, thriving CWCs on the Angolan coral mounds were encountered despite the overall hypoxic conditions. The DO concentrations were slightly higher than those on the Namibian margin but nevertheless below the lowest threshold that was so far reported for L. pertusa (Ramos et al., 2017; Davies et al., 2008, 2010). In combination with temperatures close to the upper limits for L. pertusa, metabolic energy demand probably reached a maximum. High energy requirements might have been compensated by the general high availability of fresh resuspended SPOM. Fresh SPOM accumulates on the Angolan margin just above the CWC area and is regularly supplied due to mixing by semidiurnal tidal currents, despite the restricted sinking of SPOM from the surface due to the strong stratification.
CWC and sponge communities are known to play an important role as a refuge, feeding ground and nursery for commercial fishes (Miller et al., 2012), and have a crucial role in the marine benthic pelagic coupling (Cathalot et al., 2015). Their ecosystem services are threatened by the expected expansion of OMZs due to anthropogenic activities like rising nutrient loads and climate change (Breitburg et al., 2018). This study showed that benthic fauna is able to cope with low oxygen levels as long as sufficient high-quality food is available. Further, reef-associated sponge grounds, as encountered on the Namibian margin could play a crucial role in taking over the function of CWCs in marine carbon cycling as well as in providing a habitat for associated fauna, when conditions become unsuitable for CWCs.
UH analyzed the physical and chemical data, wrote the paper and prepared the figures with contributions from all authors. FM, GD and ML designed the lander research. DH and CW led the cruise and wrote the initial cruise plan. FM and ML collected the data during the research cruise. WCD was responsible for water column measurements with the CTD. AF and ML provided habitat characteristics, including species identification of both CWC areas. KJ performed the tidal analysis and provided together with SF data from the SML lander. All authors contributed to the data interpretation and discussion of the paper.
The authors declare that they have no conflict of interest.
We thank the captain of the RV Meteor cruise M122, Rainer Hammacher, his officers and crew, who contributed to the success of this cruise. We also would like to thank the scientific and technical staff for their assistance during the cruise and their work in the laboratory. Greatly acknowledged are the efforts from the German Diplomatic Corps in the German embassies in Windhoek and Luanda and in the Foreign Office in Berlin. We thank the German Science Foundation (DFG) for providing ship time on RV Meteor and for funding the ROV Squid operations to investigate the cold-water coral ecosystems off Angola and Namibia.
This research has been supported by the DFG Research Center/Cluster of Excellence “MARUM – The Ocean in the Earth System”. Ulrike Hanz is funded by the SponGES project, which received funding from the European Union's Horizon 2020 research and innovation program (grant no. 679849). Furu Mienis is supported by the Innovational Research Incentives Scheme of the Netherlands Organisation for Scientific Research (NWO-VIDI grant no. 016.161.360). Gert-Jan Reichart is supported by the Netherlands Earth System Science Centre (NESSC), financially supported by the Ministry of Education, Culture and Science (OCW). Katriina Juva is funded through the FATE project (Fate of cold-water coral reefs – identifying drivers of ecosystem change), supported by the Norwegian Research Council (NRC).
This paper was edited by Stefano Ciavatta and reviewed by two anonymous referees.
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