On a method for estimating the shape of a gravitationally and magnetically disturbing body

Summary The demagnetisation depends on the shape of the magnetised body. Here we investigate the possibility of calculating the shape of the magnetised body by means of the demagnetisation. It can be done if the gravity field and the induced magnetic field of a body with constant susceptibility and density are known. As the method is approximative it is not restricted just to bodies with a 2nd degree surface, but can be applied to all bodies, for which the demagnetisation can be regarded as constantly dependent on the direction. This means, with certain approximation, all bodies that are homogeneously magnetised, but not in the direction of the magnetising field due to demagnetisation.

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Zusammenfassung Die Demagnetisierung hängt von der Gestalt des magnetisierten Körpers ab. Hier soll untersucht werden, inwieweit es möglich ist, aus der Demagnetisierung Rückschlüsse über die Gestalt des magnetisierten Körpers zu ziehen. Dazu besteht die Möglichkeit, wenn das Gravitationsfeld und das induzierte Magnetfeld eines Körpers mit konstanter Dichte und Suszeptibilität gegeben sind. Da die Methode approximativ ist, ist sie nicht auf Körper mit Oberfläche 2ten Grades beschränkt, sondern sie kann in allen Fällen angewandt werden, in denen die Demagnetisierung als konstant richtungsabhängig angesehen werden kann. Dies bedeutet mit einer gewissen Approximation alle Körper, die homogen magnetisiert sind, aber infolge der Entmagnetiseerung nicht in der Richtung des magnetisierenden Feldes.

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Klüfte und Schlechten im Ruhrkarbon und ihre Darstellung im Kleinriss

Ohne Zusammenfassung     

Über Strahlungseigenschaften des Gletschereises

Zusammenfassung Am Hintereisferner wurden im Sommer 1956 Strahlungsmessungen an Gletschereisplatten mit Hilfe eines Solarimeters Moll-Gorczynski durchgeführt. Dabei ergab es sich, daß die Albedo der Eisplatten gesetzmäßig mit der Plattendicke zunimmt und außerdem von der Sonnenhöhe abhängig ist. Durchlässigkeitsmessungen lieferten für die Schicht zwischen 10 und 35 cm Tiefe einen mittleren Extinktionskoeffizienten von 0,085 cm^–1.Auf theoretischem Wege wurde versucht, die Beziehungen zwischen Extinktion, Zerstreuung und Reflexion sowie die Strahlungsverhältnisse im Innern der Eisplatten zu erfassen; auf diese Weise war es auch möglich, auf die vertikale Intensitätsverteilung der eindringenden Strahlung in den obersten Dezimetern des Gletschers zu schließen und die in den verschiedenen Tiefenschichten umgesetzten Energiebeträge abzuschätzen.

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Summary Measurements of the radiative properties of slabs of glacier ice were implemented in summer 1956 on the Hintereisferner. The instrument used was a Solarimeter Moll-Gorczynski. As a result of these investigations a simple law governing the increase of the albedo of the slabs with thickness could be stated. The albedo was also found to vary with solar altitude. Measurements of transmissiblity yield a mean extinction coefficient of 0,085 cm^–1 for the layer between 10 cm and 35 cm below the surface.The interrelations of extinction, diffusion and reflection as well as the radiative properties in the interior of the ice slabs were studied theoretically. The vertical distribution of the downward radiation in the uppermost decimetres of the glacier was deduced from the theory. An estimate was made of the amounts of energy involved in the radiative processes occurring at various levels.

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Résumé Des mesures de rayonnement effectuées en été 1956 au Hintereisferner sur des plaques de glace du glacier au moyen d'un solarimètre Moll-Gorczynski, ont montré que l'albédo de ces plaques augmente avec leur épaisseur et dépend de la hauteur du soleil. Des mesures de transparence ont fourni pour la couche de 10 à 35 cm de profondeur un coefficient moyen d'extinction de 0,085 cm^–1.En cherchant à établir théoriquement les relations entre l'extinction la dispersion et la réflexion, ainsi que les conditions de rayonnement à l'intérieur des plaques de glace, il fut possible de déterminer la distribution verticale d'intensité du rayonnement incident dans les premiers décimètres de la surface du glacier et d'estimer les quantités d'énergie échangées aux différentes profondeurs.

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Mit 6 Textabbildungen     

The ocean/continent transition along a profile through the Lofoten basin,Northern Norway

The Cenozoic margins of the Norwegian-Greenland Sea offer ideal conditions for passive margin studies. A series of structural elements, first observed on these margins, led to the concept of volcanic passive margins. Questions still remain about the development of such features and the location of the boundary between oceanic and continental crust. Despite the thin sediment cover of the margins, seismic reflection data are not able to image the deeper structures due to the occurrence of igneous rocks at shallow depth.This paper presents a 320-km long profile perpendicular to the strike of the main structural units of the Lofoten Margin in Northern Norway. A geological model is proposed, based on observations made with ocean bottom seismographs, which recorded seismic refraction data and wide angle reflections, along with a seismic reflection profile covering the same area. Ray-tracing was used to calculate a geophysical model from the shelf area into the Lofoten basin. The structures typical of a volcanic passive margin were found, showing that the Lofoten Margin was influenced by increased volcanic activity during its evolution. The ocean/continent transition is located in a 30-km wide zone landwards of the Vøring Plateau escarpment.The whole margin is underlain by a possibly underplated, high velocity layer. Evidence for a pre-rift sediment basin landwards of the escarpment, overlain by basalt flows, was seen. These structural features, related to extensive volcanism on the Lofoten Margin, are not as distinct as further south along the Norwegian Margin. Viewed in the light of the hot-spot theory of White and McKenzie (1989) the Lofoten Margin can be interpreted as a transitional type between volcanic and non-volcanic passive margin.     

Multibeam Bathymetry of the Håkon Mosby Mud Volcano

The Håkon Mosby Mud Volcano is a natural laboratory to study geological, geochemical, and ecological processes related to deep-water mud volcanism. High resolution bathymetry of the Håkon Mosby Mud Volcano was recorded during RV Polarstern expedition ARK XIX/3 utilizing the multibeam system Hydrosweep DS-2. Dense spacing of the survey lines and slow ship speed (5 knots) provided necessary point density to generate a regular 10 m grid. Generalization was applied to preserve and represent morphological structures appropriately. Contour lines were derived showing detailed topography at the centre of the Håkon Mosby Mud Volcano and generalized contours in the vicinity. We provide a brief introduction to the Håkon Mosby Mud Volcano area and describe in detail data recording and processing methods, as well as the morphology of the area. Accuracy assessment was made to evaluate the reliability of a 10 m resolution terrain model. Multibeam sidescan data were recorded along with depth measurements and show reflectivity variations from light grey values at the centre of the Håkon Mosby Mud Volcano to dark grey values (less reflective) at the surrounding moat.     

Evolution of a Holsteinian (MIS 11c) palaeolake based on a 12‐ka‐long diatom record from Dethlingen (northern Germany)

To provide insights into the long‐term evolution of aquatic ecosystems without human interference, we here evaluate a decadal‐ to centennial‐scale‐resolution diatom record spanning about 12 ka of the Holsteinian interglacial (Marine Isotope Stage 11c). Using a partially varved sediment core from the Dethlingen palaeolake (northern Germany), which has previously been studied for palynological and microfacies signals, we document the co‐evolution of the aquatic and surrounding terrestrial environment. The diatom record is dominated by the genera Stephanodiscus, Aulacoseira, Ulnaria and Fragilaria. Based on the diatom assemblages and physical sediment properties, the evolution of the Dethlingen palaeolake can be subdivided into three major phases. During the oldest phase (lasting ～1900 varve years), the lake was ～10–15 m deep and characterized by anoxic bottom‐water conditions and a high nutrient content. The following ～5600 years exhibited water depths >20 m, maximum diatom and Pediastrum productivity, and a peak in allochtonous nutrient input. During this phase, water‐column mixing became more vigorous, resulting in a breakdown of anoxia. The youngest lake phase (～4000–5000 years) was characterized by decreasing water depth, turbulent water conditions and decreased nutrient loading. Based on our palaeolimnological data, we conclude that the evolution of the Dethlingen palaeolake during the Holsteinian interglacial responded closely to (i) changes within the catchment area (as documented by vegetation and sedimentation) related to the transition from closed forests growing on nutrient‐rich soils (mesocratic forest phase) to open forests developing on poor soils (oligocratic forest phase), and (ii) short‐term climate variability as reflected in centennial‐scale climate perturbations.     

Total waterborne carbon export and DOC composition from ten nested subarctic peatland catchments—importance of peatland cover,groundwater influence,and inter‐annual variability of precipitation patterns

Waterborne carbon (C) export from terrestrial ecosystems is a potentially important flux for the net catchment C balance and links the biogeochemical C cycling of terrestrial ecosystems to their downstream aquatic ecosystems. We have monitored hydrology and stream chemistry over 3 years in ten nested catchments (0.6–15.1 km²) with variable peatland cover (0%–22%) and groundwater influence in subarctic Sweden. Total waterborne C export, including dissolved and particulate organic carbon (DOC and POC) and dissolved inorganic carbon (DIC), ranged between 2.8 and 7.3 g m^–2 year^–1, representing ~10%–30% of catchment net ecosystem exchange of CO₂. Several characteristics of catchment waterborne C export were affected by interacting effects of peatland cover and groundwater influence, including magnitude and timing, partitioning into DOC, POC, and DIC and chemical composition of the exported DOC. Waterborne C export was greater during the wetter years, equivalent to an average change in export of ~2 g m^–2 year^–1 per 100 mm of precipitation. Wetter years led to a greater relative increase in DIC export than DOC export due to an inferred relative shift in dominance from shallow organic flow pathways to groundwater sources. Indices of DOC composition (SUVA₂₅₄ and a₂₅₀/a₃₆₅) indicated that DOC aromaticity and average molecular weight increased with catchment peatland cover and decreased with increased groundwater influence. Our results provide examples on how waterborne C export and DOC composition might be affected by climate change. Copyright © 2012 John Wiley & Sons, Ltd.     

The significance of chemical,isotopic, and detrital components in three coeval stalagmites from the superhumid southernmost Andes (53°S) as high-resolution palaeo-climate proxies

Stalagmites are important palaeo-climatic archives since their chemical and isotopic signatures have the potential to record high-resolution changes in temperature and precipitation over thousands of years. We present three U/Th-dated records of stalagmites (MA1–MA3) in the superhumid southern Andes, Chile (53°S). They grew simultaneously during the last five thousand years (ka BP) in a cave that developed in schist and granodiorite. Major and trace elements as well as the C and O isotope compositions of the stalagmites were analysed at high spatial and temporal resolution as proxies for palaeo-temperature and palaeo-precipitation. Calibrations are based on data from five years of monitoring the climate and hydrology inside and outside the cave and on data from 100 years of regional weather station records.Water-insoluble elements such as Y and HREE in the stalagmites indicate the amount of incorporated siliciclastic detritus. Monitoring shows that the quantity of detritus is controlled by the drip water rate once a threshold level has been exceeded. In general, drip rate variations of the stalagmites depend on the amount of rainfall. However, different drip-water pathways above each drip location gave rise to individual drip rate levels. Only one of the three stalagmites (MA1) had sufficiently high drip rates to record detrital proxies over its complete length. Carbonate-compatible element contents (e.g. U, Sr, Mg), which were measured up to sub-annual resolution, document changes in meteoric precipitation and related drip-water dilution. In addition, these soluble elements are controlled by leaching during weathering of the host rock and soils depending on the pH of acidic pore waters in the peaty soils of the cave’s catchment area. In general, higher rainfall resulted in a lower concentration of these elements and vice versa. The Mg/Ca record of stalagmite MA1 was calibrated against meteoric precipitation records for the last 100 years from two regional weather stations. Carbonate-compatible soluble elements show similar patterns in the three stalagmites with generally high values when drip rates and detrital tracers were low and vice versa. δ¹³C and δ¹⁸O values are highly correlated in each stalagmite suggesting a predominantly drip rate dependent kinetic control by evaporation and/or outgassing. Only C and O isotopes from stalagmite MA1 that received the highest drip rates show a good correlation between detrital proxy elements and carbonate-compatible elements. A temperature-related change in rainwater isotope values modified the MA1 record during the Little Ice Age (～0.7–0.1 ka BP) that was ～1.5 °C colder than today. The isotopic composition of the stalagmites MA2 and MA3 that formed at lower drip rates shows a poor correlation with stalagmite MA1 and all other chemical proxies of MA1. ‘Hendy tests’ indicate that the degassing-controlled isotope fractionation of MA2 and MA3 had already started at the cave roof, especially when drip rates were low. Changing pathways and residence times of the seepage water caused a non-climatically controlled isotope fractionation, which may be generally important in ventilated caves during phases of low drip rates. Our proxies indicate that the Neoglacial cold phases from ～3.5 to 2.5 and from ～0.7 to 0.1 ka BP were characterised by 30% lower precipitation compared with the Medieval Warm Period from 1.2 to 0.8 ka BP, which was extremely humid in this region.