Phytoplankton dynamics and sedimentation processes during spring and summer in Balsfjord,Northern Norway

Summary Chlorophyll a, phytoplankton species composition and carbon (PPC) estimated from cell-counts, were monitored together with hydrographic parameters and nutrients in the upper 50 m of Balsfjord (ca. 70° N), northern Norway between 08 February and 29 June 1982. Sediment traps were placed at 10, 50, 100, and 170 m (10 m above bottom) for intervals of 5–20 days during the study period. Trap contents were analyzed for phytoplankton as above; dry weight, particulate organic material (POM), particulate organic nitrogen and carbon (PON and POC), ash, and particulate phosphorus were also measured. The phytoplankton community exhibited three main phases: During the first (02–15 April, chiefly surface biomass) and the second (20 April–10 May, deep biomass-maximum and spring bloom peak) periods, Phaeocystis pouchetii dominated biomass (ca. 50% of PPC) followed by vegetative cells of Chaetoceros socialis. In the third period (10 May onwards, characterized by surface estuarinecir-culation), dino- and microflagellates dominated the low post-bloom biomass. Protozooplankton comprising tintinnids, other ciliates and heterotrophic dinoflagellates increased in abundance. Vegetative cells of phytoplankton were scarce in trap collections at 50 m or below; resting cells of Chaetoceros comprised nearly all the intact sedimenting phytoplankton. Krill faeces accounted for >90% by volume of the total faecal material trapped, despite a >21 biomass dominance of copepods in the fjord. The greatest sedimentation rates of krill faeces were at > 100 m, reflecting the downward migration of krill during the day. In all, 2–3 g Cm^–2 of krill faeces were collected, representing ca. twice that from intact phytoplankton cells. POC in the traps at 50 m was ca. 11 gm^–2, accounting for ca. 17% of the estimated primary production during the study period. As the secondary production is high, a large proportion of the production of P. pouchetii must be grazed by herbivores. Copepod faeces are probably remineralized in the euphotic zone, while those of krill provide the major coupling between the pelagial and the benthos. The implications of such a sedimentation model for partitioning energy flow between the pelagial and the benthos is discussed.     

Short-term variations in particulate matter sedimentation off Kapp Norvegia,Weddell Sea,Antarctica: relation to water mass advection,ice cover,plankton biomass and feeding activity

Summary A multi-cup sediment trap was deployed at 250m in the shelf area off Kapp Norvegia, Weddell Sea (630 m water depth) to determine the relative importance of water mass advection, sea ice movement, phytoplankton biomass and plankton feeding. Short-term fluctuations in sedimentation were determined using a sampling frequency of 2.7 days over 54 days during January and February 1988. Three periods of enhanced sedimentation were associated with water mass exchange, settling of diatoms following break-up of ice cover and release of fecal matter by krill feeding on particulate matter derived from phytoplankton and ice algae. An initial sedimentation pulse (28 Jan) was mainly due to sinking pelagic diatoms and krill fecal strings containing algae released from sea ice passing over the trap position. The ¹³C-composition of the sedimented organic carbon was about-24. The isotope ratio decreased sharply by about 5.5 at the end of the first pulse indicating the source of sinking matter becoming pelagic diatoms of the retreating ice-edge. At this time the diatom Corethron criophilum contributed a very high proportion of the organic flux causing an increase of the opal/C_org ratios. The second pulse (6 Feb) was due to empty diatom frustules, minipellets and small planktonic aggregates. Much of the organic carbon was transported by round fecal pellets. During the third pulse (14 Feb), round fecal pellets transported even more; the percentage of C. criophilum to the diatom organic carbon flux was more than 80% (>2mg C m^–2 day^–1).Data presented here were collected during the European Polarstern Study (EPOS) sponsored by the European Science Foundation     

The distribution and abundance of krill faecal material and oval pellets in the Scotia and Weddell Seas (Antarctica) and their role in particle flux

Summary The abundance and depth distribution of zooplankton faeces in spring to early summer were investigated along meridional transects (47°W and 49°W) that extended from the Scotia Sea (57°S) across the Weddell-Scotia Confluence and into the Weddell Gyre (62°S). The sea ice edge retreated from 59°30S to 61°S during the study. Faeces were sampled with nets, Niskin bottles and sediment traps and subsequently analysed by light and electron (SEM) microscopy. Krill faecal strings and oval faecal pellets of unknown origin were by far the most important zooplankton faeces and highest concentrations were always found in the Confluence often close to the ice border. Krill faeces were usually more abundant in the uppermost layer (0–50m) where they contributed an average of 130 g dry weight m^–3. There was an exponential decrease with depth, with a minimum of 0.6 g dry weight m^–3 in the 500–1000 m stratum. Oval pellets were more evenly distributed in the upper 1000 m of the water column, with an average of 9 g dry weight m ^–3, although there was a small peak (20 g dry weight m^–3) in the subsurface layer (50–150 m depth). Consecutive collections (day-night) of krill faeces using drifting sediment traps showed that only the larger strings sank from 50 to 150 m depth. Peritrophic membranes appeared to deteriorate during sinking. Diatoms (in particular Nitzschia and Thalassiosira spp.) contributed by far the bulk of material in krill and oval faeces. In samples collected near or under the pack ice, remains of crustaceans in both krill- and oval faeces were also found.Data presented here were collected during the European Polarstern Study (EPOS) sponsored by the European Science Foundation     

The influence of copepod and krill grazing on the species composition of phytoplankton communities from the Scotia Weddell sea

The influence of copepods (mainly Oithona sim-ilis) and krill (Euphausia superba) grazing on the species composition of plankton communities in ship board con tainers was investigated during the spring and post spring period in the Scotia Weddell Sea in the Antarctic ocean. Numbers of grazers were experimentally manipulated in containers with natural phytoplankton assemblages. With ratural levels of copepods but no krill a high (700–950 g C·l¹, ca 30 g chl a·.l¹) phytoplankton biomass developed. In these cultures large diatoms, e.g. Corethron criophilum and chains of Thalassiosira sp., made up 80% of total phytoplankton cell carbon at the end of the experiment. In cultures with elevated numbers of copepods (5X or 10X the natural level) phytoplankton biomass was somewhat reduced (ca 23 g chl a · l¹) compared to cultures with natural copepod abundance, but still high. Phytoplankton species composition was on the other hand greatly influenced. Instead of large diatoms these cultures were dominated by Phaeocystis pouchetii (70%) together with small Nitszchia sp. and Chaetoceros neogracile (20%). In containers with krill (both juveniles and adults), but without elevated numbers of copepods, phytoplankton biomass rapidly approached zero. With 10X the in situ level of copepods, krill first preyed on these before Corethron criophilum and Thalassiosira sp. were grazed. When krill were removed a plankton community dominated by flagellates (60–90%), e.g. Pyramimonas sp. and a Cryptophycean species, grazed by an unidentified droplet-shaped heterothrophic flagellate, developed. These flagellates were the same as those which dominated the plankton community in the Weddell Sea after the spring bloom. A similar succession was observed in situ when a krill swarm grazed down a phytoplankton bloom in a few hours. Our experiments show that copepods cannot control phytoplankton biomass in shipboard cultures even at artificially elevated numbers. Krill at concentrations similar to those in natural swarms have a great impact on both phytoplankton biomass and species composition in shipboard cultures. Both copepods and krill may have an impact on phytoplankton species composition and biomass in situ since the rates of phytoplankton cell division were probably artificially increased in shipboard cultures compared to natural conditions, where lower growth rates make phytoplankton more vulnerable to grazing. A similarity between phytoplankton successions in containers and in situ, especially with respect to krill grazing, supports the conclusion that grazing may structure phytoplankton communities in the Scotia-Weddell Sea.Data presented here were collected during the European Polarstern Study (EPOS) sponsored by the European Science Foundation     

Biogenic particles and nano/picoplankton in water masses over the Scotia-Weddell Sea Confluence,Antarctica

Summary We studied the particle composition in the ocean surface layer (20–100 m), in terms of non-living versus living particles (< 20 m), along a transect over the Scotia Sea/Weddell Sea transition. The data are related to characteristics of the phytoplankton community and used in a Principal Component Analysis to differentiate between water masses. There was a striking change in particle community characteristics from Scotia Sea to Weddell Sea waters, especially clear at shallow depths (20 m). Total particle concentration decreased greatly moving south over the Confluence but the proportion of living particles increased enormously. This paralleled a change in the composition of the phytoplankton community, from a bloom to a regenerating system, with a striking reduction in the prominence of non-living particles. Densities of auto- and heterotrophic nanoflagellates and bacteria reached maximal values towards the southern end of the transect (8.0 × 10³cm^–3,4.6 × 10³cm^–3,1.0 × 10⁶cm^–3). The PCA based on particle characteristics and chlorophyll a, POC and PON values, distinguished Scotia from Weddell Sea waters and separated shallow from deeper stations.Data presented here were collected during the European Polarstern Study (EPOS) sponsored by the European Science Foundation     

Biomass and composition of size fractionated phytoplankton in the Weddell-Scotia Confluence area

Summary The measurement of Chl a, Chl b and Chl c contents in four size fractions (Nuclepore filters of 10 m, 3m, 1 m and 0.2 m pore-size) together with microscopic examination illustrate the structure and the relative importance of the micro-, nano and pico-phytoplankton in the production system in the Weddell/Scotia Confluence area. In the Scotia Sea, large diatoms were prevalent and their biomass increased during the six week cruise period, exceeding 1 mg Chl a m^–3 at the beginning of January. In contrast, in the Marginal Ice Zone of the Weddell Sea, the biomass remained low, up to 0.3 mg Chl a m^–3. A diversified nanoplankton community accounted for more than 90% of this biomass: small diatoms, naked dinoflagellates, cryptophyceans, prymnesiophytes and green flagellates which increased the Chl b/Chl a ratio to values >0.20. An important trend affected the Confluence area, where a high biomass net-plankton community (4 mg Chl a m^–3) rapidly changed towards a uniform nanoplankton system of the same kind as in the Weddell Sea. At times, autotrophic cryptophyceans were almost dominating (>4.10⁶ cells/l), with a biomass up to 2 mg Chl a m^–3 and a low phaeopytin ratio (<10%). This situation probably arises because of a grazing pressure by krill. However, due to the geographic and oceanographic peculiarities of this area, it is not possible to extrapolate these observations concerning the size structure of the primary producers to the Southern Ocean in general.Data presented here were collected during the European Polarstern Study (EPOS) sponsored by the European Science Foundation     

Phytoplankton around Elephant Island,Antarctica

Phytoplankton studies were conducted in a 4·10⁴ km² grid around Elephant Island, Antarctica, during January–March 1991. In addition to profiling studies at 50 stations during each of two cruises, pumped surface water was used to continuously record in vivo chlorophyll-a (chl-a) fluorescence and beam attenuation coefficients (c_t). Measurements on discrete samples included chl-a, phytoplankton organic carbon (A_c), and total particulate organic carbon (POC). Equations were developed which permitted contour-mapping of chl-a and POC throughout the entire grid based on continuous measurements of in vivo chl-a fluorescence and c_t values. Phytoplankton abundance increased from January–February (cruise I) to February–March (cruise II) as evidenced by mean surface chl-a values (0.8 and 1.34 g l^–1, respectively) and mean A_c values for the upper 20 m of the water column (21.3 and 39.8 g Cl^–1, respectively). Microplankton accounted for 29% (cruise I) and 40% (cruise II) of the total phytoplankton, based on direct measurements of chl-a. Patterns for integrated values of chl-a, A_c and POC were similar to patterns of concentrations in surface waters. The richest areas of phytoplankton were north of Elephant and King George Islands, which coincided with high krill density areas.     

Characteristics of settling matter and its role in nutrient cycles in a deep oligotrophic lake

The settling flux of seston (dry weight, DW), chlorophyll a (Chl a), particulate organic carbon (POC), particulate organic nitrogen (PON), and particulate phosphorus (PP) was measured monthly in 1981–1983 at 10 different depths in Lake Chuzenji, Japan; an oligotrophic lake with a maximum depth of 163 m. The Ti concentration in entrapped matter was used to separate the sedimentation flux into allochthonous and autochthonous components. Inflow loads of dissolved nutrients (DN: 4.5, DP: 0.48 g m^-2a^-1) were almost sufficient to supply the autochthonous fluxes at 30 m (PON: 2.9, PP: 0.51 g m^-2a^-1 ), and this flux of POC (26.6 g m^-2a ^-1) was about one-third of primary production (84 g C M^-2a^-1). Sedimentation of particulate matter was the main path of losing nutrients from lake water, explaining more than 80% removal of inflow loads (TN, TP). Decomposition rates during sedimentation which were calculated from the vertical difference in the autochthonous flux agreed very closely with the results obtained by laboratory experiments of a 100-day incubation (content ratios from field observations were: POC 0.67, PON 0.65, PP 0.85; and from laboratory experiments they were: POC 0.68, PON 0.70, PP 0.94). These decomposition rates and those near the sediment interface were used to explain dissolved oxygen depletion and nitrate increase in the hypolimnion during stratification. The average sinking velocities were 1.82m d^-1 for seston and 1.16 m d^-1 for Chl a at 30m, they were influenced by Chl a content of seston.     

The cryptoendolithic microbial environment in the Ross Desert of Antarctica: Light in the photosynthetically active region

The vertical zonation of the Antarctic cryptoendolithic community appears to form in response to the light regime in the habitat. However, because of the structure of the habitat, the light regime is difficult to study directly. Therefore, a mathematical model of the light regime was constructed, which was used to estimate the total photon flux in different zones of the community. Maximum fluxes range from about 150m photons m^–2 s^–1 at the upper boundary of the community to about 0.1m photons m^–2 s^–1. Estimates of the annual productivity in the community indicate that the lowest zone of the community is light limited, with the maximal annual carbon uptake equivalent to less than the carbon content of one algal (Hemichloris) cell.     

Occurrence of cyclopoid copepods and faecal material in the Halley Bay region,Antarctica, during January–February 1991

Faecal material and cyclopoid copepods were collected during the expedition ANT IX/3, in the Halley Bay area (Weddell Sea, Antarctica), between January and February 1991. Faecal material comprised pellets produced by krill, copepods, ostracods and appendicularians. Cyclopoid copepods were represented by two genera, Oithona and Oncaea. In the Halley Bay area, higher concentrations of krill faecal material (420.9 mm³ m^–2) and chl.-a (39.3 mg m^–2) were found within the upper 200 m of the water column of the polynya than in ice-covered open-ocean areas (58.2 mm³m^–2 and 25.5 mg m^–2, respectively). At an ice-drift station, high concentrations of krill faecal strings under fest-ice were found. In addition, similarities between diatom assemblages in the pack-ice algae and krill faecal strings contents suggest an active utilization of ice-algae by krill populations. Sedimented material collected at 50 m depth by a sediment trap was dominated by krill faecal strings. Contents of small oval pellets (of probable cyclopoid copepod origin) resemble those of krill faecal pellets suggesting that coprophagy was involved. This suggestion is supported by: (1) The small quantity of food particles (other than krill faecal matter) available in the water column (< 0.3 g chl.-al^–1). (2) The negative in situ correlation between krill faecal strings and cyclopoid copepods. (3) The structure of cyclopoid copepod buccal appendages, which are more adapted for raptorial feeding.     

Feeding and diel vertical migration cycles of Metridia gerlachei (Giesbrecht) in coastal waters of the Antarctic Peninsula

Diel vertical migration and feeding cycles of adult female Metridia gerlachei in the upper 290 m of a 335-m water column were measured during a total of 65 h in two periods of early summer (Dec 20–21 and Dec 25–26, 1991). Samples collected in eight depth strata by 35 MOCNESS tows (333-m mesh) were analyzed for abundance and mean individual gut pigment content. Most of the copepod population was concentrated in a 50-m depth interval at all times. Feeding began simultaneously with nocturnal ascent from a depth of 200–250 m at 18:00 h (local time), when the relative change in ambient light intensity was greatest. Ingestion rate increased exponentially (k_i = 0.988 h^–1) at double the gut evacuation rate (k_e = 0.488 h^–1) as the population moved upward at 22.3–26.5 m h^–1 through increasing concentrations of particulate chlorophyll-a. Although the bulk of the population did not move to depths shallower than 50 m, and began its downward migration at a rate of 20.8–31.7 mh^–1 in complete darkness, individual females continued to make brief excursions into chlorophyll-rich surface waters (4–8 g l^–1) during the first few hours of population descent. Ingestion rate diminished abruptly by one order of magnitude (k_i = 0.068 h^–1) at dawn ( 0330 h). Within four more hours, the population had reached its daytime depth and gut pigment content remained constant at a minimum value until the next migration cycle. No feeding appeared to take place at depth during the day. Ingestion by M. gerlachei females removed < 4% of daily primary production, with only 20% of this amount being removed from surface waters by active vertical transport.     

Organic carbon transport and C/N ratio variations in a large tropical river: Godavari as a case study,India

This study gives an insight into the source of organic carbon and nitrogen in the Godavari river and its tributaries, the yield of organic carbon from the catchment, seasonal variability in their concentration and the ultimate flux of organic and inorganic carbon into the Bay of Bengal. Particulate organic carbon/particulate organic nitrogen (POC/PON or C/N) ratios revealed that the dominant source of organic matter in the high season is from the soil (C/N = 8–14), while in the rest of the seasons, the river-derived (in situ) phytoplankton is the major source (C/N = l–8). Amount of organic materials carried from the lower catchment and flood plains to the oceans during the high season are 3 to 91 times higher than in the moderate and low seasons. Large-scale erosion and deforestation in the catchment has led to higher net yield of organic carbon in the Godavari catchment when compared to other major world rivers. The total flux of POC, and dissolved inorganic carbon (DIC) from the Godavari river to the Bay of Bengal is estimated as 756 × 10⁹ and 2520 × 10⁹ g yr^–1, respectively. About 22% of POC is lost in the main channel because of oxidation of labile organic matter, entrapment of organic material behind dams/sedimentation along flood plains and river channel; the DIC fluxes as a function of alkalinity are conservative throughout the river channel. Finally, the C/N ratios (12) of the ultimate fluxes of particulate organic carbon suggest the dominance of refractory/stable soil organic matter that could eventually get buried in the coastal sediments on a geological time scale.     

Size-fractionated biomass and productivity of phytoplankton and particulate organic carbon in the southern ocean

During the austral summer of 1989/1990, surface samples were obtained of size-fractionated biomass, and the productivity of phytoplankton, its cell abundance, the composition of the dominant species, the concentration of particulate organic carbon (POC) and the related environmental surface parameters were measured in a large-scale survey primarily of the Atlantic and Indian Sectors. The results showed that the southern atlantic sector is the most fertile; chlorophylla (Chla) concentration averaged over 2 μg l⁻¹, average cell abundance was about 41.0 × 10³ cell l⁻¹, and average POC concentration was also the highest (>100 μg l⁻¹), but was lower in the Drake Passage and the southern Indian sector. The results for size-fractionated Chla showed that netplankton (>20 μm) in the South Atlantic Ocean, having abundant nutrients, accounted for the highest proportion (average 65%) of biomass. In the infertile South Indian Ocean, picoplankton (<2 μm) accounted for the highest proportion, averaging 47%. The results for size-fractionated productivity showed that the contribution of picoplankton to total productivity was the largest in the South Atlantic Ocean and Drake Passage, those of nanoplankton (2–20 μm) and netplankton being about equal. The relatively high photosynthesis assimilation number of picoplankton demonstrates their importance in the marine ecosystems of Antarctic water. In comparison with the Antarctic water, the subantarctic and subtropical waters are infertile.     

Surface distribution of size-fractionated chlorophyll a and participate organic matter in the Strait of Magellan

The surface distribution of chlorophyll a (chl a) from size-fractionated phytoplankton and of particulate organic matter was studied along the Strait of Magellan during late austral summer (February 20th to March 2nd, 1991), in order to contribute an outline of the ecological characteristics of its pelagic compartment. Sampling of surface water was carried out at 2.5 mile intervals, yielding 152 sampling points for chl a and 104 for particulate organic carbon (POC). The Strait appeared as a system strongly controlled by land forcing. Its phytoplankton community was dominated by the picoplanktonic fraction along its entire length, with mean chl a concentrations of 0.74 and 1.17 g dm^–3 for pico- and total phytoplankton, respectively. The microphytoplankton never exceeded 0.02 g dm^–3. POC concentrations, with a maximum of 242.5 and a mean of 144.8 g dm^–3, were mainly of autotrophic origin, as indicated by a mean POC:chl a ratio of 138.4.     

A review of data on production and import of organic carbon in the western Wadden Sea

Summary Annual phytoplankton primary production in the tidal channels of the western Wadden Sea cannot be estimated more precisely than 150±50 g C.m^–2a^–1, due to large spatial and short-term temporal variations. This implies that year-to-year variations and eventually long-term trends have to be very pronounced to be measurable even with a weekly sampling program.Short-term temporal variation in primary production of microphytobenthos living on the tidal flats is less pronounced, but spatial variation is large. Primary production on high tidal flats is larger than on flats lower in the tidal zone. Year-to-year variation on a tidal flat station occupied now for 12 years was large. This variation cannot be explained by year-to-year variations in nutrients, light or temperature, but probably by year-to-year variations in grazing. Macrophytobenthic primary production plays a subordinate role in the western Wadden Sea after the disappearance ofZostera fields. It is difficult to give one figure for the annual primary production of an average tidal flat due to the variations mentioned. Tentatively, microphytobenthic plus macrophytobenthic plus phytoplankton primary production on and above an average tidal flat is estimated at 150±50 g C.m^–2a^–1,i.e. the same as estimated for phytoplankton primary production in the tidal channels.The western Wadden Sea receives a considerable amount of particulate organic carbon from outside the area, estimated at 240 g C.m^–2a^–1. Formerly the North Sea was thought to be the only source. New data indicate also an import from the Ysselmeer. The import of total organic carbon, particulate plus dissolved, from the Ysselmeer exceedsin situ primary production. From this import Ysselmeer DOC is probably not used very much in the Wadden Sea. However, Ysselmeer POC, consisting for 50% on average of living phytoplankton cells, may form a suitable food source for Wadden Sea invertebrates. Cell counts ofScenedesmus sp., a freshwater alga used as a natural tracer for Ysselmeer POC in the western Wadden Sea, indicate that a large part of the Ysselmeer POC is retained here.     

Krill diet affects faecal string settling

Summary Free-floating sediment traps used on a transect from Scotia Sea to Weddell Sea collected larger, more degraded, krill faecal strings in the deeper (150 m) than in the 50 or 75 m traps. The smallest faecal strings were only present in the shallower traps. Sinking velocity of smaller faecal strings was — as expected — much lower than for larger ones, with a total range of 50 to 800 m · day ^–1 for faecal string volumes of 0.007 to 0.53 mm³. Krill feeding largely on diatoms produced faeces with higher settling velocity than those feeding on non-diatom phytoplankton. Smaller krill faecal strings do not leave the upper mixed layer. Potential settling velocities as measured in settling tubes (without turbulence), may in this respect be misleading. Small oval faecal pellets of unknown origin showed relatively high settling velocities (80 to 250 m·day^–1 for 0.002 to 0.013 mm³) due to higher compaction and lower form resistance to sinking.Data presented here were collected during the European Polarstern Study (EPOS) sponsored by the European Science Foundation     

The distribution of Heterotrissocladius oliveri Saether (Diptera: Chironomidae) in Lake Michigan

Fifty one chironomid species were identified from 504 samples collected at depths ranging 8 to 267 m in Lake Michigan, U.S.A. Heterotrissocladius oliveri Saether occurred in 32% of these samples and had an average abundance of 22 m^–2 which was similar to other estimates from the Great Lakes. Maximum average lake-wide density was at 30 to 60 m (41 m^–2). At depths 60 m, H. oliveri was the dominant chironomid species comprising 75% of total Chironomidae. The substrate preference of H. oliveri differed within each depth regime considered: at 30–60 m, 2–3 ; at 60–120 m, 3–5 , 7–9 ; and at 120–180 m, 6–8 . Abundance was notably reduced at all depths in substrates characterized as medium silt (5–6 ). On a lake-wide basis, the distribution pattern suggested H. oliveri was most numerous from 30 to 60 m along the southwestern, eastern, and northern shorelines and at 60–120 m depths along the southern and eastern shorelines. Increased abundance in the South Basin was concurrent with evidence of increased sedimentation at 60 to 100 m. However, in several other areas of the lake, high densities were associated with medium to very fine sands relatively free of silts and clays. This observation suggested occurrence of H. oliveri was minimally affected by sediment type.Widely variable, but generally elevated water temperatures likely prevent H. oliveri from establishing a substantial population density at depths < 30 m. With increased depth, temperature fluctuation is negligible and food is more stable, though the source is variable. Factors limiting abundance of H. oliveri at depths 30 m were related to decreased food supply due to distance from shore, food sources of lower value (clays), and, most importantly, to reproductive replenishment.Although still oligotrophic in nature, high density occurrences in both high and low sedimentation areas of the lake suggest the trophic indicator status of H. oliveri might be broader than previously thought.     

Long-term kinetics of the light-dependent regulation of ribulose-1,5-bisphosphate carboxylase/oxygenase activity in plants with and without 2-carboxyarabinitol 1-phosphate

The light-dependent modulation of ribulose-1,5-bisphosphate carboxylase/oxygenase (Rubisco) activity was studied in two species: Phaseolus vulgaris L., which has high levels of the inhibitor of Rubisco activity, carboxyarabinitol 1-phosphate (CA1P), in the dark, and Chenopodium album L., which has little CA1P. In both species, the ratio of initial to fully-activated Rubisco activity declined by 40–50% within 60 min of a reduction in light from high a photosynthetic photon flux density (PPFD; >700 mol · m^–2 · s^–1) to a low PPFD (65 ± 15 mol · m^–2 · s^–1) or to darkness, indicating that decarbamylation of Rubisco is substantially involved in the initial regulatory response of Rubisco to a reduction in PPFD, even in species with potentially extensive CA1P inhibition. Total Rubisco activity was unaffected by PPFD in C. album, and prolonged exposure (2–6 h) to low light or darkness was accompanied by a slow decline in the activity ratio of this species. This indicates that the carbamylation state of Rubisco from C. album gradually declines for hours after the large initial drop in the first 60 min following light reduction. In P. vulgaris, the total activity of Rubisco declined by 10–30% within 1 h after a reduction in PPFD to below 100 mol · m^–2 · s^–1, indicating CA1P-binding contributes significantly to the reduction of Rubisco capacity during this period, but to a lesser extent than decarbamylation. With continued exposure of P. vulgaris leaves to very low PPFDs (< 30 mol · m^–2 · s^–1), the total activity of Rubisco declined steadily so that after 6–6.5 h of exposure to very low light or darkness, it was only 10–20% of the high-light value. These results indicate that while decarbamylation is more prominent in the initial regulatory response of Rubisco to a reduction in PPFD in P. vulgaris, binding of CA1P increases over time and after a few hours dominates the regulation of Rubisco activity in darkness and at very low PPFDs.Abbreviations CA1P 2-carboxyarabinitol 1-phosphate - CABP 2-carboxyarabinitol 1,5-bisphosphate - k_cat substrate-saturated turnover rate of fully carbamylated enzyme - PPFD photosynthetically active photon flux density (400–700 nm) - Rubisco ribulose-1,5-bisphosphate carboxylase/oxygenase - RuBP ribulose-1,5-bisphosphate     

Respiratory electron transport activity of microplankton in the Weddell Sea during early spring: influence of the ice cover and the ice edge

Summary The activity of the respiratory electron transport system (ETS) of the microplankton (<240 m size) was measured in the Northern Weddell Sea during EPOS 1, in the Close Pack Ice (CPI), and in the ice edge (Outer and Inner Marginal Zones, OMIZ and IMIZ). During early spring the activity increased with time and in the pack ice-open water direction. The temporal trend was more obvious than the spatial one. ETS activity ranged from 0.01 to 1.25 ml O₂ m^–3 h^–1 under the ice and from 0.1 to 1.6 ml O₂ m^–3 h^–1 in the open water at the ice edge. Depth-integrated ETS activity in the upper 300 m ranged from 13 to 130 ml O₂ m^–2h^–1. 60% to 80% of the activity took place above 100 m in the OMIZ in the prebloom conditions at the end of the cruise. ETS/Chl a ratios showed the importance of microheterotrophs under the ice, versus a greater phytoplankton dominance in the ice edge-open water zone. The carbon-specific activity reached a maximum (0.43 day^–1) in the innermost zone of the CPI where bacteria dominated. Respiratory activity under the ice is important in producing the oxygen deficit observed, due to the negative balance between photosynthesis and respiration. The ETS activity was at the lower range of that found in the region in summer and is comparable to that measured in other oligotrophic, stratified systems in oceanic areas.Data presented here were collected during the European Polarstern Study (EPOS) sponsored by the European Science Foundation     

A bloom of Dunaliella parva in the Dead Sea in 1992: biological and biogeochemical aspects

A bloom of the unicellular green alga Dunaliella parva (up to 15 000 cells m1^–1) developed in the upper 5 m of the water column of the Dead Sea in May-June 1992. This was the first mass development of Dunaliella observed in the lake since 1980, when another bloom was reported (up to 8800 cells m1^–1). For a bloom of Dunaliella to develop in the Dead Sea, two conditions must be fulfilled: the salinity of the upper water layers must become sufficiently low as a result of dilution with rain floods, and phosphate must be available. During the period 1983–1991 the lake was holomictic, hardly any dilution with rainwater occurred, and no Dunaliella cells were observed. Heavy rain floods in the winter of 1991–1992 caused a new stratification, in which the upper 5 m of the water column became diluted to about 70% of their former salinity. Measurements of the isotopic composition of inorganic carbon in the upper water layer during the bloom (¹³C = 5.1) indicate a strong fractionation when compared with the estimated –3.4 prior to the bloom. The particulate organic carbon formed was highly enriched in light carbon isotopes ( ¹³ C = – 13.5). The algal bloom rapidly declined during the months June–July, probably as a result of the formation of resting stages, which sank to the bloom. A smaller secondary bloom (up to 1850 cells m1–1) developed between 6 and 10 m depth at the end of the summer. Salinity values at this deep chlorophyll maximum were much beyond those conductive for the growth of Dunaliella, and the factors responsible for the development of this bloom are still unclear.