Tektonik der Siegener Schichten im mittleren Wiedtal (Westerwald)

Zusammenfassung Feintektonische Untersuchungen, ergänzt durch stratigraphische Profilaufnahme, erbrachten den Nachweis eines Hönningen-Seifener-Sattels aus Schichten des Unteren Siegen, Im NW wie SE wird dieser Sattel von flachwelligen Muldenzonen begleitet, deren südöstliche in Richtung auf die Siegerländer Hauptüberschiebung einen zunehmenden Schuppenbau zeigt.     

The mantle rock (“laterite”) of the Gold Coast and its origin

Zusammenfassung Der Verwitterungsmantel (Laterit s. l.) der südlichen Goldküste besteht aus Horizonten, die sowohl verschiedene Entstehungsart als verschiedenes Alter haben. Brekzien oder Steinschichten sind unter aridem Klima als Wüstenpflaster entstanden. Zonen chemisch verwitterten Felses, Horizonte von lehmigem Sand (an deren Aufbau Termiten wesentlich beteiligt sind) und Konkretionen haben sich unter feuchtem Klima gebildet. Harte limonitische Oberflächen-Krusten deuten auf progressive Austrocknung hin. Unter diesen drei klimatischen Bedingungen gebildete Horizonte wiederholen sich mehrfach im Verwitterungsmantel der Goldküste. Ein junger, unvollständiger Zyklus ist weit verbreitet, ein älterer Zyklus tritt nur in begrenzten Vorkommen auf, und ein dritter Zyklus ist fast nur noch in aufgearbeiteten, limonitisierten Bruchstücken erhalten. Die wiederholten Klimaschwankungen machen es wahrscheinlich, daß der Verwitterungsmantel zeitlich dem größeren Teil des Quartärs entspricht. Wahrscheinlich können die Ergebnisse auf weit größere Gebiete angewandt werden.     

Neuere Veröffentlichungen

Ohne Zusammenfassung     

Daily Weather Observations in Sixteenth-Century Europe

Thirty-two weather diaries written in astronomical calendars in central Europe in the late fifteenth and sixteenth centuries are presented and discussed. Systematic weather observations were promoted by the rise of planetary astronomy and its application in astro-meteorology. The practice of keeping weather diaries spread from Cracow (Poland) to Ingolstadt (Germany) and from there to other universities. The data obtained from these sources provided the backbone for setting up series of precipitation indices for Poland, Germany and Switzerland. Monthly statistics of days with precipitation, snowfall and frost were computed by counting the relevant entries in the most important diaries. The results were compared with either those obtained from instrumental measurements in the same place or with those from modern instrumental measurements in a neighbouring place. The final results show that autumn was considerably colder in the early sixteenth century. April was considerably drier and July was wetter during the period 1508-1531 than during 1901-1960. In order to highlight the impact of weather patterns on grain prices in a year of crisis, the timing of wet and dry spells in southern Poland and southern Germany is compared for the year 1529. Winters became 1.7°C colder from 1564 to 1576 and the month of July tended to be wetter than in 1901-1960. Details noted in the diaries kept between 1585 and 1600 by the astronomers Brahe (near Copenhagen) and Fabricius (in the Ostfriesland region of northwestern Germany) closely agree. It rained more often in June and July and temperatures dropped. The winter months were more frequently dominated by winds from easterly directions, the frequency of snowfall was higher and a deficit occurred in precipitation. This points to a higher frequency of high pressure in the Fennoscandian area with cold air advection from the east or northeast.     

Assessment of the Uncertainties in the NO2 and O3 Measurements by Visible Spectrometers

The column amounts of nitrogen dioxide (NO2) and ozone (O3) were measured using a visible spectrometer based on the twilight zenith-sky technique at two observatories located at similar latitudes in the northern part of Japan separated by a distance of 150 km. The measurements began in April 1991 at the Moshiri Observatory (44.4°N, 142.3°E) and in April 1994 at the Rikubetsu Observatory (43.5°N, 143.8°E). Since weather conditions and the possible influence from tropospheric pollution were not always identical at these two observatories, the overall accuracy of the measurements was studied comparing these data sets. The first year data obtained at a solar zenith angle of 90 degrees indicated that the NO2 slant column values at sunrise and sunset agreed within 0.36 and 0.54 × 1016 cm-2, respectively, corresponding to 5 % (June) and to 12 % (December) of the columns. The O3 values agreed within 0.76 × 1019 cm-2, corresponding to 4 % (March) 6 % (August) of the columns, although a part of the difference was systematic. The O3 column amounts were also compared to those obtained by the Dobson spectrometer at Sapporo (43.5°N, 143.8°E), whose latitude is similar to these observatories. When an air mass factor of 17.5 was used, the two-year Moshiri vertical column values agreed with the Dobson direct sun values to within 15 Dobson Units, or 3 6 % of the column. The difference between the two values was found to be due partly to the change in the air mass factor caused by seasonal and day-to-day changes in the shape of the O3 vertical profiles. These results confirm the reliability of the NO2 and O3 measurements by visible spectrometers at these sites for the Network for the Detection of Stratospheric Change (NDSC).     

The Use of Wave-field Directivity for Velocity Estimation: Moving Source Profiling (MSP) Experiments at KTB

—Within the "Integrated Seismics Oberpfalz 1989 (ISO89)" a three-component Moving Source Profiling (MSP) experiment, also named walk-away VSP, was carried out at the drilling site of the "Kontinentales Tiefbohrprogramm der Bundesrepublik Deutschland (KTB)" in Germany. Analysis of transmitted waves traveling from the source locations at the surface down to the receiver array in the borehole reveals velocity information about the illuminated part of the subsurface. Complementary to the widely used evaluation of travel-time perturbations to locate velocity inhomogeneities we suggest the use of the directivity of transmitted wave types down in the borehole. To determine the wave-field directivity we focus on transmitted arrivals by employing principles of "Controlled Directional Reception (CDR)." We calculate local slant-stacks for three different depth positions as a function of the source offset, thus obtaining the variation of the vertical slowness (vertical ray parameter) of incident waves along the horizontal source profile and the vertical receiver array. The slowness data combined with travel times are interpreted by forward modeling taking into account geological information of the survey area. Our findings confirm results from gravity measurements which suggest the existence of large amphibolite/metabasite complexes in the vicinity of the borehole. The described method is also used to identify P-to-S converted energy originating from fracture zones above the receiver array and to locate the region in which conversion occurs.     

Differences between Mean Sea Levels for the Pacific,Atlantic and Indian Oceans From Topex/Poseidon Altimetry

Geopotential values W of the mean equipotential surfaces representing the mean ocean topography were computed on the basis of four years (1993 - 1996) TOPEX/POSEIDON altimeter data: W = 62 636 854.10m ² s ^–2 for the Pacific (P), W = 62 636 858.20m ² s ^–2 for the Atlantic (A), W = 62 636 856.28m ²s^–2 for the Indian (I) Oceans. The corresponding mean separations between the ocean levels were obtained as follows: A – P = – 42 cm, I– P = – 22 cm, I – A = 20 cm, the rms errors came out at about 0.3 cm. No sea surface topography model was used in the solution.     

Intracrystalline fractionation of Fe in synthetic (Fe, Mg, Zn) - bearing staurolite: a Mössbauer spectroscopic study

⁵⁷Fe-Mössbauer spectra of eleven Fe-Mg-bearing staurolite samples, synthesized at 5, 20 and 25 kbar and 680°C, ranging in composition from x_Fe?=1.00 to x_Fe?=0.15, and of two Zn-Fe-bearing staurolite samples, synthesized at 20 kbar and 700°C with x_Fe?=0.10 and x_Fe?=0.32 were collected at room temperature. The spectra reveal that about 80% of Fe_tot (in case of Fe-Mg-bearing staurolite) and about 70% of Fe_tot (in case of Fe-Zn-bearing staurolite) are located as Fe²⁺ at the three subsites Fe1, Fe2 and Fe3 of the tetrahedral T2-site. The refinement of the spectra results in almost identical values for the isomer shift (IS) (±1.0 mm/s) but significantly different values for the quadropole splitting (QS) for the three subsites which is in accordance with the different distortions of these sites. About 8% of Fe_tot (in case of Fe-Mg-bearing staurolite) and 13% of Fe_tot (in case of Fe-Zn-bearing staurolite) are located as Fe²⁺ at the octahedral M4 site, while the remainder percents of Fe_tot indistinguishably occur as Fe²⁺ at the octahedral M1 and M2 sites of the kyanite-like part of the structure. Within the whole Fe-Mg-staurolite solid solution series the Mössbauer parameters QS of the sites M4 and (M1, M2) vary systematically with composition whereas IS remains constant. There is a high negative correlation of the total Mg-content with Fe-occupation of all the Fe-bearing sites indicating a continuous substitution of Fe²⁺ by Mg on all these sites. Synthetic Fe-staurolites show no increasing occupation of the octahedral sites by two-valent cations with pressure, as was assumed by several authors.     

Analysis Of The Disappearing Filament And Flare Of 7 May 1992

By using Yohkoh soft X-ray data, H filtergrams, and radio data, the activation of the disappearing filament and the flare eruption on 7 May 1992 have been studied. Main conclusions are as follows: (1) the emergence of new magnetic flux tends to affect the pre-existing X-ray loops, which usually appear in arcades spanning H filament, changing the magnetic environment of the filament, and then enhance the current in the filament. Therefore newly emerging flux plays a fundamental role in the destabilization of this filament. (2) According to the H data and the rising motion of the filament, the corresponding current variation in the filament has been calculated. It seems that the current interruption may be a possible trigger mechanism for this filament disappearance. (3) The magnetic field strength and the energy flux of energetic electrons in the source region of microwave bursts have been estimated by using the microwave spectrum. During the main phase, the mean magnetic strength and the energy flux of energetic electrons are about 300–400 G and 1×1011 erg cm–2 s –1, respectively. (4) The energy provided by reconnection of the current sheet and the total energy of the current filament are estimated and we show that there is enough energy stored in the filament to feed the 7 May, 1992 flare.     

Neue Ergebnisse ans der Grenzregion zwischen der Flyschzone und den nördlichen Kalkalpen

Zusammenfassung Es wurden in großen Zügen Schichtfolge, paläogeographische Entwicklung und Tektonik im österreichischen Verbreitungsgebiet einer schmalen, größtenteils stark verschuppten Zone beschrieben, die sich zwischen der Flyschzone und den nördlichen Kalkalpen erstreckt. Sie wurde bisher für die westliche Fortsetzung der karpatischen pieninischen Klippenzone gehalten. Es konnte nachgewiesen werden, daß letztere etwa im Lainzer Tiergarten bei Wien ihr westliches Ende findet, die Grestener Schuppenzone, wie erstere bezeichnet werden soll, dagegen eine nördlichere Einheit darstellt, die mit der inneren oder Waagtaler Klippenregion der Karpaten identisch ist.Im Wiener Wald ist sie noch ziemlich breit, einfach gebaut und auch in fazieller Hinsicht dem Flysch sehr ähnlich. In dem Maße aber, in dem sie gegen Westen immer mehr von den Kalkalpen überschoben und damit schmäler wird, kompliziert sich auch ihr Bau. Aus Oberbayern, Allgäu und Westschweiz ist sie schließlich nur noch in Form vereinzelter Schubfetzen (Aroser Schuppenzone) bekannt.Bezeichnend sind Schuppen, die an ihrer Basis aus — bisher irreführenderweise Klippen genannten — jurassisch-neokomen Sandsteinen, Kalken, Mergeln usw., im Hangenden dagegen aus kretazisch-eozänen Hüllschichten in Flyschfazies bestehen.Bis zur Unterkreide lag der Sedimentationsraum dieser Zone am Nordrand der kalkalpinen Geosynklinale. Als sich darauf das Flyschbecken einsenkte, geriet er im Westen in den Schwellenbereich am Südrand dieses Beckens. Im Osten, d. h. im Wiener Wald und in den Westkarpaten, fehlen dagegen die trennenden Schwellen, so daß das Flyschmeer dort viel weiter nach Süden reichte.Die Grestener Schuppenzone nimmt also in paläogeographischer und tektonischer Hinsicht eine zwischen Flyschzone und nördlichen Kalkalpen vermittelnde Stellung ein.