Planktological-chemical observation during the International Indian Ocean Expedition (IIOE) with RV "Meteor" in 1964/65

The present volume contains the planktological data collected during the expedition of the "Meteor" to the Indian Ocean in 1964/65. It was the main objective of the expedition to study the up- and downwelling conditioned along the western and eastern coasts of the Arabian Sea by the northeastern monsoon. It is from these areas that the greater part of the data here presented was obtained. A few values from the Red Sea have been added. As the title "Planktological-Chemical Data" implies, it was chiefly with the help of chemical methods that the planktological investigations, with the exception of the particle size analysis and phytoplankton counting conducted optically, were carried out. These investigations were above all devoted to a quantitative survey of particulate matter and plankton, the latter being sampled by water-bottle and net. The zooplankton hauls were taken with the Indian Ocean Standard Net according to the international guidelines laid down for the expedition. As a rule, double catches were made at every station, one sample being intended for laboratory analysis at the Indian Ocean Biological Centre in Ernakulam, South India, and the other for the Institut für Meereskunde in Kiel. In addition to determining the standing stock, the production rate of phytoplankton was measured by the 14C method. These experiments were mainly conducted during the latter half of the expedition. The planktological studies primarily covered the euphotic zone, extending into the underlying water layers up to a depth of 600 m. The investigations were above all directed towards ascertaining the quantity of organic substance, formed by primary production, in its relation to environmental conditions and determining whether or not organic substance is actively transported from the surface into the deeper layers by the periodically migration organisms of the deep scattering layers. Depending on the station time available, a few samples could now and then be taken from deeper layers. The present volume of planktological-chemical data addresses itself to all those concerned processing the extensive material collected during the International Indian Ocean Expedition. As a readily accessible work of reference, it hopes to serve as an aid in the evaluation and interpretation of the expedition results. The complementary ecological data such as temperature, salinity, and oxygen content as well as the figures obtained on abundance and distribution in depth of the nutrients essential for primary production may be found in the volume of physical-chemical data published in Series A of the "Meteor"-Forschungsergebnisse No. 2, 1966 (Dietrich et al., 1966).

Mesozooplankton abundance data from Disko Bay, West Greenland, 2008

The study site was located in the Disko Bay off Qeqertarsuaq, western Greenland. Due to land-connected sea ice coverage during winter, 2 sampling sites were combined. At the first site in winter (21 February to 23 March 2008), sampling was conducted through a hole in the ice at ca. 65 to 160 m depth approximately 0.5 nautical mile (n mile) south of Qeqertarsuaq (69° 14' N, 53° 29' W). In spring and summer (9 April to 18 July), sampling was done at a monitoring station 1 n mile south from Qeqertarsuaq (69° 14' N, 53° 23' W) at 300 m depth. Sampling was carried out between 10:00 and 17:00 h. During sampling from the ice, mesozooplankton was collected using a modified WP-2 net (45 µm) equipped with a closing mechanism (Hydrobios). Samples were collected in 3 depth strata (0-50, 50-100, and 100-150 m). During ship-based sampling, mesozooplankton was collected with a multinet (50 µm) equipped with a flow meter (Multinet, Hydrobios type midi), and 2 additional depth strata (150-200m and 200-250 m) were included. In addition to the seasonal study one diurnal investigation with sampling every 6 h was conducted from 29 April at 12:00 h to 30 April 30 at 12:00 h. Samples were immediately preserved in buffered formalin (5% final concentration) for later analyses. Biomass values of the different copepod species were calculated based on measurements of prosome length, and length/weight relationships. Two regressions for Calanus spp. were established for biomass calculations: one applicable prior to and during the phytoplankton bloom until 4 May, and another from 9 May onwards.

Solar UV irradiances modulate effects of ocean acidification on the Coccolithophorid Emiliania huxleyi

Emiliania huxleyi, the most abundant coccolithophorid in the oceans, is naturally exposed to solar UV radiation (UVR, 280-400 nm) in addition to photosynthetically active radiation (PAR). We investigated the physiological responses of E. huxleyi to the present day and elevated CO2 (390 vs 1000 µatm; with pH(NBS) 8.20 vs 7.86) under indoor constant PAR and fluctuating solar radiation with or without UVR. Enrichment of CO2 stimulated the production rate of particulate organic carbon (POC) under constant PAR, but led to unchanged POC production under incident fluctuating solar radiation. The production rates of particulate inorganic carbon (PIC) as well as PIC/POC ratios were reduced under the elevated CO2, ocean acidification (OA) condition, regardless of PAR levels, and the presence of UVR. However, moderate levels of UVR increased PIC production rates and PIC/POC ratios. OA treatment interacted with UVR to influence the alga's physiological performance, leading to reduced specific growth rate in the presence of UVA (315-400 nm) and decreased quantum yield, along with enhanced nonphotochemical quenching, with addition of UVB (280-315 nm). The results clearly indicate that UV radiation needs to be invoked as a key stressor when considering the impacts of ocean acidification on E. huxleyi.

Effects of ultraviolet radiation and CO2 increase on winter phytoplankton assemblages in a temperate coastal lagoon

Increases in ultraviolet radiation (UVR) and CO2 affect phytoplankton growth and mortality in a variety of different ways. However, in situ responses of natural phytoplankton communities to climate change, as well as its effects on phytoplankton annual cycles, are still largely unknown. Although temperature and UVR have been increasing in temperate latitudes during winter, this season is still particularly neglected in climate change studies, being considered a non-active season regarding phytoplankton growth and production. Additionally, coastal lagoons are highly productive ecosystems and very vulnerable to climate change. This study aims, therefore, to evaluate the short-term effects of increased UVR and CO2 on the composition and growth of winter phytoplankton assemblages in a temperate coastal lagoon. During winter 2012, microcosm experiments were used to evaluate the isolated and combined effects of UVR and CO2, under ambient and high CO2 treatments, exposed to ambient UV levels and photosynthetically active radiation (PAR), or to PAR only. Phytoplankton composition, abundance, biomass and photosynthetic parameters were evaluated during the experiments. Significant changes were observed in the growth of specific phytoplankton groups, leading to changes in community composition. The cyanobacterium Synechococcus was dominant at the beginning of the experiment, but it was negatively affected by UVR and CO2. Diatoms clearly benefited from high CO2 and UVR, particularly Thalassiosira. Despite the changes observed in specific phytoplankton groups, growth and production of the whole phytoplankton community did not show significant responses to UVR and/or CO2.

(Table 1) 100 m integrated temperature, chlorophyll a content and protist biomass during Leg 7 of Galathea 3 cruise (2006)

We present a study on the protozooplankton >5 µm and copepods larger than 50 µm at a series of contrasting stations across the Southern Indian Ocean (SIO). Numerically, over 80% of the copepod community across the transect was less than 650 µm in size, dominated by nauplii, and smaller copepods, while 80% of the biomass (as mg C/m**3) was larger than 1300 µm in body length. Predation by the carnivorous copepod Corycaeus sp. was estimated to be able to remove up to 2% /d of the copepods <1000 µm in size. By the help of grazing models we estimated that primary producers were mainly grazed upon by ciliates and heterotrophic dinoflagellates (40-80% /d combined) in temperate waters but appendicularians became increasingly important in the tropical waters grazing about 40% of the biomass per day. Despite their high abundance and biomass, copepods contributed less than 20% of the grazing at most stations. Secondary production was low (carbon specific egg production <0.14 /d) but typical for food limited oligotrophic oceans.

The dust environment of comet 67P/Churyumov-Gerasimenko from Rosetta OSIRIS and VLT observations in the 4.5 to 2.9 AU heliocentric distance range inbound

Context. The ESA Rosetta spacecraft, currently orbiting around cornet 67P/Churyumov-Gerasimenko, has already provided in situ measurements of the dust grain properties from several instruments, particularly OSIRIS and GIADA. We propose adding value to those measurements by combining them with ground-based observations of the dust tail to monitor the overall, time-dependent dust-production rate and size distribution. Aims. To constrain the dust grain properties, we take Rosetta OSIRIS and GIADA results into account, and combine OSIRIS data during the approach phase (from late April to early June 2014) with a large data set of ground-based images that were acquired with the ESO Very Large Telescope (VLT) from February to November 2014. Methods. A Monte Carlo dust tail code, which has already been used to characterise the dust environments of several comets and active asteroids, has been applied to retrieve the dust parameters. Key properties of the grains (density, velocity, and size distribution) were obtained from. Rosetta observations: these parameters were used as input of the code to considerably reduce the number of free parameters. In this way, the overall dust mass-loss rate and its dependence on the heliocentric distance could be obtained accurately. Results. The dust parameters derived from the inner coma measurements by OSIRIS and GIADA and from distant imaging using VLT data are consistent, except for the power index of the size-distribution function, which is alpha = -3, instead of alpha = -2, for grains smaller than 1 mm. This is possibly linked to the presence of fluffy aggregates in the coma. The onset of cometary activity occurs at approximately 4.3 AU, with a dust production rate of 0.5 kg/s, increasing up to 15 kg/s at 2.9 AU. This implies a dust-to-gas mass ratio varying between 3.8 and 6.5 for the best-fit model when combined with water-production rates from the MIRO experiment.

3D Direct Simulation Monte Carlo Modelling of the Inner Gas Coma of Comet 67P/Churyumov-Gerasimenko: A Parameter Study

Direct Simulation Monte Carlo (DSMC) is a powerful numerical method to study rarefied gas flows such as cometary comae and has been used by several authors over the past decade to study cometary outflow. However, the investigation of the parameter space in simulations can be time consuming since 3D DSMC is computationally highly intensive. For the target of ESA's Rosetta mission, comet 67P/Churyumov-Gerasimenko, we have identified to what extent modification of several parameters influence the 3D flow and gas temperature fields and have attempted to establish the reliability of inferences about the initial conditions from in situ and remote sensing measurements. A large number of DSMC runs have been completed with varying input parameters. In this work, we present the simulation results and conclude on the sensitivity of solutions to certain inputs. It is found that among cases of water outgassing, the surface production rate distribution is the most influential variable to the flow field.

Calcium carbonate vein compositions from drill sites in the Atlantic and Pacific

Chemical (Sr, Mg) and isotopic (d18O, 87Sr/86Sr) compositions of calcium carbonate veins (CCV) in the oceanic basement were determined to reconstruct changes in Sr/Ca and Mg/Ca of seawater in the Cenozoic. We examined CCV from ten basement drill sites in the Atlantic and Pacific, ranging in age between 165 and 2.3 Ma. Six of these sites are from cold ridge flanks in basement <46 Ma, which provide direct information about seawater composition. CCV of these young sites were dated, using the Sr isotopic evolution of seawater. For the other sites, temperature-corrections were applied to correct for seawater-basement exchange processes. The combined data show that a period of constant/low Sr/Ca (4.46 - 6.22 mmol/mol) and Mg/Ca (1.12 - 2.03 mol/mol) between 165 and 30 Ma was followed by a steady increase in Mg/Ca ratios by a factor of three to modern ocean composition. Mg/Ca - Sr/Ca relations suggest that variations in hydrothermal fluxes and riverine input are likely causes driving the seawater compositional changes. However, additional forcing may be involved in explaining the timing and magnitude of changes. A plausible scenario is intensified carbonate production due to increased alkalinity input to the oceans from silicate weathering, which in turn is a result of subduction-zone recycling of CO2 from pelagic carbonate formed after the Cretaceous slow-down in ocean crust production rate.

On loader productivity, rock strength and explosive energy in metal mining

Twenty production blasts in two open pit mines were monitored, in rocks with medium to very high strength. Three different blasting agents (ANFO, watergel and emulsion blend) were used, with powder factors ranging between 0.88 and 1.45 kg/m3. Excavators were front loaders and rope shovels. Mechanical properties of the rock, blasting characteristics and mucking rates were carefully measured. A model for the calculation of the productivity of excavators is developed thereof, in which the production rate results as a product of an ideal, maximum, productivity rate times an operating efficiency. The maximum rate is a function of the dipper capacity and the efficiency is a function of rock density, strength, and explosive energy concentration in the rock. The model is statistically significant and explains up to 92 % of the variance of the production rate measurements.

Principales efectos de la aplicación de una metodología destinada a inducir la muda en ponedoras comerciales sobre su producción cuantitativa y cualitativa durante el segundo ciclo de puesta

En la presente Tesis Doctoral se ha estudiado el efecto de una metodología para inducir la muda en dos estirpes de gallinas ponedoras comerciales, una ligera y otra semipesada, mediante el suministro de tres alimentos: salvado de trigo, cebada en grano y un pienso comercial de ponedoras aportado en cantidad restringida. Se realizaron dos pruebas en dos lotes diferentes de gallinas. En la primera de ellas se utilizaron 472 animales (236 de cada estirpe) alojados en jaulas con cuatro o seis gallinas por jaula, con una estructura factorial 2 x 3 x 2 (2 estirpes, 3 alimentos, 2 densidades) y una duración total de 32 semanas (4 de muda y 28 de producción posmuda). En la segunda prueba fueron 432 animales los utilizados (216 de cada estirpe), alojados en grupos de cuatro aves por jaula, con una estructura factorial 2 x 3 (2 estirpes, 3 alimentos) y una duración de 27 semanas (4 de muda y 23 de producción postmuda). En los dos experimentos realizados se estudió el efecto del uso de los alimentos citados para inducir de la muda sobre los resultados cuantitativos: pérdida de peso vivo durante la muda e intensidad de puesta, peso medio del huevo y masa de huevo diaria, durante y después de la muda, así como la distribución de la puesta en clases comerciales durante el segundo ciclo de puesta. Así como sobre los resultados cualitativos después de la muda: color de la cáscara de los huevos morenos, espesor de la cáscara, peso específico del huevo, altura del albumen, unidades Haugh y color de la yema. En la primera prueba se estudió, además, el efecto que la inducción de la muda mediante los tres alimentos considerados tuvo sobre la regresión del aparato reproductor de las gallinas durante este período de muda. En el primer experimento se observaron diferencias entre estirpes. Las gallinas ligeras tuvieron una más rápida regresión del aparato reproductor (ovario+oviducto) (P=0,003) que las semipesadas, aunque la regresión total no presentó diferencias significativas. Las gallinas semipesadas tuvieron mejores resultados después de la muda en intensidad de puesta (P<0,0001), en peso medio del huevo (P<0,0001) y en masa de huevo diaria (P=0,0002). También hubo diferencias significativas para las variables cualitativas espesor de la cáscara (mayor en huevos de gallinas semipesadas) mientras que los huevos procedentes de gallinas ligeras presentaron mejores valores de altura del albumen, de unidades Haugh y de color de yema; todas estas variables tuvieron un nivel de significación P<0,0001. El suministro restringido de pienso dio lugar a un mayor porcentaje de pérdida de peso vivo (P<0,0001) aunque la regresión de los órganos del aparato reproductor fue la más baja (P<0,003), no habiéndose encontrado diferencias entre los otros dos alimentos utilizados. Con este alimento también fue más lenta (P<0,0001) la disminución de la puesta durante la muda, aunque fue mayor la producción durante el segundo ciclo (P<0,0001). La única variable cualitativa afectada fue el espesor de cáscara (P<0,0001), con valores más altos en los huevos producidos por las gallinas mudadas con cebada. Los grupos de seis gallinas por jaula produjeron más huevos durante la muda (P<0,0001) aunque después de ésta la densidad de animales no tuvo efecto significativo, como tampoco lo hubo sobre los parámetros de calidad del huevo. En la segunda prueba las gallinas semipesadas experimentaron un menor porcentaje de pérdida de peso corporal (P<0,01) pero tuvieron mayores índices de puesta (P<0,001) y de huevos clasificables (P<0,001) durante la muda. En cambio, durante el segundo ciclo de producción las gallinas ligeras produjeron más huevos (P=0,0041), de menor peso (P<0,02) y con menor consumo de pienso (P<0,001). Los huevos puestos por las gallinas semipesadas tuvieron mayor espesor de cáscara y mayor color de yema, pero peor calidad de albumen (P<0,0001). La mayor pérdida de peso la experimentaron las gallinas mudadas con salvado (P<0,02). La producción durante la muda fue mayor (P<0,001) en las gallinas que consumieron pienso en cantidad restringida y también fueron las que tuvieron menor intensidad de puesta (P<0,006) y masa de huevo diaria (P<0,042) durante el segundo ciclo. El tratamiento de muda no tuvo efecto significativo sobre la calidad del huevo en esta segunda prueba. La principal conclusión que merece destacarse es que es posible inducir la muda a las gallinas ponedoras utilizando alimentos bajos en energía o en proteína, o altos en fibra, con un porcentaje de pérdida de peso vivo no tan alta como las recomendaciones tradicionales, y alcanzar buenos resultados productivos, tanto cuantitativos como cualitativos, durante el segundo ciclo de puesta. ABSTRACT Present Doctoral Thesis has studied the effect of a methodology to induce molting in two strains of commercial laying hens, one light and another semi-heavy one, through the provision of three feed: wheat bran, barley grain and a commercial laying hens feed provided in limited quantity. Two tests were performed in two different lots of layers. In the first 472 animals were used (236 of each strain) housed in cages with four or six hens per cage, with a structure 2 x 3 x 2 factorial (2 strains, 3 meals, 2 densities) and a total duration of 32 weeks (4 of molt and 28 of postmolting). In the second test 432 animals were used (216 each strain), housed in groups of four birds per cage, with a structure factorial 2 x 3 (2 strain, 3 meals) along 27 weeks (4 of molt and 23 of postmolting). In both experiments, we studied the effect of the use of above mentioned foods to induce molting on the quantitative results: body weight lost during the molt and laying index, average egg weight and egg mass daily during and after the molt, as well as on grading in commercial classes during the second laying cycle. As well as on qualitative outcomes after the molt: colour of Brown eggsshell, shell thickness, specific density, albumen height, Haugh units and yolk colour. In the first test was studied, in addition, the effect of induction of molting through the three feed considered on the regression of the reproductive tract of hens during molting period. In the first experiment, differences between strains were observed. Light hens had a faster regression of the reproductive tract (ovary+oviduct) (P=0,003) than semi-heavy hens, although the total regression did not present significant differences. Semi-heavy hens had better outcomes after the molt in laying index (P<0.0001), in average egg weight (P<0.0001) and daily egg mass (P=0, 0002). There were also significant differences for the qualitative variables (higher in semi-heavy hen eggs) as shell thickness while light chicken eggs showed better values of albumen height, Haugh units and yolk color; all these variables had the same level of significance (P<0.0001). Restricted supply of layer feed resulted in a greater percentage of live weight loss (P<0.0001) although the regression of the reproductive organs was the lowest (P<0.003), having not found differences between the other two feed used. With this food decreasing of laying during molting period was also slower (P<0.0001), although production was higher during the second cycle (P < 0.0001). The only qualitative variable affected was shell thickness (P<0.0001), with higher values in the eggs produced by hens molted with barley. Groups of six hens per cage produced more eggs during the moult (P<0.0001) but after this animal density had no significant effect, as neither had it on egg quality parameters. In the second trial hens semi-heavy experienced a lower percentage of body weight loss (P<0.01) but had higher rates of egg production (P<0.001) and of grading eggs (P<0.001) during the moult. On the other hand, during the second production cycle light hens produced more eggs (P=0,0041), of lower weight (P < 0.02) and with less feed intake (P<0.001). Eggs from semi-heavy hens had thicker shell and greater color yolk, but poorer quality of albumen (P<0.0001). The greater weight loss was experimented by the hens molted with wheat bran (P=0.02). Production during molting period was greater (P<0.001) in hens which consumed feed in restricted quantities and were also less the laying index (P=0.006) and daily egg mass (P=0.042) during the second cycle. The molting treatment had no significative effect on the quality of the egg in this second test. The main conclusion that deserves to stand out is that it is possible to induce molting hens using foods low in energy or in protein or high in fiber, with a percentage of live weight loss not as high as the traditional recommendations, and achieve good productive, both quantitative and qualitative results during the second implementation cycle.