Restoration of submerged vegetation in shallow eutrophic lakes – A guideline and state of the art in Germany     

Sabine Hilt  Elisabeth M. Gross  Michael Hupfer  Harald Morscheid  Jens Mhlmann  Arnulf Melzer  Jens Poltz  Stefan Sandrock  Eva-Maria Scharf  Susanne Schneider  Klaus van de Weyer 《Limnologica》2006,36(3):155-171

One of the most serious problems caused by eutrophication of shallow lakes is the disappearance of submerged macrophytes and the switch to a turbid, phytoplankton-dominated state. The reduction of external nutrient loads often does not result in a change back to the macrophyte-dominated state because stabilising mechanisms that cause resilience may delay a response. Additional internal lake restoration measures may therefore be needed to decrease the concentration of total phosphorus and increase water clarity. The re-establishment of submerged macrophytes required for a long-term stability of clear water conditions, however, may still fail, or mass developments of tall-growing species may cause nuisance for recreational use. Both cases are often not taken into account when restoration measures are planned in Germany, and existing schemes to reduce eutrophication consider the topic inadequately. Here we develop a step-by-step guideline to assess the chances of submerged macrophyte re-establishment in shallow lakes. We reviewed and rated the existing literature and case studies with special regard on (1) the impact of different internal lake restoration methods on the development of submerged macrophytes, (2) methods for the assessment of natural re-establishment, (3) requirements and methods for artificial support of submerged macrophyte development and (4) management options of macrophyte species diversity and abundance in Germany. This guideline is intended to help lake managers aiming to restore shallow lakes in Germany to critically asses and predict the potential development of submerged vegetation, taking into account the complex factors and interrelations that determine their occurrence, abundance and diversity.  相似文献   

Secondary alteration of the impactite and mineralization in the basal Tertiary sequence,Yaxcopoil‐1, Chicxulub impact crater,Mexico     

Doreen E. AMES  Ingrid M. KJARSGAARD  Kevin O. POPE  Burkhard DRESSLER  Mark PILKINGTON 《Meteoritics & planetary science》2004,39(7):1145-1167

Abstract The 65 Ma Chicxulub impact crater formed in the shallow coastal marine shelf of the Yucatán Platform in Mexico. Impacts into water‐rich environments provide heat and geological structures that generate and focus sub‐seafloor convective hydrothermal systems. Core from the Yaxcopoil‐1 (Yax‐1) hole, drilled by the Chicxulub Scientific Drilling Project (CSDP), allowed testing for the presence of an impact‐induced hydrothermal system by: a) characterizing the secondary alteration of the 100 m‐thick impactite sequence; and b) testing for a chemical input into the lower Tertiary sediments that would reflect aquagene hydrothermal plume deposition. Interaction of the Yax‐1 impactites with seawater is evident through redeposition of the suevites (unit 1), secondary alteration mineral assemblages, and the subaqueous depositional environment for the lower Tertiary carbonates immediately overlying the impactites. The least‐altered silicate melt composition intersected in Yax‐1 is that of a calc‐alkaline basaltic andesite with 53.4–56 wt% SiO_{2(volatile‐free)}. The primary mineralogy consists of fine microlites of diopside, plagioclase (mainly Ab 47), ternary feldspar (Ab 37 to 77), and trace apatite, titanite, and zircon. The overprinting alteration mineral assemblage is characterized by Mg‐saponite, K‐montmorillonite, celadonite, K‐feldspar, albite, Fe‐oxides, and late Ca and Mg carbonates. Mg and K metasomatism resulted from seawater interaction with the suevitic rocks producing smectite‐K‐feldspar assemblages in the absence of any mixed layer clay minerals, illite, or chlorite. Rare pyrite, sphalerite, galena, and chalcopyrite occur near the base of the impactites. These secondary alteration minerals formed by low temperature (0–150°C) oxidation and fixation of alkalis due to the interaction of glass‐rich suevite with down‐welling seawater in the outer annular trough intersected at Yax‐1. The alteration represents a cold, Mg‐K‐rich seawater recharge zone, possibly recharging higher temperature hydrothermal activity proposed in the central impact basin. Hydrothermal metal input into the Tertiary ocean is shown by elevated Ni, Ag, Au, Bi, and Te concentrations in marcasite and Cd and Ga in sphalerite in the basal 25 m of the Tertiary carbonates in Yax‐1. The lower Tertiary trace element signature reflects hydrothermal metal remobilization from a mafic source rock and is indicative of hydrothermal venting of evolved seawater into the Tertiary ocean from an impact‐generated hydrothermal convective system.  相似文献   

Multiple advances of Alpine glaciers into the Jura Mountains in the Northwestern Switzerland     

Angela Graf  Naki Akçar  Susan Ivy-Ochs  Stefan Strasky  Peter W. Kubik  Marcus Christl  Martin Burkhard  Rainer Wieler  Christian Schlüchter 《Swiss Journal of Geoscience》2015,108(2-3):225-238

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Scalar field haloes as gravitational lenses     

Franz E. Schunck  Burkhard Fuchs  Eckehard W. Mielke 《Monthly notices of the Royal Astronomical Society》2006,369(1):485-491

A non-topological soliton model with a repulsive scalar self-interaction of the Emden type provides a constant-density core, similarly as the empirical Burkert profile of dark matter (DM) haloes. As a further test, we derive the gravitational lens properties of our model, in particular, the demarcation curves between 'weak' and 'strong' lensing. Accordingly, strong lensing with typically three images is almost three times more probable for our solitonic model than for the Burkert fit. Moreover, some prospective consequences of a possible flattening of DM haloes are indicated.  相似文献   

Line fitting in Euclidean 3D space     

Kyle Snow  Burkhard Schaffrin 《Studia Geophysica et Geodaetica》2016,60(2):210-227

Over a century ago Pearson solved the problem of fitting lines in 2D space to points with noisy coordinates in both dimensions. Surprisingly, however, the case of fitting lines in 3D space has seen little attention, though Adcock long ago published a brief (one page) article claiming that the solution that minimized orthogonal distances is the most probable. We solve this problem using a new algorithm for the Total Least-Squares (TLS) solution within an Errors-In-Variables Model, respectively an equivalent nonlinear Gauss-Helmert Model. Following Roberts, only four parameters are estimated, thereby avoiding over-parametrization that may lead to unnecessary singularities and, hence, require the introduction of constraints to the model. The current pervasiveness of Global Navigation Satellite Systems, robotic total stations, and digital laser scanners as sources of geodetic observations means that geodetic engineers and scientists now commonly work with observational models in 3D space as opposed to classical geodetic methods that often separated horizontal and vertical observational models. And while several papers have been written describing a TLS solution for line fitting problems in 2D space, the extension to 3D space is not readily apparent from these works. This further motivates the treatment of the 3D problem in some detail in this contribution.  相似文献   

Local variability of sedimentation rate in Lake Arendsee, Germany     

Burkhard W. Scharf  Bertram Boehrer  Conrad Kopsch 《Limnologica》2010,40(2):97-101

We measured the thickness and the dry weight of recently deposited sediment along several transects across Lake Arendsee in order to quantify the sedimentation rate and its local variability. As a time marker, we used an artificial marl layer that was deposited by a remediation program in the year 1995. A portion of the sediment deposited during the year was transported from the littoral and the top of the submerged hills to the foot of the slope, where we found the greatest deposition. Within the same lake, the deposited sediment layer varied by a factor of 4 between minimal and maximal values over the same time periods. Lake Arendsee is a holomictic and eutrophic lake with depletion of oxygen in summer time.  相似文献   

Total least-squares adjustment of condition equations     

Burkhard Schaffrin  Andreas Wieser 《Studia Geophysica et Geodaetica》2011,55(3):529-536

The usual least-squares adjustment within an Errors-in-Variables (EIV) model is often described as Total Least-Squares Solution (TLSS), just as the usual least-squares adjustment within a Random Effects Model (REM) has become popular under the name of Least-Squares Collocation (without trend). In comparison to the standard Gauss-Markov Model (GMM), the EIV-Model is less informative whereas the REM is more informative. It is known under which conditions exactly the GMM or the REM can be equivalently replaced by a model of condition equations or, more generally, by a Gauss-Helmert Model. Similar equivalency conditions are, however, still unknown for the EIV-Model once it is transformed into such a model of condition equations. In a first step, it is shown in this contribution how the respective residual vector and residual matrix look like if the TLSS is applied to condition equations with a random coefficient matrix to describe the transformation of the random error vector. The results are demonstrated using a numeric example which shows that this approach may be valuable in its own right.  相似文献   

The Tauern Window (Eastern Alps, Austria): a new tectonic map, with cross-sections and a tectonometamorphic synthesis     

Stefan M. Schmid  Andreas Scharf  Mark R. Handy  Claudio L. Rosenberg 《Swiss Journal of Geoscience》2013,106(1):1-32

We present a tectonic map of the Tauern Window and surrounding units (Eastern Alps, Austria), combined with a series of crustal-scale cross-sections parallel and perpendicular to the Alpine orogen. This compilation, largely based on literature data and completed by own investigations, reveals that the present-day structure of the Tauern Window is primarily characterized by a crustal-scale duplex, the Venediger Duplex (Venediger Nappe system), formed during the Oligocene, and overprinted by doming and lateral extrusion during the Miocene. This severe Miocene overprint was most probably triggered by the indentation of the Southalpine Units east of the Giudicarie Belt, initiating at 23–21 Ma and linked to a lithosphere-scale reorganization of the geometry of mantle slabs. A kinematic reconstruction shows that accretion of European lithosphere and oceanic domains to the Adriatic (Austroalpine) upper plate, accompanied by high-pressure overprint of some of the units of the Tauern Window, has a long history, starting in Turonian time (around 90 Ma) and culminating in Lutetian to Bartonian time (45–37 Ma).  相似文献   

The constancy of galactic cosmic rays as recorded by cosmogenic nuclides in iron meteorites     

Thomas Smith  David L. Cook  Silke Merchel  Stefan Pavetich  Georg Rugel  Andreas Scharf  Ingo Leya 《Meteoritics & planetary science》2019,54(12):2951-2976

We measured the He, Ne, and Ar isotopic concentrations and the ¹⁰Be, ²⁶Al, ³⁶Cl, and ⁴¹Ca concentrations in 56 iron meteorites of groups IIIAB, IIAB, IVA, IC, IIA, IIB, and one ungrouped. From ⁴¹Ca and ³⁶Cl data, we calculated terrestrial ages indistinguishable from zero for six samples, indicating recent falls, up to 562 ± 86 ka. Three of the studied meteorites are falls. The data for the other 47 irons confirm that terrestrial ages for iron meteorites can be as long as a few hundred thousand years even in relatively humid conditions. The ³⁶Cl‐³⁶Ar cosmic ray exposure (CRE) ages range from 4.3 ± 0.4 Ma to 652 ± 99 Ma. By including literature data, we established a consistent and reliable CRE age database for 67 iron meteorites. The high quality of the CRE ages enables us to study structures in the CRE age histogram more reliably. At first sight, the CRE age histogram shows peaks at about 400 and 630 Ma. After correction for pairing, the updated CRE age histogram comprises 41 individual samples and shows no indications of temporal periodicity, especially not if one considers each iron meteorite group separately. Our study contradicts the hypothesis of periodic GCR intensity variations (Shaviv 2002, 2003), confirming other studies indicating that there are no periodic structures in the CRE age histogram (e.g., Rahmstorf et al. 2004; Jahnke 2005). The data contradict the hypothesis that periodic GCR intensity variations might have triggered periodic Earth climate changes. The ³⁶Cl‐³⁶Ar CRE ages are on average 40% lower than the ⁴¹K‐K CRE ages (e.g., Voshage 1967). This offset can either be due to an offset in the ⁴¹K‐K dating system or due to a significantly lower GCR intensity in the time interval 195–656 Ma compared to the recent past. A 40% lower GCR intensity, however, would have increased the Earth temperature by up to 2 °C, which seems unrealistic and leaves an ill‐defined ⁴¹K‐K CRE age system the most likely explanation. Finally, we present new ²⁶Al/²¹Ne and ¹⁰Be/²¹Ne production rate ratios of 0.32 ± 0.01 and 0.44 ± 0.03, respectively.  相似文献   

Stable and Sr-isotope evidence for fluid advection during thrusting of the glarus nappe (swiss alps)     

M. Burkhard  R. Kerrich  R. Maas  W. S. Fyfe 《Contributions to Mineralogy and Petrology》1992,112(2-3):293-311

At the Glarus thrust in the Swiss Helvetic Alps, Permian Verrucano siltstones are allochthonously superimposed over Tertiary Flysch with an intermediate, about 1 metre thin layer of intensively deformed calcmylonite of probable Mesozoic provenance. The H–O–C- and Sr-isotope compositions of minerals from the calc-mylonite and strongly mylonitized Verrucano siltstones were determined in order to assess: (1) equilibrium-disequilibrium relationships; (2) isotopic composition of the fluid phase, its provenance and water/rock ratios; (3) sources of Sr in the calc-mylonite; (4) deformation temperatures. The isotopic composition of cale-mylonite micro-samples from five sites along the thrust varies from 22 to 12 and 2 to-10 for ¹⁸O and ¹³C respectively. All samples are ¹⁸O depleted by up to 14 relative to the presumed marine Helvetic carbonate protoliths (¹⁸O=25.4±2). A pronounced geographic trend of ¹⁸O depletion from 22 in the north to 12 in the south is observed. In calc-mylonites, ⁸⁷Sr/⁸⁶Sr ratios range from typical Mesozoic marine carbonate protolith signatures (0.708±0.005) to more radiogenic values as high as 0.722. A variable contribution of radiogenic ⁸⁷Sr to the calc-mylonite is though to reflect interaction with fluids that aquired their Sr from the Hercynian granitic basement. Chlorites and muscovites from the calc-mylonite and Verrucano have uniform ¹⁸O values but display D values from-40 to-147%: the D-enriched values correspond to the primary metamorphic or formational fluids expelled during thrusting, whereas the D-depleted samples reflect selective H-isotope exchange with meteoric fluids during uplift of the Alpine belt. The isotopic composition of the calc-mylonites requires exchange with ¹⁸O—depleted, ⁸⁷Sr—enriched fluids at very high water/rock ratios. Possible sources for these are dewatering of the underlying Flysch and/or metamorphic fluids, or formation brines expelled along the thrust from greater depth. These could be derived from compaction and dewatering of the Flysch in the northern part of the thrust; in the south, however, where Verrucano is thrust over ¹⁸O-rich Mesozoic carbonates, the extreme ¹⁸O depletion of the calc-mylonite has to be explained either by fluid advection within the Verrucano hanging wall and thrust zone or alternatively by exchange with metamorphic fluids from greater depth, expelled along the thrust. Microstructural evidence (abundant veins, stylolites, breccias) suggests that fluids played an important role in deformation and strain localization. Excepting albite all major components (quartz, chlorite, muscovite, calcite) are both dynamically recrystallized and crystallized as secondary minerals in pressure shadows and syn-mylonitic veins, indicating that these minerals were potentially open to oxygen isotopic exchange during alpine metamorphism and thrust deformation. Within the mylonitized Verrucano silstones, isolated quartz-chlorite and quartz-calcite fractionations yield temperatures of around 320°C close to values obtained from calcite-dolomite thermometry (355°C±30) and in agreement with the regional lower greenschist facies metamorphism. Quartz-calcite and quartz-albite fractionations indicate slightly lower temperatures around 250°C, owing to selective lower temperature re-equilibration of the calcite and albite during post peak metamorphism.  相似文献