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.
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.
We consider clay minerals, iron oxides and charcoal as major components controlling the formation of interfaces relevant for sorption of organic chemicals, as they control the assemblage of organic matter and mineral particles. We studied the formation of interfaces in batch incubation experiments with inoculated artificial soils consisting of model compounds (clay minerals, iron oxide, char) and natural soil samples. Results show a relevant contribution of both iron oxides and clay minerals to the formation of organic matter as sorptive interfaces for hydrophobic compounds. Thus, we intend to focus our work in the second phase on the characterization of the interface as formed by organic matter associated with clay minerals and iron oxides. The interfaces will be characterized by the BET-N2 and ethylene glycol monoethyl ether (EGME) methods and 129Xe and 13C NMR spectroscopy for determination of specific surface area, sorptive domains in the organic matter and microporosity. A major step forward is expected by the analysis of the composition of the interface at different resolution by reflected-light microscopy (mm scale), SEM (scanning electron microscopy, micrometer scale) and secondary ion mass spectrometry at the nanometer scale (nanoSIMS). The outcomes obtained in combination with findings from cooperation partners will help to unravel the contribution of different types of soil components on the formation and characteristics of the biogeochemical interfaces and their effect on organic chemical sorption.
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.
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.
Magnetic properties of ferrimagnetic minerals depend on their crystal lattice, anisotropy, chemical composition and grain size. The latter parameter is strongly controlled by microstructures, which are significant for the interpretation of the magnetic properties of shocked magnetic minerals. Fracturing and lattice defects are the main causes for magnetic domain size reduction and generate an increase in coercivity and the suppression of magnetic transitions (e.g. 34 K transition in pyrrhotite, Verwey transition in magnetite).Especially for an adequate investigation of shock-induced modifications in ferromagnetic minerals, a combination of microstructural and magnetic measurements is therefore essential.This project focusses on two significant aspects of extreme conditions - the consequence of shock waves on natural material on Earth and on the magnetic mineralogy of exotic magnetic minerals in iron meteorites. In order to obtain general correlations between deformation structures and magnetic properties, the specific magnetic properties and carriers as well as microstructures of samples from two impact structures in marine targets (Lockne and Chesapeake Bay) will be compared with shocked magnetite ore and magnetite-bearing target lithologies from outside the crater (Lockne) as well as from undeformed megablocks within the crater (Chesapeake Bay). We will test the hypothesis if shock-related microstructures and associated magnetic properties can significantly be overprinted by postshock hydrothermal alteration. We especially want to focus on the Verwey transition (TV) as lower TVs are described for shocked impact lithologies. Hence, the main focus of this study lies on magneto-mineralogical investigations which combine low- and high-temperature magnetic susceptibility and saturation isothermal remanent magnetization with mineralogical and microstructural investigations. The same methods will then be used for the investigation of iron meteorites, whose magnetic properties are often controled by exotic magnetic minerals like cohenite, schreibersite and daubreelite in addition to the metal phases. Magnetic transition temperatures of those phases are poorly documented in relation to their chemical composition as well as to their crystallographic and microstructural configuration. For a general understanding of shock-related magnetization processes in extraterrestrial and terrestrial material, however, it is crucial to obtain a general correlation between the initial 'unshocked' state and the subsequent shock- and alteration-related overprints.
Forschungsschwerpunkt: - Entwicklung differenzierter Materialien und E-Learning-Konzeptionen zur Qualifizierung von Zielgruppen, die in energiebezogenen Bereichen tätig sind bzw. entsprechende Qualifikationen anstreben - systematische mediendidaktische Fortentwicklung bestehender Blended-Learning-Konzeptionen. Ziele: - Vermittlung grundlegende energiewirtschaftliche Zusammenhänge für Nicht-Ökonomen, die in der Energiebranche tätig sind bzw. entsprechende Qualifikationen anstreben - Ziel ist das Erlangen vertiefter Einsichten in die verschiedenen Facetten der Energieversorgung und -nutzung, um ein breiteres Verständnis für die vielschichtigen Aufgaben und Anforderungen an Unternehmen in der Branche. Beschreibung: - Im Rahmen der ersten Projektphase wurde ein internetgestützter Qualifizierungsbaustein 'Energy Economics' entwickelt und eine internetgestützte Lehreinheit konzipiert. Diese wurde im Wintersemester 2013/2014 im Studiengang 'Engineering Physics' erprobt und evaluiert. Das Feedback der Teilnehmer fiel sehr positiv aus. - In der zweiten Projektphase (2014) ein weiterer internetgestützter Qualifizierungsbaustein entwickelt, auf dessen Basis ebenfalls eine Veranstaltung konzipiert, durchgeführt und evaluiert wird. Im Mittelpunkt steht darin die Auseinandersetzung mit den erneuerbaren Energien, insbesondere im Hinblick auf ihren Einsatz in Entwicklungs- und Schwellenländern. Die Lehrveranstaltung wird ausschließlich onlinebasiert durchgeführt werden. Ergebnisse/Materialien: Qualifizierungsbaustein 'Energy Economics', der sich thematisch mit den Schwerpunkten - grundlegende Strukturen internationaler Energiemärkte (insb. Erdöl, Erdgas, Kohle), - Besonderheiten der Märkte für leitungsgebundene Energieversorgung, - Bedeutung energiepolitischer Rahmensetzung auf den Märkten sowie - Förderung erneuerbarer Energien und ihrer Wirkung auf Märkten auseinandersetzt.
To predict ecosystem reactions to elevated atmospheric CO2 (eCO2) it is essential to understandthe interactions between plant carbon input, microbial community composition and activity and associated nutrient dynamics. Long-term observations (greater than 13 years) within the Giessen Free Air Carbon dioxide Enrichment (Giessen FACE) study on permanent grassland showed next to an enhanced biomass production an unexpected strong positive feedback effect on ecosystem respiration and nitrous oxide (N2O) production. The overall goal of this study is to understand the long-term effects of eCO2 and carbon input on microbial community composition and activity as well as the associated nitrogen dynamics, N2O production and plant N uptake in the Giessen FACE study on permanent grassland. A combination of 13CO2 pulse labelling with 15N tracing of 15NH4+ and 15NO3- will be carried out in situ. Different fractions of soil organic matter (recalcitrant, labile SOM) and the various mineral N pools in the soil (NH4+, NO3-, NO2-), gross N transformation rates, pool size dependent N2O and N2 emissions as well as N species dependent plant N uptake rates and the origin of the CO2 respiration will be quantified. Microbial analyses will include exploring changes in the composition of microbial communities involved in the turnover of NH4+, NO3-, N2O and N2, i.e. ammonia oxidizing, denitrifying, and microbial communities involved in dissimilatory nitrate reduction to ammonia (DNRA). Stable Isotope Probing (SIP) and mRNA based analyses will be employed to comparably evaluate the long-term effects of eCO2 on the structure and abundance of these communities, while transcripts of these genes will be used to target the fractions of the communities which actively contribute to N transformations.
| Origin | Count |
|---|---|
| Bund | 204 |
| Land | 1 |
| Type | Count |
|---|---|
| Förderprogramm | 204 |
| Text | 1 |
| License | Count |
|---|---|
| geschlossen | 1 |
| offen | 204 |
| Language | Count |
|---|---|
| Deutsch | 79 |
| Englisch | 153 |
| Resource type | Count |
|---|---|
| Dokument | 1 |
| Keine | 158 |
| Unbekannt | 1 |
| Webseite | 46 |
| Topic | Count |
|---|---|
| Boden | 168 |
| Lebewesen und Lebensräume | 161 |
| Luft | 153 |
| Mensch und Umwelt | 205 |
| Wasser | 140 |
| Weitere | 205 |