Light curve variations of RT lacertae

The eclipsing variable RT Lac, which is classified as an RS CVn-type binary by Hall, was observed in two colours,B andV, during the summer seasons of 1978 and 1979. The observations made during two successive seasons indicate that, outside eclipses, the system has brightened by about 0.12 and 0.15 magnitudes on average inB andV, respectively. Moreover, RT Lac was even fainter when observed by Milone in 1965. While the total brightness of the system remained unchanged at mid-secondary, it increased at mid-primary and outside eclipses. This may be interpreted as indicating that the cooler component is responsible for the peculiar light variations.     

Evaluating the salinity distribution of a shallow coastal aquifer by vertical multielectrode profiling (Denmark)

A monitoring system, including five groups of piezometers and five vertical multielectrode profiling probes (VMEP), has been installed in an aquifer beneath a coastal dune in Denmark. In order to assess the salinity distribution within the aquifer, geoelectrical data were gathered in March, June and September 2008, by measuring a dipole-dipole and gradient array using multielectrode profiling. Interpretation of the processed resistivity data was performed by regularized inversion using a one-dimensional, horizontally layered model of formation resistivity. The standard deviation on estimated layer log-resistivity was 0.01–0.03. By estimating two parameters of a power function, observed fluid conductivities derived from samples of porewater were related to corresponding estimated formation resistivities. The conductivity profiles correlate with a winter situation in March with high sea level, active recharge and significant wave activity, causing increased hydraulic heads, a thicker freshwater lens and salt water overlying freshwater close to the sea. In June, the thickness of the freshwater lens is reduced due to less recharge and prevailing offshore winds, imposing density-stable conditions and a sharper transition between fresh and brackish water. During the autumn, aquifer recharge is enhanced and hydraulic heads increase, resulting in a thicker freshwater lens.     

Kinematic analysis and palaeoseismology of the Edremit Fault Zone: evidence for past earthquakes in the southern branch of the North Anatolian Fault Zone,Biga Peninsula,NW Turkey

The Edremit Fault Zone (EFZ) forms one of the southern segments of the North Anatolian Fault Zone (NAFZ) at the northern margin of the Edremit Gulf (Biga Peninsula, South Marmara Region, Turkey). Stratigraphic, structural and kinematic results indicate that basinward younging of the fault zone, in terms of a rolling-hinge mechanism, has resulted in at least three discrete Miocene to Holocene deformational phases: the oldest one (Phase 1) directly related to the inactive Kazda? Detachment Fault, which was formed under N–S trending pure extension; Phase 2 is characterised by a strike-slip stress condition, probably related to the progression of the NAFZ towards the Edremit area in the Plio–Quaternary; and Phase 3 is represented by the high-angle normal faulting, which is directly interrelated with the last movement of the EFZ. Our palaeoseismic studies on the EFZ revealed the occurrence of three past surface rupture events; the first one occurred before 13178 BC, a penultimate event that may correspond to either the 160 AD or 253 AD historical earthquakes, and the youngest one can be associated with the 6 October 1944 earthquake (M_w = 6.8). These palaeoseismic data indicate that there is no systematic earthquake recurrence period on the EFZ.     

The High Resolution Spectrograph for Spectrum UV

The Spectrum-UV mission, a general purpose ultraviolet observatory equipped with a 170-cm aperture telescope for imaging and spectroscopy in the 912 to 3600 Å range, will be launched in a seven days, high elliptical orbit in the late '90s by a Proton booster. The German contribution to the focal plane instrument complex is described: HIRDES, a High Resolution Double Echelle Spectrograph.     

Period variation and the new light curves of V471 Tauri

The light curve and period variation of the eclipsing system V471 Tau is discussed. The migration period of 191 days obtained recently by Ibanolu agrees well with the new observations. The period decreases by about one second per century, which may correspond to a mass transfer of 1×10^–7 solar mass. Furthermore, the O–C diagram shows a noticeable sine curve super-imposed on the parabolic variation. The period of the sine curve is about 3.1 years.     

Statistical analysis of tropical climate anomaly simulations

The statistical analysis of two atmospheric general circulation simulations using the ECHAM3 GCM in permanent January conditions are presented. The two simulations utilize different oceanic surface temperatures in the Atlantic as boundary conditions: the cold simulation has SST representing the anomalous cold conditions during the decade 1904-13 while the warm simulation has SST representative for the decade 1951-60 where anomalous warm conditions have been observed. The analysis concentrates on the simulated differences between both experiments within the tropical belt to test the working hypothesis whether changes in the deep tropical heating initiated by the anomalous SST are responsible for the anomalies in the flow and mass field. We present a method which extracts the significant and dynamically consistent signal of the total difference using a multivariate statistical test based on the amplitudes of an a-priori specified mode expansion. These expansion modes are defined from a variant of the Matsuno-Gill linearized reduced gravity model for the tropical atmosphere. The application of the method shows a clear and well defined tropical signal in the flow and mass field which can be understood as the reponse of the ECHAM3 model to a deep heating anomaly not in the vicinity of the anomalous SST but on the neighboring continents especially South America and with opposite sign in remote areas between Indonesia and the dateline. The signal can be summarized as an enhancement of the GCM's tropical East-West circulation with the ascending branch over South America in the warm simulation compared to the cold run.     

Light curve variations in V471 Tauri

The light curves of V471 Tau obtained in four successive years from 1981 to 1984 are presented. The light variations due to the tidally distorted red dwarf have been computed and subtracted out from the light curves obtained so far. A pure shape of the wave-like distortion has therefore been derived. The period of the retrograde migration has been found to be 182.17 days. On the other hand, the mean brightness of the system seems to vary with a period of about 18 years. The amplitude of the variation is greater at longer wavelength. The periodic variation of the mean brightness resembles the solar cycle of about 11.2 years, which depends upon the number of spots or spot groups.