Denudation,vertical crustal movements and sedimentary basin infill

Denudation and vertical crustal movements are linked through the isostatic equation for conservation of lithospheric mass. Recent empirical results from a wide range of sources are presented on the rates of these processes. Denudation alone can cause non-tectonic (isostatic) surface uplift of the right magnitude predicted by theory. A case is made, following Ahnert, for a single linear relationship (although with much scatter) between denudation rate and mean drainage basin relief for large basins. Some recent determinations of denudational time constants have neglected to include tectonic and isostatic terms which oppose the reduction of relief by denudation. Application of diffusional transport models to determine the rate of sediment deposition are severely limited by inherent one-dimensionality and neglect of suspended and washload contributions. Basin infill sequences may be used to determine past sediment transfer coefficients from a hinterland, but problems arise in the apportionment of the various hinterland fluxes that occur in »real-world« three dimensional basins. Sediment yields in smaller half-graben and growth fold basins must reflect the magnitude of drainage basins and the complex local controls upon sediment yields. Examples are given from extensional basins in the Western USA and Greece. The »length« of tectonic relief produced in tilt blocks and growth folds will control the area of drainage basin developed (through the fractal form of Hack's Law) and hence the magnitude of deposition in sedimentary basins adjoining tectonic uplands.

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Zusammenfassung Denudation und vertikale Krustenbewegungen sind verbunden durch das isostatische Gesetz über den Erhalt der lithosphärischen Masse. Neuerliche empirische Ergebnisse aus einem weiten Quellenbereich werden im Verhältnis zu diesen Prozessen präsentiert. Denudation allein, kann nicht tektonisch bedingte (isostatische) Oberflächenhebungen hervorrufen, die in der richtigen Größenordnung liegen, wie sie auch theoretisch ermittelt wurden. Es wird in Anlehnung an Ahnert ein Fall geschaffen, in der eine einfach lineare Beziehung (obgleich mit vielen Streuungen) zwischen der Denudationsrate und dem durchschnittlichen Abflußbeckenrelief für große Becken vorliegt. Einige neue Ermittlungen der Denudationszeitkonstanten wurden vernachlässigt, um tektonische und isostatische Begriffe einzufügen, welche sich der Verringerung des Reliefs durch Denudation widersetzen. Die Anwendung des Verbreitungstransportmodells zum Bestimmen der Sedimentationsrate sind streng begrenzt durch die ihm innewohnende Eindimensionalität, und der Vernachlässigung der Schwebe- und Schwämmfrachtbeteiligung. Bekkenfüllungssequenzen können benutzt werden um vergangene Sedimenttransferkoeffizienten aus dem Hinterland festzulegen; aber es treten auch Probleme bei der Verteilung der verschiedenen Hinterlandeinträge auf, die bei einem realen dreidimensionalen Becken vorhanden sind. Sedimenteinträge in kleineren Halbgräben und Growth-fold Becken müssen die Größe des Abflußbeckens widerspiegeln, sowie die komplexen lokalen Steuerungen auf die Sedimenteinträge. Beispiele von Dehnungsbecken aus dem Westen der USA und Griechenlands werden angesprochen. Die Länge des tektonischen Reliefs in verkippten Blöcken und Growth-Folds wird die Fläche des entwickelten Abflußbeckens kontrollieren (durch die fraktale Form des Gesetzes von Hack), und daher die Ablagerungsmenge von Sedimentbecken in der Nähe von tektonischen Hochlagen.

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Résumé L'érosion et les mouvements crustaux verticaux sont liés par l'équation isostatique de conservation de la masse lithosphérique. Des résultats empiriques récents provenant d'un large éventail de sources sont présentés en relation avec ces processus. L'érosion seule peut être la cause d'une montée non tectonique (isostatique) dont l'ampleur est prévue exactement par la théorie. Un cas est présenté, d'après Ahnert, qui montre, pour de grands bassins, une relation linéaire simple (mais avec une forte dispersion des points) entre le taux de dénudation et le relief moyen de l'aire de drainage. Certaines déterminations récentes des constantes de temps de dénudation ont omis de tenir compte des termes tectonique et isostatique qui s'opposent à la destruction du relief par érosion. L'utilisation de modèles de transport diffus en vue de déterminer le taux d'accumulation des sédiments est sévèrement limitée par le caractère unidimensionnel de tels modèles et par le fait qu'il ne tiennent pas compte de la fraction en suspension. Les séquences de comblement d'un bassin sédimentaire peuvent être utilisées pour déterminer les anciens cfficients de transfert à partir de l'hinterland; mais des difficultés surgissent à propos de la répartition des différents flux en provenance de l'hinterland dans le cas réel d'un bassin à 3 dimensions. Les apports sédimentaires dans les bassins de demi-graben et de »growth-fold« doivent traduire la grandeur des aires de drainage et les facteurs locaux complexes qui régissent ces apports. Des exemples sont présentés, relatifs à des bassins d'extension de l'ouest des USA et de Grèce. La »longueur« des reliefs tectoniques en relation avec les blocs basculés et les »growth-folds« déterminent, par la forme fractale de la loi de Hack, la surface des aires de drainage ainsi engendrées et, en conséquence, l'importance des dépôts dans les bassins sédimentaires voisins des reliefs tectoniques.

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Hawaiian basalt and Icelandic rhyolite: Indicators of differentiation and partial melting

In spite of the voluminous basaltic volcanism on the island of Hawaii, rhyolite is not produced. Iceland, on the other hand, exhibits common rhyolitic volcanism amounting to some 10–12% of its surface rocks. This contrast is investigated using the fundamental igneous processes exhibited by sheet-like Hawaiian lava lakes and Shonkin Sag laccolith in Montana. Highly differentiated, residual melts normally reside within inwardly advancing solidification fronts and are generally inaccessible to eruptive processes. Only when a large initial phenocryst population is present, from which a thick basal cumulate can rapidly form, is it possible to supply highly differentiated melt into the active (i.e., eruptable) portion of the magma chamber. Although there is protracted control of differentiation at Hawaii by settling of olivine, further differentiation occurs within the solidification fronts. Only by repeated transport and holding is it possible to differentiate beyond the critical composition of the leading edge of the solidification front ( 7% MgO and 51.5% SiO₂). Crystal size distributions (CSDs) for Hawaii and Shonkin Sag are used to demonstrate the inferred physical and chemical processes of solidification, including the kinetics of crystallization.A ubiquitous feature of these basaltic bodies is the formation of coarse veins and segregations of refined melt and granophyres within the upper solidification front. It is this fundamental bimodal feature which is the key to understanding Icelandic silicic volcanism.Rhyolites in Iceland occur mainly as a bimodal population with basalts associated with central volcanoes. Rhyolites, granophyres, and felsites are common, with the intrusions often being layered. Ash flows and true granite-like intrusions are rare. The voluminous silicic lavas at Torfajokull central volcano contain disequilibrium phenocryst assemblages. This, and the disagreement in oxygen isotopic values between rhyolites and basalts, reflects extensive partial melting of the heterogeneous basaltic crust of Iceland to produce these rhyolites. Relatively small, chemically distinct, and spatially intimate silicic bodies are formed by concentrating granophyric segregations from earlier cycles of solidification. This process is also reflected in the layered granophyric instrusion of Slaufrudalur in eastern Iceland. Slaufrudalur is an unvented subterranean caldera, equivalent in igneous processes and style to the subaerial Torfajokull caldera.Hawaii is dominated by fractional crystallization due to crystal settling and does not produce rhyolite. Iceland's tectonics allow continual and extensive reprocessing of thin, hot basaltic crust which produces rhyolite by concentrating original silicic segregations and veins and by partially melting intermediate extrusives, which have subsided deep into the crust.

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Zusammenfassung Auf Hawaii treten, trotz intensiven Basalt-Vulkanismusses, keine Rhyolithe auf. Auf Island dagegen ist Rhyolith, mit 10–12% des anstehenden Gesteins, verbreitet. Dieser Kontrast wurde anhand grundlegender magmatischer Prozesse untersucht, wie sie in flachen Lava-Seen Hawaiis und im Shonkin Sag Laccolith Montanas auftreten. Hochdifferenzierte Restschmelzen verbleiben innerhalb langsam nach innen vorrückender Erstarrungsfronten und sind meist unerreichbar für eruptive Prozesse. Nur wenn anfänglich bereits große Mengen von Einsprenglingen vorhanden sind, die rasch am Boden der Magmenkammer akkumulieren, kann eine hochdifferenzierte Schmelze in den aktiven (d.h. eruptiven) Teil der Magmenkammer gelangen. Obwohl auf Hawaii die Differentiation durch die Kristallisation von Olivin anhaltend kontrolliert wird, findet an der Erstarrungsfront weitere Differentiation statt. Nur durch wiederholten Transport und zeitweiliges Verharren ist es möglich, über die kritische Zusammensetzung der vordersten Erstarrungsfront hinaus zu differenzieren (ca. 7% MgO und 51,5% SiO₂). An Kristallgrö-ßenverteilungen (CDS) von Hawaii und Shonkin Sag können die angenommenen physikalischen und chemischen Prozesse der Kristallisation und die Kristallisationskinetik gezeigt werden. Ein weit verbreitetes Merkmal dieser Basaltkörper ist die Bildung grobkristalliner Gänge und Absonderung von stark differenzierten Schmelzen und Granophyren innerhalb der oberen Erstarrungsfront. Diese ausgeprägt bimodale Charakteristik ist der Schlüssel zum Verständnis des sauren isländischen Vulkanismus.Isländische Rhyolithe treten meist in bimodaler Verbreitung mit Basalten in Zusammenhang mit zentralen Vulkanen auf. Rhyolithe, Granophyre und Feisite sind häufig, in oft geschichteten Intrusionen. Ignimbrite und echte Granitintrusionen sind selten. Die großen Mengen SiO₂-reicher Laven am Torfajokull-Zentralvulkan enthalten Ein-sprenglinge, die sich nicht im Gleichgewicht mit der Matrix befinden. Dies, und die unterschiedlichen delta-¹⁸O-Werte von Rhyolithen und Basalten, zeigen, daß ausgeprägtes teilweises Aufschmelzen der heterogenen Basaltkruste von Island zur Produktion dieser Rhyolithe führte. Relativ kleine, nahe benachbarte saure Körper, die aber deutliche Unterschiede in ihrem Chemismus aufweisen, werden gebildet durch die Konzentration granophyrischer Teilschmelzen aus früheren Kristallisationszyklen. Dieser Vorgang wird auch widergespiegelt in der »layered intrusions« von Slaufrudalur in Ostisland. Slaufrudalur ist eine geschlossene unterirdische Kaldera, deren magmatische Prozesse und Baustil der subaerischen Torfajokull-Kaldera entsprechen.Die Prozesse in Hawaii sind dominiert von gravitativer Kristallisationsdifferentiation und es werden keine Rhyolithe produziert. Die isländische Tektonik führt zu kontinuierlicher starker Wiederaufarbeitung von dünner, heißer basaltischer Kruste. Dabei wird, durch die Konzentration ursprünglicher saurer Teilschmelzen und Gänge und durch die teilweise Aufschmelzung intermediärer Intrusiva, die tief in die Kruste abgesunken sind, Rhyolith produziert.

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Résumé En dépit du volcanisme basaltique volumineux des îles Hawaï, il n'y existe pas de rhyolite. En Islande, par contre, le volcanisme rhyolitique est commun et représente 10 à 12% des roches de la surface. Ce contraste est examiné sur la base des processus ignés fondamentaux présentés par les lacs de lave d'Hawaï et le laccolite de Shonkin Sag au Montana. Normalement, les liquides résiduels hautement différenciés résident à l'intérieur des fronts de solidification qui progressent vers l'arrière et sont généralement à l'abri des processus éruptifs. Ce n'est que dans le cas d'une population initiale abondante de phénocristaux, qui se rassemblent dans un cumulat basai épais, que des liquides hautement différenciés peuvent être fournis à la portion active (c'est-à-dire »éruptible«) de la chambre magmatique. A Hawaï, bien que la différenciation soit continuellement régie par la cristallisation d'olivine, la poursuite du processus a lieu à l'intérieur des fronts de solidification. Ce n'est que par la répétition d'actions de transport et de stagnation qu'il est possible de différencier audelà de la composition critique du front de solidification (±7% MgO et 51,5% SiO₂). A partir de la distribution de la taille des cristaux à Hawaï et à Shonkin Sag, on peut déduire les processus physique et chimique de la solidification, y compris la cinétique de la cristallisation.Une particularité courante de ces corps basaltiques est la formation de veines grenues et de ségrégations de liquides très différenciés et de granophyres à l'intérieur du front supérieur de solidification. Cette manifestation bimodale est la clé qui permet de comprendre le volcanisme siliceux islandais.En Islande, les rhyolites constituent d'ordinaire une population bimodale avec les basaltes centraux. Les rhyolites, les granophyres et les felsites sont fréquents, et souvent sous forme d'intrusions litées. Les coulées ardentes et les vraies intrusions de type granitique sont rares. Les volumineuses laves siliceuses du volcan central de Torfajokull contiennent des assemblages de phénocristaux en déséquilibre. Ce fait, ainsi que la non concordance des isotopes de l'oxygène entre rhyolites et basaltes, traduisent, à l'origine de ces rhyolites, une fusion partielle extensive de la croûte basaltique hétérogène d'Islande. Des corps siliceux relativement petits et chimiquement distincts bien que d'emplacements très voisins se sont formés par concentration de fusions partielles granophyriques lors des premiers cycles de solidification. Ce processus s'exprime également dans l'intrusion granophyrique litée de Slaufrudalur, en Islande orientale. Slaufrudalur est une caldeira souterraine fermée, équivalente par son style et son processus igné à la caldeira subaérienne de Torfajokull.A Hawaï, le phénomène dominant est la cristallisation fractionnée gravitative, sans production de rhyolite. La tectonique de l'Islande permet la régénération continue et extensive d'une mince croûte basaltique chaude. Les rhyolites y sont engendrées par la concentration des veines et ségrégations siliceuses originelles et par la fusion partielle de masses extrusives intermédiaires descendues profondément dans la croûte.

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, . , 10–12% . , Shonkin Sag Laccolith Montanas. . , , . , . . ( 7% MgO 51,5% SiO₂). (CDS) Shonkin Sag , , . . . . , , . . , Torfajokull , ., ¹⁸O , . , , , , « » («layered intrusions») Slaufrudalur, . , , Torfajokull. . . , , , .

     

MRSP—The muenster redshift project. Astrometric determination of the reference point for wavelength measurements on low-dispersion objective prism plates

The zero point of galaxy redshifts measured from objective prism plates (dispersion 246 nm/mm at H) as part of the Muenster Redshift Project (MRSP) is obtained through transformation of object positions from the corresponding direct plate. Approximately 1000 G-type stars, classified automatically, are used. On the direct plate, positions are obtained from intensity-weighted first moments. On the objective prism plate, object positions are give through the CaII-break and marginal fits to the unwidened spectra. The transformation equations include quadratic terms in the direction of dispersion. The inclusion of third-order and colour terms is discussed. The mean residuals are approximately 0".33 (5 m on the plate), corresponding to a redshift error of about 700 km/s at z=0.0. This error results mainly from the uncertainty in locating the CaII-break in the low-dispersion spectra. Radial velocities are obtained from the difference between the expected and the measured positions of the CaII-break in the galaxy spectra.     

Laser radiation in active amplifying media treated as a transport problem: Transfer equation derived and exactly solved

The flow of laser radiation in a plane-parallel cylindrical slab of active amplifying medium with axial symmetry is treated as a problem in radiative transfer. The appropriate one-dimensional transfer equation describing the transfer of laser radiation has been derived by an appeal to Einstein'sA, B coefficients (describing the processes of stimulated line absorption, spontaneous line emission, and stimulated line emission sustained by population inversion in the medium) and considering the rate equations to completely establish the rational of the transfer equation obtained. The equation is then exactly solved and the angular distribution of the emergent laser beam intensity is obtained; its numerically computed values are given in tables and plotted in graphs showing the nature of peaks of the emerging laser beam intensity about the axis of the laser cylinder.     

Astrometric investigation with the Tautenburg Schmidt telescope

The observations and the plate reduction technique for the determination of positions and absolute proper motions which is used in Potsdam are described. Recent results have shown that an accuracy of about 0 _. 1 for positions and 0 _. ⁷ cent _. ^–1 for proper motions can be achieved both for bright (8^m–12^m) and faint (16^m–18^m) stars. Three astrometric programmes using the Tautenburg plates are presented.     

Declination variations for zenith stars

The variations of the declinations of 36 Belgrade zenith stars from BZS1₇₀ Catalogue published in Astronomy and Astrophysics,177, 313–316 (1987) are examined by spectral analysis. The prospect is to evaluate multiples of the Chandler period of which the most prominent for all stars is the double one.     

Cosmological implications of BL Lac objects

It has become clear in recent years that relativistic beaming is a good explanation for the BL Lac phenomenon. Of studies based on the relativistic beaming model of BL Lac objects, we note that the orientation of jet's axis to the line-of-sight is very small and, therefore, the observed flux emitted from a rapidly moving source is orders of magnitude higher than the flux in its rest-frame:F _obs = ^{3 +} F _intr, where is the bulk relativistic Doppler factor. Then the observed apparent magnitudem _v must be corrected for this effect. For our 39 samples, the corrected apparent magnitudem _v ^corr and logZ have a good correlation.     

The maximum limit of the density variation parameter λ for a stable neutron star

A static spherically-symmetric model, based on an exact solution of Einstein's equation, gives the permissible matter density 2×10¹⁴ g cm^–3. If we use the change in the ratio of central density to the radiusr=a (i.e., central density per unit radius (₀/a), we call it radius density) minimum, we have estimated the upper limit of the density variation parameter () and minimum mass limit of a superdense star like a neutron star. This limit gives an idea of the domain where the neutron abundance with negligible number of electrons and protons (may be treated as pure neutrons) and equilibrium in neutrons begins.     

Diurnal photometric conditions at Teide observatory and long-term solar irradiance variations

Monochromatic extinction coefficients at four wavelengths have been obtained over a period of more than two years at the Observatorio del Teide (Izaña Tenerife) using a full disc, direct sunlight, quadruple photometer devoted to the detection of integral luminosity oscillations of the Sun. The mean extinction coefficients (0.13 at 500 nm) show a seasonal variation of about 15%, the best atmospheric conditions being in winter and autumn. Moreover, in anyone day the extinction coefficient in the afternoon is always lower than the one in the morning by 7%. A one-year period fluctuation, with an amplitude of 0.035 mag, has been identified in the instrumental magnitudes outside the atmosphere, and is interpreted as the variation produced by the different Sun-Earth distance from winter to summer. Finally, the study made to detect periodic time fluctuations in both, Sun's magnitude and extinction coefficients, has given null results at levels of 0.04 and 1.8%, respectively.     

Bidimensional spectroscopy of network bright points

We develop an automatic, computer controlled procedure to select and to analyze the Network Bright Points (NBPs) on solar images. These have been obtained at the Sac Peak Vacuum Tower Telescope by means of the Universal Birefringent Filter and Zeiss H filters, tuned, respectively, along the profiles of the H, Mg-b1, Na-D2, and H lines.A structure is identified as an NBP if at the wavelength H- 1.5 A its maximum intensity is greater than I + 3 and its area is greater than 1.5 arc sec² at I + 1.5, where I is the mean value and the standard deviation of the intensity distribution on the image. Each detected NBP is then searched and confirmed in all the remaining 31 images at different wavelengths.For each NBP several parameters are measured (position, area, mean and maximum contrast, Dopplergram velocity, compactness, and so on) and some identification constraints are applied.The statistical analysis of the various parameter distributions, for NBPs present within an active region and its surroundings, shows that two types of NBPs can be identified according to the value of their mean contrast C _min the H- 1.5 Å image (C _m 0.1 type I, C _m> 0.1 type II). The type I NBPs (all occurring on the boundaries of the supergranular network) appear to be much more frequent (180/26) than the type II ones.The size A of type I NBPs is less than 1.0 arc sec for H/H wings but of the order of 1.2 arc sec for Na-D2 and Mg-bl. The mean contrast C _m is around the value of 10% along the Na-D2 and Mg-bl profiles and of 20% along the H/H wings.The C _m - A scatter diagrams show, for the photospheric radiation (h < 100 km), a narrow range of variability for C _min correspondence with a wide range for A. For radiation orginated at higher levels (h > 200 km), the C _m- A scatter diagrams seem to indicate, even if with a large variance, that the highest C _m's tend to correspond to the highest A values.The mean Doppler shift is close to zero for Na-D2 and Mg-bl lines but negative (downward motion) for H and H lines.The type II NBPs tends to be preferentially located in the neighbourhood of small, compact sunspots and their detectability is almost constant through all the 4 studied line profiles. No conclusions can be derived on the mean size, contrast and Doppler shift values because their distributions are too dispersed. The only positive information is that its C _m- A scatter diagram, in H and H wings, indicates a wide range of variability for C _m in correspondence with very narrow range of variability for A.