Die Grenzfläche zwischen Ozean und Atmosphäre ist durch einen allgegenwärtigen, < 1 mm dicken marinen Oberflächenfilm, den sogenannten sea-surface microlayer (SML), charakterisiert. Der SML ist nicht nur direkter UV-Strahlung und atmosphärischen Oxidantien ausgesetzt, sondern zeichnet sich im Vergleich zum unterliegenden Wasser auch durch höhere Konzentrationen an organischen Stoffen aus. Bisher ist unklar, welche Bedeutung die dadurch bedingten SML-spezifischen abiotischen Prozesse für die Umsetzung und die Emission organischer Stoffe insgesamt haben und wie man diese Prozesse parametrisieren kann. In diesem Projekt, das eng mit anderen Projekten der interdisziplinären Forschungsgruppe â€ÌBiogeochemische Prozesse und Ozean/Atmosphäre- Austauschprozesse in marinen Oberflächenfilmen (BASS)â€Ì verbunden ist, sollen daher molekulare Details SML-spezifischer Reaktionen (Photochemie, heterogene Oxidation, Radikalchemie) genauer untersucht werden. Ziel ist es, Reaktionsprodukte und -geschwindigkeiten quantitativ zu erfassen und Unterschiede zwischen Reaktionen im SML und in der freien Wassersäule herauszuarbeiten. Basierend auf der Expertise der drei beteiligten Arbeitsgruppen im Bereich Photochemie, Reaktionskinetik, Laserspektroskopie, Analytik und theoretischer Modellierung, soll ein molekulares Verständnis ausgewählter Reaktionen und des Einflusses der komplexen SML-Reaktionsumgebung erreicht werden. Dazu sollen experimentelle Verfahren wie Schwingungs-Summenfrequenzerzeugung, hochempfindliche Chromatographie-Massenspektrometrie und gepulste Laserphotolyse-Langwegabsorption mit Methoden der Quantenchemie und Molekulardynamik kombiniert werden. Arbeitsschwerpunkte bilden die Oxidationskinetik von Halogen- bzw. Hydroxyl-Radikalreaktionen in der flüssigen Phase, die Ozonolyse von Fettsäure-Monoschichten und die durch Photosensibilisatoren verstärkte Bildung von reaktiven Radikalen bzw. Zersetzung von organischen Schichten. Neben wohldefinierten Labor-Modellsystemen werden auch natürliche Proben analysiert werden. Dabei stellt sich z.B. die Frage nach den Einflussfaktoren der während einer Algenblüte zunehmenden Bildung von oberflächenaktiven Stoffen im SML und der Bedeutung der durch die Sonne bedingten Photolyse auf die abiotische Umsetzung organischer Stoffe. Flankierend werden im Projekt auch die eingesetzten Untersuchungsmethoden weiterentwickelt; das beinhaltet sowohl die Ausarbeitung von Messprotokollen zur Quantifizierung bestimmter organischen Substanzklassen (z.B. Carbonyle und Kohlenhydrate) im SML, die Synthese und Charakterisierung von neuartigen oberflächenaktiven Photosensibilisatoren (z.B. Benzoyl-Benzoesäure-funktionalisierte Lipide) sowie die Entwicklung und Erprobung mehrstufiger Modellierungsverfahren zur theoretischen Beschreibung von Struktur-Reaktivitätsbeziehungen der Fettsäure-Ozonolyse (z.B. Beschreibung des Einflusses sterischer und elektronischer Effekte der organischen Matrix).
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.
Bamboos (Poaceae) are widespread in tropical and subtropical forests. Particularly in Asia, bamboos are cultivated by smallholders and increasingly in large plantations. In contrast to trees, reliable assessments of water use characteristics for bamboo are very scarce. Recently we tested a set of methods for assessing bamboo water use and obtained first results. Objectives of the proposed project are (1) to further test and develop the methods, (2) to compare the water use of different bamboo species, (3) to analyze the water use to bamboo size relationship across species, and (4) to assess effects of bamboo culm density on the stand-level transpiration. The study shall be conducted in South China where bamboos are very abundant. It is planned to work in a common garden (method testing), a botanical garden (species comparison, water use to size relationship), and on-farm (effects of culm density). Method testing will include a variety of approaches (thermal dissipation probes, stem heat balance, deuterium tracing and gravimetry), whereas subsequent steps will be based on thermal methods. The results may contribute to an improved understanding of bamboo water use characteristics and a more appropriate management of bamboo with respect to water resources.
Beach sand deposits are widespread in the area around Sandefjord, at the western coast of the Oslofjord, southern Norway. The age of the deposits continuously increases with elevation, as the area has been subject to steady glacio-isostatic uplift throughout the Holocene. Existing local sea level curves provide age control related to elevation. Thus, the area offers excellent conditions to test hypotheses on soil formation and OSL dating. A chronosequence covering the last 10 000 years will be established. A preliminary study showed that soil formation leads to Podzols within 4300 - 6600 years. Micromorphological analyses suggest that clay illuviation takes place before and below podzolisation. It is hypothesised that clay translocation goes on contemporarily with podzolisation, but at greater soil depth, where the chemical conditions are suitable. This hypothesis will be proved by more detailed micromorphological investigation and chemical analyses. The factors controlling soil forming processes and their rates, will be determined by analyzing elemental composition, primary minerals and clay mineralogy. Preliminary OSL dating tests suggest that the beach sand deposits are OSL dateable despite the high latitude. This hypothesis will be checked by comparing OSL datings to ages derived from the 14C-based sea level curves.
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.
Chlorinated ethylenes are prevalent groundwater contaminants. Numerous studies have addressed the mechanism of their reductive dehalogenation during biodegradation and reaction with zero-valent iron. However, despite insight with purified enzymes and well-characterized chemical model systems, conclusive evidence has been missing that the same mechanisms do indeed prevail in real-world transformations. While dual kinetic isotope effect measurements can provide such lines of evidence, until now this approach has not been possible for chlorinated ethylenes because an adequate method for continuous flow compound specific chlorine isotope analysis has been missing. This study attempts to close this prevalent research gap by a combination of two complementary approaches. (1) A novel analytical method to measure isotope effects for carbon and chlorine. (2) A carefully chosen set of well-defined model reactants representing distinct dehalogenation mechanisms believed to be important in real-world systems. Isotope trends observed in biotic and abiotic environmental dehalogenation will be compared to these model reactions, and the respective mechanistic hypotheses will be confirmed or discarded. With this hypothesis-driven approach it is our goal to elucidate for the first timdehalogenation reactions.
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.
Perennial fodder cropping potentially increases subsoil biopore density by formation of extensive root systems and temporary soil rest. We will quantify root length density, earthworm abundance and biopore size classes after Medicago sativa, Cichorium intybus and Festuca arundinacea grown for 1, 2 and 3 years respectively in the applied research unit's Central Field Trial (CeFiT) which is established and maintained by our working group. Shoot parameters including transpiration, gas exchange and chlorophyll fluorescence will frequently be recorded. Precrop effects on oilseed rape and cereals will be quantified with regard to crop yield, nutrient transfer and H2-release. The soil associated with biopores (i.e. the driloshpere) is generally rich in nutrients as compared to the bulk soil and is therefore supposed to be a potential hot spot for nutrient acquisition. However, contact areas between roots and the pore wall have been reported to be low. It is still unclear to which extent the nutrients present in the drilosphere are used and which potential relevance subsoil biopores may have for the nutrient supply of crops. We will use a flexible videoscope to determine the root-soil contact in biopores. Nitrogen input into the drilosphere by earthworms and potential re-uptake of nitrogen from the drilosphere by subsequent crops with different rooting systems (oilseed rape vs. cereals) will be quantified using 15N as a tracer.
Im Auftrag des Bayerischen Landesamtes für Umwelt hat bifa den erstmals 2003 durchgeführten Ökoeffizienzvergleich der Entsorgungsstrukturen Bayerns, Deutschlands und der Schweiz erweitert und aktualisiert. Die Ergebnisse aus dem Jahr 2003 zeigten, dass der bayerische Weg zur Gestaltung der Abfallwirtschaft in seiner Ökoeffizienz im Vergleich mit den Entsorgungsstrukturen der Schweiz und dem deutschen Durchschnitt am besten abschnitt. Nach der, im Rahmen der aktuellen Beauftragung, durchgeführten Datenaktualisierung, der Bilanzierung zusätzlicher Wertstoffströme und der Berücksichtigung des Verbots der Ablagerung nicht vorbehandelter Abfälle rücken die Entsorgungsstrukturen hinsichtlich Ihrer Ökoeffizienz deutlich enger zusammen. Die Entsorgungsstruktur Bayerns weist im Vergleich zur Entsorgungsstruktur Deutschlands zwar noch ein geringfügig besseres ökologisches Gesamtergebnis auf, ist aber gleichzeitig mit leicht höheren Gesamtkosten verbunden. Die Entsorgungsstruktur der Schweiz ist etwas weniger ökoeffizient. Die Ursachen dafür sind eine geringere Umweltentlastung im ökologischen Gesamtergebnis, gepaart mit vergleichsweise hohen Entsorgungskosten. Methoden: Analyse und Moderation sozialer Prozesse, Ökobilanzierung und Systemanalyse, Ökonomie und Managementberatung.
In dem Vorhaben wird untersucht, wie wirksam die absorbierte Lichtenergie in Biomasse konvertiert wird. Vergleichend werden Grünalgen und Diatomeen unter verschiedenen Licht- und Nährstoffbedingungen studiert. Auf diese Weise können die metabolischen Kosten unter Nährstoffmangel oder anderen produktivitätsbegrenzenden Bedingungen studiert werden. So wird auch die Säureanpassung ausgewählter Phytoplankter untersucht, um die Biomassebildung in extrem sauren Tagebaurestseen auf physiologischer Ebene zu verstehen. Es konnte gezeigt werden, dass unter Stickstoffmangel die Überführung anorganischen Kohlenstoffs in Biomassebildung durch eine Veränderung der makromolekularen Zusammensetzung der Zellen ähnlicher Effizienz stattfindet, wie unter optimaler Stickstoffversorgung. Dies führt zu einer ökologisch bedeutsamen Teilentkopplung des C und N Kreislaufs im Ökosystem. Ähnliches beobachtet man auch bei der Anpassung von Phytoplanktonalgen an extrem saure Bedingungen wie man sie in sauren Tagebaurestseen vorfindet.
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