In bog ecosystems, vegetation controls key processes such as the retention of carbon, water and nutrients. In northern hemispherical bogs, a shift from Sphagnum- to vascular plant-dominated vegetation is often traced back to Climate Change and increased anthropogenic nitrogen deposition and coincides with substantially reduced capacities in carbon, water and nutrient retention. In southern Patagonia, bogs dominated by Sphagnum and vascular plants coexist since millennia under similar environmental settings. Thus, South Patagonian bogs may serve as ideal examples for the long-term effect of vascular plant invasion on carbon, water and nutrient balances of bog ecosystems. The contemporary balances of carbon and water of both a bog dominated by Sphagnum and vascular plants are determined by CO2- H2O and CH4 flux measurements and an estimation of lateral water losses as well as losses via dissolved organic and inorganic carbon compounds. The high time resolution of simultaneous eddy covariance measurements of CO2 and H2O in both bog types and the strong interaction between climatic variables and the physiology of bog plants allow for direct comparisons of carbon and water fluxes during cold, warm, dry, wet, cloudy or sunny periods. By the combination with leaf-scale measurements of gas exchange and fluorescence, plant-physiological controls of photosynthesis and transpiration can be identified. Long-term peat accumulation rates will be determined by carbon density and age-depth profiles including a characterization of peat humification characteristics. A reciprocal transplantation experiment with incorporated shading, liming and labeled N addition treatments is conducted to explore driving factors affecting competition between Sphagnum and vascular plants as well as the interactions between CO2-, CH4-, and water fluxes and decisive plant functional traits affecting key processes for carbon sequestration and nutrient cycling. Decomposition rates and driving below ground processes are analyzed with a litter bag field experiment and an incubation experiment in the laboratory.
The relevance of biogeochemical gradients for turnover of organic matter and contaminants is yet poorly understood. This study aims at the identification and quantification of the interaction of different redox processes along gradients. The interaction of iron-, and sulfate reduction and methanogenesis will be studied in controlled batch and column experiments. Factors constraining the accessibility and the energy yield from the use of these electron acceptors will be evaluated, such as passivation of iron oxides, re-oxidation of hydrogen sulfide on iron oxides. The impact of these constraints on the competitiveness of the particular process will then be described. Special focus will be put on the evolution of methanogenic conditions in systems formerly characterized by iron and sulfate reducing condition. As methanogenic conditions mostly evolve from micro-niches, methods to study the existence, evolution and stability of such micro-niches will be established. To this end, a combination of Gibbs free energy calculations, isotope fractionation and tracer measurements, and mass balances of metabolic intermediates (small pool sizes) and end products (large pool sizes) will be used. Measurements of these parameters on different scales using microelectrodes (mm scale), micro sampling devices for solutes and gases (cm scale) and mass flow balancing (column/reactor scale) will be compared to characterize unit volumes for organic matter degradation pathways and electron flow. Of particular interest will be the impact of redox active humic substances on the competitiveness of involved terminal electron accepting processes, either acting as electron shuttles or directly providing electron accepting capacity. This will be studied using fluorescence spectroscopy and parallel factor analysis (PARAFAC) of the gained spectra. We expect that the results will provide a basis for improving reactive transport models of anaerobic processes in aquifers and sediments.
Dissolved organic matter (DOM) is one major source of subsoil organic matter (OM). P5 aims at quantifying the impact of DOM input, transport, and transformation to the OC storage in the subsoil environment. The central hypotheses of this proposal are that in matric soil the increasing 14C age of organic carbon (OC) with soil depth is due to a cascade effect, thus, leading to old OC in young subsoil, whereas within preferential flowpaths sorptive stabilization is weak, and young and bioa-vailable DOM is translocated to the subsoil at high quantities. These hypotheses will be tested by a combination of DOC flux measurements with the comparative analysis of the composition and the turnover of DOM and mineral-associated OM. The work programme utilizes a DOM monitoring at the Grinderwald subsoil observatory, supplemented by defined experiments under field and labora-tory conditions, and laboratory DOM leaching experiments on soils of regional variability. A central aspect of the experiments is the link of a 13C-leaf litter labelling experiment to the 14C age of DOM and OM. With that P5 contributes to the grand goal of the research unit and addresses the general hypotheses that subsoil OM largely consists of displaced and old OM from overlying horizons, the sorption capacity of DOM and the pool size of mineral-associated OM are controlled by interaction with minerals, and that preferential flowpaths represent 'hot spots' of high substrate availability.
The geomagnetic field shields our habitat against solar wind and radiation from space. Due to the geometry of the field, the shielding in general is weakest at high latitudes. It is also anomalously weak in a region around the south Atlantic known as South Atlantic Anomaly (SAA), and the global dipole moment has been decreasing by nearly 10 percent since direct measurements of field intensity became possible in 1832. Due to our limited understanding of the geodynamo processes in Earths core, it is impossible to reliably predict the future evolution of both dipole moment and SAA over the coming decades. However, lack of magnetic field shielding as would be a consequence of further weakening of dipole moment and SAA region field intensity would cause increasing problems for modern technology, in particular satellites, which are vulnerable to radiation damage. A better understanding of the underlying processes is required to estimate the future development of magnetic field characteristics. The study of the past evolution of such characteristics based on historical, archeo- and paleomagnetic data, on time-scales of centuries to millennia, is essential to detect any recurrences and periodicities and provide new insights in dynamo processes in comparison to or in combination with numerical dynamo simulations. We propose to develop two new global spherical harmonic geomagnetic field models, spanning 1 and 10 kyrs, respectively, and designed in particular to study how long the uninterrupted decay of the dipole moment has been going on prior to 1832, and if the SAA is a recurring structure of the field.We will combine for the first time all available historical and archeomagnetic data, both directions and intensities, in a spherical harmonic model spanning the past 1000 years. Existing modelling methods will be adapted accordingly, and existing data bases will be complemented with newly published data. We will further acquire some new archeomagnetic data from the Cape Verde islands from historical times to better constrain the early evolution of the present-day SAA. In order to study the long-term field evolution and possible recurrences of similar weak field structures in this region, we will produce new paleomagnetic records from available marine sediment cores off the coasts of West Africa, Brazil and Chile. This region is weakly constrained in previous millennial scale models. Apart from our main aim to gain better insights into the previous evolution of dipole moment and SAA, the models will be used to study relations between dipole and non-dipole field contributions, hemispheric symmetries and large-scale flux patterns at the core-mantle boundary. These observational findings will provide new insights into geodynamo processes when compared with numerical dynamo simulation results.Moreover, the models can be used to estimate past geomagnetic shielding above Earths surface against solar wind and for nuclide production from galactic cosmic rays.
For surface soils, the mechanisms controlling soil organic C turnover have been thoroughly investigated. The database on subsoil C dynamics, however, is scarce, although greater than 50 percent of SOC stocks are stored in deeper soil horizons. The transfer of results obtained from surface soil studies to deeper soil horizons is limited, because soil organic matter (SOM) in deeper soil layers is exposed to contrasting environmental conditions (e.g. more constant temperature and moisture regime, higher CO2 and lower O2 concentrations, increasing N and P limitation to C mineralization with soil depth) and differs in composition compared to SOM of the surface layer, which in turn entails differences in its decomposition. For a quantitative analysis of subsoil SOC dynamics, it is necessary to trace the origins of the soil organic compounds and the pathways of their transformations. Since SOM is composed of various C pools which turn over on different time scales, from hours to millennia, bulk measurements do not reflect the response of specific pools to both transient and long-term change and may significantly underestimate CO2 fluxes. More detailed information can be gained from the fractionation of subsoil SOM into different functional pools in combination with the use of stable and radioactive isotopes. Additionally, soil-respired CO2 isotopic signatures can be used to understand the role of environmental factors on the rate of SOM decomposition and the magnitude and source of CO2 fluxes. The aims of this study are to (i) determine CO2 production and subsoil C mineralization in situ, (ii) investigate the vertical distribution and origin of CO2 in the soil profile using 14CO2 and 13CO2 analyses in the Grinderwald, and to (iii) determine the effect of environmental controls (temperature, oxygen) on subsoil C turnover. We hypothesize that in-situ CO2 production in subsoils is mainly controlled by root distribution and activity and that CO2 produced in deeper soil depth derives to a large part from the mineralization of fresh root derived C inputs. Further, we hypothesize that a large part of the subsoil C is potentially degradable, but is mineralized slower compared with the surface soil due to possible temperature or oxygen limitation.
Eine Brennstoffzelle als Primärenergiequelle mit einem Doppelschichtkondensator (Supercap) als Zwischenspeicher zu kombinieren ist ein vielversprechender Ansatz für zukünftige Elektrofahrzeuge. In Kooperation mit einem Fahrzeughersteller wurden verschiedene Strategien für ein Energiemanagement für die Kombination einer Brennstoffzelle mit einem Doppelschichtkondensatormodul entworfen und verglichen. Basierend auf der aktuellen Geschwindigkeit und Beschleunigung werden verschiedene Fahrzeugzustände bezüglich kinetischer Energie und Leistungsbedarf unterschieden. In Abhängigkeit von der verfügbaren Leistung von Supercaps und Brennstoffzelle wird eine optimale Leistungsaufteilung zwischen den beiden Energiequellen ermittelt. In Bremsphasen wird durch Rekuperation Energie zurückgewonnen und in den Supercaps gespeichert. Wenn die Supercaps vollgeladen sind oder ihre maximale Ladeleistung erreicht haben, übernehmen mechanische Bremsen die übrige Ladeleistung. Da diese Situation zu einem Energieverlust führt, sollte sie möglichst vermieden werden. Um immer die notwendige Beschleunigungsleistung und gleichzeitig auch ein Maximum an Rekuperation zu garantieren, wird der Ladezustand der Supercaps kontinuierlich und dynamisch an die kinetische Energie des Fahrzeugs angepasst. Verschiedene Strategien wurden in Matlab/Simulink mit einem Stateflow-Chart zur Abbildung der Zustände implementiert. Die verfügbare Supercapleistung wird mit Hilfe eines impedanzbasierten Modells für Supercaps berechnet. Mit diesen Strategiemodellen können die Leistungsfähigkeit der verschiedenen Strategien verglichen und die Einflüsse von Parametern untersucht werden. Ziel eines Energiemanagements ist es, den Wasserstoffverbrauch zu minimieren und die notwendige Leistung zu jeder Zeit sicherzustellen. Bei der Bewertung der Strategien wird der Wasserstoffverbrauch, die verlorene Bremsenergie und eine mögliche Geschwindigkeitsreduzierung verglichen. Mit einer optimalen Strategie können bis zu 23 Prozent Wasserstoff während eines definierten Fahrprofils gespart werden.
Die Beobachtungen der Radio Science Experimente Mars Express Radio Science, Mars Global Surveyor Radio Science und Venus Express Radio Science liefern eine sehr große Datenbasis für die Elektronendichteverteilung der Tagionosphäre von Mars und Venus. In der Laufzeit des Original-Antrags erfolgte die Ableitung von Profileigenschaften/Umgebungsparametern und die Entwicklung eines schnellen, flexiblen zeitunabhängigen photochemischen Modells der ionosphärischen Elektronendichte (IonA-1) für Mars (Neutralatmosphäre: Mars Climate Database) und Venus (Neutralatmosphäre: VenusGRAM). Der Vergleich der beobachteten und modellierten MaRS und VeRa Parameter des ionosphärischen Hauptmaximums (M2/V2) ergaben für Mars global eine exzellente Übereinstimmung, aber nicht für Venus (unrealistische VenusGRAM Neutralatmosphäre, Peter et al., 2014). Für die Modellierung kleinskaliger Ionosphärenmerkmale wird jedoch die individuelle Übereinstimmung der jeweiligen M2/V2 Höhen und Breiten benötigt, da dies auf Ähnlichkeiten zwischen realer und Modellatmosphäre zur Zeit der Beobachtung hinweist. Für die Modellierung von Meteorschichten unterhalb der Sekundärschicht M1/V1 wurden Fallstudien mit entsprechenden MaRS Profilen in Kombination mit einem Modell für Meteorschichten (IonA/MSDM) durchgeführt. MSDM berücksichtigt die Deponierung von Mg und Fe in eine Atmosphäre und simuliert die Bildung von Metallionen durch Photoionisation/Ladungsaustausch. Ein zusätzlich entwickeltes hydrostatisches 1D Modell der Neutralatmosphäre für ionosphärischen Höhen (NIA) bildet als flexiblere Neutralatmosphäre mit kleinskaligem Höhengitter die Basis für die Anwendung von IonA auf einen größeren Beobachtungsdatensatz. Die Weiterentwicklung von IonA-1 zu einem zeitabhängigen photochemischen Modell mit komplexem Reaktionsschema (Iona-2) ermöglicht die Modellierung von ionosphärischen Ionen. Der Fortsetzungsantrag soll NIA und IonA-2 koppeln, um ein detaillierteres Verständnis der Wechselwirkung zwischen den Ionosphären und Neutralatmosphären in ionosphärischen Höhen zu erreichen. Die Radio Science Beobachtungen der unteren Neutralatmosphäre erfolgen fast zeitgleich mit den Ionosphärenbeobachtungen und bietet so eine erste Abschätzung der Neutraldichte für NIA. Das gekoppelte Modell der Neutralatmosphäre/Ionosphäre mit konsistenter Berechnung der Neutral, Ionen- und Elektronentemperaturen (a) deckt den transportdominierten Bereich der Ionosphäre oberhalb von M2/V2 ab, (b) liefert eine realistischere Modellierung der Anomalien unterhalb von M1/V1, (c) schätzt den Beitrag der sekundären Ionisation in M1/V1/M2/V2 ab, (d) liefert Erklärungen für den sog. Bulge, eine anomale Anhäufung von Elektronen in der Topside und (e) stellt mögliche Zustände der Neutralatmosphäre in ionosphärischen Höhen während der Beobachtungen zur Verfügung. Der letzte Punkt dient der Weiterentwicklung von globalen Zirkulationsmodellen, besonders für Venus, da die Datenlage im entsprechenden Höhenbereich sehr schlecht ist.
Terrestrial green algae and cyanobacteria are typical and abundant components of biological soil crusts in the Polar Regions. These communities form water-stable aggregates that have important ecological roles in primary production, nitrogen fixation, nutrient cycling, water retention and stabilization of soils. Although available data on green algae and cyanobacteria are generally very limited for the Arctic and Antarctica, their functional importance as ecosystem developers in nutrient poor environments is regarded as high. Therefore, the main goal of the interdisciplinary project is, for the first time, a precise evaluation of their 1.) Biodiversity as well as of 2.) The infra-specific genetic diversity, 3.) ecophysiological performance and 4.) transcriptomics of the most abundant taxa in biological soil crusts isolated from the Antarctic Peninsula and Arctic Svalbard. Biodiversity will be investigated using a classical culture approach in combination with molecular-taxonomical methods as well as with metagenomics. The infra-specific genetic diversity of the most abundant green algae and cyanobacteria will be studied using fingerprinting techniques, and a range of selected populations characterized in relation to their physiological plasticity. Temperature and water availability, two key environmental factors for terrestrial organisms, are currently changing in Polar Regions due to global warming, and hence their effect on growth and photosynthesis response patterns will be comparatively investigated. The data will indicate whether and how global change influence population structure and ecological performance of key organisms in polar soil crusts, and help to make predictions on the future significance of the ecological functions of these pioneer communities. Such a multiphasic approach has never been applied before to soil algae and cyanobacteria in both Polar Regions, and hence represents one of the key innovations of this proposal.
The magnetosphere of a planet is controlled by a number of factors such as the intrinsic magnetic field, the atmosphere and ionosphere, and the solar wind. Different combinations of these control factors are at work at the terrestrial planets Mercury, Venus, Earth, and Mars, hence they form a very suitable set for quantitative comparative studies. A significant intrinsic dipolar magnetic field is present only on Earth and on Mercury. However, the configuration at Mercury differs considerably from that at Earth because Mercury does not support an atmosphere and ionosphere, the dipolar field is much weaker, the solar wind denser, and the interplanetary magnetic field stronger. Both Mars and Venus have atmospheres but lack a global planetary magnetic field, with regional crustal magnetization being present on Mars. This proposal aims at investigating and comparing electrical current systems in the space environments of terrestrial planets using magnetic vector data collected by orbiting spacecraft such as Venus Express, Mars Global Surveyor, CHAMP (Earth), and MESSENGER (Mercury). We propose to construct data-driven and physically meaningful representations that reveal and quantify the influence of various control factors. To achieve this, we will tailor Empirical Orthogonal Function (EOF) analysis and other multivariate methods to the specifics of planetary magnetic field observations. In contrast to representations that build on predefined functions like spherical harmonics, basis functions in the EOF approach are derived directly from the data. EOFs are designed to extract dominant coherent variations for further interpretation in terms of known physical phenomena, and then, in a regression step, for modeling using suitable control variables. The EOF methodology thus allows quantifying the relative importance of control factors for each planet individually, and thus contributes to the solution of topical science questions. The resulting empirical models will facilitate comparative studies of current systems at the terrestrial planets.
Groundwater contamination by organic compounds represents a widespread environmental problem. The heterogeneity of geological formations and the complexity of physical and biogeochemical subsurface processes, often hamper a quantitative characterization of contaminated aquifers. Compound specific stable isotope analysis (CSIA) has emerged as a novel approach to investigate contaminant transformation and to relate contaminant sources to downgradient contamination. This method generally assumes that only (bio)chemical transformations are associated with isotope effects. However, recent studies have revealed isotope fractionation of organic contaminants by physical processes, therefore pointing to the need of further research to determine the influence of both transport and reactive processes on the observed overall isotope fractionation. While the effect of gasphase diffusion on isotope ratios has been studied in detail, possible effects of aqueous phase diffusion and dispersion have received little attention so far.The goals of this study are to quantify carbon (13C/12C) and, for chlorinated compounds, chlorine (37Cl/35Cl) isotope fractionation during diffusive/dispersive transport of organic contaminants in groundwater and to determine its consequences for source allocation and assessment of reactive processes using isotopes. The proposed research is based on the combination of high-resolution experimental studies, both at the laboratory (i.e. zero-, one- and two-dimensional systems) and at the field scales, and solute transport modeling. The project combines the expertise in the field of contaminant transport with the expertise on isotope methods in contaminant hydrogeology.
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