Possible types of rotations and translations in the Scandinavian Caledonides

Folding, faulting and large scale translation nappe movements are well-known classical collision zone features, which are also found in the Scandinavian Caledonides where lateral movements of up to a few hundred kilometres have been suggested. In contrast to this, azimuthal rotations around vertical axes are rarely or never observed geologically. In a few cases, palaeomagnetic data, however, show abnormal directions of the remanent magnetic components, which may indicate vertical axes of rotations. Different types and scales of palaeomagnetic interpretations are classified and discussed in relation to 5 examples from the Scandinavian Caledonides (the Särv nappe, the Lönset dome, the Fongen gabbro, the Sulitjelma gabbro, and the Trollfjord-Komagelv fault), and various models to explain segmental rotations of the crust are suggested.     

Copper(II) humate mobility in kaolinite soil

An investigation of the influence of humate on the mobility of copper(II) ions in a kaolinite soil using leaching tests and electrokinetic experiments is reported. The data are interpreted in terms of humate–copper–clay interactions and humate electrical charge. Humate is mostly immobile below pH8 but is more mobile in alkaline conditions (sorption to kaolinite reduces its mobility in neutral conditions). Copper humate complexes are mobile in both acidic and alkaline conditions, but not in neutral conditions where they are sorbed. The dissolved copper humate complexes that form in acidic conditions are positively charged. The net effect of humate is to increase cupric ion mobility in kaolinite soil, especially in alkaline conditions.     

NGC 4650 A: A nearly edge-on ring galaxy?

The peculiar galaxy NGC 4650 A (α=12^h 42^m. 1; = δ—40° 26′; 1950·0) has been studied by means of direct and spectral observations with the ESO 3·6-m telescope. It is interpreted as a prolate, elliptical galaxy surrounded by a warped ring of H II regions, dust and stars. The distance is 47 Mpc (H ₀=55 km s⁻¹ Mpc⁻¹). The ring is seen nearly edge-on (inclination 85°) and it rotates. It has a diameter of about 21 kpc and is bluer than the elliptical galaxy for which the (M/L _v) ratio is ∼12 in solar units. The observed configuration may be the result of interaction with the nearby galaxy, NGC 4650.     

Angular distributions of solar protons and electrons

High angular-resolution measurements of directional fluxes of solar particles in space have been obtained with detectors aboard OGO-5 during the cosmic ray event of 18 November 1968. This is the only case on record for which sharply-defined directional observations of protons and electrons covering a wide rigidity range (0.3 MV to 1.5 GV) are available.The satellite experiment provided data for determining pitch-angle distributions with respect to the direction of the local interplanetary magnetic field lines during the lengthy highly anisotropic phase of the event. It was found that the unidirectional differential intensities j(θ) of 3- to 25-MeV protons varied in accordance with the relationship j(θ) = b₀ + b₁cosθ + b₂cos²θ, where b₀ and b₁ ? 0, and b₂, is positive, zero or negative. Soon after onset, 79–266-keV electrons arriving from the direction of the Sun displayed an anisotropic component with the intensity varying as cos θ. Later, a double-peaked distribution appeared at the lower energies, whereas the flux at the upper end of the range covered by the experiment became isotropic. These results have been interpreted in the light of the temporal flux profiles and the state of the interplanetary medium.The observation of the unusually large and long-lasting anisotropies lead to several conclusions including: (1) If injection of the solar particles was instantaneous, the diffusion coefficient was either constant or increasing with distance from the Sun. (2) If the solar source emitted particles over an extended period, and there is evidence to that effect, there was weak scattering in the region between the Sun and the Earth and a strong scattering region beyond the Earth's orbit. (3) Solar electrons were stored near the Sun. (4) The observed angular distribution of 200-MV protons in the magnetosheath was in good agreement with that deduced in an earlier analysis of polar orbiting satellite observations and trajectory calculations.     

Eliminating Virtual Impactors with the Very Large Telescope: An ESO Program with the FORS2 Camera

We have used the ESO Very Large Telescope (VLT) to perform as trometric observations of Near Earth Asteroids (NEAs) having remote collision possibilities with the Earth. The observations were made for those objects which became too faint to be observed elsewhere. Using the 4 hours allocated in the semester April–September 2003, 5 faint NEAs were observed. As a result, no NEA that could impact the Earth was lost.     

Mg and Sr distribution in carbonate rocks from the Maastrichtian/Danian boundary of the Danish subbasin and the North Sea Central Graben

Examination of the Mg and Sr concentrations in carbonate rocks in a number of sections provides the basis for the establishment of two geochemical facies within the region studied: (1) a basinal facies, including the axial part of the Danish Subbasin and the North Sea Central Graben, indicating relatively stable geochemical conditions; and (2) an eastern marginal facies in the Danish Subbasin reflecting unstable geochemical conditions and distinguished by partial cementation and increasing Mg and Sr concentrations towards the northeastern limits of the basin. A slight microtextural variation in the chalk between the basinal and marginal facies indicates that the origin and composition of the biogenic carbonate components strongly influence the bulk-rock geochemistry.

The elemental distribution reveals a negative correlation between the Mg and Sr concentrations in the topmost Maastrichtian chalk, expressed by increasing Mg and decreasing Sr upwards towards the Maastrichtian/Danian boundary. This relation occurs in both geochemical facies and in all sections studied and is believed to have been governed by changing physicochemical conditions in the late Maastrichtian sea.     

Low enthalpy geothermal energy resources in Denmark

The deep oil exploration drillings in Denmark have shown that especially the Danish Embayment contains low enthalpy geothermal resources associated with warm aquifers. The most promising reservoirs have been found in highly permeable Upper Triassic sand and sandstone beds, which cover at least 5000 km² at depths of 2000–3000 m and at temperatures of 60–100°C. The porosity of the main reservoir is of 15–25%, and the permeability is presumed to be approximately 1 darcy (10^–12 m²) or higher. A layer thickness of 30–60 m has been observed on a number of localities. Also the Middle Jurassic and the Lower Triassic contain reservoirs of interest. A major geothermal exploration work is planned with seismic investigations, drillings to depths of 2000–4000 m and probably establishment of pilot district heating plants.