Kenntnis der Randstrukturen des Witwatersrand-Beckens im nördlichen Oranje-Freistaat-Goldfeld (Südafrika)     

Dipl.-Geol. Dr. M. Manfred Schidlowski 《International Journal of Earth Sciences》1968,57(2):557-585

Zusammenfassung Eine Analyse der Randstrukturen des Witwatersrand-Beckens im nördlichen Oranje-Freistaat-Goldfeld zeigt, daß das tektonische Bild der Beckenrandregion nacheinander durch verschiedene Deformationsakte von unterschiedlichem Charakter geprägt worden ist. Auf eine Einengungsphase von spät-Witwatersrand-Alter, die zur Bildung einer randlichen Aufrichtungszone und zum Aufreißen eines Systems von 'normalen und antivergenten Aufschiebungen führte, folgte während des Unteren Ventersdorp eine jüngere Zerrungsphase, bei der es zu einem staffeiförmlgen Zerbrechen der ursprünglich eingeengten Scholle kam. Die Zerrung hängt sehr wahrscheinlich mit dem Zerbrechen der Beckenrandregion während oder unmittelbar nach der Extrusion der Unteren Ventersdorp-Laven zusammen. Dabei wurde ein schmaler randparalleler Streifen der Beckenfüllung in einem Graben versenkt ('Odendaalsrus-Graben). Die abgesunkenen Schollenteile sind in sich noch stark zerbrochen und gewöhnlich schiefgestellt. Da der versenkte Streifen durch ein primäres Einmuldungsstadium hindurchgegangen ist, deutet die Grabenbildung offenbar eine Fortsetzung der Beckenbildungsvorgänge 'mit anderen Mitteln an. — Die Bewegungen haben ein Alter von etwa 2,1 Mrd. Jahren; sie fallen somit ins frühe Präkambrium und sind keinesfalls 'intraalgonkisch, wie es noch bis in die jüngste Vergangenheit angenommen wurde.Tektonische Experimente haben ergeben, daß sich die wichtigsten Störungssysteme der realen Beckenrandstrukturen bei entsprechend gewählter Versuchsanordnung auch künstlich erzeugen lassen.

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The Orange Free State goldfield represents the southernmost part of the Witwatersrand Basin (Fig. 1) which is completely buried under a cover of Ventersdorp and Karroo rocks. The pre-Karroo geology of this area is characterized by a major rift system trending SSW-NNE ('Odendaalsrus graben), followed to the east by a V-shaped horst and two minor rift blocks (Fig. 2). The main graben is bounded by two principal faults (Border Fault, De Bron Fault, Fig. 4) which are roughly parallel to the western rim of the basin.A tectonic analysis of the basin-edge structures in the northern part of the graben reveals that the basin rim has been subjected to a sequence of deformational acts working over a considerable period of time. A primary compression of the basin-edge region in Upper Witwatersrand times resulted in the formation of a marginal fold; since sedimentation continued, the different stages of the folding process were sometimes preserved by a set of minor unconformities within the youngest sediments (Elsburg A Reefs, Fig. 5). With increasing lateral pressure a couple of reverse faults developed to support the folding (faults No. 10 and 11, Figs. 6 and 7); the minor thrust faults No. 19 and 21 represent the second component of this fault system. A reconstruction of the original depositional plain of the Lower Agglomerate shows that the main thrust faults (No. 10 and 11) are definitely older than the Elsburg A 1 Reef and have been obviously revived after the younger sediments had been laid down (Fig. 8 a).In a later stage compression gave way to tensional forces bringing about a fracturing of the overturned limb of the marginal fold along normal faults (faults No. 4 and 7, Figs. 6 and 7). There is reason to believe that the tensional phase was associated with the incipient rifting during early Ventersdorp times and that these faults were more or less contemporaneous with the general tilting of the basin-edge as displayed to-day (cf. Figs. 3 and 4). Because of the westerly tilt the Boulder Beds dip towards the west, although they must have been originally deposited on a ± horizontal or slightly basinward dipping plain. Faulting was mostly accomplished before deposition of the Ventersdorp sediments and the Upper Ventersdorp Lavas took place; the latter are seldom or only to a small degree affected by the fractures (Figs. 3 and 4). — The age of the tectonics is about 2,1×10⁹ years, i. e. early Precambrian and not Algonkian as formerly supposed.Experimental work aiming at an imitation of the observed basin-edge structures has shown that the principal tectonic features can be produced artificially (Figs. 8 a and b). This refers in particular to the main system of thrust-faults as well as to the younger step-faults caused by tension.

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Résumé Les structures tectoniques au bord du Bassin de Witwatersrand dans le district de mines d'or septentrional de la République d'Orange (Afrique du Sud) ont été analysées. Il s'est montré qu'elles sont déterminées par l'action de plusieurs phases de déformation successives de caractères différents. Une phase de compression d'âge Witwatersrand supérieur a d'abord amené un redressement des couches dans une zone marginale du bassin, avec chevauchements à vergences «normales» et inverses. Elle était suivie pendant le Ventersdorp inférieur d'une phase de traction qui produisit des cassures en gradins dans le secteur primitivement comprimé. La traction est très vraisemblablement en relation avec l'effondrement de la zone marginale du bassin pendant ou peu après l'extrusion des laves inférieures de Ventersdorp. Une bande étroite de sédiments, parallèle au bord du bassin, fut alors affectée d'un affaissement (formation du «graben d'Odendaalsrus») où de nombreuses cassures à l'intérieur des compartiments affaissés ont résulté dans la formation de blocs plus ou moins inclinés. Puisque cette zone a d'abord passé par un stade synclinal, on a l'impression que l'effondrement du graben ne représente que la reprise de l'affaissement général du bassin à l'aide d'une «technique nouvelle». - Les mouvements ont un âge de 2.1 milliards d'années, ils datent par conséquent du Précambrien inférieur et ne sont point «intra-algonkiques» comme il fut encore admis tout récemment.Il a été possible de reproduire artificiellement les systèmes de failles les plus importants de la zone marginale du bassin, si les conditions de l'expériment étaient favorables.

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Witwatersrand . . 2,1 , . . . , .

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Über die Beziehung zwischen äquatorialen Konvektionsregen und der Meereshöhe auf Ceylon     

Dr. Manfred Domrös 《Theoretical and Applied Climatology》1968,16(2-3):164-173

Zusammenfassung Die Beziehung zwischen äquatorialen Konvektionsregen und der Meereshöhe wird am Beispiel der Südabdachung der Haputale Range auf Ceylon (etwa 7° nördl. Br. und rund 1400 m Höhenunterschied) untersucht. Auf der Grundlage unveröffentlichter Niederschlagsmessungen von 21 Stationen, vorwiegend Teeplantagen, für die Periode von 1951–1965 wird die Änderung der Niederschlagsmenge mit der Höhe an Hand der mittleren jährlichen und mittleren monatlichen Niederschlagsmengen diskutiert. Hierbei ergibt sich im Jahresmittel und in den Monaten mit vorwiegend konvektiver Niederschlagsbildung — das sind die Intermonsunmonate März, April und Mai sowie Oktober und November —, daß nach anfänglicher Zunahme des Niederschlags mit wachsender Höhe oberhalb einer kritischen Höhenlage zwischen 900–1400 m NN eine stetige Abnahme des Niederschlags eintritt.

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Summary The relationship between equatorial convective rain and altitude above sea-level is investigated taking the southern slope of the Haputale Range in Ceylon (7° N, about 1400 m range of altitude) as an example. On the basis of unpublished precipitation observations of 21 stations, most of them on tea-estates, from the period 1951 to 1965 the variation of the amount of precipitation with altitude is discussed using mean annual and mean monthly precipitation totals. It appears that in the annual mean and during the months with prevailing convective rain — these are the intermonsoonal months March, April, May and October, November — the precipitation totals increase with altitude up to a critical level between 900 and 1400 m a.s.l. and then decrease again monotonically.

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Résumé On examine ici la relation existant entre les précipitations équatoriales de convection d'une part et l'altitude d'autre part. Pour ce faire, on se sert de l'exemple offert par le versant sud de l'Haputale Range de Ceylan (situé à environ 7° de latitude N et présentant une différence d'altitude de 1400 m environ). Sur la base de mesures non publiées des précipitations — mesures effectuées de 1951 à 1965 à 21 stations, en majeure partie des plantations de thé — on discute les modifications que subissent les sommes de précipitations avec l'altitude. Dans ce but, on utilise les moyennes annuelles et mensuelles de cet élément. Il en résulte que les précipitations augmentent tout d'abord avec l'altitude et cela jusqu'à une zone critique située entre 900 et 1400 m. Au-dessus, les précipitations diminuent de nouveau régulièrement. Cette constatation est valable aussi bien pour la moyenne annuelle que pour les mois caractérisés avant tout par des précipitations d'origine convective c'est à dire ceux qui se situent entre les périodes de mousson (mars, avril, mai, octobre et novembre).

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Midlatitude F-region neutral winds and temperatures during the priority regular world day 14 August 1980     

Dwight P. Sipler  Manfred A. Biondi  R. G. Roble 《Planetary and Space Science》1981,29(12):1367-1372

Midlatitude F-region neutral winds and temperatures determined from Fabry-Perot interferometer measurements of the doppler shifts and widths of nightglow 630.0 nm line profiles are presented for the priority regular world day 14 August 1980. They exhibit, in many respects, the observed behavior for other summer, geomagnetically quiet nights at solar maximum. The neutral temperature decreases from 1500°K after sunset (21 h LT) to a minimum of ˜ 1200°K before dawn (05 h LT), except to the north of the observatory. The zonal winds are eastward at sunset at 50 m/sec, decrease to zero at 02 h LT and are westward just before dawn. The meridional winds are zero just after sunset and reach a maximum equatorward value of 50–70 m/sec at local midnight but do not decrease as predicted; instead, they remain at roughly these values towards dawn. The NCAR thermospheric general circulation model (TGCM) is used to predict the global upper atmospheric temperature and circulation patterns for this world day. The model predictions agree with the measured neutral temperatures and exhibit qualitative similarities to the measured neutral winds. It is concluded that inclusion in the model of ion drift at midlatitudes should improve the agreement with observations.  相似文献   

Chemical Mechanism Development: Laboratory Studies and Model Applications     

Harald Geiger  Ian Barnes  Karl H. Becker  Birger Bohn  Theo Brauers  Birgit Donner  Hans-Peter Dorn  Manfred Elend  Carlos M. Freitas Dinis  Dirk Grossmann  Heinz Hass  Holger Hein  Axel Hoffmann  Lars Hoppe  Frank Hülsemann  Dieter Kley  Björn Klotz  Hans G. Libuda  Tobias Maurer  Djuro Mihelcic  Geert K. Moortgat  Romeo Olariu  Peter Neeb  Dirk Poppe  Lars Ruppert  Claudia G. Sauer  Oleg Shestakov  Holger Somnitz  William R. Stockwell  Lars P. Thüner  Andreas Wahner  Peter Wiesen  Friedhelm Zabel  Reinhard Zellner  Cornelius Zetzsch 《Journal of Atmospheric Chemistry》2002,42(1):323-357

Within the German Tropospheric Research Programme (TFS) numerous kinetic and mechanistic studies on the tropospheric reaction/degradation of the following reactants were carried out: oxygenated VOC, aromatic VOC, biogenic VOC, short-lived intermediates, such as alkoxy and alkylperoxy radicals.At the conception of the projects these selected groups were classes of VOC or intermediates for which the atmospheric oxidation mechanisms were either poorly characterised or totally unknown. The motivation for these studies was the attainment of significant improvements in our understanding of the atmospheric chemical oxidation processes of these compounds, particularly with respect to their involvement in photooxidant formation in the troposphere. In the present paper the types of experimental investigations performed and the results obtained within the various projects are briefly summarised. The major achievements are highlighted and discussed in terms of their contribution to improving our understanding of the chemical processes controlling photosmog formation in the troposphere.  相似文献   

Parameterization of Ozone Photolysis Frequency in the Lower Troposphere Using Data from Photodiode Array Detector Spectrometers     

Evelyn Jäkel  Manfred Wendisch  Barry L. Lefer 《Journal of Atmospheric Chemistry》2006,54(1):67-87

Spectroradiometers using photodiode array detectors (PDAs) are increasingly applied for airborne and ground-based atmospheric measurements of spectral actinic flux densities due to their high time resolution (less than one second). However they have limited sensitivity of ultraviolet (UV) radiation for wavelengths less than about 305 nm. This results in uncertainties of ozone photolysis frequencies derived from spectral actinic flux density measurements using PDA spectrometers. To overcome this limitation a parameterization method is introduced which extrapolates the data towards the wavelength range of limited sensitivity of the PDA spectrometers (less than about 305 nm). The parameterization is based on radiative transfer simulations and is valid for measurements in the lower troposphere. The components of the suggested parameterization are the lower threshold wavelength of the PDA spectrometer, the slant ozone column (ratio of the total ozone column and the cosine of the solar zenith angle), and the ambient temperature. Tests of the parameterization with simulated actinic flux density spectra have revealed an uncertainty of the derived ozone photolysis frequency of ±5%. Field comparisons of the parameterization results with independent measurements of the ozone photolysis frequency were within ±10% for solar zenith angles less than 70^∘. Finally the parameterization was applied to airborne measurements to emphasize the advantage of high time resolution of PDA spectrometers to study ozone photolysis frequency fields in inhomogeneous cloud condtitions.  相似文献   

Fractal generation of surface area of porous media     

Hongbing Sun  Manfred Koch 《Stochastic Hydrology and Hydraulics》1998,12(2):83-96

Many natural porous geological rock formations, as well as engineered porous structures, have fractal properties, i.e., they are self-similar over several length scales. While there have been many experimental and theoretical studies on how to quantify a fractal porous medium and on how to determine its fractal dimension, the numerical generation of a fractal pore structure with predefined statistical and scaling properties is somewhat scarcer. In the present paper a new numerical method for generating a three-dimensional porous medium with any desired probability density function (PDF) and autocorrelation function (ACF) is presented. The well-known Turning Bands Method (TBM) is modified to generate three-dimensional synthetic isotropic and anisotropic porous media with a Gaussian PDF and exponential-decay ACF. Porous media with other PDF's and ACF's are constructed with a nonlinear, iterative PDF and ACF transformation, whereby the arbitrary PDF is converted to an equivalent Gaussian PDF which is then simulated with the classical TBM. Employing a new method for the estimation of the surface area for a given porosity, the fractal dimensions of the surface area of the synthetic porous media generated in this way are then measured by classical fractal perimeter/area relationships. Different 3D porous media are simulated by varying the porosity and the correlation structure of the random field. The performance of the simulations is evaluated by checking the ensemble statistics, the mean, variance and ACF of the simulated random field. For a porous medium with Gaussian PDF, an average fractal dimension of approximately 2.76 is obtained which is in the range of values of actually measured fractal dimensions of molecular surfaces. For a porous medium with a non-Gaussian quadratic PDF the calculated fractal dimension appears to be consistently higher and averages 2.82. The results also show that the fractal dimension is neither strongly dependent of the porosity nor of the degree of anisotropy assumed.  相似文献   

A model for the evolution of photosynthetic oxygen     

Manfred Schidlowski 《Pure and Applied Geophysics》1978,116(2-3):234-238

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Geochronology of high-pressure rocks on Sifnos (Cyclades,Greece)     

Rainer Altherr  Manfred Schliestedt  Martin Okrusch  Eberhard Seidel  Hans Kreuzer  Wilhelm Harre  Heinz Lenz  Immo Wendt  Günther A. Wagner 《Contributions to Mineralogy and Petrology》1979,70(3):245-255

Polymetamorphic rocks of Sifnos (Greece) have been investigated by Rb-Sr, K-Ar, and fission track methods. Critical mineral assemblages from the northern and southernmost parts of Sifnos include jadeite+quartz+3T phengite, and omphacite+garnet +3T phengite, whereas the central part is characterized by the assemblage albite+chlorite+epidote+2M ₁ phengite.K-Ar and Rb-Sr dates on phengites (predominantly 3T) of the best preserved high P/itTmetamorphic rocks from northern Sifnos gave concordant ages around 42 m.y., indicating a Late Lutetian age for the high P/T metamorphism. Phengites (2M ₁+3T) of less preserved high P/T assemblages yielded K-Ar dates between 48 and 41 m.y. but generally lower Rb-Sr dates. The higher K-Ar dates are interpreted as being elevated by excess argon.K-Ar and Rb-Sr ages on 2M ₁ phengites from central Sifnos vary between 24 and 21 m.y. These ages date a second, greenschist-facies metamorphism which overprinted the earlier high-pressure metamorphic rocks.  相似文献   

Component registration in two-dimensional model seismology     

Rolf Gutdeutsch  Manfred Koenig 《Studia Geophysica et Geodaetica》1966,10(3):314-322

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The influence of sea waves on the wind profile     

Lutz Krügermeyer  Manfred Grünewald  Michael Dunckel 《Boundary-Layer Meteorology》1978,14(3):403-414

From wind profile and wave measurements performed during the JONSWAP II experiment, relations between the dimensionless profile slope and the significant wave height are derived. It is shown that the wind profile is distorted by the waves especially in the vicinity of the water surface. The wave influence on the profile seems to be restricted to heights below about three wave heights. Above this level, the dimensionless profile slope is an approximately constant value corresponding to a drag coefficient of about 1.15 × 10^–3.  相似文献