We study the effects of plants and root-associated fungi on wind erosion within the alpine environment of Tibet. China is one of the countries most affected by desertification processes and Tibet, in particular, a key region in desertification combat. The presented project focuses on the Barkha Plain surrounded by Mount Kailash and the Lake of Manasarovar (Ngari Prefecture). This Western Tibet region experienced little scientific attention but, nowadays, faces rapidly increasing touristic activities and expanding local settlements associated with socio-economic changes that are serious threats to the delicate ecological balance and potential triggers of desertification. It exists almost unanimous agreement that revegetation is the most efficient and promising strategy to combat wind erosion and desertification in the long term. However, re-colonising success is often poor, mainly under extreme environmental conditions. Compared to conventional practices, the approach of the presented project attains better accordance with natural succession processes and promises acceleration of both plant and soil development and, conclusively, more efficient desertification control. The project assesses the potential of native plants and symbiotic fungi to control wind erosion and desertification processes. It aims to identify key plants and fungi that increase soil aggregate stability and efficiently drive succession into a natural and self-maintaining cycle of the ecosystem. Furthermore, it provides crucial information for implementing environmentally compatible and cost-effective measures to protect high-elevation ecosystems against desertification. Within three successional stages (early, intermediate, late), field investigations are performed on the basis of Modified-Whittaker plots. Classic methods of vegetation analysis and myco-sociology are combined with analysis of distribution patterns at different scales (patchiness, connectivity). Comprehensive soil analysis is performed comprising grain size distribution, aggregate stability, pH as well as water and nutrient contents. Additionally, important parameters of wind erosion are measured concurrently and continuously to assess their magnitude and variability with respect to vegetation and soil at different levels of development. The parameters addressed, include sediment transport, air temperature, radiation, precipitation, relative humidity as well as speed and direction of wind. Surface moisture is recorded periodically and roughness described. Species and environmental parameters are checked for spatial correlation. Cutting edge technologies are applied in laboratory work, comprising molecular methods for fungal species identification and micro-tomography to analyse soil structure. Furthermore, successfully cultivated fungi and plants are subject of synthesis experiments and industrial propagation in view of practical implementation in restoration measures.
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.
Der Verlauf der atmosphärischen CO2-Konzentrationen während der vergangenen Klimazyklen ist durch ein Sägezahnmuster mit Maxima in Warmzeiten und Minima in Kaltzeiten geprägt. Es besteht derzeit Konsens, dass insbesondere der Süd Ozean (SO) eine Schlüsselfunktion bei der Steuerung der CO2-Entwicklung einnimmt. Allerdings sind die dabei wirksamen Mechanismen, die in Zusammenhang mit Änderungen der Windmuster, Ozeanzirkulation, Stratifizierung der Wassersäule, Meereisausdehnung und biologischer Produktion stehen, noch nicht ausreichend bekannt. Daten zur Wirkung dieser Prozesse im Wechsel von Warm- und Kaltzeiten beziehen sich bislang fast ausschließlich auf den atlantischen SO. Um ein umfassendes Bild der Klimasteuerung durch den SO zu erhalten muss geklärt werden, wie weit sich die aus dem atlantischen SO bekannten Prozesswirkungen auf den pazifischen SO übertragen lassen. Dies ist deshalb von Bedeutung, da der pazifische SO den größten Teil des SO einnimmt. Darüber hinaus stellt er das hauptsächliche Abflussgebiet des Westantarktischen Eisschildes (WAIS) in den SO dar. Im Rahmen des Projektes sollen mit einer neu entwickelten Proxy-Methode Paläoumwelt-Zeitreihen an ausgewählten Sedimentkernen von latitudinalen Schnitten über den pazifischen SO hinweg gewonnen werden. Dabei handelt es sich um kombinierte Sauerstoff- und Siliziumisotopenmessungen an gereinigten Diatomeen und Radiolarien. Es sollen erstmalig die physikalischen Eigenschaften und Nährstoffbedingungen in verschiedenen Stockwerken des Oberflächenwassers aus verschiedenen Ablagerungsräumen und während unterschiedlicher Klimabedingungen beschrieben werden. Dies umfasst Bedingungen von kälter als heute (z.B. Letztes Glaziales Maximum) bis zu wärmer als heute (z.B. Marines Isotopen Stadium, MIS 5.5). Die Untersuchungen geben Hinweise zur (1) Sensitivität des antarktischen Ökosystems auf den Eintrag von Mikronährstoffen (Eisendüngung), (2) Oberflächenwasserstratifizierung und (3) 'Silicic-Acid leakage'-Hypothese, und tragen damit zur Überprüfung verschiedener Hypothesen zur Klimawirksamkeit von SO-Prozessen bei. Die neuen Proxies bilden überdies Oberflächen-Salzgehaltsanomalien ab, die Hinweise zur Stabilität des WAIS unter verschiedenen Klimabedingungen geben. Darüber hinaus kann die Hypothese getestet werden, nach der der WAIS während MIS 5.5 vollständig abgebaut war. Die Projektergebnisse sollen mit Simulationen mit einem kombinierten biogeochemischen (Si-Isotope beinhaltenden) Atmosphäre-Ozean-Zirkulations-Modell aus einem laufenden SPP1158-DFG Projekt an der CAU Kiel (PI B. Schneider) verglichen werden. Damit sollen die jeweiligen Beiträge der Ozeanzirkulation und der biologischen Produktion zum CO2-Austausch zwischen Ozean und Atmosphäre getrennt und statistisch analysiert werden. Informationen zu Staubeintrag, biogenen Flussraten, physikalischen Ozeanparametern und zur Erstellung von Altersmodellen stehen durch Zusammenarbeit mit anderen (inter)nationalen Projekten zur Verfügung.
Chromium (Cr) is introduced into the environment by several anthropogenic activities. A striking ex-ample is the area around Kanpur in the Indian state of Uttar Pradesh, where large amounts of Cr-containing wastes have been recently illegally deposited. Hexavalent Cr, a highly toxic and mobile contaminant, is present in significant amounts in these wastes, severely affecting the quality of sur-roundings soils, sediments, and ground waters. The first major goal of this study is to clarify the solid phase speciation of Cr in these wastes and to examine its leaching behavior. X-ray diffraction and synchrotron-based X-ray absorption spectroscopy techniques will be employed for quantitative solid phase speciation of Cr. Its leaching behavior will be studied in column experiments performed at un-saturated moisture conditions with flow interruptions simulating monsoon rain events. Combined with geochemical modeling, the results will allow the evaluation of the leaching potential and release kinetics of Cr from the waste materials. The second major goal is to investigate the spatial distribution, speciation, and solubility of Cr in the rooting zone of chromate-contaminated soils surrounding the landfills, and to study the suitability of biochar as novel soil amendment for mitigating the deleterious effects of chromate pollution. Detailed field samplings and laboratory soil incubation studies will be carried out with two agricultural soils and biochar from the Kanpur region.
When released into surface waters, engineered inorganic nanoparticles (EINP) can be subject to multiple transformations. The objectives of MASK are to understand under which conditions EINP in aquatic systems will attach to suspended matter, under which conditions and in which time scale EINP are coated by NOM present in freshwater systems, how these coated colloidal particles are stabilized in the aquatic system and to which extent the aquatic aging processes are reversible. Homo-aggregation, coating changes, biological interactions and hetero-aggregation are hypothesized as key processes governing EINP aging in water bodies. In process orientated laboratory incubation experiments (50 ml to 6 l) with increasing complexity, MASK unravels the relevance and the interplay of inorganic colloids, aquagenic and pedogenic organic matter and solution physicochemistry for stability of EINP. These systems will successively approach situations in real waters. MASK thus provides information on EINP fluxes in the aquatic compartment, their time scales, reversibility and relative relevance. EINP will be analysed by standard light scattering techniques, ICP-MS, ESEM/EDX, WetSTEM and AFM. A method coupling hydrodynamic radius chromatography (HDC) with ICPMS recently developed by K. Tiede for nAg0 will be optimized and developed for further EINP analysis, MASK is further responsible for the virtual subproject ANALYSIS, the development and optimization of joint research unit methods of EINP analysis, sample preparation and sample storage, the exchange of methods and coordinates the joint analyses and the central EINP database.
In the Bavarian Forest National Park a brief, but intense storm event on 1 August 1983 created large windfall areas. The windfall ecosystems within the protection zone of the park were left develop without interference; outside this zone windfall areas were cleared of dead wood but not afforested. A set of permanent plots (transect design with 10 to 10 m plots) was established in 1988 in spruce forests of wet and cool valley bottoms in order to document vegetation development. Resampling shall take place every five years; up to now it was done in 1993 and 1998. On cleared areas an initial raspberry (Rubus idaeus) shrub community was followed by pioneer birch (Betula pubescens, B. pendula) woodland, a sequence well known from managed forest stands. In contrast to this, these two stages were restricted to root plates of fallen trees in uncleared windfalls; here shade-tolerant tree species of the terminal forest stages established rather quickly from saplings that had already been present in the preceeding forest stand. Soil surface disturbances are identified to be causal to the management pathway of forest development, wereas the untouched pathway is caused by relatively low disturbance levels. The simulation model FORSKA-M is used to analyse different options of further stand development with a simulation time period of one hundred years.
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.
The present-day configuration of Indonesia and SE Asia is the results of a long history of tectonic movements, volcanisms and global eustatic sea-level changes. Not indifferent to these dynamics, fauna and flora have been evolving and dispersing following a complicate pattern of continent-sea changes to form what are today defined as Sundaland and Wallacea biogeographical regions. The modern intraannual climate of Indonesia is generally described as tropical, seasonally wet with seasonal reversals of prevailing low-level winds (Asian-Australian monsoon). However at the interannual scale a range of influences operating over varying time scales affect the local climate in respect of temporal and spatial distribution of rainfall. Vegetation generally reflects climate and to simplify it is possible to distinguish three main ecological elements in the flora of Malaysia: everwet tropical, seasonally dry tropical (monsoon) and montane. Within those major ecological groups, a wide range of specific local conditions caused a complex biogeography which has and still attract the attention of botanists and biogeographers worldwide. Being one of the richest regions in the Worlds in terms of species endemism and biodiversity, Indonesia has recently gone through intensive transformation of previously rural/natural lands for intensive agriculture (oil palm, rubber, cocoa plantations and rice fields). Climate change represents an additional stress. Projected climate changes in the region include strengthening of monsoon circulation and increase in the frequency and magnitude of extreme rainfall and drought events. The ecological consequences of these scenarios are hard to predict. Within the context of sustainable management of conservation areas and agro-landscapes, Holocene palaeoecological and palynological studies provide a valuable contribution by showing how the natural vegetation present at the location has changed as a consequence of climate variability in the long-term (e.g. the Mid-Holocene moisture maximum, the modern ENSO onset, Little Ice Age etc.). The final aim of my PhD research is to compare the Holocene history of Jambi province and Central Sulawesi. In particular: - Reconstructing past vegetation, plant diversity and climate dynamics in the two study areas Jambi (Sumatra) and Lore Lindu National Park (Sulawesi) - Comparing the ecological responses of lowland monsoon swampy rainforest (Sumatra) and everwet montane rainforests (Sulawesi) to environmental variability (vulnerability/resilience) - Investigating the history of human impact on the landscape (shifting cultivation, slash and burn, crop cultivation, rubber and palm oil plantation) - Assessing the impact and role of droughts (El Niño) and fires - Adding a historical perspective to the evaluation of current and future changes.
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.
(1) Terrestrische Biota der Antarktis sind durch geografische Isolation und inselhafte Verteilung geprägt. Die isolierte Lage der Antarktis und die Beschränkung auf weit voneinander entfernte kleine Habitatflecken haben zu einem hohen Endemiten-Anteil und einer starken Regionalisierung der Fauna und Flora geführt. Genetische Differenzierung, lokale Anpassung und die Evolution kryptischer Arten sind die Folge. Die Biodiversitäts-Konvention (CBD) betrachtet genetische Diversität als einen Eckpfeiler biologischer Vielfalt und stellt sie damit in eine Reihe mit der Diversität von Arten und Ökosystemen. Durch Einschleppung ortsfremder Arten und Homogenisierung bislang getrennter Genpools bedroht der Mensch jedoch zunehmend diese Isolation und genetische Differenzierung vieler antarktischer Biota. (2) Obwohl Flechten als wichtigste Primärproduzenten antarktische terrestrische Lebensräume dominieren, fehlen zurzeit Daten zu ihrer genetischen Struktur und Diversität. Der Umfang inter- und intrakontinentalen Genflusses ist bisher völlig unbekannt. Es ist deswegen derzeit unmöglich, den aktuellen und zukünftigen menschlichen Einfluss auf antarktische Flechtenpopulationen auch nur annähernd abzuschätzen.(3) Wir schlagen vor, mittels molekulargenetischer Daten die populationsgenetische Struktur von sechs weit verbreiteten Flechtenarten mit unterschiedlichen Ausbreitungsstrategien zu untersuchen. Dabei soll die Nullhypothese überprüft werden, dass Flechtenpopulationen genetisch nicht differenziert sind. Zusätzlich wollen wir abschätzen, ob menschliche Aktivitäten zur Einschleppung ortsfremder Arten oder Genotypen und zur Homogenisierung von Genpools beitragen. Hierfür sollen Lokalitäten mit hohem und niedrigem menschlichen Einfluss verglichen werden. Das Projekt schafft damit unverzichtbare Grunddaten für die Entwicklung von Schutzstrategien in der Antarktis.
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