Rain-cracking limits the production of many soft and fleshy fruit including sweet cherries world wide. Cracking is thought to result from increased water uptake through surface and pedicel. Water uptake increases fruit volume, and hence, turgor of cells (Pcell) and the pressure inside the fruit (Pfruit) and subjects the skin to tangential stress and hence, strain. When the strain exceeds the limits of extensibility the fruit cracks. This hypothesis is referred to as the Pfruit driven strain cracking. Based on this hypothesis cracking is related to two independent groups of factors: (1) water transport characteristics and (2) the intrinsic cracking susceptibility of the fruit defined as the amount of cracking per unit water uptake. The intrinsic cracking susceptibility thus reflects the mechanical constitution of the fruit. Most studies focussed on water transport through the fruit surface (factors 1), but only little information is available on the mechanical constitution (i.e., Pfruit and Pcell, tensile properties such as fracture strain, fracture pressure and modulus of elasticity of the exocarp; factors 2). The few published estimates of Pfruit in sweet cherry are all obtained indirectly (calculated from fruit water potential and osmotic potentials of juice extracts) and unrealistically high. They exceed those measured by pressure probe techniques in mature grape berry by several orders of magnitude. The objective of the proposed project is to test the hypothesis of the Pfruit driven strain cracking. Initially we will focus on establishing systems of widely differing intrinsic cracking susceptibility by varying species (sweet and sour cherry, Ribes and Vaccinium berries, plum, tomato), genotype (within sweet cherry), stage of development and temperature. These systems will then be used for testing the hypothesis of Pfruit driven strain cracking. We will quantify Pfruit und Pcell by pressure probe techniques and compression tests and the mechanical properties of the exocarp using biaxial tensile tests. When the presence of high Pfruit and Pcell is confirmed by direct measurements, subsequent studies will focus on the mode of failure of the exocarp (fracture along vs. across cell walls) and the relationship between failure thresholds and morphometric characteristics of the exocarp. However, when Pfruit und Pcell are low, the hypothesis of Pfruit driven strain cracking must be rejected and the mechanistic basis for low pressures (presence of apoplastic solutes) clarified on a temporal (in the course of development) and a spatial scale (exocarp vs. mesocarp). We focus on sweet cherry, because detailed information on this species and experience in extending the short harvest period is available. Where appropriate, other cracking susceptible species (sour cherry, plum, Vaccinium, Ribes, tomato) will be included to further extend the experimental period and to maximize the range in intrinsic cracking susceptibility.
To overcome the limitation in spatial and temporal resolution of methane oceanic measurements, sensors are needed that can autonomously detect CH4-concentrations over longer periods of time. The proposed project is aimed at:- Designing molecular receptors for methane recognition (cryptophane-A and -111) and synthesizing new compounds allowing their introduction in polymeric structure (Task 1; LC, France); - Adapting, calibrating and validating the 2 available optical technologies, one of which serves as the reference sensor, for the in-situ detection and measurements of CH4 in the marine environments (Task 2 and 3; GET, LAAS-OSE, IOW) Boulart et al. (2008) showed that a polymeric filmchanges its bulk refractive index when methane docks on to cryptophane-A supra-molecules that are mixed in to the polymeric film. It is the occurrence of methane in solution, which changes either the refractive index measured with high resolution Surface Plasmon Resonance (SPR; Chinowsky et al., 2003; Boulart et al, 2012b) or the transmitted power measured with differential fiber-optic refractometer (Boulart et al., 2012a; Aouba et al., 2012).- Using the developed sensors for the study of the CH4 cycle in relevant oceanic environment (the GODESS station in the Baltic Sea, Task 4 and 5; IOW, GET); GODESS registers a number of parameters with high temporal and vertical resolution by conducting up to 200 vertical profiles over 3 months deployment with a profiling platform hosting the sensor suite. - Quantifying methane fluxes to the atmosphere (Task 6); clearly, the current project, which aims at developing in-situ aqueous gas sensors, provides the technological tool to achieve the implementation of ocean observatories for CH4. The aim is to bring the fiber-optic methane sensor on the TRL (Technology Readiness Level) from their current Level 3 (Analytical and laboratory studies to validate analytical predictions) - to the Levels 5 and 6 (Component and/or basic sub-system technology validation in relevant sensing environments) and compare it to the SPR methane sensor, taken as the reference sensor (current TRL 5). This would lead to potential patent applications before further tests and commercialization. This will be achieved by the ensemble competences and contributions from the proposed consortium in this project.
Agriculture is the major contributor of nitrogen to ecosystems, both by organic and inorganic fertilizers. Percolation of nitrate to groundwater and further transport to surface waters is assumed to be one of the major pathways in the fate of this nitrogen. The quantification of groundwater and associated nitrate flux to streams is still challenging. In particular because we lack understanding of the spatial distribution and temporal variability of groundwater and associated NO3- fluxes. In this preliminary study we will focus on the identification and quantification of groundwater and associated nitrate fluxes by combining high resolution distributed fiber-optic temperature sensing (DTS) with in situ UV photometry (ProPS). DTS is a new technique that is capable to measure temperature over distances of km with a spatial resolution of ca1 m and an accuracy of 0.01 K. It has been applied successfully to identify and quantify sources of groundwater discharge to streams. ProPS is a submersible UV process photometer, which uses high precision spectral analyses to provide single substance concentrations, in our case NO3-, at minute intervals and a detection limit of less than 0.05 mg l-1 (ca.0.01 mg NO3--Nl-1). We will conduct field experiments using artificial point sources of lateral inflow to test DTS and ProPS based quantification approaches and estimate their uncertainty. The selected study area is the Schwingbach catchment in Hessen, Germany, which has a good monitoring infrastructure. Preliminary research on hydrological fluxes and field observations indicate that the catchment favors the intended study.
Im letzten Jahrzehnt war der grönländische Eisschild mehreren Extremereignissen ausgesetzt, mit teils unerwartet starken Auswirkungen auf die Oberflächenmassebilanz und den Eisfluss, insbesondere in den Jahren 2010, 2012 und 2015. Einige dieser Schmelzereignisse prägten sich eher lokal aus (wie in 2015), während andere fast die gesamte Eisfläche bedeckten (wie in 2010).Mit fortschreitendem Klimawandel ist zu erwarten, dass extreme Schmelzereignisse häufiger auftreten und sich verstärken bzw. länger anhalten. Bisherige Projektionen des Eisverlustes von Grönland basieren jedoch typischerweise auf Szenarien, die nur allmähliche Veränderungen des Klimas berücksichtigen, z.B. in den Representative Concentration Pathways (RCPs), wie sie im letzten IPCC-Bericht genutzt wurden. In aktuellen Projektionen werden extreme Schmelzereignisse im Allgemeinen unterschätzt - und welche Konsequenzen dies für den zukünftigen Meeresspiegelanstieg hat, bleibt eine offene Forschungsfrage.Ziel des vorgeschlagenen Projektes ist es, die Auswirkungen extremer Schmelzereignisse auf die zukünftige Entwicklung des grönländischen Eisschildes zu untersuchen. Dabei werden die unmittelbaren und dauerhaften Auswirkungen auf die Oberflächenmassenbilanz und die Eisdynamik bestimmt und somit die Beiträge zum Meeresspiegelanstieg quantifiziert. In dem Forschungsprojekt planen wir zudem, kritische Schwellenwerte in der Häufigkeit, Intensität sowie Dauer von Extremereignissen zu identifizieren, die - sobald sie einmal überschritten sind - eine großräumige Änderung in der Eisdynamik auslösen könnten.Zu diesem Zweck werden wir die dynamische Reaktion des grönländischen Eisschilds in einer Reihe von Klimaszenarien untersuchen, in denen extreme Schmelzereignisse mit unterschiedlicher Wahrscheinlichkeit zu bestimmten Zeitpunkten auftreten, und die Dauer und Stärke prognostisch variiert werden. Um indirekte Effekte durch verstärktes submarines Schmelzen hierbei berücksichtigen zu können, werden wir das etablierte Parallel Ice Sheet Model (PISM) mit dem Linearen Plume-Modell (LPM) koppeln. Das LPM berechnet das turbulente submarine Schmelzen aufgrund von Veränderungen der Meerestemperatur und des subglazialen Ausflusses. Es ist numerisch sehr effizient, so dass das gekoppelte PISM-LPM Modell Ensemble-Läufe mit hoher Auflösung ermöglicht. Folglich kann eine breite Palette von Modellparametern und Klimaszenarien in Zukunftsprojektionen in Betracht gezogen werden.Mit dem interaktiv gekoppelten Modell PISM-LPM werden wir den Beitrag Grönlands zum Meeresspiegelanstieg im 21. Jahrhundert bestimmen, unter Berücksichtigung regionaler Veränderungen von Niederschlag, Oberflächen- und Meerestemperaturen, und insbesondere der Auswirkungen von Extremereignissen. Ein Hauptergebnis wird eine Risikokarte sein, die aufzeigt, in welchen kritischen Regionen Grönlands zukünftige extreme Schmelzereignisse den stärksten Eisverlust zur Folge hätten.
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.
The decomposition of terrestrial organic material such as leaf litter represents a fundamental ecosystem function in streams that delivers energy for local and downstream food webs. Although agriculture dominates most regions in Europe and fungicides are applied widely, effects of currently used fungicides on the aquatic decomposer community and consequently the leaf decomposition rate are largely unknown. Also potential compensation of such hypothesised adverse effects due to nutrients or higher average water temperatures associated with climate change are not considered. Moreover, climate change is predicted to alter the community of aquatic decomposers and an open question is, whether this alteration impacts the leaf decomposition rate. The current projects follows a tripartite design to answer these research questions. Firstly, a field study in a vine growing region where fungicides are applied in large amounts will be conducted to whether there is a dose-response relationship between the exposure to fungicides and the leaf decomposition rate. Secondly, experiments in artificial streams with field communities will be carried out to assess potential compensatory mechanisms of nutrients and temperature for effects of fungicides. Thirdly, field experiments with communities exhibiting a gradient of taxa sensitive to climate change will be used to investigate potential climate-related effects on the leaf decomposition rate.
Die Asian Tropopause Aerosol Layer (ATAL), eine Schicht mit erhöhtem Aerosolgehalt, tritt jedes Jahr von Juni bis September in 14-18 km Höhe in einem Gebiet auf, das sich vom Mittelmeer bis zum westlichen Pazifik erstreckt. Hinsichtlich der Zusammensetzung der Partikel, sowie ihrer Bedeutung für die Strahlungsbilanz in dieser klimasensitiven Höhenregion bestehen große Unsicherheiten. Die bisher einzigen Flugzeugmessungen aus dem Zentrum der ATAL wurden 2017 im Rahmen der StratoClim Kampagne von Kathmandu aus gewonnen. Dabei entdeckten wir mit Hilfe des Infrarotspektrometers GLORIA auf dem Forschungsflugzeug Geophysica, dass feste Ammoniumnitrat (AN) â€Ì Partikel einen beträchtlichen Teil der Aerosolmasse ausmachen. Diese zählen zu den effizientesten Eiskeimen in der Atmosphäre. Zudem zeigte die gleichzeitige Messung von Ammoniakgas (NH3) durch GLORIA, dass dieses Vorläufergas durch starke Konvektion in die obere Troposphäre verfrachtet wird. Im Rahmen der PHILEAS-Kampagne schlagen wir eine gemeinsamen Betrachtung von atmosphärischen Modellsimulationen und Messungen vor, um die Zusammensetzung, Ursprung, Auswirkungen und Verbleib der ATAL-Partikel zu untersuchen â€Ì insbesondere im Hinblick auf ihre Prozessierung sowie ihren Einfluss auf die obere Troposphäre und die untere Stratosphäre der nördlichen Hemisphäre. Messungen von monsunbeeinflussten Luftmassen über dem östlichen Mittelmeer sowie über dem nördlichen Pazifik werden es uns erlauben, Luft mit gealtertem Aerosol- und Spurengasgehalt zu analysieren und damit die StratoClim-Beobachtungen aus dem Inneren des Monsuns zu komplementieren. Um dabei die wahrscheinlich geringeren Konzentrationen an Aerosol und Spurengasen zu quantifizieren, schlagen wir vor, die GLORIA-Datenerfassung von NH3 und AN u.a. durch die Verwendung neuartiger spektroskopischer Daten zu verbessern. Ferner werden wir die Analyse der GLORIA-Spektren auf Sulfataerosole sowie deren Vorläufergas SO2 auszudehnen. Auf der Modellseite werden wir das globale Wetter- und Klimamodellsystem ICON-ART weiterentwickeln, um die ATAL unter Einbeziehung verschiedener Aerosoltypen (Nitrat, Ammonium, Sulfat, organische Partikel, Staub) zu simulieren â€Ì unter Berücksichtigung der hohen Eiskeimfähigkeit von festem AN. Modellläufe werden durchgeführt, um einerseits einen globalen Überblick über die Entwicklung der ATAL 2023 zu gewinnen und zudem detaillierte, auf die relevanten Kampagnenperioden zugeschnittene, wolkenauflösende Informationen über die Aerosol-Wolken-Strahlungs-Wechselwirkungen zu erhalten. Über die direkte Analyse der PHILEAS-Kampagne hinausgehend wird diese Arbeit die Grundlage für eine verbesserte Analyse von Aerosolparametern aus GLORIA-Beobachtungen früherer und zukünftiger HALO-Kampagnen sowie aus Satellitenbeobachtungen legen. Darüber hinaus wird sie ICON-ART, einem der zentralen Klimamodellsysteme in Deutschland die Simulation von Aerosolprozessen sowie Aerosol/Wolken-Wechselwirkungen im Zusammenhang mit der ATAL ermöglichen.
The aim of P2 within the Research Unit 'The Forgotten Part of Carbon Cycling: Organic Matter Storage and Turnover in Subsoils (SUBSOM)' is to contribute to the understanding of the different sources and stabilization processes of subsoil organic matter. This will be achieved by the analysis of the soil organic matter composition in topsoil versus subsoil by 13C NMR spectroscopy in bulk soils as well as organo-mineral associations. This will be done on a number of soil profiles differing in parent material and mineralogy and therefore also in the relevance of organo-mineral associations for subsoil C stabilization. In addition, a specific sampling approach will allow to differentiate three zones associated with the dominating effect of (1) leaching of DOC (the 'bulk soil' between trees), (2) root litter decomposition (the 'root-affected zone'), and (3) direct rhizodeposition of root exudates (the 'rhizosphere' sensu strictu). The contribution of above-ground versus below-ground litter is differentiated by the analysis of cutin and suberin biomarkers. Organic matter derived from microbial sources will be identified by the microbial signature of polysaccharides in the subsoil through the analysis of neutral sugars and amino sugars. Organo-mineral associations will be further characterized by N2-BET analyses to delineate the coverage of the mineral phase with organic matter. With these analyses and our specific analytical expertise at the submicron scale (nanoSIMS) we will participate in selected joint experiments of the research unit.
The CHAMP mission provided a great amount of geomagnetic data all over the globe from 2000 to 2010. Its dense data coverage has allowed us to build GRIMM - GFZ Reference Internal Magnetic Model - which has the highest ever resolution for the core field in both space and time. We have already modeled the fluid flow in the Earth's outer core by applying the diffusionless magnetic induction equation to the latest version of GRIMM, to find that the flow evolves on subdecadal timescales, with a remarkable correlation to the observed fluctuation of Earth rotation. These flow models corroborated the presence of six-year torsional oscillations in the outer core fluid. Torsional oscillation (TO) is a type of hydromagnetic wave, theoretically considered to form the most important element of decadal or subdecadal core dynamics. It consists of relative azimuthal rotations of rigid fluid annuli coaxial with the mantle's rotation and dynamically coupled with the mantle and inner core. In preceding works, the TOs have been studied by numerical simulations, either with full numerical dynamos, or solving eigenvalue problems ideally representing the TO system. While these studies drew insights about dynamical aspects of the modeled TOs, they did not directly take into account the observations of geomagnetic field and Earth rotation. Particularly, there have been no observation-based studies for the TO using satellite magnetic data or models. In the proposed project, we aim at revealing the subdecadal dynamics and energetics of the Earth's core-mantle system on the basis of satellite magnetic observations. To that end, we will carry out four work packages (1) to (4), for all of which we use GRIMM. (1) We perform timeseries analyses of core field and flow models, to carefully extract the signals from TOs at different latitudes. (2) We refine the conventional flow modeling scheme by parameterizing the magnetic diffusion at the core surface. Here, the diffusion term is reinstated in the magnetic induction equation, which is dynamically constrained by relating it to the Lorentz term in the Navier-stokes equation. (3) We develop a method to compute the electromagnetic core-mantle coupling torque on the core fluid annuli, whereby the energy dissipation due to the Joule heating is evaluated for each annulus. This analysis would provide insights on whether the Earth's TOs are free or forced oscillations. (4) Bringing together physical implications and computational tools obtained by (1) to (3), we finally construct a dynamical model for the Earth's TOs and core-mantle coupling such that they are consistent with GRIMM and Earth rotation observation. This modeling is unique in that the force balances concerning the TOs are investigated in time domain, as well as that the modeling also aims at improving the observation-based core flow model by considering the core dynamics.
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.
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