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MRH Wissenschaft und Forschung

Der Datensatz enthält Hochschulen und Forschungseinrichtungen in der Metropolregion Hamburg. Hochschulen bilden die Grundlage für spezialisierten Aufbau von Wissen. Über die Metropolregion verteilt bieten diverse, teils auch kleinere private Hochschulen international ausgerichtete Standards an. Neben den Hochschulen beheimatet die Metropolregion eine große Zahl an weltweit renommierten Forschungseinrichtungen, die in ihrer Bandbreite die Internationalität der Metropolregion widerspiegeln. Detailliertere Informationen zu diesen Themen erhalten Sie auf den Internetseiten der Metropolregion Hamburg unter: https://metropolregion.hamburg.de/wirtschaft-wissenschaft/hochschulen und https://metropolregion.hamburg.de/wirtschaft-wissenschaft/forschungseinrichtungen Hochschulen und Forschungseinrichtungen dominieren dieses Thema. Die Hochschulen bilden die Grundlage für spezialisierten Aufbau von Wissen. Über die Metropolregion verteilt bieten diverse , teils auch kleinere private Hochschulen international ausgerichtete Standards an. Neben den Hochschulen beheimatet die Metropolregion eine große Zahl an weltweit renommierten Forschungseinrichtungen, die in ihrer bandbreite die Internationalität der Metropolregion widerspiegelt. Unterschiedlichste Bereiche werden dabei abgedeckt. Detailiertere Informationen zu diesen Themen erhalten Sie auf den Internetseiten der Metropolregion Hamburg unter: http://metropolregion.hamburg.de/hochschulen/ und http://metropolregion.hamburg.de/forschungseinrichtungen/

Dynamic (redox) interfaces in soil - Carbon turnover in microbial biomass and flux into soil organic matter

Existing models of soil organic matter (SOM) formation consider plant material as the main source of SOM. Recent results from nuclear magnetic resonance analyses of SOM and from own incubation studies, however, show that microbial residues also contribute to a large extent to SOM formation. Scanning electron microscopy showed that the soil mineral sur-faces are covered by numerous small patchy fragments (100 - 500 nm) deriving from microbial cell wall residues. We will study the formation and fate of these patchy fragments as continuously produced interfaces in artificial soil systems (quartz, montmorillonite, iron oxides, bacteria and carbon sources). We will quantify the relative contributions of different types of soil organisms to patchy fragment formation and elucidate the effect of redox con-ditions and iron mineralogy on the formation and turnover of patchy fragments. The develop-ment of patchy fragments during pedogenesis will be followed by studying soil samples from a chronosequence in the forefield of the retreating Damma glacier. We will characterize chemical and physical properties of the patchy fragments by nanothermal analysis and microscale condensation experiments in an environmental scanning electron microscope. The results will help understanding the processes at and characteristics of biogeochemical interfaces.

DFG Trilateral collaboration Deutschland-Israel-Palestine: 'Biotic and abiotic factor affecting biological soil crust formation and recovery in a semiarid dune ecosystem : Gaza and NW Negev'

Sandy soils of the arid/semiarid dune fields of the Palestinian Gaza Strip and the Israeli western Negev are extensively covered by biological soil crusts (BSC), which stabilize the surface and prevent desertification. Political discussions in Israel suggest transferring a large part of this sand belt to the Gaza Strip within a final peace accord. Inappropriate land uses may lead to destruction of the BSC and initiate desertification, as already occurring in parts of the Gaza Strip. In this interdisciplinary project the influence of environmental factors on the vitality, stability and the recovery potential of the BSC will be investigated in order to evaluate the carrying capacity of this fragile landscape, in relation to rainfall, soil and relief conditions. A transect stretching from the Mediterranean coast in the Palestinian Gaza Strip (370 mm rainfall) to 65 km southwards in Israel ( Nizzana , less than 100 mm rainfall) has been selected. The interactions of molecular biological, physiological, physical and soil chemical processes, expressed in specific characteristics of the BSC and the underlying soil, will be assessed from the molecular to the landscape scale.

Europaeischer Pool Informations- und Schulungsmaterialien Solartechnik (EUPOS)

Root distribution and dynamics and their contribution to subsoil C-fluxes

It has been suggested that dying and decaying fine roots and root exudation represent important, if not the most important, sources of soil organic carbon (SOC) in forest soils. This may be especially true for deep-reaching roots in the subsoil, but precise data to prove this assumption are lacking. This subproject (1) examines the distribution and abundance of fine roots (greater than 2 mm diameter) and coarse roots (greater than 2 mm) in the subsoil to 240 cm depth of the three subsoil observatories in a mature European beech (Fagus sylvatica) stand, (2) quantifies the turnover of beech fine roots by direct observation (mini-rhizotron approach), (3) measures the decomposition of dead fine root mass in different soil depths, and (4) quantifies root exudation and the N-uptake potential with novel techniques under in situ conditions with the aim (i) to quantify the C flux to the SOC pool upon root death in the subsoil, (ii) to obtain a quantitative estimate of root exudation in the subsoil, and (iii) to assess the uptake activity of fine roots in the subsoil as compared to roots in the topsoil. Key methods applied are (a) the microscopic distinction between live and dead fine root mass, (b) the estimation of fine and coarse root age by the 14C bomb approach and annual ring counting in roots, (c) the direct observation of the formation and disappearance of fine roots in rhizotron tubes by sequential root imaging (CI-600 system, CID) and the calculation of root turnover, (d) the measurement of root litter decomposition using litter bags under field and controlled laboratory conditions, (e) the estimation of root N-uptake capacity by exposing intact fine roots to 15NH4+ and 15NO3- solutions, and (f) the measurement of root exudation by exposing intact fine root branches to trap solutions in cuvettes in the field and analysing for carbohydrates and amino acids by HPLC and Py-FIMS (cooperation with Prof. A. Fischer, University of Trier). The obtained data will be analysed for differences in root abundance and activity between subsoil (100-200 cm) and topsoil (0-20 cm) and will be related to soil chemical and soil biological data collected by the partner projects that may control root turnover and exudation in the subsoil. In a supplementary study, fine root biomass distribution and root turnover will also be studied at the four additional beech sites for examining root-borne C fluxes in the subsoil of beech forests under contrasting soil conditions of different geological substrates (Triassic limestone and sandstone, Quaternary sand and loess deposits).

Schwerpunktprogramm (SPP) 1315: Biogeochemische Grenzflächen in Böden; Biogeochemical Interfaces in Soil, Importance of soil organic carbon and mineral particle size fractions for the fate of soil supplied organic chemicals and their microbial transformations

The biogeochemical interface (BGI) in this project is defined as the organo-mineral surface of soil particles colonized by microorganisms. In the preceding project it was demonstrated that the different soil particle size fractions were associated with specifically structured microbial communities, a characteristic amount of soil organic carbon, and a specific capacity for adsorption of the organic chemicals phenol and 2,4-dichlorophenol, respectively. While the diversity of the microbial community was responsive to fertilization-determined additional organic soil carbon in the larger particle size fractions, it was unaffected in clay. Stable isotope probing with 13C-labelled phenol and 2,4-dichlorophenol revealed that the soil organic carbon in the BGIs also affected the diversity of microorganisms involved in the degradation of these chemicals. All these results are yet only based on studying one soil with three organic carbon variants (Bad Lauchstädt) and only two organic compounds. The objective of this 2nd phase project is to apply the innovative technology developed in the 1st phase for studying the BGI processes with soil organic carbon variants from another soil (Ultuna, SPP 1315 site) and with the chiralic anilide Fungicide metalaxyl as an additional compound. This 2nd phase SPP 1315 project will also, in a collaborative effort with two other SPP 1315 partners, investigate (1) the importance of BGIs for the entantio-selective degradation of metalaxyl and (2) the role of soil microorganisms in the formation of bound residues, respectively. Furthermore, the project will utilize stable isotope probing and next-generation DNA sequencing to link the structural and functional diversity of the microbial communities responsible for metabolism of organic chemicals in the different BGIs determined by particle size fractions and soil organic carbon variants.

Die Strukturen der Tagionosphären von Mars und Venus: Vergleich und Interpretation eines schnellen und flexiblen Modells mit laufenden Beobachtungen

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.

Physicochemical Aging Mechanisms in Soil Organic Matter (SOM- AGING): II. Hydration-dehydration mechanisms at Biogeochemical Interfaces

Soil organic matter (SOM) controls large part of the processes occurring at biogeochemical interfaces in soil and may contribute to sequestration of organic chemicals. Our central hypothesis is that sequestration of organic chemicals is driven by physicochemical SOM matrix aging. The underlying processes are the formation and disruption of intermolecular bridges of water molecules (WAMB) and of multivalent cations (CAB) between individual SOM segments or between SOM and minerals in close interaction with hydration and dehydration mechanisms. Understanding the role of these mediated interactions will shed new light on the processes controlling functioning and dynamics of biogeochemical interfaces (BGI). We will assess mobility of SOM structural elements and sorbed organic chemicals via advanced solid state NMR techniques and desorption kinetics and combine these with 1H-NMR-Relaxometry and advanced methods of thermal analysis including DSC, TGADSC- MS and AFM-nanothermal analysis. Via controlled heating/cooling cycles, moistening/drying cycles and targeted modification of SOM, reconstruction of our model hypotheses by computational chemistry (collaboration Gerzabek) and participation at two larger joint experiments within the SPP, we will establish the relation between SOM sequestration potential, SOM structural characteristics, hydration-dehydration mechanisms, biological activity and biogechemical functioning. This will link processes operative on the molecular scale to phenomena on higher scales.

Schwerpunktprogramm (SPP) 1488: Planetary Magnetism (PlanetMag), Ground-truthing magnetic recording in meteorites

Whether primordial bodies in the solar system possessed internally-generated dynamos is a fundamental constraint to understand the dynamics and timing of early planetary formation. Paleointensity studies on several meteorites reveal that their host planets possessed magnetic fields within an order-of magnitude of the present Earths field. Interpretation of paleointensity data relies heavily on fundamental knowledge of the magnetic properties of the magnetic carriers, such as the single to multidomain size threshold or how the saturation magnetization varies as a function of grain size, yet very little knowledge exists about these key parameters for some of the main magnetic recorders in meteorites: the iron-nickel alloys. Moreover, most meteorites have experienced some amount of shock during their histories, yet the consequence of even very small stresses on paleointensity data is poorly known.We wish to fill these gaps by magnetically characterizing Fe-Ni alloys as a function of grain size and by determining how absolute and relative paleointensity data are biased by strain levels lower than those petrologically observable (less than 4-5 GPa). For example, our preliminary work shows that an imposed stress of 0.6 GPa will reduce absolute paleointensity estimates by 46Prozent for single domain magnetite-bearing rocks. In general, paleointensity determinations possess inherent disadvantages regarding measurement precision and the inordinate amount of human time investment. We intend to overcome these limitations by extending and improving our fully automated magnetic workstation known as the SushiBar.

Polen auf dem Weg in die Europaeische Union - Chancen, Notwendigkeiten und Moeglichkeiten im Umweltschutz

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