Description: Schwerpunkt der Arbeit ist die Untersuchung der geographischen Verbreitung und Vertikalverteilung der Chaetagnathen im Gebiet rund um die Antarktische Halbinsel. Die bearbeiteten Proben stammen hauptsächlich aus dem RMT-8 M, vergleichend werden auch Nansen-Schließnetzfänge (NSN) und im Gebiet der nördlichen Weddell See RMT-1 M-Proben analysiert. Die nördliche Weddell See weist von allen untersuchten Gebieten in den drei Netzen die höchsten Häufigkeiten an Chaetagnathen auf. Im Untersuchungsgebiet sind in den RMT-8-Fängen regelmäßig die Arten S. gazellae, E. hamata, S. marri, S. maxima und E. bathypelagica in Abhängigkeit von der Tiefe vertreten. E. bathyantarctica kommt vereinzelt - hauptsächlich in den NSN-Fängen aus über 1000 m Tiefe - vor. S. gazellae und S. maxima sind in den NSN-Proben kaum vertreten. Zwei möglicherweise bisher unbekannte Arten der Gattung Heterakrohnia (n=10) sowie ein nicht einzuordnendes Exemplar einer vielleicht neuen Gattung ("Heterospadella") sind in den NSN-Fängen aus großer Tiefe (〉1000 m) enthalten, bedürfen jedoch noch der Absicherung. Die im Untersuchungsgebiet am häufigsten anzutreffende Art E. hamata ist mit Ausnahme des direkten Oberflächenbereichs in der gesamten Wassersäule bis in über 1000 m Tiefe nachzuweisen. In den NSN-Proben ist diese Art hauptsächlich zwischen 200 m und 500 m vertreten, in den RMT-1-Proben liegt ihr Abundanzmaximum ebenfalls in diesem Bereich. Mit zunehmender Tiefe ansteigende Häufigkeiten weisen dagegen die RMT-8-Proben auf. Dieses Netz (4,5 mm Maschenweite) erfaßt die kleineren Chaetagnathen nicht. S. gazellae ist in den RMT-8-Proben schwerpunktmäßig zwischen 250 bis 400 m zu finden, die RMT-1-Fänge zeigen maximale Abundanzen zwischen 75 m und 135 m, im RMT-1 nehmen die Häufigkeiten von S. gazellae mit zunehmender Tiefe ab. S. marri, S. maxima und E. bathypelagica kommen verstärkt in größeren Tiefen unterhalb von 200 m in den Proben vor. S. marri und die seltenere S. maxima besiedeln hauptsächlich den mesopelagischen Bereich, die Hauptverbreitungszone von E. bathypelagica liegt tiefer als die von S. marri und S. maxima. Die untersuchten Dauerstationen lassen keine tagesperiodischen Wanderungen der Chaetognathen erkennen. Die Verteilungen der Längen-Häufigkeiten und der Reifestadien zeigen für S. gazellae und E. hamata eine tiefengebundene Größenstaffelung, gekoppelt mit einem fortschreitenden Reifungsprozeß, d.h. mit zunehmender Tiefe treten durchschnittlich größere, reifere lndividuen auf. Für S. marri und S. maxima lassen die Ergebnisse ein ähnliches Phänomen vermuten. Über E. bathypelagica und E. bathyantarctica können aufgrund der geringen Anzahl an gefangenen Tieren keine Aussagen gemacht werden. Eine Korrelation der Abundanzen mit den hydrographischen Umweltdaten (Temperatur, Salzgehalt) weist S. gazellae und E. hamata für antarktische Verhältnisse als eher eurytherme und euryhaline Arten aus. S. marri, S. maxima und E. bathypelagica sind geringeren Salzgehaltsänderungen unterworfen. Minimale Salzgehaltsschwankungen treten im Bereich maximaler Abundanz auf. Die Temperatur- und Salzgehaltsspektren, in denen die fünf Arten im Untersuchungsgebiet vorkommen, bzw. Verbreitungsschwerpunkte haben, werden angegeben. Es werden Angaben zu Darminhalt und Parasitenbefall der Chaetognathen gemacht.

Description: The northern Humboldt Current upwelling system (HCS) belongs to the most productive marine ecosystems, providing five to eight times higher fisheries landings per unit area than other coastal upwelling systems. To solve this “Peruvian puzzle”, to elucidate the pelagic food-web structure and to better understand trophic interactions in the HCS, a combined stable isotope and fatty acid trophic biomarker approach was adopted for key zooplankton taxa and higher trophic positions with an extensive spatial coverage from 8.5 to 16°S and a vertical range down to 1,000 m depth. A pronounced regional shift by up to ∼5‰ in the δ15N baseline of the food web occurred from North to South. Besides regional shifts, δ15N ratios of particulate organic matter (POM) also tended to increase with depth, with differences of up to 3.8‰ between surface waters and the oxygen minimum zone. In consequence, suspension-feeding zooplankton permanently residing at depth had up to ∼6‰ higher δ15N signals than surface-living species or diel vertical migrants. The comprehensive data set covered over 20 zooplankton taxa and indicated that three crustacean species usually are key in the zooplankton community, i.e., the copepods Calanus chilensis at the surface and Eucalanus inermis in the pronounced OMZ and the krill Euphausia mucronata, resulting in an overall low number of major trophic pathways toward anchovies. In addition, the semi-pelagic squat lobster Pleuroncodes monodon appears to play a key role in the benthic-pelagic coupling, as indicated by highest δ13C’ ratios of −14.7‰. If feeding on benthic resources and by diel vertical migration, they provide a unique pathway for returning carbon and energy from the seafloor to the epipelagic layer, increasing the food supply for pelagic fish. Overall, these mechanisms result in a very efficient food chain, channeling energy toward higher trophic positions and partially explaining the “Peruvian puzzle” of enormous fish production in the HCS.

Description: Highlights: • Environmental conditions cause specific zooplankton life strategies. • No ontogenetic or diel vertical migration in the life cycle of Calanus chilensis. • Spatial expansion of Calanus chilensis secondary production far offshore. • Compacted surface biomass of Calanus chilensis allows easy foraging by anchovy. Abstract: Calanid copepods of the genera Calanus and Calanoides are key components of zooplankton communities in upwelling systems. Here, we compare the life-history traits of Calanus chilensis from the Humboldt Current Systems (HCS) off northern Peru and its counterpart Calanoides natalis from the northern Benguela Current System (BCS) off Namibia. A comprehensive data set of the distribution and abundance patterns of these species along extensive horizontal and vertical scales is presented. C. chilensis from the HCS was almost exclusively restricted to the surface layer (50–0 m) above the oxygen minimum zone (OMZ), whereas C. natalis from the BCS inhabited the entire water column down to 800 m performing ontogenetic vertical migration (OVM) through the OMZ. Resting stages of C. natalis at depth accumulated high amounts of lipid (30–60% of dry mass, DM), whereas C. chilensis did not rely on lipid reserves. These findings confirm that the life cycle of C. chilensis does not include OVM with diapause at depth. Surprisingly, the regional distribution of C. chilensis secondary production extended much further offshore (〉200 km from the coast) than is typical of other coastal upwelling systems. Deviating environmental conditions forced the two key calanid species to develop specific, but different life strategies for HCS and BCS. Compacted biomass concentrations of C. chilensis in the surface layer from the shelf (≤3 g DM m−2) to offshore waters (≤1.5 g DM m−2) facilitate easy and efficient foraging by predators such as juvenile Peruvian anchovies. In contrast, a large fraction of the C. natalis biomass occurs within the OMZ and is thus out of reach for hypoxia-sensitive predators. Calanoid copepods (e.g. C. chilensis) play a crucial role as important prey for growth and recruitment of small pelagic fish. Thus, the compacted biomass and high productivity of C. chilensis at the surface derived from its adaptive life-history traits (no OVM) may explain the superior trophic transfer efficiency and hence enormous fisheries yield of the HCS compared to the BCS.

Description: The Humboldt Current Upwelling System (HCS) is the most productive eastern boundary upwelling system (EBUS) in terms of fishery yield on the planet. EBUSs are considered hotspots of climate change with predicted expansion of mesopelagic oxygen minimum zones (OMZs) and related changes in the frequency and intensity of upwelling of nutrient-rich, low-oxygen deep water. To increase our mechanistic understanding of how upwelling impacts plankton communities and trophic links, we investigated mesozooplankton community succession and gut fluorescence, fatty acid and elemental compositions (C, N, O, P), and stable isotope (δ13C, δ15N) ratios of dominant mesozooplankton and microzooplankton representatives in a mesocosm setup off Callao (Peru) after simulated upwelling with OMZ water from two different locations and different N:P signatures (moderate and extreme treatments). An oxycline between 5 and 15 m with hypoxic conditions (〈50 µmol L−1) below ∼10 m persisted in the mesocosms throughout the experiment. No treatment effects were determined for the measured parameters, but differences in nutrient concentrations established through OMZ water additions were only minor. Copepods and polychaete larvae dominated in terms of abundance and biomass. Development and reproduction of the dominant copepod genera Paracalanus sp., Hemicyclops sp., Acartia sp., and Oncaea sp. were hindered as evident from accumulation of adult copepodids but largely missing nauplii. Failed hatching of nauplii in the hypoxic bottom layer of the mesocosms and poor nutritional condition of copepods suggested from very low gut fluorescence and fatty acid compositions most likely explain the retarded copepod development. Correlation analysis revealed no particular trophic relations between dominant copepods and phytoplankton groups. Possibly, particulate organic matter with a relatively high C:N ratio was a major diet of copepods. C:N ratios of copepods and polychaetes ranged 4.8–5.8 and 4.2–4.3, respectively. δ15N was comparatively high (∼13 ‰–17 ‰), potentially because the injected OMZ source water was enriched in δ15N as a result of anoxic conditions. Elemental ratios of dinoflagellates deviated strongly from the Redfield ratio. We conclude that opportunistic feeding of copepods may have played an important role in the pelagic food web. Overall, projected changes in the frequency and intensity of upwelling hypoxic waters may make a huge difference for copepod reproduction and may be further enhanced by varying N:P ratios of upwelled OMZ water masses.