Galactic Dynamo and Spiral Arms - 3D MHD Simulations

In the present project we investigate the evolution of a three-dimensional (3D), large-scale galactic magnetic field under the influence of gas flows in spiral arms and in the presence of dynamo action. Our principal goal is to check how the dynamical evolution of gaseous spiral arms affects the global magnetic field structure and to what extent our models could explain the observed spiral patterns of polarization B-vectors in nearby galaxies. A two-step scheme is used: the N-body simulations of a two-component, self-gravitating disk provide the time-dependent velocity fields which are then used as the input to solve the mean-field dynamo equations. We found that the magnetic field is directly influenced by large-scale non-axisymmetric density wave flows yielding the magnetic field locally well-aligned with gaseous spiral arms in a manner similar to that discussed already by Otmianowska-Mazur et al. 1997. However, an additional field amplification, introduced by a non-zero -term in the dynamo equations, is required to cause a systematic increase of magnetic energy density against the diffusive losses. Our simulated magnetic fields are also used to construct the models of a high-frequency (Faraday rotation-free) polarized radio emission accounting for effects of projection and limited resolution, thus suitable for direct comparisons with observations.     

Possible clay structures in frustules of living diatoms

Comparison of X-ray diffraction spectra of marine diatom frustules and suspended clay minerals suggests the presence of a distinctive smectite in diatoms. The frustules contained 1.5% Al₂O₃ and were partly covered with particles of 0.02 μm in diameter. The source of Al and the fate of diatoms in the sediment are briefly discussed.     

Spurenelemente in der Aare (Schweiz)

Instrumental neutron activation analysis was used for the determination of more than 20 trace and minor elements in water and silt samples (suspended load) of the river Aare. The samples were collected at four different locations along the river between its source and the lake of Bienne. The principal results are: 1. The concentrations of all elements investigated are much lower than WHO-limits for drinking water. 2. Human activities are responsible for an increase of some elements along the river. 3. The concentrations of dissolved trace elements are generally anticorrelated with the water flow rate. 4. The concentrations of the trace elements in particulates (in μg/l) are correlated with the flow rate of water. Except for Ca?Sr there are no significant interelement correlations for all four sampling stations.     

Die Geowissenschaft und ihre Bedeutung für die Zukunft der Zivilisation

Geoscience forms — besides Physics, Astronomy, Chemistry, and Biology — a specific domain of Science, characterized by its subjects and objects. Geoscience embraces all disciplines which are inquiring into the present configuration of the earth and its spheres, which intend to explain by natural laws the evolution of the earth and the life and which try to predict future developments. Solid bodies of the planetary system are subjects of geoscience insofar geoscientific methods can be applied. Geoscientists have profoundly contributed to the growth of the technological civilisation by discovering and exploiting sources for the supply of energy and raw materials. During the last decades the annual production of most of these materials has grown exponentially. This is shown, exemplarily, for iron, copper and mercury. Considering the exponential growth of the world population, the future life of mankind on earth is at stake because conventional resources, necessary for the maintenance of agriculture and technology, are running short and physical conditions essential for life are, because of geological reasons, finite and deteriorated by human activities. It is only by changing moral, political, economic and technical foundations of culture and civilisation that mankind can avoid extinction which was the ultimate fate of all species in the geological past. In the attempts to overcome the impending difficulties Geoscience has to play an important role of great responsibility: Only Geoscience can provide and develop by further research methods and knowledge which are necessary in order to evaluate the finite potentials available in the earth and the geological processes which both form the framework to which the future life of mankind has to be adjusted.     

The erosion history of the Central Alps: evidence from zircon fission track data of the foreland basin sediments

Fission track dating on detrital zircons of Alpine debris in the Swiss molasse basin provides information about the erosion history of the Central Alps and the thermal evolution of source terrains. During Oligocene times, only sedimentary cover nappes, and Austroalpine basement units were eroded. Incision into Austroalpine basement units is indicated by increasing importance of Cretaceous cooling ages in granite pebbles upsection. Erosion of Penninic basement units started between 25 and 20 Ma. Early Oligocene zircon FT ages show that Penninic basement units were exposed at ∼20 Ma. Deeper Penninic units of the Lepontine Dome became exposed first at ∼14 Ma, contemporaneously with the opening of the Tauern window in the Eastern Alps. A middle Miocene cooling rate of 40 °C Myr⁻¹ is deduced for the Lower Penninic units of the Lepontine Dome.     

IV. Bücher- und Zeitschriftenschau

Ohne Zusammenfassung     

Radiation from an impulsive line source in an unbounded homogeneous anisotropic medium

Summary. The space-time elastic wave motion generated by an impulsive line source in a homogeneous anisotropic medium is calculated with the aid of the Cagniard-de Hoop method. Two types of sources are considered in detail, viz. a line source of expansion (model for an explosive source) and a line force (model for a mechanical vibrator). Numerical results are presented for the radiated particle velocity in the medium including those regions of space where shear-wave triplication occurs. There is a marked difference in the time response observed for the two types of sources and for the different positions of the receiver with respect to the source position. These waveform differences are important when the radiated wave is used to determine experimentally the elastic properties of the medium. As compared with the traditional Fourier-integral transform method to handle this problem, the computation time with the present method is considerably less.     

Geochemistry and field spectrometry for detecting hydrocarbon microseepage

Remote sensing detection of hydrocarbon reserves would be a valuable addition to conventional methods used currently. Tests were made in a drilled, proven hydrocarbon area predominantly covered by wheat. Field-spectroradiometers measured spectral characteristics of wheat and soil associated with hydrocarbon microseepage. Soil gas and secondary carbonate produced only by hydrocarbon microseepage were at anomalously high levels at the oil–water or gas–water boundaries. Kaolinite and illite in the soil have higher percentages above petroleum reservoirs. The inflection point positions of spectra on oil-field wheat were shifted 7 nm to longer wavelengths than off-field wheat samples, and can be positively correlated with the delta carbonate and soil-gas. The absorption of soil spectra at 2.346 mm is at least 0.2% higher over oil-fields than off-fields. This research proves that remote sensing can be used in an monocultural agricultural area to detect hydrocarbon microseepage.